Constrain the processes driving present-day gully modification at Sisyphi Cavi

Establish which physical mechanism drives present-day gully modification at Sisyphi Cavi among competing processes involving CO2 ice, H2O ice, CO2-ice-driven fluidization, and avalanche-like granular flows.

Background

The paper evaluates several competing explanations for contemporary gully activity, including liquid-water or water-ice processes, CO2 geysers beneath translucent ice, CO2-ice fluidization, and avalanche or granular-flow mechanisms. The observations exclude neither every possible CO2-based process nor all combinations of ice and substrate effects.

The authors find no evidence for independently exposed H2O ice and identify a temporal mismatch between CO2 geyser indicators and gully modification. They therefore favor late-season CO2-ice-driven fluidization or avalanche processes, but do not claim that the mechanism has been definitively established.

References

The processes driving this activity remain incompletely constrained, with several competing hypotheses involving CO2 ice , H2O ice, or a combination of both.

— Properties of Seasonal Ice at Sisyphi Cavi and Implications for Current Modification of Martian Gullies  (2609.03885 - Leclef et al., 3 Sep 2026) in Conclusion, opening paragraph