low energy transfers in the solar system: applications i

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Low Energy Transfer Applications MWL - [email protected] JPL 2004 Summer Workshop on Advanced Topics in Astrodynamics Low Energy Transfers in the Solar System: Applications I Objectif Lune (Tintin) 7/5/2004 2004 Summer Workshop on Advanced Topics in Astrodynamics Martin.Lo@ jpl.nasa.gov

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Low Energy Transfers in the Solar System: Applications I Objectif Lune ( Tintin ). Martin.Lo @ jpl.nasa.gov. 7/5/2004. 2004 Summer Workshop on Advanced Topics in Astrodynamics. Interplanetary Superhighway. JPL Lagrange Group. 1/21/03. Outline. - PowerPoint PPT Presentation

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Page 1: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 1

[email protected]

JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Low Energy Transfers in the Solar System:

Applications I

Objectif Lune (Tintin)

7/5/2004 2004 Summer Workshop on Advanced Topics in Astrodynamics

Martin.Lo@ jpl.nasa.gov

Page 2: Low Energy Transfers                            in the Solar System: Applications I

1/21/03 JPL Lagrange Group

Interplanetary Superhighway

Page 3: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 3

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Outline

• Restricted 3 Body Problem Review– Interactive Shooting Method

– Weak Stability Boundary Method (Tuesday)

– Dynamical System Methods

• Goal and Philosophy

• Low Energy Transfers in Earth-Moon Space– Shoot the Moon

– Lunar L1 Gateway

– Lunar Sample Return

– New Mission Concepts & Orbits

• Low Energy Transfers Between Galilean Moons– Petit Grand Tour

– Jupiter Icy Moons Tour

– Anatomy of a Flyby

Page 4: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 4

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Outline I: Objectif Lune

• Restricted 3 Body Problem Review

• Low Energy Transfers in Earth-Moon Space– Shoot the Moon

– Lunar L1 Gateway

– Lunar Sample Return

– Potential New Mission Orbits

Page 5: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 5

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Some Historical Notes • Classical 3-Body Problem

Newton, Euler, Lagrange, Jacobi , Moulton

• Dynamical Systems Theory– Poincaré, Birkhoff, Moser, Conley, McGehee

• Development of Libration Missions– Colombo, Farquhar, Dunham, Folta

• Dynamical Systems Theory for Libration Missions (mid 1980’s)– Simó, Llibre, Goméz, Masdemont, Jorba, Martinez

• Weak Stability Boundary– Miller & Belbruno (1990)

• Resonant Transport via Invariant Manifolds– Bolt & Meiss (1995), Schroer & Ott (1996)

• Mission Design Using Invariant Manifolds– Howell, Lo (1996)

Page 6: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 6

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

First Halo Oribt Mission: ISEE3/ICE

LOGO.049

Goddard Space Flight Center

GSFC: Farquhar, Dunham, Folta, et al

Courtesy of D. Folta, GSFC

Page 7: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 7

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Current Libration Missions

• z

WIND SOHO ACE

GENESISMAP JWST

LOGO.049

Goddard Space Flight Center

Courtesy of D. Folta, GSFC

Page 8: Low Energy Transfers                            in the Solar System: Applications I
Page 9: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 9

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Genesis Mission Design, Comet Orbit

Martin Lo JPL Genesis Mission Design Manager

Kathleen Howell Purdue University Department of Aeronautics and Astronautics

Brian Barden JPL, Purdue University

Roby Wilson JPL, Purdue University

Belinda Marchand Purdue University

Page 10: Low Energy Transfers                            in the Solar System: Applications I

Genesis Mission: Uses LGenesis Mission: Uses L11, L, L22 Heteroclinic Heteroclinic Behavior to Collect & Return Solar Wind Behavior to Collect & Return Solar Wind

Samples to Earth Samples to Earth UTTR 84 x 30 km

September 8th, 2004!

