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EXCERPT:
Mars has lots of glaciers located along its mid-latitudes. We’ve known this for years thanks to the Mars Reconnaissance Orbiter’s (MRO’s) SHARAD sounder. But, despite all of the excellent data it’s managed to gather, SHARAD doesn’t have high enough resolution to accurately measure the boundary between the glacier itself and the rocky material that has been deposited on top of it over the course of billions of years. A new study, published in the journal JGR Planets, details a potential method of finding that boundary—by using a drone.
So what exactly does that boundary matter? Debris-covered glaciers (or DCGs) are a common feature on Mars. The debris that rests on top of them stops the sublimation that would otherwise cause the entire glacier to disappear into Mars’ thin atmosphere. But, we aren’t entirely sure how deeply buried these glaciers are. And if we’re to utilize the water they hold, either for direct astrobiological study or in-situ resource utilization (ISRU), we need a better idea of how much rock and dirt we have to dig through in order to access them.
SHARAD is great for tracking big macro features over the surface of the planet. But it’s not great for the nitty-gritty details of how much regolith actually covers a specific glacier. This is largely due to the fact that it’s around 300 kilometers away. In order to get that fine level of detail, we need something closer.
