To be or not to be oxidized: A case study of olivine behavior in the fusion crust of ureilite A 09368 and H chondrites A 09004 and A 09502-Reference-Cited by-同舟云学术

To be or not to be oxidized: A case study of olivine behavior in the fusion crust of ureilite A 09368 and H chondrites A 09004 and A 09502

Published:2019-03-28 Issue:7 Volume:54 Page:1563-1578
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Pittarello Lidia¹^ORCID,Yamaguchi Akira²³^ORCID,Roszjar Julia⁴,Debaille Vinciane⁵,Koeberl Christian¹⁴^ORCID,Claeys Philippe⁶^ORCID

Affiliation:

1. Department of Lithospheric Research University of Vienna Althanstraße 14 A‐1090 Vienna Austria

2. National Institute of Polar Research 10‐3 Midori‐cho Tachikawa Tokyo 190‐8518 Japan

3. Department of Polar Science School of Multidisciplinary Science SOKENDAI (The Graduate University for Advanced Studies) Tokyo 190‐8518 Japan

4. Natural History Museum Vienna Burgring 7 A‐1010 Vienna Austria

5. Laboratoire G‐Time (Géochimie: Traçage isotopique, minéralogique et élémentaire) Université Libre de Bruxelles Av. F.D. Roosevelt 50 1050 Brussels Belgium

6. Analytical, Environmental and Geo‐Chemistry (AMGC) Vrije Universiteit Brussel Pleinlaan 2 B‐1050 Brussels Belgium

Funder

Fonds De La Recherche Scientifique - FNRS

Fonds Wetenschappelijk Onderzoek

Austrian Science Fund

Society for Ambulatory Anesthesia

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13284

Reference43 articles.

1. BauerJ. F.1979.Experimental shock metamorphism of mono‐and polycrystalline olivine: A comparative study. Proceedings of the 10th Lunar and Planetary Science Conference pp.2573–2596.

2. Mineralogical alteration of artificial meteorites during atmospheric entry. The STONE-5 experiment

3. An experimental investigation of olivine morphology

4. Fusion crust of iron meteorites and mesosiderites and production of cosmic spherules;El Goresy A.;Smithsonian Contributions to Astrophysics,1967

5. Isotopic compositions of oxygen, iron, chromium, and nickel in cosmic spherules: Toward a better comprehension of atmospheric entry heating effects

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