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CRANFIELD UNIVERSITY
GEORGIOS GALANOS
RIICS:
Rapid Imminent Impactor Characterization System:
ELECTRICAL POWER SYSTEM
SCHOOL OF AEROSPACE, TRANSPORT AND
MANUFACTURING
Group Design Project
MSc in Astronautics and Space Engineering
Academic Year: 2018 - 2019
Supervisor: Dr Joan-Pau Sánchez Cuartielles
October 2018
CRANFIELD UNIVERSITY
SCHOOL OF AEROSPACE, TRANSPORT AND
MANUFACTURING
Group Design Project
MSc in Astronautics and Space Engineering
Academic Year 2018 - 2019
GEORGIOS GALANOS
RIICS: ELECTRICAL POWER SYSTEM
Supervisor: Dr Joan-Pau Sánchez Cuartielles
October 2018
This report is submitted in partial fulfilment of the requirements for
the degree of MSc in Astronautics and Space Engineering
© Cranfield University 2018. All rights reserved. No part of this
publication may be reproduced without the written permission of the
copyright owner.
Georgios Galanos
i
ABSTRACT
This report is part of a group project of fifteen students of Cranfield University
and is the preliminary design of the RIICS mission: Rapid Imminent Impactor
Characterisation system.
RIICS is a science-driven mission, which aims to characterise and detect near
earth objects and exoplanets as a secondary science. A low cost mission of a
50M € budget.
This report is the written proof work of Georgios Galanos, a member of the
group project and responsible for the electrical power subsystem of the
spacecraft.
This report contains an analytical design of the electrical power subsystem of
the RIICS project. The main requirement of the project is to design a low cost
and reliable system. The final design successfully achieved to fulfil the above
requirements (low cost and reliable power system).
This report assesses the final design of the electrical power subsystem. The
report includes the analysis and sizing of the primary and secondary power
source, and comparison of the different design options. It also includes the main
power control and distribution system to the loads.
Keywords: Electrical, Power, Solar P-V, Batteries, PCDU
Georgios Galanos
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ACKNOWLEDGEMENTS
First of all I would like to thank all the group members of the RIICS project and
our supervisor Dr Joan-Pau Sánchez Cuartielles who was meeting us every
single week from the beginning of the year to help and advise us. Moreover, I
would like to thank Dr Leonard Felicetti who taught me about power systems
with the most efficient way.
Finally I would like to thank my family for always being by my side.
Georgios Galanos
v
TABLE OF CONTENTS
© Cranfield University 2018. All rights reserved. No part of this publication
may be reproduced without the written permission of the copyright owner......... ii	
ABSTRACT ..........................................................................................................i	
ACKNOWLEDGEMENTS................................................................................... iii	
LIST OF FIGURES............................................................................................ vii	
LIST OF TABLES ............................................................................................... ix	
LIST OF ABBREVIATIONS...............................................................................xiii	
1 Introduction.......................................................................................................1	
1.1 RIICS Background .....................................................................................1	
1.2 Electrical power background......................................................................1	
2 Main power sources .........................................................................................3	
2.1 Comparison of primary power sources based on mission’s
requirements....................................................................................................6	
3 Power Control...................................................................................................7	
3.1 Direct Energy Transfer (DET) ....................................................................8	
3.1.1 Fully regulated Bus..............................................................................8	
3.1.2 Sun - Regulated Bus (Unregulated Bus).............................................9	
3.1.3 Comparing Regulated and Unregulated Bus.....................................10	
3.2 Peak Power Tracker (PPT) - Power control.............................................11	
3.3 Power Control Trade-off...........................................................................12	
3.4 Bus voltage selection...............................................................................14	
4 Solar arrays ....................................................................................................15	
4.1 Solar PV technology ................................................................................15	
4.2 Solar array structure ................................................................................16	
4.2.1 Rigid Panels ......................................................................................16	
4.2.2 Body–Mounted ..................................................................................17	
4.2.3 Three or More Wings.........................................................................18	
4.2.4 Flexible Array ....................................................................................19	
4.2.5 Selection of Construction ..................................................................19	
5 Energy storage - Secondary battery...............................................................20	
5.1 Types of secondary batteries...................................................................21	
6 Analyze and Size the Power System..............................................................23	
6.1 Study Case 1 ...........................................................................................23	
6.2 Study Case 2 ...........................................................................................25	
6.3 Comparison of Cases ..............................................................................26	
6.4 Power Consumption Analysis ..................................................................29	
7 Solar Arrays Sizing.........................................................................................36	
7.1 Battery’s Component Selection................................................................38
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vi
7.1.1 Configuration.....................................................................................38	
8 Power Control and Distribution Unit (PCDU)..................................................40	
9 Conclusion......................................................................................................44	
REFERENCES..................................................................................................45	
BIBLIOGRAPHY................................................................................................47	
APPENDICES ...................................................................................................49
Georgios Galanos
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LIST OF FIGURES
Figure 1-1 Typical Architecture of a Power System ...........................................2	
Figure 2-1 Energy sources options for various power requirements ..................6	
Figure 3-1 Regulated Bus DET...........................................................................9	
Figure 3-2 Sun- Regulated Bus (Unregulated Bus) DET..................................10	
Figure 3-3 Peak Power Tracker Architecture....................................................11	
Figure 3-4 Battery charge and discharge options in peak power tracking
architecture.................................................................................................12	
Figure 3-5 Optimum voltage for various power levels ......................................14	
Figure 4-1 Typical Solar Array Design Parameters ..........................................15	
Figure 4-2 A fully deployed dollar array............................................................16	
Figure 4-3 Panels section with cells mounted on a honeycomb substrate with
face sheets.................................................................................................17	
Figure 4-4 A body mounted solar array ............................................................18	
Figure 4-5 Three wings array architecture........................................................18	
Figure 4-6 Final design of the Solar arrays.......................................................20	
Figure 6-1 Solar arrays comparison .................................................................27	
Figure 6-2 Batteries Comparison......................................................................28	
Figure 6-3 Total Mass and Cost Comparison...................................................29	
Figure 6-4 Average Power Consumption..........................................................34	
Figure 6-5 Power Consumption during Operational Phase ..............................35	
Figure B-1 Selected Orbit.................................................................................62	
Figure B-3 Soyuz ST-B - SYLDA-S dual launch configuration.........................63	
Figure B-4 Mission Phases Timeline................................................................64	
Figure B-5 Launch and Early Operations Phase Timeline ...............................66	
Figure B-6 Commissioning Phase Timeline .....................................................68	
Figure B-7 Paints and surface coatings............................................................72	
Figure B-8 Overview of the shapes of the secondary structures......................74	
Figure B-9 Transfer phase propulsion schematic.............................................75
Georgios Galanos
viii
Figure B-10 Reaction Control Schematic after propulsion module separation.75	
Figure B-11 Fully deployed spacecraft overview in its operational configuration
at the L1 point.............................................................................................78	
Figure B-12 Folded launch configuration combining the spacecraft and the
propulsion module......................................................................................78	
Figure B-13 Compatibility verification with the upper position of the SYLDA-S78	
Figure B-14 List of the main components of the spacecraft .............................79	
Figure B-15 Outer and Inner Structure of the main spacecraft.........................79	
Figure B-16 External configuration of the main spacecraft...............................80	
Figure B-17 Internal bottom body configuration ...............................................80	
Figure B-18 Internal top body configuration .....................................................80	
Figure B-19 Overview of the propulsion module configuration.........................81	
Figure B-20 Spacecraft Overview Design ........................................................82	
Figure B-21 Cassegrain Design of Telescope..................................................82	
Figure B-22 Probability inside scan area centered (-120,0) .............................86	
Figure B-23 Position at detection comparison with limiting magnitude 21 and 17
...................................................................................................................88	
Figure B-24 Difference between maximum apparent motion with perturbations
and maximum apparent motion without perturbations .............................89	
Figure B-25 Mean apparent motion for each object in degrees per day........89	
Figure C-1 Shunt Regulator specifications and functional schematic.............115	
Figure C-2 Pyro Firing Drive Module specifications and functional schematic
.................................................................................................................116	
Figure C-3 Equipment Power Distribution Module specifications and functional
schematic .................................................................................................117	
Figure C-4 Battery Charge / Discharge Regulator specifications and functional
schematic .................................................................................................118	
Figure C-5 Heater Power Distribution Module specifications and functional
schematic .................................................................................................119	
Figure C-6 Modular Medium Power Unit specifications..................................120
Georgios Galanos
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LIST OF TABLES
Table 2-1 Technology options and status ...........................................................5	
Table 3-1 Advantages and Disadvantages of different architectures................13	
Table 5-1 Number of cells as a factor of bus voltage........................................20	
Table 5-2 Issues in Designing the Energy Storage Capability..........................21	
Table 5-3 Characteristics of Selected Secondary Batteries .............................22	
Table 6-1 Solar Arrays Specifications Case 1...................................................24	
Table 6-2 Battery Specifications Case 1...........................................................24	
Table 6-3 Total Specifications Case 1 ..............................................................25	
Table 6-4 Solar Arrays Specifications Case 2...................................................26	
Table 6-5 Battery Specifications Case 2...........................................................26	
Table 6-6 Total Specifications Case 2 ..............................................................26	
Table 6-7 Battery Discharge for cases tat peak power is required ...................31	
Table 6-8 Cycle life of battery ...........................................................................32	
Table 6-9 Part of the Power Break During Operational Phase .........................34	
Table 6-10 Battery Specifications for operational phase...................................36	
Table 7-1 Solar arrays main features................................................................38	
Table 7-2 Battery’s worst Case Scenario Parameters ......................................39	
Table 7-3 VES 140 Shaft Battery......................................................................40	
Table B-1 Highest Criticality Events and Key Prevention Actions ....................52	
Table B-2 Trade off...........................................................................................52	
Table B-3 Mass Budget Breakdown .................................................................53	
Table B-4 AOCS Mass Breakdown...................................................................55	
Table B-5 HGA Link Budget..............................................................................56	
Table B-6 LGA Link Budget ..............................................................................57	
Table B-7 Power Budget...................................................................................60	
Table B-8 Propellant mass and ΔV break down ...............................................60	
Table B-9 Development Cost of the spacecraft ................................................61
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Table B-10 Overall Mission Cost Budget..........................................................61	
Table B-11 Selected Orbit.................................................................................62	
Table B-12 Orbit’s Characteristics ....................................................................62	
Table B-13 Transfer trajectory parameters.......................................................63	
Table B-14 Mission Phases Timeline................................................................65	
Table B-15 Launch and Early Operations Phase Timeline...............................67	
Table B-16 Commissioning Phase Timeline.....................................................69	
Table B-17 Science Operations Priorities.........................................................69	
Table B-18 Thermal Control Breakdown...........................................................71	
Table B-19 Main thermal control elements .......................................................71	
Table B-20 Properties of the central tubes of the primary structure .................72	
Table B-21 Properties of the vertical panels of the primary structure...............73	
Table B-22 Properties of the horizontal decks of the primary structure............73	
Table B-23 Properties of the secondary structures...........................................74	
Table B-24 Size, throughout and data produced estimates for the telescope ..76	
Table B-25 Final size and throughput estimates...............................................76	
Table B-26 Onboard Computer performance specifications.............................76	
Table B-27 Communications design hardware selection mass and power
budgets.......................................................................................................77	
Table B-28 Main Mechanisms Configurations ..................................................81	
Table B-29 Optical Configuration of Telescope ................................................83	
Table B-30 Integration time to achieve a SNR = 5 with 0.3m aperture.............83	
Table B-31 Modified visible camera from the UVIS instrument specifications..84	
Table B-32 NIR Spectrometer specifications....................................................84	
Table B-33 Requirements imposed for baseline design ...................................85	
Table B-34 Telescope performance analysis for secondary science operations
...................................................................................................................85	
Table B-35 Requirement performance in Characterisation mode.....................86	
Table B-36 Requirement performance in Scan mode.......................................86
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Table B-37 Warning time with the frozen design ..............................................87	
Table C-1 Power Breakdown. Analytic Power consumption for each instrument,
charge and discharge mode and total consumption of each phase.........111	
Table C-2 Analytical operation of the battery during each phase of the mission
.................................................................................................................112	
Table C-3 Analytic data for the cycle life of the battery...................................113	
Table C-4 Comparison between VES 100, VES 140 and VES 180.
Specifications of each battery type...........................................................114	
Table C-5 PCDU Dimensions and Mass.........................................................114
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Georgios Galanos
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LIST OF ABBREVIATIONS
AU Astronomical Unit
BCDR Battery Charge / Discharge Regulator
BOL Beginning of Life
CM Command and Monitoring
DC Direct Current
DET Direct Energy Transfer
DoE Department of Energy
EOC End Of Charge
EOD End Of Discharge
EOL End of Life
EPD Equipment Power Distribution
ESA European Space Agency
GaAs Gallium Arsenide
GEO Geostationary Orbit
HPD Heaters Power Distribution
ISS International Space Station
LCL Latching Current Limiters
Li-ion Lithium
MJ Multi Junction
MMPU Modular Medium Power Unit
NASA National Astronautics and Space Administration
NEO Near Earth Object
Ni-Cd Nickel Cadmium
Ni-H2 Nickel Hydrogen
PCDU Power Control and Distribution Unit
PFD Pyro Firing Drive
PPT Peak Power Tracker
PV Photovoltaic
RIICS Rapid Imminent impactor Characterization
RSO Resident Space Objects
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RTG Radioisotope Thermoelectric Generators
S4R Shunt Regulation Module
Si Silicon
SJ Single Junction
SSA Space Situation Awareness
SSTL Surrey Satellite Technology
TE Thermoelectric
TJ Triple Junction
Introduction Georgios Galanos
1
1 Introduction
1.1 RIICS Background
RIICS mission is based on the ESA’s SSA (Space Situation Awareness
Program). The SSA program has been created from the need of awareness to
predict and detect man-made space orbits, in-orbit events, potential impacts of
NEO’s and effects of space weather phenomena and ground based
infrastructures. As a result, the life risk and other undesired situations such as
the Chelyabinsk meteorite will be eliminated. NEOs can be defined as asteroids
or comets that pass near the Earth. SSA program aims to understand these
kinds of objects in order to decrease the risk of causing damages. Around
600,000 asteroids are known in our Solar system and 16,000 of them are
classified as NEOs. Constant and efficient monitoring has to be carried out to
ensure Earth is not being affected by potential impacts.
RIICS mission is designed to achieve two main objectives. The first objective is
the physical characterisation and scanning system for NEO’s on the order of
few meters. A better understanding of the NEO’s can be obtained by
characterising imminent impactors and comparing the information collected
prior and to the impact. Current ground telescopes have low capability detection
due to the atmosphere and the Sun effects, which can be avoided by setting the
telescope in orbit (Seurin, N., 2019).
During the 6-year mission (5 in operations), the spacecraft will operate
secondary science with the use of the existing telescope and sensors. The
observation and characterisation of exoplanets and identification of RSO
(resident space objects) form the secondary science of the mission.
1.2 Electrical power background
The power system is one of the most critical subsystems of a spacecraft. The
failure of the power system and inability to supply the required power to the
spacecraft results in the failure of the entire mission. (Fortescue and Stark,
Introduction Georgios Galanos
2
2003) It is of high importance to design a reliable and efficient power system. In
the early 80s, space agencies focused mainly on large satellites such as ISS
and manned missions to the moon. The necessity of using large satellites led
the agencies to design high power consuming systems. The American Nasa
and DoE and the European Space Agency (ESA) made extensive studies to
accomplish these requirements (SPS Concept). Many research projects were
forced to slow down or even stop due to political and technical issues,
regardless the critical threat of global warming (Landis, 2006). Despite that in
the beginning most space agencies attempted to build large spacecrafts,
nowadays space projects focus more on small satellites in order to maintain the
low cost and high efficiency (Fortescue and Stark, 2003).
The power subsystem has to follow one important rule:
Pow_direct_01 - The power subsystem must generate, distribute and control
the required power and spread it accordingly to all the subsystems during the
mission (Seurin, N., 2019)
To achieve this requirement, the design of each of the power system’s
components must be taken into sensitive and accurate consideration.
Figure 1-1 Typical Architecture of a Power System (Fortescue and Stark, 2003)
Main power sources Georgios Galanos
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2 Main power sources
The selection of the main power source of the spacecraft depends on several
parameters. The spacecraft’s configuration is one of these parameters. Weight,
size limitations, constraints set by the launch vehicle and heat dissipation
capability are some of the main variables that affect the power subsystem of the
spacecraft (Wertz et al, 2015). The main drivers for the sizing of the power
system are the lifetime of the mission, duration of each mode and respective
power consumption. As every subsystem is linked to each other, attitude control
scheme, orbital parameters, communications, payload, mechanisms, thermal
control and on board data handling are affecting the power source selection.
Payload is one of the most important subsystems that affects the power system,
as it is the one that sets the limitations for all the subsystems and consequently
the power subsystem. Finally, the environment of the mission is a very critical
parameter that has to be taken into account. Different missions require different
approaches of power sources and energy storage methods depending on the
type of orbit and distance from the sun, especially if the mission is
interplanetary.
Spacecraft’s primary power source:
• Primary batteries
• Solar PV – secondary battery
• Radioisotope – Thermoelectric Generators (RTGs)
• Fuel cells
• Solar Concentrator – Dynamic
• Chemical Dynamic
1. Primary batteries are producing direct current by electrochemistry. One
of their main advantage is that they are the most economical primary
source for small spacecrafts with short lifetime (Miller, Keesee, 2003).
2. Solar photovoltaic power source is the most common source for
spacecraft power systems as it can provide power in tens of watts to
Main power sources Georgios Galanos
4
several of kilowatts up to 20 years lifetime. This method is converging the
sun radiation power into electrical power. Hence, it is considered to be
one of the most reliable and economical primary sources. In cases where
the spacecraft is under eclipses, the spacecraft must provide energy
from a different source due to the lack of solar power. During eclipses
secondary batteries must be applied for providing the necessary power
requirements. Secondary batteries are not used only for eclipses but also
for emergency cases and peak power requirements for when a direct
transfer power is in use (Jensenh, 2003).
3. As previously noted, the type of the mission is one of the main
parameters taken into account. RTGs are used generally for
interplanetary missions, particularly in deep space, where the power
consumption is very large. One of the main advantages of RTGs is its
capability of generating power in the absence of the sun and can last up
to several decades (The Viking landers were operating for 4-6 years
supplied by RTGs). Moreover, it is insensitive to the cold of the deep
space and can be exposed to the high radiation space fields. More power
can be supplied proportionally to the spacecraft’s mass. No moving parts
and absent of fluids, safe and flight-proven, and free of maintenance are
some extra advantages of the RTGs that make that power source very
reliable. On the other hand, the fact that RTGs cannot be turned on and
off and the power is decreasing exponentially with time makes it
undesired for many types of missions. From the thermal control point of
view, RTGs must be under cooling mechanisms and coverage during the
course of the mission. The main disadvantages of the RTGs power
source are the limited conversion efficiency (5%) and high cost. (Miller,
Keesee, 2003)
4. Fuel cells are extremely flexible. They can provide power during sunlight
and eclipse. Fuel cells have a high energy density, which causes them to
be a very compact comparing solution, especially regarding solar PV.
The main disadvantage of using fuel cells is the spaceship’s required fuel
Main power sources Georgios Galanos
5
carriage capacity. It is a good primary source for manned mission (Wertz
et al, 2015).
5. Dynamic and chemical power sources are to be applied in future
missions (Wertz et al, 2015).
The table below provides an overview of the available technology options and
their status.
Table 2-1 Technology options and status (Patel, 2005)
Main power sources Georgios Galanos
6
2.1 Comparison of primary power sources based on mission’s
requirements
The selection of the primary power source must be based on the mission’s
requirements. For the RIICS mission the main requirements that affect the
power source selection are the following:
• Cost
• Orbit
• Lifetime
• Power consumption
The RIICS spacecraft is a small-sized spacecraft, which requires some
hundreds of Watts to operate. Its lifetime is estimated to be 6 years with the
option of extension, if possible. The figure below is the main guide for the
decision of the main power source.
Figure 2-1 Energy sources options for various power requirements (Angrist, 1982)
Power Control Georgios Galanos
7
According to the requirements of the mission, fuel cell, Radioisotope – TE and
solar PV with secondary batteries appear to be the most suitable approaches to
our mission.
Fuel cells and RTG have specific cost in the order of tens of thousands of $/W.
In the case of PV technology the cost ranges between 300 and 900 $/W (Wertz
and Larson, 1999). Solar dynamic systems have a cost range between 1000
and 2000 $/W, and are designed to provide much more power (Patel, 2005).
The combination of PV cells and secondary batteries is the most common and
safe method of power supply for missions orbiting the Earth or orbiting the L1
point. Overall, it may be said that in order of cost, reliability and simplicity solar
PV cells and secondary batteries are chosen as primary and secondary power
source (Johnson, 2012).
