Subtype
Recurring slope lineae that are observed to grow incrementally and also recur in multiple Mars years (McEwen et al. 2011c; Ojha et al. 2014).
Formation
Slope lineae is a descriptive term not implying any particular formation mechanism. Slope lineae are typically possible recurring slope lineae.
Age
Recent features, forming currently, under the present climate.
Studied Locations
Asimov crater (Fig. 1), Cerberus Fossae (Fig. 2); for other locations, see recurring slope lineae.
References
McEwen A, Ojha L, Dundas C, Mattson S, Byrne S, Wray J, Cull S (2011a) Transient slope lineae: evidence for summertime briny flows on Mars? 42nd Lunar Planet Sci Conf, abstract #2314, Houston
McEwen AS, Ojha L, Dundas CM, Mattson SS, Byrne S, Wray JJ, Cull SC, Murchie SL, Thomas N, Gulick VC (2011b) Seasonal flows on warm Martian slopes. Science 333:740–743
McEwen AS, Ojha L, Dundas CM, Mattson SS, Byrne S, Wray JJ, Cull SC, Murchie SL, Thomas N, Mass M (2011c) Recurring slope lineae: warm-season incremental flows in the middle southern latitudes of Mars. In: Fifth Mars polar science conference #6017
Ojha L, McEwen A, Dundas C, Byrne S, Mattson S, Wray J, Masse M, Schaefer E (2014) HiRISE Observations of Recurring Slope Lineae (RSL) during southern summer on Mars. Icarus 231:65–376. doi:http://dx.doi.org/10.1016/j.icarus.2013.12.021
Runyon KD, Davatzes AK, Gulick VC (2012) Putative active brine flows in the Cerberus Fossae, Mars. 42rd Lunar Planet Sci Conf, abstract #2072, Houston
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Runyon, K., Ojha, L., Hargitai, H. (2014). Slope Lineae. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_632-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_632-1
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