Comparison of central pit craters on Mars, Mercury, Ganymede, and the Saturnian satellites-Reference-Cited by-同舟云学术

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Comparison of central pit craters on Mars, Mercury, Ganymede, and the Saturnian satellites

Published:2017-05-11 Issue:7 Volume:52 Page:1371-1387
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Barlow Nadine G.¹^ORCID,Ferguson Sierra N.²,Horstman Ryan M.³,Maine Aviva⁴

Affiliation:

1. Department of Physics and Astronomy; Northern Arizona University; Flagstaff Arizona 86011-6010 USA

2. School of Earth and Space Exploration; Arizona State University; Tempe Arizona 85287-1404 USA

3. W.L. Gore & Associates; Flagstaff Arizona 86004 USA

4. Department of Geology; Northern Arizona University; Flagstaff Arizona 86011-5694 USA

Funder

Outer Planets Research Program

Mars Data Analysis Program

Planetary Geology and Geophysics Program

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.12857/fullpdf

Reference63 articles.

1. Central peaks in lunar craters;Allen;The Moon,1975

2. Central pit craters on Ganymede;Alzate;Icarus,2011

3. Central pit craters: Observations from Mars and Ganymede and implications for formation models

4. Martian impact craters: Correlations of ejecta and interior morphologies with diameter, latitude, and terrain;Barlow;Icarus,1990

5. Becker T. Archinal B. Colvin T. Davies M. Gitlin A. Kirk R. L. Weller L. 2001 Final digital global maps of Ganymede, Europa, and Callisto

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