Holden (Martian crater)

Holden is a 140 km wide crater situated within the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars, located with the southern highlands. It is named after American astronomer Edward Singleton Holden. It is part of the Uzboi-Landon-Morava (ULM) system.

Description

Like Gusev, it is notable for an outlet channel, Uzboi Vallis, that runs into it, and for many features that seem to have been created by flowing water. It's believed that Holden crater was formed by an impact during the Noachian or Hesperian periods.Grant, J. et al. 2008. HiRISE imaging of impact megabreccia and sub-meter aqueous strata in Holden Crater, Mars. Geology: 36, 195-198.

The crater's rim is cut with gullies, and at the end of some gullies are fan-shaped deposits of material transported by water. The crater is of great interest to scientists because it has some of the best-exposed lake deposits. One of the layers has been found by the ''Mars Reconnaissance Orbiter'' to contain clays.

Clays only form in the presence of water. There are two units of sediments in the crater. The lower unit formed in a large lake. It is believed the lake waters originated from the crater walls/or groundwater. Water from the crater walls may have come from precipitation when the Martian climate was different. The upper unit formed when water that was ponded to the south in Uzboi Vallis broke through Holden's rim. It is believed that great amount of water went through the rim; one flow was caused by a body of water larger than Earth's Lake Huron. Some of the evidence for such a large flow of water is the presence of boulders tens of meters in size sticking above the surface. To transport such huge rocks takes a great deal of water.

Holden is an old crater, containing numerous smaller craters, many of which are filled with sediment. The crater's central mountain is also obscured by sediment. Holden crater was a proposed landing site for NASA's Mars Science Laboratory, until Gale crater which contains a large delta. The lower beds of Holden are thought by some to maybe similar to materials in Eberswalde. However, Holden was considered a potential landing site for the Mars 2020 rover. In the second Mars 2020 Landing Site Workshop it survived the cut and was named to be among the top 8 sites in the running for the landing. Despite its promising features, Jezero Crater was ultimately chosen.

Holden Crater Rim.jpg, West rim of Holden crater, as seen by THEMIS.
Holden Crater Close-up.JPG, Close-up of channels on rim of Holden crater, as seen by THEMIS.
26126contextb22 018333 1548delta.jpg, Wide view of a delta in Holden crater, as seen by CTX.
ESP 026126 1530delta.jpg, Close up view of part of delta from the previous image, as seen by HiRISE under HiWish program
26126 1530deltalayers.jpg, Close view of the previous image showing layers, as seen by HiRISE under HiWish program and enlarged with HiView

Geologic history of Holden crater

Studies of the whole region around Holden crater have resulted in an understanding of a complex sequence of events that shaped the crater, which included two different lakes. A large series of rivers called the Uzboi-Ladon-Morava (ULM) system drained water from the Argyre Basin, the site of a large lake. When an impact occurred and produced Holden crater, the system was blocked by a crater rim almost a kilometer in height. Eventually, water from drainage from the walls, with possibly a contribution from groundwater, collected to make the first lake.Cabrol, N. and E. Grin (eds.). 2010. Lakes on Mars. Elsevier. NY This lake was deep and long-lasting. The lowest level of sedimentary rocks was deposited in this lake. Much water was inbounded in Uzboi Vallis because the rim of Holden blocked the flow. Some of the backed-up water came from Nirgal Vallis which had a discharge of 4800 cubic meters/second. At a certain point the stored water broke through the rim of Holden and created a second, shorter-lived lake 200–250 m deep. Water with a depth of at least 50 m entered Holden at a rate that 5-10 times the discharge of the Mississippi River.Grant, J., T. Parker. 2002. Drainage evolution of the Margaritifer Sinus region, Mars. J. Geophysic. Res. 107, doi:10.1029/2001JE001678. Terraces and the presence of large rocks (tens of meters across) support these high discharge rates.

Mars Science Laboratory

Several sites in the Margaritifer Sinus quadrangle were proposed as areas to send NASA's major Mars rover, the Mars Science Laboratory, ''Curiosity''. Holden crater made the cut to be among the top four, although Gale crater, Mawrth Vallis, Miyamoto crater, Nili Fossae trough, and southern Meridiani Planum.
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See also

* List of craters on Mars

References

External links

ESA Mars Express: Crater Holden and Uzboi Vallis

HiRISE image of layers in Holden
*

Lakes on Mars - Nathalie Cabrol (SETI Talks)

High resolution video
by Seán Doran of overflight of Holden (reached about 3/4 of the way through; passes to the right of Hale and Bono earlier)

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Impact craters on Mars
Mars 2020
Margaritifer Sinus quadrangle