Challenges in detecting olivine on the surface of 4 Vesta-Reference-Cited by-同舟云学术

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Challenges in detecting olivine on the surface of 4 Vesta

Published:2013-07-30 Issue:11 Volume:48 Page:2155-2165
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Beck Andrew W.¹,McCoy Timothy J.¹,Sunshine Jessica M.²,Viviano Christina E.³,Corrigan Catherine M.¹,Hiroi Takahiro⁴,Mayne Rhiannon G.⁵

Affiliation:

1. Department of Mineral Sciences; Smithsonian Institution; Washington District of Columbia 20560-0112 USA

2. Department of Astronomy; University of Maryland; College Park Maryland 20742-2421 USA

3. Johns Hopkins University Applied Physics Laboratory; Laurel Maryland 20723 USA

4. Department of Geological Sciences; Brown University; Providence Rhode Island 02912 USA

5. Department of Geology; Texas Christian University; Fort Worth Texas 76129 USA

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.12160/fullpdf

Reference36 articles.

1. Visible and near-infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the solar system;Adams;Journal of Geophysical Research,1974

2. Geochemistry of diogenites; still more diversity in their parental melts;Barrat;Meteoritics & Planetary Science,2008

3. Diogenites as polymict breccias composed of harzburgite and orthopyroxenite;Beck;Meteoritics & Planetary Science,2010

4. MIL 03443, a Dunite from asteroid 4 Vesta: Evidence for its classification and cumulate origin;Beck;Meteoritics & Planetary Science,2011

5. NIR spectral trends of HED meteorites: Can we discriminate between the magmatic evolution, mechanical mixing and observation geometry effects?;Beck;Icarus,2011

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