| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773597 | Icarus | 2012 | 11 Pages |
Abstract
⺠Many Copernican lunar craters have well preserved impact melt flows. ⺠Meter-scale digital terrain models allow quantitative analysis of impact melt flow deposits. ⺠Observations of impact melt deposits show that they were highly fluid and emplaced at high temperatures (superheated). ⺠Melt volume per impact event can vary significantly above model predictions.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Brett W. Denevi, Steven D. Koeber, Mark S. Robinson, W. Brent Garry, B. Ray Hawke, Thanh N. Tran, Samuel J. Lawrence, Laszlo P. Keszthelyi, Olivier S. Barnouin, Carolyn M. Ernst, Livio L. Tornabene,