3 Power Control
“Bus voltage level, power generation and energy storage must be jointly
selected to optimize the total power” (Patel, 2005). Patel states that the design
of an Electrical Power System is very complex because of the linkage between
the system components. The size of the solar panels, batteries, general
architecture of the system, bus voltage and system components discussed
below are interacting with each other in such manner that many iterations must
be made in order to achieve the desired result. It will be noticed that throughout
this report, system components are being mentioned that are only being
discussed in later chapters.
The voltage source of a spacecraft must provide the required amount of voltage
for each load. Spacecraft’s loads often require different amounts of voltage than
the voltage amount the bus operates with (Wertz et al, 2015). DC-DC voltage
converters are generally used to control and adjust the voltage amounts.
Considering that all power requirements of the subsystems and instruments are
known, a DC-DC converter is able to spread the voltage to the subsystems as
Power Control Georgios Galanos
8
required. A DC-DC converter can also maintain the voltage, which is specified
by the load, within a range.
The bus must be able to control the electrical power for all subsystems and
instruments so to prevent overcharging the battery or overheating other
subsystems or instruments, including the electrical system. To control the power
bus two techniques are usually being applied: direct energy transfer (DET) and
peak power tracker (PPT) (Wertz et al, 2015). The main difference between the
two technics is the system’s reaction to the power generated by the solar
panels.
3.1 Direct Energy Transfer (DET)
In the case of DET, the power input deriving from the solar panels is being
transferred directly to the bus. As a result, all the subsystems must run by using
the same power used by the bus. In the case that a subsystem requires more
power than the available, the battery may provide the extra required power.
A shunt regulator is usually applied to the DET system in order to increase its
efficiency and reliability (Wertz et al, 2015). The shunt regulator operates in
parallel to the solar arrays and keeps the current of the arrays away from the
subsystems and battery when it is not needed. A DET - shunt regulator system
provides high efficiency at the EOL, low mass system and cost efficiency.
However, one disadvantage is that the DET system cannot operate peak power
requirements without the power support of the battery.
The DET system can be divided into two categories: fully regulated bus and
sunlight regulated bus (often referred as unregulated bus) (Patel, 2005).
3.1.1 Fully regulated Bus
Fully regulated bus, which is also known as regulated bus, controls the bus
voltage within a range of ±2 to 5% of the nominal voltage during the entire
mission (Patel, 2005). The following figure describes the architecture of a
Power Control Georgios Galanos
9
regulated bus. This type of system allows the batteries to be used in parallel
with the solar arrays, which improves the system’s reliability.
Figure 3-1 Regulated Bus DET (Patel, 2005)
3.1.2 Sun - Regulated Bus (Unregulated Bus)
To minimise the complexity of the spacecraft and the power system it is more
convenient to distribute power from both sources (solar panels and secondary
batteries) but not in parallel. The case of a direct energy transfer to the bus is
known us sun–regulated bus or unregulated bus. In this method the bus voltage
is regulated during daytime via the shunt control and is unregulated during
night-time. The basic difference between a regulated and an unregulated bus is
found on the Power Regulated Unit. In the unregulated bus, the battery charger
regulator controls the battery during daytime, however, a discharge converter is
not included in the architecture, which leads to battery discharges during night-
time via a diode ‘d’ called ‘battery discharge diode’. The battery disconnects
from the bus during day-time while it is been regulated by the shunt controller.
The system allows only the battery to be discharged at night-time and blocks
any uncontrolled charge current received from the battery (Patel, 2005). The
basic architecture of such system is the following:
Power Control Georgios Galanos
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Figure 3-2 Sun- Regulated Bus (Unregulated Bus) DET (Patel, 2005)
3.1.3 Comparing Regulated and Unregulated Bus
The power system must take into consideration both day–time and night–time
phases of the mission.
A full-regulated bus is usually applied in GEO orbits where the power
requirements are above 3kW, whereas the unregulated bus is mostly used in
satellites with requirements below 3kW. (Patel, 2005)
The sun–regulated bus is often less complex and reliable than the fully
regulated bus. The main disadvantage is that the battery cannot be used during
daytime as it is disconnected from the bus. The fact that a battery charger
converter is missing contributes in reducing the system’s cost and power.
On a fully regulated bus operation, the battery can be used during daytime. The
attendance and use of a battery when peak power is required, leads to the
reduction of the area, mass and cost of the solar arrays and could save up to
20% of the mass and area of the solar panels. By using a fully regulated bus the
mission automatically becomes more reliable as the bus is continuously
Power Control Georgios Galanos
11
regulated and can provide the required voltage to the loads at any time.
Nowadays, most of the space missions are using regulated buses.
3.2 Peak Power Tracker (PPT) - Power control
It is known that solar arrays generate more power at the BOL and during cold
phases of the mission at higher voltage rates. The maximum power of the
system occurs at a point where, the power is transferred by the solar arrays at
the maximum power and operates at maximum efficiency (Jiang et al, 2002).
The maximum power point of the solar arrays can be varied with time, solar
radiation, temperature and lifetime of the solar panels (Huynh and Cho, 1999).
A suitable switching regulator must be located between the solar arrays and the
bus to control the maximum power voltage that the solar arrays produce and the
voltage that the loads need to be supplied with. The figure below displays the
main architecture of a Peak Power Tracker system.
Figure 3-3 Peak Power Tracker Architecture (Patel, 2005)
The series-switching regulator stays constant at the maximum power producing
voltage using the peak power tracker. The output voltage can be adjusted to the
required level by varying the duty ratio controller. The peak power tracker can
be activated while the battery is being charged. If not, the power that left in the
solar arrays can increase their temperature.
Power Control Georgios Galanos
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PPT is mostly used for satellites that are not able to point continuously the sun
or the solar radiation and in cases when the temperature varies at a high range.
The PPT system can be designed in three ways: series, parallel and series–
parallel as shown in the figure below.
Figure 3-4 Battery charge and discharge options in peak power tracking architecture.
(Patel, 2005)
3.3 Power Control Trade-off
The table below indicates the pros and cons of each option. Cost, mass and
efficiency are the most important variables in every mission. The table shows
the best application for each case, which is not always valid since parameters
other than the cost, mass and efficiency may be equally important.
Power Control Georgios Galanos
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Table 3-1 Advantages and Disadvantages of different architectures (Patel, 2005)
According to past missions, any architecture is suitable for specific missions,
however it is proved that this is not always true. For small satellites, which
require less than 500W of power and have low orbits, PPT is the most suitable
solution. Between 1000W and 3000W, sun-regulated bus is the most
advantageous option. For power requirements above 3000W a regulated bus is
the best approach.
At this stage a PPT system seems to be the most matching system for a
spacecraft that demands power below 500W. The fact that the spacecraft will
orbit the L1 point may add some extra things to notice before the decision.
In the L1 point the spacecraft has been designed to face the Sun during the
whole mission at the most desirable angle between the Sun and the solar
arrays to avoid high losses. It is remarkable to notice that in the L1 point the
Power Control Georgios Galanos
14
spacecraft will never come across eclipses, which leads to the use of the solar
arrays power during the entire mission.
Despite that in the RIICS project the power requirements remain constant in the
operation phase and peak power is absent, in some cases the battery will be
used to split the power consumption (will be discussed later on). A DET
regulated system seems to be closer to our needs, as it is more reliable and
cost-effective.
3.4 Bus voltage selection
The selection of the bus voltage of the spacecraft must be linked with the power
requirement, nominal voltage of each of the loads and buses available in the
market, in order to reduce the cost. The figure below indicates that for the RIICS
project, in which the power requirement is less than 500W, a 28V bus is the
ideal solution. All the subsystems must comply with the voltage requirement of
the electrical power subsystem.
Figure 3-5 Optimum voltage for various power levels (Patel, 2005)
Solar arrays Georgios Galanos
15
4 Solar arrays
4.1 Solar PV technology
Nowadays there are plenty of choices in Solar PV technology. This report
examines the most common technologies in space applications: Silicon, Gallium
Arsenide (GaAs) single junction, Gallium Arsenide (GaAs) multijunction and
Gallium Arsenide (GaAs) triple junction. (De Luca, 2011)
Figure 4-1 Typical Solar Array Design Parameters (Wertz et al, 2015)
The chart above clearly shows that Silicon technology is the cheapest of all the
available technologies. As the power requirements increase so do the area and
mass of the spacecraft. According to the configuration of the spacecraft and the
launcher, the area of the solar arrays is not as significant as the reduction of the
cost of each component (Jurian, T., 2019). RIICS spacecraft will consume an
average of 222,1W power. The latter, means that the Silicon option costs
around 126,000$, and for the GaAs (SJ), GaAs (MJ), and GaAs (3J) the costs
are 283,000$, 232,000$ and 206,000$ respectively. Silicon technology is the
most inexpensive solution for the spacecraft. As mentioned previously, this
project aims to minimise the total cost of the mission and for that reason Silicon
0
5
10
15
20
25
30
35
Area
(m2)
Weight
(kg)
Cost ($)
x 10^4
Power
BOL (W)
x 10
Power
EOL (W)
x 10
Solar array type Trade - off
Silicon
GaAs (SJ)
GaAS (MJ)
GaAs (TJ)
Solar arrays Georgios Galanos
16
technology was chosen. The performance of the power system can be adapted
and provide the required power at the Beginning of Life and End of Life at the
same level of efficiency.
4.2 Solar array structure
The configuration of the solar arrays can be divided into planar and
concentrator (Wertz et al, 2015) and each type can be divided in body or panel
mounted. Up to date, results from past missions, show that most of the satellites
use planar arrays.
4.2.1 Rigid Panels
A traditional way to build the solar array is to mount the cells onto a rigid
substrate often made from aluminium and carbon face sheets. Solar cell
insulation sheets like Kapton®
, Kevlar®
and fiberglass are able to successfully
reduce the mass of the array (Wertz et al, 2015). Cover glass such as fused
silica Microsheet ®
is used to protect the array from the space environment. To
successfully produce more output power by the cell, an antireflective coating is
installed so to minimise the light reflection and allow the sunlight energy to be
absorbed by the solar cells. A coating that controls the temperature of the
surface must cover the back site of the array (Patel, 2005). The following figure
displays one wing of a rigid panel solar array.
Figure 4-2 A fully deployed dollar array (Patel, 2005)
Solar arrays Georgios Galanos
17
The solar arrays are stowed with the satellite structure in the launch vehicle until
the phase of the separation when the solar arrays are deployed. This particular
method is discussed in the mechanism’s report (Liébana Moradillo, O., 2019).
Figure 4-3 Panels section with cells mounted on a honeycomb substrate with face
sheets (Patel, 2005).
4.2.2 Body–Mounted
Body-mounted planar cells are typically used on spinning spacecrafts. During its
rotation, the spacecraft’s surface can capture the energy of the Sun. The solar
cells can increase their thermal energy, however, the constant rotation of the
spacecraft does not allow the temperature increase of the spacecraft’s
elements. Body-mounted cells operate in less efficiency compared to deployed
solar cells, as they have to run in higher temperatures. The main disadvantage
of body-mounted cells is that the area of the solar arrays will be increased
because the cells are not illuminating all the time. Consequently, the overall
cost increases, a fact that this project attempts to eliminate. RIICS spacecraft is
a 3-axis stabiliser spacecraft that needs to be stable to operate its science
functions, thus it is more convenient to use panel mounted solar arrays (Wertz
et al, 2015).
Solar arrays Georgios Galanos
18
Figure 4-4 A body mounted solar array (Patel, 2005)
4.2.3 Three or More Wings
This solar array construction is generally used for small science mission
satellites with Peak Power Tracker. It practically offers the same benefits as a
body-mounted array, for the reason that the arrays do not always face the sun.
The benefit of using three or more wings is that the solar arrays do not interfere
with any of the instruments located on the spacecraft body. The three or more
wings construction needs different Peak Power Tracker for each of the arrays,
or else the arrays will obstruct each other (Patel, 2005).
Figure 4-5 Three wings array architecture (Patel, 2005)
Solar arrays Georgios Galanos
19
4.2.4 Flexible Array
Hubble Space Telescope and ISS are the most well-known satellites to use a
flexible array construction. As in the rigid panel method, the arrays are stowed
on the spacecraft when the spacecraft is in the launch vehicle and rolled out or
deployed like an accordion panel after the spacecraft’s separation with the
vehicle. As all the constructions, protection from thermal risks and control of
temperature differences when exiting the eclipses must be assured. In cases
where a flexible array is not totally flat, a reduction of the power output of the
array could occur. A temperature difference reshapes the array. Once the
temperature is being equalised, which should happen approximately 30 minutes
after the temperature changes, the array returns to its normal flat shape. This
inefficiency of the solar arrays is something that a rigid panel will never face as
it transfers the front heat to the back in a very quick way (Patel, 2005).
4.2.5 Selection of Construction
There is one more construction called concentrator. Concentrator construction
uses mirrors and lenses to collect more sun light in order to generate more
power. This construction adds more complexity to the system, therefore it has
not been taken into consideration (Wertz et al, 2015).
The RIICS spacecraft is designed be a 3-axis stabilised satellite. This
information tends to discharge the possibility of having a body-mounted array,
since it is commonly used for a spinning spacecraft (Wertz et al, 2015).
Moreover, the instruments and payload of the body mounted array spacecraft
will face very high temperatures and add complexity to the thermal design.
Finally, the spacecraft in this project uses its outer surface to accommodate
instruments, as a result there is no available surface area to provide the
required power.
Rigid panels is the selected solar construction as it is the most common, reliable
and less complex system. It is also used on 3 axis-stabilised spacecrafts. It is
important to notice that in the configuration of the spacecraft, the solar arrays
Energy storage - Secondary battery Georgios Galanos
20
are able to track continuously the sun but with a worst-case scenario incidence
angle to be accounted (will be discussed later on the report). Two rigid arrays
consisted of 3 panels each, form the solar panel system. The figure below
indicates the existing design of the solar arrays.
Figure 4-6 Final design of the Solar arrays (Jurian, T.,2019)
5 Energy storage - Secondary battery
Secondary batteries are commonly used during times of eclipses and peak
power requirements for energy storage. As mentioned previously, this project
does not call for an eclipse, given that the spacecraft will orbit the L1 point. A
secondary battery will be used to provide enough power in case of emergency
and Peak Power in the course of the mission. The power system size and its
various design options will be thoroughly discussed later in the report.
Individual cells connected in series or parallel create a pack of batteries. The
number of the individual cells required depends on the bus voltage
requirements and can be defined by the following table.
Table 5-1 Number of cells as a factor of bus voltage (Samina Asif,2008)
Energy storage - Secondary battery Georgios Galanos
21
The decision of the number of cells per battery is made after the analysis of the
available battery types.
There are some basic parameters that should be considered prior to the design
of the battery and the type selection. The battery must always provide constant
voltage when required. Table 5-2 displays the issues in designing a secondary
battery.
Table 5-2 Issues in Designing the Energy Storage Capability (Wertz et al, 2015)
The conversion from chemical into electrical power and reverse is done by the
battery. A secondary battery can perform these operations up to thousand times
during its lifetime. The selection of a secondary battery is basically done by
taking into account the capacity of the battery, cost, weight, cycle life
(depending on the depth of discharge) and the way the spacecraft is going to
use it. In this project the secondary battery must be of low-cost and have long
cycle life capability in order to provide enough power throughout the mission.
5.1 Types of secondary batteries
Nowadays spacecrafts use mostly three types of secondary batteries: Nickel-
Cadmium (Ni-Cd), Nickel-Hydrogen (Ni-H2) and Lithium Ion (Li-Ion) (Broussely
Pistoia and Knovel, 2007).
Up to the 80’s, Nickel-Cadmium battery was the traditional battery for 28V
spacecrafts and buses. It usually consisted of 22-23 series-connected cells.
Their nominal capacity ranges between 5 and 100Ah. Today, Nickel-Cadmium
Physical Size, weight, configuration, operating position, static and
dynamic environments
Electrical Voltage, current loading, duty cycles, number of duty cycles,
activation time and storage time, limits on depth of
discharge, and short-circuit (fault) recovery
Programmatic Cost, shelf and cycle life, mission, reliability, maintainability,
produceability and safety
Energy storage - Secondary battery Georgios Galanos
22
batteries’ application is considered to be extensive and very low risk – related to
the storage system missions (Wertz et al, 2015).
After the Nickel-Cadmium battery was introduced to the industry, Nickel-
Hydrogen (Ni-H2) batteries became the most common energy storage. Ni-H2
design configuration can be divided into three categories: single pressure
vessel, common pressure vessel and individual pressure vessel. The main
difference between each of the categories of a Ni-H2 battery is the diameter of
the cells and their working terminal voltage (Wertz et al, 2015).
Li-Ion batteries have significant advantages over Ni-Cd and Ni-H2 batteries. This
kind of battery technology offers a reduction in size, higher energy density,
higher efficiency, less complexity, less costly thermal control system and lower
self-discharge rate. The main disadvantage of the Lithium Ion batteries is that
they are are approximately double the cost of Ni-Cd and Ni-H2 (Patel, 2005).
The main characteristics of each type of batteries are shown on the table below.
Battery Type Ni-Cd Ni-H2 Li-ion
Energy Density of Battery
(Whr/kg)
30 60 125
Cycle life (80% DoD) 750 500 1500
Self discharge (per month)
*100%
0.5 0.3 0.05
Cell Voltage (V) 1.2 1.2 - 3 3.7
Charge temperature
(Celsius)
0 - 40 -20 - 30 10 - 25
Discharge temperature
(Celsius)
-20 - 65 -20 -65 -20 - 60
Maintenance requirement Full discharge
every 90 days
when in full use
Full discharge
every 90 days
when in full use
Free
Table 5-3 Characteristics of Selected Secondary Batteries (Battery University, 2019)
As stated earlier, the battery used in this project must be not only cost-effective
but also capable of providing enough power to the loads. The Nickel-Cadmium
battery seems to be the ideal solution as it is reliable and economical. The only
disadvantages of the Nickel–Cadmium battery and its cycle of life and mass.
Analyze and Size the Power System Georgios Galanos
23
The RIICS spacecraft must be able to provide a charge/discharge mode for
around 1800 cycles through the mission. It is obvious that if Nickel batteries
were used, the system would require more than 4 batteries (one additional for
redundancy), which would lead to higher battery system mass and possibly
higher launching cost. Moreover, the battery must be able to be regulated from
the PCDU. As it will be explained in the following chapters, the only available
charge/discharge regulator provided by TERMA regulates only Lithium battery
systems. In addition to all the above, Clyde Space (2010) states: “Li-Ion is fast
becoming the main energy storage technology used in space applications (Li-
ion is used on ESA deep space missions Rosetta, RoLand, Mars Express, and
many more missions including all of SSTL's recent small satellite missions)“. To
conclude, a Lithium Battery is the best approach in this particular project,
considering the cycle life of the mission, high cost due to a higher launch mass,
and charge/discharge regulator factor.
6 Analyze and Size the Power System
The power subsystem is generally quite complex. It is often interacting with the
rest of the subsystems. This system is so vulnerable that each iteration could
create undesired system alternations. This chapter examines the two most
feasible and reliable Power System designs. The effort to minimise the cost,
mass and area is not always leading to a single solution. Consequently, a trade-
off must be applied.
The only constraint in deciding the final design of the Power system is the
minimisation of costs, which is the main objective of this study.
6.1 Study Case 1
After collecting the inputs of all the subsystems, the study proceeds with the first
iteration of the design. The analysis of the power requirements of each of the
subsystems proves that the design is simple and of low cost. The power
requirements for each of the subsystems remain stable only in the operational
Analyze and Size the Power System Georgios Galanos
24
modes. This conclusion means that there is no need for Peak Power or battery
use in these modes. For that reason the Power system could be designed in
such way that the solar arrays could supply the required energy to the loads at
any time of the mission without the use of batteries. This design will occur by
increasing the solar arrays area to provide enough power during the BOL and
EOL. The battery should be used only in emergencies, resulting in adding only
one pack of batteries to the system. All types of emergencies must be studied
and included in the system design. The RIICS mission is a low cost mission of
as high reliability as possible. For that reason, in the event of both solar arrays
failing to provide the required power, the satellite will still operate normally. The
satellite will automatically switch to survival mode, in which all the subsystems
will operate the minimum number of actions possible. The survival mode has
been designed to provide enough power to all the subsystems to survive for 24
hours or until the issue has been resolved. In the event of different emergency
scenarios, the duration of the mode can be extended, given that there is no limit
of power. The solar arrays will provide the necessary power. The specifications
of this design are shown on the following tables.
Solar arrays Case 1
Area (m2
) 4.6
Cost ($) 187,200
Mass (kg) 10.5
Power available (W) 424
Table 6-1 Solar Arrays Specifications Case 1
Table 6-2 Battery Specifications Case 1
Battery Case 1
Mass (k) 7.9
Cost ($) 2,374
Capacity (Whr) 989
Analyze and Size the Power System Georgios Galanos
25
Total Case 1
Mass (k) 18.4
Cost ($) 189,574
Table 6-3 Total Specifications Case 1
Although case study 1 is simple to design and it is of low mass, its relatively
high cost does not make it a good enough case for such missions.
