After a decade of searching, NASA’s MAVEN (Mars Atmosphere Volatile Evolution) mission has, for the first time, reported a direct observation of an elusive atmospheric escape process called sputtering that could help answer longstanding questions about the history of water loss on Mars.
Scientists have known for a long
time, through an abundance of evidence, that water was present on Mars’ surface
billions of years ago, but are still asking the crucial question, “Where did
the water go and why?”
Early on in Mars’ history, the
atmosphere of the Red Planet lost its magnetic field, and its atmosphere became
directly exposed to the solar wind and solar storms. As the atmosphere began to erode, liquid water was
no longer stable on the surface, so much of it escaped to space. But how did
this once thick atmosphere get stripped away? Sputtering could explain it.
Sputtering is an atmospheric escape
process in which atoms are knocked out of the atmosphere by energetic charge
particles.
“It’s like doing a cannonball in a
pool,” said Shannon Curry, principal investigator of MAVEN at the Laboratory
for Atmospheric and Space Physics at the University of Colorado Boulder and
lead author of the study. “The cannonball, in this case, is the heavy ions
crashing into the atmosphere really fast and splashing neutral atoms and
molecules out.”
While scientists had previously found traces of evidence that this process was happening, they had never
observed the process directly. The previous evidence came from looking at
lighter and heavier isotopes of argon in the upper atmosphere of Mars. Lighter
isotopes sit higher in the atmosphere than their heavier counterparts, and it
was found that there were far fewer lighter isotopes than heavy argon isotopes
in the Martian atmosphere. These lighter isotopes can only be removed by
sputtering.
“It is like we found the ashes from
a campfire,” said Curry. “But we wanted to see the actual fire, in this case
sputtering, directly.”
To observe sputtering, the team
needed simultaneous measurements in the right place at the right time from
three instruments aboard the MAVEN spacecraft: the Solar Wind Ion Analyzer, the
Magnetometer, and the Neutral Gas and Ion Mass Spectrometer. Additionally, the
team needed measurements across the dayside and the nightside of the planet at
low altitudes, which takes years to observe.
The combination of data from these
instruments allowed scientists to make a new kind of map of sputtered argon in
relation to the solar wind. This map revealed the presence of argon at high
altitudes in the exact locations that the energetic particles crashed into the
atmosphere and splashed out argon, showing sputtering in real time. The
researchers also found that this process is happening at a rate four times
higher than previously predicted and that this rate increases during solar
storms.
The direct observation of
sputtering confirms that the process was a primary source of atmospheric loss
in Mars’ early history when the Sun’s activity was much stronger.
“These results establish
sputtering’s role in the loss of Mars’ atmosphere and in determining the
history of water on Mars,” said Curry.
The finding, published this week in
Science Advances, is critical to scientists’ understanding of the conditions
that allowed liquid water to exist on the Martian surface, and the implications
that it has for habitability billions of years ago.
The MAVEN mission is part
of NASA’s Mars Exploration Program portfolio. MAVEN’s principal investigator is based at
the Laboratory for Atmospheric and Space Physics (LASP) at the University of
Colorado Boulder, which is also responsible for managing science operations and
public outreach and communications. NASA’s Goddard Space Flight
Center in Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space
built the spacecraft and is responsible for mission operations. NASA’s Jet
Propulsion Laboratory in Southern California provides navigation and Deep Space
Network support.
More information on NASA's MAVEN
mission
By Willow Reed
Laboratory for Atmospheric and Space Physics, University of Colorado Boulder
Source: NASA’s MAVEN Makes First Observation of Atmospheric Sputtering at Mars - NASA Science

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