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ASTM001/MTH724U SOLAR SYSTEM. Carl Murray / Nick Cooper. Lecture 2: Structure of the Solar System. Books That Changed the World. The Almagest. Copernicus’ De Revolutionibus Orbium Celestium. Kepler’s Harmonices Mundi. The Five Convex Regular Polyhedra. cube. octahedron. tetrahedron.
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ASTM001/MTH724U SOLAR SYSTEM Carl Murray / Nick Cooper Lecture 2: Structure of the Solar System
The Five Convex Regular Polyhedra cube octahedron tetrahedron icosahedron dodecahedron
Kepler’s Model of Planetary Spacing • Each planet moves in a shell separated from next by regular polyhedron • Six planets separated by five shells • Thickness of shell is important • Ordering of polyhedra is important Orbits of Jupiter, Saturn and Mars
The “Retrograde” Path of Mars Apparent motion of Mars, June – November 2003
Kepler’s First Law The planets move in ellipses with the Sun at one focus
Kepler’s Second Law A line drawn from the Sun to a planet sweeps out equal areas in equal times
Kepler’s Third Law It is most certain and most exact that the proportion between the periods of any two planets is precisely three halves the proportion of the mean distance J. Kepler, 15 May 1618 The square of the orbital period of a planet is proportional to the cube of its semi-major axis
Daphnis making waves in the Keeler Gap Keeler Gap ‘Fast lane’ Arrows show direction of motion of ring particles relative to Daphnis ‘Slow lane’
Newton’s Universal of Gravitation Any two bodies attract each other with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between them
Newton’s Laws of Motion • Bodies remain in a state of rest or uniform motion unless acted upon by a force • The force experienced by a body is equal to the rate of change of momentum • To every action there is an equal and opposite reaction
Orbit Determination Choose an appropriate mathematical model for the orbit. The model is defined by a set of parameters. The numerical values of the model parameters are initially unkown. Orbit Models Fixed Ellipse 2-body Point-masses Orbital elements Precessing Ellipse 2-body Oblate primary Orbital elements Full Equations of Motion n-body Oblate primary Position/velocity Use the model to estimate the observed quantities. Iteratively solve for the set of parameter values which generates a satisfactory match between the estimated and actual observations.
Titius’ 1766 Translation of Bonnet’s Contemplation de la Nature
The Titius-Bode ‘Law’ of Planetary Distance The distance of a planet from the Sun obeys a geometric progression.
Uniqueness of Uranian System Actual system: Generate 100,000 sets of 5 satellites and calculate best fit for each set
The Saturn System (as of 1997) 2:1 2:1 4:3
The Geometry of Orbital Resonance 2:1 Resonance, Stable configuration: 2:1 Resonance, Unstable configuration:
Resonance in the Saturn System • Saturn Ring Features (gaps, edge waves, density waves) • Janus : Epimetheus (co-orbital - horseshoe motion) • Dione : Helene : Polydeuces (co-orbital - tadpole motion) • Tethys : Telesto : Calypso (co-orbital - tadpole motion) • Mimas : Tethys (4:2) • Titan : Hyperion (4:3) • Enceladus : Dione (2:1) • Mimas : Anthe (10:11), Mimas : Methone (14:15), Mimas : Aegaeon (7:6) • Most regular satellites are in synchronous rotation (like The Moon). Hyperion (shown in the movie) is an exception. Hyperion
Polydeuces Longitude lag (deg) Longitude lag (deg) Helene Saturn Dione Y (km) Polydeuces X (km)
Resonance in the Uranus System Currently no known resonances between the major satellites 5:3 near-resonance between Cordelia and Rosalind Anomalously high inclination of Miranda (4.22 deg) suggests existence of resonances in the past
Resonance in Uranus’ Ring System 24:25 resonance between Cordelia and epsilon ring inner edge 14:13 resonance between Ophelia and epsilon ring outer edge
Resonance in Neptune’s Ring System 42:43 resonance between Galatea and Adams ring
Resonance in the Planetary System Jupiter-Saturn near 5:2 resonance Neptune-Pluto 3:2 resonance
Spin-orbit Resonance in the Planetary System Mercury 3:2 spin-orbit resonance Pluto-Charon 1:1:1 spin-orbit resonance
Preference for Commensurability Two orbits are commensurate when For orbits in the solar system Let ratio be bounded by and Let
Preference for Commensurability A: Enceladus-Dione B: Mimas-Tethys C: Titan-Hyperion D: Io-Europa E: Europa-Ganymede F: Neptune-Pluto
Websites NASA Solar System Exploration http://solarsystem.nasa.gov/index.cfm JPL Solar System Dynamics http://ssd.jpl.nasa.gov JPL Cassini http://saturn.jpl.nasa.gov/ Royal Astronomical Society http://www.ras.org.uk