6.2 Study Case 2
After working on the first design of the Power system of the spacecraft, the next
step is to investigate the possibility of further system improvements. Improving
the cost factor is essential for a small consuming spacecraft. An area of 4,6 m2
solar arrays appears to be large and costly compared to similar low power
consuming spacecrafts. The maximum power that the subsystem requires is
about 330W and with a direct energy transfer system the available power has to
be 412W. These amounts derive from the need in generating power from the
solar arrays during the mission. During the phases from the start-up mode until
the spacecraft reach the L1 point and starts the operation mode, there is need
of peak power. Consequently, the power system will oversized in order to
provide the required power. All these factors increase the final area required. In
order to minimize the space used by the solar arrays on the spacecraft, is best
to make use of the battery for peak power demands. As previously discussed,
peak power is required only in phases prior to the mission’s operational phase.
It also adds complexity to the design. The use of battery for peak power will add
one more component to the power system, as two batteries will require (one
extra for redundancy). According to this design, the spacecraft is already using
a battery for phases before the operational phase and for that reason a study
was carried out as for the use of the battery for splitting the power requirements
for the operational phase and decreasing even more the space used by the
solar arrays. In this design, the mass will be higher given the need for 3 battery
Analyze and Size the Power System Georgios Galanos
26
packs because of the length of the mission and the need of redundancy. The
main specifications of this case study are included in the following tables.
Solar arrays Case 2
Area (m2
) 3.06
Cost ($) 125,931
Mass (kg) 7.1
Power available (W) 278
Table 6-4 Solar Arrays Specifications Case 2
Battery Case 2
Mass (k) 23.73
Cost ($) 7,120
Capacity (Whr) 989
Table 6-5 Battery Specifications Case 2
Total Case 2
Mass (k) 30.8
Cost ($) 133,051
Table 6-6 Total Specifications Case 2
6.3 Comparison of Cases
Understanding the requirements of the mission is of utmost importance in the
process of selecting one of the above case studies. The first case study
includes the use of solar arrays and a secondary battery in the event of an
emergency. Installing such system would only reduce the weight of the
spacecraft, as the cost and the area of the solar arrays will be very high. On the
other hand, the second case of using both solar arrays and batteries for
providing power would reduce the cost and the total area of the system but not
the system’s mass. The graphs below indicate the most important differences
between the two options.
Note: The charts below include a scaled method for comparing the values.
Analyze and Size the Power System Georgios Galanos
27
Figure 6-1 Solar arrays comparison
In the comparison of the two study cases in regards to the solar arrays design, it
can be seen that based on all specifications the second case study is more
efficient. Case study 1 calls for a larger solar array to cover the power demand
of the mission. It is essential to underline that in the first case study the
unexploited power will be dissipated and put more pressure on the thermal
subsystem. In the second case study however, the dissipated power from the
solar arrays is used directly to charge the batteries. In addition, a Maximum
Power Tracker (MPP) system could possibly be added in the first case study to
ensure constant maximum power availability. This observation leads to a small
reduction of the power available, as the efficiency of a MPP system is slightly
higher than a DET system. As a result, the area of the solar arrays could be
significantly reduced, which makes a third study focusing on a MPP system
unnecessary. For all the above, case study 2 is a better approach regarding the
design of the solar arrays, especially considering the cost minimization factor. A
discussion on the battery and total compression is following, which will give a
better understanding of the two studies.
0
2
4
6
8
10
12
14
16
18
20
	Area	(m^2)	 	Cost	($)																
x	10^4	
	Mass	(kg)		 	Power	
available	(W)																											
x	10^2	
Case	1	 4.6	 18.72	 10.5	 4.24	
Case	2	 3.06	 12.59	 7.1	 2.78	
Axis	Title	
Solar arrays
Analyze and Size the Power System Georgios Galanos
28
Figure 6-2 Batteries Comparison
As for the battery design, case study 1 is the ideal solution. Figure 6-2
Batteries Comparison proves that the mass and cost of the first case study
are significantly lower than the second case study. It is important though to
note, that in both cases a Lithium battery is been used, as already discussed in
Chapter 5.1. Using batteries in the cases of peak power and power split
requirements for a 6-year lifetime mission, would increase the required quantity
of the batteries to complete the mission in a reliable and safe manner.
0
1
2
3
4
5
6
7
8
9
10
	Mass	(kg)	x	10	 	Cost	($)	x	10^3	 	Capacity	(Whr)															
x	10^2	
Case	1	 0.79	 2.3735	 9.89	
Case	2	 2.373	 7.12	 9.89	
Axis	Title	
Battery
Analyze and Size the Power System Georgios Galanos
29
Figure 6-3 Total Mass and Cost Comparison
The final step for the selection of the ideal design approach is to compare the
results of the most important parameters of the designs, mass and cost of the
power system. The above diagram shows the inversed results in the two cases,
a fact that adds complexity in making the final decision. This study aims on the
minimisation of the cost, which simplifies the decision process. After examining
the launch and configuration system (Jurian, T., 2019), (Picavez C., 2019), the
mass of the power system shows only a 12kg difference, which is not a
significant factor in the decision process. On the other hand, the area utilized by
the solar arrays has to be as small as possible. For these reasons, case 2 has
been selected as the final design of the power system. The sizing and analysis
of the power system design is discussed in Chapter (7).
6.4 Power Consumption Analysis
The most important requirement for the power system is to be able to generate,
control, distribute and store the energy and provide the appropriate power to all
components during the mission. To examine if this requirement is applied to our
mission, the study conducts a power breakdown. Analysing the power
0
5
10
15
20
25
30
35
Mass (kg) Cost ($) x10^4
Total
Case 1
Case 2
Analyze and Size the Power System Georgios Galanos
30
breakdown derives a better overview of the design selection and process that
was followed to complete it.
The first step is to discuss the process followed to size the battery and solar
arrays. By having the results and the power breakdown from the first simple
design, which was exclusively based on the use of solar arrays as a power
source, the study attempts to reduce the solar array space. Table 6-1, Table 6-2
and Table 6-3 provide the basic specifications of the first power system’s design.
The battery has been sized at first for emergencies. After the selection of the
second case, in which the battery supports the system in peak power and
power split requirements during the operational phase, the power availability of
the existing battery in the event of peak power has to be examined. As it can be
seen from the table below, the total energy battery discharge in any phase is
much lower than the total energy of the battery (988Whr), therefore there is no
need to oversize the battery.
Phase Subsystem Energy
Discharged
(Whr)
Total Battery
Discharge (W)
Orbit Transfer Payload 221.1
Structure and
Mechanics
Thermal
Comms 61.2
OBDH
ADCS
Propulsion 160.6
Sun Safe During
Commissioning
Payload 169.35
Structure and
Mechanics
1.4
Thermal
Comms 150.25
OBDH
ADCS 12.70
Propulsion 5
Analyze and Size the Power System Georgios Galanos
31
Start up Payload 49.44
Structure and
Mechanics
1.34
Thermal
Comms
OBDH
ADCS
Propulsion 48.1
Stand By Payload 8.4
Structure and
Mechanics
Thermal
Comms
OBDH
ADCS
Propulsion 8.4
Table 6-7 Battery Discharge for cases tat peak power is required
A more analytical document can be found in Appendix (9C.2). The energy each
phase needs is much lower than the battery’s, which allows the operation of
more than one cycles prior to the battery charge. A study was made to calculate
the number of battery cycles that each phase can operate with in order to
extend the battery’s lifespan. The following table states the numbers concluded
by this study.
Phase Orbit transfer Sun Safe (During
commissioning)
Total Capacity of Battery
(Whr)
988.95 988.95
Capacity that needs
(Whr)
277.26 211.65
Times that battery can
be used
3.6 4.7
Duration of the Phase 173 (days) 30 (days)
Cycles of Battery 49 7
Analyze and Size the Power System Georgios Galanos
32
Phase Start-Up Stand-By
Total Capacity of
Battery (Whr)
988.95 988.95
Capacity that needs
(Whr)
61.7675 0.0105
Times that battery can
be used
16. 94185.7
Duration of the Phase 17.217 (hours) 1 (hour)
Cycles of Battery 1 1
Table 6-8 Cycle life of battery
During the research for the selection of the battery, which is discussed later on,
there were no available products in the market with an acceptable battery cycle
life and for this reason a factor of 80% of Depth of Discharge was taken into
account to provide around 1500 cycles (Battery University, 2019). It is of high
importance to use the battery efficiently and reduce the battery life cycles and
battery packs, whilst targeting the extension of the mission.
The next table displays the power consumption, charge/discharge mode,
energy consumed by the battery and power required for charging the battery
during the operational phase. A more detailed power breakdown document can
be found in Appendix 9C.1. The detailed power breakdown document contains
information about the power consumption and duration of each instrument of
the subsystems.
Phase Sub-
system
Aver.
Power
(W)
Peak
Power
(W)
Charge Dis-
charge
Energy
Disch.
(Whr)
Power
to
charge
(W)
Total
Power
(W)
Scan. Payload 56 OFF ON 222.1
Structure
/
Mechanic
s
18
Thermal 44
Comms 13.5
OBDH 33
ADCS 57.6 69 136.67
Propulsio
n
0
Analyze and Size the Power System Georgios Galanos
33
Chara.
/
NEOs
Payload 56 OFF ON 222.1
Structure
/
Mechanic
s
18
Thermal 44
Comms 13.5
OBDH 33
ADCS 57.6 69 87.74
Propulsio
n
0
Target
Acqui.
Payload 0 ON OFF 49.6 222.1
Structure
/
Mechanic
s
18
Thermal 44
Comms 13.5
OBDH 28
ADCS 69
Propulsio
n
0
Orbit
Maint.
Payload 0 ON OFF 85.54 219.1
Structure
/
Mechanic
s
18
Thermal 0
Comms 13.5
OBDH 28
ADCS 19.5
Propulsio
n
54.56
Comm Payload 0 ON OFF 137.1 221.4
Structure
/
Mechanic
s
18
Thermal 0
Comms 30.01
OBDH 33
ADCS 3.25
Propulsio
n
0
Analyze and Size the Power System Georgios Galanos
34
Table 6-9 Part of the Power Break During Operational Phase
The above table proves that there is no peak power in any of the phases except
for scanning and characterization/NEOs. This conflicts previous discussions
according to which there is no peak power in the operational phase. This
happens because on scanning and characterization/NEOs the battery shares
the power requirements of the ADCS to further decrease the solar arrays area.
Usually, the battery can be charged when not used by the system in the various
phases. In this project the battery is being used for the period of the operational
phases and modes. For that reason the battery must be charge in any phase
with available time and power for charging. Orbit maintenance, target
acquisition and communications have a total of 160 minutes available for
charging the battery.
The use of battery to split the power takes place in the operational phase. While
the battery is being used for peak power for all the other phases, operational
phase requires the maximum average power. Next chart displays the average
power for each phase of the mission.
Figure 6-4 Average Power Consumption
0.00	
50.00	
100.00	
150.00	
200.00	
250.00	
Average	Power	Consump6on	
Power	(W)
Analyze and Size the Power System Georgios Galanos
35
Based on the above chart, the battery is being used to split the power usage in
order to reduce the solar arrays area and cost. The maximum power that can be
supplied from the battery to the system during the operational phase has to be
examined. During operational phase the modes that consume the most average
power are the Scanning and Characterization/NEOs modes as it can be seen
on the chart below.
Figure 6-5 Power Consumption during Operational Phase
To examine how much power the battery can supply to these two modes in
every cycle of the mission, the study looks on the maximum time and power
available to the rest of the modes. The following table indicates the power
discharge for each mode, the available energy for the battery charge and the
power needed to charge the battery enough to secure the required amount of
energy.
Operational Mode
Battery
discharged
(Whr)
Energy
Available
to charge
(Whr)
Power
Available
(W)
Power
needed to
charge (W)
Scanning 138.67 0 0 0
Characterisation
/NEOs
84.74 0 0 0
0
50
100
150
200
250
Power(W)
Operational Phase
Scanning	
CharacterizaLon/NEOs	
Target	AcquisiLon	
Orbital	maintenance	
CommunicaLons
Solar Arrays Sizing Georgios Galanos
36
Target Acquisition 0 14.23 61.00 61
Orbit maintenance 0 22.62 99.94 96.94
Communicaitons 0 207.94 149.24 148.53
Total 223.41 244.9
Table 6-10 Battery Specifications for operational phase
The study calculates the maximum power the battery can supply in the course
of the operational phase. By using the batteries to split the Power requirements
on the operational phase the area of the solar arrays decreases by 0,3m2
and
the cost by 7000$. This is an addition reduction to the area and cost of the
system after using the battery for peak power demands. The total reduction can
be found in Figure 6-1 Solar arrays comparison
7 Solar Arrays Sizing
Nine basic parameters have to be taken into account for the solar arrays sizing:
1. Operational scheme of the mission: This parameter indicates the time when
the solar arrays must provide power to the load during the mission.
• During launch the spacecraft is not required to provide power to
the loads.
• There will be no power supply in the event that both solar arrays
fail.
2. Solar radiation variation during the mission: As the spacecraft orbits the L1
point, the distance between the spacecraft and the Sun will be between
0,9928 and 0,9891AU and the solar radiation will range between 1400,84–
1411,27W/m2
. This design is using the minimum value. The study also takes
into account the worst-case scenario, when the distance is almost 1AU and
the solar radiation is 1368 W/m2
during the start-up mode.
3. Incidence angle between Sun and solar arrays: The solar arrays have been
designed to be deployable and able to track the sun at any time of the
mission. To ensure reliability, this study also considers the scenario of facing
an undesired angle. According to the literature (Wertz et al, 2015) most of the
Solar Arrays Sizing Georgios Galanos
37
missions have ran on a 23.5 degrees value, which is the chosen angle for the
design of the solar arrays for the RIICS project.
4. Cells conversion efficiency: The efficiency of the silicon technology is
estimated to be 14,8% (Wertz et al, 2015).
5. Performance degradation: The degradation of the Silicon technology cells is
estimated to be 3,75% per year (Wertz et al, 2015).
6. Inherent degradation: The solar cells are located on a substrate, which
usually results in a 0,77 factor of losses of the solar arrays substrate area
(Wertz et al, 2015).
7. Losses due to transmission inefficiencies: For a Direct Transfer System the
losses due to transmission inefficiencies are projected to be 20%. This
amount of losses is thermally dissipated in the distribution process (Wertz et
al, 2015).
8. Power consumption of each subsystem and component: The power variation
of the solar panels that needs to be provided in the course of the mission
starts from 50.5W and can get up to 222,.W.
9. Power to be provided by the battery: The amount of the power that batteries
need to provide to the system ranges from 4.01W to 171.5W.
After examining all the parameters (the design selection, design selection
analysis and worst-case scenario) the study proceeds in the calculation of
the final size of the solar arrays. In the worst-case scenario, the solar arrays
must be able to provide 222.1W of power to the loads. This leads to a total
3.07m2
area of solar panels and 125,930$ cost. The main features of the
solar arrays are displayed on the table below
Solar Arrays Features
Solar cell efficiency 0.148
DET system efficiency 0.8
Inerent degradation 0.77
Solar cell degradation per year 0.0375
Sun angle (deg) 23.5
Specific cost ($/W) 378
Solar Arrays Sizing Georgios Galanos
38
Maximum Average Power (W) 222.1
Mass (kg) 7.05
Area (m^2) 3.07
Cost ($) 125,930
Table 7-1 Solar arrays main features
7.1 Battery’s Component Selection
The battery component was selected from the available space applications
market, so to achieve the minimisation of the cost. However, the cost of the
batteries is not available in this study. The calculations were made according to
Patel’s references. A 0.3% per day of self-discharge has also been taken into
consideration (Broussely Pistoia and Knovel, 2007).
The trade-off was made between the products that are provided by SAFT. VES
100, VES 140 and VES 180 were included in the trade-off (Saft, 2008).
To select the appropriate component, the study calculates the total cycles of the
battery to ensure that the selection will be made by the most efficient approach.
The component must provide the necessary energy to the closest approach in
order to reduce the required quantities regarding the cycles of the mission. The
total cycle life of the battery must be over 1881 cycles. This amount of cycles of
life is adequate for all operations from BOL to EOL, however it excludes
emergencies. Case of emergencies will be included later on.
The PCDU will regulate the 28V bus and examine the effects of having lower
battery voltage on the operation of the mission. Given that no price for the
battery has been provided, VES 140 (Saft, 2008) is the selected component as
it is matching the appropriate requirements of the mission. Appendix 9C.2.3
shows the technical specifications of the cells.
7.1.1 Configuration
The specific energy of the VES 140 is sufficient for one cell to provide the
required energy to the spacecraft. As a result, the topology of the battery will be
designed in series so to reach the desired voltage.
Solar Arrays Sizing Georgios Galanos
39
The nominal voltage of each cell connected in series determines the total output
voltage. “A general guideline is to place cells in series to make the nominal
battery voltage during discharge equal to 80% and during charge about 93% of
the bus voltage” (Patel, 2005), meaning that to reach the 28V requirements 7
cells need to be placed into series. Having less or more than 7 cells will impact
the total mass of the battery and area of the solar arrays as the battery will
require more energy to charge.
The final selection of the cells’ number in series is made by taking into account
the possibility of failure of one cell. The failure of a cell will drop the output
voltage from 25.2V to 21.6V. The failure of one cell will allow the normal
operation of the battery, which means that the system will still be able to provide
the required power to the loads, given that the battery discharge and charge
regulators have approximately 21.6V output (Chapter 8).
The battery is typically designed based on the standards of the worst-case
energy demand scenario during the mission. In the RIICS project the battery is
designed to provide the required peak power in any phase and necessary
power when both solar arrays have failed (worst-case emergency). The battery
will then be charged on Sun safe Mode for 6,7hours. The table below indicates
all the parameters to design the battery according to worst-case scenarios.
Battery's Worst Case Scenario Parameters
Total Battery Discharge 791.16
Total Power Needed to charge the battery in 6,7 hours 171.51
Capacity needed 988.95
Power available during Sun Safe Mode 171.60
Table 7-2 Battery’s worst Case Scenario Parameters
The 7 series cell with the VES 140 component can provide 996.66Whr of
energy, 8Whr higher than the required without the need of parallel configuration.
For the above reasons the topology of the battery pack will be 7 cells in series.
As mentioned in previous chapters, the total battery life must be more that 1881
cycles. Lithium batteries have an average of 1500 cycles at 80% Depth of
Power Control and Distribution Unit (PCDU) Georgios Galanos
40
Discharge (Battery University, 2019). That means that the spacecraft must
accommodate two secondary batteries and an extra battery for redundancy.
The total quantity is three battery packs. The basic specifications of the VES
140 are the following:
Battery VES 140
Specific energy
(Wh/kg)
126
Mass per module (kg) 1.13
Energy (Wh) 142.38
Capacity (Ah) 39
Discharge voltage (V) 3.6
Charge Voltage (V) 4.1
Cells in series 7
Cells in parallel 1
Total capacity (Ah) 39
Total energy (Wh) 996.66
Total mass (kg) 7.91
Table 7-3 VES 140 Shaft Battery
As the power system includes 3 packs of batteries the total mass will be
23.73kg. The cost for each pack of battery is estimated to be around 2,300$
(Patel, 2005)
Finally, since the available power and capacity of the battery are higher than the
required, the batteries will not be installed with oversized margins. Therefore,
the design maintains a cost low.
8 Power Control and Distribution Unit (PCDU)
A PCDU must be able to control and distribute the power through the mission
according to the spacecraft’s needs. For that reason, a PCDU contains a
number of modules, which assist the controlled power distribution. Generally, it
is more convenient to select a PCDU from the existing market. The PCDUs
available in the market are not suitable for the power system, therefore this
project builds the PCDU from components provided by TERMA.
Power Control and Distribution Unit (PCDU) Georgios Galanos
41
To build a proper PCDU for the mission, TERMA provides a Modular Medium
Power Unit concept, which is designed for observation, navigation, science or
low power spacecrafts. The modules used to build the PCDU are all plugged in
a backplane motherboard and can be removed or replaced without any internal
wiring. The module has been designed for a 28V regulated bus with one-single
failure tolerant. Finally, the PCDU can accommodate 21 modules (Terma
space, 2012d).
The components of the PCDU are:
1) 3 Shunt Regulation Modules (S4R) (Terma space, 2012f)
2) 2 Battery Charge / Discharge Regulator Modules (Terma space, 2012a)
3) 3 Equipment Power Distribution Modules (Terma space, 2012b)
4) 4 Heater Power Distribution Modules (Terma space, 2012c)
5) 2 Pyro Firing Drive Modules (Terma space, 2012e)
6) 2 Command and Monitoring Modules
7) 1 Backplane
1. Shunt Regulation Module (S4R): During the mission the available power
from the solar arrays often differs. In many occasions the power that each
loads requires varies. For that reason it is critical to include a regulator to
the system in order to control the available power and protect the loads and
the bus by switching in and out segments of the solar arrays. The individual
segment in the shunt regulator module can be grounded to achieve the
switching out. The configuration of the S4R is a sequential switching shunt
switch regulator module and it accommodates four independent shunt cells.
