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Published March 2013 | Published
Journal Article Open

The Ksar Ghilane 002 shergottite-The 100th registered Martian meteorite fragment

Abstract

We report on the discovery of a new shergottite from Tunisia, Ksar Ghilane (KG) 002. This single stone, weighing 538 g, is a coarse-grained basaltic shergottite, mainly composed of maskelynitized plagioclase (approximately 52 vol%) and pyroxene (approximately 37 vol%). It also contains Fe-rich olivine (approximately 4.5 vol%), large Ca-phosphates, including both merrillites and Cl-apatites (approximately 3.4 vol%), minor amounts of silica or SiO_2-normative K-rich glass, pyrrhotite, Ti-magnetite, ilmenite, and accessory baddeleyite. The largest crystals of pyroxene and plagioclase reach sizes of approximately 4 to 5 mm. Pyroxenes (Fs_(26–96)En_(5–50)Wo_(2–41)). They typically range from cores of about Fs_(29)En_(41)Wo_(30) to rims of about Fs_(68)En_(14)Wo_(17). Maskelynite is Ab_(41–49)An_(39–58)Or_(1–7) in composition, but some can be as anorthitic as An_(93). Olivine (Fa_(91–96)) occurs mainly within symplectitic intergrowths, in paragenesis with ilmenite, or at neighboring areas of symplectites. KG 002 is heavily shocked (S5) as indicated by mosaic extinction of pyroxenes, maskelynitized plagioclase, the occurrence of localized shock melt glass pockets, and low radiogenic He concentration. Oxygen isotopes confirm that it is a normal member of the SNC suite. KG 002 is slightly depleted in LREE and shows a positive Eu anomaly, providing evidence for complex magma genesis and mantle processes on Mars. Noble gases with a composition thought to be characteristic for Martian interior is a dominant component. Measurements of ^(10)Be, ^(26)Al, and ^(53)Mn and comparison with Monte Carlo calculations of production rates indicate that KG 002 has been exposed to cosmic rays most likely as a single meteoroid body of 35–65 cm radius. KG 002 strongly resembles Los Angeles and NWA 2800 basaltic shergottites in element composition, petrography, and mineral chemistry, suggesting a possible launch-pairing. The similar CRE ages of KG 002 and Los Angeles may suggest an ejection event at approximately 3.0 Ma.

Additional Information

© 2013 The Meteoritical Society. Received 28 December 2011; revision accepted 01 January 2013. J. L. is grateful to ICREA Academia program. We thank U. Heitmann (Münster) for sample preparation. The DREAMS accelerator team, in particular S. Akhmadaliev, is gratefully thanked for helping with ^(10)Be and ^(26)Al measurements, and T. Faestermann and G. Korschinek for ^(53)Mn and ^(60)Fe measurements at Munich.

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Created:
August 19, 2023
Modified:
October 25, 2023