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Satellites were used to map the crater that developed as the 2.7km-thick overlying ice sheet slumped to fill the void left by the escaping water.
He also conducted field research to map the crater's hydrology.
The researchers also used the orbiter to map the crater's floor and the slope of its walls.
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The CTX image mosaic (base map) was used to map the craters.
Uwingu raises money for space research through campaigns, such as selling naming rights to martian craters on an unofficial Uwingu map (the bigger the crater, the more expensive the name).
The European satellite's radar altimeter was then employed to map the shape of the crater that resulted.
Data for the map of Posidonius Crater was collected by the Lunar Reconnaissance Orbiter Camera.
Mare basalt covers an area of 2400 km2 within the central western portion of the crater and was previously mapped as Imbrian age (Stuart-Alexander, 1978; Wilhelms, 1987).
By convention these features are identified on lunar maps by placing a letter on the side of the crater midpoint that is closest to the primary crater.
Now scientists who have mapped Shackleton Crater with unprecedented detail have found evidence of ice inside the crater.
Substantial processing of the crater floor material due to variety of geological processes is evident in the generated maps, making straight forward interpretations difficult.
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