This approach has the ability to feed the main bus section current via a
series diodes by a parallel switch or to feed the battery section current via
series switch and two series diodes (Terma space, 2012f). This approach is
ideal for the RIICS spacecraft as the dissipated power is directly feeding the
battery. The S4R module provided by TERMA is being designed to provide
an output power capability of 600W (more than the required output power
for the RIICS mission). Missions that have used the TERMA S4R:
Power Control and Distribution Unit (PCDU) Georgios Galanos
42
• Galileo IOV
2. Battery Charge/Discharge Regulator Module (BCDR): The module provided
by TERMA includes two power regulators, a battery Charge Regulator
(BCR) and a battery Discharge Regulator (BCDR). The system is designed
to target a Lithium battery configuration. This module consists of two battery
charging and discharging functions. The first function, which is called End
Of Charge (EOC), is the function that sets the charging limits. The battery is
charging until it reaches the maximum selected level of voltage, after this
point the battery is ready to be discharged. It is important to notice that a
telecommand adjusts the EOC voltage to eight different levels. The second
function regulates the discharge power to the main bus until the voltage
reaches the limits that have been set. This function is called End Of
Discharge. The battery at this stage is not allowed to re-enter a discharge
mode until it reaches again the minimum level of the EOD. The output
power capability of this module is 300W (higher than the required). The
Lithium battery system is been designed in a 7s topology. With this method
the nominal output voltage of the battery is 25.2V and 21.6V in the case of
cell failure. Additionally, the BDR module operates in a range of 0–25.6V
and BDR with the range of 16–27V. Therefore, in the case of failure of one
cell, the PCDU will be able to operate normally. The voltage output of the
battery is often lower than the voltage output of the bus in PCDU designs.
The BDR is a conventional step-up regulator (Jensen and Laursen, 2002)
that increases the output voltage. Missions that have used the TERMA
BCDR are the following:
• Mars Express
• Rosetta
• Venus Express
3. Equipment Power Distribution Module (EPD): This module provides a
number of protection switchers. The PCDU must be designed in a way that
all the spacecraft loads are equipped with one switch protection. The
current module, which is provided by TERMA, consists of sixteen Latching
Power Control and Distribution Unit (PCDU) Georgios Galanos
43
Current Limiters (LCL) and can be applied to the loads. There are twenty
loads on the spacecraft and for that reason three Modules are needed of
which one is for redundancy. The function of this module is protecting the
upstream main power bus from an overload or short circuit current.
Missions that have used the TERMA EPD are as follows:
• XMM-Newton
• Integral
4. Heaters Power Distribution Modules (HPD): This module is responsible for
the distribution of the bus power to the spacecraft heaters. At the moment
TERMA provides this module with sixteen output switches divided in two
groups of eight switches. Upstream LCL protects each of these groups. The
RIICS spacecraft includes thirty six heaters, which leads to the selection of
four HPDM of which one is for redundancy. Missions that have used the
TERMA HPD are the following:
• XMM-Newton
• Integral
5. Pyro Firing Drive Modules (PFD): This module is responsible for turning on
and off the valves of the thrusters. One extra module is for redundancy.
Missions that have used the TERMA PFD:
• Hispasat
6. Command and Monitoring Modules (CM): This module introduces the
communication interface to the data management subsystem. Two modules
are being accommodated, the one for redundancy. Missions that have used
the TERMA CM are:
• Mars Express
• Rosetta
• Venus Express
7. Backplane: This module interconnects the aforementioned modules and
closes the PCDU.
Conclusion Georgios Galanos
44
The main final specifications of the PCDU are the mass, width, height and
length which are 11.37kg, 235mm, 156mm and 379mm respectively.
9 Conclusion
The following conclusion summarises the final design of the Electrical Power
system.
The distribution of the power demand to the loads is achieved with a fully
regulated 28V bus working with a DET system.
Two deployable 3.07m2
solar arrays are placed on two rigid structures and
support the spacecraft with the required power during the mission. This
excludes the worst-case scenario of emergency (discussed in previous
Chapter). The two solar arrays cost 125,930$ and weigh 7.07kg.
During peak power, scanning and characterisation/detection NEOs modes and
emergencies, a battery supplies the necessary power demand. Three units of
batteries are projected to cover the entire mission, of which one battery is for
redundancy. The battery consists of a 7s cell configuration and weighs 7.91kg.
The total cost is around 6,900$ and total mass is 23.73kg.
A power control and distribution unit is being attached to ensure the efficient
operation of the solar arrays and battery and the successful and safe power
distribution to the loads. The PCDU weighs 11.37kg.
The total approximate cost of the Electrical Power will be around 133,000$ and
total weigh will be 42.17kg.
The Electrical Power system successfully covers the corresponding
requirements set by the project’s system engineers.
Further analysis of the solar cells and their configuration is essential. Studying
the sensitivity of the battery regarding temperature, actual voltage requirements
for each subsystem and instrument of the mission and more possible efficient
designs of the electrical power system is desired.
REFERENCES Georgios Galanos
45
REFERENCES
Angrist, S. W. (1982) Direct Energy Conversion, 4th edn, Copyright Allyn and Bacon,
New York)
Antonio De Luca (2011). Architectural Design Criteria for Spacecraft Solar Arrays,
Solar Cells - Thin-Film Technologies, Prof. Leonid A. Kosyachenko (Ed.), ISBN: 978-
953-307-570-9, InTech, Available from: http://www.intechopen.com/books/solar-cells-
thin-film-technologies/architectural-design-criteria-for-spacecraft- solar-arrays
Battery University (2019) Comparison Table of Secondary batteries available at:
https://batteryuniversity.com/learn/article/secondary_-batteries (accessed February
2019)
Ben Johnson (2012) Power Sources for Space Exploration, Stanford University
available at: http://large.stanford.edu/courses/2012/ph240/-johnson1/ (accessed in
November 2018)
Broussely, M., Pistoia, G. and Knovel, (2007), Industrial applications of batteries, 1st
ed., Elsevier, Amsterdam ; Boston.
Clyde Space (2010), Secondary Batteries, available at:
http://www.clydespace.com/resources/powerschool/power_storage/secondary_batterie
s, (accessed January 2019).
David W. Miller and John Keesee, Spacecraft Power System, MIT OpenCOurseWare
available at: https://ocw.mit.edu/courses/-aeronautics-and-astronautics/16-851-
satellite-engineering-fall-2003-/lecture-notes/l3_scpowersys_dm_done2.pdf, (2003)
(accessed December 2019)
Fortescue, P. W., Stark, J. and Swinerd, G. (2003), Spacecraft systems engineering,
3rd ed, Wiley, Chichester.
Huynh, P. T. and Cho, B. O. H. (1999), "Design and analysis of a regulated peak-power
tracking system", IEEE Transactions on Aerospace and Electronic Systems, vol. 35,
no. 1, pp. 84-92.
James R. Wertz, David F. Everett and Jeffery J. Puschell (2015), Space Mission
Engineering: The New SMAD, Microcosm Press, USA; Hawthorne.
Jensen, H. and Laursen, J. (2002), "Power conditioning unit for Rosetta/Mars express",
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6th European Space Power Conference, 6 May 2002 through 10 May 2002, Porto, pp.
249.
Jiang, J. -., Huang, T. -., Hsiao, Y. -. and Chen, C. -. (2005), "Maximum power tracking
for photovoltaic power systems", Tamkang Journal of Science and Engineering, vol. 8,
no. 2, pp. 147-153.
Jurian, T. 2019 RIICS: Rapid Imminent Impactor Characterisation System -
Configuration & Structures
Landis, G. A. (2006) Reevaluating Solar Power Systems for Earth, IEEE 4th World
Conference on Photovoltaic Energy Conversion 2006 , NTRS-2007-0005136.
Liébana Moradillo, O., 2019 RIICS: Rapid Imminent Impactor Characterisation System
- Operations and Mechanisms
Niels E. Jensenh (2003), Satellite Power System, ESA available at:
http://www.esa.int/esapub/br/br202/br202.pdf (accessed December 2019)
Patel, M. R. (2005), Spacecraft power systems, CRC Press, Boca Raton.
Picavez, C. (2019) RIICS: Rapid Imminent Impactor Characterisation System – Launch
System
Saft (2008), VES 180 - Rechargeable lithium battery datasheet, available at:
http://www.saftbatteries.com/doc/Documents/space/Cube712/VES%20180.e9cf5d8f-
3cbd-4921-8ac0-89d7b13bd0c0.pdf (accessed March 2019).
Salina Asif (2008) Evolutionary computation based multi-OBJECTIVE design search
and optimization of spacecraft electrical power subsystem, University of Glasgow,
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Seurin, N. 2019 RIICS: Rapid Imminent Impactor Characterisation System - System
Engineering Requirements & Risks
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https://www.terma.com/media/177695/equipment_power_-distribution_module.pdf
(accessed February 2019)
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(accessed February 2019)
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Bewick, R., CUTE, Communication and Power Subsystems. Group Design Project
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Busquets Corominas J., Marco Polo ‘Lite’, Systems engineering (Requirements,
baseline and coordination) and Electrical power subsystem. Group Design Project
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Zane Brough, Claudio Paoloni, (2015), Advanced Deployable/Rectractable Solar Panel
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6b70fa7f8fa.pdf?_ga=2.166006782.1760230267.15435815401910833425.154358154
0
Executive Summary: RIICS - Electrical Power Subsystem Georgios Galanos
49
APPENDICES
Appendix A Executive Summary: RIICS - Electrical
Power Subsystem
The Appendix A summarise the Electrical Power subsystem work package.
The main features of the Electrical Power subsystem are:
1. Two Silicon rigid deployable solar arrays, each consist of three panels.
To be able to provide the power requirement (50.5W – 222.1W) the area
of each of the array must be 1.535m2
.
2. Three pack of battery (one for redundancy). The total capacity of the
battery is 998Wh and is consists of 7 cells in series provided by saft
(VES 140 model). The total weight of the batteries is 23.73kg.
3. The total approximate cost of the Electrical Power will be 133,000$ and
weights 42.17kg.
4. A PCDU will control and distribute the power generated and will weight
11.37kg.
5. A fully regulated bus operating up to 28V.
6. No eclipses during the mission.
7. 6 years designed lifetime.
The electrical power subsystem was designed to be able to provide the required
power during the whole mission of the spacecraft in the most efficient and low
cost approach. The cost of each of the components may be different in reality.
References have been used for calculating the approximate cost of the
electrical power system and the values are not reliable.
Common Appendix Georgios Galanos
50
Appendix B Common Appendix
	
B.1 Mission objectives
Mission statement
“The	 aim	 of	 the	 mission	 is	 to	 build,	 in	 partnership	 with	 Aistech	 Space,	 a	 Physical	
Characterization	and	Scanning	System	for	small	Rapid	Imminent	Impactors”	
B.1.1 Primary objectives
● Characterization	of	imminent	impactors	to	improve	the	understanding	of	the	
small	Near-Earth	Objects	by	comparing	information	obtained	pre-impact	from	
the	spacecraft	and	post-impact	information	
● Detection	of	imminent	impactors	that	are	not	detectable	from	the	ground	by	
using	the	spacecraft	as	an	orbital	scanning	station	
B.1.2 Secondary objectives
● Detection	of	Residual	Space	Objects	(RSOs)	and	utilisation	of	Space	Surveillance	
Network	(SSN)	database	
● Classification	of	NEOs	and	detection	of	a	range	of	compounds	on	NEOs	surface	
● Exoplanets	characterisation	through	photometry	and	spectroscopy	
B.2 Key mission requirements
B.2.1 Mission performance
● Mission_01	 -	 One	 third	 of	 all	 NEOs	 not	 detected	 by	 Earth	 with	 a	 closest	
approach	distance	to	Earth	<=	0.03	AU	with	absolute	magnitude	H	<=	30	
shall	be	characterized	
● Mission_02	-	The	s/c	shall	be	able	to	obtain	the	light	curve	of	the	target	
● Mission_03	-	The	s/c	shall	be	able	to	obtain	the	reflectance	spectrum	of	the	
target	
● Mission_04	-	The	s/c	shall	be	able	to	observe	the	target	in	the	Near	Infrared	
(0.7	μm	<	𝜆	<	2.5	μm)	and	Visible	spectral	regions	(0.4	μm	<	𝜆	<0.7	μm)
Common Appendix Georgios Galanos
51
● Mission_05	 -	 The	 s/c	 shall	 be	 able	 to	 observe	 targets	 not	 detected	 by	
terrestrial	telescopes	
B.2.2 Mission constraints
● Political_Constraint	 -	 The	 mission	 shall	 satisfy	 a	 hypothetical	 mission	 call	
from	ESA’s	Space	Situational	Awareness	(SSA)	Program	
● Cost_Constraint	-	The	total	RIIC	cost	should	be	50	M€	
● Schedule_Constraint	 -	 Small-Class	 mission:	 the	 mission	 should	 be	
implemented	under	a	fast	scheme	of	5	years		
● Development_Constraint	-	The	Technical	Readiness	Level	(TRL)	should	be	5-
6	 (ISO	 scale)	 by	 the	 end	 of	 the	 short	 preparation	 phase	 and	 before	 the	
mission	adoption	
B.3 Risk
	
● Regarding	 the	 mission,	 the	 most	 critical	 work	 packages	 are:	 Payload,	
Communications	&	OBDH,	AOCS	and	Propulsion.	
Highest	Criticality	Events	 Key	prevention	actions	
Payload:	detector	
degradation	
-Payload	instruments	shall	be	protected	against	impacts	
-The	s/c	shielding	materials	should	have	high	hardness	
-Add	little	cameras	on	the	s/c	to	detect	failures	
Comms	and	OBDH:	Loss	of	
scientific	and	housekeeping	
data		
-Provide	redundancy	
-Use	dispatched	ground	stations	to	avoid	interferences	
-Mount	antennas	in	less	risky	part	(potential	impacts,	
radiations…)	considering	the	pointing	requirements	
-Provide	safe-mode	in	case	of	anomaly	
AOCS:	Wrong	attitude	of	
the	spacecraft	
-Correlate	computations	with	the	one	of	similar	past	
missions	
-Organize	frequent	team	meetings	(several	per	week)	to	
improve	communication	and	transmit	information	and	
results
Common Appendix Georgios Galanos
52
-	Apply	margins	when	designing	the	propellant	budget	
-Reduce	orbit	eccentricity	and	pointing	errors	to	acceptable	
limit	
Propulsion:	Loss	of	
spacecraft	
-Check	the	quality	of	the	system	
-Add	cameras	on	the	s/c	to	provide	follow	up	of	the	orbit	
phase	
-Ensure	electrical	continuity	of	the	surfaces	
-Prevent	propellant	mixing	between	opposite	tanks		
Table B-1 Highest Criticality Events and Key Prevention Actions
B.4 Trade-off
		 Weigh	 Geo	EW	 Geo	CH	 L1	EW	 L1	CH	 DRO	EW	 DRO	CH	
Performance	 5	 1	 2	 3	 5	 1	 1	
Impact	 4	 5	 3	 5	 3	 4	 2	
Cost	 4	 4	 5	 2	 4	 1	 2	
AOCS	demands	 3	 3	 3	 5	 5	 5	 5	
Feasibility	 2	 5	 3	 3	 3	 3	 3	
Environmental	
effects	
2	 3	 3	 5	 5	 4	 4	
Communications	 1	 5	 5	 2	 3	 1	 2	
Total	 105	 71	 68	 76	 87	 55	 52	
Table B-2 Trade off
Common Appendix Georgios Galanos
53
B.5 Budgets
B.5.1 Mass Budgets
Table B-3 Mass Budget Breakdown
Component	 Units	 Unit	mass	(kg)	 Total	dry	mass	
Propulsion	module	
Primary	thruster	 1	 5.4	 5.4	
Fuel		tank	 4	 6.81	 27.24	
Oxidiser	tank	 2	 9.29	 18.58	
2 Subsystem	 Mass	(Kg)	
Payload	 80	
Power	 10.06	
Structure	 102.36	
Mechanisms	 34.71	
AOCS	 55.13	
Communications	 31.8	
Thermal	 7.59	
OBDH	 12.8	
Margin	 5%	
Total	dry	mass	 350	
Wet	Mass	 520.17
Common Appendix Georgios Galanos
54
Pressurant		tank	 1	 6.04	 6.04	
Pyro	valve	 9	 0.16	 1.44	
Non	return	valve	 4	 0.3	 1.2	
Fill/drain		valve	 19	 0.09	 1.71	
Pressure		regulator	 2	 1.72	 3.44	
Isolation	valve	 6	 0.545	 3.27	
Filter	 7	 0.114	 0.798	
Pressure	transducer	 10	 0.14	 1.4	
Piping	 1	 15	 15	
Structure	 1	 140	 140	
Pressurent	 1	 1.27	 1.27	
Total	dry	mass	 		 		 222	
Reaction	Control	System	(RCS)	
RCS	thruster	 16	 0.33	 5.28	
Fuel		tank	 1	 2.66	 2.66	
Pressurant		tank	 1	 1.98	 1.98	
Pyro	valve	 4	 0.16	 0.64	
Non	return	valve	 2	 0.3	 0.6	
Fill/drain		valve	 7	 0.09	 0.63	
Pressure		regulator	 2	 1.72	 3.44
Common Appendix Georgios Galanos
55
Isolation	valve	 6	 0.545	 3.27	
Filter	 2	 0.114	 0.228	
Pressure	transducer	 6	 0.14	 0.84	
Piping	 1	 10	 10	
Pressurant	 1	 0.03	 0.03	
Total	dry	mass	 		 		 29.60	
Attitude	Control	and	Determination	System	(ACDS)	
Star	tracker	camera	 2	 1	 2	
Star	tracker	processor	 2	 1.2	 2.4	
Star	tracker	baffle	 2	 0.53	 1.06	
Sun	sensor	 2	 0.215	 0.43	
MIMU	 2	 4.44	 8.88	
Reaction	wheels	 4	 4.1	 16.4	
Total	dry	mass	 		 		 31.17	
Table B-4 AOCS Mass Breakdown
B.5.2 Link Budgets
Parameter	 Value	 Unit	 Comments	
Frequency	 8.45	 GHz	 X-Band	downlink	
Transmit	Power	 100	 W	 X-TWTA	
Transmit	Power	 50	 dBm	 		
Transmitter	Diameter	 1.2	 	m
Common Appendix Georgios Galanos
56
Peak	Transmitter	Gain	 37.9	 dBi	 		
EIRP	 85.9	 dBm	 DSN	34m	
Propagation	path	
length	
1.748E+06	 Km	 Maximum	distance	in	the	orbit	from	
Earth	
Space	loss	 236	 dB	 		
Atmospheric	
Attenuation	
1	 dB	 		
Other	losses	 1	 dB	 Cables,	switches	etc.	
Receiver	Diameter	 34	 	m	 		
Receiver	gain	 68.9	 dBw	 		
System	Noise	
Temperature	
28	 K	 		
Eb/No	 13.5	 dB	 		
Link	Margin	 3	 dB	 		
Required	Eb/No	 10.5	 dB	 BPSK	modulation	
Data	rate	 9.14	 Mbps	 		
Table B-5 HGA Link Budget
Parameter	 Value	 Unit	 Comments	
Frequency	 8	 GHz	 X-Band	downlink	
Transmit	Power	 100	 W	 X-TWTA	
Transmit	Power	 50	 dBm	 		
Transmitter	Diameter	 0.5	 	M	 		
Peak	Transmitter	Gain	 29.8412	 dBi
Common Appendix Georgios Galanos
57
EIRP	 77.8	 dBm	 ESA	15	m		
Propagation	path	
length	
1.74E+06	 Km	 Maximum	distance	in	the	orbit	from	Earth	
Space	loss	 236	 dB	 		
Atmospheric	
Attenuation	
1	 dB	 		
Other	losses	 1	 dB	 Cables,	switches	etc.	
