Mars’ atmosphere isn’t (electrically) dead

Rover mic catches Mars' first electric discharges in dust devils and storms, hinting at impacts on dust, chemistry, and exploration.

Sparks fly on the Red Planet, as rover recordings catch crackling discharges in Martian dust devils and storms.

The dusty skies of Mars crackle with triboelectric discharges, the first direct evidence of atmospheric electrical activity on the planet, researchers report in Nature. Captured by the Perseverance rover’s SuperCam microphone, these sparks reveal a lively electric environment that could reshape dust cycles and chemistry.

Lightning has lit up atmospheres on Earth, Jupiter, and Saturn, but Mars’ thin air and dusty woes left its electric potential a mystery — until now.

The rover’s microphone, perched on its mast, eavesdropped on Mars’ soundscape, picking up 55 events over two Martian years amid 28 hours of recordings. “Here we report in situ detections of triboelectric discharges, identified by their electrical and acoustic signatures captured by the SuperCam microphone aboard the Perseverance rover,” the study authors note.

Each zap showed a telltale pattern: a sharp electromagnetic overshoot, a relaxing drop, and an N-shaped acoustic shock wave, plus surrounding spikes from smaller charges. Lab tests with a microphone replica confirmed the signatures match triboelectric sparks from colliding dust grains.

Most strikes, 54 of 55, hit during gusty winds, tying them to aeolian action. Sixteen zapped during two dust devils whirlwinding right over the rover, one a hefty vortex dropping pressure by 5.5 pascals. Thirty-five more were fired amid dust storm fronts, like a regional blowout sweeping Jezero crater.

Energies ranged from 0.1 to 150 nanojoules for most, up to 40 millijoules for one whopper — enough to suggest fields hitting Mars’ low breakdown threshold of about 15 kilovolts per meter. “Such electrical activity could affect dust dynamics and potentially fuel a reactive electrochemical environment, enhancing the oxidizing capacity of the atmosphere, with consequences for the preservation of organic molecules,” the researchers write.

This buzz could tweak dust lifting, clumping, and settling, juicing the global dust cycle that drives the Martian climate. It might brew oxidants like hydrogen peroxide, zapping surface organics and fueling chlorine chemistry — key for habitability clues and rover safety.

Dust devils and storms likely dominate planetary power, with fronts outpacing vortices in energy output. Beyond Mars, this hints at sparks on dusty Venus or Titan.”This in situ evidence may have implications for surface chemistry, habitability, and human exploration,” the authors conclude.

Citations: Nature. DOI: 10.1038/s41586-025-09736-y

Uday Kakade
Uday Kakade
Uday Kakade is an India-based freelance science writer. Uday is a graduate in Computer Science, and his interests hover around technology, gadgets, biology, and health.