“Global dust storms are really unusual,” said Mars Climate Sounder scientist David Kass of NASA’s Jet Propulsion Laboratory. “We really don’t have anything like this on the Earth, where the entire planet’s weather changes for several months.”
Last year, a fleet of NASA spacecraft got a detailed look at the life cycle of the 2018 global dust storm that ended the Opportunity rover’s mission on June 10, 2019 after more than a thousand commands to restore contact by engineers in the Space Flight Operations Facility at JPL.
While scientists are still puzzling over the data, two papers recently shed new light on a phenomenon observed within the storm: dust towers, or concentrated clouds of dust that warm in sunlight and rise high into the air. Scientists think that dust-trapped water vapor may be riding them like an elevator to space, where solar radiation breaks apart their molecules. This might help explain how Mars’ water disappeared over billions of years.
Mars Massive Dust Towers
Dust towers are massive, churning clouds that are denser and climb much higher than the normal background dust in the thin Martian atmosphere. While they also occur under normal conditions, the towers appear to form in greater numbers during global storms.
A tower starts at the planet’s surface as an area of rapidly lifted dust about as wide as the state of Rhode Island. By the time a tower reaches a height of 50 miles (80 kilometers), as seen during the 2018 global dust storm, it may be as wide as Nevada. As the tower decays, it can form a layer of dust 35 miles (56 kilometers) above the surface that can be wider than the continental United States.
The recent findings on dust towers come courtesy of NASA’s Mars Reconnaissance Orbiter (MRO), which is led by the agency’s Jet Propulsion Laboratory in Pasadena, California. Though global dust storms cloak the planet’s surface, MRO can use its heat-sensing Mars Climate Sounder instrument to peer through the haze. The instrument is designed specifically for measuring dust levels. Its data, coupled with images from a camera aboard the orbiter called the Mars Context Imager (MARCI), enabled scientists to detect numerous swelling dust towers.
The yellow-white cloud in the bottom-center of the image at the top of the page is a Mars “dust tower” – a concentrated cloud of dust that can be lofted dozens of miles above the surface. The blue-white plumes are water vapor clouds. This image was taken on Nov. 30, 2010, by NASA’s Mars Reconnaissance Orbiter. (NASA/JPL-Caltech/MSSS)
Dust towers appear throughout the Martian year, but MRO observed something different during the 2018 global dust storm. “Normally the dust would fall down in a day or so,” said the paper’s lead author, Nicholas Heavens of Hampton University in Hampton, Virginia. “But during a global storm, dust towers are renewed continuously for weeks.” In some cases, multiple towers were seen for as long as 3 1/2 weeks.
The rate of dust activity surprised Heavens and other scientists. But especially intriguing is the possibility that dust towers act as “space elevators” for other material, transporting them through the atmosphere. When airborne dust heats up, it creates updrafts that carry gases along with it, including the small quantity of water vapor sometimes seen as wispy clouds on Mars.
A previous paper led by Heavens showed that during a 2007 global dust storm on Mars, water molecules were lofted into the upper atmosphere, where solar radiation could break them down into particles that escape into space. That might be a clue to how the Red Planet lost its lakes and rivers over billions of years, becoming the freezing desert it is today.
Scientists can’t say with certainty what causes global dust storms; they’ve studied fewer than a dozen to date.
With time and more data, the MRO team hopes to better understand the dust towers created within global storms and what role they may play in removing water from the Red Planet’s atmosphere.
Nicholas G. Heavens et al. An Observational Overview of Dusty Deep Convection in Martian Dust Storms, Journal of the Atmospheric Sciences (2019). DOI: 10.1175/JAS-D-19-0042.1
Nicholas G. Heavens et al. Dusty Deep Convection in the Mars Year 34 Planet‐Encircling Dust Event, Journal of Geophysical Research: Planets (2019). DOI: 10.1029/2019JE006110
The Daily Galaxy, Sam Cabot, via JPL