 Topographic location map of Slipher Crater. | |
| Planet | Mars |
|---|---|
| Coordinates | 47°18′S84°36′W / 47.3°S 84.6°W /-47.3; -84.6 |
| Quadrangle | Thaumasia |
| Diameter | 127 km (79 mi) |
| Eponym | Vesto andEarl Slipher |
Slipher is animpact crater in theThaumasia quadrangle ofMars, located at 47.3°S latitude and 84.6°W longitude. It measures 127 kilometres (79 mi) in diameter and was named after American astronomersVesto andEarl Slipher. The naming was approved by IAU'sWorking Group for Planetary System Nomenclature in 1973.[1]
Gullies are visible on the walls of a crater that is on the rim of Slipher. They can be seen in the pictures below.Martian gullies are small, incised networks of narrow channels and their associated downslopesediment deposits, found on the planet of Mars. They are named for their resemblance to terrestrialgullies. First discovered on images fromMars Global Surveyor, they occur on steep slopes, especially on the walls of craters. Usually, each gully has adendriticalcove at its head, afan-shapedapron at its base, and a single thread of incisedchannel linking the two, giving the whole gully an hourglass shape.[2] They are believed to be relatively young because they have few, if any craters. A subclass of gullies is also found cut into the faces of sand dunes which themselves considered to be quite young.
On the basis of their form, aspects, positions, and location amongst and apparent interaction with features thought to be rich in water ice, many researchers believed that the processes carving the gullies involve liquid water. However, this remains a topic of active research.
As soon as gullies were discovered,[2] researchers began to image many gullies over and over, looking for possible changes. By 2006, some changes were found.[3] Later, with further analysis it was determined that the changes could have occurred by dry granular flows rather than being driven by flowing water.[4][5][6] With continued observations many more changes were found in Gasa Crater and others.[7]
With more repeated observations, more and more changes have been found; since the changes occur in the winter and spring, experts are tending to believe that gullies were formed from dry ice. Before-and-after images demonstrated the timing of this activity coincided with seasonal carbon-dioxide frost and temperatures that would not have allowed for liquid water. When dry ice frost changes to a gas, it may lubricate dry material to flow especially on steep slopes.[8][9][10] In some years frost, perhaps as thick as 1 meter.
