Convective activity in a Martian magma chamber recorded by P‐zoning in Tissint olivine. (7th May 2020)

• Record Type: Journal Article
• Authors: Mari, N.; Hallis, L. J.; Daly, L.; Lee, M. R.
• Is Part Of: Meteoritics & planetary science. Volume 55:Number 5(2020)
• Page Start: 1057
• Page End: 1072
• Publication Date: 2020-05-07
• Subjects: Meteorites -- Periodicals; Planetology -- Periodicals; 523.4
• DOI: 10.1111/maps.13488
• Languages: English
• ISSNs: 1086-9379

Abstract

Abstract: The Tissint Martian meteorite is an unusual depleted olivine‐phyric shergottite, reportedly sourced from a mantle‐derived melt within a deep magma chamber. Here, we report major and trace element data for Tissint olivine and pyroxene, and use these data to provide new insights into the dynamics of the Tissint magma chamber. The presence of irregularly spaced oscillatory phosphorous (P)‐rich bands in olivine, along with geochemical evidence indicative of a closed magmatic system, implies that the olivine grains were subject to solute trapping caused by vigorous crystal convection within the Tissint magma chamber. Calculated equilibration temperatures for the earliest crystallizing (antecrystic) olivine cores suggest a Tissint magma source temperature of 1680 °C, and a local Martian mantle temperature of 1560 °C during the late Amazonian—the latter being consistent with the ambient mantle temperature of Archean Earth.