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How the Martian Residual South Polar Cap Develops Quasi-Circular and Heart-Shaped Pits, Troughs, and Moats

Buhler, Peter B. and Ingersoll, Andrew P. and Ehlmann, Bethany L. and Fassett, Caleb I. and Head, James W. (2017) How the Martian Residual South Polar Cap Develops Quasi-Circular and Heart-Shaped Pits, Troughs, and Moats. Icarus, 286 . pp. 69-93. ISSN 0019-1035. http://resolver.caltech.edu/CaltechAUTHORS:20170118-154814373

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Abstract

The martian Residual South Polar Cap (RSPC) is a 1-10 m thick deposit of permanent CO_2 ice perched on the much larger H_2O ice cap. The CO_2 ice is dissected into mesas by erosional landforms that can be broadly classified as (i) quasi-circular pits, (ii) heart-shaped pits, (iii) linear troughs, and (iv) moats. We use HiRISE (25-50 cm/px) images taken at a cadence of days to months to track meter-scale changes in the RSPC in order to investigate the mechanisms that lead to the development of these four distinct morphologies. For the first time, we report the development of dark fans on the sides of the CO_2 mesas and the fracturing and deterioration of the initially smooth upper surface of CO_2 mesas. We interpret these features as indicating the sublimation and subsequent escape of CO_2 from the interiors of mesas, which undermines structural support of mesa tops, causing them to collapse. The collapse of mesa tops, along with uneven deposition of CO_2 ice, creates steep scarps that erode during the summer due to preferential sunlight absorption. During the winter, CO_2 deposition acts to smooth topography, creating gently sloping ramps. We propose that the interplay between the steep scarps and gentle slopes leads to either quasi-circular pits, heart-shaped pits, linear troughs, or moats, depending on local conditions.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/j.icarus.2017.01.012DOIArticle
http://www.sciencedirect.com/science/article/pii/S0019103516304171PublisherArticle
ORCID:
AuthorORCID
Ingersoll, Andrew P.0000-0002-2035-9198
Ehlmann, Bethany L.0000-0002-2745-3240
Additional Information:© 2017 The Authors. Published by Elsevier Inc. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/). Received 25 July 2016, Available online 13 January 2017. We gratefully acknowledge funding from NESSF grant #16-PLANET16F-0071 and MFRP grant #NNX14AG54G. We also thank Timothy Titus and an anonymous reviewer for their feedback, which helped to improve this work.
Funders:
Funding AgencyGrant Number
NASA Earth and Space Science Fellowship16-PLANET16F-0071
NASANNX14AG54G
Record Number:CaltechAUTHORS:20170118-154814373
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170118-154814373
Official Citation:Peter B. Buhler, Andrew P. Ingersoll, Bethany L. Ehlmann, Caleb I. Fassett, James W. Head, How the martian residual south polar cap develops quasi-circular and heart-shaped pits, troughs, and moats, Icarus, Volume 286, April 2017, Pages 69-93, ISSN 0019-1035, http://dx.doi.org/10.1016/j.icarus.2017.01.012. (http://www.sciencedirect.com/science/article/pii/S0019103516304171)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:73535
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Jan 2017 18:56
Last Modified:07 Mar 2017 22:17

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