Dust devils on Mars

NASA's Phoenix lander sees and feels these martian whirlwinds.Provided by the University of Arizona, Tucson
By | Published: September 12, 2008 | Last updated on May 18, 2023
dust devils on mars
The Surface Stereo Imager caught this dust devil in action west of the lander at 11:49 a.m. local Mars time on the 104th martian day, Sept. 9, 2008.
NASA/JPL-Caltech/University of Arizona/Texas A&M University
September 12, 2008
NASA’s Phoenix Mars Lander photographed several dust devils dancing across the arctic plain this week and sensed a dip in air pressure as one passed near the lander.

These dust-lofting whirlwinds had been expected in the area, but none had been detected in earlier Phoenix images.

The Surface Stereo Imager camera on Phoenix took 29 images of the western and southwestern horizon on September 8, during mid-day hours of the lander’s 104th martian day. The next day, after the images had been transmitted to Earth, the Phoenix science team noticed a dust devil right away.

“It was a surprise to have a dust devil so visible that it stood with just the normal processing we do,” says Mark Lemmon of Texas A&M University, lead scientist for the stereo camera. “Once we saw a couple that way, we did some additional processing and found there are dust devils in 12 of the images.”

At least six different dust devils appear in the images, some of them in more than one image. They range in diameter from about 7 feet (2 meters) to about 16 feet (5 meters).

dust devils on Mars
The Surface Stereo imager caught this dust devil in action west-southwest of the lander at 11:16 A.M. local Mars time September 9, the lander’s 104th martian day.
NASA/JPL-Caltech/University of Arizona/Texas A&M University
“It will be very interesting to watch over the next days and weeks to see if there are lots of dust devils or if this was an isolated event,” Lemmon says.

The Phoenix team is not worried about any damage to the spacecraft from these swirling winds.

“With the thin atmosphere on Mars, the wind loads we might experience from dust devil winds are well within the design of the vehicle,” says Ed Sedivy, Phoenix program manager at Lockheed Martin Space Systems Company, Denver, Colorado, which made the spacecraft. “The lander is very rigid with the exception of the solar arrays, which once deployed, latched into position and became a tension structure.”

Phoenix monitors air pressure every day, and on the same day the camera saw dust devils, the pressure meter recorded a sharper dip than ever before. The change was still less than the daily change in air pressure from daytime to nighttime, but over a much shorter time.

“Throughout the mission, we have been detecting vortex structures that lower the pressure for 20 to 30 seconds during the middle part of the day,” says Peter Taylor of York University, Toronto, Canada, a member of the Phoenix science team. “In the last few weeks, we’ve seen the intensity increasing, and now these vortices appear to have become strong enough to pick up dust.”

A key factor in the whirlwinds getting stronger is an increase in the difference between day and night temperatures. Daytime highs at the Phoenix site are still about -22° F (-30° C), but nighttime lows have been dropping a few degrees, getting close to -130° F (-90° C).

The same day as the dust devils were seen, the photographed swinging of Phoenix’s telltale wind gauge indicated wind speeds exceeding 11 miles per hour (300 meters per hour).

Images from spacecraft orbiting Mars had previously indicated that dust devils exist in the region where Phoenix landed.

“We expected dust devils, but we are not sure how frequently,” says Phoenix Project Scientist Leslie Tamppari of NASA’s Jet Propulsion Laboratory, Pasadena, Calififornia. “It could be they are rare and Phoenix got lucky. We’ll keep looking for dust devils at the Phoenix site to see if they are common or not.”

The dust devils that Phoenix has observed so far are much smaller than dust devils that NASA’s Mars Exploration Rover Spirit has photographed much closer to the equator.