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Modification of secondary craters on the Martian South Polar Layered Deposits

Schaller, E. L. and Murray, B. and Pathare, A. V. and Rasmussen, J. and Byrne, S. (2005) Modification of secondary craters on the Martian South Polar Layered Deposits. Journal of Geophysical Research E, 110 (E2). Art. No. E02004. ISSN 0148-0227. https://resolver.caltech.edu/CaltechAUTHORS:20140414-132022144

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Abstract

Secondary crater fields are important stratigraphic markers that can shed light on resurfacing processes that have occurred since their formation. We examine the morphologies of secondary craters formed from the ejection of material from two large impacts on the Martian South Polar Layered Deposits (SPLD): McMurdo crater at 84.5°S, 0°W, and an unnamed impact at 80.8°S, 284°W. The morphologies of these secondary craters allow us to impose constraints on the modification history of the SPLD. We have quantified crater morphologies using data sets from the Mars Global Surveyor and Mars Odyssey missions. We find a complete lack of secondary craters smaller than 300 m in diameter in both crater fields, which implies that at least the upper 30 m of the deposits have been resurfaced since the time of these impacts. Secondary crater depth-to-diameter ratios are low (average of 0.016), indicating that significant degradation has occurred since their emplacement. We find that vertical resurfacing alone is not enough to explain the observed depth-to-diameter distribution and suggest that viscous relaxation of craters coupled with a small amount of vertical resurfacing best fits the data. In the McMurdo field, high depth-to-diameter craters are found preferentially on steeper terrain associated with scarps cutting through the secondary field. This observation suggests that crater modification exhibits a dependence on slope. We comment on possible mechanisms that may explain this observation. The morphologies of secondary craters on the SPLD point to modification processes without lunar parallel and not yet fully modeled for Mars.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/2004JE002334PublisherArticle
http://onlinelibrary.wiley.com/doi/10.1029/2004JE002334/abstractAuthorArticle
Additional Information:© 2005 American Geophysical Union. Received 28 July 2004; revised 21 September 2004; accepted 7 December 2004; published 15 February 2005. This work was supported by NASA grants NAG5-13343 and NAG5-9606, and JPL PO 1216592. E.L.S. also acknowledges the support of an NSF Graduate Research Fellowship. We benefited from the helpful criticism and suggestions by Alfred McEwen and Nadine Barlow.
Funders:
Funding AgencyGrant Number
NASANAG5-13343
NASANAG5-9606
JPLPO 1216592
NSF Graduate Research FellowshipUNSPECIFIED
Subject Keywords:polar layered deposits; secondary craters
Issue or Number:E2
Record Number:CaltechAUTHORS:20140414-132022144
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140414-132022144
Official Citation:Schaller, E. L., B. Murray, A. V. Pathare, J. Rasmussen, and S. Byrne (2005), Modification of secondary craters on the Martian South Polar Layered Deposits, J. Geophys. Res., 110, E02004, doi:10.1029/2004JE002334.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:44931
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:14 Apr 2014 22:09
Last Modified:03 Oct 2019 06:24

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