The Open UniversitySkip to content
 

Igneous Differentiation of the Martian Crust

Bridges, J.C.; Hicks, L.J.; Bedford, C.; Schwenzer, S.P.; MacArthur, J. and Edwards, P.H. (2017). Igneous Differentiation of the Martian Crust. In: 1st British Planetary Science Congress, 3-5 Dec 2017, Glasgow.

Google Scholar: Look up in Google Scholar

Abstract

Our understanding about the differentiation of the Mars crust is increasing rapidly as a result of the combination of 129 distinct SNC meteorites, lander and orbiter data. Recent debates have centred on the existence of alkaline versus tholeiitic and silicic magmatism, crystal fractionation versus partial melting controls on melt composition, and the oxidation state of mantle source regions. Recently we have used MSL ChemCam data to show the presence of trachybasalt float rocks, of tholeiitic affinity, in Gale Crater [1]. Other igneous components recorded in Gale sediments suggest the presence of alkaline and silica oversaturated magmatism as well [2,3,4]. When we compare martian datasets, it is apparent that a key primary melt composition in the ancient highlands is basalt with SiO2 45 wt%, Na2O + K2O 3.5 wt%, and high Fe, low Al. Crystal fractionation from this has led to trachybasalt and possibly in extreme cases to rhyolites [4]. The juxtaposition with some likely alkaline source regions is analogous to intraplate magmatism on Earth. Although one martian meteorite (a regolith breccia) shows clasts of alkaline affinity [5,6], the 112 shergottites are silica saturated. We classify them on the basis of their REE abundances, reflecting mantle source compositions rather than crustal contamination [7]. Bulk compositions indicate that their source regions – probably under Tharsis and the Northern Lowlands - were alkali-poor compared to the Ancient Highlands’ basalts. Limited evidence for crystal fractionation has been identified. Here we present the results of new work comparing shergottites, Gale, MER and terrestrial analogue igneous rocks to determine the key controls on martian magmatism.

[1] Edwards P.H. et al. (2017) MAPS. DOI: 10.1111/maps.1295. [2] Bedford C. et al. GCA (in rev.). [3] Treiman et al. (2016) doi: 10.1002/2015JE004932. [4] Morris et al. (2016) doi: 10.1073/pnas.1607098113. [5] Santos A. et al. (2015) doi.org/10.1016/j.gca.2015.02.02. [6] MacArthur J. et al. (2017) MetSoc. #6108. [7] Bridges J.C. and Warren P.H. (2006) doi:10.1144/0016-764904-501.

Item Type: Conference or Workshop Item
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Environment, Earth and Ecosystem Sciences
Related URLs:
Item ID: 52920
Depositing User: Candice Bedford
Date Deposited: 19 Jan 2018 15:14
Last Modified: 07 Dec 2018 11:01
URI: http://oro.open.ac.uk/id/eprint/52920
Share this page:

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU