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Electromagnetic Formation Flight (EMFF) 
NIAC Phase I Review 
October 23-24, 2002 
PI: David Miller 
Co-I: Raymond Sedwick 
Massachusetts Institute of Technology 
Space Systems Laboratory
Motivation 
• Traditional propulsion uses propellant as a reaction mass 
• Advantages 
– Ability to move center of mass of spacecraft 
(Momentum conserved when propellant is included) 
– Independent (and complete) control of individual spacecraft 
• Disadvantages 
– Propellant is a limited resource 
– Momentum conservation requires that propellant mass increase 
exponentially with the velocity increment (ΔV) 
– Some propellants can be a surface contaminant to precision optics and 
solar arrays 
– Lingering propellant clouds can obscure or blind infrared telescopes 
• Is there an alternative ?? 
NIAC Phase I Midterm Review Oct 23, 2002
A Candidate Solution 
• Yes… inter-spacecraft forces can be used… 
– …provided it is not necessary to alter the center of mass motion of the 
system 
• What forces must be transmitted between satellites to allow for all relative 
degrees of freedom to be controlled? 
– In 2 dimensions, N spacecraft have 3N DOFs, but we are at most able to 
control 3N-2 (no translation of the center of mass) 
– For 2 spacecraft, that’s a total of 4: 
1 2 3 4 
• DOFs 1-3 can be controlled with inter-spacecraft axial forces and on-board 
torques, but 4 requires a transverse force 
• Electrostatic monopoles cannot provide this type of force, but Electromagnetic 
and electrostatic dipoles can! 
• Tethers attached away from the center of mass of the spacecraft will also work, 
but that’s a different project… 
• So, are there missions where controlling cluster center of mass doesn’t matter? 
NIAC Phase I Midterm Review Oct 23, 2002
EMFF Applications in 10-20 Years 
-3000 
Terrestrial Planet Finder 
-1500 
Image from 1999 TPF Book 
Cluster Reconfiguring 
0 
1500 
-3000 3000 
-1500 
0 
1500 
1500 
750 
0 
-750 
-1500 
3000 
NGST 
Docking 
NIAC Phase I Midterm Review Oct 23, 2002
EMFF Applications in 30-40 Years 
Reconfigurable Arrays & Staged Deployment 
Adaptive Membrane for Imaging 
Planet Imager 
Image from 1999 TPF Book 
NIAC Phase I Midterm Review Oct 23, 2002
Electromagnetics vs. Electrostatics 
• Electromagnetic Dipoles 
– Force Scaling: 
 
 
7 2 πμ μ π 
3 
2 
4 
2 
  
  
= − 
I NA EM ~ ( ) [ ] 
F 
a 
x 
4 10 0 
0 
– a = coil radius, x = separation distance, I = current (Amp-turns) 
• Electrostatic Dipoles 
– Force Scaling: 
4 
 
 
= − 
α π ε ε 12 2 
V NV ES ~ 24 2 8.85(10 ) [ ] 
F 
a 
x 
0 
2 
0 
  
  
– a = electrode spacing, α = electrode radius / a, V = Voltage difference 
F 
F 
μ 
I 
ε V 
α 
= 
 
  
 
  
⇒ ≈ 
 
  
 
