Exploration of A Magma-Sediment Hydrothermal System on Earth: Constraints on the Habitability Potential of Martian Noachian Hydrothermal Systems
The martian crust is predominantly composed of basalt [1] and hosts a large variety of alteration materials caused by wide-ranging processes from volcanic hydrothermal processes to sedimentary and post-magmatic (e.g., see [2] and reference within). Specifically, there is an abundance of evidence that water previously flowed on Mars, ranging from ancient stream beds [3], lake basins [4], sedimentary fans in Jezero crater [5, 6], and clay minerals [7]. These secondary minerals have been observed by landers and rovers [2], from orbit [8], and in martian meteorites [9-11]. Along with low temperature alteration, high temperature hydrothermal systems from volcanic processes, as well as meteorite impacts, should have been present [12,13]. However, finding evidence of high-temperature hydrothermal activity has been challenging. To better understand these processes on Mars, Earth analogs can be used and then compared to potential scenarios and locations on Mars. Therefore, here we investigate a mafic dike and the surrounding metamorphic contact zone that has been hydrothermally altered from contact with ground water as it was emplaced. We will also compare our results to previous work on Robbers Roost Dike, an older mafic dike near our field location that intruded a similar protolith causing a potentially habitable hydrothermal system [14. 15].