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Color and albedo heterogeneity of Vesta from Dawn
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  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
Institution:Max Planck Institute for Solar System Research, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany. reddy@mps.mpg.de
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.
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