Evidence for K-rich terranes on Vesta from impact spherules

The howardite-eucrite-diogenite (HED) clan is a group of meteorites that probably originate from the asteroid Vesta. Some of them are complex breccias that contain impact glasses whose compositions mirror that of their source regions. Some K-rich impact glasses (up to 2 wt% K2O) suggest that in addition to basalts and ultramafic cumulates, K-rich rocks are exposed on Vesta's surface. One K-rich glass (up to 6 wt% K2O), with a felsic composition, provides the first evidence of highly differentiated K-rich rocks on a large asteroid. They can be compared to the rare lunar granites and suggest that magmas generated in a large asteroid are more diverse than previously thought.


Published in:
Meteoritics & Planetary Science, 44, 359-374
Year:
2009
Keywords:
Laboratories:




 Record created 2011-09-29, last modified 2018-09-13


Rate this document:

Rate this document:
1
2
3
 
(Not yet reviewed)