Difference between revisions of "Medusae Fossae"

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The '''Medusae Fossae Formation''' is a large geological formation of probable volcanic origin on the planet [[Mars]].<ref name=esa-mff>{{cite web|title=The Medusa Fossae formation on Mars|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/The_Medusa_Fossae_formation_on_Mars/(print)|publisher=[[European Space Agency]]|date=29 March 2005}}</ref>
 
The '''Medusae Fossae Formation''' is a large geological formation of probable volcanic origin on the planet [[Mars]].<ref name=esa-mff>{{cite web|title=The Medusa Fossae formation on Mars|url=http://www.esa.int/Our_Activities/Space_Science/Mars_Express/The_Medusa_Fossae_formation_on_Mars/(print)|publisher=[[European Space Agency]]|date=29 March 2005}}</ref>
  
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It is named for the [[Medusa (mythology)|Medusa]] of Greek mythology. "Fossae" is Latin for "trenches".  
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It is named for the [[Medusa (mythology)|Medusa]] of Greek mythology. "Fossae" is Latin for "trenches".  
 
The formation is a collection of soft, easily eroded deposits that extends off and on for more than 5,000&nbsp;km along the equator.
 
The formation is a collection of soft, easily eroded deposits that extends off and on for more than 5,000&nbsp;km along the equator.
  
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Its density and high content of sulfur and chlorine, suggests an explosive volcanic origin. It may have been deposited in periodic eruptions over an interval of 500 million years.<ref name="Ojha2018a">{{cite journal |doi=10.1029/2018JE005565 |title=The Density of the Medusae Fossae Formation: Implications for its Composition, Origin, and Importance in Martian History |journal=Journal of Geophysical Research: Planets |volume=123 |issue=6 |pages=1368–1379 |year=2018 |last1=Ojha |first1=Lujendra |last2=Lewis |first2=Kevin |bibcode=2018JGRE..123.1368O |doi-access=free }}</ref>
 
Its density and high content of sulfur and chlorine, suggests an explosive volcanic origin. It may have been deposited in periodic eruptions over an interval of 500 million years.<ref name="Ojha2018a">{{cite journal |doi=10.1029/2018JE005565 |title=The Density of the Medusae Fossae Formation: Implications for its Composition, Origin, and Importance in Martian History |journal=Journal of Geophysical Research: Planets |volume=123 |issue=6 |pages=1368–1379 |year=2018 |last1=Ojha |first1=Lujendra |last2=Lewis |first2=Kevin |bibcode=2018JGRE..123.1368O |doi-access=free }}</ref>
  
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The surface of the formation has been eroded by the wind into a series of linear ridges called [[yardang]]s.<ref>{{cite book |doi=10.2110/pec.12.102.0169 |chapter=Duststones on Mars: Source, Transport, Deposition, and Erosion |title=Sedimentary Geology of Mars |pages=169–182 |year=2012 |last1=Bridges |first1=Nathan T. |last2=Muhs |first2=Daniel R. |isbn=978-1-56576-312-8 }}</ref> These ridges generally point in direction of the [[prevailing winds]] that carved them, and demonstrate the erosive power of Martian winds. The easily eroded nature of the Medusae Fossae Formation suggests that it is composed of weakly cemented particles, and was most likely formed by the deposition of wind-blown dust or [[volcanic ash]].
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The surface of the formation has been eroded by the wind into a series of linear ridges called [[yardang]]s.<ref>{{cite book |doi=10.2110/pec.12.102.0169 |chapter=Duststones on Mars: Source, Transport, Deposition, and Erosion |title=Sedimentary Geology of Mars |pages=169–182 |year=2012 |last1=Bridges |first1=Nathan T. |last2=Muhs |first2=Daniel R. |isbn=978-1-56576-312-8 }}</ref> These ridges generally point in direction of the prevailing winds that carved them, and demonstrate the erosive power of Martian winds. The easily eroded nature of the Medusae Fossae Formation suggests that it is composed of weakly cemented particles, and was most likely formed by the deposition of wind-blown dust or volcanic ash.
  
 
Yardangs are parts of rock that have been sand blasted into long, skinny ridges by bouncing sand particles blowing in the wind.<ref>{{cite web | url=http://www.uahirise.org/ESP_039563_1730 | title=HiRISE &#124; Yardangs in Arsinoes Chaos (ESP_039563_1730) }}</ref> Layers are seen in parts of the formation.  
 
Yardangs are parts of rock that have been sand blasted into long, skinny ridges by bouncing sand particles blowing in the wind.<ref>{{cite web | url=http://www.uahirise.org/ESP_039563_1730 | title=HiRISE &#124; Yardangs in Arsinoes Chaos (ESP_039563_1730) }}</ref> Layers are seen in parts of the formation.  
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==Yardangs==
 
  
 
Yardangs are common on Mars.<ref>Grotzinger, J. and R. Milliken (eds.)  2012.  Sedimentary Geology of Mars.  SEPM</ref>  They are generally visible as a series of parallel linear ridges.  Their parallel nature is thought to be caused by the direction of the prevailing wind.<ref>name="hiroc.lpl.arizona.edu"</ref>  Yardangs are common in the Medusae Fossae Formation on Mars.
 
