Cassini (Martian crater)

{{Short description|Crater on Mars}}

{{Too many images|date=November 2024}}

{{Infobox crater data

| titlecolor = #FA8072

| title = Cassini Crater

| image = CassiniMartianCrater.jpg

| caption = Location of Cassini Crater

| region = Arabia quadrangle

| coordinate_title = Coordinates

| globe = Mars

| coordinates = {{coord|23.4|N|327.9|W|globe:mars_type:landmark|display=inline,title}}

| diameter = 415 km

| eponym = Giovanni Domenico Cassini

}}

Cassini is a crater on Mars named in honour of the Italian astronomer Giovanni Cassini. The name was approved in 1973, by the International Astronomical Union (IAU) Working Group for Planetary System Nomenclature.{{cite web|title=Gazetteer of Planetary Nomenclature {{!}} Cassini|url=http://planetarynames.wr.usgs.gov/Feature/1046|website=usgs.gov|publisher=International Astronomical Union|access-date=24 August 2017}}

The crater measures approximately 415 kilometers in diameter and can be found at 327.9°W and 23.4°N.{{cite web |url=http://ic.arc.nasa.gov/projects/bayes-group/Atlas/Mars/features/crater/index.html |title=Archived copy |access-date=2007-02-03 |url-status=dead |archive-url=https://web.archive.org/web/20061009234124/http://ic.arc.nasa.gov/projects/bayes-group/Atlas/Mars/features/crater/index.html |archive-date=2006-10-09 }} It is in the Arabia quadrangle of Mars. Pictures of small craters on the floor of Cassini reveal multiple layers. Some of these layers can be easily seen in the pictures below. Many places on Mars show rocks arranged in layers. Rock can form layers in a variety of ways. Volcanoes, wind, or water can produce layers.{{cite web|url=http://hirise.lpl.arizona.edu/?PSP_008437_1750 |title=HiRISE – High Resolution Imaging Science Experiment |publisher=University of Arizona |access-date=2012-08-04}}

A detailed discussion of layering with many Martian examples can be found in Sedimentary Geology of Mars.Grotzinger, J. and R. Milliken (eds.). 2012. Sedimentary Geology of Mars. SEPM.

Recent research leads scientists to believe that some of the craters in Arabia may have held huge lakes. Cassini Crater probably once was full of water since its rim seems to have been breached by the waters. Both inflow and outflow channels have been observed on its rim. The lake would have contained more water than Earth's Lake Baikal, our largest freshwater lake by volume.Fassett, C. and J. Head III. 2008. Valley network-fed, open-basin lakes on Mars: Distribution and implications for Noachian surface and subsurface hydrology. Icarus: 198. 39-56.

Many craters once contained lakes.Cabrol, N. and E. Grin. 2001. The Evolution of Lacustrine Environments on Mars: Is Mars Only Hydrologically Dormant? Icarus: 149, 291-328.Fassett, C. and J. Head. 2008. Open-basin lakes on Mars: Distribution and implications for Noachian surface and subsurface hydrology. Icarus: 198, 37-56.Fassett, C. and J. Head. 2008. Open-basin lakes on Mars: Implications of valley network lakes for the nature of Noachian hydrology.

Image:Cassini crater 378S66.jpg|Oblique view of Cassini and vicinity from Viking Orbiter 1, also showing Pasteur crater (lower left), Indus Vallis (right), Scamander Vallis (bottom), and Arago crater (bottom right corner)

Cassini crater Viking Orbiter 1 mosaic.jpg|Viking Orbiter 1 mosaic

Image:Arabia map.JPG|Map of Arabia quadrangle with major craters. Cassini is in the upper right.

Image:Cassini crater floor.JPG|Crater in the middle of Cassini crater, as seen by HiRISE.

WikicassinilayersESP 028919 2030.jpg|Layers in a crater on the floor of Cassini Crater, as seen by HiRISE, under HiWish program

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|cWidth = 300

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|Description = The surroundings of the Cassini crater.

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See also

References

{{commons category|Cassini (Martian crater)}}

{{Reflist}}

{{Geography of Mars}}

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Category:Impact craters on Mars

Mars

Category:Arabia quadrangle