Green Valley (Mars)
Coordinates | 68°21′N 233°00′E / 68.35°N 233°E |
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Naming | Informal name based on danger assessment map color |
Green Valley is a region on Mars within Vastitas Borealis that was chosen as the landing site of NASA's Phoenix lander. It is located at 68.35 degrees north, 233 degrees east. The valley is about 50 kilometres wide, but only about 250 metres deep; either it was filled in, or was never any deeper than that. The edges are not visible from the middle of the valley.[1]
The name "Green Valley" is not officially recognised by the International Astronomical Union. It came from the decision process by which it was selected as Phoenix's landing site: prospective landing areas were color-coded based on how hazardous they were, with red being most hazardous through yellow to green being the safest.[1] Green Valley has relatively few of the large boulders that could have tipped the lander if it had hit one during touchdown.[2]
The ground within Green Valley is covered with polygonal features several metres across and roughly ten centimetres high, thought to be caused either by thermal contraction (ice-wedge polygons) or by the effects of wind-blown dust (sand-wedge polygons). Water ice is thought to be just below the surface.[1] During the local winter as much as three feet of carbon dioxide ice is expected to appear on the surface.[3]
Shortly before Phoenix's scheduled landing, the Mars Reconnaissance Orbiter photographed a pair of kilometer-tall dust devils in the Green Valley area.[4]
References
[edit]- ^ a b c A Green Valley for Phoenix – Planetary News | The Planetary Society Archived 13 May 2008 at the Wayback Machine
- ^ Mars lander aims for touchdown in 'Green Valley' – space – 11 April 2008 – New Scientist Space
- ^ SPACE.com – Phoenix Lander Readied For Mars Exploration
- ^ Dust devils spotted at Mars probe's landing site – space – 7 May 2008 – New Scientist Space
Further reading
[edit]- Arvidson; et al. (2008). "Mars Exploration Program 2007 Phoenix landing site selection and characteristics". Journal of Geophysical Research. 113 (E6): E00A03. Bibcode:2008JGRE..113.0A03A. doi:10.1029/2007JE003021.