  
1 
16 
94 
0 
2 
EM V I 
α 
2 
ES 
0 
(For break-even and comparable size) 
NIAC Phase I Midterm Review Oct 23, 2002
Is This a Lot? 
Current (amp-turns) vs. Force . 
140.0 
120.0 
100.0 
80.0 
60.0 
40.0 
20.0 
0.0 
0.0 0.2 0.4 0.6 0.8 1.0 
Force (N) . 
Current (kA) 
x/a 
30 
25 
20 
15 
10 
• For regular wire… yes (except for low force or close operations) 
• For high temperature superconducting wire… no! 
– Commercially available wire will carry 13 kA/cm2 
– Laboratory demonstrations up to 6 MA/cm2 (even in high B-field) 
• However, voltages required for Electrostatics are prohibitive 
• Debye shielding in LEO also a problem for electrostatics 
NIAC Phase I Midterm Review Oct 23, 2002
EM Design: Steerable Dipoles 
• Using ferromagnetic cores in a tetrahedron, 
the dipole direction can be steered by 
energizing different combinations 
• Tend to be heavy for a given force 
• Likewise, a set of 3 orthogonal coils 
can achieve the same effect 
• Much lighter weight 
• A set of 3 orthogonal gimbaled reaction wheels used in conjunction with these 
steerable dipoles will decouple spacecraft orientation from EM control 
• Gimbals could be locked during spin-up maneuver, and unlocked during steady-state 
spin to eliminate gyroscopic stiffening 
NIAC Phase I Midterm Review Oct 23, 2002
Satellite Formation Spin-Up 
• Electromagnets exert forces/torques on each other 
– Equal and opposite “shearing” forces 
– Torques in the same direction 
• Reaction wheels counteract EM torques 
S N 
– Resultant is shearing force 
– Angular momentum conserved by spin of the system 
S 
N 
EM Torque RW 
• There are many possible combinations of EM strength and dipole 
orientation, causing different distributions of angular momentum storage. 
Torque 
NIAC Phase I Midterm Review Oct 23, 2002
• Steady-state spin 
Steady-State Spin 
– Constant spin rate for data collection 
– Relative position and orientation maintenance 
– Disturbance rejection 
– Linearized dynamics about nominal spin 
• Optimal control design 
λ 
– Choose ratio of penalties on state and control ( ) 
– Can stabilize dynamics and reject disturbances 
• Experimental validation on linear air track 
– Similar unstable dynamics 
– Stabilized using optimal control 
acentrifugal 
acentrifugal 
N S N S 
Ω 
FEM FEM 
ρ Unstable poles: 
= ±Ω 1,2 s 
Open-Loop: Closed-Loop: 
NIAC Phase I Midterm Review Oct 23, 2002
Radar Mode Geolocation Mode 
* Figure courtesy of AFOSR Techsat21 
Research Review (29 Feb - 1 Mar 2000) 
-3000 
500m 5km 
-1500 
Optimal Cluster Reconfiguration 
0 
1500 
Reconfigure 
-3000 3000 
-1500 
0 
1500 
1500 
750 
0 
-750 
-1500 
3000 
• Multiple trajectories to initialize or 
resize the EMFF cluster 
• Can be framed as an optimal 
control problem with Quadratic 
cost function (Energy) and Linear 
dynamics (Hill Equations) 
• Balancing between power 
requirements for reaction wheels 
and electromagnets 
• Reaction wheel torques and 
power constraints must also be 
considered 
• Previous work applied to TechSat 
21 clusters for both cluster 
initialization and geo-location 
problems 
Optimal Techsat21 Cluster Re-sizing 
NIAC Phase I Midterm Review Oct 23, 2002
Disturbance Rejection 
• EMFF must counteract the disturbances present in LEO 
– Earth’s Gravitational Potential (J2) 
• Differential forces causes satellite formations to separate 
• Causes Satellite Formations to ‘Tumble’ 
– Differential Drag 
– Earth’s Magnetic Field 
• When counteracting the disturbances, EMFF produces unwanted 
torques on each spacecraft. 
• Reaction wheels are used to 
temporarily store the change 
in the angular momentum 
• The reaction wheels must be 
de-saturated by means other 
than traditional propulsion 
Differential J2 acc. (mm/s2) 
1 2 3 4 5 6 
0.0001 
0.00005 
- 0.00005 
- 0.0001 
Normal Tangential 
NIAC Phase I Midterm Review Oct 23, 2002
Angular Momentum Management 
• Zero net angular momentum gain 
– There is a limited subset of 
formation designs that produce 
