Maat Mons - Highest Volcano on Venus
Maat Mons is a massive
shield volcano that erupts every few thousand years. On Venus, it is the
planet's second-highest mountain, as well as its highest volcano. At 0.5°N
194.6°E, it rises 8 kilometers (5.0 miles) above the mean planetary radius and
nearly 5 kilometers above the plains around it. Ma'at, the Egyptian goddess of
truth and justice, is the inspiration for the name.
Maat Mons has a large summit caldera with a diameter of 28×31 kilometers. There are at least five smaller collapse craters within the large caldera, each measuring up to 10 kilometers in diameter. A 40-kilometer-long chain of small craters measuring 3–5 km in diameter runs along the volcano's southeast flank, but instead of indicating a large fissure eruption, they appear to have been formed by collapse: full-resolution imagery from the Magellan probe shows no evidence of lava flows from these craters. On Maat Mons, at least two large-scale structural collapse events appear to have occurred in the past.
In the form of ash
flows near the summit and on the northern flank, the Magellan probe's radar
sounding revealed evidence of comparatively recent volcanic activity at Maat
Mons. The Pioneer Venus probes' atmospheric studies in the early 1980s revealed
a significant variation in sulphur dioxide (SO2) and methane (CH4)
concentrations in Venus' middle and upper atmosphere, which piqued the interest
of planetary geologists. The injection of volcanic gases into the atmosphere by
Plinian eruptions at Maat Mons could be one explanation.
Recent research has
suggested that the volcano structure, lava flow distribution, pit craters,
summit morphology and other small-scale features on Maat Mons are indicative
of recent volcanic activity. Despite the fact that many lines of evidence
suggest Venus is volcanically active, current eruptions at Maat Mons have yet
to be confirmed.
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