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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS - - PowerPoint PPT Presentation

6 th International Conference on Astrodynamics Tools and Technique (ICATT) INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS LI Xiangyu, Qiao Dong, Cui Pingyuan Beijing Institute of Technology Institute of Deep Space


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Beijing Institute of Technology Institute of Deep Space Exploration Technology

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

LI Xiangyu, Qiao Dong, Cui Pingyuan

6th International Conference on Astrodynamics Tools and Technique (ICATT)

15 March 2016

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  • I. Introduction
  • II. Concept of Indirect Planetary Capture
  • III. Orbit Selection for Periodic Orbit
  • IV. Simulation and Comparisons
  • V. Conclusion

Contents

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

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  • I. Introduction

Planetary Capture  A key process in planet exploration mission  Plays an important role in the trajectory design

Interplanetary Trajectory Mission Orbits

Planetary Capture

Capture Trajectory Design Fuel Consumption Flight System Design Interplanetary Trajectory Design Midcourse Correction INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

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4

Current Capture Strategy  Direct Capture  Aerocapture  Ballistic Capture

Easy to design INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • I. Introduction

Exploits the gravitational force of planets to capture a spacecraft Take advantage of the aerodynamic force to reduce the velocity

From Belbruno and Miller 1993

Single impulsive maneuver at periapsis

v 

p

r v

Fuel Saving Protection for high heat rate and overload Precise guidance and control Low energy Capture Long transfer time Multi capture

  • pportunities

Fall when is high

v

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5

Circular Restricted Three body Problem (CRTBP)  Libration(Lagrange) Points  Periodic orbits  Stable/Unstable Manifolds

Space observation Capture to periodic orbit Low energy transfer

3 3 3 3 3 3

(1 )( ) ( 1 ) 2 (1 ) 2 (1 )

s m s m s m

x x x y x r r y y y x y r r z z z r r                                    

Communication relay

  • I. Introduction

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS Planetary Capture

Nakamiya and Scheeres (2008,2010) Wang (2014)

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Concept  Use periodic orbit as a park orbit  Connect with interplanetary trajectory by stable manifolds  Connect with mission orbit by unstable manifolds

Periapsis maneuver Stable manifold Periapsis maneuver Periodic orbit about libration points Interplanetary Trajectory Unstable manifold Mission orbit Small perturbation

  • II. Concept of Indirect Planetary Capture

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

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  • II. Concept of Indirect Planetary Capture

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

Process  Three impulsive maneuver First periapsis maneuver Perturbation to generate unstable manifolds Second Periapsis maneuver

1

v v  

2

v 

3

, v a e   Initial guess and correction

Process  Three impulsive maneuver First periapsis maneuver Perturbation to generate unstable manifolds Second Periapsis maneuver

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  • II. Concept of Indirect Planetary Capture

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

Maneuver  Three impulsive maneuver First periapsis maneuver Perturbation to generate unstable manifolds Second Periapsis maneuver

1

v v  

2

v 

3

, v a e   Initial guess and correction

Design  Construct the periodic parking orbit  Generate proper unstable manifolds same periapsis distance as mission orbit  Generate proper stable manifolds for interplanetary design and midcourse correction

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  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

Orbit Selection  Two criteria

  • Energy constrain

First maneuver as low as possible

  • State constrain

The periapsis distance of natural unstable manifolds should close to that of mission orbits

1

v 

2 1

2 2

ex ps ex es ps ps

v v v v v v r r  

        2

es ps

v r  

2 1 2 3 3 2 2

2 2 1 2 2 2 2

p p ps p p p p p

v r r v r r r r v v r r       

  

         

0,

ps

v v r

    

Periapsis of stable manifolds should close to the surface of Mars

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • III. Orbit Selection for Periodic Orbit

Sun-Mars System Planar Orbits  Planar Lyapunov orbit

  • L1 orbit from to
  • L2 orbit from to

Periapsis distance of stable manifolds

4

7.3 10

y

A km  

5

7.5 10

y

A km  

5

1.0 10

y

A km  

6

1.5 10

y

A km  

5

5.5 10

yc

A km  

5

5.7 10

yc

A km  

Critical amplitude

yc

A

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  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

Planar Orbits Periapsis distance of unstable manifolds from to

5

5.5 10

y

A km  

Candidate parking orbits

L1 orbit from L2 orbit from

5

5.7 10

y

A km  

3589km 300000km

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Planar Orbits  Periapsis State Periapsis phase angle

  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

 10   20 ~ 50 

L1:

190   140 ~ 260

L2:

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • III. Orbit Selection for Periodic Orbit

