spaceSpace and PhysicsspaceAstronomy

First-Ever Sounds Of A Dust Devil On Mars Revealed

Weather monitoring on other planets now comes with sound.


Dr. Alfredo Carpineti


Dr. Alfredo Carpineti

Senior Staff Writer & Space Correspondent

Alfredo (he/him) has a PhD in Astrophysics on galaxy evolution and a Master's in Quantum Fields and Fundamental Forces.

Senior Staff Writer & Space Correspondent

A towering dust devil casts a serpentine shadow over the Martian surface in this image acquired by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.  The scene is a late-spring afternoon in the Amazonis Planitia region of northern Mars. The view covers an area about four-tenths of a mile (644 meters) across. North is toward the top. The length of the dusty whirlwind's shadow indicates that the dust plume reaches more than half a mile (800 meters) in height. The plume is about 30 yards or meters in diameter.
A sinous dust devil seen from space by the Mars Recoinnasance Orbiter. Image credit: NASA/JPL-Caltech/Univ. of Arizona

Dust devils are a common feature seen in many locations across Mars by the robotic explorers we have sent there. They have been extensively photographed but now, for the first time, we also know what they sound like. Thanks to the SuperCam microphones onboard NASA’s Perseverance scientists were able to record a dust devil as it engulfed the rover.

“We've been able to record for the first time ever, the sounds of dust devil coming over the rover, the first Martian dust devil’s sounds,” lead author Dr Naomi Murdoch, from the Université de Toulouse, told IFLScience. “We had not only the sound but also all of the meteorology sensors on and we also had the cameras on. We were able to put that all together, and we were able to characterize really well this vortex.”


We hope that this shows how valuable acoustic data are

Dr Naomi Murdoch

The team determined that the vortex was at least 25 meters across (82 feet), about 10 times the size of the rover, and at least 118 meters (387 feet) tall. Luckily, the Martian atmosphere is just 1 percent the density of Earth’s so the wind pressure from the dust devil was not damaging to Perseverance and instead just rolled over it.

“When we listen to the microphone data, we can hear a big wind gust, then silence when we're in the eye of the vortex, and then a big wind gust again as we come out. So that's how we know it went right over the head of the rover,” Dr Murdoch explained to IFLScience.

The SuperCam microphone team had already announced earlier this year the first-ever measurement of the speed of sound on Mars. We were then delighted to hear the different artificial sounds also recorded, from the rover's laser-equipped instruments to Ingenuity spinning its blades as it flew around Mars.

This figure shows the relative size of the dust devil with respect to the Perseverance rover. The dust devil diameter (white circles), determined from combined data and modelling, is 25 m.  The blue dashed arrow shows the dust devil trajectory direction. The rover Navigation camera (Navcam) field of view is indicated by the pale triangle. At t1 Perseverance is in the leading vortex wall, at t2 Perseverance is inside the eye of the vortex, and at t3 Perseverance is in the tailing vortex wall. The vortex and the rover are drawn to scale. The orange arrows indicate the clockwise rotational direction of the vortex winds.
Schematic of the trajectory of the dust devils through Perseveranca. Image Credits: N. Murdoch / ISAE-SUPAERO

The recordings from the microphones are so sophisticated and responsive that the team was able to hear impacting dust particles. They were able to quantify how much dust is lifted by dust devils and in dust clouds. 


Dust devils were also seen by Spirit and Opportunity. In fact, these weather phenomena actually helped clean the rovers when they got covered in dust and keep them going.

InSight, however, did not see any throughout its mission, and yet, the team did manage to measure some dustless devils, knowns as convective vortices, that don’t seem to pick up dust. Interactions between the atmosphere and surface can lift dust in some areas of Mars but not in others. The reason behind this discrepancy is a major open question. 

Dust devils are seen merging on the rocky terrain of Jezero Crater
Dust devils spotted by Perseverance in Jezero Crater. Image Credit: NASA/JPL-Caltech/SSI


“We hope that with these acoustic recordings, we're actually going to help to answer that question," Dr Murdoch told IFLScience. 


"Because we can hear the dust impacts, that means that we can count the number of particles, because we can count the impact. And we have the wind measurements and the atmospheric measurements and that allows us to quantify how much dust is lifted, how many particles are being transported, and under what conditions. So we hope that this shows how valuable acoustic data are as we go forward for studying this poorly understood dust lifting process on Mars."

The findings are published in Nature Communications.


spaceSpace and PhysicsspaceAstronomy
  • tag
  • Mars,

  • Astronomy,

  • dust devil,

  • Perseverance