Receiver	Diameter	 15	 	m	 		
Receiver	gain	 50	 dBw	 		
System	Noise	
Temperature	
133	 K	 		
Eb/No	 13.5	 dB	 		
Link	Margin	 3	 dB	 		
Required	Eb/No	 10.5	 dB	 BPSK	modulation	
Data	rate	 611.863	 Kbps	 		
Table B-6 LGA Link Budget
B.5.3 Power Budget
Phase	 Subsystem	 Average	
Power	(W)	
Peak	
Power	
(W)	
Charge	 Discharge	 Energy	
Discharged
(Whr)	
Power		
to	charge	
(W)	
Total	
Power	
(W)	
Scanning	 Payload	 56	 		 OFF	 ON	 		 		 222,1	
		 Structure	/	
Mechanics	
18	 		 		 		 		 		 		
		 Thermal	 44	 		 		 		 		 		 		
		 Comms	 13,5	 		 		 		 		 		 		
		 OBDH	 33	 		 		 		 		 		 		
		 ADCS	 57,6	 69	 		 		 136,67	 		 		
		 Propulsion	 0	 		 		 		 		 		 		
Characterisation	/	 Payload	 56	 		 OFF	 ON	 		 		 222,1
Common Appendix Georgios Galanos
58
NEOs	
		 Structure	/	
Mechanics	
18	 		 		 		 		 		 		
		 Thermal	 44	 		 		 		 		 		 		
		 Comms	 13,5	 		 		 		 		 		 		
		 OBDH	 33	 		 		 		 		 		 		
		 ADCS	 57,6	 69	 		 		 87,74	 		 		
		 Propulsion	 0	 		 		 		 		 		 		
Target	
Acquisition	
Payload	 0	 		 ON	 OFF	 		 49,6	 222,1	
		 Structure	/	
Mechanics	
18	 		 		 		 		 		 		
		 Thermal	 44	 		 		 		 		 		 		
		 Comms	 13,5	 		 		 		 		 		 		
		 OBDH	 28	 		 		 		 		 		 		
		 ADCS	 69	 		 		 		 		 		 		
		 Propulsion	 0	 		 		 		 		 		 		
Orbit	
Maintenance	
Payload	 0	 		 ON	 OFF	 		 85,54	 219,1	
		 Structure	/	
Mechanics	
18	 		 		 		 		 		 		
		 Thermal	 0	 		 		 		 		 		 		
		 Comms	 13,5	 		 		 		 		 		 		
		 OBDH	 28	 		 		 		 		 		 		
		 ADCS	 19,5	 39	 		 		 		 		 		
		 Propulsion	 54,56	 		 		 		 		 		 		
Communications	 Payload	 0	 		 ON	 OFF	 		 137,126	 221,38	
		 Structure	/	
Mechanics	
18	 		 		 		 		 		 		
		 Thermal	 0	 		 		 		 		 		 		
		 Comms	 30,01	 		 		 		 		 		 		
		 OBDH	 33	 		 		 		 		 		 		
		 ADCS	 3,25	 39	 		 		 		 		 		
		 Propulsion	 0	 		 		 		 		 		 		
Transfer	 Payload	 0	 		 ON	 ON	 221,8	 51,37	 145,32	
		 Structure	/	
Mechanics	
18	 		 		 		 		 		 		
		 Thermal	 0	 		 		 		 		 		 		
		 Comms	 2,5	 30,05	 		 		 		 		 		
		 OBDH	 28
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system
Design study for a Rapid Imminent Impactor Characterization system

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Design study for a Rapid Imminent Impactor Characterization system

  • 1. CRANFIELD UNIVERSITY GEORGIOS GALANOS RIICS: Rapid Imminent Impactor Characterization System: ELECTRICAL POWER SYSTEM SCHOOL OF AEROSPACE, TRANSPORT AND MANUFACTURING Group Design Project MSc in Astronautics and Space Engineering Academic Year: 2018 - 2019 Supervisor: Dr Joan-Pau Sánchez Cuartielles October 2018
  • 2.
  • 3. CRANFIELD UNIVERSITY SCHOOL OF AEROSPACE, TRANSPORT AND MANUFACTURING Group Design Project MSc in Astronautics and Space Engineering Academic Year 2018 - 2019 GEORGIOS GALANOS RIICS: ELECTRICAL POWER SYSTEM Supervisor: Dr Joan-Pau Sánchez Cuartielles October 2018 This report is submitted in partial fulfilment of the requirements for the degree of MSc in Astronautics and Space Engineering © Cranfield University 2018. All rights reserved. No part of this publication may be reproduced without the written permission of the copyright owner.
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  • 5. Georgios Galanos i ABSTRACT This report is part of a group project of fifteen students of Cranfield University and is the preliminary design of the RIICS mission: Rapid Imminent Impactor Characterisation system. RIICS is a science-driven mission, which aims to characterise and detect near earth objects and exoplanets as a secondary science. A low cost mission of a 50M € budget. This report is the written proof work of Georgios Galanos, a member of the group project and responsible for the electrical power subsystem of the spacecraft. This report contains an analytical design of the electrical power subsystem of the RIICS project. The main requirement of the project is to design a low cost and reliable system. The final design successfully achieved to fulfil the above requirements (low cost and reliable power system). This report assesses the final design of the electrical power subsystem. The report includes the analysis and sizing of the primary and secondary power source, and comparison of the different design options. It also includes the main power control and distribution system to the loads. Keywords: Electrical, Power, Solar P-V, Batteries, PCDU
  • 6. Georgios Galanos iii ACKNOWLEDGEMENTS First of all I would like to thank all the group members of the RIICS project and our supervisor Dr Joan-Pau Sánchez Cuartielles who was meeting us every single week from the beginning of the year to help and advise us. Moreover, I would like to thank Dr Leonard Felicetti who taught me about power systems with the most efficient way. Finally I would like to thank my family for always being by my side.
  • 7. Georgios Galanos v TABLE OF CONTENTS © Cranfield University 2018. All rights reserved. No part of this publication may be reproduced without the written permission of the copyright owner......... ii ABSTRACT ..........................................................................................................i ACKNOWLEDGEMENTS................................................................................... iii LIST OF FIGURES............................................................................................ vii LIST OF TABLES ............................................................................................... ix LIST OF ABBREVIATIONS...............................................................................xiii 1 Introduction.......................................................................................................1 1.1 RIICS Background .....................................................................................1 1.2 Electrical power background......................................................................1 2 Main power sources .........................................................................................3 2.1 Comparison of primary power sources based on mission’s requirements....................................................................................................6 3 Power Control...................................................................................................7 3.1 Direct Energy Transfer (DET) ....................................................................8 3.1.1 Fully regulated Bus..............................................................................8 3.1.2 Sun - Regulated Bus (Unregulated Bus).............................................9 3.1.3 Comparing Regulated and Unregulated Bus.....................................10 3.2 Peak Power Tracker (PPT) - Power control.............................................11 3.3 Power Control Trade-off...........................................................................12 3.4 Bus voltage selection...............................................................................14 4 Solar arrays ....................................................................................................15 4.1 Solar PV technology ................................................................................15 4.2 Solar array structure ................................................................................16 4.2.1 Rigid Panels ......................................................................................16 4.2.2 Body–Mounted ..................................................................................17 4.2.3 Three or More Wings.........................................................................18 4.2.4 Flexible Array ....................................................................................19 4.2.5 Selection of Construction ..................................................................19 5 Energy storage - Secondary battery...............................................................20 5.1 Types of secondary batteries...................................................................21 6 Analyze and Size the Power System..............................................................23 6.1 Study Case 1 ...........................................................................................23 6.2 Study Case 2 ...........................................................................................25 6.3 Comparison of Cases ..............................................................................26 6.4 Power Consumption Analysis ..................................................................29 7 Solar Arrays Sizing.........................................................................................36 7.1 Battery’s Component Selection................................................................38
  • 8. Georgios Galanos vi 7.1.1 Configuration.....................................................................................38 8 Power Control and Distribution Unit (PCDU)..................................................40 9 Conclusion......................................................................................................44 REFERENCES..................................................................................................45 BIBLIOGRAPHY................................................................................................47 APPENDICES ...................................................................................................49
  • 9. Georgios Galanos vii LIST OF FIGURES Figure 1-1 Typical Architecture of a Power System ...........................................2 Figure 2-1 Energy sources options for various power requirements ..................6 Figure 3-1 Regulated Bus DET...........................................................................9 Figure 3-2 Sun- Regulated Bus (Unregulated Bus) DET..................................10 Figure 3-3 Peak Power Tracker Architecture....................................................11 Figure 3-4 Battery charge and discharge options in peak power tracking architecture.................................................................................................12 Figure 3-5 Optimum voltage for various power levels ......................................14 Figure 4-1 Typical Solar Array Design Parameters ..........................................15 Figure 4-2 A fully deployed dollar array............................................................16 Figure 4-3 Panels section with cells mounted on a honeycomb substrate with face sheets.................................................................................................17 Figure 4-4 A body mounted solar array ............................................................18 Figure 4-5 Three wings array architecture........................................................18 Figure 4-6 Final design of the Solar arrays.......................................................20 Figure 6-1 Solar arrays comparison .................................................................27 Figure 6-2 Batteries Comparison......................................................................28 Figure 6-3 Total Mass and Cost Comparison...................................................29 Figure 6-4 Average Power Consumption..........................................................34 Figure 6-5 Power Consumption during Operational Phase ..............................35 Figure B-1 Selected Orbit.................................................................................62 Figure B-3 Soyuz ST-B - SYLDA-S dual launch configuration.........................63 Figure B-4 Mission Phases Timeline................................................................64 Figure B-5 Launch and Early Operations Phase Timeline ...............................66 Figure B-6 Commissioning Phase Timeline .....................................................68 Figure B-7 Paints and surface coatings............................................................72 Figure B-8 Overview of the shapes of the secondary structures......................74 Figure B-9 Transfer phase propulsion schematic.............................................75
  • 10. Georgios Galanos viii Figure B-10 Reaction Control Schematic after propulsion module separation.75 Figure B-11 Fully deployed spacecraft overview in its operational configuration at the L1 point.............................................................................................78 Figure B-12 Folded launch configuration combining the spacecraft and the propulsion module......................................................................................78 Figure B-13 Compatibility verification with the upper position of the SYLDA-S78 Figure B-14 List of the main components of the spacecraft .............................79 Figure B-15 Outer and Inner Structure of the main spacecraft.........................79 Figure B-16 External configuration of the main spacecraft...............................80 Figure B-17 Internal bottom body configuration ...............................................80 Figure B-18 Internal top body configuration .....................................................80 Figure B-19 Overview of the propulsion module configuration.........................81 Figure B-20 Spacecraft Overview Design ........................................................82 Figure B-21 Cassegrain Design of Telescope..................................................82 Figure B-22 Probability inside scan area centered (-120,0) .............................86 Figure B-23 Position at detection comparison with limiting magnitude 21 and 17 ...................................................................................................................88 Figure B-24 Difference between maximum apparent motion with perturbations and maximum apparent motion without perturbations .............................89 Figure B-25 Mean apparent motion for each object in degrees per day........89 Figure C-1 Shunt Regulator specifications and functional schematic.............115 Figure C-2 Pyro Firing Drive Module specifications and functional schematic .................................................................................................................116 Figure C-3 Equipment Power Distribution Module specifications and functional schematic .................................................................................................117 Figure C-4 Battery Charge / Discharge Regulator specifications and functional schematic .................................................................................................118 Figure C-5 Heater Power Distribution Module specifications and functional schematic .................................................................................................119 Figure C-6 Modular Medium Power Unit specifications..................................120
  • 11. Georgios Galanos ix LIST OF TABLES Table 2-1 Technology options and status ...........................................................5 Table 3-1 Advantages and Disadvantages of different architectures................13 Table 5-1 Number of cells as a factor of bus voltage........................................20 Table 5-2 Issues in Designing the Energy Storage Capability..........................21 Table 5-3 Characteristics of Selected Secondary Batteries .............................22 Table 6-1 Solar Arrays Specifications Case 1...................................................24 Table 6-2 Battery Specifications Case 1...........................................................24 Table 6-3 Total Specifications Case 1 ..............................................................25 Table 6-4 Solar Arrays Specifications Case 2...................................................26 Table 6-5 Battery Specifications Case 2...........................................................26 Table 6-6 Total Specifications Case 2 ..............................................................26 Table 6-7 Battery Discharge for cases tat peak power is required ...................31 Table 6-8 Cycle life of battery ...........................................................................32 Table 6-9 Part of the Power Break During Operational Phase .........................34 Table 6-10 Battery Specifications for operational phase...................................36 Table 7-1 Solar arrays main features................................................................38 Table 7-2 Battery’s worst Case Scenario Parameters ......................................39 Table 7-3 VES 140 Shaft Battery......................................................................40 Table B-1 Highest Criticality Events and Key Prevention Actions ....................52 Table B-2 Trade off...........................................................................................52 Table B-3 Mass Budget Breakdown .................................................................53 Table B-4 AOCS Mass Breakdown...................................................................55 Table B-5 HGA Link Budget..............................................................................56 Table B-6 LGA Link Budget ..............................................................................57 Table B-7 Power Budget...................................................................................60 Table B-8 Propellant mass and ΔV break down ...............................................60 Table B-9 Development Cost of the spacecraft ................................................61
  • 12. Georgios Galanos x Table B-10 Overall Mission Cost Budget..........................................................61 Table B-11 Selected Orbit.................................................................................62 Table B-12 Orbit’s Characteristics ....................................................................62 Table B-13 Transfer trajectory parameters.......................................................63 Table B-14 Mission Phases Timeline................................................................65 Table B-15 Launch and Early Operations Phase Timeline...............................67 Table B-16 Commissioning Phase Timeline.....................................................69 Table B-17 Science Operations Priorities.........................................................69 Table B-18 Thermal Control Breakdown...........................................................71 Table B-19 Main thermal control elements .......................................................71 Table B-20 Properties of the central tubes of the primary structure .................72 Table B-21 Properties of the vertical panels of the primary structure...............73 Table B-22 Properties of the horizontal decks of the primary structure............73 Table B-23 Properties of the secondary structures...........................................74 Table B-24 Size, throughout and data produced estimates for the telescope ..76 Table B-25 Final size and throughput estimates...............................................76 Table B-26 Onboard Computer performance specifications.............................76 Table B-27 Communications design hardware selection mass and power budgets.......................................................................................................77 Table B-28 Main Mechanisms Configurations ..................................................81 Table B-29 Optical Configuration of Telescope ................................................83 Table B-30 Integration time to achieve a SNR = 5 with 0.3m aperture.............83 Table B-31 Modified visible camera from the UVIS instrument specifications..84 Table B-32 NIR Spectrometer specifications....................................................84 Table B-33 Requirements imposed for baseline design ...................................85 Table B-34 Telescope performance analysis for secondary science operations ...................................................................................................................85 Table B-35 Requirement performance in Characterisation mode.....................86 Table B-36 Requirement performance in Scan mode.......................................86
  • 13. Georgios Galanos xi Table B-37 Warning time with the frozen design ..............................................87 Table C-1 Power Breakdown. Analytic Power consumption for each instrument, charge and discharge mode and total consumption of each phase.........111 Table C-2 Analytical operation of the battery during each phase of the mission .................................................................................................................112 Table C-3 Analytic data for the cycle life of the battery...................................113 Table C-4 Comparison between VES 100, VES 140 and VES 180. Specifications of each battery type...........................................................114 Table C-5 PCDU Dimensions and Mass.........................................................114
  • 15. Georgios Galanos xiii LIST OF ABBREVIATIONS AU Astronomical Unit BCDR Battery Charge / Discharge Regulator BOL Beginning of Life CM Command and Monitoring DC Direct Current DET Direct Energy Transfer DoE Department of Energy EOC End Of Charge EOD End Of Discharge EOL End of Life EPD Equipment Power Distribution ESA European Space Agency GaAs Gallium Arsenide GEO Geostationary Orbit HPD Heaters Power Distribution ISS International Space Station LCL Latching Current Limiters Li-ion Lithium MJ Multi Junction MMPU Modular Medium Power Unit NASA National Astronautics and Space Administration NEO Near Earth Object Ni-Cd Nickel Cadmium Ni-H2 Nickel Hydrogen PCDU Power Control and Distribution Unit PFD Pyro Firing Drive PPT Peak Power Tracker PV Photovoltaic RIICS Rapid Imminent impactor Characterization RSO Resident Space Objects
  • 16. Georgios Galanos xiv RTG Radioisotope Thermoelectric Generators S4R Shunt Regulation Module Si Silicon SJ Single Junction SSA Space Situation Awareness SSTL Surrey Satellite Technology TE Thermoelectric TJ Triple Junction
  • 17. Introduction Georgios Galanos 1 1 Introduction 1.1 RIICS Background RIICS mission is based on the ESA’s SSA (Space Situation Awareness Program). The SSA program has been created from the need of awareness to predict and detect man-made space orbits, in-orbit events, potential impacts of NEO’s and effects of space weather phenomena and ground based infrastructures. As a result, the life risk and other undesired situations such as the Chelyabinsk meteorite will be eliminated. NEOs can be defined as asteroids or comets that pass near the Earth. SSA program aims to understand these kinds of objects in order to decrease the risk of causing damages. Around 600,000 asteroids are known in our Solar system and 16,000 of them are classified as NEOs. Constant and efficient monitoring has to be carried out to ensure Earth is not being affected by potential impacts. RIICS mission is designed to achieve two main objectives. The first objective is the physical characterisation and scanning system for NEO’s on the order of few meters. A better understanding of the NEO’s can be obtained by characterising imminent impactors and comparing the information collected prior and to the impact. Current ground telescopes have low capability detection due to the atmosphere and the Sun effects, which can be avoided by setting the telescope in orbit (Seurin, N., 2019). During the 6-year mission (5 in operations), the spacecraft will operate secondary science with the use of the existing telescope and sensors. The observation and characterisation of exoplanets and identification of RSO (resident space objects) form the secondary science of the mission. 1.2 Electrical power background The power system is one of the most critical subsystems of a spacecraft. The failure of the power system and inability to supply the required power to the spacecraft results in the failure of the entire mission. (Fortescue and Stark,
  • 18. Introduction Georgios Galanos 2 2003) It is of high importance to design a reliable and efficient power system. In the early 80s, space agencies focused mainly on large satellites such as ISS and manned missions to the moon. The necessity of using large satellites led the agencies to design high power consuming systems. The American Nasa and DoE and the European Space Agency (ESA) made extensive studies to accomplish these requirements (SPS Concept). Many research projects were forced to slow down or even stop due to political and technical issues, regardless the critical threat of global warming (Landis, 2006). Despite that in the beginning most space agencies attempted to build large spacecrafts, nowadays space projects focus more on small satellites in order to maintain the low cost and high efficiency (Fortescue and Stark, 2003). The power subsystem has to follow one important rule: Pow_direct_01 - The power subsystem must generate, distribute and control the required power and spread it accordingly to all the subsystems during the mission (Seurin, N., 2019) To achieve this requirement, the design of each of the power system’s components must be taken into sensitive and accurate consideration. Figure 1-1 Typical Architecture of a Power System (Fortescue and Stark, 2003)
