The e.Deorbit CDF Study - Space...
Transcript of The e.Deorbit CDF Study - Space...
ESA UNCLASSIFIED – Releasable to the Public
The e.Deorbit CDF Study
A design study for the safe removal of a large space debris
Robin Biesbroek and the e.Deorbit CDF [email protected]
6th IAASS ConferenceMontréal, Canada, 22/05/2013
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 2
ESA UNCLASSIFIED – Releasable to the Public
e.Deorbit Mission Objectives
1. The mission is to perform active space debris removal
a. uncooperative target (large satellite or upper
stage) with heavy mass
b. in the 800-1000 km SSO/polar region
2. A study to design this mission was launched in the frame
of ESA Cleanspace initiative
3. The e.Deorbit study was performed in ESA’s Concurrent
Design Facility (CDF) between June and September
2012.
ESTEC CDF is a state-of-the-art facility equipped with a
network of computers, multimedia devices and software
tools, allowing a team of experts from several disciplines
to apply the concurrent engineering method to the design
of future space missions (www.esa.int/cdf)
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 3
ESA UNCLASSIFIED – Releasable to the Public
e.Deorbit Mission Objectives
The e.Deorbit CDF study is intended to produce a preliminary system design for
the most promising option(s), identify the required technology roadmap(s), and
investigate its (their) applicability to relevant ESA missions. In details:
1. Assess the feasibility of a mission for the controlled de-orbiting and re-entry
of a large target in SSO, using technologies analyzed in previous CDF
studies (e.g. tentacles, robotic arm, harpoon, net, …)
2. Carry out a system level conceptual design of the spacecraft with the
participation of all discipline specialists
3. Trade-off different mission scenarios
4. Assess programmatics, risk and cost aspects of the various alternatives
5. Consolidate the technology road maps in line with the programmatic aspects
of the mission
6. Evaluate the applicability of the technologies to different categories of
satellites and debris remediation mission
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 4
ESA UNCLASSIFIED – Releasable to the Public
Target assumptions
1. The target is in the ±8t mass range
2. The target is inactive, not cooperative, and not passivated
3. The orbit is SSO, ±800 km, near dawn-dusk
4. It is assumed that the target LV-PL adapter zone is not accessible (deployed solar
panel may obstruct it)
5. Long term attitude assumption: gravity-gradient stabilized (various attitudes possible)
6. Possibility of oscillation around equilibrium with angular rates comparable with ω0
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 5
ESA UNCLASSIFIED – Releasable to the Public
Will the target break up?
1. Analysis of Fragmentation Events in
DISCOS (257 total, 58 relevant)
2. Analysis concentrated on SSO missions
only and excluded (Russian)
reconnaissance: this leaves 15 events
3. Statistics with low confidence (only 15
events for EO satellites) however results
allow to assume that the target will likely
be still intact after 10 years in orbit
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 6
ESA UNCLASSIFIED – Releasable to the Public
Mission timeline
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 7
ESA UNCLASSIFIED – Releasable to the Public
Main system trade-off options
1. Disposal:
a. Re-orbit to >2000 km
b. De-orbit to <600 km
c. Controlled re-entry
2. Propulsion:
a. Chemical (CP)
b. Electrical (EP)
3. Capture technique:
a. Robotic arm
b. Tentacles
c. Net
d. Ion-beam shepherd
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 8
ESA UNCLASSIFIED – Releasable to the Public
System trade-off (re-orbit & de-orbit to 600 km)
Re-o
rbit
De-o
rbit t
o 6
00 k
m
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 9
ESA UNCLASSIFIED – Releasable to the Public
System trade-off (controlled re-entry)Contr
olled r
e-e
ntr
y
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 10
ESA UNCLASSIFIED – Releasable to the Public
System trade-off results
Two options received the best scores in terms of cost, programmatics,
safety and risk evaluation criteria:
Tentacles option
• Controlled re-entry
• Chemical propulsion
• Capture with tentacles
Net option
• Controlled re-entry
• Chemical propulsion
• Capture with net
For these options a conceptual design was performed by the CDF team,
which is shown in the following slides
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 11
ESA UNCLASSIFIED – Releasable to the Public
Tentacles Option
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 12
ESA UNCLASSIFIED – Releasable to the Public
Tentacles: launch & transfer
1. S/C main dimension of 1.2 x 1.2m x 2.92m
2. Fits in Vega LV fairing
3. 4x 425N bi-prop thrusters mounted on the side panel (w.r.t.
