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Vesta in the light of dawn, but without heds?
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Mittlefehldt, D. W. McSween, H. Y. |
| Copyright Year | 2014 |
| Description | The derivation of HEDs from Vesta is strongly supported by Dawn data [1], and these meterorites have made interpretations of Dawn spectra much more rigorous. Compared to the Moon, where samples became available after geologic mapping, the exploration of Vesta has been backwards. But what if HEDs had not been available or identified as vestan samples? What petrologic and geochemical predictions would have been possible using Dawn data, without the benefit of HEDs? |
| File Size | 19379 |
| Page Count | 2 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20140004232 |
| Archival Resource Key | ark:/13960/t3gx99n4v |
| Language | English |
| Publisher Date | 2014-02-03 |
| Access Restriction | Open |
| Subject Keyword | Lunar And Planetary Science And Exploration Geochronology Geological Surveys Vesta Asteroid Meteorites Geochemistry Basalt Regolith Magma Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
