Marsquake Detection Sensors Will Take Search For Water Underground

MARSDAILY

our future on ice

File image: Looking west from from Valles Marineris to the three Mons, Arsia, Pavonis and Olympus. 3D Rending based on MOC and MOLA data from MGS. Imaging designed and processed by Kees Veenenbos

London - Jun 03, 2002
Researchers at Imperial College London have just begun a 5-year project to design and build tiny earthquake measuring devices to go to Mars on the 2007 NetLander mission.

Unlike the instruments on next year's European Mars Express/Beagle II mission, the Marsquake sensors will be the first to look deep inside the planet.

The internal structure of Mars is a key to understanding some fundamental questions about the planet including whether life ever existed there.

The sensors are capable of detecting liquid water reservoirs hidden below the surface, where life could possibly survive on Mars today.

The recent discovery by the Mars Odyssey orbiter of large amounts of ice at the poles opens up the possibility of liquid water existing in the warmer conditions underground near the Martian equator.

Dr Tom Pike, of Imperial College London, is designing the heart of the sensor, a two-centimetre square of silicon.

"We're micromachining a near-perfect spring and weight from a single piece of silicon. We'll be able to detect the weight shuddering in response to a Marsquake from anywhere on the planet," he said.

The 2007 NetLander mission, led by the French space agency, CNES, will land four modules across the surface of Mars, each containing instruments to look at the structure and weather of Mars on a global scale. All four will be near the equator.

"The network of instruments will help us to pinpoint each Marsquake by triangulation," said Dr Pike. "We'll look at how the vibrations from Marsquakes travel through the planet and work out what's going on deep inside. If these vibrations hit liquid water under the landing sites, we should see a distinctive signature. That's when the search for life on Mars will move underground."

Dr Pike is currently building up the team at Imperial College to develop the sensors under a contract from the Jet Propulsion Laboratory. The Rutherford Appleton Laboratory, Oxfordshire, is providing the fabrication facilities. The Marsquake instrument consortium includes Imperial College, NASA's Jet Propulsion Laboratory in Pasadena, the Institute de Physique du Globe in Paris and ETH, Zurich.

MARSDAILY

The Carbon Versus Water Battle Goes Hemispherical

Pasadena - Mar 21, 2002
When astronauts finally land on Mars, a safe bet is that they'll head for northern climes if they intend to spend much time there. That's because nearly all the available water is frozen as ice at the north pole. Planetary scientists have been aware of this for some time, but they now have a new clue why it is so.

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