Identification of buried lunar impact craters from GRAIL data and implications for the nearside maria

Alexander J. Evans, Jason M. Soderblom, Jeffrey C. Andrews-Hanna, Sean C. Solomon, Maria T. Zuber

Research output: Contribution to journalArticlepeer-review

34 Scopus citations

Abstract

Gravity observations from the dual Gravity Recovery and Interior Laboratory (GRAIL) spacecraft have revealed more than 100 quasi-circular mass anomalies, 26-300 km in diameter, on the lunar nearside. These anomalies are interpreted to be impact craters filled primarily by mare deposits, and their characteristics are consistent with those of impact structures that formed prior to, and during, intervals of flooding of feldspathic terrane by mare basalt lavas. We determine that mare deposits have an average density contrast of 850-200+300 kg m-3 relative to the surrounding crust. The presence of a large population of volcanically buried craters with minimal topographic expression and diameters up to 300 km requires an average nearside mare thickness of at least 1.5 km and local lenses of mare basalt as thick as ∼7 km.

Original languageEnglish (US)
Pages (from-to)2445-2455
Number of pages11
JournalGeophysical Research Letters
Volume43
Issue number6
DOIs
StatePublished - Mar 28 2016
Externally publishedYes

Keywords

  • GRAIL
  • Moon
  • buried
  • crater
  • lunar
  • maria

ASJC Scopus subject areas

  • Geophysics
  • Earth and Planetary Sciences(all)

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