NASA Reveals 'Dust Devil' as it Skirts Across The Red Planet's Surface

Published August 31st, 2020 - 10:59 GMT
We often have to process these images, by enhancing what’s changed between them, before dust devils clearly show up,' wrote NASA scientist Claire Newman.

A new series of images sent to Earth by NASA's Curiosity rover on Mars show a spinning 'dust devil' as it skirts across the surface of the Red Planet.  

NASA Curiosity Rover has been moving across the Gale crater for the past eight years, conducting experiments and sending sending stunning still images to Earth.

Gale crater is going through its 'windy season', stirring up dust devils - caused by vortices of fast wind raising dust from the ground - captured by Curiosity. 

According to NASA researchers, being able to study weather phenomena on Mars that we can also see on Earth can help us understand seasons on the Red Planet. 

NASA hasn't confirmed the size of the dust devil as it was too far away for accurate measurements, but orbiting spacecraft have seen some reaching 12 miles high. 

It’s almost summer on Mars and because of this the surface of the Gale crater is heating up - this heating runs from early spring through to the Martian mid-summer.

When the surface warms enough, it causes convection and in turn vortices made up of fast winds that whip around low pressure cores - much like on Earth.

When the wind is strong enough - as has happened this year - they can pick up soil from the surface and create dust devils that can be seen across multiple still images sent back to Earth by the Curiosity rover.

'We often have to process these images, by enhancing what’s changed between them, before dust devils clearly show up,' wrote NASA scientist Claire Newman.

'This dust devil was so impressive that - if you look closely - you can just see it moving to the right, at the border between the darker and lighter slopes, even in the raw images.'

Dust devils happen the same way on Earth as on Mars and form best when the terrain is relatively flat and dry and the air is warmer at the surface than above it. 

They are actually very common on Mars - but actually seeing on in motion is rare as they are relatively short-lived and Curiosity only sends back still images.

We know about them because Curiosity and orbiting spacecraft have spotted the tracks these dust devils leave behind them - rather than one in motion. 

To capture a dust devil movie the team had to get Curiosity to take a lot of images of the same region for between five and 30 minutes.

Then back on Earth the team worked to stitch the images together to creation a moving video that allowed them to track its path.

Monitoring their motion can provide information about a dust devil's movement, where they initiate and how they evolve.

'Looking at how fast they’re moving and in what direction also tells us about the background wind speed and direction at their location,' said Newman. 

'We also made sure to take meteorological measurements with throughout each movie, in case we image a vortex that’s close enough for us to also measure its pressure drop, impact on local temperatures, or even UV radiation if it’s dusty enough to partially block out the Sun.'

Monitoring dust devils isn't the primary mission of the atmospheric team, their goal is to drill and sample material as part of a 'wet chemistry' experiment.

This involves transforming less volatile organic chemistry into forms that can be detected by the equipment onboard the Curiosity rover. 

While drilling and checking the samples, cameras on Curiosity could be used to monitor and capture images of the dust devil.

They also examined the dust seen above the rover in the crater. 

'The dust measurements will help us to track the regional dust activity on Mars that has been seen from the surface and orbit in recent years,' Newman wrote.

Curiosity is currently the only moving rover on the Red Planet, but Perseverance is currently in flight between the worlds and is due to land on Mars early in 2021. 

Full details of the discovery can be found on the NASA Mars Mission updates blog. 

This article has been adapted from its original source.     

© Associated Newspapers Ltd.

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