Noble gases in angrites Northwest Africa 1296, 2999/4931, 4590, and 4801: Evolution history inferred from noble gas signatures

Author:

Nakashima Daisuke12ORCID,Nagao Keisuke23,Irving Anthony J.4

Affiliation:

1. Department of Earth and Planetary Material Sciences; Faculty of Science; Tohoku University; Aoba Sendai Miyagi 980-8578 Japan

2. Geochemical Research Center; Graduate School of Science; University of Tokyo; Hongo Bunkyo Tokyo 113-0033 Japan

3. Division of Polar Earth-System Sciences; Korea Polar Research Institute; Incheon 21990 Korea

4. Department of Earth & Space Sciences; University of Washington; Seattle Washington 98915 USA

Funder

Japan Society for the Promotion of Science

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference90 articles.

1. Weathering of meteorites from Oman: Correlation of chemical and mineralogical weathering proxies with 14C terrestrial ages and the influence of soil chemistry;Al-Kathiri;Meteoritics & Planetary Science,2005

2. Amelin Y. Irving A. J. 2007 Seven million years of evolution on the angrite parent body from Pb-isotopic data (abstract) 20 21

3. Lead isotopic ages of chondrules and calcium-aluminum-rich inclusions;Amelin;Science,2002

4. U-Pb chronology of the solar system's oldest solids with variable 238U/235U;Amelin;Earth and Planetary Science Letters,2010

5. Early planetesimal melting from an age of 4.5662 Gyr for differentiated meteorites;Baker;Nature,2005

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