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Small Body Evolution and Planetary Differentiation 2
Tuesday, July 30, 2024, 1:30 PM
King Baudouin Room
Chairs:
Hayley Lowe
Shiyong Liao
Shiyong Liao
1:30 PM
Takir D.*
Emery J. P.
Bottke W. F.
Arredondo A.
Origin Of Asteroid (101955) Bennu and Its Connection to the New Polana Family
[#6231]
We investigate the origin of the asteroid (101955) Bennu and its spectral connection to the New Polana family.
We investigate the origin of the asteroid (101955) Bennu and its spectral connection to the New Polana family.
1:45 PM
Nuth J. A.*
Ferguson F. T.
Johnson N. M.
Where Do Comets Go When Their Regoliths Become Desiccated?
[#6421]
Comets are active for ~1000 perihelion passages: Their orbits are stable for much longer. There must be many more inactive comets than active comets. We argue that C-complex asteroids are extinct comets and carbonaceous meteorites are comet samples.
Comets are active for ~1000 perihelion passages: Their orbits are stable for much longer. There must be many more inactive comets than active comets. We argue that C-complex asteroids are extinct comets and carbonaceous meteorites are comet samples.
2:00 PM
Ogliore R. C.*
Bolton S. J.
Hofmann A. E.
Burchell M. J.
Canup R. M.
et al.
Io's Record of Planet Formation in the Outer Solar System
[#6315]
We present a sample-return mission concept to Jupiter's volcanic moon, Io.
We present a sample-return mission concept to Jupiter's volcanic moon, Io.
*presenter
