Thickness of proximal ejecta from the Orientale Basin from Lunar Orbiter Laser Altimeter (LOLA) data: Implications for multi-ring basin formation

Author:

Fassett Caleb I.1,Head James W.1,Smith David E.,Zuber Maria T.2,Neumann Gregory A.3

Affiliation:

1. Department of Geological Sciences; Brown University; Providence; Rhode Island; USA

2. Department of Earth, Atmospheric, and Planetary Sciences; Massachusetts Institute of Technology; Cambridge; Massachusetts; USA

3. Solar System Exploration Division; NASA Goddard Space Flight Center; Greenbelt; Maryland; USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference32 articles.

1. The transition from complex craters to peak-ring basins on the Moon: New observations from the Lunar Orbiter Laser Altimeter (LOLA) instrument;Baker;Icarus,2011

2. Scaling impact melting and crater dimensions: Implications for the lunar cratering record;Cintala;Meteorit. Planet. Sci.,1998

3. Radial thickness variations of Orientale Basin ejecta;Cordell;Mod. Geol.,1978

4. Morphology of the Manicouagan ring structure, Quebec, and some comparisons with lunar basins and craters;Floran;Proc. Lunar Sci. Conf.,1976

5. Earth-based radar data reveal extended deposits of the Moon's Orientale Basin;Ghent;Geology,2008

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