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[会议论文] 作者:E.AMMANNITO,G.MAGNI,S.MARCHI,T.B.MCCORD,L.A.MCFADDEN,H.Y.MCSWEEN,E.PALOMBA,C.M.PIETERS,C.A.POLANSKEY,, 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:E.AMMANNITO[1]G.MAGNI[1]S.MARCHI[2]T.B.MCCORD[3]L.A.MCFADDEN[4]H.Y.MCSWEEN[5]E.PALOMBA[1]C.M.PIETERS[, 来源:International Symposium & Summer School on Planetary Sci 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 feature...
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