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Homework. Turn in first page of Icarus article (now) Read Chapter 1: 19 pages (by Tuesday) Read Chapter 13: 37 pages (by Thursday) Review Equations (pending). Possible Projects. hot topics Messenger results Spirit/Opportunity results Dawn results Cassini results
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Homework Turn in first page of Icarus article (now) Read Chapter 1: 19 pages (by Tuesday) Read Chapter 13: 37 pages (by Thursday) Review Equations (pending) Planetary Sciences
Possible Projects hot topics Messenger results Spirit/Opportunity results Dawn results Cassini results outstanding objects Jovian moons edge of the Solar System (KBOs/SDOs) comet chemistry planet formation the “Nice Model” timescales in Solar System formation chaos in planetary motions life in the Solar System organisms on Mars mission to Mars humans in space observing project … INDEPENDENT AND NEW 2
Nomenclature • terrestrials • Mercury, Venus, Earth, Mars • many moons • jovians • gas giants • Jupiter, Saturn • ice giants • Uranus, Neptune • minor planets • asteroids • Main Belt • Near-Earth Objects (NEOs) • Trojans (and Greeks and Hildas) • Trans-Neptunian Objects (TNOs) • Plutinos (Classical) Kuiper Belt Objects (KBOs) • Centaurs Scattered Disk Objects (SDOs) • comets
non-trends in the Solar System surface gravities not radically different obliquities do not behave 7 large moons are worlds of their own: Moon, Io, Europa, Ganymede, Callisto, Titan, Triton Planetary Sciences
Asteroids Ceres Vesta Eros Itokawa
Asteroidssemimajor axis Trojans Earth has 1 Mars has 6 + Jupiter has 5221 + Neptune has 7 + ?! Hildas Planetary Sciences
Absolute Magnitude = H V magnitude if 1 AU from Earth and 1 AU from Sun while having phase angle of 0 degrees (an impossible scenario) H = 16 means diameter of 2-4 km Planetary Sciences
Asteroidseccentricity Planetary Sciences
Asteroidsinclination Planetary Sciences
Inner S.S. 2009 ASTEROIDS green dots: “normal” m.p. red dots: < 1.3 AU periastron filled: > 1 opposition obs. blue dots: Jupiter Trojans COMETS solid blue sqr: numbered open blue sqr: others Planetary Sciences
Inner S.S. 2012 ASTEROIDS green dots: “normal” m.p. red dots: < 1.3 AU periastron filled: > 1 opposition obs. blue dots: Jupiter Trojans COMETS solid blue sqr: numbered open blue sqr: others Planetary Sciences
Zoom-in 2009 ASTEROIDS green dots: “normal” m.p. red dots: < 1.3 AU periastron filled: > 1 opposition obs. blue dots: Jupiter Trojans COMETS solid blue sqr: numbered open blue sqr: others Planetary Sciences
Zoom-in 2012 ASTEROIDS green dots: “normal” m.p. red dots: < 1.3 AU periastron filled: > 1 opposition obs. blue dots: Jupiter Trojans COMETS solid blue sqr: numbered open blue sqr: others Planetary Sciences
Outer S.S.2003 KBOs red: classical KBOs white: Plutinos magenta: scattered disk orange tri: Centaurs cyan tri: “unusual” COMETS solid blue sqr: numbered open blue squ: others Planetary Sciences
Outer S.S.2009 KBOs red: classical KBOs white: Plutinos magenta: scattered disk orange tri: Centaurs cyan tri: “unusual” COMETS solid blue sqr: numbered open blue squ: others Planetary Sciences
Outer S.S.2012 KBOs red: classical KBOs white: Plutinos magenta: scattered disk orange tri: Centaurs cyan tri: “unusual” COMETS solid blue sqr: numbered open blue squ: others Planetary Sciences
Outer S.S.2012 Plutinos/TNOs Pluto Quaoar Ixion Varuna Orcus Centaurs/SDOs Chiron Sedna Nessus Asbolus Eris Comets 1P Halley 2P Encke Planetary Sciences
TNOs/SDOs and Friends Hydra Nix Planetary Sciences
The Pluto System: 2012 Hydra Nix Planetary Sciences
The Outer Limits Planetary Sciences
Disk: Protostellar or Debris? Planetary Sciences
Fomalhaut Planet background star movie
Solar System Formation I Planetary Sciences
Clues to Solar System Formation • Internal Motion Clues • Internal Bodies Clues • External Clues Planetary Sciences
Internal Motion Clues to S.S. Formation 1. planetary orbits are roughly circular 2. planets are isolated 3. planetary orbits are roughly coplanar 4. planetary orbits are prograde (all) 5. moons’ orbits are prograde 6. … but not all 7. planetary rotations are prograde 8. … but not all 9. cometary orbits have high a, e, i 10. many moons are tidally locked and/or in resonance PAPER TOPIC: Where is the Oort Cloud anyway? Planetary Sciences
Internal Bodies Clues to S.S. Formation • Sun contains 99.9% of Solar System mass • chondritic meteorites are 4.56 ± 0.01 Gyr old (Pb isotopes) • planet types/compositions depend on location (beware Moon) • planetary atmospheres contain ice fractions dependent on temp • all planets, large moons/asteroids differentiated (were warm) • meteorites have mineralogical differences, rapid heating/cooling • rapid impact cratering widespread, past far more than today’s rate • asteroids old, size distribution implies collisional evol (0.05 Mmoon) • angular momentum resides in giant planets • TNOs and Oort comets old and unevolved • PAPER TOPIC: How does the Kuiper Belt fit into S.S. origin? Planetary Sciences
External Clues to S.S. Formation 21. clouds of gas/dust observed 22. proplyds observed at very young ages --- a few million years 23. T Tauri stars observed 24. substantial disks observed at 10-100 million years 25. no disks seen (yet) past ~ 1 billion years 26. …but, planets and planetary systems now detected PAPER TOPIC: What’s the latest on disk statistics with age? Planetary Sciences
Formation Scenarios • 1. CAPTURE free floaters, planet theft • 2. COLLISION passing star, Sun fragmented • 3. CONDENSATION nebular hypothesis Planetary Sciences