Chronology of martian breccia NWA 7034 and the formation of the martian crustal dichotomy-Reference-Cited by-同舟云学术

Chronology of martian breccia NWA 7034 and the formation of the martian crustal dichotomy

Published:2018-05-04 Issue:5 Volume:4 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Cassata William S.¹^ORCID,Cohen Benjamin E.²³^ORCID,Mark Darren F.²⁴^ORCID,Trappitsch Reto¹^ORCID,Crow Carolyn A.¹^ORCID,Wimpenny Joshua¹,Lee Martin R.³^ORCID,Smith Caroline L.³⁵^ORCID

Affiliation:

1. Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore, CA 94550, USA.

2. Isotope Geoscience Unit, Scottish Universities Environmental Research Centre, Rankine Avenue, East Kilbride, G75 0QF, UK.

3. School of Geographical and Earth Sciences, University of Glasgow, G12 8QQ, UK.

4. Department of Earth and Environmental Sciences, University of St. Andrews, St. Andrews, KY16 9AJ, UK.

5. Department of Earth Sciences, Natural History Museum, London, SW7 5BD, UK.

Abstract

The metamorphic history of martian meteorite NWA 7034 suggests that the martian crustal dichotomy may have formed within 100 million years of planetary formation.

Funder

National Aeronautics and Space Administration

Science and Technology Facilities Council

LLNL Laboratory Directed Research and Development

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference82 articles.

1. Petrology of igneous clasts in Northwest Africa 7034: Implications for the petrologic diversity of the martian crust

2. Origin and age of the earliest Martian crust from meteorite NWA 7533

3. Rare-earth-element minerals in martian breccia meteorites NWA 7034 and 7533: Implications for fluid–rock interaction in the martian crust;Liu Y.;Earth Planet. Sci. Lett.,2016