Evidence for the presence of chondrule‐ and CAI‐derived material in an isotopically anomalous Antarctic micrometeorite-Reference-Cited by-同舟云学术

Evidence for the presence of chondrule‐ and CAI‐derived material in an isotopically anomalous Antarctic micrometeorite

Published:2020-11-24 Issue:12 Volume:55 Page:2703-2726
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Soens Bastien¹²^ORCID,Suttle Martin D.³⁴^ORCID,Maeda Ryoga¹,Vanhaecke Frank⁵^ORCID,Yamaguchi Akira⁶^ORCID,Van Ginneken Matthias⁷^ORCID,Debaille Vinciane²,Claeys Philippe¹^ORCID,Goderis Steven¹^ORCID

Affiliation:

1. Analytical‐, Environmental‐, and Geo‐Chemistry Vrije Universiteit Brussel Pleinlaan 2 Brussels 1050 Belgium

2. Laboratoire G‐Time Université Libre de Bruxelles 50 Av. F.D. Roosevelt CP 160/02 Brussels 1050 Belgium

3. Dipartimento di Scienze della Terra Università di Pisa Via S. Maria 53 Pisa 56126 Italy

4. Planetary Materials Group Department of Earth Sciences Natural History Museum Cromwell Road London SW7 5BD UK

5. Atomic & Mass Spectrometry – A&MS Research Group Department of Chemistry Ghent University Krijgslaan 218 – S12 Ghent 9000 Belgium

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

7. Centre for Astrophysics and Planetary Science University of Kent Canterbury Kent CT2 7NZ UK

Funder

European Research Council

Vrije Universiteit Brussel

Universiteit Gent

Belgian Federal Science Policy Office

Fonds Wetenschappelijk Onderzoek

Science and Technology Facilities Council

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13599

Reference131 articles.

1. Oxygen isotopic composition of chondritic interplanetary dust particles: A genetic link between carbonaceous chondrites and comets

2. Carbonaceous chondrites—II. Carbonaceous chondrite phyllosilicates and light element geochemistry as indicators of parent body processes and surface conditions

3. Forming Planetesimals in Solar and Extrasolar Nebulae

4. The Nebular Shock Wave Model for Chondrule Formation: Shock Processing in a Particle–Gas Suspension

5. Oxygen Isotopes in Meteorites

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