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[会议论文] 作者：,C.A.POLANSKEY,C.A.RAYMOND,J.M.SUNSHINE,M.C.DE SANCTIS,F.TOSI,F.ZAMBON,C.T.RUSSELL,E CAPACCIONI,M.T.CAPRIA,
来源：International Symposium & Summer School on Planetary Science 年份：2013
4 Vesta is known to have a surface of basaltic material through visible/near-infrared reflectance spectroscopy.Vestas spectrum has strong absorption features centered near 0.9 and 1.9 μm, indicative o...
[会议论文] 作者：M.T.Capria,H.U.Keller,T.McCord,L.McFadden,H.McSween,S.Mottola,A.Nathues,G.Neukum,C.Pieters,T.Prettyman,
来源：International Symposium & Summer School on Planetary Science 年份：2013
The NASA mission Dawn was launched on September 27, 2007 and reached Vesta on July 16, 2011.Dawn orbited Vesta until September 2012, and then departed for Ceres, where it will arrive in early 2015.Ves...
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