conference presentation - design and stability analysis of a de-orbiting system for small sats
DESCRIPTION
de Crombrugghe, Guerric; Michiels Laurent (2012). Preliminary Design and Stability Analysis of a De-Orbiting System for Small Satellites. Presentation at the 4th European CubeSat Symposium, Brussels, Belgium. 30 January - 1 February 2012. Session 8.TRANSCRIPT
Preliminary design and stability analysis of ade-orbiting system for CubeSats
Guerric de Crombrugghe & Laurent Michiels
Promoters: Pr. P. Chatelain (EPL) & Pr. Th. Magin (VKI)
Supervisor: C. Asma (VKI)
Ecole Polytechnique de Louvain, UCLouvain
January 29, 2012
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PART I: INTRODUCTION
PART II: OBJECTIVES
PART III: PROJECT STRATEGY
PART IV: APPLICATION
PART V: CONCLUSION AND PERSPECTIVES
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PART I: INTRODUCTION
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Origin of the idea: Two major concerns (1/3)
1. Atmospheric re-entry
• Key for space exploration• human spaceflight• robotic exploration on Mars, Venus,
and even Titan
• Validation tools• costly• extended development timeline
2. Debris mitigation
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Origin of the idea: Two major concerns (2/3)
1. Atmospheric re-entry
2. Debris mitigation
• Unexpected collisions betweensatellites
• Guidelines: on orbit 25 years afterthe mission’s end
• difficult to respect• especially for small satellites
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Origin of the idea: Two major concerns (3/3)
1. Atmospheric re-entry
2. Debris mitigation
Ñ Need for CubeSat re-entry vehicle
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Opportunity: QB50 (1/2)
Mission
• Initiated by the von KarmanInstitute for Fluid Dynamics
• Dedicated to in-situ exploration ofthe lower thermosphere
• Network of over fifty CubeSats
• Some of them will experience acontrolled re-entry
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Opportunity: QB50 (2/2)
Breakthrough
• QB50 opens a new type ofmissions: very low Earth orbit
• Allows for affordable in-orbitdemonstration
• New environment need forinnovative stability and de-orbitingsystem
Credits: G. Bailet
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PART II: OBJECTIVES
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Objectives
No spacecraft with such reduced dimension has ever performed acontrolled re-entry.
The challenges
• Communication: no recovery
• De-orbiting: short timescale to avoid passing over the poles
• Thermal loads: keeping the electronics below 70�C
• Stability: heat shield facing the flow
satellite’s trajectoryEarth
Ñ
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Objectives
No spacecraft with such reduced dimension has ever performed acontrolled re-entry.
The challenges
• Communication: no recovery
• De-orbiting: short timescale to avoid passing over the poles
• Thermal loads: keeping the electronics below 70�C
• Stability: heat shield facing the flow
satellite’s trajectoryEarth
Ñ
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PART III: PROJECT STRATEGY
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Survey of de-orbiting techniques (1/3)
PropulsionSatellite slowed down with an engine (chemical, cold gas, or electrical)providing thrust against its movement.
• Integration issues
• Manoeuvre complexity
Credits: ATK
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Survey of de-orbiting techniques (2/3)
TethersSatellite slowed down by electromagnetic interactions between a tetherand the Earth’s magnetic field.
• Low Technology Readiness Level (TRL)
• De-orbiting duration to count in years
Credits: NASA
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Survey of de-orbiting techniques (3/3)
Aerodynamic dragSatellite slowed down by the atmosphere.
• Fits the requirement enveloppe
• Allows for passive stabilization if well-dimensionned
Credits: NASA
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2D re-entry stability model (1/2)
Sum of forces: m BvBt� �Fg er �D eD � L eL
Sum of moments: BωBt�
Mz
Jzzez
Fg �G �MEarth
|r|2m
D � ρphq � CDph, αq �v2
2� Aref
L � ρphq � CLph, αq �v2
2� Aref
Mz � ρphq�v2
2�Aref �Lref �pC
αMph, αq�CMωph, αq�ωq
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2D re-entry stability model (2/2)
OutputAltitude, velocity, acceleration and angle of attack for every point of theobject’s trajectory.
