Difference between revisions of "Ismenius Lacus quadrangle"

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File: Image:Mamers Valles Cliff.jpg|Wide view of [[Mamers Vallis]] with cliffs, as seen by [[HiRISE]]
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File: Mamers Valles Cliff.jpg|Wide view of [[Mamers Vallis]] with cliffs, as seen by [[HiRISE]]
File: Image:Mamers Valles Smooth Cliff.JPG|Smooth cliff of Mamers Valles.  Note the lack of boulders.  Much of the surface may have just been blown in or dropped from the sky (as dirty frost).  Image from HiRISE.
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File: Mamers Valles Smooth Cliff.JPG|Smooth cliff of Mamers Valles.  Note the lack of boulders.  Much of the surface may have just been blown in or dropped from the sky (as dirty frost).  Image from HiRISE.
File: Image:Mamers Valles Layer Deposit.JPG|Layered deposit in Mamers Valles, as seen by HiRISE.
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File: Mamers Valles Layer Deposit.JPG|Layered deposit in Mamers Valles, as seen by HiRISE.
 
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File:ESP 053420 2160inverted channel.jpg|Possible inverted channel,  as seen by HiRISE under HiWish program  
 
File:ESP 053420 2160inverted channel.jpg|Possible inverted channel,  as seen by HiRISE under HiWish program  
 
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==See also==
 
==See also==

Revision as of 08:32, 7 March 2020

Mars topography (MOLA dataset) HiRes (1).jpg
MC-05 Ismenius Lacus 30–65° N 0–60° E Quadrangles Atlas


This quadrangle has some of the most mysterious-looking landscapes on the planet. It truly looks like another world here. The Ismenius Lacus quadrangle contains regions called Deuteronilus Mensae and Protonilus Mensae, two places that are of special interest to scientists. They contain abundant evidence of present and past glacial activity. They also have a landscape unique to Mars, called Fretted terrain. The largest crater in the area is Lyot Crater, which contains channels probably carved by liquid water.Cite error: Closing </ref> missing for <ref> tag The Ismenius Lacus quadrangle contains parts of regions named Acidalia Planitia, Arabia Terra, Vastitas Borealis, and Terra Sabaea.[1]

Origin of names

Ismenius Lacus is the name of a classical albedo feature located at 40° N and 30° E on Mars. The term is Latin for Ismenian Lake, and refers to the Ismenian Spring near Thebes in Greece where Cadmus slew the guardian dragon. Cadmus was the legendary founder of Thebes, and had come to the spring to fetch water. The name was approved by the International Astronomical Union (IAU) in 1958.[2] All names suggested for astronomical features have to eventually approved by the International Astronomical Union (IAU). Some important areas in this quadrangle derive from the names of canals that some early astronomers saw in this broad area. One such large canal they called Nilus. Since 1881–1882 it was split into other canals, some were called Nilosyrtis, Protonilus (first Nile),and Deuteronilus (second Nile).[3]

Channels (Rivers)

Many features were probably rivers with water flowing in them billions of years ago. In eastern Ismenius Lacus, lies Mamers Valles, a giant outflow channel.


The channel shown below goes quite a long distance and has branches. It ends in a depression that may have been a lake at one time. The first picture is a wide angle, taken with CTX; while the second is a close up taken with HiRISE.[4]


See also

References

  1. http://planetarynames.wr.usgs.gov/SearchResults?target=MARS&featureType=Terra,%20terrae
  2. USGS Gazetteer of Planetary Nomenclature. Mars. http://planetarynames.wr.usgs.gov/.
  3. Blunck, J. 1982. Mars and its Satellites. Exposition Press. Smithtown, N.Y.
  4. http://www.uahirise.org/ESP_039997_2170