Distribution of Early, Middle, and Late Noachian cratered surfaces in the Martian highlands: Implications for resurfacing events and processes-Reference-Cited by-同舟云学术

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Distribution of Early, Middle, and Late Noachian cratered surfaces in the Martian highlands: Implications for resurfacing events and processes

Published:2013-02 Issue:2 Volume:118 Page:278-291
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Irwin Rossman P.¹,Tanaka Kenneth L.²,Robbins Stuart J.³

Affiliation:

1. Center for Earth and Planetary Studies, National Air and Space Museum; Smithsonian Institution; Washington D.C. USA

2. U. S. Geological Survey; Astrogeology Science Center; Flagstaff Arizona USA

3. Laboratory for Atmospheric and Space Physics; University of Colorado; Boulder Colorado USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference72 articles.

1. Early Mars hydrology: Meridiani playa deposits and the sedimentary record of Arabia Terra;Andrews-Hanna;J. Geophys. Res.,2010

2. Early Mars hydrology: 2. Hydrological evolution in the Noachian and Hesperian epochs;Andrews-Hanna;J. Geophys. Res.,2011

3. Morphologic classification of Martian craters and some implications;Arvidson;Icarus,1974

4. Overview of the Spirit Mars Exploration Rover Mission to Gusev crater: Landing site to Backstay Rock in the Columbia Hills;Arvidson;J. Geophys. Res.,2006

5. Crater size-frequency distributions and a revised Martian relative chronology;Barlow;Icarus,1988

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