2007
DOI: 10.1029/2007gl030709
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THEMIS observes possible cave skylights on Mars

Abstract: [1] Seven possible skylight entrances into Martian caves were observed on and around the flanks of Arsia Mons by the Mars Odyssey Thermal Emission Imaging System (THEMIS). Distinct from impact craters, collapse pits or any other surface feature on Mars, these candidates appear to be deep dark holes at visible wavelengths while infrared observations show their thermal behaviors to be consistent with subsurface materials. Diameters range from 100 m to 225 m, and derived minimum depths range between 68 m and 130 … Show more

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Cited by 138 publications
(105 citation statements)
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“…Holt et al 2008). The specific interest in lava tubes on Earth is motivated by their presence in volcanic, basaltic environments analogous to the geological context of lava tubes on Mars (Cushing et al 2007;Williams et al 2010). On Mars, lava tubes provide a natural way to access the deep subsurface.…”
Section: Lava Tubes and Cavesmentioning
confidence: 99%
“…Holt et al 2008). The specific interest in lava tubes on Earth is motivated by their presence in volcanic, basaltic environments analogous to the geological context of lava tubes on Mars (Cushing et al 2007;Williams et al 2010). On Mars, lava tubes provide a natural way to access the deep subsurface.…”
Section: Lava Tubes and Cavesmentioning
confidence: 99%
“…For broad-scale prospecting, airborne-or satellite-based remote sensing is necessary. Because caves have a more stable temperature than the surface environment, there has been an effort to use thermal remote sensing on earth (Griffith, 2000) and on other planets (Cushing et al, 2007;Wynne et al, 2008) to detect cave openings. Though a temperature gradient of 7.2 uC was detected on the ground 50 to 100 m away from cave openings in Belize (Griffith, 2001), this method is challenging, given the coarse resolution of most satellite thermal sensors.…”
Section: Introductionmentioning
confidence: 99%
“…They also provide a model system of a biomat that might occur on the interiors of various cave types on Mars. Lavatubes have been identified on Mars [4], and more recently confirmed in a more elaborate study [12]. Mechanisms to create solutional caves in evaporite mineral deposits on Mars have also been proposed [5].…”
Section: Biovermiculationsmentioning
confidence: 99%