launch configuration)
4. Injection orbit:
• The lower the altitude, the higher the S/C dry mass
• Injection altitude: 300 km
• circular orbit
• Inclination: 98.2 deg
• Daily launch opportunity
• Launcher performance: 1660 kg
5. Launcher dispersions correction: 7m/s (also covers the
phasing worst case)
6. Hohmann transfer from injection orbit to target orbit (260
m/s)
7. RDV with target followed by attitude manoeuvre to match
rotation
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 13
ESA UNCLASSIFIED – Releasable to the Public
Tentacles: capture
1. Strategy :
a. Capture a holding point using a robotic arm
b. Embrace the target with clamping mechanism so that it
cannot escape
c. Positively lock the clamping mechanism with a force higher
than the de-orbiting force (using pushing rods based on
IBDM actuator)
d. Composite (chaser + target) is stiff during de-orbit operation
e. The method is generic: it can be applied to the LV I/F
adapter
2. Is the robotic arm necessary?
a. If no robotic arm is used, bouncing may occur
b. Current simulations make the assumption that there is no relative
motion between chaser & target during the clamping mechanism closing
time (after AOCS cut-off and before achieving capture)
c. Detailed analysis should conclude if this assumption is valid or not
d. If not, a robotic arm is used to achieve the first capture; allows to guide
the clamping mechanism to a position suitable for capture
e. The robotic arm also helps for contingency reasons
3. For this reason a robotic arm is baseline, at the price of an extra cost
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 14
ESA UNCLASSIFIED – Releasable to the Public
Tentacles: de-orbit strategy
1. Impulsive burn: 202 m/s
2. Initial mass: 9350 kg
3. Engine Isp: 321 s
4. Different set of engines: 1x425 N, 2x425 N = 850 N, 4x425 N = 1700 N, 8x425 N = 3400 N, 16x425 N = 6800 N
5. Different scenarios:a. Immediate de-orbit
b. Perigee reduction to 200 km, then re-entry
c. One intermediate perigee altitude to 200 km, then re-entry
d. Two intermediate perigee altitude to 200 km, then re-entry
e. Three intermediate perigee altitude to 200 km, then re-entry
6. In case of intermediate perigee altitudes, they are optimised to minimise the gravity losses
7. Final burn should lower the perigee to 40 km in order to obtain <3000 km footprint
If one burn, 4x425 N is
recommended to get
reasonable gravity losses
If 3+1 = 4 burns, 2x425 N or even
1x425 N is enough
Baseline for tentacles option: 2x425N
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 15
ESA UNCLASSIFIED – Releasable to the Public
Tentacles: Baseline design overview (1)
Spacecraft Characteristics
Mass
Dry mass 784.2 kg
Propellant
mass810 kg
Total mass 1648 kg incl. adapter
AOCS/GNC
3-axis stabilized
Sensors
3 x Star Tracker
2 x Sun Sensor
2 x IMU
2 x GPS receiver
2 x LiQuaRD LiDAR
2 x Far Field Camera
2 x Near Field Camera
Actuators 4 x Reaction Wheels
RCS 24 x 22 N Thrusters
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 16
ESA UNCLASSIFIED – Releasable to the Public
Tentacles: Baseline design overview (2)
Spacecraft Characteristics
Propulsion
Bi-propellant system
Main Engine: 2 x 425N LAE (+ 2 redundant)
Tanks: 4 polar mounted based on Eurostar 2000, 2
pressurant tanks
Power
SA
1 wing
Solar cells: 30% 3J GaAs
Area: 2.8 m2
785 W (EOL)
Battery1 x Lithium Ion ( -HC cells)
BoL energy: 562 Wh
Bus 28V MPPT dual reg/unregulated bus
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 17
