NASA just sent out this press release discussing the various ways that we watch out for dust storms that might be dangerous to the rovers. I have actually used data from the Mars Color Imager (MARCI) that they mention in the release, but I used it for the exact opposite task! I wrote programs that search through the images taken by that camera (there are a lot of them, it gets global coverage every day!) over a certain timeframe and choose the least dusty ones. This is useful for removing the effect of the atmosphere and tracking changes on the surface: for example, if I run my program before and after the huge dust storm in 2007, you can see the wind streaks in Gusev crater changing.
Anyway, here’s the NASA press release. You may also be interested in Emily’s post about recent dust activity on Mars.
PASADENA, Calif. — Heading into a period of the Martian year prone to major dust storms, the
team operating NASA’s twin Mars rovers is taking advantage of eye-in-the-sky weather reports.
On April 21, Mars will be at the closest point to the sun in the planet’s 23-month, elliptical orbit.
One month later, the planet’s equinox will mark the start of summer in Mars’ southern
hemisphere. This atmospheric-warming combination makes the coming weeks the most likely
time of the Martian year for dust storms severe enough to minimize activities of the rovers.
“Since the rovers are solar powered, the dust in the atmosphere is extremely important to us,” said
Bill Nelson of NASA’s Jet Propulsion Laboratory, Pasadena, Calif., chief of the engineering team
for Spirit and Opportunity.
Unexplained computer reboots by Spirit in the past week are not related to dust’s effects on the
rover’s power supply, but the dust-storm season remains a concern. Spirit received commands
Tuesday to transmit more engineering data in coming days to aid in diagnosis of the reboots.
After months of relatively clear air, increased haze in March reduced Spirit’s daily energy supply
by about 20 percent and Opportunity’s by about 30 percent. Widespread haze resulted from a
regional storm that made skies far south of the rovers very dusty. Conditions at the rovers’ sites
remained much milder than the worst they have endured. In July 2007, nearly one Martian year
ago, airborne dust blocked more than 99 percent of the direct sunlight at each rover’s site.
The rovers point cameras toward the sun to check the clarity of the atmosphere virtually every
day. These measurements let the planning team estimate how much energy the rovers will have
available on the following day. Observations of changes in the Martian atmosphere by NASA’s
Mars Reconnaissance Orbiter, which reached Mars in 2006, and NASA’s Mars Odyssey, which
reached Mars in 2001, are available to supplement the rover’s own skywatch.
The Mars Color Imager camera on Mars Reconnaissance Orbiter sees the entire planet every day
at resolution comparable to weather satellites around Earth.
“We can identify where dust is rising into the atmosphere and where it is moving from day to
day,” said Michael Malin of Malin Space Science Systems, San Diego, principal investigator for
Mars Color Imager. “Our historical baseline of observing Martian weather, including data from
the Mars Global Surveyor mission from 1998 to 2007, helps us know what to expect. Weather on
Mars is more repetitive from year to year than weather on Earth. Global dust events do not occur
every Mars year, but if they do occur, they are at this time of year.”
Two other instruments — the Thermal Emission Imaging System on Mars Odyssey and the Mars
Climate Sounder on Mars Reconnaissance Orbiter — monitor changes in airborne dust or dust-
related temperatures in Mars’ upper atmosphere. Orbiters also aid surface missions with radio
relays, imaging to aid drive plans, and studies of possible future landing sites.
When orbital observations indicate a dust-raising storm is approaching a rover, the rover team can
take steps to conserve energy. For example, the team can reduce the length of time the rover will
be active or can shorten or delete some communication events.
In recent weeks, frequent weather reports from Bruce Cantor of Malin’s Mars Color Imager team
let the rover team know that the March increase in haziness was not the front edge of a bad
storm. “Bruce’s weather reports have let us be more aggressive about using the rovers,” said Mark
Lemmon, a rover-team atmospheric scientist at Texas A&M University, College Station. “There
have been fewer false alarms. Earlier in the mission, we backed off a lot on operations whenever
we saw a small increase in dust. Now, we have enough information to know whether there’s
really a significant dust storm headed our way.”
At other times, the weather reports prompt quick precautionary actions. On Saturday, Nov. 8,
2008, the rover team received word from Cantor of a dust storm nearing Spirit. The team deleted
a communication session that Sunday and sent a minimal-activity set of commands that Monday.
Without those responses, Spirit would likely have depleted its batteries to a dangerous level.
Winds that can lift dust into the air can also blow dust off the rovers’ solar panels. The five-year-
old rover missions, originally planned to last for three months, would have ended long ago if
beneficial winds didn’t occasionally remove some of the dust that accumulates on the panels. A
cleaning event in early April aided Opportunity’s power output, and Spirit got two minor
cleanings in February, but the last major cleaning for Spirit was nearly a full Martian year ago.
Nelson said, “We’re all hoping we’ll get another good cleaning.”
JPL, a division of the California Institute of Technology, Pasadena, manages the Mars
Exploration Rovers, Mars Odyssey and Mars Reconnaissance Orbiter for NASA’s Science
Mission Directorate, Washington. More information about the rovers is at
http://www.nasa.gov/rovers . Dust reports from the Thermal Emission Imaging System,
operated by Arizona State University, Tempe, are at http://themis.asu.edu/dustmaps/ . Weather
reports from the Mars Color Imager team are at