Moon pits could be portals to ‘kilometres’ of underground tunnels (Wired UK)


Hundreds of pits discovered on the Moon could be portals to
underground tunnels formed by lava flows, a new paper published in the journal Icarus has suggested.

Ranging from between five to 900 metres in diameter, the pits
could offer shelter to explorers in future and also help us peek
beneath the lunar surface.

Detected using a computer algorithm that analysed the way
shadows fall across the Moon’s surface in photos from Nasa’s Lunar
Reconnaissance Orbiter. Just 40 percent of the Moon has been
photographed with the correct level of lighting for the algorithm
to work, meaning there could be hundreds more yet undiscovered.

“A habitat placed in a pit would provide a very safe location
for astronauts: no radiation, no micrometeorites, possibly very
little dust, and no wild day-night temperature swings,” said the paper’s lead author, Robert Wagner of Arizona State

On Earth, underground lava flows sometimes leave behind
extensive tunnel networks that can become accessible if a section
of the roof caves in. Similar processes on the Moon could have
caused by what are called “impact melt ponds”.

Robert Wagner/Icarus

In essence, the energy from a meteoroid impact can heat and melt
rock, which then takes thousands of years to cool. Before it cools,
the molten rock can flow, creating features similar to those
created by volcanoes on Earth.

One feature could be underground tunnels stretching for
kilometres, the paper suggests.

“Pits represent evidence of subsurface voids of unknown extents.
By analogy with terrestrial counterparts, the voids associated with
mare pits may extend for hundreds of metres to kilometres in
length, thereby providing extensive potential habitats and access
to subsurface geology,” it reads.

The majority of the 231 pits are found in impact craters, but a
small number were found in the “maria”, which are the Moon’s large
dark patches.

The maria, once thought to be the Moon’s seas, were created by
large ancient lava flows that occurred before the Moon cooled,
rather than by meteorite impacts.

Pits found in the maria could help us better understand how the
maria formed, said Wagner: “We’ve taken images from orbit looking
at the walls of these pits, which show that they cut through dozens
of layers, confirming that the maria formed from lots of thin
flows, rather than a few big ones. Ground-level exploration could
determine the ages of these layers, and might even find solar wind
particles that were trapped in the lunar surface billions
of years ago.”

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