Sierra Gorda 009: A new member of the metal‐rich G chondrites grouplet-Reference-Cited by-同舟云学术

Sierra Gorda 009: A new member of the metal‐rich G chondrites grouplet

Published:2020-08 Issue:8 Volume:55 Page:
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Ivanova Marina A.¹^ORCID,Lorenz Cyril A.¹^ORCID,Humayun Munir²,Corrigan Catherine M.³,Ludwig Thomas⁴,Trieloff Mario⁴^ORCID,Righter Kevin⁵^ORCID,Franchi Ian A.⁶,Verchovsky Alexander B.⁶^ORCID,Korochantseva Ekaterina V.¹,Kozlov Vladimir V.⁷,Teplyakova Svetlana N.¹,Korochantsev Alexander V.¹,Grokhovsky Victor I.⁸

Affiliation:

1. Vernadsky Institute of Geochemistry and Analytical Chemistry Moscow 119991 Russia

2. National High Magnetic Field Laboratory and Department of Earth, Ocean & Atmospheric Science Florida State University 1800 E. Paul Dirac Drive Tallahassee Florida 32310 USA

3. National Museum of Natural History Smithsonian Institution Washington District of Columbia 20560 USA

4. Institut für Geowissenschaften Klaus Tschira‐Labor für Kosmochemie Ruprecht‐Karls‐Universität Heidelberg D‐69120 Heidelberg Germany

5. NASA – Johnston Space Center Mailcode XI2 Houston Texas 77058 USA

6. Planetary and Space Sciences Research Institute Open University Milton Keynes MK7 6AA UK

7. Oxford Instruments OM & Gatan Inc Moscow Office 26 Denisovskii Pereulok Moscow 105005 Russia

8. Ural Federal University Ekaterinburg 620002 Russian Federation

Funder

National Science Foundation

Ministerstwo Nauki i Szkolnictwa Wyższego

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13546

Reference85 articles.

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2. AmelinY.andKrotA. E.2005.Young Pb‐isotopic ages of chondrules in CB carbonaceous chondrites (abstract # 1247). 36th Lunar and Planetary Science Conference. CD‐ROM.

3. Abundances of the elements: Meteoritic and solar

4. Acfer 217-A new member of the Rumuruti chondrite group (R)

5. Origin of opaque assemblages in C3V meteorites: Implications for nebular and planetary processes

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