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Recently, cave candidates have been discovered on other planets besides the Earth, such as the Moon and Mars. When\udwe go to other planets, caves could be possible human habitats providing natural protection from cosmic threats. In this\udstudy, seven cave candidates have been found on Pavonis Mons and Ascraeus Mons in Tharsis Montes on Mars. The cave\udcandidates were selected using the images of the Context Camera (CTX) on the Mars Reconnaissance Orbiter (MRO). The\udContext Camera could provide images with the high resolution of 6 meter per pixel. The diameter of the candidates ranges\udfrom 50 to 100m. Cushing et al. (2007) have analyzed the temperature change at daytime and nighttime using the Thermal\udEmission Imaging System (THEMIS) for the sites of potential cave candidates. Similarly, we have examined the temperature\udchange at daytime and at nighttime for seven cave candidates using the method of Cushing et al. (2007). Among those, only\udone candidate showed a distinct temperature change. However, we cannot verify a cave based on the temperature change\udonly and further study is required for the improvement of this method to identify caves more clearly

Identification of Martian Cave Skylights Using the Temperature Change During Day and Night