Cosmic dust may create Mars’ wispy clouds | Science News



Science News is a nonprofit.

Help us keep you informed.

News in Brief

Cosmic dust may create Mars’ wispy clouds

Magnesium from passing comets could be a key part of the Red Planet’s cloud-starter kit

5:08pm, March 13, 2018

HEAD IN THE CLOUDS  The rover Opportunity snapped this picture of wispy clouds drifting through the Martian sky in 2006. New findings suggest the clouds might have condensed around particles of dust from comets.

Sponsor Message

The seeds for Martian clouds may come from the dusty tails of comets.

Charged particles, or ions, of magnesium from the cosmic dust can trigger the formation of tiny ice crystals that help form clouds, a new analysis of Mars’ atmosphere suggests.

For more than a decade, rovers and orbiters have captured images of Martian skies with wispy clouds made of carbon dioxide ice. But “it hasn’t been easy to explain where they come from,” says chemist John Plane of the University of Leeds in England. The cloud-bearing layer of the atmosphere is between –120° and –140° Celsius — too warm for carbon dioxide clouds to form on their own, which can happen at about –220° C.

Then in 2017, NASA’s MAVEN orbiter detected a layer of magnesium ions hovering about 90 kilometers above the Martian surface (SN: 4/29/17, p. 20). Scientists think the magnesium, and possibly other metals not yet detected, comes from cosmic dust left by passing comets. The dust vaporizes as it hits the atmosphere, leaving a sprinkling of metals suspended in the air. Earth has a similar layer of atmospheric metals, but none had been observed elsewhere in the solar system before.

According to the new calculations, the bits of magnesium clump with carbon dioxide gas — which makes up about 95 percent of Mars’ atmosphere — to produce magnesium carbonate molecules. These larger, charged molecules could attract the atmosphere’s sparse water, creating what Plane calls “dirty” ice crystals.

At the temperatures seen in Mars’ cloud layer, pure carbon dioxide ice crystals are too small to gather clouds around them. But clouds could form around dirty ice at temperatures as high as –123° C, Plane and colleagues report online March 6 in the Journal of Geophysical Research: Planets.


J.M.C. Plane et al. Meteoric metal chemistry in the Martian atmosphere. Journal of Geophysical Research: Planets. Published online March 6, 2018. doi:10.1002/2017JE005510.

Further Reading

M.M.J. Crismani et al. Detection of a persistent meteoric metal layer in the Martian atmosphere. Nature Geoscience. Published online May 22, 2017. doi:10.1038/ngeo2958.

A. Yeager. Mars has nighttime snow storms. Science News Online, August 21, 2017.

A. Yeager. Extreme gas loss dried out Mars, MAVEN data suggest. Science News. Vol. 191, April 29, 2017, p. 20.

C. Crockett. Martian aurora, high-altitude dust clouds surprise scientists. Science News. Vol. 187, April 18, 2015, p. 15.

Get Science News headlines by e-mail.

More Astronomy articles

From the Nature Index Paid Content