ESA UNCLASSIFIED – Releasable to the Public
Tentacles: Baseline design overview (3)
Spacecraft Characteristics
Communications
TDRS – S-
band
2 x TRSP
3 x Antenna
2 x HPA
DTE – X-
band
2 x TRSP
3 x Omniantenna
Thermal MLI, OSR, black paint, heaters
DHSdynamically reconfigurable payload processor
(DRPM)
Mechanism
Clamping mechanisms & drive mechanism
Pushing rods
SADM & SADE
Robotics Robotic arm incl. gripper
StructureBox-shaped structure with central shear panel and
stiffeners for the tank panels
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 18
ESA UNCLASSIFIED – Releasable to the Public
Net Option
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 19
ESA UNCLASSIFIED – Releasable to the Public
Net: launch & transfer
1. Use Ø 937mm VEGA I/F
2. Ø 937mm central cylinder (2.4m high)
3. 2x Ø 430mm pressurant tanks (inside the central cylinder)
4. Use 4x425N biprop thrusters + 4x ATV 220N thrusters
5. Solar Panel of 2m x 1m x 1.5m
6. Injection orbit same as Tentacles option:• The lower the altitude, the higher the S/C dry mass
• Injection altitude: 300 km
• circular orbit
• Inclination: 98.2 deg
• Daily launch opportunity
• Launcher performance: 1660 kg
7. Launcher dispersions correction: 7m/s (also covers the phasing worst case)
8. Hohmann transfer from injection orbit to target orbit
(260 m/s)
9. RDV with target (up to 50 m)
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 20
ESA UNCLASSIFIED – Releasable to the Public
Net: capture
1. Approximately 250 (~6000 DOF per simulation) multi-body simulations performed:
a. Included capture of the target, tensioning, and de-orbitation burn.b. For a variety of relative rotation rates, velocity, tether parameters and
controllers2. Mesh: 2m (to limit computation time), 0.25m shall be analysed
The following parameters were varied in the 250
simulations:
a. Relative position (3 axis)
b. Relative rotation (3 angles)
c. Relative rotation rates (3 axis)
d. Relative motion (3 axis)
e. Tether length
f. Tether stiffness
g. Tether material damping
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 22
ESA UNCLASSIFIED – Releasable to the Public
Net: de-orbit strategy
1. Impulsive burn: 202 m/s
2. Initial mass: 9350 kg
3. Engine Isp: 321 s
4. Different set of engines: 1x425 N, 2x425 N = 850 N, 4x425 N = 1700 N, 8x425 N = 3400 N, 16x425 N = 6800 N
5. Different scenarios:a. Immediate de-orbit
b. Perigee reduction to 200 km, then re-entry
c. One intermediate perigee altitude to 200 km, then re-entry
d. Two intermediate perigee altitude to 200 km, then re-entry
e. Three intermediate perigee altitude to 200 km, then re-entry
6. In case of intermediate perigee altitudes, they are optimised to minimise the gravity losses
7. Multiple burns lead to complicate AOCS control of the stack
If one burn, 4x425 N is
recommended to get
reasonable gravity losses
If 3+1 = 4 burns, 2x425 N or even
1x425 N is enough
Baseline for net: 2x425N+ 2x220N (pulse mode / off modulation)
option for net
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 23
ESA UNCLASSIFIED – Releasable to the Public
Net: Baseline design overview (1)
Spacecraft Characteristics
Mass
Dry mass 708.9 kg
Propellant
mass878.2 kg
Total mass 1622 kg incl. adapter
AOCS/GNC
3-axis stabilized
Sensors
3 x Star Tracker
2 x Sun Sensor
2 x Gyrometer
2 x GPS receiver
2 x LiQuaRD LiDAR
2 x Far Field Camera
RCS 24 x 22 N Thrusters
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 24
