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Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

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Page 1: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Predicting the Future of the Solar System:Nonlinear Dynamics, Chaos and Stability

Dr. Russell HermanUNC Wilmington

Page 2: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Outline

• Chaos in the Solar System

• The Stability of the Solar System

• Linear and Nonlinear Oscillations

• Nonspherical Satellite Dynamics

• Numerical Studies

• Summary

Page 3: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The Solar System

Planet

Orbit Parameters

Distance PeriodInclination(degrees) Eccentricity

Compared to Earth

Mercury 0.387 0.241 7 0.206

Venus 0.723 0.615 3.39 0.007

Earth 1.00 1.00 0 0.017

Mars 1.524 1.88 1.85 0.093

Jupiter 5.203 11.86 1.3 0.048

Saturn 9.539 29.46 2.49 0.056

Uranus 19.18 84 0.77 0.047

Neptune 30.06 164.8 1.77 0.009

Pluto 39.53 247.7 17.15 0.248

Page 4: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Chaos in the Solar System

Page 5: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Chaos in the News

Page 6: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Kirkwood Gaps

http://ssd.jpl.nasa.gov/a_histo.html

Daniel Kirkwood -1886

Few asteroids have an orbital period close to1/2, 1/3, or 2/5 that of Jupiter

Due to Mean Motion Resonances

3:1 Resonance - the asteroid completes 3 orbits for every 1 orbit of Jupiter

Page 7: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington
Page 8: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Celestial Mechanics – from Aristotle to Newton

• Aristotle 384-322 BCE• Hipparchus of Rhodes 190-120 BCE – season errors• Claudius Ptolemy 85- 165 – epicycles• Nicolaus Copernicus 1473-1543 – heliocentric • Tycho Brahe 1546-1601 – planetary data • Galileo Galilei 1564-1642 – kinematics • Johannes Kepler 1571-1630 – Planetary Laws • Sir Isaac Newton 1642-1727 – Gravity/Motion

Robert Hooke 1635-1703 – Inverse Square?• Edmond Halley 1656-1742 - Comets • … Euler, Laplace, Lagrange, Jacobi, Hill, Poincare, Birkhoff ...

Page 9: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The Stability of the Solar System

• King Oscar II of Sweden - Prize: How stable is the universe?

• Jules Henri Poincaré (1854-1912)– Sun (large) plus one planet (circular orbit)

• Stable

– Added 3rd body – not a planet!• Strange behavior noted • … not periodic!

– But there is more …

Page 10: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Sensitivity to Initial Conditions"A very small cause which escapes our notice determines a

considerable effect that we cannot fail to see, and then we say that the effect is due to chance. If we knew exactly the laws of nature and the situation of the universe at the initial moment, we could predict exactly the situation of the same universe at a succeeding moment. But even if it were the case that the natural laws had no longer any secret for us, we could still know the situation approximately. If that enabled us to predict the succeeding situation with the same approximation, that is all we require, and we should say that the phenomenon had been predicted, that it is governed by the laws. But is not always so; it may happen that small differences in the initial conditions produce very great ones in the final phenomena. A small error in the former will produce an enormous error in the latter. Prediction becomes impossible...". (Poincaré)

Page 11: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Can one predict the motion of a single planet

a billion years from now?

• Laplace and Lagrange – Yes

• Poincare’ – No

• Lyapunov – speed neighboring orbits diverged

• Lorenz – 1963 – “Butterfly Effect”

Page 12: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Solar System Simulations• Sun plus 7 planets – 21 degrees of freedom• Numerical Studies

– Mitchtchenko and Ferraz-Mello 2004• 35 Gyr – 660 MHz Alpha 21264A – 15 weeks of CPU time

– 1988 – Sussman and Wisdom • Lyapunov time - 10 Myrs

– Laskar, et. Al. • 8 planets w/corrections – 5 Myrs• 1 km error = 1 au error in 95 Myrs

• Planets– Pluto – chaotic– Inner Planets – chaotic– Earth – stabilizer

• Klavetter – 1987– Observations of Hyperion wobbling

Page 13: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Nonlinear DynamicsContinuous Systems