zero net angular momentum gain 
• Re-phasing of the formation 
– Re-phasing causes the torques to be 
applied in the opposite direction. 
Thus de-spinning the wheels. 
Ang. Mom. (N mm s) 
Re-phase 
2 4 6 8 10 
0.8 
0.6 
0.4 
0.2 
- 0.2 
Ang. Mom. (N mm s) 
2 4 6 8 10 
0.05 
- 0.05 
- 0.1 
- 0.15 
Orbit 
Orbit 
Normal Tangential Normal Tangential 
• Earth’s magnetic field 
– By varying the dipole strength, the torque distribution can be varied without 
affecting the resulting forces. 
– If the Earth is considered as another dipole, some of the torques can be 
preferentially distributed to the earth 
NIAC Phase I Midterm Review Oct 23, 2002
Case Study: TPF Retrofit 
• PPTs 
– Higher efficiency system but still 
requires significant propellant over 
a 10 year mission lifetime 
• FEEPs 
– Ideal for very short mission lifetime 
systems (less than 6 yrs) 
– Must consider contamination issue 
• EM coil (R = 4 m) (Mtot = 4198 kg) 
– Less ideal option when compared 
to FEEPs even for long mission 
lifetime 
• EM Super Conducting Coil (R = 2 m) 
(Mtot = 3089 kg) 
– Best option if mission lifetime of 
greater than 6.2 years is desired 
– No additional mass is required to 
increase mission lifetime 
PPTs 
Colloids 
FEEPs 
Cold Gas 
EM Coil 
EM SuperCon 
Total Dry Mass 
0 1 2 3 4 5 6 7 8 9 10 
4400 
4200 
4000 
3800 
3600 
3400 
3200 
3000 
• Cold Gas and Colloids 
– Low Isp systems translate to high 
propellant requirements 
– Not viable options 
NIAC Phase I Midterm Review Oct 23, 2002
EMFF System Trades 
• Identical or Mother-Daughter Configuration for spinning case? 
• Define Mass Fractions: 
Center Spacecraft experiences no 
translation ! no mass penalty ! suggests 
larger center spacecraft 
M M inner totalarray =γ 
M =γ −1 
M outer 2 
totalarray • Identical Configuration is non-optimal 
• Higher rotation rate for mother-daughter 
configuration for fixed masses 
NIAC Phase I Midterm Review Oct 23, 2002
Phase II Objectives 
• Conduct more in-depth systems trades using various NASA missions 
– Terrestrial Planet Finder 
– Life Finder 
– Constellation-X 
• Analyze impact on various subsystems 
– Tolerance of avionics 
– Inter-vehicle power coupling 
– Inter-vehicle communications 
– Angular momentum redistribution for enabling precision operations 
• Formulate arbitrary n-body dynamics to analyze control complexity growth as a 
function of array growth 
• Build a prototype to test simultaneous control in translation and rotation 
– Coordinate with undergraduate design-build class 
– Previous classes developed SPHERES and ARGOS testbeds 
– Provides opportunity for undergraduates to participate in, and have impact 
on, space research 
NIAC Phase I Midterm Review Oct 23, 2002
Conclusions (1) 
• Lifetime and contamination are two compelling reasons to seek 
alternate solutions to using propellants 
• Dipole fields and reaction wheels can produce all of the necessary 
actuation for complete controllability of relative degrees of freedom 
• There are many missions where relative DOF control is all that is 
necessary 
– Agencies that have interest: JPL, GSFC, LMCO, NRO 
• Debye shielding in LEO, and problems with high E-fields in general 
make electrostatic dipoles less attractive (no pun intended) 
– Electrostatic monopoles could provide a stronger attractive force for 
constant spin rate, but charge exchange between spacecraft is an 
issue 
NIAC Phase I Midterm Review Oct 23, 2002
Conclusions (2) 
• Constrained Steady-state spin control has been 
demonstrated in hardware 
• In LEO, disturbance rejection is the main concern and 
angular momentum management is the biggest problem 
– Three approaches: Zero not torque solution, Re-phasing, 
Using Earth’s Field 
• EMFF retrofit of TPF looks like the best solution if FEEP 
contamination is a high risk 
• Optimal distribution of Torque for TPF-like maneuver is not 
necessarily to have identical spacecraft 
NIAC Phase I Midterm Review Oct 23, 2002

