Gas flow in Martian spider formation

TL;DR

This paper investigates the mechanisms of gas flow in Martian spider formations, concluding that gas likely flows through gaps between the ice and regolith rather than solely through permeable regolith, influencing spider morphology.

Contribution

It provides a quantitative analysis supporting gas flow through ice-regolith gaps over porous regolith in Martian spiders, constraining regolith properties affecting their formation.

Findings

Gas flows mainly through ice-regolith gaps, not porous regolith.

Gap sizes of about a centimeter can support observed flow rates.

Regolith cohesion influences the erosion and morphology of spiders.

Abstract

Martian araneiform terrain, located in the Southern polar regions, consists of features with central pits and radial troughs which are thought to be associated with the solid state greenhouse effect under a CO$_{2}$ ice sheet. Sublimation at the base of this ice leads to gas buildup, fracturing of the ice and the flow of gas and entrained regolith out of vents and onto the surface. There are two possible pathways for the gas: through the gap between the ice slab and the underlying regolith, as proposed by Kieffer et al (2007), or through the pores of a permeable regolith layer, which would imply that regolith properties can control the spacing between adjacent spiders, as suggested by Hao et al. We test this hypothesis quantitatively in order to place constraints on the regolith properties. Based on previously estimated flow rates and thermophysical arguments, we suggest that there is insufficient depth of porous regolith to support the full gas flow through the regolith. By contrast, free gas flow through a regolith--ice gap is capable of supplying the likely flow rates for gap sizes on the order of a centimetre. This size of gap can be opened in the centre of a spider feature by gas pressure bending the overlying ice slab upwards, or by levitating it entirely as suggested in the original Kieffer et al (2007) model. Our calculations therefore support at least some of the gas flowing through a gap opened between the regolith and ice. Regolith properties most likely still play a role in the evolution of spider morphology, by regolith cohesion controlling the erosion of the central pit and troughs, for example.