Asteroid Surface Processes
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Our group is currently interested in
the formational conditions of meteorites, especially chondritic meteorites.
Since nearly all meteorites are believed to be fragments of asteroids that
were sent toward earth after a collision, it is necessary to consider what
chemical and physical processes could be occurring on asteroids. The recent imaging of asteroids (Sears, 2015) along with theoretical
calculations suggest that substantial regoliths
(loosely consolidated surface material) up to a few km deep may exist on many
asteroids. If asteroids were originally volatile rich (e.g. H20)
degassing through radiometric and impact heating would have created a
"dynamic" regolith.
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We
suspect that when gases are evolved from a volatile rich CI-like interior
pass through the regolith of a 10-100 km parent body, chondrule and metal
size-sorting results in surface materials with ordinary chondrite-like
properties. Thermal heating of the body could mobilize the entrapped water
and create a "fluidized bed". This process could account for
particle size-sorting, redox properties of chondrites, oxygen isotopic
characteristics, thermal trends, and chondrule formation. |
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Click here for publications on
this research
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