Page 11: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 11

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

The Genesis Trajectory

L1L2Sun (size &

position not to scale)

2Lunar Orbit

1 3

4 5

Begin Science

End Science

1. Transfer 2. Science3. Return4. Entry5. Backup

Page 12: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 12

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Stable Manifold Transfer to Halo Orbit

Page 13: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 13

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Stable Manifold for Genesis Transfer

Page 14: Low Energy Transfers                            in the Solar System: Applications I

Lunar Orbit

L1

L2

Halo OrbitPortal

Earth

10/17/2001

Genesis Unstable Manifold: Unifies Many Different Types

of Orbital Motions

JPL Lagrange Group

Earth Flyby & Capture Earth Return

Via L2

Lunar Capture

Lunar Flyby Escape to Earth Trailer

Page 15: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 16

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Restricted Three Body Problem (RTBP)

• Newton, first studied the 3 Body Problem

• Rotating Frame

• Euler: L1, L2, L3

• Lagrange: L4, L5

• Restricted Problem– 3rd body infinitessimal– Two primaries move in

circles– Sun-Earth-Spacecraft,

Sun-Jupiter-Comet, …

• Jacobi Integral

Page 16: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 17

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Restricted Three Body Problem

• Simplified model with energy integral– Useful for analytic studies– Symmetries avoid phasing and timing problems

• Still non-integrable, i.e. no orbital elements– Solutions requires numerical integration– Key Problem: How to replace orbital elements?

• Model sufficiently faithful for mission design– Can “move” solutions into full JPL ephemeris models– Key Problem: How to move solutions between

models?

Page 17: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 18

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Coupled Restricted Three Body Problem

• Simplified Model of Solar System– More complex than Copernican coupled “two body problems”

• Example: Sun-Earth-Moon-Spacecraft System

– Earth-Moon-S/C: LL1, LL2, … LL5

– Sun-Earth-S/C: EL1, EL2, …

Page 18: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 19

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

• (a) Planet, Sun, eXterior regions separated by grey

forbidden region

• (b) L1 energy level opens regions between P and S

• (c) L2 energy level opens regions between P, S, and X

• (d) L4 and L5 regmain trapped in grey region

Projection of Energy Surfaces at 4 Levels

x x x x

Page 19: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 20

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

From AU to au: Comets & Atomic Physics

Atomic L1

Comet’s Potential Energy Surface

Comet L1 , L2

• Uncanny Similarity of Transport Theory in 3 Body Problem

• Rydberg Atom In Cross Fields

• Chemical Transition State Theory

• Jupiter

• Nucleus

• Jupiter

Atomic Halo Orbit

Atomic Potential Energy Surface

Page 20: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 21

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Dynamical Systems Theory

Page 21: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 25

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Orbital Zoology Near the Lagrange Points

• Four Families of Orbits, Conley [1968], McGehee [1969], Ref. Paper

• Periodic Orbit (Planar Lyapunov)

• Spiral Asymptotic Orbit (Stable Manifold Pictured)

• Transit Orbits

• Non-Transit Orbits (May Transit After Several Revolutions)

Page 22: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 27

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Poincare Sections

Orbits

.. ..Poincare Map

• Invariant Manifold Structures in Higher Dimensions Too Complex

• Poincare Sections Reduce the Dimensions by 1

• Turns Differential Equations into Maps in Phase Space

• Periodic Orbits Become Finite Number of Points

• Chaotic Orbits Cover Large Portions of Phase Space

• Reveals Resonance Structure of Phase Space

• Show the Existence of Chaos in the System

Page 23: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 28

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Mapping the Space Using Cross Sections

.

.Orbits

..

PoincareMap

.

Page 24: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 29

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Manifolds Connect Solar System

Legend

Comets

Asteroids

Kuiper Belt

Object

L1 IPS Orbits

L2 IPS Orbits

Jupiter

Saturn

Uranus

Neptune

(Lo & Ross)

Page 25: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 33

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Page 26: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 34

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Page 27: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 35

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Invariant Manifolds & Jupiter Comets

• Transport Between 3:2 and 2:3 resonances – Via heteroclinic orbits between orbits around JL1, JL2

– Temporary Capture (Ballistic Capture)Koon, Lo, Marsden, Ross, 2000

Howell, Marchand, Lo, 2000Belbruno, B. Marsden, 1997: WSB Theory

Page 28: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 36

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Shoot the Moon!

