Potential Effects of Atmospheric Collapse on Martian Heat Flow and Application to the InSight Measurements
Nicholas Attree, Narissa Patel, Axel Hagermann, Matthias Grott, Tilman, Spohn, Matthew Siegler

TL;DR
This study models how past atmospheric collapses on Mars could influence current heat flow measurements, suggesting that such effects are minor but potentially detectable with precise instrumentation like InSight.
Contribution
The paper introduces a numerical model to estimate the impact of atmospheric pressure changes on Martian heat flow measurements, highlighting the potential significance for interpreting InSight data.
Findings
Atmospheric collapse could increase heat flow by up to 8%.
The effect is within the measurement error of InSight's HP3 instrument.
Detecting climate perturbations via heat flow remains challenging.
Abstract
Heat flow is an important constraint on planetary formation and evolution. It has been suggested that Martian obliquity cycles might cause periodic collapses in atmospheric pressure, leading to corresponding decreases in regolith thermal conductivity (which is controlled by gas in the pore spaces). Geothermal heat would then build up in the subsurface, potentially affecting present-day heat flow - and thus the measurements made by a heat-flow probe such as the InSight HP instrument. To gauge the order of magnitude of this effect, we model the diffusion of a putative heat pulse caused by thermal conductivity changes with a simple numerical scheme and compare it to the heat-flow perturbations caused by other effects. We find that an atmospheric collapse to 300 Pa in the last 40 kyr would lead to a present-day heat flow that is up to larger than the average geothermal…
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