TY - JOUR
T1 - Shergottite Northwest Africa 6963
T2 - A Pyroxene-Cumulate Martian Gabbro
AU - Filiberto, Justin
AU - Gross, Juliane
AU - Udry, Arya
AU - Trela, Jarek
AU - Wittmann, Axel
AU - Cannon, Kevin M.
AU - Penniston-Dorland, Sarah
AU - Ash, Richard
AU - Hamilton, Victoria E.
AU - Meado, Andrea L.
AU - Carpenter, Paul
AU - Jolliff, Brad
AU - Ferré, Eric C.
N1 - Funding Information:
Data supporting the entire paper are available in Tables 1–7, supporting information tables, and through the RELAB database: http://www.planetary. brown.edu/relabdocs/relab_disclaimer. htm. Samples are available upon request from the corresponding author. J. F. and J. G. acknowledge partial support from NASA Mars Fundamental Research award #NNX13AG35G. The authors would like to thank Takahiro Hiroi for the RELAB measurements and Brian Balta for helpful comments on this version and a previous version of this manuscript, as well as an anonymous reviewer of this manuscript. LPI Contribution #2102.
Funding Information:
Data supporting the entire paper are available in Tables 1–7, supporting information tables, and through the RELAB database: http://www.planetary.brown.edu/relabdocs/relab_disclaimer.htm. Samples are available upon request from the corresponding author. J. F. and J. G. acknowledge partial support from NASA Mars Fundamental Research award #NNX13AG35G. The authors would like to thank Takahiro Hiroi for the RELAB measurements and Brian Balta for helpful comments on this version and a previous version of this manuscript, as well as an anonymous reviewer of this manuscript. LPI Contribution #2102.
Publisher Copyright:
©2018. American Geophysical Union. All Rights Reserved.
PY - 2018/7
Y1 - 2018/7
N2 - Northwest Africa (NWA) 6963 was found in Guelmim-Es-Semara, Morocco, and based on its bulk chemistry and oxygen isotopes, it was classified as a Martian meteorite. On the basis of a preliminary study of the textures and crystal sizes, it was resubclassified as a gabbroic shergottite because of the similarity with terrestrial and lunar gabbros. However, the previous work was not a quantitative investigation of NWA 6963; to supplement the original resubclassification and enable full comparison between this and other Martian samples; here we investigate the mineralogy, petrology, geochemistry, quantitative textural analyses, and spectral properties of gabbroic shergottite NWA 6963 to constrain its petrogenesis, including the depth of emplacement (i.e., base of a flow versus crustal intrusion). NWA 6963 is an enriched shergottite with similar mineralogy to the basaltic shergottites but importantly does not contain any fine-grained mesostasis. Consistent with the mineralogy, the reflectance (visible/near-infrared and thermal infrared) spectrum of powdered NWA 6963 is similar to other shergottites because they are all dominated by pyroxene, but its reflectance is distinct in terms of albedo and spectral contrast due to its gabbroic texture. NWA 6963 represents a partial cumulate gabbro that is associated with the basaltic shergottites. Therefore, NWA 6963 could represent a hypabyssal intrusive feeder dike system for the basaltic shergottites that erupted on the surface.
AB - Northwest Africa (NWA) 6963 was found in Guelmim-Es-Semara, Morocco, and based on its bulk chemistry and oxygen isotopes, it was classified as a Martian meteorite. On the basis of a preliminary study of the textures and crystal sizes, it was resubclassified as a gabbroic shergottite because of the similarity with terrestrial and lunar gabbros. However, the previous work was not a quantitative investigation of NWA 6963; to supplement the original resubclassification and enable full comparison between this and other Martian samples; here we investigate the mineralogy, petrology, geochemistry, quantitative textural analyses, and spectral properties of gabbroic shergottite NWA 6963 to constrain its petrogenesis, including the depth of emplacement (i.e., base of a flow versus crustal intrusion). NWA 6963 is an enriched shergottite with similar mineralogy to the basaltic shergottites but importantly does not contain any fine-grained mesostasis. Consistent with the mineralogy, the reflectance (visible/near-infrared and thermal infrared) spectrum of powdered NWA 6963 is similar to other shergottites because they are all dominated by pyroxene, but its reflectance is distinct in terms of albedo and spectral contrast due to its gabbroic texture. NWA 6963 represents a partial cumulate gabbro that is associated with the basaltic shergottites. Therefore, NWA 6963 could represent a hypabyssal intrusive feeder dike system for the basaltic shergottites that erupted on the surface.
KW - Geochemistry
KW - Martian meteorite
KW - NWA6963
KW - Petrology
KW - Spectroscopy
KW - shergottite
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U2 - 10.1029/2018JE005635
DO - 10.1029/2018JE005635
M3 - Article
AN - SCOPUS:85049850757
SN - 2169-9097
VL - 123
SP - 1823
EP - 1841
JO - Journal of Geophysical Research: Planets
JF - Journal of Geophysical Research: Planets
IS - 7
ER -