Lunar "Cold Spots": A New Class of Thermophysically and Morphologically Distinct Craters

Details Lunar "Cold Spots": A New Class of Thermophysically and Morphologically Distinct Craters Lunar "Cold Spots": A New Class of Thermophysically and Morphologically Distinct Craters

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1487b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1487

Physics

Scientific paper

A class of lunar craters are surrounded by a highly insulating regolith
layer that can extend over 100 crater radii from the source. Visible
images do not show this layer but display layered near-crater ejecta
with fluidized flow morphologies.

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