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Numerical computation (1/2)
Rarefied flows vs continuum flows
• the satellite will experience from free-molecular while on orbit tocontinuum in lower altitudes
• degree of rarefaction defined by the Knudsen number Kn � λL
• experimentation of rarefied flows: complex and expensiveÑ numerical approach: Direct Simulation Monte Carlo (DSMC)
Y
Z
X
Mach
1412108642
Kn = 30.2Altitude = 130 kmFlow direction Ð
X Y
Z
Mach
2218141062
Kn = 2.14Altitude = 110 kmFlow direction Ð
X Y
Z
Mach
25211713951
Kn = 0.345Altitude = 100 kmFlow direction Ð
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Numerical computation (2/2)
Z
X
Y
# collisions / particle / s
26002400200016001200800
Number of collision perunit of volumeAltitude = 110 kmFlow direction Ð
Z
X
Y
Pressure (Pa)
0.450.350.250.150.05
PressureAltitude = 110 kmFlow direction Ð
Output
• Aerodynamic coefficient characterising the object as a function ofthe altitude / angle of attack.
• Flow-field description (pressure, temperature, number of collisions,etc.) allows for defining the interesting geometrical features.
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PART IV: APPLICATION
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Geometry design
BasicDirection of flight: Ò
BadmintonDirection of flight: Ò
FlowerDirection of flight: Ò
PlateDirection of flight: Ò
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Aerodynamic characteristics
10−2
100
102
104
106
1.6
1.8
2
2.2
2.4
2.6
2.8
3
Knudsen number
Dra
g c
oeffic
ient
angle of attack: 0°
angle of attack: 15°
rarefiedregime
continuumregime
transition
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Flight characteristics: Basic geometry
satellite’s trajectoryEarth
0 5 10 15100
110
120
130
140
150
160
170
180
Time (hours)
Alti
tude
(km
)
initial angle of attack: 0°initial angle of attack: 15°
107.7 km
100120140160−15
−10
−5
0
5
10
15
Altitude (km)
Ang
le o
f atta
ck (
°)
107.7km
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Flight characteristics: Plate geometry
satellite’s trajectoryEarth
0 50 100 150100
110
120
130
140
150
160
170
Time (minutes)
Alti
tude
(km
)
901101301501707720
7760
7800
7840
Altitude (km)
Abs
olut
e ve
loci
ty (
m/s
)
satellite’s velocityorbital velocity
115 m/s
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Geometry selection
• better for de-orbiting but slightly less efficient for stabilization
• more degrees of freedom
• more likely to resist
• less points of failure
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Design
• Pressure is not a problematic issue
• Passive deployment based on the drag is not possible
• Materials should be chosen for their thermal properties
• A 1 m link is optimal
• A 1 m2 plate is enough, more is not interesting
0.09 m2
satellite’s trajectoryEarth
1 m2 2 m2
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Flight characteristics: Influence of the mass
plate of 0.09 m2
0 1 2 3100
110
120
130
140
150
160
170
Time (hours)
Alti
tude
(km
)
mass: 3kgmass: 2kgmass: 4kg
Re-writing sum of forces: BvBt � �
GM|r|2
er �Dm eD �
Lm eL
Ñ The lower the mass, the greater the effect of the aerodynamic forces
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Flight characteristics: Influence of the atmospheric model
plate of 0.09 m2
0 1 2 3100
110
120
130
140
150
160
170
Time (hours)
Alti
tude
(km
)
JacchiaMSISE90 − medium activityMSISE90 − high activityMSISE90 − low activity
Expected launch window during low solar activity
Ñ Longer re-entry duration
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Flight characteristics: Influence of the trigger altitude
plate of 0.09 m2
1001201401601802000
10
20
30
40
50
60
70
80
Altitude (km)
Rad
ial v
eloc
ity (
m/s
)
trigger altitude: 150kmtrigger altitude: 200kmtrigger altitude: 170km
Trigger altitude has only an influence in the beginning the trajectory.
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PART V: CONCLUSION AND PERSPECTIVES
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Achievements
• 2D re-entry simulation tool• more accurate• adaptable to every geometry
• Design of a de-orbiting and stabilization device for QB50 re-entrysatellite
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Perspectives
• Further development of the system’s design
• Upgrade of the Simulink program
• Complete the aerodynamic coefficients databases
• Investigation of the non-monotonic behaviour of the aerodynamiccoefficients
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THANK YOUAny questions?
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