[meteorite-list] NASA Mars Orbiter Tracks Back-to-Back Regional Storms (MRO)

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Mon, 20 Mar 2017 13:18:18 -0700 (PDT)
Message-ID: <201703202018.v2KKIItA003987_at_zagami.jpl.nasa.gov>

https://www.jpl.nasa.gov/news/news.php?feature=6771

NASA Mars Orbiter Tracks Back-to-Back Regional Storms
Jet Propulsion Laboratory
March 9, 2017

A regional dust storm currently swelling on Mars follows unusually closely
on one that blossomed less than two weeks earlier and is now dissipating,
as seen in daily global weather monitoring by NASA's Mars Reconnaissance
Orbiter.

Images from the orbiter's wide-angle Mars Color Imager (MARCI) show each
storm growing in the Acidalia area of northern Mars, then blowing southward
and exploding to sizes bigger than the United States after reaching the
southern hemisphere.

That development path is a common pattern for generating regional dust
storms during spring and summer in Mars' southern hemisphere, where it
is now mid-summer.

"What's unusual is we're seeing a second one so soon after the first one,"
said Mars meteorologist Bruce Cantor of Malin Space Science Systems, San
Diego, which built and operates MARCI. "We've had orbiters watching weather
patterns on Mars continuously for nearly two decades now, and many patterns
are getting predictable, but just when we think we have Mars figured out,
it throws us another surprise."

Weekly Martian weather reports including animated sequences of MARCI observations
are available at:

http://www.msss.com/msss_images/latest_weather.html

Weather updates from the Mars Reconnaissance Orbiter science team provide
operators of Mars rovers advance notice both for taking precautions and
for planning observations of storms, particularly in case a regional storm
grows to encircle the whole planet. A planet-encircling Martian storm
last occurred in 2007.

The orbiter monitors storms with its Mars Climate Sounder (MCS) instrument
as well as with MARCI. MCS measurements of high-altitude atmospheric warming
associated with dust storms have revealed an annual pattern in the occurrence
of large regional storms, and the first of these back-to-back storms fits
into the identified pattern for this time of the Martian year.

Researchers have watched effects of the latest storms closely. "We hope
for a chance to learn more about how dust storms become global, if that
were to happen," said David Kass of NASA's Jet Propulsion Laboratory,
Pasadena, California. "Even if it does not become a global storm, the
temperature effects due to thin dust hazes will last for several weeks."

Cantor reported the second of the current back-to-back regional storms
on March 5 to the team operating NASA's Mars Exploration Rover Opportunity.
The earlier storm, which had become regional in late February, was dissipating
by then but still causing high-altitude haziness and warming.

"There's still a chance the second one could become a planet-encircling
storm, but it's unlikely because we're getting so late in the season,"
Cantor said this week. All previously observed planet-encircling dust
storms on Mars occurred earlier in the southern summer.

Opportunity Project Manager John Callas, at JPL, credits MARCI weather
reports with helping his team protect rovers when sudden increases in
atmospheric dust decrease sunlight reaching the rover solar arrays. For
example, Cantor's warning about a regional storm approaching the rover
Spirit in November 2008 prompted JPL to send an emergency weekend command
to conserve energy by deleting a planned radio transmission by Spirit.
That saved enough charge in Spirit's batteries to prevent "what would
likely have been a very serious situation," Callas said.

During the most recent global dust storm on Mars, in 2007, both of the
rovers then operating on the planet -- Spirit and Opportunity -- were
put into a power-saving mode for more than a week with minimal communication.
The early-2010 ending of Spirit's mission was not related to a dust storm.

The same winds that raise Martian dust into the atmosphere can clear some
of the dust that accumulates on the rovers. On Feb. 25, as the first back-to-back
was spreading regionally, Opportunity experienced a significant cleaning
of its solar panels that increased their energy output by more than 10
percent, adjusted for the clarity of the atmosphere. Dust-removing events
typically clean the panels by only one or two percent. The Opportunity
operations team has noticed over the years that a large dust-cleaning
event often precedes dusty skies. Since Feb. 25, the atmosphere over Opportunity
has become dustier, and some of the dust has already fallen back onto
the solar panels.

"Before the first regional dust storm, the solar panels were cleaner than
they were during the last four Martian summers, so the panels generated
more energy," said JPL rover-power engineer Jennifer Herman. "It remains
to be seen whether the outcome of these storms will be a cleaner or dirtier
Opportunity. We have seen both results from dust storms in the past."

NASA's Curiosity rover, on Mars since 2012, uses a radioisotope thermoelectric
generator for power instead of solar panels, so it doesn't face the same
hazard from dust storms as Opportunity does. The possibility of observing
the growth and life cycle of a regional or global storm offers a research
opportunity for both missions, though. Scientists temporarily modified
Curiosity's weather-monitoring regime last week in response to learning
that a regional dust storm was growing.

"We'll keep studying this for weeks as the dust clears from the sky,"
said atmospheric scientist Mark Lemmon of Texas A&M University, College
Station. Sky observations at multiple lighting angles can provide information
about changes in the size distribution of suspended dust particles as
additional dust is lifted into the sky and larger particles drop more
quickly than smaller ones.

News Media Contact
Guy Webster
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278
guy.webster at jpl.nasa.gov

Laurie Cantillo / Dwayne Brown
NASA Headquarters, Washington
202-358-1077 / 202-358-1726
laura.l.cantillo at nasa.gov / dwayne.c.brown at nasa.gov

2017-064
Received on Mon 20 Mar 2017 04:18:18 PM PDT