Mars Express Radar Gauges Water Quantity Around Martian South Pole

MARSDAILY

The upper image of this composite is a 'radargram' from the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) on board ESA's Mars Express. It shows data from the subsurface of Mars in the water-ice-rich layered deposits that surround the south pole of the planet. The lower image shows the position of the ground track of the spacecraft (indicated by a white line) on a topographic map of the area based on data from the MOLA laser altimeter on board NASA's Mars Global Surveyor. The MARSIS radar echo trace splits into two traces on the left side of the image, at the point where the ground track crosses from the surrounding plains onto elevated layered deposits. The upper trace is the echo from the surface of the deposits, while the lower trace is interpreted to be the boundary between the lower surface of the deposits and the underlying material. The strength of the lower echo suggests that the intervening material is nearly pure water ice. Near the image center, the bright lower echo abruptly disappears for unknown reasons. The time delay between the two echoes reaches a maximum of 42 microseconds left of center, corresponding to a thickness of 3.5 kilometres of ice. The total elevation difference shown in the topographic map is about 4 kilometres between the lowest surface (purple) and the highest (red). Credits: NASA/JPL/ASI/ESA/Univ. of Rome/MOLA Science Team

Additional images at ESA

by Staff Writers
Paris, France (ESA) Mar 16, 2007
The amount of water trapped in frozen layers over Mars' south polar region is equivalent to a liquid layer about 11 metres deep covering the planet. This new estimate comes from mapping the thickness of the dusty ice by the Mars Express radar instrument that has made more than 300 virtual slices through layered deposits covering the pole. The radar sees through icy layers to the lower boundary, which in places is as deep as 3.7 kilometres below the surface.

"The south polar layered deposits of Mars cover an area as wide as a big portion of Europe. The amount of water they contain has been estimated before, but never with the level of confidence this radar makes possible," said Dr Jeffrey Plaut of NASA's Jet Propulsion Laboratory, Pasadena (California), co-Principal Investigator for the radar and lead author of the study.

The instrument, named the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS), is also mapping the thickness of similar layered deposits at the north pole of Mars.

"Our radar is doing its job extremely well," said Prof. Giovanni Picardi of the University of Rome 'La Sapienza', Principal Investigator for the instrument. "MARSIS is showing to be a very powerful tool to probe underneath the Martian surface, and it's showing how our team's goals - such as probing the polar layered deposits - are being successfully achieved," he continued.

"Not only MARSIS is providing us with the first ever views of Mars' subsurface at those depths, but the details we are seeing are truly amazing. We are expecting even greater results when we will have concluded an on-going, sophisticated fine-tuning of our data processing methods. These should enable us to understand even better the surface and subsurface composition."

Polar layered deposits hold most of the known water on modern Mars, though other areas of the planet appear to have been very wet at times in the past. Understanding the history and fate of water on Mars is a key to studying whether Mars has ever supported life, because all known life depends on liquid water.

Plaut, Picardi and 22 other researchers report analysis of the Mars Express radar instrument's south polar observations in the online edition of the journal Science this week.

The polar layered deposits extend beyond and beneath a polar cap of bright-white frozen carbon dioxide and water at Mars' south pole. Dust darkens many of the layers. However, the strength of the echo that the radar receives from the rocky surface underneath the layered deposits suggests the composition of the layered deposits is at least 90 percent frozen water.

One area with an especially bright reflection from the base of the deposits puzzles researchers. It resembles what a thin layer of liquid water might look like to the radar instrument, but the conditions are so cold that the presence of melted water is deemed highly unlikely.

Detecting the shape of the ground surface beneath the ice deposits provides information about even deeper structure of Mars. "We didn't really know where the bottom of the deposit was," Plaut said. "We can see now that the crust has not been depressed by the weight of the ice as it would be on the Earth. The crust and upper mantle of Mars are stiffer than the Earth's, probably because the interior of Mars is so much colder."

The results appear in the 15 March 2007 issue of the Science magazine, in an article by J. Plaut, G. Picardi et al., titled: "Subsurface Radar Sounding of the South Polar Layered Deposits of Mars."

Community
Email This Article
Comment On This Article

Related Links
Mars Express instruments
MARSIS team website
MARSIS at NASA JPL
Mars News and Information at MarsDaily.com
Mars News and Information at MarsDaily.com
Lunar Dreams and more

Memory Foam Mattress Review

SPACE MEDIA NETWORK PROMOTIONS
Solar Energy Solutions
Tempur-Pedic Mattress Comparison ...

Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News

MARSDAILY

NASA Mars Rover Churns Up Questions With Sulfur-Rich Soil

Pasadena CA (JPL) Mar 15, 2007
Some bright Martian soil containing lots of sulfur and a trace of water intrigues researchers who are studying information provided by NASA's Spirit rover.

NUCLEAR SPACE Could NASA Get To Pluto Faster? Space Expert Says Yes - By Thinking Nuclear NASA plans to send new robot to Jupiter Los Alamos Hopes To Lead New Era Of Nuclear Space Tranportion With Jovian Mission Boeing Selects Leader for Nuclear Space Systems Program	MOON DAILY Shooting Marbles At Four Miles A Second A SMART Bridge To The Future Exploration Of The Moon First Chinese Lunar Probe Assembled And Ready For Launch The Edge Of Luna Incognita By SMART-1
SPACE TRAVEL Russia To Shut Down Svobodny Space Centre The Story Of Women In Space NASA To Host Space University Session JAXA Hosts Kyoto Workshop For Global Space Exploration Strategy	OUTER PLANETS Smash And Grab On The Edge Of Sol Billions Of Year Ago Jupiter Play Back Begins As Downlink Initiated From New Horizons The Tip of the Iceberg New Horizons Completes First Stage Of Long Journey To Pluto And Beyond
JOVIAN DREAMS The Alien Volcano Of Io Is A Tvashtar Juno Gets A Little Bigger With One More Payload For Jovian Delivery Plume Of Tvashtar Rises From Io Jovian Junior Red Spot Growing Stronger	VENUSIAN HEAT Hot stuff on Venus! Venus Express Sees Right Down To The Hell-Hot Surface Saturn Joins Venus In The Vortex Club Venus Express Program Wins Popular Science Award
SATURN DAILY Cassini Spacecraft Images Seas Of Titan A Hot Start Might Explain Geysers on Enceladus Huygens Landing Site To Be Named After Hubert Curien Cassini Returns Never-Before-Seen Views Of The Ringed Planet	TECH SPACE Saab Space To Supply Antennas For New Generation Direct-To-Mobile Satellites Virtual Reality For Virtual Eternity Boeing Orbital Express to Demonstrate New On-Orbit Servicing Capability Austin Physicists Slow And Control Supersonic Helium Beam

The content herein, unless otherwise known to be public domain, are Copyright 1995-2006 - SpaceDaily.AFP and UPI Wire Stories are copyright Agence France-Presse and United Press International. ESA PortalReports are copyright European Space Agency. All NASA sourced material is public domain. Additionalcopyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by SpaceDaily on any Web page published or hosted by SpaceDaily. Privacy Statement