• Simple Harmonic Motion

• Phase Portraits

• Damping

• Nonlinearity

• Forced Oscillations

• Poincaré Surface of Section

Page 14: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Linear Oscillations

2

2d x

m kxdt

2

21d qq

LCdt

2

2d g

Ldt

22

2d x

xdt

Page 15: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Phase Portrait for

0 1

0

x xdk

v vdtm

dxv

dtdv k

xdt m

2

2d x

m kxdt

Equilibrium:

0 0, 0dx dv

x vdt dt

Classification by Eigenvalues:

2 0k

m

-5 0 5-5

-4

-3

-2

-1

0

1

2

3

4

5y(2) vs y(1)

y(1)

y(2)

System:

Page 16: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Damped Oscillations

2

2d x dx

m kx bdtdt

0 1

/ /

x xd

v k m b m vdt

2 0m b k

System:

Classification by Eigenvalues:

2 4

2 2

b b mk

m m

-2 -1.5 -1 -0.5 0 0.5 1 1.5 2-2

-1.5

-1

-0.5

0

0.5

1

1.5

2Damped Pendulum

xy

Page 17: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Nonlinear Pendulum 2

2sin

d x gx

Ldt

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

•Integrable Hamiltonian System

•Separatrix

•Perturbations – entangle stable/unstable manifolds

Page 18: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Damped Nonlinear Pendulum

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

No Damping vs Damping

Page 19: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Forced Oscillations2

2cos 2

d xm kx A ftdt

0 1 0

/ 0 cos 2

x xd

v k m v A ftdt

System:

Resonance

Page 20: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Phase Plots – Forced Pendulum

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

No Damping vs Damping

Page 21: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Poincaré Surface of Section2

2cos 2

d xm kx A ftdt

System:

cos

2

dxv

dtdv k

x Adt md

fdt

Regular orbit movie (Henon-Heiles equations)

Page 22: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Damped, Driven Pendulum

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

-8 -6 -4 -2 0 2 4 6 8-5

-4

-3

-2

-1

0

1

2

3

4

5v vs x

x

v

No Damping vs Damping

Page 23: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The Onset of Chaos

Lorenz Equations, Strange Attractors, Fractals …

-2 -1.5 -1 -0.5 0 0.5 1 1.5 2-2

-1.5

-1

-0.5

0

0.5

1

1.5

2

x

yPoincare Section of the Duffing System

Page 24: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Nonspherical Satellites

• Hyperion

• Rotational Motion

• Orbital Mechanics

• Nonlinear System

• Phase Portraits

http://www.solarviews.com/cap/ast/toutat9.htm

Page 25: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Hyperion

  MPEG (no audio)

http://www.planetary.org/saturn/hyperion.html

http://www.nineplanets.org/hyperion.html

Page 26: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The Hyperion Problem

Page 27: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Rotational Motion

Page 28: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Computing Torque I

Page 29: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Computing Torque II

Page 30: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Computing Torque III

Page 31: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Summary

Page 32: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Orbital Motion

Page 33: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Constants of the Motion

Page 34: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Equation of the Orbit

Page 35: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Orbit as a Function of Time

Page 36: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Kepler’s Equation I

Page 37: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The Anomalies

Page 38: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Kepler’s Equation II

Page 39: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The Reduced Problem

Page 40: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

The System of Equations

Page 41: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Dimensionless System

Page 42: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Numerical Results

Page 43: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Spin-Orbit Resonance

• Satellite moves about Planet– triaxial (A<B<C)– Keplerian Orbit

• Nearly Hamiltonian System– Oblateness Coefficient – Orbital Eccentricity

• Resonance Trev/Trot = p/q– 1:1 – Synchronous – like Moon-Earth– Mercury 3:2

Page 44: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Moon e = 0.0549, = 0.026

Page 45: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Mercury e = 0.2056, = 0.017

Page 46: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

e = 0.02

Page 47: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

e= 0.04

Page 48: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

e = 0.06

Page 49: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

e = 0.08

Page 50: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

e = 0.10

Page 51: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

= 0.1

Page 52: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

= 0.3

Page 53: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

= 0.5

Page 54: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

= 0.7

Page 55: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

= 0.9

Page 56: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

Summary• Chaos in the Solar System

• The Stability of the Solar System

• Linear and Nonlinear Oscillations

• Nonspherical Satellite Dynamics

• Numerical Studies

• Where now?

Page 57: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

More in the Fall …

Page 58: Predicting the Future of the Solar System: Nonlinear Dynamics, Chaos and Stability Dr. Russell Herman UNC Wilmington

References