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      Detection of serpentine in exogenic carbonaceous chondrite material on Vesta from Dawn FC data

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          Bidirectional reflectance spectroscopy: 1. Theory

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            Optical properties of carbonaceous chondrites and their relationship to asteroids

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              Elemental mapping by Dawn reveals exogenic H in Vesta's regolith.

              Using Dawn's Gamma Ray and Neutron Detector, we tested models of Vesta's evolution based on studies of howardite, eucrite, and diogenite (HED) meteorites. Global Fe/O and Fe/Si ratios are consistent with HED compositions. Neutron measurements confirm that a thick, diogenitic lower crust is exposed in the Rheasilvia basin, which is consistent with global magmatic differentiation. Vesta's regolith contains substantial amounts of hydrogen. The highest hydrogen concentrations coincide with older, low-albedo regions near the equator, where water ice is unstable. The young, Rheasilvia basin contains the lowest concentrations. These observations are consistent with gradual accumulation of hydrogen by infall of carbonaceous chondrites--observed as clasts in some howardites--and subsequent removal or burial of this material by large impacts.
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                Author and article information

                Journal
                Icarus
                Icarus
                Elsevier BV
                00191035
                September 2014
                September 2014
                : 239
                :
                : 222-237
                Article
                10.1016/j.icarus.2014.06.003
                3c3f83fe-2ddb-4b66-9329-99c00b59ddb8
                © 2014
                History

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