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 o...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
Elsevier
2012
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| Online Access: | http://hdl.handle.net/1721.1/73477 |