Ion propulsion is an efficient form of spacecraft propulsion that can enable high-speed space travel using small amounts of propellant. It works by ionizing and accelerating propellant with electricity, allowing spacecraft to attain high velocities. Recent NASA missions like Dawn have demonstrated the advantages of ion propulsion, such as reaching high speeds while consuming minimal propellant. This makes ion propulsion potentially more cost-effective than traditional chemical propulsion for deep space missions.
This presentation gives an overview of the networking and conceptualize the terms of the Satellite networking systems, and also provide a glance of the typical functionality of the satellite system in establishing the worldwide mobile communication system, as well as the broadcasting system.
With the support and encouragement of my faculty and friends developed this presentation...
Thank you
Gravitational Wave Astronomy is a fascinating discovery made a few years ago that changed the notions of modern physics. This presentation won the 3rd Prize in the SPIE student chapter's Oral Presetation in my college.
Gravitational waves are 'ripples' in the fabric of space-time caused by some of the most violent and energetic processes in the Universe. Albert Einstein predicted the existence of gravitational waves in 1916 in his general theory of relativity.
Gravitational waves are ripples in the curvature of spacetime that propagate as waves at the speed of light, generated in certain gravitational interactions that propagate outward from their source.these are very much different from all other topics regarding gravitation.
Observation of gravitational waves from a binary black hole mergerSérgio Sacani
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave
Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in
frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0 × 10−21. It matches the waveform
predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the
resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a
false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater
than 5.1σ. The source lies at a luminosity distance of 410þ160
−180 Mpc corresponding to a redshift z ¼ 0.09þ0.03 −0.04 .
In the source frame, the initial black hole masses are 36þ5
−4M⊙ and 29þ4
−4M⊙, and the final black hole mass is
62þ4
−4M⊙, with 3.0þ0.5 −0.5M⊙c2 radiated in gravitational waves. All uncertainties define 90% credible intervals.
These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct
detection of gravitational waves and the first observation of a binary black hole merger
Kinetic Energy Transfer of Near-Earth Objects for Interplanetary Manned Missi...Winston Sanks
This report outlines the rationale, procedures, technical feasibility, risk assessment, and cost-benefit
analysis of utilizing a Near-Earth Object, 101955 Bennu (provisional designation 1999 RQ36 - the target of
the OSIRIS-REx mission), as a source of energy to minimize the propulsion requirements of an
interplanetary spacecraft. The planet Mars is the target body in this study and the outbound Trans-Mars
injection in the years between 2175 and 2199 will be analyzed (within this timeframe Bennu’s orbit is
predicted to approach Earth within two Earth radii on at least 80 occasions). The Mars orbit insertion burn,
Trans-Earth injection burn, and Earth orbit insertion burn are assumed to be achieved with propulsive
maneuvers outlined in standard manned interplanetary mission architectures. To accomplish this mission,
two methods of transferring kinetic energy are examined: direct capture and release of the asteroid by a
spacecraft using a Kevlar net and an inertial reel, and indirect capture by establishing a station on the
asteroid to manufacture compressed material from the carbonaceous regolith in order to fire a mass stream
to be captured by the spacecraft. This mission architecture analysis takes into account the associated safety
risks of perturbations within Bennu’s orbit (which could result in inaccurate rendezvous location
predictions), the implications of altering the orbit of 101955 Bennu after transferring a portion of its energy
(since there is a possibility of collision with Earth in the late 22nd century if the asteroid is slowed too
significantly), g-limit restrictions of the spacecraft and its occupants during an acceleration by the asteroid,
and the possibility of a collision between Bennu and the spacecraft. In addition, the cost-benefit
considerations of this mission architecture are weighed. This examination concludes that a direct capture Net
and Reel system aboard the spacecraft is not a viable capture method due to an insufficient maximum ΔV
available through a best-case perfectly elastic collision (capture) with the asteroid, as well as a prohibitive
weight penalty aboard the spacecraft due to the Net and Reel system. However, this report finds that the
method of establishing a station on Bennu with the capability to separate mass from the asteroid and fire it at
a spacecraft is a plausible (if costly) means of transferring a significant ΔV. A KETNEO-FIMM Asteroid
Station mission architecture could also be used in subsequent interplanetary missions providing cost-sharing
over many decades for future interplanetary missions.
This presentation gives an overview of the networking and conceptualize the terms of the Satellite networking systems, and also provide a glance of the typical functionality of the satellite system in establishing the worldwide mobile communication system, as well as the broadcasting system.
With the support and encouragement of my faculty and friends developed this presentation...
