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Icaria Planum

Coordinates:39°40′S130°00′W / 39.667°S 130.000°W /-39.667; -130.000
From Wikipedia, the free encyclopedia
Planum on Mars

Icaria Planum
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MOLA colorized relief map showing boundaries of Icaria Planum and other regions
Feature typeRegion
LocationThaumasia quadrangle,Mars
Coordinates39°40′S130°00′W / 39.667°S 130.000°W /-39.667; -130.000[1]
EponymIkaria
Crater and one of many nearby channels, as seen by HiRISE under HiWish program. Picture is from Icaria Planum.

Icaria Planum is a region on Mars in theThaumasia quadrangle. It is located roughly south-southwest of theTharsis Rise. Icaria Planum is named after the island ofIkaria, where, according toGreek mythology,Icarus fell and died in the sea.[1]

Icaria Planum is relatively ancient and cratered, with an estimated age of 3.59 billion years.[2]: 31  Some subsequent volcanic resurfacing occurred ~0.94 billion years ago, in theMiddle Amazonian period.[3] Icaria Planum hosts numerous wrinkle ridges, a class of compressionalfaults thought to have formed from stresses in the Martian crust. The wrinkle ridges in Icaria Planum formed roughly 3.46 billion years ago and are largely concentric to the Tharsis Rise, likely due to the immense weight of the emplaced volcanic material as Tharsis formed.[4] Icaria Planum hosts analluvial fan, likely due to the breach of an ancient paleolake from an impact crater close to the nearbyClaritas Fossae.[5]

  • CTX image from Icaria Planum that shows location of next image.
    CTX image from Icaria Planum that shows location of next image.
  • Layers in mantle deposit, as seen by HiRISE, under the HiWish program. Mantle was probably formed from snow and dust falling during a different climate.
    Layers in mantle deposit, as seen by HiRISE, under theHiWish program. Mantle was probably formed from snow and dust falling during a different climate.

See also

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References

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  1. ^ab"Icaria Planum".Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program. (Center Latitude: -39.67°, Center Longitude: 230.00°)
  2. ^Leone, Giovanni, ed. (27 October 2021).Mars: A Volcanic World (1st ed.). Springer Cham.Bibcode:2021mvw..book.....L.doi:10.1007/978-3-030-84103-4.ISBN 978-3-030-84102-7. Retrieved29 April 2024.
  3. ^Platz, Thomas; Michael, Gregory; Tanaka, Kenneth L.; Skinner, James A.; Fortezzo, Corey M. (July 2013). "Crater-based dating of geological units on Mars: Methods and application for the new global geological map".Icarus.225 (1):806–827.Bibcode:2013Icar..225..806P.doi:10.1016/j.icarus.2013.04.021.
  4. ^Ruj, Trishit; Kawai, Kenji (November 2021)."A global investigation of wrinkle ridge formation events; Implications towards the thermal evolution of Mars".Icarus.369.Bibcode:2021Icar..36914625R.doi:10.1016/j.icarus.2021.114625.
  5. ^Raitala, J.; Korteniemi, J.; Aittola, M.; Kostama, V. -P.; Hauber, E.; Kronberg, P.; Neukem, G. (March 2006).Fluvial Activity Resulted in Alluvial Fan in Icaria Planum, Mars. 37th Annual Lunar and Planetary Science Conference. League City, Texas, United States.Bibcode:2006LPI....37.1299R. 1299.
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