Space history of the High Possil and Strathmore meteorites from Ne and Ar isotopes

Author:

Carracedo A.1ORCID,Stuart F.M.1,Di Nicola L.1,Faithfull J.W.2

Affiliation:

1. Scottish Universities Environmental Research Centre, Rankine Avenue, East Kilbride G75 0QF, UK

2. Hunterian Museum & Art Gallery, University of Glasgow, 82 Hillhead Street, Glasgow G12 8QQ, UK

Abstract

The High Possil and Strathmore L6 chondrites fell in Scotland in 1804 and 1917 respectively. Unravelling their cosmic-ray exposure (CRE) ages provides crucial information about when they were ejected from the parent body, how they were delivered to Earth and is ultimately important for understanding the dynamics of small bodies in the solar system. Here we use new measurements of the Ne and Ar isotopic composition to determine CRE ages of both meteorites. Duplicated cosmogenic 21 Ne and 38 Ar concentrations yield CRE ages of 44.6 ± 4.6 Ma for High Possil and 15.4 ± 1.3 Ma for Strathmore. These coincide with well-established peaks in the ejection record for the L6 chondrites. They yield 40 Ar gas retention ages in excess of 3.15 Ga, which is consistent with both meteorites originating at depth within the parent body at the time of asteroidal break-up. Thematic collection: This article is part of the Early Career Research collection available at: https://www.lyellcollection.org/cc/SJG-early-career-research

Funder

Natural Environment Research Council

Publisher

Geological Society of London

Subject

Geology

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