Shock veins and brown olivine in Martian meteorites: Implications for their shock pressure-temperature histories-Reference-Cited by-同舟云学术

Shock veins and brown olivine in Martian meteorites: Implications for their shock pressure-temperature histories

Published:2018-06-04 Issue:11 Volume:53 Page:2259-2284
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Takenouchi Atsushi¹²^ORCID,Mikouchi Takashi¹³,Yamaguchi Akira⁴⁵^ORCID

Affiliation:

1. Department of Earth and Planetary Science; Graduate School of Arts and Sciences; The University of Tokyo; 7-3-1 Hongo Bunkyo-ku Tokyo 113-0033 Japan

2. Department of Basic Sciences; Graduate School of Science; The University of Tokyo; 3-8-1 Komaba Meguro-ku Tokyo 153-8902 Japan

3. The University Museum; The University of Tokyo; 7-3-1 Hongo Bunkyo-ku Tokyo 113-0033 Japan

4. National Institute of Polar Research; 10-3 Midori-cho Tachikawa-shi Tokyo 190-8518 Japan

5. Department of Polar Science; School of Multidisciplinary Science; SOKENDAI (The Graduate University for Advanced Studies); Tachikawa-shi Tokyo 190-8518 Japan

Funder

National Institute of Polar Research

Japan Society for the Promotion of Science

NIPR General Collaboration Project

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.13120/fullpdf

Reference57 articles.

1. Tissint Martian meteorite: A fresh look at the interior, surface, and atmosphere of Mars;Aoudjehane;Science,2012