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Electromagnetic formationflightoct02

  • 1. Electromagnetic Formation Flight (EMFF) NIAC Phase I Review October 23-24, 2002 PI: David Miller Co-I: Raymond Sedwick Massachusetts Institute of Technology Space Systems Laboratory
  • 2. Motivation • Traditional propulsion uses propellant as a reaction mass • Advantages – Ability to move center of mass of spacecraft (Momentum conserved when propellant is included) – Independent (and complete) control of individual spacecraft • Disadvantages – Propellant is a limited resource – Momentum conservation requires that propellant mass increase exponentially with the velocity increment (ΔV) – Some propellants can be a surface contaminant to precision optics and solar arrays – Lingering propellant clouds can obscure or blind infrared telescopes • Is there an alternative ?? NIAC Phase I Midterm Review Oct 23, 2002
  • 3. A Candidate Solution • Yes… inter-spacecraft forces can be used… – …provided it is not necessary to alter the center of mass motion of the system • What forces must be transmitted between satellites to allow for all relative degrees of freedom to be controlled? – In 2 dimensions, N spacecraft have 3N DOFs, but we are at most able to control 3N-2 (no translation of the center of mass) – For 2 spacecraft, that’s a total of 4: 1 2 3 4 • DOFs 1-3 can be controlled with inter-spacecraft axial forces and on-board torques, but 4 requires a transverse force • Electrostatic monopoles cannot provide this type of force, but Electromagnetic and electrostatic dipoles can! • Tethers attached away from the center of mass of the spacecraft will also work, but that’s a different project… • So, are there missions where controlling cluster center of mass doesn’t matter? NIAC Phase I Midterm Review Oct 23, 2002
  • 4. EMFF Applications in 10-20 Years -3000 Terrestrial Planet Finder -1500 Image from 1999 TPF Book Cluster Reconfiguring 0 1500 -3000 3000 -1500 0 1500 1500 750 0 -750 -1500 3000 NGST Docking NIAC Phase I Midterm Review Oct 23, 2002
  • 5. EMFF Applications in 30-40 Years Reconfigurable Arrays & Staged Deployment Adaptive Membrane for Imaging Planet Imager Image from 1999 TPF Book NIAC Phase I Midterm Review Oct 23, 2002
  • 6. Electromagnetics vs. Electrostatics • Electromagnetic Dipoles – Force Scaling:   7 2 πμ μ π 3 2 4 2     = − I NA EM ~ ( ) [ ] F a x 4 10 0 0 – a = coil radius, x = separation distance, I = current (Amp-turns) • Electrostatic Dipoles – Force Scaling: 4   = − α π ε ε 12 2 V NV ES ~ 24 2 8.85(10 ) [ ] F a x 0 2 0     – a = electrode spacing, α = electrode radius / a, V = Voltage difference F F μ I ε V α =       ⇒ ≈       1 16 94 0 2 EM V I α 2 ES 0 (For break-even and comparable size) NIAC Phase I Midterm Review Oct 23, 2002
  • 7. Is This a Lot? Current (amp-turns) vs. Force . 140.0 120.0 100.0 80.0 60.0 40.0 20.0 0.0 0.0 0.2 0.4 0.6 0.8 1.0 Force (N) . Current (kA) x/a 30 25 20 15 10 • For regular wire… yes (except for low force or close operations) • For high temperature superconducting wire… no! – Commercially available wire will carry 13 kA/cm2 – Laboratory demonstrations up to 6 MA/cm2 (even in high B-field) • However, voltages required for Electrostatics are prohibitive • Debye shielding in LEO also a problem for electrostatics NIAC Phase I Midterm Review Oct 23, 2002
  • 8. EM Design: Steerable Dipoles • Using ferromagnetic cores in a tetrahedron, the dipole direction can be steered by energizing different combinations • Tend to be heavy for a given force • Likewise, a set of 3 orthogonal coils can achieve the same effect • Much lighter weight • A set of 3 orthogonal gimbaled reaction wheels used in conjunction with these steerable dipoles will decouple spacecraft orientation from EM control • Gimbals could be locked during spin-up maneuver, and unlocked during steady-state spin to eliminate gyroscopic stiffening NIAC Phase I Midterm Review Oct 23, 2002
  • 9. Satellite Formation Spin-Up • Electromagnets exert forces/torques on each other – Equal and opposite “shearing” forces – Torques in the same direction • Reaction wheels counteract EM torques S N – Resultant is shearing force – Angular momentum conserved by spin of the system S N EM Torque RW • There are many possible combinations of EM strength and dipole orientation, causing different distributions of angular momentum storage. Torque NIAC Phase I Midterm Review Oct 23, 2002
  • 10. • Steady-state spin Steady-State Spin – Constant spin rate for data collection – Relative position and orientation maintenance – Disturbance rejection – Linearized dynamics about nominal spin • Optimal control design λ – Choose ratio of penalties on state and control ( ) – Can stabilize dynamics and reject disturbances • Experimental validation on linear air track – Similar unstable dynamics – Stabilized using optimal control acentrifugal acentrifugal N S N S Ω FEM FEM ρ Unstable poles: = ±Ω 1,2 s Open-Loop: Closed-Loop: NIAC Phase I Midterm Review Oct 23, 2002
