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Evolution of Occator Crater on (1) Ceres 

Nathues, A.; Platz, T.; Thangjam, G.; Hoffmann, M.; Mengel, K.; Cloutis, E. A.; Le Corre, L.; Reddy, V.; Kallisch, J.; D. A. Crown, D. A. (The Astronomical Journal, 2017-02-17)
The dwarf planet Ceres (diameter 939 km) is the largest object in the main asteroid belt. Recent investigations suggest that Ceres is a thermally evolved, volatile-rich body with potential geological activity, a body which ...
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Oxo Crater on (1) Ceres: Geological History and the Role of Water-ice 

Nathues, A.; Platz, T.; Hoffmann, M.; Thangjam, G.; Cloutis, E. A.; Applin, D. M.; Le Corre, L.; Reddy, V.; Mengel, K.; Protopapa, S.; Takir, D.; Preusker, F.; Schmidt, B. E.; Russell, C. T. (The Astronomical Journal, 2017-08-04)
Dwarf planet Ceres (∅ ∼ 940 km) is the largest object in the main asteroid belt. Investigations suggest that Ceres is a thermally evolved, volatile-rich body with potential geological activity, a body that was never ...
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Detection of rotational spectral variation on the M-type asteroid (16) Psyche 

Sanchez, Juan A.; Reddy, Vishnu; Shepard, Michael K.; Thomas, Cristina; Cloutis, Edward A.; Takir, Driss; Conrad, Albert; Kiddell, Cain; Applin, Daniel (The Astronomical Journal, 2016-12-28)
The asteroid (16) Psyche is of scientific interest because it contains ∼1% of the total mass of the asteroid belt and is thought to be the remnant metallic core of a protoplanet. Radar observations have indicated the ...

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AuthorCloutis, E. A. (2)Hoffmann, M. (2)Le Corre, L. (2)Mengel, K. (2)Nathues, A. (2)Platz, T. (2)Reddy, V. (2)Thangjam, G. (2)Applin, D. M. (1)Applin, Daniel (1)... View MoreSubject
minor planets (3)
asteroids: general (2)asteroids: general – techniques: spectroscopic (1)... View MoreDate Issued2017 (2)2016 (1)Has File(s)Yes (3)

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