Sun-Mars System Spatial Orbits  Vertical Lyapunov orbit Large periapsis distance Infeasible  Halo orbit

  • L1 orbit from to
  • L2 orbit from to

Periapsis distance of stable manifolds

5

2.9 10

zc

A km  

Critical amplitude

4

2.7 10

z

A km  

4

6.6 10

z

A km  

4

3.7 10

z

A km  

5

6.5 10

z

A km  

5

2.9 10

zc

A km  

zc

A

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  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

Halo Orbits Periapsis distance of unstable manifolds from to Candidate parking orbits

L1 orbit from to L2 orbit from to

3589km 300000km

5

2.9 10

z

A km  

5

2.9 10

z

A km  

5

6.6 10

z

A km  

5

6.5 10

z

A km  

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Halo Orbits  Periapsis State Orbital Inclination Periapsis phase angle Periapsis Spatial angle

  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

 20 i 

L1: L2:

 i 140 i  20 i  130 i 

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Halo Orbits  Periapsis State Orbital Inclination Periapsis phase angle Periapsis Spatial angle

  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

 10  

L1: L2:

 i 5 ~ 20 190   182 ~ 202

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Halo Orbits  Periapsis State Orbital Inclination Periapsis phase angle Periapsis Spatial angle

  • III. Orbit Selection for Periodic Orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

 19  

L1: L2:

 i 41   17   40  

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

 Direct capture  Indirect capture First impulsive maneuver Perturbation velocity Third impulsive maneuver

2

2 (1 )

d p p

e v v r r  

    

(1 )

p

r a e  

2 1

2

ps ps

v v v r 

   

3

(1 )

pu p

e v v r     

2

1 / v m s  

1 2 3

v v v v      3589

ps

r km 

s p u

T T T T   

Capture Time

s

T

Stable manifold transfer time

p

T

Parking time

u

T

Unstable manifold transfer time

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

 Mission Orbit I 200km circular orbit  Parking orbit L2 planar Lyapunov orbit

5

5.7 10

y

A km   (km/s) Direct Capture (km/s) Indirect capture (km/s) (km/s) (day) 1.88 1.780 1.779 775.37 0.001 2.09 1.859 1.858 0.001 3.39 2.492 2.487 0.005

v

d

v  v 

T

d

v v   

Low orbit capture:

  • Cost the same velocity as direct capture

Long transfer time Provides a chance to explore the space environment in the vicinity of Mars and Lagrange points without extra velocity increment

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

 Mission Orbit I 200km circular orbit  Parking orbit L2 planar Lyapunov orbit

5

5.7 10

y

A km  

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

 Mission Orbit II 800km*60000km elliptic orbit  Parking orbit L2 Halo orbit (km/s) Direct Capture (km/s) Indirect capture (km/s) (km/s) (day) 1.88 0.518 0.493 696.85 0.025 2.09 0.602 0.572 0.030 3.39 1.272 1.205 0.067

v

d

v  v 

T

d

v v   

5

4.6 10

z

A km  

Middle orbit capture:

  • As the periapsis of mission orbit increases, the indirect capture

requires less velocity than direct capture

  • Save more fuel for higher excess velocity v
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 Mission Orbit II 800km*60000km elliptic orbit  Parking orbit L2 Halo orbit

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

5

4.6 10

z

A km  

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

 Mission Orbit III 20000km circular orbit  Parking orbit L1 Halo orbit (km/s) Direct Capture (km/s) Indirect capture (km/s) (km/s) (day) 1.88 1.329 0.897 691.03 0.432 2.09 1.481 0.976 0.505 3.39 2.540 1.609 0.931

v

d

v  v 

T

d

v v   

5

3.4 10

z

A km  

High orbit capture:

  • Save more than 30% velocity
  • Keep the same efficiency in high v
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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • IV. Simulation and Comparisons

 Mission Orbit III 20000km circular orbit  Parking orbit L1 Halo orbit

5

3.4 10

z

A km  

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  • IV. Simulation and Comparisons

INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

 Mission Orbit IV Elliptic orbit with different periapsis distances  Parking orbit L1 Lyapunov orbit

0.9 e 

  • Cost is approximately constant regardless of the periapsis distance

2.5 / v km s

 

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS

  • V. Conclusion

 Indirect capture could save velocity increment than direct capture at the cost of long transfer time  Shows better efficiency for high altitude and high

  • rbit

insertion  Extra scientific returns  Increases transfer flexibility  Reduce gravity loss

v

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INDIRECT PLANETARY CAPTURE VIA PERIODIC ORBIT ABOUT LIBRATION POINTS