  • 19. Main power sources Georgios Galanos 3 2 Main power sources The selection of the main power source of the spacecraft depends on several parameters. The spacecraft’s configuration is one of these parameters. Weight, size limitations, constraints set by the launch vehicle and heat dissipation capability are some of the main variables that affect the power subsystem of the spacecraft (Wertz et al, 2015). The main drivers for the sizing of the power system are the lifetime of the mission, duration of each mode and respective power consumption. As every subsystem is linked to each other, attitude control scheme, orbital parameters, communications, payload, mechanisms, thermal control and on board data handling are affecting the power source selection. Payload is one of the most important subsystems that affects the power system, as it is the one that sets the limitations for all the subsystems and consequently the power subsystem. Finally, the environment of the mission is a very critical parameter that has to be taken into account. Different missions require different approaches of power sources and energy storage methods depending on the type of orbit and distance from the sun, especially if the mission is interplanetary. Spacecraft’s primary power source: • Primary batteries • Solar PV – secondary battery • Radioisotope – Thermoelectric Generators (RTGs) • Fuel cells • Solar Concentrator – Dynamic • Chemical Dynamic 1. Primary batteries are producing direct current by electrochemistry. One of their main advantage is that they are the most economical primary source for small spacecrafts with short lifetime (Miller, Keesee, 2003). 2. Solar photovoltaic power source is the most common source for spacecraft power systems as it can provide power in tens of watts to
  • 20. Main power sources Georgios Galanos 4 several of kilowatts up to 20 years lifetime. This method is converging the sun radiation power into electrical power. Hence, it is considered to be one of the most reliable and economical primary sources. In cases where the spacecraft is under eclipses, the spacecraft must provide energy from a different source due to the lack of solar power. During eclipses secondary batteries must be applied for providing the necessary power requirements. Secondary batteries are not used only for eclipses but also for emergency cases and peak power requirements for when a direct transfer power is in use (Jensenh, 2003). 3. As previously noted, the type of the mission is one of the main parameters taken into account. RTGs are used generally for interplanetary missions, particularly in deep space, where the power consumption is very large. One of the main advantages of RTGs is its capability of generating power in the absence of the sun and can last up to several decades (The Viking landers were operating for 4-6 years supplied by RTGs). Moreover, it is insensitive to the cold of the deep space and can be exposed to the high radiation space fields. More power can be supplied proportionally to the spacecraft’s mass. No moving parts and absent of fluids, safe and flight-proven, and free of maintenance are some extra advantages of the RTGs that make that power source very reliable. On the other hand, the fact that RTGs cannot be turned on and off and the power is decreasing exponentially with time makes it undesired for many types of missions. From the thermal control point of view, RTGs must be under cooling mechanisms and coverage during the course of the mission. The main disadvantages of the RTGs power source are the limited conversion efficiency (5%) and high cost. (Miller, Keesee, 2003) 4. Fuel cells are extremely flexible. They can provide power during sunlight and eclipse. Fuel cells have a high energy density, which causes them to be a very compact comparing solution, especially regarding solar PV. The main disadvantage of using fuel cells is the spaceship’s required fuel
  • 21. Main power sources Georgios Galanos 5 carriage capacity. It is a good primary source for manned mission (Wertz et al, 2015). 5. Dynamic and chemical power sources are to be applied in future missions (Wertz et al, 2015). The table below provides an overview of the available technology options and their status. Table 2-1 Technology options and status (Patel, 2005)
  • 22. Main power sources Georgios Galanos 6 2.1 Comparison of primary power sources based on mission’s requirements The selection of the primary power source must be based on the mission’s requirements. For the RIICS mission the main requirements that affect the power source selection are the following: • Cost • Orbit • Lifetime • Power consumption The RIICS spacecraft is a small-sized spacecraft, which requires some hundreds of Watts to operate. Its lifetime is estimated to be 6 years with the option of extension, if possible. The figure below is the main guide for the decision of the main power source. Figure 2-1 Energy sources options for various power requirements (Angrist, 1982)
  • 23. Power Control Georgios Galanos 7 According to the requirements of the mission, fuel cell, Radioisotope – TE and solar PV with secondary batteries appear to be the most suitable approaches to our mission. Fuel cells and RTG have specific cost in the order of tens of thousands of $/W. In the case of PV technology the cost ranges between 300 and 900 $/W (Wertz and Larson, 1999). Solar dynamic systems have a cost range between 1000 and 2000 $/W, and are designed to provide much more power (Patel, 2005). The combination of PV cells and secondary batteries is the most common and safe method of power supply for missions orbiting the Earth or orbiting the L1 point. Overall, it may be said that in order of cost, reliability and simplicity solar PV cells and secondary batteries are chosen as primary and secondary power source (Johnson, 2012). 3 Power Control “Bus voltage level, power generation and energy storage must be jointly selected to optimize the total power” (Patel, 2005). Patel states that the design of an Electrical Power System is very complex because of the linkage between the system components. The size of the solar panels, batteries, general architecture of the system, bus voltage and system components discussed below are interacting with each other in such manner that many iterations must be made in order to achieve the desired result. It will be noticed that throughout this report, system components are being mentioned that are only being discussed in later chapters. The voltage source of a spacecraft must provide the required amount of voltage for each load. Spacecraft’s loads often require different amounts of voltage than the voltage amount the bus operates with (Wertz et al, 2015). DC-DC voltage converters are generally used to control and adjust the voltage amounts. Considering that all power requirements of the subsystems and instruments are known, a DC-DC converter is able to spread the voltage to the subsystems as
  • 24. Power Control Georgios Galanos 8 required. A DC-DC converter can also maintain the voltage, which is specified by the load, within a range. The bus must be able to control the electrical power for all subsystems and instruments so to prevent overcharging the battery or overheating other subsystems or instruments, including the electrical system. To control the power bus two techniques are usually being applied: direct energy transfer (DET) and peak power tracker (PPT) (Wertz et al, 2015). The main difference between the two technics is the system’s reaction to the power generated by the solar panels. 3.1 Direct Energy Transfer (DET) In the case of DET, the power input deriving from the solar panels is being transferred directly to the bus. As a result, all the subsystems must run by using the same power used by the bus. In the case that a subsystem requires more power than the available, the battery may provide the extra required power. A shunt regulator is usually applied to the DET system in order to increase its efficiency and reliability (Wertz et al, 2015). The shunt regulator operates in parallel to the solar arrays and keeps the current of the arrays away from the subsystems and battery when it is not needed. A DET - shunt regulator system provides high efficiency at the EOL, low mass system and cost efficiency. However, one disadvantage is that the DET system cannot operate peak power requirements without the power support of the battery. The DET system can be divided into two categories: fully regulated bus and sunlight regulated bus (often referred as unregulated bus) (Patel, 2005). 3.1.1 Fully regulated Bus Fully regulated bus, which is also known as regulated bus, controls the bus voltage within a range of ±2 to 5% of the nominal voltage during the entire mission (Patel, 2005). The following figure describes the architecture of a
  • 25. Power Control Georgios Galanos 9 regulated bus. This type of system allows the batteries to be used in parallel with the solar arrays, which improves the system’s reliability. Figure 3-1 Regulated Bus DET (Patel, 2005) 3.1.2 Sun - Regulated Bus (Unregulated Bus) To minimise the complexity of the spacecraft and the power system it is more convenient to distribute power from both sources (solar panels and secondary batteries) but not in parallel. The case of a direct energy transfer to the bus is known us sun–regulated bus or unregulated bus. In this method the bus voltage is regulated during daytime via the shunt control and is unregulated during night-time. The basic difference between a regulated and an unregulated bus is found on the Power Regulated Unit. In the unregulated bus, the battery charger regulator controls the battery during daytime, however, a discharge converter is not included in the architecture, which leads to battery discharges during night- time via a diode ‘d’ called ‘battery discharge diode’. The battery disconnects from the bus during day-time while it is been regulated by the shunt controller. The system allows only the battery to be discharged at night-time and blocks any uncontrolled charge current received from the battery (Patel, 2005). The basic architecture of such system is the following:
  • 26. Power Control Georgios Galanos 10 Figure 3-2 Sun- Regulated Bus (Unregulated Bus) DET (Patel, 2005) 3.1.3 Comparing Regulated and Unregulated Bus The power system must take into consideration both day–time and night–time phases of the mission. A full-regulated bus is usually applied in GEO orbits where the power requirements are above 3kW, whereas the unregulated bus is mostly used in satellites with requirements below 3kW. (Patel, 2005) The sun–regulated bus is often less complex and reliable than the fully regulated bus. The main disadvantage is that the battery cannot be used during daytime as it is disconnected from the bus. The fact that a battery charger converter is missing contributes in reducing the system’s cost and power. On a fully regulated bus operation, the battery can be used during daytime. The attendance and use of a battery when peak power is required, leads to the reduction of the area, mass and cost of the solar arrays and could save up to 20% of the mass and area of the solar panels. By using a fully regulated bus the mission automatically becomes more reliable as the bus is continuously
  • 27. Power Control Georgios Galanos 11 regulated and can provide the required voltage to the loads at any time. Nowadays, most of the space missions are using regulated buses. 3.2 Peak Power Tracker (PPT) - Power control It is known that solar arrays generate more power at the BOL and during cold phases of the mission at higher voltage rates. The maximum power of the system occurs at a point where, the power is transferred by the solar arrays at the maximum power and operates at maximum efficiency (Jiang et al, 2002). The maximum power point of the solar arrays can be varied with time, solar radiation, temperature and lifetime of the solar panels (Huynh and Cho, 1999). A suitable switching regulator must be located between the solar arrays and the bus to control the maximum power voltage that the solar arrays produce and the voltage that the loads need to be supplied with. The figure below displays the main architecture of a Peak Power Tracker system. Figure 3-3 Peak Power Tracker Architecture (Patel, 2005) The series-switching regulator stays constant at the maximum power producing voltage using the peak power tracker. The output voltage can be adjusted to the required level by varying the duty ratio controller. The peak power tracker can be activated while the battery is being charged. If not, the power that left in the solar arrays can increase their temperature.
  • 28. Power Control Georgios Galanos 12 PPT is mostly used for satellites that are not able to point continuously the sun or the solar radiation and in cases when the temperature varies at a high range. The PPT system can be designed in three ways: series, parallel and series– parallel as shown in the figure below. Figure 3-4 Battery charge and discharge options in peak power tracking architecture. (Patel, 2005) 3.3 Power Control Trade-off The table below indicates the pros and cons of each option. Cost, mass and efficiency are the most important variables in every mission. The table shows the best application for each case, which is not always valid since parameters other than the cost, mass and efficiency may be equally important.
  • 29. Power Control Georgios Galanos 13 Table 3-1 Advantages and Disadvantages of different architectures (Patel, 2005) According to past missions, any architecture is suitable for specific missions, however it is proved that this is not always true. For small satellites, which require less than 500W of power and have low orbits, PPT is the most suitable solution. Between 1000W and 3000W, sun-regulated bus is the most advantageous option. For power requirements above 3000W a regulated bus is the best approach. At this stage a PPT system seems to be the most matching system for a spacecraft that demands power below 500W. The fact that the spacecraft will orbit the L1 point may add some extra things to notice before the decision. In the L1 point the spacecraft has been designed to face the Sun during the whole mission at the most desirable angle between the Sun and the solar arrays to avoid high losses. It is remarkable to notice that in the L1 point the
  • 30. Power Control Georgios Galanos 14 spacecraft will never come across eclipses, which leads to the use of the solar arrays power during the entire mission. Despite that in the RIICS project the power requirements remain constant in the operation phase and peak power is absent, in some cases the battery will be used to split the power consumption (will be discussed later on). A DET regulated system seems to be closer to our needs, as it is more reliable and cost-effective. 3.4 Bus voltage selection The selection of the bus voltage of the spacecraft must be linked with the power requirement, nominal voltage of each of the loads and buses available in the market, in order to reduce the cost. The figure below indicates that for the RIICS project, in which the power requirement is less than 500W, a 28V bus is the ideal solution. All the subsystems must comply with the voltage requirement of the electrical power subsystem. Figure 3-5 Optimum voltage for various power levels (Patel, 2005)
  • 31. Solar arrays Georgios Galanos 15 4 Solar arrays 4.1 Solar PV technology Nowadays there are plenty of choices in Solar PV technology. This report examines the most common technologies in space applications: Silicon, Gallium Arsenide (GaAs) single junction, Gallium Arsenide (GaAs) multijunction and Gallium Arsenide (GaAs) triple junction. (De Luca, 2011) Figure 4-1 Typical Solar Array Design Parameters (Wertz et al, 2015) The chart above clearly shows that Silicon technology is the cheapest of all the available technologies. As the power requirements increase so do the area and mass of the spacecraft. According to the configuration of the spacecraft and the launcher, the area of the solar arrays is not as significant as the reduction of the cost of each component (Jurian, T., 2019). RIICS spacecraft will consume an average of 222,1W power. The latter, means that the Silicon option costs around 126,000$, and for the GaAs (SJ), GaAs (MJ), and GaAs (3J) the costs are 283,000$, 232,000$ and 206,000$ respectively. Silicon technology is the most inexpensive solution for the spacecraft. As mentioned previously, this project aims to minimise the total cost of the mission and for that reason Silicon 0 5 10 15 20 25 30 35 Area (m2) Weight (kg) Cost ($) x 10^4 Power BOL (W) x 10 Power EOL (W) x 10 Solar array type Trade - off Silicon GaAs (SJ) GaAS (MJ) GaAs (TJ)
  • 32. Solar arrays Georgios Galanos 16 technology was chosen. The performance of the power system can be adapted and provide the required power at the Beginning of Life and End of Life at the same level of efficiency. 4.2 Solar array structure The configuration of the solar arrays can be divided into planar and concentrator (Wertz et al, 2015) and each type can be divided in body or panel mounted. Up to date, results from past missions, show that most of the satellites use planar arrays. 4.2.1 Rigid Panels A traditional way to build the solar array is to mount the cells onto a rigid substrate often made from aluminium and carbon face sheets. Solar cell insulation sheets like Kapton® , Kevlar® and fiberglass are able to successfully reduce the mass of the array (Wertz et al, 2015). Cover glass such as fused silica Microsheet ® is used to protect the array from the space environment. To successfully produce more output power by the cell, an antireflective coating is installed so to minimise the light reflection and allow the sunlight energy to be absorbed by the solar cells. A coating that controls the temperature of the surface must cover the back site of the array (Patel, 2005). The following figure displays one wing of a rigid panel solar array. Figure 4-2 A fully deployed dollar array (Patel, 2005)
  • 33. Solar arrays Georgios Galanos 17 The solar arrays are stowed with the satellite structure in the launch vehicle until the phase of the separation when the solar arrays are deployed. This particular method is discussed in the mechanism’s report (Liébana Moradillo, O., 2019). Figure 4-3 Panels section with cells mounted on a honeycomb substrate with face sheets (Patel, 2005). 4.2.2 Body–Mounted Body-mounted planar cells are typically used on spinning spacecrafts. During its rotation, the spacecraft’s surface can capture the energy of the Sun. The solar cells can increase their thermal energy, however, the constant rotation of the spacecraft does not allow the temperature increase of the spacecraft’s elements. Body-mounted cells operate in less efficiency compared to deployed solar cells, as they have to run in higher temperatures. The main disadvantage of body-mounted cells is that the area of the solar arrays will be increased because the cells are not illuminating all the time. Consequently, the overall cost increases, a fact that this project attempts to eliminate. RIICS spacecraft is a 3-axis stabiliser spacecraft that needs to be stable to operate its science functions, thus it is more convenient to use panel mounted solar arrays (Wertz et al, 2015).
  • 34. Solar arrays Georgios Galanos 18 Figure 4-4 A body mounted solar array (Patel, 2005) 4.2.3 Three or More Wings This solar array construction is generally used for small science mission satellites with Peak Power Tracker. It practically offers the same benefits as a body-mounted array, for the reason that the arrays do not always face the sun. The benefit of using three or more wings is that the solar arrays do not interfere with any of the instruments located on the spacecraft body. The three or more wings construction needs different Peak Power Tracker for each of the arrays, or else the arrays will obstruct each other (Patel, 2005). Figure 4-5 Three wings array architecture (Patel, 2005)
  • 35. Solar arrays Georgios Galanos 19 4.2.4 Flexible Array Hubble Space Telescope and ISS are the most well-known satellites to use a flexible array construction. As in the rigid panel method, the arrays are stowed on the spacecraft when the spacecraft is in the launch vehicle and rolled out or deployed like an accordion panel after the spacecraft’s separation with the vehicle. As all the constructions, protection from thermal risks and control of temperature differences when exiting the eclipses must be assured. In cases where a flexible array is not totally flat, a reduction of the power output of the array could occur. A temperature difference reshapes the array. Once the temperature is being equalised, which should happen approximately 30 minutes after the temperature changes, the array returns to its normal flat shape. This inefficiency of the solar arrays is something that a rigid panel will never face as it transfers the front heat to the back in a very quick way (Patel, 2005). 4.2.5 Selection of Construction There is one more construction called concentrator. Concentrator construction uses mirrors and lenses to collect more sun light in order to generate more power. This construction adds more complexity to the system, therefore it has not been taken into consideration (Wertz et al, 2015). The RIICS spacecraft is designed be a 3-axis stabilised satellite. This information tends to discharge the possibility of having a body-mounted array, since it is commonly used for a spinning spacecraft (Wertz et al, 2015). Moreover, the instruments and payload of the body mounted array spacecraft will face very high temperatures and add complexity to the thermal design. Finally, the spacecraft in this project uses its outer surface to accommodate instruments, as a result there is no available surface area to provide the required power. Rigid panels is the selected solar construction as it is the most common, reliable and less complex system. It is also used on 3 axis-stabilised spacecrafts. It is important to notice that in the configuration of the spacecraft, the solar arrays
  • 36. Energy storage - Secondary battery Georgios Galanos 20 are able to track continuously the sun but with a worst-case scenario incidence angle to be accounted (will be discussed later on the report). Two rigid arrays consisted of 3 panels each, form the solar panel system. The figure below indicates the existing design of the solar arrays. Figure 4-6 Final design of the Solar arrays (Jurian, T.,2019) 5 Energy storage - Secondary battery Secondary batteries are commonly used during times of eclipses and peak power requirements for energy storage. As mentioned previously, this project does not call for an eclipse, given that the spacecraft will orbit the L1 point. A secondary battery will be used to provide enough power in case of emergency and Peak Power in the course of the mission. The power system size and its various design options will be thoroughly discussed later in the report. Individual cells connected in series or parallel create a pack of batteries. The number of the individual cells required depends on the bus voltage requirements and can be defined by the following table. Table 5-1 Number of cells as a factor of bus voltage (Samina Asif,2008)
  • 37. Energy storage - Secondary battery Georgios Galanos 21 The decision of the number of cells per battery is made after the analysis of the available battery types. There are some basic parameters that should be considered prior to the design of the battery and the type selection. The battery must always provide constant voltage when required. Table 5-2 displays the issues in designing a secondary battery. Table 5-2 Issues in Designing the Energy Storage Capability (Wertz et al, 2015) The conversion from chemical into electrical power and reverse is done by the battery. A secondary battery can perform these operations up to thousand times during its lifetime. The selection of a secondary battery is basically done by taking into account the capacity of the battery, cost, weight, cycle life (depending on the depth of discharge) and the way the spacecraft is going to use it. In this project the secondary battery must be of low-cost and have long cycle life capability in order to provide enough power throughout the mission. 5.1 Types of secondary batteries Nowadays spacecrafts use mostly three types of secondary batteries: Nickel- Cadmium (Ni-Cd), Nickel-Hydrogen (Ni-H2) and Lithium Ion (Li-Ion) (Broussely Pistoia and Knovel, 2007). Up to the 80’s, Nickel-Cadmium battery was the traditional battery for 28V spacecrafts and buses. It usually consisted of 22-23 series-connected cells. Their nominal capacity ranges between 5 and 100Ah. Today, Nickel-Cadmium Physical Size, weight, configuration, operating position, static and dynamic environments Electrical Voltage, current loading, duty cycles, number of duty cycles, activation time and storage time, limits on depth of discharge, and short-circuit (fault) recovery Programmatic Cost, shelf and cycle life, mission, reliability, maintainability, produceability and safety
  • 38. Energy storage - Secondary battery Georgios Galanos 22 batteries’ application is considered to be extensive and very low risk – related to the storage system missions (Wertz et al, 2015). After the Nickel-Cadmium battery was introduced to the industry, Nickel- Hydrogen (Ni-H2) batteries became the most common energy storage. Ni-H2 design configuration can be divided into three categories: single pressure vessel, common pressure vessel and individual pressure vessel. The main difference between each of the categories of a Ni-H2 battery is the diameter of the cells and their working terminal voltage (Wertz et al, 2015). Li-Ion batteries have significant advantages over Ni-Cd and Ni-H2 batteries. This kind of battery technology offers a reduction in size, higher energy density, higher efficiency, less complexity, less costly thermal control system and lower self-discharge rate. The main disadvantage of the Lithium Ion batteries is that they are are approximately double the cost of Ni-Cd and Ni-H2 (Patel, 2005). The main characteristics of each type of batteries are shown on the table below. Battery Type Ni-Cd Ni-H2 Li-ion Energy Density of Battery (Whr/kg) 30 60 125 Cycle life (80% DoD) 750 500 1500 Self discharge (per month) *100% 0.5 0.3 0.05 Cell Voltage (V) 1.2 1.2 - 3 3.7 Charge temperature (Celsius) 0 - 40 -20 - 30 10 - 25 Discharge temperature (Celsius) -20 - 65 -20 -65 -20 - 60 Maintenance requirement Full discharge every 90 days when in full use Full discharge every 90 days when in full use Free Table 5-3 Characteristics of Selected Secondary Batteries (Battery University, 2019) As stated earlier, the battery used in this project must be not only cost-effective but also capable of providing enough power to the loads. The Nickel-Cadmium battery seems to be the ideal solution as it is reliable and economical. The only disadvantages of the Nickel–Cadmium battery and its cycle of life and mass.
