Tracing the oxygen isotope composition of the upper Earth’s atmosphere using cosmic spherules
Andreas Pack (),
Andres Höweling,
Dominik C. Hezel,
Maren T. Stefanak,
Anne-Katrin Beck,
Stefan T. M. Peters,
Sukanya Sengupta,
Daniel Herwartz and
Luigi Folco
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Andreas Pack: Universität Göttingen, Geowissenschaftliches Zentrum
Andres Höweling: Universität Göttingen, Geowissenschaftliches Zentrum
Dominik C. Hezel: Universität Köln, Institut für Geologie und Mineralogie
Maren T. Stefanak: Universität Göttingen, Geowissenschaftliches Zentrum
Anne-Katrin Beck: Universität Göttingen, Geowissenschaftliches Zentrum
Stefan T. M. Peters: Universität Göttingen, Geowissenschaftliches Zentrum
Sukanya Sengupta: Universität Göttingen, Geowissenschaftliches Zentrum
Daniel Herwartz: Universität Köln, Institut für Geologie und Mineralogie
Luigi Folco: Universitá di Pisa
Nature Communications, 2017, vol. 8, issue 1, 1-7
Abstract:
Abstract Molten I-type cosmic spherules formed by heating, oxidation and melting of extraterrestrial Fe,Ni metal alloys. The entire oxygen in these spherules sources from the atmosphere. Therefore, I-type cosmic spherules are suitable tracers for the isotopic composition of the upper atmosphere at altitudes between 80 and 115 km. Here we present data on I-type cosmic spherules collected in Antarctica. Their composition is compared with the composition of tropospheric O2. Our data suggest that the Earth's atmospheric O2 is isotopically homogenous up to the thermosphere. This makes fossil I-type micrometeorites ideal proxies for ancient atmospheric CO2 levels.
Date: 2017
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Persistent link: https://EconPapers.repec.org/RePEc:nat:natcom:v:8:y:2017:i:1:d:10.1038_ncomms15702
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DOI: 10.1038/ncomms15702
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