First Light for MAVEN
 
Oct 10, 2014:  After 10-month voyage across more than 400 million miles of
empty space, NASA's MAVEN spacecraft reached Mars on Sept. 21st 2014.  Less
than 8 hours later, the data started to flow.
 
"Our Imaging Ultraviolet Spectrograph (IUVS) obtained these
false-color images of Mars on Sept. 22nd," says Nick Schneider who
leads the instrument team at the University of Colorado. "They trace
the distribution of hydrogen and oxygen in the Martian atmosphere."
 
https://www.youtube.com/watch?v=c_ez2G5Efus&feature=youtu.be
 
A new ScienceCast video presents MAVEN's first observations of the Martian
atmosphere.  Play it
 
MAVEN is on a mission to investigate a planetary mystery. Billions of years
ago, Mars was blanketed by an atmosphere massive enough to warm the planet
and allow liquid water to flow on its surface. Life could have thrived in
such an environment. Today, however, only a tiny fraction of that ancient
air remains, leaving Mars a desiccated wasteland.
 
What happened to the atmosphere of Mars? MAVEN will attempt to answer the
question by studying the upper atmosphere, where gaseous material could be
lost to space.
 
Schneider explains what the IUVS saw in its first look: "The oxygen
gas is held close to the planet by Mars' gravity, while lighter hydrogen
gas expands to higher altitudes and extends past the edges of the image.
These gases come from the breakdown of water and carbon dioxide in Mars'
atmosphere."
 
Among researchers, a popular candidate for atmospheric loss is space
weather: Eons of solar storms and the relentless buffeting of solar wind
might have stripped away much of the Martian atmosphere.
 
The IUVS might be able to see this process in action, especially in the
aftermath of a CME strike.
 
http://www.nasa.gov/mission_pages/maven/main/#.U-lkt2MYmsM
 
Click to visit the MAVEN home pageA CME, or coronal mass ejection, is a
billion-ton cloud of ionized gas blasted away from the sun in the aftermath
of a solar flare.  When CMEs hit Earth, they rattle our planet's magnetic
field, causing Northern Lights and, in extreme cases, power blackouts.
 
Unlike Earth, Mars has no global magnetic field to protect it.  For the
most part, the Martian atmosphere is unshielded. That's why gusts of solar
wind and CME strikes could strip material away.
 
"MAVEN's primary science goal is to see how the atmosphere responds to
solar forcing," says Bruce Jakosky, the Principal Investigator for
MAVEN. "So on the one hand, a CME might strip the outermost layers of
the atmosphere. On the other, it might also energize the atmosphere below
and repopulate the extended atmosphere with a lot of new material."
 
Either way, he says, "we expect to see something."
 
The instrument is also capable of observing Martian auroras.  Here on
Earth, auroras ring the magnetic poles, north and south.  Mars, however,
has a different magnetic structure.  There is no coherent global magnetic
field. Instead, Mars has a patchwork of magnetic umbrellas that sprout out
of the surface in hundreds of places all around the planet.  If Martian
auroras occur, they would appear in the canopies of those umbrellas.
 
"We are on the edges of our seats, hoping for our first
detection," says Schneider.
 
Having just reached Mars, MAVEN is still in its commissioning phase.
Instruments are being checked out, the spacecraft's orbit is being
adjusted. The fact that data are already arriving at Earth is an impressive
achievement.
 
This is just the beginning.  IUVS is only one of three instrument suites on
MAVEN.  The Neutral Gas and Ion Spectrometer from the Goddard Space Flight
Center and the Particles and Fields Package from UC Berkeley will soon be
making their own revelations about Mars.
 
Stay tuned for updates.
 
Credits:
Author: Dr. Tony Phillips | Production editor: Dr. Tony Phillips | Credit:
Science{at}NASA
 
More information:
 
NASA Science Fleet Prepares for Mars Comet -- Science{at}NASA
 
Colliding Atmospheres: Mars vs. Comet Siding Spring -- Science{at}NASA
 
 
Regards,
 
Roger

--- D'Bridge 3.99