Pit-floor craters on Mercury: Evidence of near-surface igneous activity

Jeffrey J. Gillis-Davis, David T. Blewett, Robert W. Gaskell, Brett W. Denevi, Mark Robinson, Robert G. Strom, Sean C. Solomon, Ann L. Sprague

Research output: Contribution to journalArticle

30 Citations (Scopus)

Abstract

High-resolution images obtained during the first MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) flyby of Mercury show evidence for igneous modification of the surface through the formation of pit craters on the floors of several impact craters. Pit craters are rimless steep-sided depressions that are inferred to have formed by non-impact processes. Among the arguments in favor of this interpretation are that the features lack evident rims; exhibit no observable ejecta; are irregularly shaped (e.g., subcircular, elliptical, or arcuate), with the long axis of the pit crater often concentric to the rim of the host impact crater; and are superposed on smooth plains deposits within the craters. Pit craters documented to date do not exhibit signs of extrusive flows. Impact craters hosting pit craters, termed pit-floor craters, vary in size from 55 to 120 km in diameter, while the associated pit craters range in maximum horizontal dimension from 20 to almost 40 km. Pit crater radius and host crater radius are not well correlated for pit-floor craters on Mercury, in contrast to the situation for otherwise similar features on Mars. On the basis of morphology, structural association, relative age, and proximity to smooth plains for pit craters on Mercury, we test mechanisms of pit crater formation previously proposed for such features on other planetary bodies (e.g., Earth, Moon, Mars, and Venus). We conclude that pit craters on Mercury formed through collapse into an underlying drained magma chamber. Pit-floor craters thus provide evidence for near-surface magmatic activity on Mercury and extend the range of evidence for magmatism beyond such surface expressions as smooth plains and pyroclastic deposits.

Original languageEnglish (US)
Pages (from-to)243-250
Number of pages8
JournalEarth and Planetary Science Letters
Volume285
Issue number3-4
DOIs
StatePublished - Aug 15 2009

Fingerprint

Mercury
craters
crater
Deposits
Geochemistry
Moon
Image resolution
plains
mercury
Earth (planet)
Association reactions
rims
mars
Mars
deposits
Mercury surface
pyroclastic deposit
radii
aerospace environments
Venus (planet)

Keywords

  • Mercury
  • MESSENGER
  • pit crater
  • remote sensing
  • volcanism

ASJC Scopus subject areas

  • Geochemistry and Petrology
  • Geophysics
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

Cite this

Gillis-Davis, J. J., Blewett, D. T., Gaskell, R. W., Denevi, B. W., Robinson, M., Strom, R. G., ... Sprague, A. L. (2009). Pit-floor craters on Mercury: Evidence of near-surface igneous activity. Earth and Planetary Science Letters, 285(3-4), 243-250. https://doi.org/10.1016/j.epsl.2009.05.023

Pit-floor craters on Mercury : Evidence of near-surface igneous activity. / Gillis-Davis, Jeffrey J.; Blewett, David T.; Gaskell, Robert W.; Denevi, Brett W.; Robinson, Mark; Strom, Robert G.; Solomon, Sean C.; Sprague, Ann L.

In: Earth and Planetary Science Letters, Vol. 285, No. 3-4, 15.08.2009, p. 243-250.

Research output: Contribution to journalArticle

Gillis-Davis, JJ, Blewett, DT, Gaskell, RW, Denevi, BW, Robinson, M, Strom, RG, Solomon, SC & Sprague, AL 2009, 'Pit-floor craters on Mercury: Evidence of near-surface igneous activity', Earth and Planetary Science Letters, vol. 285, no. 3-4, pp. 243-250. https://doi.org/10.1016/j.epsl.2009.05.023
Gillis-Davis, Jeffrey J. ; Blewett, David T. ; Gaskell, Robert W. ; Denevi, Brett W. ; Robinson, Mark ; Strom, Robert G. ; Solomon, Sean C. ; Sprague, Ann L. / Pit-floor craters on Mercury : Evidence of near-surface igneous activity. In: Earth and Planetary Science Letters. 2009 ; Vol. 285, No. 3-4. pp. 243-250.
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