Thank you
Gravitational Wave Astronomy is a fascinating discovery made a few years ago that changed the notions of modern physics. This presentation won the 3rd Prize in the SPIE student chapter's Oral Presetation in my college.
Gravitational waves are 'ripples' in the fabric of space-time caused by some of the most violent and energetic processes in the Universe. Albert Einstein predicted the existence of gravitational waves in 1916 in his general theory of relativity.
Gravitational waves are ripples in the curvature of spacetime that propagate as waves at the speed of light, generated in certain gravitational interactions that propagate outward from their source.these are very much different from all other topics regarding gravitation.
Observation of gravitational waves from a binary black hole mergerSérgio Sacani
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave
Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in
frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0 × 10−21. It matches the waveform
predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the
resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a
false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater
than 5.1σ. The source lies at a luminosity distance of 410þ160
−180 Mpc corresponding to a redshift z ¼ 0.09þ0.03 −0.04 .
In the source frame, the initial black hole masses are 36þ5
−4M⊙ and 29þ4
−4M⊙, and the final black hole mass is
62þ4
−4M⊙, with 3.0þ0.5 −0.5M⊙c2 radiated in gravitational waves. All uncertainties define 90% credible intervals.
These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct
detection of gravitational waves and the first observation of a binary black hole merger
Kinetic Energy Transfer of Near-Earth Objects for Interplanetary Manned Missi...Winston Sanks
This report outlines the rationale, procedures, technical feasibility, risk assessment, and cost-benefit
analysis of utilizing a Near-Earth Object, 101955 Bennu (provisional designation 1999 RQ36 - the target of
the OSIRIS-REx mission), as a source of energy to minimize the propulsion requirements of an
interplanetary spacecraft. The planet Mars is the target body in this study and the outbound Trans-Mars
injection in the years between 2175 and 2199 will be analyzed (within this timeframe Bennu’s orbit is
predicted to approach Earth within two Earth radii on at least 80 occasions). The Mars orbit insertion burn,
Trans-Earth injection burn, and Earth orbit insertion burn are assumed to be achieved with propulsive
maneuvers outlined in standard manned interplanetary mission architectures. To accomplish this mission,
two methods of transferring kinetic energy are examined: direct capture and release of the asteroid by a
spacecraft using a Kevlar net and an inertial reel, and indirect capture by establishing a station on the
asteroid to manufacture compressed material from the carbonaceous regolith in order to fire a mass stream
to be captured by the spacecraft. This mission architecture analysis takes into account the associated safety
risks of perturbations within Bennu’s orbit (which could result in inaccurate rendezvous location
predictions), the implications of altering the orbit of 101955 Bennu after transferring a portion of its energy
(since there is a possibility of collision with Earth in the late 22nd century if the asteroid is slowed too
significantly), g-limit restrictions of the spacecraft and its occupants during an acceleration by the asteroid,
and the possibility of a collision between Bennu and the spacecraft. In addition, the cost-benefit
considerations of this mission architecture are weighed. This examination concludes that a direct capture Net
and Reel system aboard the spacecraft is not a viable capture method due to an insufficient maximum ΔV
available through a best-case perfectly elastic collision (capture) with the asteroid, as well as a prohibitive
weight penalty aboard the spacecraft due to the Net and Reel system. However, this report finds that the
method of establishing a station on Bennu with the capability to separate mass from the asteroid and fire it at
a spacecraft is a plausible (if costly) means of transferring a significant ΔV. A KETNEO-FIMM Asteroid
Station mission architecture could also be used in subsequent interplanetary missions providing cost-sharing
over many decades for future interplanetary missions.
Advance Propulsion System in Space Exploration - Ion PropulsionVINOTHE9
As part of the assignment for the course Propulsion 2, a presentation was given on an overview of advanced propulsion systems. The presentation specifically focused on electric propulsion systems, including ion propulsion. It also covered the Dawn Mission and the MIT Ion Propulsion Glider.
