Modal mineralogy of the surface of Vesta: Evidence for ubiquitous olivine and identification of meteorite analogue
• Modal mineralogy of the surface of Vesta is derived from modeling VIR/Dawn spectra. • Coarse-grained olivine is likely ubiquitous in all major units of Vesta. • The olivine modeled abundance ranges is 10–20%±10%. • Terrains with strongest LCP signatures are well representative of diogenites. • How...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Poulet, F. [verfasserIn] |
|---|
| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Schlagwörter: |
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| Umfang: |
14 |
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| Übergeordnetes Werk: |
Enthalten in: Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users - Mathew, Rajeev ELSEVIER, 2018, international journal of solar system studies, Orlando, Fla |
|---|---|
| Übergeordnetes Werk: |
volume:253 ; year:2015 ; pages:364-377 ; extent:14 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.icarus.2014.06.002 |
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| 520 | |a • Modal mineralogy of the surface of Vesta is derived from modeling VIR/Dawn spectra. • Coarse-grained olivine is likely ubiquitous in all major units of Vesta. • The olivine modeled abundance ranges is 10–20%±10%. • Terrains with strongest LCP signatures are well representative of diogenites. • Howardites containing olivine-bearing melt are good petrologic analogues of Vesta. | ||
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Modal mineralogy of the surface of Vesta: Evidence for ubiquitous olivine and identification of meteorite analogue |
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• Modal mineralogy of the surface of Vesta is derived from modeling VIR/Dawn spectra. • Coarse-grained olivine is likely ubiquitous in all major units of Vesta. • The olivine modeled abundance ranges is 10–20%±10%. • Terrains with strongest LCP signatures are well representative of diogenites. • Howardites containing olivine-bearing melt are good petrologic analogues of Vesta. |
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• Modal mineralogy of the surface of Vesta is derived from modeling VIR/Dawn spectra. • Coarse-grained olivine is likely ubiquitous in all major units of Vesta. • The olivine modeled abundance ranges is 10–20%±10%. • Terrains with strongest LCP signatures are well representative of diogenites. • Howardites containing olivine-bearing melt are good petrologic analogues of Vesta. |
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• Modal mineralogy of the surface of Vesta is derived from modeling VIR/Dawn spectra. • Coarse-grained olivine is likely ubiquitous in all major units of Vesta. • The olivine modeled abundance ranges is 10–20%±10%. • Terrains with strongest LCP signatures are well representative of diogenites. • Howardites containing olivine-bearing melt are good petrologic analogues of Vesta. |
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