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List of extraterrestrial dune fields

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Tree-like dunes on Mars. Groups of dark brown streaks have been photographed by theMars Reconnaissance Orbiteron melting pinkish sand dunes covered with light frost. The image was taken near the North Pole of Mars, spring 2010. Objects about 25 centimetres across are resolved on this image, which is about one kilometre wide. Close ups of some parts of this image show billowing plumes indicating that the sand slides were occurring at the time of the photo; see center left.

This is alist ofdune fieldsnot on Earthwhich have been given official names by theInternational Astronomical Union.Dune fields are named according to the IAU's rules ofplanetary nomenclature.The relevant descriptor term isundae.As of now, the only twoSolar Systemplanets, besides Earth, with named dune fields areVenusandMars.Dune fields have also been discovered onSaturn's moonTitan,[1]Pluto[2][3]and comet67P/Churyumov–Gerasimenko.[4]

Venus[edit]

There are three officially named dune fields on Venus. They are named after desert goddesses, as per the IAU's rules. They are listed below.

Mars[edit]

Dunes in Abalos Undae, Mars appear blueish due to basalt, while the reddish-white areas may be dust.

There are six officially named dune fields on Mars, which are named after nearbyclassical albedo featuresin accordance with the IAU's rules. Five of them lie between 75°N to 85°N, betweenPlanum BoreumandVastitas Borealis.These dune fields span over 200 degrees of longitude. The sixth, Ogygis Undae, lies on the southern hemisphere of Mars. They are listed below.

Unofficial field names[edit]

Namib sand dune (downwind side) on Mars
(Curiosityrover;17 December 2015).
  • Bagnold dune field, Gale crater. This dune field was explored byCuriositybetween initially between mission Sols ~1174–1248, where the rover investigated High dune, and Namib dune. Three orders of bedform were identified: wind ripple, large ripple (or wind drag ripple[6]) and dune.[7]Sand grains in this section of the dune field had a modal grain size of 120 μm[8]
  • Namib dune, Gale crater. This is a prominent feature that looks like the giant dunes of Africa’s Namib Desert.[9]
  • As part of theMars Exploration Rovermission, a small dune field unofficially named El Dorado on the south side ofHusband HillinGusev craterwas investigated by theSpiritroverfromsols706 to 710.[10]Analysis of El Dorado showed that it consists of black wind-blown sand which is "well-sorted, well-rounded andolivinerich.[11]
Detail of the dunes of the Hagal Dune Field

Titan[edit]

There are five officially named dune fields on Titan, which are named after Greek gods, goddesses or personifications of wind. They are listed below:[12]

Literature also uses names of dark albedo features when referring to Titan's dune fields:

Pluto[edit]

Dune fields in Sputnik Planitia near Planitia

Analysis of high resolution photos fromNew Horizonstaken on 14 July 2015 of Pluto'sSputnik Planumregion in 2018 has confirmed the presence oftransverse dunes(perpendicular to the wind streaks) within the cellular nitrogen plains, spaced about 0.4 to 1 km apart, that are thought to be composed of 200-300 μm diameter particles of methane ice believed to be derived from the nearbyAl-Idrisi Montes.[2][3]These features are yet to be formally named.

References[edit]

  1. ^"Titan's Seas Are Sand, Cassini's Images Of Saturn's Moon Show".Retrieved22 April2021.
  2. ^abTelfer, M.W.; Parteli, E.R.J.; Radebaugh, J.; et al. (1 June 2018)."Dunes on Pluto".Science.360(6392): 992–997.Bibcode:2018Sci...360..992T.doi:10.1126/science.aao2975.PMID29853681.
  3. ^abHayes, A.G. (1 June 2018). "Dunes across the Solar System".Science.360(6392): 960–961.Bibcode:2018Sci...360..960H.doi:10.1126/science.aat7488.PMID29853671.S2CID44138724.
  4. ^Jia, P.; B. Andreotti; P. Claudin (March 2017)."Giant ripples on comet 67P/Churyumov–Gerasimenko sculpted by sunset thermal wind".Proceedings of the National Academy of Sciences.114(10): 2509–2514.arXiv:1703.02592.Bibcode:2017PNAS..114.2509J.doi:10.1073/pnas.1612176114.PMC5347604.PMID28223535.
  5. ^"USGS Gazetteer of Planetary Nomenclature: Abalos Undae".Retrieved8 August2007.
  6. ^Lapotre, M. G. A.; Ewing, R. C.; Lamb, M. P.; Fischer, W. W.; Grotzinger, J. P.; Rubin, D. M.; Lewis, K. W.; Ballard, M. J.; Day, M. (1 July 2016)."Large wind ripples on Mars: A record of atmospheric evolution".Science.353(6294): 55–58.Bibcode:2016Sci...353...55L.doi:10.1126/science.aaf3206.ISSN0036-8075.PMID27365444.
  7. ^Ewing, R. C.; Lapotre, M. G. A.; Lewis, K. W.; Day, M.; Stein, N.; Rubin, D. M.; Sullivan, R.; Banham, S.; Lamb, M. P. (2017)."Sedimentary processes of the Bagnold Dunes: Implications for the eolian rock record of Mars".Journal of Geophysical Research: Planets.122(12): 2544–2573.Bibcode:2017JGRE..122.2544E.doi:10.1002/2017je005324.ISSN2169-9097.PMC5815379.PMID29497590.
  8. ^Ehlmann, B. L.; Edgett, K. S.; Sutter, B.; Achilles, C. N.; Litvak, M. L.; Lapotre, M. G. A.; Sullivan, R.; Fraeman, A. A.; Arvidson, R. E. (2017)."Chemistry, mineralogy, and grain properties at Namib and High dunes, Bagnold dune field, Gale crater, Mars: A synthesis of Curiosity rover observations".Journal of Geophysical Research: Planets.122(12): 2510–2543.Bibcode:2017JGRE..122.2510E.doi:10.1002/2017je005267.ISSN2169-9097.PMC5815393.PMID29497589.
  9. ^Sandoval, Greg (9 February 2016)."NASA's updated 360-degree view from Mars offers clear look at giant Namib Dune".GeekWire.
  10. ^"Mars Exploration Rovers Update: Spirit Descends Husband Hill as Opportunity Works at a Standstill on Olympia".Retrieved21 November2006.
  11. ^"Recent results from the Spirit rover at Gusev crater"(PDF).Retrieved21 November2006.
  12. ^"USGS Gazetteer of Planetary Nomenclature: Search: TITAN: Unda, undae".Retrieved9 December2018.
  13. ^abcArnold, K.; J. Radebaugh; C. J. Savage; E.P. Turtle; R.D. Lorenz; E.R. Stofan; A. Le-Gall & the Cassini Radar Team."Areas of Sand Seas on Titan from Cassini Radar and ISS: Fensal and Aztlan"(PDF).42nd Lunar and Planetary Science Conference, March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608.Lunar and Planetary Institute. p. 2804.
  14. ^abLe Gall, A.; M.A. Janssen; L.C. Wye; J. Radebaugh; R.D. Lorenz & the Cassini Radar Team (September 2010)."Regional variations among Titan's dunes: Belet versus Fensal dune fields"(PDF).European Planetary Science Congress 2010 Abstracts.5:247.Bibcode:2010epsc.conf..247L.

A large portion of this article was sourced from theGazetteer of Planetary Nomenclature,the official IAU database of planetary names.

  • Ralph Lorenz; James Zimbelman (2014).Dune Worlds: How Wind-blown Sand Shapes Planetary Landscapes.Springer.ISBN978-3-540-89724-8.
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