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Chemical and genetic characterization of the ungrouped pallasite Lieksa
Authors:Emily M Chiappe  Richard D Ash  Arto Luttinen  Sari Lukkari  Jukka Kuva  Connor D Hilton  Richard J Walker
Institution:1. Department of Geology, University of Maryland, College Park, Maryland, USA;2. Finnish Museum of Natural History, University of Helsinki, Helsinki, Finland;3. Geological Survey of Finland, Espoo, Finland;4. Pacific Northwest National Laboratory, Richland, Washington, USA
Abstract:The meteorite Lieksa was found in 2017 in Löpönvaara, Finland, and later donated to the Finnish Museum of Natural History. Here, we report siderophile element concentrations, genetic isotopic data, and a metal–silicate segregation age for the meteorite. The ~280 g Lieksa is ~80% metal and ~20% silicate and oxide inclusions by volume, with the inclusions consisting primarily of Fe-rich olivine. Due to Lieksa's silicate content, coupled with a texture characterized by metal enclosing the silicates, it has been classified as a pallasite. Lieksa's olivine and bulk chemical characteristics are distinct from those of the known pallasite and iron meteorite groups, consistent with its classification as ungrouped. The meteorite exhibits a flat, chondrite-normalized highly siderophile element pattern, consistent with an origin as an early crystallization product from a metallic melt with chondritic relative abundances. Molybdenum, Ru, and 183W isotopic data indicate that Lieksa formed in the non-carbonaceous (NC) domain of the solar nebula. Radiogenic 182W abundances for Lieksa yield a model metal–silicate segregation age of 1.5 ± 0.8 Myr after calcium-aluminum-rich inclusion formation, which is within the range established for other NC-type pallasite and iron meteorite parent bodies.
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