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Using Measurements of Topography to Infer Rates of Crater Degradation and Surface Evolution on the Moon and MercuryMotivating questions: 1. How does the topography of airless bodies evolve? 2. What is the relative rate on the Moon and Mercury? 3. Can we constrain the age of features and units from their topography?
Document ID
20170011721
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Fassett, Caleb (NASA Marshall Space Flight Center Huntsville, AL, United States)
Crowley, Lindy (Wellesley Coll. MA, United States)
Leight, Clarissa (Mount Holyoke Coll. South Hadley, MA, United States)
Dyar, Darby (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Minton, David (Purdue Univ. Fort Wayne, IN, United States)
Hirabayashi, Toshi (Purdue Univ. Fort Wayne, IN, United States)
Thomson, Brad (Tennessee Univ. Knoxville, TN, United States)
Watters, Wesley (Wellesley Coll. MA, United States)
Date Acquired
December 13, 2017
Publication Date
December 12, 2017
Subject Category
Lunar And Planetary Science And Exploration
Geophysics
Report/Patent Number
MSFC-E-DAA-TN50154
Meeting Information
Meeting: AGU Fall Meeting 2017
Location: New Orleans, LA
Country: United States
Start Date: December 11, 2017
End Date: December 15, 2017
Sponsors: American Geophysical Union
Funding Number(s)
CONTRACT_GRANT: NNN12AA01C
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.

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