A marsquake is a theoretical natural phenomenon which, much like an earthquake, would be a shaking of the surface or interior of the planet Mars as a result of the sudden release of energy in the planet's interior, such as the result of plate tectonics, which most quakes on Earth originate from, or possibly from hotspots such as Olympus Mons or the Tharsis Montes. The detection and analysis of marsquakes could be informative to probing the interior structure of Mars, as well as identifying whether any of Mars's many volcanoes continue to be volcanically active or not.
While quakes have been observed and well-documented on the Moon, as well as compelling evidence of quakes on Venus, very little is known about the current seismic activity of Mars, with some estimations suggesting that marsquakes occur as rarely as once every million years or more. Nevertheless, compelling evidence has been found that Mars has in the past been seismically active, with clear magnetic striping over a large region of southern Mars. Magnetic striping on Earth is often a sign of a region of particularly thin crust splitting and spreading, forming new land in the slowly separating rifts; a prime example of this being the Mid-Atlantic Ridge. However, no clear spreading ridge has been found in this region, suggesting that another, possibly non-seismic explanation may be needed
The 4,000 kilometres (2,500 miles) long canyon system, Valles Marineris, has been suggested to be the remnant of an ancient Martian strike-slip fault. However, even if it was at some point an active fault, it is unknown whether the fault is still active, or if it has "frozen" into place.
The first attempts to detect seismic activity on Mars was with the Viking program in 1975, and the landers were operated for several years. However, the seismographs were mounted on top of the landers and were unable to detect any clear seismic activity, the Martian wind blowing them too much. It was possible to rule out frequent and large marsquakes at that time. The Viking 2 device collected data for 2100 hours (89 days) of data over 560 sols of lander runtime. The Viking 1 lander did not return any data due to a problem activating the seismometer. Times when the windspeed was low at the Viking 2 site, allowed limits to be placed on seismic activity at the time and place on Mars.
There was one candidate for a Mars quake on Sol 80 by the Viking 2 seismometer, however there was no wind speed data collected so its not possible to say if it was the wind or not. For the Sol 80 event, the problem was not wind noise but rather a lack of wind data making it unclear if it was a wind gust or possible Mars quake. Much of data set has been converted to ASCII files from the original recordings. 30 Years after the collections the InSight mission lead to an increased interest in the Viking data set, and further analysis may reveal one of the largest collection of dust devil detections.
The InSight Mars lander, launched in May 2018, landed on Mars on 26 November 2018 and will deploy a seismometer called Seismic Experiment for Interior Structure (SEIS) to search for marsquakes and analyze Mars's internal structure. Even if no seismic events are detected, the seismometer is expected to be sensitive enough to detect possibly several dozen meteors causing airbursts in Mars's atmosphere per year, as well as meteorite impacts. It will also investigate how the Martian crust and mantle respond to the effects of meteorite impacts, which gives clues to the planet's inner structure.
Candidate seismic eventEdit
Despite the drawbacks of significant wind interference, on Sol 80 of the Viking 2 lander's mission (roughly November 23, 1976), the on-board seismometer detected an unusual acceleration event during a period of relatively low wind speed. Based on the features of the signal and assuming Mars's crust behaves similar to Earth's crust near the lander's testing site in Southern California, the event was estimated to have a magnitude of 2.7[clarification needed] and a distance of roughly 110 kilometers. However, the wind speed was only measured 20 minutes previously, and 45 minutes after, at 2.6 and 3.6 meters per second, respectively. While a sudden wind gust of 16 m/s would have been required to produce the event, it cannot be completely ruled out.
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|url=value (help). Earth and Space Science. 4 (11): 681–688. doi:10.1002/2017ea000306. ISSN 2333-5084. Retrieved 21 November 2018.