  • 11. Radar Mode Geolocation Mode * Figure courtesy of AFOSR Techsat21 Research Review (29 Feb - 1 Mar 2000) -3000 500m 5km -1500 Optimal Cluster Reconfiguration 0 1500 Reconfigure -3000 3000 -1500 0 1500 1500 750 0 -750 -1500 3000 • Multiple trajectories to initialize or resize the EMFF cluster • Can be framed as an optimal control problem with Quadratic cost function (Energy) and Linear dynamics (Hill Equations) • Balancing between power requirements for reaction wheels and electromagnets • Reaction wheel torques and power constraints must also be considered • Previous work applied to TechSat 21 clusters for both cluster initialization and geo-location problems Optimal Techsat21 Cluster Re-sizing NIAC Phase I Midterm Review Oct 23, 2002
  • 12. Disturbance Rejection • EMFF must counteract the disturbances present in LEO – Earth’s Gravitational Potential (J2) • Differential forces causes satellite formations to separate • Causes Satellite Formations to ‘Tumble’ – Differential Drag – Earth’s Magnetic Field • When counteracting the disturbances, EMFF produces unwanted torques on each spacecraft. • Reaction wheels are used to temporarily store the change in the angular momentum • The reaction wheels must be de-saturated by means other than traditional propulsion Differential J2 acc. (mm/s2) 1 2 3 4 5 6 0.0001 0.00005 - 0.00005 - 0.0001 Normal Tangential NIAC Phase I Midterm Review Oct 23, 2002
  • 13. Angular Momentum Management • Zero net angular momentum gain – There is a limited subset of formation designs that produce zero net angular momentum gain • Re-phasing of the formation – Re-phasing causes the torques to be applied in the opposite direction. Thus de-spinning the wheels. Ang. Mom. (N mm s) Re-phase 2 4 6 8 10 0.8 0.6 0.4 0.2 - 0.2 Ang. Mom. (N mm s) 2 4 6 8 10 0.05 - 0.05 - 0.1 - 0.15 Orbit Orbit Normal Tangential Normal Tangential • Earth’s magnetic field – By varying the dipole strength, the torque distribution can be varied without affecting the resulting forces. – If the Earth is considered as another dipole, some of the torques can be preferentially distributed to the earth NIAC Phase I Midterm Review Oct 23, 2002
  • 14. Case Study: TPF Retrofit • PPTs – Higher efficiency system but still requires significant propellant over a 10 year mission lifetime • FEEPs – Ideal for very short mission lifetime systems (less than 6 yrs) – Must consider contamination issue • EM coil (R = 4 m) (Mtot = 4198 kg) – Less ideal option when compared to FEEPs even for long mission lifetime • EM Super Conducting Coil (R = 2 m) (Mtot = 3089 kg) – Best option if mission lifetime of greater than 6.2 years is desired – No additional mass is required to increase mission lifetime PPTs Colloids FEEPs Cold Gas EM Coil EM SuperCon Total Dry Mass 0 1 2 3 4 5 6 7 8 9 10 4400 4200 4000 3800 3600 3400 3200 3000 • Cold Gas and Colloids – Low Isp systems translate to high propellant requirements – Not viable options NIAC Phase I Midterm Review Oct 23, 2002
  • 15. EMFF System Trades • Identical or Mother-Daughter Configuration for spinning case? • Define Mass Fractions: Center Spacecraft experiences no translation ! no mass penalty ! suggests larger center spacecraft M M inner totalarray =γ M =γ −1 M outer 2 totalarray • Identical Configuration is non-optimal • Higher rotation rate for mother-daughter configuration for fixed masses NIAC Phase I Midterm Review Oct 23, 2002
  • 16. Phase II Objectives • Conduct more in-depth systems trades using various NASA missions – Terrestrial Planet Finder – Life Finder – Constellation-X • Analyze impact on various subsystems – Tolerance of avionics – Inter-vehicle power coupling – Inter-vehicle communications – Angular momentum redistribution for enabling precision operations • Formulate arbitrary n-body dynamics to analyze control complexity growth as a function of array growth • Build a prototype to test simultaneous control in translation and rotation – Coordinate with undergraduate design-build class – Previous classes developed SPHERES and ARGOS testbeds – Provides opportunity for undergraduates to participate in, and have impact on, space research NIAC Phase I Midterm Review Oct 23, 2002
  • 17. Conclusions (1) • Lifetime and contamination are two compelling reasons to seek alternate solutions to using propellants • Dipole fields and reaction wheels can produce all of the necessary actuation for complete controllability of relative degrees of freedom • There are many missions where relative DOF control is all that is necessary – Agencies that have interest: JPL, GSFC, LMCO, NRO • Debye shielding in LEO, and problems with high E-fields in general make electrostatic dipoles less attractive (no pun intended) – Electrostatic monopoles could provide a stronger attractive force for constant spin rate, but charge exchange between spacecraft is an issue NIAC Phase I Midterm Review Oct 23, 2002
  • 18. Conclusions (2) • Constrained Steady-state spin control has been demonstrated in hardware • In LEO, disturbance rejection is the main concern and angular momentum management is the biggest problem – Three approaches: Zero not torque solution, Re-phasing, Using Earth’s Field • EMFF retrofit of TPF looks like the best solution if FEEP contamination is a high risk • Optimal distribution of Torque for TPF-like maneuver is not necessarily to have identical spacecraft NIAC Phase I Midterm Review Oct 23, 2002