Color and albedo heterogeneity of Vesta from Dawn

2012-05-11 | journal article

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​Color and albedo heterogeneity of Vesta from Dawn​
Reddy, V.; Nathues, A.; Le Corre, L.; Sierks, H.; Li, J.-Y.; Gaskell, R. & McCoy, T. et al.​ (2012) 
Science336(6082) pp. 700​-704​.​ DOI: https://doi.org/10.1126/science.1219088 

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Authors
Reddy, Vishnu; Nathues, Andreas; Le Corre, Lucille; Sierks, Holger; Li, Jian-Yang; Gaskell, Robert; McCoy, Timothy; Beck, Andrew W; Schröder, Stefan E; Pieters, Carle M; Becker, Kris J; Buratti, Bonnie J; Denevi, Brett; Blewett, David T; Christensen, Ulrich R.; Gaffey, Michael J; Gutierrez-Marques, Pablo; Hicks, Michael; Keller, Horst Uwe; Maue, Thorsten; Mottola, Stefano; McFadden, Lucy A; McSween, Harry Y; Mittlefehldt, David; O'Brien, David P; Raymond, Carol; Russell, Christopher
Abstract
Multispectral images (0.44 to 0.98 μm) of asteroid (4) Vesta obtained by the Dawn Framing Cameras reveal global color variations that uncover and help understand the north-south hemispherical dichotomy. The signature of deep lithologies excavated during the formation of the Rheasilvia basin on the south pole has been preserved on the surface. Color variations (band depth, spectral slope, and eucrite-diogenite abundance) clearly correlate with distinct compositional units. Vesta displays the greatest variation of geometric albedo (0.10 to 0.67) of any asteroid yet observed. Four distinct color units are recognized that chronicle processes--including impact excavation, mass wasting, and space weathering--that shaped the asteroid's surface. Vesta's color and photometric diversity are indicative of its status as a preserved, differentiated protoplanet.
Issue Date
11-May-2012
Journal
Science 
ISSN
0036-8075; 1095-9203
eISSN
1095-9203
Language
English

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