Martian pedestal craters: Marginal sublimation pits implicate a climate-related formation mechanism
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چکیده
[1] Pedestal craters on Mars are defined by an outwardfacing scarp forming a plateau perched tens of meters above the surrounding terrain. Their origin has been attributed to impact armoring of the surface and subsequent removal of inter-crater terrain by either eolian deflation or sublimation of an ice-rich substrate. We identified 2696 pedestal craters between 60 N and 60 S latitude; 98% are poleward of 33 N and 40 S. The majority of pedestal crater margins are smoothly sloped, but 3%, concentrated in Utopia Planitia and Malea Planum, display distinctive marginal pits. These pedestal crater scarps are anomalously tall (usually >80– 100 m) and the pits resemble sublimation depressions seen on Earth and elsewhere on Mars, providing evidence for sublimation of volatiles in the scarp, where the armored surface has tapered. The pitted scarps provide insight into the origin of the general pedestal crater population, favoring formation via deposition of a volatile-rich substrate, impact armoring, and sublimation of intervening volatiles. Crater densities and overlapping pedestal craters suggest multiple periods of emplacement and loss of these climate-related, latitude-dependent deposits throughout the Amazonian. Citation: Kadish, S. J., J. W. Head, N. G. Barlow, and D. R. Marchant (2008), Martian pedestal craters: Marginal sublimation pits implicate a climate-related formation mechanism, Geophys. Res. Lett., 35, L16104, doi:10.1029/2008GL034990.
منابع مشابه
Latitude dependence of Martian pedestal craters: Evidence for a sublimation-driven formation mechanism
[1] We report on the results of a survey to document and characterize pedestal craters on Mars equatorward of 60 N and 65 S latitude. The identification of 2696 pedestal craters reveals a strong latitude dependence, with the vast majority found poleward of 33 N and 40 S. This latitudinal extent is correlated with many climate indicators consistent with the presence of an ice-rich substrate and ...
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Preservation of layered paleodeposits in high-latitude pedestal craters on Mars
0019-1035/$ see front matter 2011 Elsevier Inc. A doi:10.1016/j.icarus.2011.03.029 ⇑ Corresponding author. Fax: +1 401 863 3978. E-mail address: [email protected] (S.J. Kadi An outstanding question in Mars’ climate history is whether or not pedestal craters represent the armored remnants of ice-rich paleodeposits. We address this question using new high-resolution images; in a survey of sev...
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We compare three previously independently studied crater morphologies – excess ejecta craters, perched craters, and pedestal craters – each of which has been proposed to form from impacts into an ice-rich surface layer. Our analysis identifies the specific similarities and differences between the crater types; the commonalities provide significant evidence for a genetic relationship among the m...
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تاریخ انتشار 2008