A Martian tale of ice and fire

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Explosive volcanic eruptions on Mars may have transported water to equatorial regions where it froze into thick ice, according to computer simulations of the red planet's ancient history by US and Italian researchers. The authors suggest these eruptions may also have led to conditions that allowed these ice deposits to continue to exist under the surface today, and the findings could be useful in identifying potential sites for exploration in future manned missions. We had thought most of Mars' ice was at its poles, but recent measurements have suggested there is also ice nearer the planet's equator, leading scientists to ponder how it got there. The simulations suggest volcanic eruptions may explain this, releasing steam that then froze in the frosty Martian atmosphere around the equator. If this ice was buried under volcanic debris, it could still be there today, the simulations suggest.

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From: Springer Nature

A Martian tale of ice and fire

Explosive volcanic eruptions on early Mars may have transported water ice to equatorial regions, according to a modelling study in Nature Communications. The authors suggest that these eruptions could have led to conditions that allow these ice deposits to still exist under the surface today, which would expand our knowledge of Mars’ terrain for future exploration.

Mars is known to have an ice-rich surface, but the majority of ice deposits are expected to be found towards the polar regions of the planet. However, recent measurements in equatorial regions have detected elevated levels of near-surface hydrogen, which could indicate the presence of bulk ice below the surface. This raises the question of how this ice originated in this unexpected area, with one potential explanation being explosive volcanic eruptions.

Using a planetary climate model, Saira Hamid and colleagues test this hypothesis by simulating explosive volcanic eruptions that are known to have occurred on Mars between 4.1 and 3 billion years ago. The modelling suggests that water vapor released during the eruptions could have frozen in the cold Martian atmosphere, triggering ice precipitation and leading to an accumulation of up to five-metre-thick ice deposits on the Martian surface during a single three-day eruptive event. This ice could have persisted for long periods if buried under dust or volcanic debris, meaning that it could still be present below the surface of equatorial regions. In addition, the researchers suggest that the release of sulfuric acid into the Martian atmosphere during volcanically active periods may have plunged the planet into a global winter, in turn allowing for the accumulation of ice for a sustained period.

The conditions predicted by these models in the event of multiple volcanic eruptions over time could help explain the detections of elevated near-surface hydrogen in the equatorial regions of Mars, with implications for human exploration of the red planet.

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conference:
Nature Communications
Research:Paper
Organisation/s: Arizona State University, USA
Funder: Based upon work supported by the National Science Foundation Graduate Research Fellowship under Grant No. 026257- 001 to S.S.H. and NASA Solar SystemWorkings Grant 20-SSW20-0086 to L.K.
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