The formation of Ca-, Fe-rich silicates in reduced and oxidized CV chondrites: The roles of impact-modified porosity and permeability, and heterogeneous distribution of water ices-Reference-Cited by-同舟云学术

The formation of Ca-, Fe-rich silicates in reduced and oxidized CV chondrites: The roles of impact-modified porosity and permeability, and heterogeneous distribution of water ices

Published:2014-06-10 Issue:7 Volume:49 Page:1250-1270
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

MacPherson Glenn J.¹,Krot Alexander N.²

Affiliation:

1. Department of Mineral Sciences; U.S. National Museum of Natural History; Smithsonian Institution; Washington District of Columbia 20560-0119 USA

2. Hawai‘i Institute of Geophysics and Planetology; School of Ocean; Earth Science and Technology; University of Hawai‘i at Mānoa; Honolulu Hawai‘i 96821 USA

Funder

National Aeronautics and Space Administration

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.12316/fullpdf

Reference75 articles.

1. Deciphering the nebular and asteroidal record of silicates and organic material in the matrix of the reduced CV3 chondrite Vigarano;Abreu;Meteoritics & Planetary Science,2011

2. Fine-grained, spinel-rich inclusions from the reduced CV chondrite Efremovka: II. Oxygen isotopic compositions;Aléon;Meteoritics & Planetary Science,2005

3. Why aqueous alteration in asteroids was isochemical: High porosity ≠ high permeability;Bland;Earth and Planetary Science Letters,2009