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Potential of Radar Imaging and Sounding Methods in Mapping Heavily Eroded Impact Craters: Mapping Some Structural Elements of the Hico Crater, TXShuttle Radar Topography Mission (SRTM) and Ground Penetrating Radar (GPR) data collected over an area north of the town of Hico, central Texas, have been used to map disturbances in the surface topography and subsurface stratigraphy. The Radar topography results confirm the presence of multiple rings suggestive of an impact crater. Correlation between the orbital SRTM and on-the-ground GPR field data are affected by different biases related to variations in terrain and vegetation cover. Nevertheless, the correspondence of the two data sets supports the earlier conclusions that a complex, multiple ring impact structure is reflected in the topography of this area. The SRTM data reveal three previously unrecognized rings; with the outermost ring some 5-6 km in diameter. The crater appears to be significantly larger than the size (2.5 km diameter) previously inferred on the basis of aerial images. In addition, the GPR data suggest the presence of subsurface faulting that spatially coincides with the two inner rings of the crater. This suggests that the topographic rings are structurally controlled by faulting.
Document ID
20040062051
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Heggy, E.
(Lunar and Planetary Inst. Houston, TX, United States)
Horz, F.
(NASA Johnson Space Center Houston, TX, United States)
Reid, A. M.
(Lunar and Planetary Inst. Houston, TX, United States)
Hall, S. A.
(Houston Univ. TX, United States)
Chan, C.
(Houston Univ. TX, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Publication Information
Publication: Lunar and Planetary Science XXXV: Impacts: Observations and Experiments
Subject Category
Geosciences (General)
Distribution Limits
Public
Copyright
Public Use Permitted.
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