Ultrafast transfer of low-mass payloads to Mars and beyond using aerographite...Sérgio Sacani
With interstellar mission concepts now being under study by various space agencies and institutions,
a feasible and worthy interstellar precursor mission concept will be key to the success of the long
shot. Here we investigate interstellar-bound trajectories of solar sails made of the ultra lightweight
material aerographite. Due to its extremely low density (0.18 kgm−3) and high absorptivity (∼1), a
thin shell can pick up an enormous acceleration from the solar irradiation. Payloads of up to 1 kg can
be transported rapidly throughout the solar system, e.g. to Mars and beyond. Our simulations consider
various launch scenarios from a polar orbit around Earth including directly outbound launches as well
as Sun diver launches towards the Sun with subsequent outward acceleration. We use the poliastro
Python library for astrodynamic calculations. For a spacecraft with a total mass of 1 kg (including
720 g aerographite) and a cross-sectional area of 104 m2, corresponding to a shell with a radius of 56m,
we calculate the positions, velocities, and accelerations based on the combination of gravitational and
radiation forces on the sail. We find that the direct outward transfer to Mars near opposition to Earth
results in a relative velocity of 65 kms−1 with a minimum required transfer time of 26 d. Using an
inward transfer with solar sail deployment at 0.6AU from the Sun, the sail’s velocity relative to Mars
is 118 kms−1 with a transfer time of 126 d, whereMars is required to be in one of the nodes of the two
orbital planes upon sail arrival. Transfer times and relative velocities can vary substantially depending
on the constellation between Earth andMars and the requirements on the injection trajectory to the Sun
diving orbit. The direct interstellar trajectory has a final velocity of 109 kms−1. Assuming a distance
to the heliopause of 120AU, the spacecraft reaches interstellar space after 5.3 yr. When using an
initial Sun dive to 0.6AU instead, the solar sail obtains an escape velocity of 148 kms−1 from the
solar system with a transfer time of 4.2 yr to the heliopause. Values may differ depending on the
rapidity of the Sun dive and the minimum distance to the Sun. The mission concepts presented in this
paper are extensions of the 0.5 kg tip mass and 196m2 design of the successful IKAROS mission to
Venus towards an interstellar solar sail mission. They allow fast flybys atMars and into the deep solar
system. For delivery (rather than fly-by) missions of a sub-kg payload the biggest obstacle remains in
the deceleration upon arrival.
Ok, we found a new Earth nearby. Next question is: how do we get there?
The amazing challenge to get mankind to become an interstellar species and how we could potentially get there.
The different technologies involved and the key challenges to overcome.
Welcome to teh next chapter of mankind.
Orbit design for exoplanet discovery spacecraft dr dora musielak 1 april 2019Dora Musielak, Ph.D.
Most exoplanets have been discovered with space telescopes. Starting with an overview of rocket propulsion, this presentation introduces spacecraft trajectories in the Sun-Earth-Moon System, focusing especially on those appropriate for exoplanet detection spacecraft. It reviews past, present, and future exoplanet discovery missions.
THE HUMAN CHALLENGES OF CONQUERING SPACE AND COLONIZING OTHER WORLDS.pdfFaga1939
This article aims to present the human challenges of the conquest of space and the human colonization of other worlds. These challenges are described below:
1- Production of rockets that reach speeds close to that of light to travel to the limits of the Universe
2- Production of technologies capable of protecting human beings in space travel
3- Identification of other Earth-like worlds capable of being habitable by humans
4- Enabling human beings to survive in space and in habitable places outside Earth
1. Ion Propulsion: The Future of Space Travel
Jacob Benner, Augustana College
Abstract:
Chemical propulsion is typically the main type of propulsion used today. Recently however, ion propulsion technology has been implemented in space missions such as NASA’s Deep Space 1 and Dawn.
These missions, in particular the Dawn mission, have shed a great deal of light on the advantages of ion thruster systems. By using ionized propellant and sending it through a electrode grid, high
velocities can be attained with little propellant. This reduces the cost of the missions which makes ion propulsion an appealing new approach to space travel.
Introduction:
Since the space race of the 1950’s people have been
fascinated with space travel. Because of that, there have
been vast improvements in the field. Despite this there is
still a problem that gets in the way of going deeper into
space, time and distance. Increasing propulsion velocity is
the most effective way to travel deeper into space. Today
most propulsion systems are chemical based. The most
promising propulsion system however, is ion propulsion.
Ion propulsion offers a more efficient system and higher
velocities.
Conclusion:
• Ion propulsion is an efficient way of space travel
• Great velocities achievable
• High specific impulse
• Ion propulsion is cost effective
How Ion Propulsion works:
In a typical ion propulsion system electrons are
generated by the discharge cathode. The electrons flow
out of the cathode and are attracted to the chamber
walls. The walls are charged with a high positive
potential from the ship’s power supply. These electrons
then ionize the propellant (an inert gas, typically xenon)
by electron bombardment. These ions are then
accelerated using two electrodes (ion optics or grids).
There is an upstream grid and a downstream one. The
upstream grid is highly positively charged, whereas the
downstream grid is highly negatively charged. Since
these ions are highly positive they are accelerated
through the grid at high rates of speed. This creates a
stream of ion jets. Since the thrusters exhaust speed is
based on the voltage applied to the electrodes the speed
attainable is very high. Now, because the thruster expels
positive ions an equal amount of negative ions must be
expelled to keep the charge of the beam equal. Because
of this an extra cathode is added called the neutralizer
to release the extra ions.
