Mineralogical characterization of near-Earth Asteroid (1036) Ganymed

► A mineralogical assessment of near-Earth Asteroid (1036) Ganymed was completed. ► Ganymed is an S(VI) asteroid consisting primarily of orthopyroxene, Fs23(±5)Wo3(±3). ► Ganymed was once part of a mesosiderite containing HED pyroxenes mixed with metal. ► Ganymed is not a parent body of the OCs and...

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Published inIcarus (New York, N.Y. 1962) Vol. 212; no. 1; pp. 149 - 157
Main Authors Fieber-Beyer, Sherry K., Gaffey, Michael J., Abell, Paul A.
Format Journal Article
LanguageEnglish
Published Amsterdam Elsevier Inc 01.03.2011
Elsevier
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Summary:► A mineralogical assessment of near-Earth Asteroid (1036) Ganymed was completed. ► Ganymed is an S(VI) asteroid consisting primarily of orthopyroxene, Fs23(±5)Wo3(±3). ► Ganymed was once part of a mesosiderite containing HED pyroxenes mixed with metal. ► Ganymed is not a parent body of the OCs and is not genetically related to 433 Eros. We present a mineralogical assessment of near-Earth Asteroid, (1036) Ganymed, using data obtained May 18, 2006 UT combined with 24 Color Asteroid Survey data to cover the spectral interval of 0.3–2.45μm. Results of the analysis indicate (1036) Ganymed is an S (VI) asteroid with a surface silicate assemblage consisting primarily of orthopyroxene, (Fs23(±5)Wo3(±3)), consistent with calculated band centers and band area ratios (BAR). (1036) Ganymed appears to be once part of a large mesosiderite containing howardite, eucrite, and diogenite (HED) pyroxenes mixed with metal that was broken apart and dispersed. The calculated composition of the average pyroxenes in the surface material of (1036) Ganymed is consistent with mesosiderite pyroxenes, in particular the diogenites. A second possibility could be (1036) Ganymed is not yet represented in the meteorite collection. Our investigation has confirmed Ganymed is not a parent body of the ordinary chondrites and is not genetically related to (433) Eros.
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ISSN:0019-1035
1090-2643
DOI:10.1016/j.icarus.2010.12.013