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Dust devil tracks

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Title: Dust devil tracks  
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Subject: Noachis quadrangle, Arcadia quadrangle, Climate of Mars, Frento Vallis, Icaria Fossae
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Dust devil tracks

Martian Dust Devil - in Amazonis Planitia (April 10, 2001) (also) (video (02:19)).

Many areas on Mars experience the passage of giant dust devils. A thin coating of fine bright dust covers most of the Martian surface. When a dust devil goes by it blows away the coating and exposes the underlying dark surface, which within a few weeks assumes its former bright colour, either from being re-covered through wind action or some form of oxidation through exposure to sunlight and air. 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]

These dust devils have been seen from the ground and high overhead from orbit. They have even blown dust off the solar panels of the two Rovers on Mars, thereby greatly extending their usefulness.[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]



  1. ^ HiRISE | (PSP_00481_2410). Retrieved on 7 August 2011.
  2. ^ Mars Exploration Rover Mission: Press Release Images: Spirit. Retrieved on 7 August 2011.
  3. ^ [1]
  4. ^ Reiss, D. et al. 2011. Multitemporal observations of identical active dust devils on Mars with High Resolution Stereo Camera (HRSC) and Mars Orbiter Camera (MOC). Icarus. 215:358-369.
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