Image: A peppering of craters at the Moon's south pole

May 26, 2014
Credit: ESA/SMART-1/AMIE camera team; image mosaic: M. Ellouzi/B. Foing

(Phys.org) —The dark and shadowed regions of the Moon fascinate astronomers and Pink Floyd fans alike. Our Moon's rotation axis has a tilt of 1.5º, meaning that some parts of its polar regions never see sunlight – the bottoms of certain craters, for example, are always in shadow.

Imaged during summertime in the Moon's southern hemisphere by the Advanced Moon Imaging Experiment on ESA's SMART-1 spacecraft, this mosaic shows a crater-riddled region spanning the lunar south pole. It is made up of around 40 individual images taken between December 2005 and March 2006, and covers an area of about 500 x 150 km.

The craters visible here include (from right to left, starting with the largest round shape visible in the frame) the Amundsen, Faustini, Shoemaker, Shackleton and de Gerlache craters. Click here for an annotated map.

Amundsen is the largest of the bunch at 105 km across, followed by Shoemaker (50 km), Faustini (39 km), de Gerlache (32 km) and Shackleton (19 km). This group of craters all look different, see varying levels of sunlight and display a range of interesting properties.

Shackleton crater, the small circle visible to the left of centre, contains the south pole within its rim. By using SMART-1 images to explore the number of small scattered on the smooth, dark surface surrounding Shackleton, scientists have found this crater to be older than the Apollo 15 landing site (3.3 billion years), but younger than the Apollo 14 site (3.85 billion years).

Shoemaker crater, visible to the upper left of centre, is notable because of the 1999 Lunar Prospector mission, which deliberately crashed into the crater in an attempt to create a detectable plume of water vapour by heating any that may have been present. No vapour was spotted. However, all is not lost; some permanently shadowed regions have been in the dark for millions of years, and it is still possible that they may contain water ice deposited by comets and water-rich asteroids.

Studying the dark depths of these craters could tell us not just about the history of the Moon, but also about Earth, helping us to understand better how, and how much, water and organic material may have been transferred from the Moon to Earth over its history.

Explore further: Cascading dunes in a Martian crater

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User comments : 1

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rockwolf1000
not rated yet May 27, 2014
"Our Moon's rotation axis has a tilt of 1.5º, meaning that some parts of its polar regions never see sunlight – the bottoms of certain craters, for example, are always in shadow."

I fail to see how the axial tilt has anything to do with how much sunlight it receives. Earth has a much higher axial tilt and all regions get pretty much the same amount of daylight yearly. Now, IF the axial tilt was somehow tidally locked to the sun then it would be possible for the polar region tilted away from the sun would be continually dark, but this is not the case.

Craters near the poles are different story however.

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