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[会议论文] 作者:L.A.MCFADDEN,H.Y.MCSWEEN,E.PALOMBA,C.M.PIETERS,C.A.POLANSKEY,C.A.RAYMOND,J.M.SUNSHINE,M.C.DE SANCTIS,F.TOSI,F.ZAMBON, 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.PALOMBA[1]C.M.PIETERS[6]C.A.POLANSKEY[7]C.A.RAYMOND[7]J.M.SUNSHINE[8]M.C.DESANCTIS[1]F.TOSI[1]F.ZAMBON, 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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