Cited by 167Planetary Science and ExplorationAstro and Planetary ScienceClimate change and permafrost

The DOI matches its Crossref record; 27 of the 27 references it cites were found in a registry or an index.

THEMIS observes possible cave skylights on Mars

Open access
Cushing, G. E., Titus, T. N., Wynne, J. J., Christensen, P. R.·2007·Geophysical Research Letters

Abstract

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 m. Most candidates seem directly related to pit‐craters, and may have formed in a similar manner with overhanging ceilings that remain intact.

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Registry

Crossref · 10.1029/2007gl030709

Cites

27 of 27 references verified0 citation errors · 0 not checkable

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  • Observations from orbit of Mars revealed that possible cave skylights or lava tubes are not uncommon on the Martian surface.

    “Observations from the orbit of Mars revealed that possible cave skylights (Cushing et al. 2007) or lava tubes (Le ´veille ´and Datta 2010) are not uncommon on the Martian surface.”

    From Radiation environment for future human exploration on the surface of Mars: the current understanding based on MSL/RAD dose measurements (2021) · cites this paper as Cushing et al. 2007

    The Abstract and Introduction report seven possible cave skylights observed from orbit on or near Arsia Mons. They do not establish that such features are not uncommon across the Martian surface; the Observations section says entrances detectable by THEMIS are probably rare. (LLM, conf=0.88)

    Experimental — accuracy not yet measured

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Metadata

Authors
Cushing, G. E., Titus, T. N., Wynne, J. J., & Christensen, P. R.
Affiliations
  • United States Geological Survey (US)
  • Northern Arizona University (US)
  • Arizona State University (US)
Corresponding author
Cushing, G. E.
Venue
Geophysical Research Letters
Published
2007-09
Volume
34
Issue
17
Pages
1371
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
OpenAlex
W2076708908
Cited by
167
References
27
Citations by year
2026: 8 · 2025: 12 · 2024: 9 · 2023: 6 · 2022: 19 · 2021: 16 · 2020: 10 · 2019: 3 · 2018: 6 · 2017: 7 · 2016: 6 · 2015: 11 · 2014: 16 · 2013: 8 · 2012: 11
FWCI
2.19
Type
journal article
Language
en
Open access
Locations
  • Geophysical Research Letters (publishedVersion)
  • Digital Commons - University of South Florida (University of South Florida) (submittedVersion)
  • LPI
Topics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
  • Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Climate change and permafrost
Keywords
Arsia Mons, THEMIS, pit craters, subsurface materials, Mars surface features

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