Visualizing Shackleton Crater
- Visualizations by:
- Ernie Wright
- View full credits
These computer-generated images are centered on Shackleton, a well-preserved, bowl-shaped crater, 21 kilometers wide and 4 km deep, at the Moon's south pole. Shackleton's floor is in perpetual shadow, but LOLA, the laser altimeter on Lunar Reconnaissance Orbiter, reveals boulders and low hills, or hummocks, formed by material slumping from the crater's sides. Shackleton's cold interior may harbor water ice and other volatiles that would evaporate rapidly if exposed to the Sun. In contrast, some points on the rim of the crater are in persistent sunshine and may be ideal places for solar panels. The ridge on the far side of the crater in this view connects Shackleton's rim to the rim of the adjacent crater Slater. Another ridge, just out of frame on the left, connects to de Gerlache crater. Certain points on these ridges are also in persistent sunshine.
For More Information
See Researchers Estimate Ice Content of Crater at Moon's South Pole (NASA.gov)
Please give credit for this item to:
NASA's Scientific Visualization Studio
- Ernie Wright (USRA) [Lead]
- David Smith (NASA/GSFC)
- Erwan M. Mazarico (NASA/GSFC)
- Gregory A. Neumann (NASA/GSFC)
- Maria Zuber (Massachusetts Institute of Technology)
PapersThis visualization is based on the following papers:
- Zuber et al., Constraints on the volatile distribution within Shackleton crater at the lunar south pole, Nature486, 378-381 (21 June 2012)
MissionsThis visualization is related to the following missions:
SeriesThis visualization can be found in the following series:
Datasets used in this visualization
LRO DEM (A.K.A. Digital Elevation Map) (Collected with the LOLA sensor)
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.
You may also like...