ESA UNCLASSIFIED – Releasable to the Public
Net: Baseline design overview (2)
Spacecraft Characteristics
Propulsion
Bi-propellant system
Main Engine: 4 x 425N LAE (+ 2 redundant)
4 x 220 N thruster
Tanks: 4 polar mounted based on Eurostar 2000,
3 pressurant tanks
Power
SA
2 wings
Solar cells: 30% 3J GaAs
Area: 2.8 m2
785 W (EOL)
Battery1 x Lithium Ion (- HC cells)
BoL energy: 562 Wh
Bus 28V MPPT unregulated bus
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 25
ESA UNCLASSIFIED – Releasable to the Public
Net: Baseline design overview (3)
Spacecraft Characteristics
Communications
TDRS – S-
band
2 x TRSP
2 x Antenna
2 x HPA
DTE – X-band2 x TRSP
2 x Omniantenna
Thermal MLI, OSR, black paint, heaters
DHSdynamically reconfigurable payload processor
(DRPM)
Mechanism
2 x Net & ejector
2 x Tether & Cable Cutter
2 x SADM & SADE
StructureCentral cylinder with box-shaped structure around,
stabilized with shear panels
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 26
ESA UNCLASSIFIED – Releasable to the Public
e.Deorbit CDF study: conclusions
• Two options were designed showing feasible first assessments
a. Both are similar in mass & dimensions and appear suitable for a VEGA launch within one decade
b. Net option shows fewer severe risk items, is less sensitive to target shape, 6-7% cheaper and 6 months lower development time
• Open points tentacles:
a. Further analysis of the rendezvous and mating operations for the option using only the tentacles (need for extra LIDAR, tentacles closing parameters)
b. Good models of the target and sensor models are required, namely for the points being used for relative navigation in the close range (SAR antenna)
c. Need for ground in the loop for the capture operations has to be re-assessed
d. Structural integrity of the target holding points should be further analyzed
• Open points net:
a. Plume impingement and chemical reactions with the tether material.
b. ATD analysis for optimization of the thrusters configuration of both the multi and single burn designs (number of thrusters, tilting angle, TPS required)
c. Tether cutting scenario, behavior of the tether after cutting, interaction with following capture
d. Optimization of the tether control and tensioning ΔV can have an important impact on the propellant mass
e. Detailed analysis and definition of the operation concept for the de-orbit phase and tether dynamics damping
f. For single-burn option, out-gassing of the TPS after orbit raise burn should be assessed (even though it is a shorter burn)
e.Deorbit CDF Study | Robin Biesbroek | 6th IAASS Conference | Montreal, Canada, 22/05/2013 | Slide 27
ESA UNCLASSIFIED – Releasable to the Public
Life after the e.Deobit CDF study
1. Three system activities were initiated:
a. Service oriented approach towards the procurement/development of an
ADR mission (Astrium SAS, Kayser Threde, SSTL)
2. Activities in support of ADR capturing (ITT already issued):
a. Advanced GNC for ADR (net/tether control during burns)
b. Assessment and simulation of a tentacles based capture mechanism for ADR
3. GSP proposals (detumbling, etc.)
4. GSTP compendium published on EMITS
a. GNC activities (nav-cam, LIDAR, image recognition)
b. Net activities (characterisation and 0g testing, throwing mechanism,
locking)
c. Clamping mechanism activities (breadboard)
d. Other sub-systems (harpoon, ATD, reconfigurable payload processor)
e. Debris attitude modelling
5. E.Deorbit Phase A ITT release planned for Summer 2013