Investigation of the Characteristic Nighttime Temperature of Potential Caves on Mars

Author:

Park NuriORCID,Hong Ik-SeonORCID,Jung JongilORCID

Abstract

By providing an environment where energetic particles and micrometeorites can not penetrate, caves on Mars may serve as a human shelter in future Mars explorations. More than 1,000 cave entrance candidates have been detected; however, their physical characteristics that can be utilized in detecting more candidates have not been explored in detail. In this paper, we explore the nighttime temperature of 100 cave entrance candidates and their surrounding areas to investigate 1) the nighttime temperature tendencies relative to their surrounding areas and 2) the extent of these temperature differences. We find that 79% of the cave entrance candidates exhibit higher temperatures than the surrounding areas, and 59% show a temperature difference over 20K, suggesting that the cave entrances may generally show higher temperatures than the surrounding areas during the nighttime.

Publisher

The Korean Space Science Society

Subject

General Earth and Planetary Sciences,General Physics and Astronomy

Reference10 articles.

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2. Christensen PR, Engle E, Anwar S, Dickenshied S, Noss D, et al., JMARS-a planetary GIS, in 2009 AGU Fall Meeting, San Francisco, CA, 14-18 Dec 2009.

3. Christensen PR, Jakosky BM, Kieffer HH, Malin MC, McSween HY Jr, et al., The thermal emission imaging system (THEMIS) for the Mars 2001 Odyssey Mission, Space Sci. Rev. 110, 85-130 (2004). 10.1023/B:SPAC.0000021008.16305.94

4. Cushing GE, Candidate cave entrances on Mars, J. Cave Karst Stud. 74, 33-47 (2012). 10.4311/2010EX0167R

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