  • 39. Analyze and Size the Power System Georgios Galanos 23 The RIICS spacecraft must be able to provide a charge/discharge mode for around 1800 cycles through the mission. It is obvious that if Nickel batteries were used, the system would require more than 4 batteries (one additional for redundancy), which would lead to higher battery system mass and possibly higher launching cost. Moreover, the battery must be able to be regulated from the PCDU. As it will be explained in the following chapters, the only available charge/discharge regulator provided by TERMA regulates only Lithium battery systems. In addition to all the above, Clyde Space (2010) states: “Li-Ion is fast becoming the main energy storage technology used in space applications (Li- ion is used on ESA deep space missions Rosetta, RoLand, Mars Express, and many more missions including all of SSTL's recent small satellite missions)“. To conclude, a Lithium Battery is the best approach in this particular project, considering the cycle life of the mission, high cost due to a higher launch mass, and charge/discharge regulator factor. 6 Analyze and Size the Power System The power subsystem is generally quite complex. It is often interacting with the rest of the subsystems. This system is so vulnerable that each iteration could create undesired system alternations. This chapter examines the two most feasible and reliable Power System designs. The effort to minimise the cost, mass and area is not always leading to a single solution. Consequently, a trade- off must be applied. The only constraint in deciding the final design of the Power system is the minimisation of costs, which is the main objective of this study. 6.1 Study Case 1 After collecting the inputs of all the subsystems, the study proceeds with the first iteration of the design. The analysis of the power requirements of each of the subsystems proves that the design is simple and of low cost. The power requirements for each of the subsystems remain stable only in the operational
  • 40. Analyze and Size the Power System Georgios Galanos 24 modes. This conclusion means that there is no need for Peak Power or battery use in these modes. For that reason the Power system could be designed in such way that the solar arrays could supply the required energy to the loads at any time of the mission without the use of batteries. This design will occur by increasing the solar arrays area to provide enough power during the BOL and EOL. The battery should be used only in emergencies, resulting in adding only one pack of batteries to the system. All types of emergencies must be studied and included in the system design. The RIICS mission is a low cost mission of as high reliability as possible. For that reason, in the event of both solar arrays failing to provide the required power, the satellite will still operate normally. The satellite will automatically switch to survival mode, in which all the subsystems will operate the minimum number of actions possible. The survival mode has been designed to provide enough power to all the subsystems to survive for 24 hours or until the issue has been resolved. In the event of different emergency scenarios, the duration of the mode can be extended, given that there is no limit of power. The solar arrays will provide the necessary power. The specifications of this design are shown on the following tables. Solar arrays Case 1 Area (m2 ) 4.6 Cost ($) 187,200 Mass (kg) 10.5 Power available (W) 424 Table 6-1 Solar Arrays Specifications Case 1 Table 6-2 Battery Specifications Case 1 Battery Case 1 Mass (k) 7.9 Cost ($) 2,374 Capacity (Whr) 989
  • 41. Analyze and Size the Power System Georgios Galanos 25 Total Case 1 Mass (k) 18.4 Cost ($) 189,574 Table 6-3 Total Specifications Case 1 Although case study 1 is simple to design and it is of low mass, its relatively high cost does not make it a good enough case for such missions. 6.2 Study Case 2 After working on the first design of the Power system of the spacecraft, the next step is to investigate the possibility of further system improvements. Improving the cost factor is essential for a small consuming spacecraft. An area of 4,6 m2 solar arrays appears to be large and costly compared to similar low power consuming spacecrafts. The maximum power that the subsystem requires is about 330W and with a direct energy transfer system the available power has to be 412W. These amounts derive from the need in generating power from the solar arrays during the mission. During the phases from the start-up mode until the spacecraft reach the L1 point and starts the operation mode, there is need of peak power. Consequently, the power system will oversized in order to provide the required power. All these factors increase the final area required. In order to minimize the space used by the solar arrays on the spacecraft, is best to make use of the battery for peak power demands. As previously discussed, peak power is required only in phases prior to the mission’s operational phase. It also adds complexity to the design. The use of battery for peak power will add one more component to the power system, as two batteries will require (one extra for redundancy). According to this design, the spacecraft is already using a battery for phases before the operational phase and for that reason a study was carried out as for the use of the battery for splitting the power requirements for the operational phase and decreasing even more the space used by the solar arrays. In this design, the mass will be higher given the need for 3 battery
  • 42. Analyze and Size the Power System Georgios Galanos 26 packs because of the length of the mission and the need of redundancy. The main specifications of this case study are included in the following tables. Solar arrays Case 2 Area (m2 ) 3.06 Cost ($) 125,931 Mass (kg) 7.1 Power available (W) 278 Table 6-4 Solar Arrays Specifications Case 2 Battery Case 2 Mass (k) 23.73 Cost ($) 7,120 Capacity (Whr) 989 Table 6-5 Battery Specifications Case 2 Total Case 2 Mass (k) 30.8 Cost ($) 133,051 Table 6-6 Total Specifications Case 2 6.3 Comparison of Cases Understanding the requirements of the mission is of utmost importance in the process of selecting one of the above case studies. The first case study includes the use of solar arrays and a secondary battery in the event of an emergency. Installing such system would only reduce the weight of the spacecraft, as the cost and the area of the solar arrays will be very high. On the other hand, the second case of using both solar arrays and batteries for providing power would reduce the cost and the total area of the system but not the system’s mass. The graphs below indicate the most important differences between the two options. Note: The charts below include a scaled method for comparing the values.
  • 43. Analyze and Size the Power System Georgios Galanos 27 Figure 6-1 Solar arrays comparison In the comparison of the two study cases in regards to the solar arrays design, it can be seen that based on all specifications the second case study is more efficient. Case study 1 calls for a larger solar array to cover the power demand of the mission. It is essential to underline that in the first case study the unexploited power will be dissipated and put more pressure on the thermal subsystem. In the second case study however, the dissipated power from the solar arrays is used directly to charge the batteries. In addition, a Maximum Power Tracker (MPP) system could possibly be added in the first case study to ensure constant maximum power availability. This observation leads to a small reduction of the power available, as the efficiency of a MPP system is slightly higher than a DET system. As a result, the area of the solar arrays could be significantly reduced, which makes a third study focusing on a MPP system unnecessary. For all the above, case study 2 is a better approach regarding the design of the solar arrays, especially considering the cost minimization factor. A discussion on the battery and total compression is following, which will give a better understanding of the two studies. 0 2 4 6 8 10 12 14 16 18 20 Area (m^2) Cost ($) x 10^4 Mass (kg) Power available (W) x 10^2 Case 1 4.6 18.72 10.5 4.24 Case 2 3.06 12.59 7.1 2.78 Axis Title Solar arrays
  • 44. Analyze and Size the Power System Georgios Galanos 28 Figure 6-2 Batteries Comparison As for the battery design, case study 1 is the ideal solution. Figure 6-2 Batteries Comparison proves that the mass and cost of the first case study are significantly lower than the second case study. It is important though to note, that in both cases a Lithium battery is been used, as already discussed in Chapter 5.1. Using batteries in the cases of peak power and power split requirements for a 6-year lifetime mission, would increase the required quantity of the batteries to complete the mission in a reliable and safe manner. 0 1 2 3 4 5 6 7 8 9 10 Mass (kg) x 10 Cost ($) x 10^3 Capacity (Whr) x 10^2 Case 1 0.79 2.3735 9.89 Case 2 2.373 7.12 9.89 Axis Title Battery
  • 45. Analyze and Size the Power System Georgios Galanos 29 Figure 6-3 Total Mass and Cost Comparison The final step for the selection of the ideal design approach is to compare the results of the most important parameters of the designs, mass and cost of the power system. The above diagram shows the inversed results in the two cases, a fact that adds complexity in making the final decision. This study aims on the minimisation of the cost, which simplifies the decision process. After examining the launch and configuration system (Jurian, T., 2019), (Picavez C., 2019), the mass of the power system shows only a 12kg difference, which is not a significant factor in the decision process. On the other hand, the area utilized by the solar arrays has to be as small as possible. For these reasons, case 2 has been selected as the final design of the power system. The sizing and analysis of the power system design is discussed in Chapter (7). 6.4 Power Consumption Analysis The most important requirement for the power system is to be able to generate, control, distribute and store the energy and provide the appropriate power to all components during the mission. To examine if this requirement is applied to our mission, the study conducts a power breakdown. Analysing the power 0 5 10 15 20 25 30 35 Mass (kg) Cost ($) x10^4 Total Case 1 Case 2
  • 46. Analyze and Size the Power System Georgios Galanos 30 breakdown derives a better overview of the design selection and process that was followed to complete it. The first step is to discuss the process followed to size the battery and solar arrays. By having the results and the power breakdown from the first simple design, which was exclusively based on the use of solar arrays as a power source, the study attempts to reduce the solar array space. Table 6-1, Table 6-2 and Table 6-3 provide the basic specifications of the first power system’s design. The battery has been sized at first for emergencies. After the selection of the second case, in which the battery supports the system in peak power and power split requirements during the operational phase, the power availability of the existing battery in the event of peak power has to be examined. As it can be seen from the table below, the total energy battery discharge in any phase is much lower than the total energy of the battery (988Whr), therefore there is no need to oversize the battery. Phase Subsystem Energy Discharged (Whr) Total Battery Discharge (W) Orbit Transfer Payload 221.1 Structure and Mechanics Thermal Comms 61.2 OBDH ADCS Propulsion 160.6 Sun Safe During Commissioning Payload 169.35 Structure and Mechanics 1.4 Thermal Comms 150.25 OBDH ADCS 12.70 Propulsion 5
  • 47. Analyze and Size the Power System Georgios Galanos 31 Start up Payload 49.44 Structure and Mechanics 1.34 Thermal Comms OBDH ADCS Propulsion 48.1 Stand By Payload 8.4 Structure and Mechanics Thermal Comms OBDH ADCS Propulsion 8.4 Table 6-7 Battery Discharge for cases tat peak power is required A more analytical document can be found in Appendix (9C.2). The energy each phase needs is much lower than the battery’s, which allows the operation of more than one cycles prior to the battery charge. A study was made to calculate the number of battery cycles that each phase can operate with in order to extend the battery’s lifespan. The following table states the numbers concluded by this study. Phase Orbit transfer Sun Safe (During commissioning) Total Capacity of Battery (Whr) 988.95 988.95 Capacity that needs (Whr) 277.26 211.65 Times that battery can be used 3.6 4.7 Duration of the Phase 173 (days) 30 (days) Cycles of Battery 49 7
  • 48. Analyze and Size the Power System Georgios Galanos 32 Phase Start-Up Stand-By Total Capacity of Battery (Whr) 988.95 988.95 Capacity that needs (Whr) 61.7675 0.0105 Times that battery can be used 16. 94185.7 Duration of the Phase 17.217 (hours) 1 (hour) Cycles of Battery 1 1 Table 6-8 Cycle life of battery During the research for the selection of the battery, which is discussed later on, there were no available products in the market with an acceptable battery cycle life and for this reason a factor of 80% of Depth of Discharge was taken into account to provide around 1500 cycles (Battery University, 2019). It is of high importance to use the battery efficiently and reduce the battery life cycles and battery packs, whilst targeting the extension of the mission. The next table displays the power consumption, charge/discharge mode, energy consumed by the battery and power required for charging the battery during the operational phase. A more detailed power breakdown document can be found in Appendix 9C.1. The detailed power breakdown document contains information about the power consumption and duration of each instrument of the subsystems. Phase Sub- system Aver. Power (W) Peak Power (W) Charge Dis- charge Energy Disch. (Whr) Power to charge (W) Total Power (W) Scan. Payload 56 OFF ON 222.1 Structure / Mechanic s 18 Thermal 44 Comms 13.5 OBDH 33 ADCS 57.6 69 136.67 Propulsio n 0
  • 49. Analyze and Size the Power System Georgios Galanos 33 Chara. / NEOs Payload 56 OFF ON 222.1 Structure / Mechanic s 18 Thermal 44 Comms 13.5 OBDH 33 ADCS 57.6 69 87.74 Propulsio n 0 Target Acqui. Payload 0 ON OFF 49.6 222.1 Structure / Mechanic s 18 Thermal 44 Comms 13.5 OBDH 28 ADCS 69 Propulsio n 0 Orbit Maint. Payload 0 ON OFF 85.54 219.1 Structure / Mechanic s 18 Thermal 0 Comms 13.5 OBDH 28 ADCS 19.5 Propulsio n 54.56 Comm Payload 0 ON OFF 137.1 221.4 Structure / Mechanic s 18 Thermal 0 Comms 30.01 OBDH 33 ADCS 3.25 Propulsio n 0
  • 50. Analyze and Size the Power System Georgios Galanos 34 Table 6-9 Part of the Power Break During Operational Phase The above table proves that there is no peak power in any of the phases except for scanning and characterization/NEOs. This conflicts previous discussions according to which there is no peak power in the operational phase. This happens because on scanning and characterization/NEOs the battery shares the power requirements of the ADCS to further decrease the solar arrays area. Usually, the battery can be charged when not used by the system in the various phases. In this project the battery is being used for the period of the operational phases and modes. For that reason the battery must be charge in any phase with available time and power for charging. Orbit maintenance, target acquisition and communications have a total of 160 minutes available for charging the battery. The use of battery to split the power takes place in the operational phase. While the battery is being used for peak power for all the other phases, operational phase requires the maximum average power. Next chart displays the average power for each phase of the mission. Figure 6-4 Average Power Consumption 0.00 50.00 100.00 150.00 200.00 250.00 Average Power Consump6on Power (W)
  • 51. Analyze and Size the Power System Georgios Galanos 35 Based on the above chart, the battery is being used to split the power usage in order to reduce the solar arrays area and cost. The maximum power that can be supplied from the battery to the system during the operational phase has to be examined. During operational phase the modes that consume the most average power are the Scanning and Characterization/NEOs modes as it can be seen on the chart below. Figure 6-5 Power Consumption during Operational Phase To examine how much power the battery can supply to these two modes in every cycle of the mission, the study looks on the maximum time and power available to the rest of the modes. The following table indicates the power discharge for each mode, the available energy for the battery charge and the power needed to charge the battery enough to secure the required amount of energy. Operational Mode Battery discharged (Whr) Energy Available to charge (Whr) Power Available (W) Power needed to charge (W) Scanning 138.67 0 0 0 Characterisation /NEOs 84.74 0 0 0 0 50 100 150 200 250 Power(W) Operational Phase Scanning CharacterizaLon/NEOs Target AcquisiLon Orbital maintenance CommunicaLons
  • 52. Solar Arrays Sizing Georgios Galanos 36 Target Acquisition 0 14.23 61.00 61 Orbit maintenance 0 22.62 99.94 96.94 Communicaitons 0 207.94 149.24 148.53 Total 223.41 244.9 Table 6-10 Battery Specifications for operational phase The study calculates the maximum power the battery can supply in the course of the operational phase. By using the batteries to split the Power requirements on the operational phase the area of the solar arrays decreases by 0,3m2 and the cost by 7000$. This is an addition reduction to the area and cost of the system after using the battery for peak power demands. The total reduction can be found in Figure 6-1 Solar arrays comparison 7 Solar Arrays Sizing Nine basic parameters have to be taken into account for the solar arrays sizing: 1. Operational scheme of the mission: This parameter indicates the time when the solar arrays must provide power to the load during the mission. • During launch the spacecraft is not required to provide power to the loads. • There will be no power supply in the event that both solar arrays fail. 2. Solar radiation variation during the mission: As the spacecraft orbits the L1 point, the distance between the spacecraft and the Sun will be between 0,9928 and 0,9891AU and the solar radiation will range between 1400,84– 1411,27W/m2 . This design is using the minimum value. The study also takes into account the worst-case scenario, when the distance is almost 1AU and the solar radiation is 1368 W/m2 during the start-up mode. 3. Incidence angle between Sun and solar arrays: The solar arrays have been designed to be deployable and able to track the sun at any time of the mission. To ensure reliability, this study also considers the scenario of facing an undesired angle. According to the literature (Wertz et al, 2015) most of the
  • 53. Solar Arrays Sizing Georgios Galanos 37 missions have ran on a 23.5 degrees value, which is the chosen angle for the design of the solar arrays for the RIICS project. 4. Cells conversion efficiency: The efficiency of the silicon technology is estimated to be 14,8% (Wertz et al, 2015). 5. Performance degradation: The degradation of the Silicon technology cells is estimated to be 3,75% per year (Wertz et al, 2015). 6. Inherent degradation: The solar cells are located on a substrate, which usually results in a 0,77 factor of losses of the solar arrays substrate area (Wertz et al, 2015). 7. Losses due to transmission inefficiencies: For a Direct Transfer System the losses due to transmission inefficiencies are projected to be 20%. This amount of losses is thermally dissipated in the distribution process (Wertz et al, 2015). 8. Power consumption of each subsystem and component: The power variation of the solar panels that needs to be provided in the course of the mission starts from 50.5W and can get up to 222,.W. 9. Power to be provided by the battery: The amount of the power that batteries need to provide to the system ranges from 4.01W to 171.5W. After examining all the parameters (the design selection, design selection analysis and worst-case scenario) the study proceeds in the calculation of the final size of the solar arrays. In the worst-case scenario, the solar arrays must be able to provide 222.1W of power to the loads. This leads to a total 3.07m2 area of solar panels and 125,930$ cost. The main features of the solar arrays are displayed on the table below Solar Arrays Features Solar cell efficiency 0.148 DET system efficiency 0.8 Inerent degradation 0.77 Solar cell degradation per year 0.0375 Sun angle (deg) 23.5 Specific cost ($/W) 378
  • 54. Solar Arrays Sizing Georgios Galanos 38 Maximum Average Power (W) 222.1 Mass (kg) 7.05 Area (m^2) 3.07 Cost ($) 125,930 Table 7-1 Solar arrays main features 7.1 Battery’s Component Selection The battery component was selected from the available space applications market, so to achieve the minimisation of the cost. However, the cost of the batteries is not available in this study. The calculations were made according to Patel’s references. A 0.3% per day of self-discharge has also been taken into consideration (Broussely Pistoia and Knovel, 2007). The trade-off was made between the products that are provided by SAFT. VES 100, VES 140 and VES 180 were included in the trade-off (Saft, 2008). To select the appropriate component, the study calculates the total cycles of the battery to ensure that the selection will be made by the most efficient approach. The component must provide the necessary energy to the closest approach in order to reduce the required quantities regarding the cycles of the mission. The total cycle life of the battery must be over 1881 cycles. This amount of cycles of life is adequate for all operations from BOL to EOL, however it excludes emergencies. Case of emergencies will be included later on. The PCDU will regulate the 28V bus and examine the effects of having lower battery voltage on the operation of the mission. Given that no price for the battery has been provided, VES 140 (Saft, 2008) is the selected component as it is matching the appropriate requirements of the mission. Appendix 9C.2.3 shows the technical specifications of the cells. 7.1.1 Configuration The specific energy of the VES 140 is sufficient for one cell to provide the required energy to the spacecraft. As a result, the topology of the battery will be designed in series so to reach the desired voltage.
  • 55. Solar Arrays Sizing Georgios Galanos 39 The nominal voltage of each cell connected in series determines the total output voltage. “A general guideline is to place cells in series to make the nominal battery voltage during discharge equal to 80% and during charge about 93% of the bus voltage” (Patel, 2005), meaning that to reach the 28V requirements 7 cells need to be placed into series. Having less or more than 7 cells will impact the total mass of the battery and area of the solar arrays as the battery will require more energy to charge. The final selection of the cells’ number in series is made by taking into account the possibility of failure of one cell. The failure of a cell will drop the output voltage from 25.2V to 21.6V. The failure of one cell will allow the normal operation of the battery, which means that the system will still be able to provide the required power to the loads, given that the battery discharge and charge regulators have approximately 21.6V output (Chapter 8). The battery is typically designed based on the standards of the worst-case energy demand scenario during the mission. In the RIICS project the battery is designed to provide the required peak power in any phase and necessary power when both solar arrays have failed (worst-case emergency). The battery will then be charged on Sun safe Mode for 6,7hours. The table below indicates all the parameters to design the battery according to worst-case scenarios. Battery's Worst Case Scenario Parameters Total Battery Discharge 791.16 Total Power Needed to charge the battery in 6,7 hours 171.51 Capacity needed 988.95 Power available during Sun Safe Mode 171.60 Table 7-2 Battery’s worst Case Scenario Parameters The 7 series cell with the VES 140 component can provide 996.66Whr of energy, 8Whr higher than the required without the need of parallel configuration. For the above reasons the topology of the battery pack will be 7 cells in series. As mentioned in previous chapters, the total battery life must be more that 1881 cycles. Lithium batteries have an average of 1500 cycles at 80% Depth of
  • 56. Power Control and Distribution Unit (PCDU) Georgios Galanos 40 Discharge (Battery University, 2019). That means that the spacecraft must accommodate two secondary batteries and an extra battery for redundancy. The total quantity is three battery packs. The basic specifications of the VES 140 are the following: Battery VES 140 Specific energy (Wh/kg) 126 Mass per module (kg) 1.13 Energy (Wh) 142.38 Capacity (Ah) 39 Discharge voltage (V) 3.6 Charge Voltage (V) 4.1 Cells in series 7 Cells in parallel 1 Total capacity (Ah) 39 Total energy (Wh) 996.66 Total mass (kg) 7.91 Table 7-3 VES 140 Shaft Battery As the power system includes 3 packs of batteries the total mass will be 23.73kg. The cost for each pack of battery is estimated to be around 2,300$ (Patel, 2005) Finally, since the available power and capacity of the battery are higher than the required, the batteries will not be installed with oversized margins. Therefore, the design maintains a cost low. 8 Power Control and Distribution Unit (PCDU) A PCDU must be able to control and distribute the power through the mission according to the spacecraft’s needs. For that reason, a PCDU contains a number of modules, which assist the controlled power distribution. Generally, it is more convenient to select a PCDU from the existing market. The PCDUs available in the market are not suitable for the power system, therefore this project builds the PCDU from components provided by TERMA.
