Articles | Volume 11, issue 4
https://doi.org/10.5194/esurf-11-713-2023
https://doi.org/10.5194/esurf-11-713-2023
Research article
 | 
02 Aug 2023
Research article |  | 02 Aug 2023

Morphologic and morphometric differences between gullies formed in different substrates on Mars: new insights into the gully formation processes

Rishitosh K. Sinha, Dwijesh Ray, Tjalling De Haas, Susan J. Conway, and Axel Noblet

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Cited articles

Arango, M. I., Aristizábal, E., and Gómez, F.: Morphometrical analysis of torrential flows-prone catchments in tropical and mountainous terrain of the Colombian Andes by machine learning techniques, Nat. Hazards, 105, 983–1012, https://doi.org/10.1007/s11069-020-04346-5, 2021. 
Arfstrom, J. and Hartmann, W. K.: Martian flow features, moraine-like ridges, and gullies: terrestrial analogs and interrelationships, Icarus, 174, 321–335, https://doi.org/10.1016/j.icarus.2004.05.026, 2005. 
Aston, A., Conway, S., and Balme, M.: Identifying Martian Gully Evolution, in: Martian Geomorphology, edited by: Balme, M. R., Bargery, A. S., Gallagher, C. J., and Gupta, S., Geological Society, London, Special Publications, 356, 151–169, https://doi.org/10.1144/SP356.9, 2011. 
Baker, D. M. H, James W. H., and David R. M.: Flow patterns of lobate debris aprons and lineated valley fill north of Ismeniae Fossae, Mars: Evidence for extensive mid-latitude glaciation in the Late Amazonian, Icarus, 207, 186–209, https://doi.org/10.1016/j.icarus.2009.11.017, 2010. 
Balme, M., Mangold, N. Et Al.: Orientation and distribution of recent gullies in the Southern Hemisphere of Mars: observations from High Resolution Stereo Camera/Mars Express (HRSC/MEX) and Mars Orbiter Camera/Mars Global Surveyor (MOC/MGS) data, J. Geophys. Res.-Planet., 111, E05001, https://doi.org/10.1029/2005JE002607, 2006. 
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Short summary
Our detailed investigation of Martian gullies formed in different substrates in 29 craters distributed between 30°–75° S latitude suggests that they can be differentiated from one another in terms of (1) morphology and length of alcoves and (2) mean gradient of the gully fans. The comparison between the Melton ratio, alcove length, and fan gradient of Martian and terrestrial gullies suggests that Martian gullies were likely formed by terrestrial debris-flow-like processes in the past.