Regolith and Megaregolith Formation of H-Chondrites: Thermal Constraints on the Parent Body
Spectral reflectivity data and its location near an orbital resonance suggest that Asteroid 6 Hebe may be the source body for H-chondrites, the second largest meteorite group. Recent spacecraft images of asteroids and theoretical modeling indicate that, contrary to previous ideas, asteroids can reta...
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| Published in: | Icarus (New York, N.Y. 1962) Vol. 132; no. 1; pp. 185 - 195 |
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| Main Authors: | , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
Elsevier Inc
01-03-1998
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| Online Access: | Get full text |
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