Sinuosity of Martian rampart ejecta deposits

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Abstract

The sinuosities of 2213 Martian rampart ejecta craters are quantified through measurement of the ejecta flow front perimeter and ejecta area. This quantity, called lobateness, was computed for each complete lobe of the 1582 single lobe (SL), 251 double lobe (DL), and 380 multiple lobe (ML) craters included in this study. Evaluation of the lobateness values reveals that the outer lobes of DL and ML craters have higher median lobateness values (i.e., are more sinuous) that the inner lobes. The outermost lobe of ML craters displays higher lobateness values than the outer lobe of DL craters or the single lobe of SL craters. The results of this study taken together with a previous analysis of the distribution and diameter dependence of different ejecta morphologies are most consistent with the theory that Martian lobate ejecta morphologies form from impact into subsurface volatiles. -from Author

Original languageEnglish (US)
JournalJournal of Geophysical Research E: Planets
Volume99
Issue numberE5
StatePublished - 1994
Externally publishedYes

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ASJC Scopus subject areas

  • Earth and Planetary Sciences(all)
  • Environmental Science(all)

Cite this

Sinuosity of Martian rampart ejecta deposits. / Barlow, Nadine.

In: Journal of Geophysical Research E: Planets, Vol. 99, No. E5, 1994.

Research output: Contribution to journalArticle

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