RESCUE MISSION 911:

Hiten, HAC, …

Discover, June 1999

Page 29: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 37

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Shoot the Moon

Shadowing Unstable Manifold of

Sun-Earth L2 Lyapunov Orbit

Shadowing Stable Manifold of Sun-

Earth L2 Lyapunov Orbit to Leave Earth

Earth

Lunar Orbit

Maneuver to Transfer to Stable Manifold of Earth-Moon L2 Lyapunov Orbit

Ballistic Lunar Capture

Shoot the Moon: Low Energy Transfer & Ballistic Capture

Page 30: Low Energy Transfers                            in the Solar System: Applications I

7/5/04 JPL Lagrange Group

Gateway Module

LL1

Moon

Lunar L1 Entry Portal

Lunar Orbit

LL2Lunar L2 Exit Portal

Lunar L1 Gateway Station

Page 31: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 39

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Problem: Human Service to Libration Missions

• ISSUE: 3 Months Transfers to EL2 Too Long for Humans

• Short Transfers Too Difficult

• Infrastructure Too Expensive

STA-103 astronauts replaced gyros needed for orientation of the Hubble Space Telescope.

JSC

TPF @Earth L2

Page 32: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 40

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Page 33: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 41

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Lunar L1 to Earth L2 Transfer

• Build Instruments & S/C Lunar L1 Station

• Transfer S/C from L1 to Earth-L2 LIO (Libration Oribit)

• Service S/C at Earth L2 LIO from Lunar L1 Gateway Hub

L1

Lunar L2

Earth

L2

Lunar Rotating Frame Earth Rotating Frame

Lunar

Page 34: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 42

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Solution: Human Servicing at Lunar L1 Gatewy

• Build Instruments & S/C Lunar L1 Gateway for EL2

• Service S/C at Earth L2 from Lunar L1 Gateway Module

EARTH

EARTH L2 HALO ORBIT

MOON

LUNAR L1 HALO ORBIT

LUNAR L2 HALO ORBIT

LUNAR L1 GATEWAY

ARTIST CONCEPTION

Page 35: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 43

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

IPS in Earth’s Neighborhood

• Portals/Interchange = Halo Orbits, Unstable Orbits

• Lanes = Invariant Manifold Tubes

EARTH

EARTH L2 HALO ORBIT

MOON

LUNAR L1 HALO ORBIT

LUNAR L2 HALO ORBIT

LUNAR L1 GATEWAY

ARTIST CONCEPTION

Page 36: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 44

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Gateway Architecture (JSC)

Crew departs from and returns

to ISSL1 Gateway

GPS Constellation

Lunar Lander

Crew Transfer Vehicle•Transports crew between ISS and Gateway•Nominal aerocapture to ISS, or direct Earth return contingency capability

“Earth’s Neighborhood”

Lunar Habitat

L1 Gateway

•“Gateway” to the Lunar surface•Outpost for staging missions to Moon, Mars and telescope construction•Crew safe haven

Lunar Lander•Transports crew between Gateway and Lunar Surface•9 day mission (3 days on Lunar surface)

Lunar Habitat•30-day surface habitat placed at Lunar South Pole•Enables extended-duration surface exploration and ops studies

Crew Transfer Vehicle

Source: James Geffre, JSC

Page 37: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 45

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

Gateway Configurations (JSC)

LEO, Transit, L1 Stand-by Configuration

Telescope Operations ConfigurationLunar Operations Configuration

Launch Configuration

Source: James Geffre, JSC

Page 38: Low Energy Transfers                            in the Solar System: Applications I

8/6/2002

Goto LSR Vugraphs

JPL Caltech

Lunar Orbit

Lunar Sample Return via the Interplanetary

Supherhighway

EL1

Moon

Earth

Moon

LL2

LanderSeparation

Lander

Orbiter

EL2

LanderReturn

LL2 Stable Manifold Insertion

LanderReturn

Page 39: Low Energy Transfers                            in the Solar System: Applications I

Low Energy Transfer Applications

MWL - 47

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JPL

2004 Summer Workshop on Advanced Topics in Astrodynamics

New Mission Concepts & Orbits