Yardangs are common on Mars.<ref>Grotzinger, J. and R. Milliken (eds.)  2012.  Sedimentary Geology of Mars.  SEPM</ref>  They are generally visible as a series of parallel linear ridges.  Their parallel nature is thought to be caused by the direction of the prevailing wind.<ref>name="hiroc.lpl.arizona.edu"</ref>  Yardangs are common in the Medusae Fossae Formation on Mars.

Revision as of 06:52, 8 January 2024

The Medusae Fossae Formation is a large geological formation of probable volcanic origin on the planet Mars.[1]

It is named for the Medusa of Greek mythology. "Fossae" is Latin for "trenches". The formation is a collection of soft, easily eroded deposits that extends off and on for more than 5,000 km along the equator.

Its roughly-shaped regions extend from just south of Olympus Mons to Apollinaris Patera, with a smaller additional region closer to Gale Crater.[2]

The total area of the Medusae Fossae Formation is equal to 20% the size of the continental United States.[3]

The formation straddles what is called the martian dichotomy|highland - lowland boundary near the Tharsis and Elysium (volcanic province)|Elysium volcanic areas, and extends across five quadrangles: Amazonis, Tharsis, Memnonia, Elysium, and Aeolis.

Origin and age

The origin of the formation is unknown, but many theories have been presented over the years.

In 2020, a group of researchers headed by Peter Mouginis-Mark has hypothesized that the formation could have been formed from pumice rafts from the volcano Olympus Mons.[4] In 2012, a group headed by Laura Kerber hypothesized that it could have been formed from ash from the volcanoes Apollinaris Mons, Arsia Mons, and possibly Pavonis Mons.[5]

Its density and high content of sulfur and chlorine, suggests an explosive volcanic origin. It may have been deposited in periodic eruptions over an interval of 500 million years.[6]

The surface of the formation has been eroded by the wind into a series of linear ridges called yardangs.[7] These ridges generally point in direction of the prevailing winds that carved them, and demonstrate the erosive power of Martian winds. The easily eroded nature of the Medusae Fossae Formation suggests that it is composed of weakly cemented particles, and was most likely formed by the deposition of wind-blown dust or volcanic ash.

Yardangs are parts of rock that have been sand blasted into long, skinny ridges by bouncing sand particles blowing in the wind.[8] Layers are seen in parts of the formation.

Yardangs are common on Mars.[9] They are generally visible as a series of parallel linear ridges. Their parallel nature is thought to be caused by the direction of the prevailing wind.[10] Yardangs are common in the Medusae Fossae Formation on Mars.

Aeolis Mensae Yardangs, as seen by HiRISE. Scale bar is 500 meters long. An inverted stream channel is also visible

  • Map of location of Medusae Fossae Formation

  • Medusae Fossae Formation southeast of Apollinaris Patera

  • Small yardangs

Images from spacecraft show that they have different degrees of hardness probably because of significant variations in the physical properties, composition, particle size, and/or cementation. Very few impact craters are visible throughout the area so the surface is relatively young.[11]

See also

External links

References

  1. ↑ Template:Cite web
  2. ↑ Lujendra Ojha (July 20, 2018). "[https://www.nature.com/articles/s41467-018-05291-5/figures/1 Fig. 1, It has been determined that the Medusae Fossae Formation as the single largest source of dust on Mars]" (in en). Nature Communications. ISSN 2041-1723. 
  3. ↑ "The Medusae Fossae Formation as the single largest source of dust on Mars" (2018). Nature Communications 9 (1): 2867. doi:10.1038/s41467-018-05291-5. PMID 30030425. Bibcode: 2018NatCo...9.2867O. 
  4. ↑ Template:Cite web
  5. ↑ "The dispersal of pyroclasts from ancient explosive volcanoes on Mars: Implications for the friable layered deposits" (2012). Icarus 219 (1): 358–381. doi:10.1016/j.icarus.2012.03.016. Bibcode: 2012Icar..219..358K. 
  6. ↑ "The Density of the Medusae Fossae Formation: Implications for its Composition, Origin, and Importance in Martian History" (2018). Journal of Geophysical Research: Planets 123 (6): 1368–1379. doi:10.1029/2018JE005565. Bibcode: 2018JGRE..123.1368O. 
  7. ↑ Template:Cite book
  8. ↑ Template:Cite web
  9. ↑ Grotzinger, J. and R. Milliken (eds.) 2012. Sedimentary Geology of Mars. SEPM
  10. ↑ name="hiroc.lpl.arizona.edu"
  11. ↑ Template:Cite web
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