  • 57. Power Control and Distribution Unit (PCDU) Georgios Galanos 41 To build a proper PCDU for the mission, TERMA provides a Modular Medium Power Unit concept, which is designed for observation, navigation, science or low power spacecrafts. The modules used to build the PCDU are all plugged in a backplane motherboard and can be removed or replaced without any internal wiring. The module has been designed for a 28V regulated bus with one-single failure tolerant. Finally, the PCDU can accommodate 21 modules (Terma space, 2012d). The components of the PCDU are: 1) 3 Shunt Regulation Modules (S4R) (Terma space, 2012f) 2) 2 Battery Charge / Discharge Regulator Modules (Terma space, 2012a) 3) 3 Equipment Power Distribution Modules (Terma space, 2012b) 4) 4 Heater Power Distribution Modules (Terma space, 2012c) 5) 2 Pyro Firing Drive Modules (Terma space, 2012e) 6) 2 Command and Monitoring Modules 7) 1 Backplane 1. Shunt Regulation Module (S4R): During the mission the available power from the solar arrays often differs. In many occasions the power that each loads requires varies. For that reason it is critical to include a regulator to the system in order to control the available power and protect the loads and the bus by switching in and out segments of the solar arrays. The individual segment in the shunt regulator module can be grounded to achieve the switching out. The configuration of the S4R is a sequential switching shunt switch regulator module and it accommodates four independent shunt cells. This approach has the ability to feed the main bus section current via a series diodes by a parallel switch or to feed the battery section current via series switch and two series diodes (Terma space, 2012f). This approach is ideal for the RIICS spacecraft as the dissipated power is directly feeding the battery. The S4R module provided by TERMA is being designed to provide an output power capability of 600W (more than the required output power for the RIICS mission). Missions that have used the TERMA S4R:
  • 58. Power Control and Distribution Unit (PCDU) Georgios Galanos 42 • Galileo IOV 2. Battery Charge/Discharge Regulator Module (BCDR): The module provided by TERMA includes two power regulators, a battery Charge Regulator (BCR) and a battery Discharge Regulator (BCDR). The system is designed to target a Lithium battery configuration. This module consists of two battery charging and discharging functions. The first function, which is called End Of Charge (EOC), is the function that sets the charging limits. The battery is charging until it reaches the maximum selected level of voltage, after this point the battery is ready to be discharged. It is important to notice that a telecommand adjusts the EOC voltage to eight different levels. The second function regulates the discharge power to the main bus until the voltage reaches the limits that have been set. This function is called End Of Discharge. The battery at this stage is not allowed to re-enter a discharge mode until it reaches again the minimum level of the EOD. The output power capability of this module is 300W (higher than the required). The Lithium battery system is been designed in a 7s topology. With this method the nominal output voltage of the battery is 25.2V and 21.6V in the case of cell failure. Additionally, the BDR module operates in a range of 0–25.6V and BDR with the range of 16–27V. Therefore, in the case of failure of one cell, the PCDU will be able to operate normally. The voltage output of the battery is often lower than the voltage output of the bus in PCDU designs. The BDR is a conventional step-up regulator (Jensen and Laursen, 2002) that increases the output voltage. Missions that have used the TERMA BCDR are the following: • Mars Express • Rosetta • Venus Express 3. Equipment Power Distribution Module (EPD): This module provides a number of protection switchers. The PCDU must be designed in a way that all the spacecraft loads are equipped with one switch protection. The current module, which is provided by TERMA, consists of sixteen Latching
  • 59. Power Control and Distribution Unit (PCDU) Georgios Galanos 43 Current Limiters (LCL) and can be applied to the loads. There are twenty loads on the spacecraft and for that reason three Modules are needed of which one is for redundancy. The function of this module is protecting the upstream main power bus from an overload or short circuit current. Missions that have used the TERMA EPD are as follows: • XMM-Newton • Integral 4. Heaters Power Distribution Modules (HPD): This module is responsible for the distribution of the bus power to the spacecraft heaters. At the moment TERMA provides this module with sixteen output switches divided in two groups of eight switches. Upstream LCL protects each of these groups. The RIICS spacecraft includes thirty six heaters, which leads to the selection of four HPDM of which one is for redundancy. Missions that have used the TERMA HPD are the following: • XMM-Newton • Integral 5. Pyro Firing Drive Modules (PFD): This module is responsible for turning on and off the valves of the thrusters. One extra module is for redundancy. Missions that have used the TERMA PFD: • Hispasat 6. Command and Monitoring Modules (CM): This module introduces the communication interface to the data management subsystem. Two modules are being accommodated, the one for redundancy. Missions that have used the TERMA CM are: • Mars Express • Rosetta • Venus Express 7. Backplane: This module interconnects the aforementioned modules and closes the PCDU.
  • 60. Conclusion Georgios Galanos 44 The main final specifications of the PCDU are the mass, width, height and length which are 11.37kg, 235mm, 156mm and 379mm respectively. 9 Conclusion The following conclusion summarises the final design of the Electrical Power system. The distribution of the power demand to the loads is achieved with a fully regulated 28V bus working with a DET system. Two deployable 3.07m2 solar arrays are placed on two rigid structures and support the spacecraft with the required power during the mission. This excludes the worst-case scenario of emergency (discussed in previous Chapter). The two solar arrays cost 125,930$ and weigh 7.07kg. During peak power, scanning and characterisation/detection NEOs modes and emergencies, a battery supplies the necessary power demand. Three units of batteries are projected to cover the entire mission, of which one battery is for redundancy. The battery consists of a 7s cell configuration and weighs 7.91kg. The total cost is around 6,900$ and total mass is 23.73kg. A power control and distribution unit is being attached to ensure the efficient operation of the solar arrays and battery and the successful and safe power distribution to the loads. The PCDU weighs 11.37kg. The total approximate cost of the Electrical Power will be around 133,000$ and total weigh will be 42.17kg. The Electrical Power system successfully covers the corresponding requirements set by the project’s system engineers. Further analysis of the solar cells and their configuration is essential. Studying the sensitivity of the battery regarding temperature, actual voltage requirements for each subsystem and instrument of the mission and more possible efficient designs of the electrical power system is desired.
  • 61. REFERENCES Georgios Galanos 45 REFERENCES Angrist, S. W. (1982) Direct Energy Conversion, 4th edn, Copyright Allyn and Bacon, New York) Antonio De Luca (2011). Architectural Design Criteria for Spacecraft Solar Arrays, Solar Cells - Thin-Film Technologies, Prof. Leonid A. Kosyachenko (Ed.), ISBN: 978- 953-307-570-9, InTech, Available from: http://www.intechopen.com/books/solar-cells- thin-film-technologies/architectural-design-criteria-for-spacecraft- solar-arrays Battery University (2019) Comparison Table of Secondary batteries available at: https://batteryuniversity.com/learn/article/secondary_-batteries (accessed February 2019) Ben Johnson (2012) Power Sources for Space Exploration, Stanford University available at: http://large.stanford.edu/courses/2012/ph240/-johnson1/ (accessed in November 2018) Broussely, M., Pistoia, G. and Knovel, (2007), Industrial applications of batteries, 1st ed., Elsevier, Amsterdam ; Boston. Clyde Space (2010), Secondary Batteries, available at: http://www.clydespace.com/resources/powerschool/power_storage/secondary_batterie s, (accessed January 2019). David W. Miller and John Keesee, Spacecraft Power System, MIT OpenCOurseWare available at: https://ocw.mit.edu/courses/-aeronautics-and-astronautics/16-851- satellite-engineering-fall-2003-/lecture-notes/l3_scpowersys_dm_done2.pdf, (2003) (accessed December 2019) Fortescue, P. W., Stark, J. and Swinerd, G. (2003), Spacecraft systems engineering, 3rd ed, Wiley, Chichester. Huynh, P. T. and Cho, B. O. H. (1999), "Design and analysis of a regulated peak-power tracking system", IEEE Transactions on Aerospace and Electronic Systems, vol. 35, no. 1, pp. 84-92. James R. Wertz, David F. Everett and Jeffery J. Puschell (2015), Space Mission Engineering: The New SMAD, Microcosm Press, USA; Hawthorne. Jensen, H. and Laursen, J. (2002), "Power conditioning unit for Rosetta/Mars express",
  • 62. REFERENCES Georgios Galanos 46 6th European Space Power Conference, 6 May 2002 through 10 May 2002, Porto, pp. 249. Jiang, J. -., Huang, T. -., Hsiao, Y. -. and Chen, C. -. (2005), "Maximum power tracking for photovoltaic power systems", Tamkang Journal of Science and Engineering, vol. 8, no. 2, pp. 147-153. Jurian, T. 2019 RIICS: Rapid Imminent Impactor Characterisation System - Configuration & Structures Landis, G. A. (2006) Reevaluating Solar Power Systems for Earth, IEEE 4th World Conference on Photovoltaic Energy Conversion 2006 , NTRS-2007-0005136. Liébana Moradillo, O., 2019 RIICS: Rapid Imminent Impactor Characterisation System - Operations and Mechanisms Niels E. Jensenh (2003), Satellite Power System, ESA available at: http://www.esa.int/esapub/br/br202/br202.pdf (accessed December 2019) Patel, M. R. (2005), Spacecraft power systems, CRC Press, Boca Raton. Picavez, C. (2019) RIICS: Rapid Imminent Impactor Characterisation System – Launch System Saft (2008), VES 180 - Rechargeable lithium battery datasheet, available at: http://www.saftbatteries.com/doc/Documents/space/Cube712/VES%20180.e9cf5d8f- 3cbd-4921-8ac0-89d7b13bd0c0.pdf (accessed March 2019). Salina Asif (2008) Evolutionary computation based multi-OBJECTIVE design search and optimization of spacecraft electrical power subsystem, University of Glasgow, available at: http://theses.gla.ac.uk/373/1/2008AsifPhD.pdf Seurin, N. 2019 RIICS: Rapid Imminent Impactor Characterisation System - System Engineering Requirements & Risks SPS Concept Development and Evaluation Programme Reference System Report (1978) US DOE and NASA DOE/ER 0023. Terma space (2012a) Battery C/D Regulation Module, available at: https://www.terma.com/media/177689/battery_cd_regulation_module.pdf (accessed February 2019) Terma space (2012b) Equipment Power Distribution Module, available at:
  • 63. BIBLIOGRAPHY Georgios Galanos 47 https://www.terma.com/media/177695/equipment_power_-distribution_module.pdf (accessed February 2019) Terma space (2012c) Heater Power Distribution Module, available at: https://www.terma.com/media/177698/heater_power_distribution_module.pdf (accessed February 2019) Terma space (2012d) Modular Medium Power Unit, available at: https://www.terma.com/media/150039/modular_medium_power_unit.pdf (accessed February 2019) Terma space (2012e) Pyro firing Drive Module, available at: https://www.terma.com/media/177719/pyro_firing_drive_module.pdf (accessed February 2019) Terma space (2012f) S4R Shunt Regulation Module, available at: https://www.terma.com/media/177725/s4r_shunt_regulation_module.pdf (accessed February 2019) Wertz, J. R. and Larson, W. J. (1999), Space mission analysis and design, 3rd ed, Microcosm Press; Kluwer Academic Publishers, Torrance,CA; Dordrecht. BIBLIOGRAPHY Bewick, R., CUTE, Communication and Power Subsystems. Group Design Project report for MSc in Astronautics and Space Engineering, Cranfield University, 2009. Busquets Corominas J., Marco Polo ‘Lite’, Systems engineering (Requirements, baseline and coordination) and Electrical power subsystem. Group Design Project report for MSc in Astronautics and Space Engineering, Cranfield University, 2010. Lim, Timothy M., (2016), "A modular electrical power system architecture for small spacecraft ". Theses and Dissertations--Electrical and Computer Engineering. 90. Available at: https://uknowledge.uky.edu/ece_etds/90 (accessed December 2018) Zane Brough, Claudio Paoloni, (2015), Advanced Deployable/Rectractable Solar Panel System for Satellite Applications, World Academy of Science, Engineering and Technology International Journal of Mechanical and Mechatronics Engineering Vol:9, No:1, available at: https://pdfs.semanticscholar.org/c770/e1fba84b72fdeee7531cfd20d-
  • 65. Executive Summary: RIICS - Electrical Power Subsystem Georgios Galanos 49 APPENDICES Appendix A Executive Summary: RIICS - Electrical Power Subsystem The Appendix A summarise the Electrical Power subsystem work package. The main features of the Electrical Power subsystem are: 1. Two Silicon rigid deployable solar arrays, each consist of three panels. To be able to provide the power requirement (50.5W – 222.1W) the area of each of the array must be 1.535m2 . 2. Three pack of battery (one for redundancy). The total capacity of the battery is 998Wh and is consists of 7 cells in series provided by saft (VES 140 model). The total weight of the batteries is 23.73kg. 3. The total approximate cost of the Electrical Power will be 133,000$ and weights 42.17kg. 4. A PCDU will control and distribute the power generated and will weight 11.37kg. 5. A fully regulated bus operating up to 28V. 6. No eclipses during the mission. 7. 6 years designed lifetime. The electrical power subsystem was designed to be able to provide the required power during the whole mission of the spacecraft in the most efficient and low cost approach. The cost of each of the components may be different in reality. References have been used for calculating the approximate cost of the electrical power system and the values are not reliable.
  • 66. Common Appendix Georgios Galanos 50 Appendix B Common Appendix B.1 Mission objectives Mission statement “The aim of the mission is to build, in partnership with Aistech Space, a Physical Characterization and Scanning System for small Rapid Imminent Impactors” B.1.1 Primary objectives ● Characterization of imminent impactors to improve the understanding of the small Near-Earth Objects by comparing information obtained pre-impact from the spacecraft and post-impact information ● Detection of imminent impactors that are not detectable from the ground by using the spacecraft as an orbital scanning station B.1.2 Secondary objectives ● Detection of Residual Space Objects (RSOs) and utilisation of Space Surveillance Network (SSN) database ● Classification of NEOs and detection of a range of compounds on NEOs surface ● Exoplanets characterisation through photometry and spectroscopy B.2 Key mission requirements B.2.1 Mission performance ● Mission_01 - One third of all NEOs not detected by Earth with a closest approach distance to Earth <= 0.03 AU with absolute magnitude H <= 30 shall be characterized ● Mission_02 - The s/c shall be able to obtain the light curve of the target ● Mission_03 - The s/c shall be able to obtain the reflectance spectrum of the target ● Mission_04 - The s/c shall be able to observe the target in the Near Infrared (0.7 μm < 𝜆 < 2.5 μm) and Visible spectral regions (0.4 μm < 𝜆 <0.7 μm)
  • 67. Common Appendix Georgios Galanos 51 ● Mission_05 - The s/c shall be able to observe targets not detected by terrestrial telescopes B.2.2 Mission constraints ● Political_Constraint - The mission shall satisfy a hypothetical mission call from ESA’s Space Situational Awareness (SSA) Program ● Cost_Constraint - The total RIIC cost should be 50 M€ ● Schedule_Constraint - Small-Class mission: the mission should be implemented under a fast scheme of 5 years ● Development_Constraint - The Technical Readiness Level (TRL) should be 5- 6 (ISO scale) by the end of the short preparation phase and before the mission adoption B.3 Risk ● Regarding the mission, the most critical work packages are: Payload, Communications & OBDH, AOCS and Propulsion. Highest Criticality Events Key prevention actions Payload: detector degradation -Payload instruments shall be protected against impacts -The s/c shielding materials should have high hardness -Add little cameras on the s/c to detect failures Comms and OBDH: Loss of scientific and housekeeping data -Provide redundancy -Use dispatched ground stations to avoid interferences -Mount antennas in less risky part (potential impacts, radiations…) considering the pointing requirements -Provide safe-mode in case of anomaly AOCS: Wrong attitude of the spacecraft -Correlate computations with the one of similar past missions -Organize frequent team meetings (several per week) to improve communication and transmit information and results
  • 68. Common Appendix Georgios Galanos 52 - Apply margins when designing the propellant budget -Reduce orbit eccentricity and pointing errors to acceptable limit Propulsion: Loss of spacecraft -Check the quality of the system -Add cameras on the s/c to provide follow up of the orbit phase -Ensure electrical continuity of the surfaces -Prevent propellant mixing between opposite tanks Table B-1 Highest Criticality Events and Key Prevention Actions B.4 Trade-off Weigh Geo EW Geo CH L1 EW L1 CH DRO EW DRO CH Performance 5 1 2 3 5 1 1 Impact 4 5 3 5 3 4 2 Cost 4 4 5 2 4 1 2 AOCS demands 3 3 3 5 5 5 5 Feasibility 2 5 3 3 3 3 3 Environmental effects 2 3 3 5 5 4 4 Communications 1 5 5 2 3 1 2 Total 105 71 68 76 87 55 52 Table B-2 Trade off
  • 69. Common Appendix Georgios Galanos 53 B.5 Budgets B.5.1 Mass Budgets Table B-3 Mass Budget Breakdown Component Units Unit mass (kg) Total dry mass Propulsion module Primary thruster 1 5.4 5.4 Fuel tank 4 6.81 27.24 Oxidiser tank 2 9.29 18.58 2 Subsystem Mass (Kg) Payload 80 Power 10.06 Structure 102.36 Mechanisms 34.71 AOCS 55.13 Communications 31.8 Thermal 7.59 OBDH 12.8 Margin 5% Total dry mass 350 Wet Mass 520.17
  • 70. Common Appendix Georgios Galanos 54 Pressurant tank 1 6.04 6.04 Pyro valve 9 0.16 1.44 Non return valve 4 0.3 1.2 Fill/drain valve 19 0.09 1.71 Pressure regulator 2 1.72 3.44 Isolation valve 6 0.545 3.27 Filter 7 0.114 0.798 Pressure transducer 10 0.14 1.4 Piping 1 15 15 Structure 1 140 140 Pressurent 1 1.27 1.27 Total dry mass 222 Reaction Control System (RCS) RCS thruster 16 0.33 5.28 Fuel tank 1 2.66 2.66 Pressurant tank 1 1.98 1.98 Pyro valve 4 0.16 0.64 Non return valve 2 0.3 0.6 Fill/drain valve 7 0.09 0.63 Pressure regulator 2 1.72 3.44
  • 71. Common Appendix Georgios Galanos 55 Isolation valve 6 0.545 3.27 Filter 2 0.114 0.228 Pressure transducer 6 0.14 0.84 Piping 1 10 10 Pressurant 1 0.03 0.03 Total dry mass 29.60 Attitude Control and Determination System (ACDS) Star tracker camera 2 1 2 Star tracker processor 2 1.2 2.4 Star tracker baffle 2 0.53 1.06 Sun sensor 2 0.215 0.43 MIMU 2 4.44 8.88 Reaction wheels 4 4.1 16.4 Total dry mass 31.17 Table B-4 AOCS Mass Breakdown B.5.2 Link Budgets Parameter Value Unit Comments Frequency 8.45 GHz X-Band downlink Transmit Power 100 W X-TWTA Transmit Power 50 dBm Transmitter Diameter 1.2 m
  • 72. Common Appendix Georgios Galanos 56 Peak Transmitter Gain 37.9 dBi EIRP 85.9 dBm DSN 34m Propagation path length 1.748E+06 Km Maximum distance in the orbit from Earth Space loss 236 dB Atmospheric Attenuation 1 dB Other losses 1 dB Cables, switches etc. Receiver Diameter 34 m Receiver gain 68.9 dBw System Noise Temperature 28 K Eb/No 13.5 dB Link Margin 3 dB Required Eb/No 10.5 dB BPSK modulation Data rate 9.14 Mbps Table B-5 HGA Link Budget Parameter Value Unit Comments Frequency 8 GHz X-Band downlink Transmit Power 100 W X-TWTA Transmit Power 50 dBm Transmitter Diameter 0.5 M Peak Transmitter Gain 29.8412 dBi
  • 73. Common Appendix Georgios Galanos 57 EIRP 77.8 dBm ESA 15 m Propagation path length 1.74E+06 Km Maximum distance in the orbit from Earth Space loss 236 dB Atmospheric Attenuation 1 dB Other losses 1 dB Cables, switches etc. Receiver Diameter 15 m Receiver gain 50 dBw System Noise Temperature 133 K Eb/No 13.5 dB Link Margin 3 dB Required Eb/No 10.5 dB BPSK modulation Data rate 611.863 Kbps Table B-6 LGA Link Budget B.5.3 Power Budget Phase Subsystem Average Power (W) Peak Power (W) Charge Discharge Energy Discharged (Whr) Power to charge (W) Total Power (W) Scanning Payload 56 OFF ON 222,1 Structure / Mechanics 18 Thermal 44 Comms 13,5 OBDH 33 ADCS 57,6 69 136,67 Propulsion 0 Characterisation / Payload 56 OFF ON 222,1
  • 74. Common Appendix Georgios Galanos 58 NEOs Structure / Mechanics 18 Thermal 44 Comms 13,5 OBDH 33 ADCS 57,6 69 87,74 Propulsion 0 Target Acquisition Payload 0 ON OFF 49,6 222,1 Structure / Mechanics 18 Thermal 44 Comms 13,5 OBDH 28 ADCS 69 Propulsion 0 Orbit Maintenance Payload 0 ON OFF 85,54 219,1 Structure / Mechanics 18 Thermal 0 Comms 13,5 OBDH 28 ADCS 19,5 39 Propulsion 54,56 Communications Payload 0 ON OFF 137,126 221,38 Structure / Mechanics 18 Thermal 0 Comms 30,01 OBDH 33 ADCS 3,25 39 Propulsion 0 Transfer Payload 0 ON ON 221,8 51,37 145,32 Structure / Mechanics 18 Thermal 0 Comms 2,5 30,05 OBDH 28