*This process is seen in Figure 1 below
Figure 2: an ion thrusters operation. Photo courtesy of NASA
Specific Impulse (Isp):
Definition- thrust divided by weight of propellant
per unit time.
Specific impulse gives a effeciency of a propulsion
system. A higher specific impulse suggests a lower
mass of propellant, higher thrust or both. Therefore,
a higher specific impulse is desired. Figure 2 shows
the relationship between the specific impulse and
mass of the propellant for ion thrusters. This data is
assuming two ion thrusters producing a thrust of
25kN. The data shows how specific impulse can be
attained with little propellant showcasing the ion
propulsion systems efficiency.
NASA’s Dawn Spacecraft:
NASA is currently conducting a mission using ion thruster
technology. The spacecraft (Dawn) is expected to venture 3
billion miles to the asteroid Vesta and the dwarf planet Ceres.
Feats of the spacecraft include:
• Surpassing Deep Space 1’s all-time velocity record at 9,600
mph.
• Reached this velocity using only 165 kg of propellant.
• Over the course of the mission Dawn will reach a velocity of
24,000 mph.
• In a year of thruster operation the spacecraft will reach a
speed of 5,500 mph with only the equivalent of 16 gallons of
gas.
Figure 3: Propellant Mass versus Specific impulse. Graph shows three different points off
the earth. From 300km off earths surface more propellant is required to reach needed
Isp than from 2000km off earths surface and even more so from geosyncronous transfer
orbit (42,164km).
Graph courtesy of: “The impact of advanced platform and ion propulsion technologies
on small, low-cost interplanetary spacecraft”
Figure 1: velocity versus time for the Dawn space mission. The slow acceleration of
ion thrusters is evident.
Data from: “NASA Spacecraft Breaks Speed Boost Record”
Cost:
Ion thrusters are not only efficient but also cost effective. We
see this present in the Dawn mission. NASA says this about
the mission “The use of ion propulsion, combined with other
systems that have extensive flight heritage, allows a project
that can yield significant advances in planetary science at an
affordable price”. The affordability of these projects is a major
advantage of using ion propulsion systems.
References:
• Clark, Stephen D., and David G. Fearn. "The impact of advanced platform and ion propulsion
technologies on small, low-cost interplanetary spacecraft." Acta Astronautica 59.8-11 (2006):
899-910. Print.
• "Ion Propulsion." NASA. NASA, n.d. Web. 14 Mar.
2013.<http://www.nasa.gov/centers/glenn/about/fs21grc.html>.
• Chow, Denise. "NASA Spacecraft Breaks Speed Boost Record." Space. N.p., 11 June 2010. Web.
29 Apr. 2013. <http://www.space.com/8579-nasa-spacecraft-breaks-speed-boost-
record.html>.
• Marc, Rayman D., et al. "Dawn:A mission in development for exploration of main belt
asteroids Vesta and Ceres." Acta Astronautica 58 (2006): 605-15. Print.
• "Spacecraft Propulsion." Wikiipedia. N.p., n.d. Web. 6 May 2013.
<http://en.wikipedia.org/wiki/ Spacecraft_propulsion#Electromagnetic_propulsion>.
Engine
Effective
Exhaust
Velocity
(km/s)
Specific
Impulse
(s)
Fuel mass
(kg)
Energy
required
(GJ)
Energy
per kg
of
propellant
minimum
power/thr
ust
Power
generator
mass/thru
st*
Solid Rocket
1 100 190,000 95 500 kJ 0.5 kW/N N/A
Bipropellant
Rocket
5 500 8,200 103 12.6 MJ 2.5 kW/N N/A
Ion Thruster 50 5,000 620 775 1.25 GJ 25 kW/N 25 kg/N
Rocket propulsion vs. Ion Propulsion:
Chemical propulsion, also known as rocket propulsion, is the most
commonly used propulsion method. Below is a table comparing
rocket and ion propulsion in different categories. This data
assumes a mass of 10,000kg and a delta V of 3000m/s. It also
assumes a specific power of 1kW/kg. Ion propulsion has a great
exhaust velocity and specific impulse which are desired. It also has
the lowest fuel mass which means it is most efficient. The
downsides of ion propulsion rather than rocket propulsion is it
requires more energy, power, and mass.
Figure 4: comparison of different propulsion systems.
Table courtesy of: “Space Propulsion”