Dust storms linked to gas escape from Martian atmosphere
Some Mars experts are eager and optimistic for a dust storm this year to grow so grand it darkens skies around the entire Red Planet. This type of phenomenon in the environment of modern Mars could be examined as never before possible, using the combination of spacecraft now at Mars.
A study published today and co-authored by CU Boulder scientists looked at observations by NASA's Mars Reconnaissance Orbiter (MRO) during the most recent Martian global dust storm. That 2007 event suggests such storms play a role in the ongoing process of gas escaping from the top of Mars' atmosphere, a process which long ago transformed wetter, warmer ancient Mars into today's arid, frozen planet.
"We found there's an increase in water vapor in the middle atmosphere in connection with dust storms," said Nicholas Heavens of Hampton University, Hampton, Virginia, lead author of the report in Nature Astronomy. "Water vapor is carried up with the same air mass rising with the dust."
A link between the presence of water vapor in Mars' middle atmosphere—roughly 30 to 60 miles (50 to 100 kilometers) high—and escape of hydrogen from the top of the atmosphere has been detected by NASA's Hubble Space Telescope and the European Space Agency's Mars Express orbiter, but mainly in years without the dramatic changes produced in a global dust storm. NASA's MAVEN mission arrived at Mars in 2014 to study the process of atmosphere escape.
"It would not be a surprise to see a global dust storm this year, and we would love that opportunity," said MAVEN Principal Investigator Bruce Jakosky of CU Boulder.
"It would be great to have a global dust storm we could observe with all the assets now at Mars, and that could happen this year," said David Kass of NASA's Jet Propulsion Laboratory, Pasadena, California. He is a co-author of the new report and deputy principal investigator for the instrument that is the main source of data for it, MRO's Mars Climate Sounder.
Not all Mars watchers are thrilled with the idea of a global dust storm, which can adversely affect ongoing missions. For instance: Opportunity, as a solar powered rover, would have to hunker down to save energy; the upcoming InSight lander's parameters will need to be adjusted for safe entry, descent and landing in November; and all the cameras on rovers and orbiters will need to deal with low visibility.
Decades of Mars observations document a pattern of multiple regional dust storms arising during the northern spring and summer. In most Martian years, which are nearly twice as long as Earth years, all the regional storms dissipate and none swells into a global dust storm. But such expansion happened in 1977, 1982, 1994, 2001 and 2007. The next Martian dust storm season is expected to begin this summer and last into early 2019.
The Mars Climate Sounder on MRO can scan the atmosphere to directly detect dust and ice particles and can indirectly sense water vapor concentrations from effects on temperature. Heavens and co-authors of the new paper report the sounder's data show slight increases in middle-atmosphere water vapor during regional dust storms and reveal a sharp jump in the altitude reached by water vapor during the 2007 global dust storm. Using recently refined analysis methods for the 2007 data, the researchers found an increase in water vapor by more than a hundred-fold in the middle atmosphere during that global storm.
Before MAVEN reached Mars, many scientists expected to see loss of hydrogen from the top of the atmosphere occurring at a rather steady rate, with variation tied to changes in the solar wind's flow of charged particles from the Sun. Data from MAVEN and Mars Express haven't fit that pattern, instead showing a pattern that appears more related to Martian seasons than to solar activity. Heavens and coauthors present the dust storms' hoisting of water vapor to higher altitudes as a likely key to the seasonal pattern in hydrogen escape from the top of the atmosphere. MAVEN observations during the stronger effects of a global dust storm could boost understanding of their possible link to the escape of gas from the atmosphere.
"What would the climate have been like when the atmosphere was thicker?" said Michael Chaffin, a researcher at CU Boulder's Laboratory for Atmospheric and Space Physics (LASP) and a co-author of the study.
"Perhaps not as dry, but perhaps windier. We can't really say whether there would have been more dust storms or what their effect on loss of gas from the atmosphere would have been during those earlier conditions. A good way to improve our understanding about dust storms on ancient Mars would be to get more observations during a global dust storm on today's Mars."
More information: Nicholas G. Heavens et al. Hydrogen escape from Mars enhanced by deep convection in dust storms, Nature Astronomy (2018). DOI: 10.1038/s41550-017-0353-4
Journal information: Nature Astronomy
Provided by University of Colorado at Boulder