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Martian dust devils
Martian dust devils are convective atmospheric vortices that occur on the surface of Mars. They were discovered from data reported by NASA's Viking probes, and have been photographed by orbiting satellites and surface rovers in subsequent missions.
Although comparable to terrestrial dust devils in formation and appearance, Martian dust devils can be many times larger than ones found on Earth. They can be powerful enough to pose a threat to rovers and other technology, although some documented encounters have actually benefitted rovers by cleaning them of dust.
The existence of dust devils on Mars was confirmed by analysis of data from the Viking probes in the early 1980s. Photographs from the Viking orbiters revealed tracks across the Martian surface suspected to be caused by dust devils, and data from the landers' meteorological instruments confirmed convective vortices as the cause. Orbital photographs previously taken by Mariner 9 also showed surface lineations initially thought to be the ridges of seif dunes, but they were also shown to be dust devil tracks based on the data from Viking.
Martian dust devils have since been detected and photographed by both orbiting satellites and rovers on the surface. The Mars Pathfinder rover detected 79 convective vortices through atmospheric pressure data, and imaged several dust devils with its wide-angle camera. On 7 November 2016, five dust devils ranging in height from 0.5 to 1.9 kilometers (0.31 to 1.18 mi) were imaged in a single observation by the Mars Orbiter Mission in the Martian southern hemisphere. On 27 September 2021, the Perseverance rover directly encountered a Martian dust devil, imaging and recording the sound of the vortex as it passed, the first such observation in the history of Mars exploration.
Perseverance Rover recorded a very tall dust devil in the distance on Aug. 30, 2023. It was about 2.5 miles (4 kilometers) away and was moving east to west at about 12 mph (19 kph). Its width was about 200 feet (60 meters). Even though only the bottom 387 feet (118 meters) of the devil was visible in the camera frame, scientists estimated its total height at about 1.2 miles (2 kilometers) based on the length of its shadow---higher than the average tornado on Earth.
Dust devils on Mars form by the same basic mechanism as ones on Earth; specifically, solar energy heats the Martian surface, causing warm air near the ground to rise through the cooler air above, creating an updraft. Horizontal wind then causes rotation, forming a vortex. The lifting of surface material through the vortex creates a visible dust devil. On average, however, Martian dust devils are about three times as large as their terrestrial counterparts. The largest vortices can reach heights of up to 8 kilometers and widths of up to 700 meters, and last more than 25 minutes. The greater height of Martian dust devils may be due to a planetary boundary layer which is several kilometers thicker on average than Earth's.
Dust devils occur very frequently on Mars. One team of researchers have calculated a rate of 1 event per sol for each square kilometer of the Martian surface.
As on Earth, they occur during warmer times of year. Research has revealed highly predictable seasonal behavior, with activity escalating sharply just before Martian vernal equinox, peaking in midsummer, and declining after the autumnal equinox. Amazonis Planitia has been identified as the region most prone to dust devil activity on Mars.
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Martian dust devils
Martian dust devils are convective atmospheric vortices that occur on the surface of Mars. They were discovered from data reported by NASA's Viking probes, and have been photographed by orbiting satellites and surface rovers in subsequent missions.
Although comparable to terrestrial dust devils in formation and appearance, Martian dust devils can be many times larger than ones found on Earth. They can be powerful enough to pose a threat to rovers and other technology, although some documented encounters have actually benefitted rovers by cleaning them of dust.
The existence of dust devils on Mars was confirmed by analysis of data from the Viking probes in the early 1980s. Photographs from the Viking orbiters revealed tracks across the Martian surface suspected to be caused by dust devils, and data from the landers' meteorological instruments confirmed convective vortices as the cause. Orbital photographs previously taken by Mariner 9 also showed surface lineations initially thought to be the ridges of seif dunes, but they were also shown to be dust devil tracks based on the data from Viking.
Martian dust devils have since been detected and photographed by both orbiting satellites and rovers on the surface. The Mars Pathfinder rover detected 79 convective vortices through atmospheric pressure data, and imaged several dust devils with its wide-angle camera. On 7 November 2016, five dust devils ranging in height from 0.5 to 1.9 kilometers (0.31 to 1.18 mi) were imaged in a single observation by the Mars Orbiter Mission in the Martian southern hemisphere. On 27 September 2021, the Perseverance rover directly encountered a Martian dust devil, imaging and recording the sound of the vortex as it passed, the first such observation in the history of Mars exploration.
Perseverance Rover recorded a very tall dust devil in the distance on Aug. 30, 2023. It was about 2.5 miles (4 kilometers) away and was moving east to west at about 12 mph (19 kph). Its width was about 200 feet (60 meters). Even though only the bottom 387 feet (118 meters) of the devil was visible in the camera frame, scientists estimated its total height at about 1.2 miles (2 kilometers) based on the length of its shadow---higher than the average tornado on Earth.
Dust devils on Mars form by the same basic mechanism as ones on Earth; specifically, solar energy heats the Martian surface, causing warm air near the ground to rise through the cooler air above, creating an updraft. Horizontal wind then causes rotation, forming a vortex. The lifting of surface material through the vortex creates a visible dust devil. On average, however, Martian dust devils are about three times as large as their terrestrial counterparts. The largest vortices can reach heights of up to 8 kilometers and widths of up to 700 meters, and last more than 25 minutes. The greater height of Martian dust devils may be due to a planetary boundary layer which is several kilometers thicker on average than Earth's.
Dust devils occur very frequently on Mars. One team of researchers have calculated a rate of 1 event per sol for each square kilometer of the Martian surface.
As on Earth, they occur during warmer times of year. Research has revealed highly predictable seasonal behavior, with activity escalating sharply just before Martian vernal equinox, peaking in midsummer, and declining after the autumnal equinox. Amazonis Planitia has been identified as the region most prone to dust devil activity on Mars.