Dust devil tracks

Dust devils occur when the sun warms up the air near a flat, dry surface. The warm air then rises quickly through the cooler air and begins spinning while moving ahead. This spinning, moving cell may pick up dust and sand and leave behind a clean surface.[1]

Dust devils on Mars have been photographed both from the ground and high overhead from orbit. They have even blown dust off the solar panels of two Rovers on Mars, thereby greatly extending their useful lifetime.[2] The pattern of the tracks has been shown to change every few months.[3] A study that combined data from the High Resolution Stereo Camera (HRSC) and the Mars Orbiter Camera (MOC) found that some large dust devils on Mars have a diameter of 700 metres (2,300 ft) and last at least 26 minutes.[4] Measurements from the Curiosity Rover confirms that the pressure drops when a dust devil passes nearby.[5]

A dust devil that was previously imaged in 2009, there was information found about two years later showing the tracks visible from the previous imaging are completely different from the old ones meaning there had been a dust storm to erase the old tracks.[6]

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  Mars without a dust storm on June 2001 (on left) and with a global dust storm on July 2001 (on right), as seen by Mars Global Surveyor

Since it is not always too easy to observe these dust devil tracks on Mars tests have been done on Earth to further our understanding of these storms. Traditionally dust devils leave tracks that are darker, but satellite images have captured some cases where they are lighter than the traditional markings. In conclusion the marks were not darker than usual but the sand had been darkened by five minutes of rainfall during the previous night. Since there is no proof of water on Mars indefinitely it is believed that these lighter marks are being held together by electrostatic forces.[7]

Dust devil on Mars (MGS).

Dust devils cause twisting dark trails on the Martian surface.

Serpent dust devil of Mars (MRO).

Dust devils in Valles Marineris (MRO).

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  Kepler (Martian crater) showing dust devil tracks, as seen by Mars Global Surveyor.
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  Pattern of large and small tracks made by giant dust devils, as seen by Mars Global Surveyor under the MOC Public Targeting Program..
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  Russell Crater dust devil changes in Noachis quadrangle, as seen by HiRISE. Click on image to see changes in dust devil tracks in just 3 months.
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  Milankovic Crater central area, as seen by HiRISE. Click on image to see more details: dark dunes, clear dust devil tracks, and boulders (small bright dots).
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  Dust devil tracks, as seen by HiRISE under HiWish program. Location is Casius quadrangle.
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  Layers in Danielson Crater, as seen by HiRISE. Dust devil tracks are also visible at the top. Location is Arabia quadrangle.
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  A dust devil on hilly terrain in the Amazonis quadrangle.