dynamics_lecture

dynamics_lecture - Etc. etc. etc. N Plutinos 3:2 2:1 N ros...

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Unformatted text preview: Etc. etc. etc. N Plutinos 3:2 2:1 N ros ne c eptu sing scattered KBOs classical KBOs N S J U N P Pluto Uranus Neptune Saturn Jupiter Asteroid belt Mars Earth Venus Mercury Pluto Earth Saturn Jupiter Asteroid belt Venus Mercury Mars Uranus Neptune ? Kuiper belt Pluto Earth Saturn Jupiter Asteroid belt Venus Mercury Mars Uranus Neptune ? S J U N P Pluto Quaoar Neptune Uranus J S # discovered KBOs Pluto Quaoar Neptune Uranus J S number 0 50 100 heliocentric distance number r-3/2 0 50 100 heliocentric distance number r-11 0 50 100 heliocentric distance Kuiper belt Pluto Earth Saturn Jupiter Asteroid belt Venus Mercury Mars Uranus Neptune ? Pluto Uranus Neptune inne Saturn Jupiter r Asteroid belt Mars Earth Venus Mercury The edge of the solar system Kuiper belt > 20,000 – 100,000 AU ? S J U N P a=480 AU e=0.85 i=12 q=76 AU Q=900 AU P=10,500 yr Where did it come from? -in situ formation -scattered by modest-sized planet @ ~70AU -close stellar encounter Where did it come from? -in situ -scattered by modest-sized planet @ ~70AU -close stellar encounter Where did it come from? -in situ -scattered by modest-sized planet @ ~70AU -close stellar encounter -dense stellar birth environment 26 Al → Mg t h = 0.7 Myr 26 ( 26 Al / 27 Al) = (5.1 ± 0.6) x 10-5 ...
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This note was uploaded on 01/03/2012 for the course GEL 133 taught by Professor List during the Fall '10 term at Caltech.

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dynamics_lecture - Etc. etc. etc. N Plutinos 3:2 2:1 N ros...

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