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Ge/Ay133 an the asteroid belt tell us about the early ? 433 Eros Phobo s
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Ge/Ay133

Jan 13, 2016

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What can the asteroid belt tell us about the early S.S.?. 433 Eros. ?. Phobos. Ge/Ay133. These types are not strongly separated, radially. - PowerPoint PPT Presentation
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Page 1: Ge/Ay133

Ge/Ay133

What can the asteroid belt tell us about the early S.S.?

?

433 Eros

Phobos

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These types are not strongly separated, radially.

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See also http://www.ifa.hawaii.edu/~hsieh/mbcs.html

Comets are icy bodies that sublimate and become active when close to the Sun. They are believed to originate in two cold reservoirs beyond the orbit of Neptune: the Kuiper Belt (equilibrium temperatures of ~40 kelvin) and the Oort Cloud (~  10 kelvin). We

present optical data showing the existence of a population of comets originating in a third reservoir: the main asteroid belt. The main-belt comets are unlike the Kuiper Belt and Oort Cloud comets in that they likely formed where they currently reside

and may be collisionally activated. The existence of the main-belt comets lends new support to the idea that main-belt objects could be a major source of terrestrial water.

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Asteroid Itokawa as imaged by the Hayabusa probe.

http://www.isas.jaxa.jp/e/snews/2005/1102.shtml

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Collisions II

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How do we measure rotation states?

•Lightcurves (lots of objects)•Radar measurements (NEOs)•Spacecraft exploration

Toutatis Radar Image

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What do simulations tell us about the asteroid belt?

Jupiter inserted at 10 Myr

Hard to generate observed properties with just Jupiter & planetesimals or single large core, need mixture:

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Radial mixing extends over several 0.1 AU

May help explain the spatial overlap of the various types?

What about the large fraction of bodies that are strongly scattered?

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What determines the water content of the inner S.S.?

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D/H ratios argue that comets did not deliver the bulk of the water…

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Suppose there is an initial snow line… What happens?

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In such a story, the orbital properties of Jupiter are critical…

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What sort of systems emerge?

Hierachical (most mass added in large collisions), so great variety, both in orbital properties…

… and ultimate water content.

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Question for later:What determines whether a planet is “habitable”? How much can the water vary?

What is the maximum eccentricity for which liquid water can be maintained over several AE?