A spectroscopic comparison of HED meteorites and V-type asteroids in the inner Main Belt

V-type asteroids in the inner Main Belt ( a < 2.5 AU) and the HED meteorites are thought to be genetically related to one another as collisional fragments from the surface of the large basaltic Asteroid 4 Vesta. We investigate this relationship by comparing the near-infrared (0.7–2.5 μm) spectra...

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Veröffentlicht in:	Icarus (New York, N.Y. 1962) N.Y. 1962), 2010-08, Vol.208 (2), p.773-788
Hauptverfasser:	Moskovitz, Nicholas A., Willman, Mark, Burbine, Thomas H., Binzel, Richard P., Bus, Schelte J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Asteroid Vesta Asteroids Asteroids, Composition Astronomy Earth, ocean, space Exact sciences and technology Meteorites Solar system Spectroscopy
Online-Zugang:	Volltext
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