Shallow craters on Moon and Mercury may hide thick ice slabs
These findings could have positive consequences for any future human explorers
An artist’s depiction of permanently shadowed craters near the Moon’s south pole. Image credit: UCLA/NASA
Would-be moon explorers are eager to learn better tactics for tracking down ice, which they hope to turn into water and rocket fuel – and new research may have found a new key to spotting buried ice.
The research focused on both the Moon and Mercury, the tiny innermost planet, and pulled together from two crucial NASA missions: the Lunar Reconnaissance Orbiter (LRO) still circling the Moon and the Mercury Surface, Space Environment, Geochemistry and Ranging (MESSENGER) mission that ended its time at the planet in 2015. Scientists believe both bodies hide water ice near their poles, where the bottom of craters never see sunlight – and the ice lurking at the south pole of the Moon is particularly intriguing.
“If confirmed, this potential reservoir of frozen water on the moon may be sufficiently massive to sustain long-term lunar exploration,” Noah Petro, Lunar Reconnaissance Orbiter Project Scientist at NASA’s Goddard Space Flight Center in Maryland, United States, said in a statement.
All told, the scientists behind the new research looked at about 14,000 craters on the two small, grey bodies. Scientists have spotted thick deposits of water ice below the surface near the poles of Mercury. They’re less confident that lunar ice is as slab-like in structure – previous research has suggested the ice here is more mixed.
Artist’s impression of the BepiColombo mission at Mercury. Image credit: Astrium
So the team decided to compare data between Mercury and the Moon to try to better understand what the ice beneath the moon’s poles might look like. By looking at more than 2,000 craters on Mercury, they realised that the craters that seem to hide thick slabs of ice also sport shallower sides than those that don’t.
Then, the researchers turned their sights on the Moon, and found that at the south pole, where previous researchers had identified buried ice, craters tend to be shallower. But that isn’t the case at the Moon’s north pole, which also sports less water overall. The researchers think that combination may reflect a loss of ice near the north pole.
Scientists’ next intensive mission to Mercury, dubbed BepiColombo, is on its way but won’t reach the tiny planet until 2025. But the Moon, so convenient to Earth, will likely see new robots – and possibly even astronauts – touching down before BepiColombo’s arrival. Such missions could help scientists decode the story of lunar water ice.
The research is described in a paper published 22 July 2019 in the journal Nature Geoscience.
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