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Maat Mons is a massive shield volcano. It is the second-highest mountain, and the highest volcano, on the planet Venus. It rises 8 kilometres (5.0 mi) above the mean planetary radius at 0°30′N 194°36′E / 0.5°N 194.6°E / 0.5; 194.6, and nearly 5 km above the surrounding plains.[2] It is named after the Egyptian goddess of truth and justice, Ma'at.

Maat Mons
Maat Mons on Venus.jpg
Maat Mons is displayed in this three-dimensional perspective view of the surface of Venus, with the horizontal scale multiplied by 22.5. Based on Magellan probe radar images
Feature typeMountain
Coordinates0°30′N 194°36′E / 0.5°N 194.6°E / 0.5; 194.6Coordinates: 0°30′N 194°36′E / 0.5°N 194.6°E / 0.5; 194.6[1]
Diameter395 km


Maat Mons has a large summit caldera, 28×31 km in size. Within the large caldera there are at least five smaller collapse craters, up to 10 km in diameter.[3]

A chain of small craters 3–5 km in diameter extends some 40 km along the southeast flank of the volcano, but rather than indicating a large fissure eruption, they seem to also be formed by collapse: full resolution imagery from the Magellan probe reveals no evidence of lava flows from these craters.[3]

At least two large scale structural collapse events seem to have occurred in the past on Maat Mons.[3]


Radar sounding by the Magellan probe revealed evidence for comparatively recent volcanic activity at Maat Mons, in the form of ash flows near the summit and on the northern flank.

Intriguingly for planetary geologists, atmospheric studies carried out by the Pioneer Venus probes in the early 1980s revealed a considerable variation in the concentrations of sulfur dioxide (SO2) and methane (CH4) in Venus' middle and upper atmosphere. One possible explanation for this was the injection of volcanic gases into the atmosphere by plinian eruptions at Maat Mons.[4]

More recent studies have suggested that the volcano structure, distribution of lava flows, pit craters, summit morphology, and other small-scale features are indicative of recent volcanic activity on Maat Mons.[5]

Although many lines of evidence suggest that Venus is likely to be volcanically active, present-day eruptions at Maat Mons have not been confirmed.

See alsoEdit


  1. ^ "Maat Mons". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ^ "PIA00106: Venus - 3D Perspective View of Maat Mons". Planetary Photojournal. Jet Propulsion Lab. 1996-08-01. Retrieved 2012-06-30.
  3. ^ a b c Mouginis-Mark P. J. (1994). "Morphology of Venus Calderas: Sif and Maat Montes" (PDF). Abstracts of the 25th Lunar and Planetary Science Conference, Held in Houston, TX, 14–18 March 1994: 949. Bibcode:1994LPI....25..949M.
  4. ^ Robinson, Cordula A.; Thornhill, Gill D.; Parfitt, Elisabeth A. (1995). "Large-scale volcanic activity at Maat Mons: Can this explain fluctuations in atmospheric chemistry observed by Pioneer Venus?". Journal of Geophysical Research. 100 (E6): 11755–11763. Bibcode:1995JGR...10011755R. doi:10.1029/95JE00147.
  5. ^ Mouginis-Mark, Peter J. (2016-10-01). "Geomorphology and volcanology of Maat Mons, Venus". Icarus. 277: 433–441. Bibcode:2016Icar..277..433M. doi:10.1016/j.icarus.2016.05.022.

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