T66 Best Practices and Exciting Discoveries in Identifying, Mapping, and Analyzing Planetary Landforms and Terrestrial Analogues
Sunday, 22 September 2019
1:30 PM - 5:30 PM
Room 232BC, North Building
GEOLOGIC MAPPING FOR SMALL ROCKY BODIES: THE VESTA EXAMPLE
Paper number: T66-4
Program: Technical Sessions
Time: 2:15 PM – 2:30 PM
Authors
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Daniel C. BermanPlanetary Science Institute, Tucson, AZ
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Scott MestPlanetary Science Institute, Tucson, AZ
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David A. WilliamsArizona State University, Tempe, AZ
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Tracy K.P. GreggThe University at Buffalo, State University of New York, Buffalo, NY
Abstract
Our initial approach was to characterize units based on morphology, surface textures, and albedo, as well as crater size-frequency distribution and superposition relations. Color data from the FC (and VIR) were examined as an overlay on the first draft of units, to refine unit boundaries where morphologic characteristics provided more than one possible border, or the interpretation of the unit type was ambiguous. However, this method did not provide us with sufficient ability to assess and interpret the spectroscopic and color data on its own merits. As a result, the color and morphologic data were not being incorporated synergistically into interpretations.
Recently we have begun a different approach, one initially used to test how the availability of various types of datasets affects mapping results. This method requires creating a GIS map based on each available dataset in isolation, then comparing the resulting maps to assess the information unique to each dataset, and of that, what best summarizes the geologic history of the region. We report on initial results of this approach.
Geological Society of America Abstracts with Programs. Vol. 51, No. 5
doi: 10.1130/abs/2019AM-338561
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