Investigating Evolved Compositions Around Wolf CraterWolf crater is an irregularly shaped, approximately 25 km crater in the south-central portion of Mare Nubium on the lunar nearside. While not previously identified as a lunar "red spot", Wolf crater was identified as a Th anomaly by Lawrence and coworkers. We have used data from the Lunar Reconnaissance Orbiter (LRO) to determine the area surrounding Wolf crater has composition more similar to highly evolved, non-mare volcanic structures than typical lunar crustal lithology. In this presentation, we will investigate the geomorphology and composition of the Wolf crater and discuss implications for the origin of the anomalous terrain.
Document ID
20170001959
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Greenhagen, B. T. (Johns Hopkins Univ. Laurel, MD, United States)
Cahill, J. T. S. (Johns Hopkins Univ. Laurel, MD, United States)
Jolliff, B. L. (Washington Univ. Saint Louis, MO, United States)
Lawrence, S. J. (NASA Johnson Space Center Houston, TX, United States)
Glotch, T. D. (Stony Brook Univ. Stony Brook, NY, United States)