Scientist finds Martian ice is patchy and variable

May 02, 2007
Scientist finds Martian ice is patchy and variable
This color-coded map indicates the depth to icy layers at a site in southern Mars. The dense, icy layer retains heat better than the looser soil above it, so where the icy layer is closer to the surface, the surface temperature changes more slowly than where the icy layer is buried deeper. Image credit: NASA/JPL/ASU

For the first time, scientists have found that water ice lies at variable depths over small-scale patches on the Red Planet. The discovery draws a much more detailed picture of underground ice on Mars than was previously available. The new results appear in the May 3 issue of the scientific journal Nature.

"We find the top layer of soil has a huge effect on the water ice in the ground," says Joshua Bandfield, a research specialist in Arizona State University's School of Earth and Space Exploration and sole author of the paper. His findings come from data sent back to Earth by the Thermal Emission Imaging System (THEMIS) on NASA's Mars Odyssey orbiter.

THEMIS is a sophisticated camera that takes images in 5 visual bands and 10 heat-sensing (infrared) ones. At infrared wavelengths, the smallest details THEMIS can see on the surface are 330 feet (100 meters) wide.

The new results were made using infrared images of several Martian sites, each at a latitude of 60 to 70 degrees, north and south. "These sites are in regions where subsurface water ice is known to exist," Bandfield says.

THEMIS' Sharp View

He explains that water ice lying at shallow depths was first detected and mapped by the Gamma Ray Spectrometer (GRS) suite of instruments, also on Mars Odyssey. But, as Bandfield notes, "the smallest patches detectable by GRS are 300 miles, or 500 kilometers, wide." The new work shows that THEMIS' heat-sensing capability gives scientists a much sharper tool to hunt for buried ice.

"Scientists have known for more than a decade that water is on Mars, mostly in the form of ice," says Philip Christensen of ASU's Mars Space Flight Facility. Christensen, a Regents' Professor of geological sciences at ASU, designed THEMIS but did not participate in this research. "What's exciting is finding out where the ice is in detail and how it got there. We've reached the next level of sophistication in our questions."

Christensen adds, "GRS can probe a meter deep, but it has a giant footprint. Most infrared spectrometers can detect surface ice and ice a few fractions of a millimeter down. THEMIS is sensitive to thermal waves which can penetrate several inches deep – and it can spot details the size of a football field."

Seeking Warmth

Bandfield's approach used THEMIS as a thermometer to measure how fast the ground changed temperature during local spring, summer and fall at the sites. The nature of the surface soil, he says, "makes a big difference in how deep the ice is."

Areas with many rocks at the surface, Bandfield explains, "pump a lot of heat into the ground and increase the depth where you'll find stable ice." In contrast, he says, dusty areas tend to insulate the ice, allowing it to survive closer to the surface. "These two surface materials – rock and dust – vary widely across the ground, giving underground ice a patchy distribution."

Computer models helped him interpret the temperature observations, he says. "They show areas where water ice would be only an inch or so under the soil, while in other areas ice could lie many feet below the surface."

Mars Climate Cycles

Bandfield notes the results fit long-term climatic models for Mars. These show the planet has been both warmer and colder in the past, similar to glacial cycles on Earth.

He says, "The fact that ice is present near the depth of stability in the current Martian climate shows that the ground ice is responding to climate cycles." In turn, he adds, this implies that water ice in the ground can swap places with water vapor in the atmosphere as the climate changes.

Bandfield concludes, "The THEMIS measurements support an active water cycle on Mars such as other research has predicted."

"This work has improved our understanding of the water cycle as part of the ongoing exploration of Mars," says Christensen.

Phoenix: Hunting For Ice

In August 2007, NASA will launch Phoenix, a mission designed to sample Martian ground ice directly. The Phoenix spacecraft is a non-roving lander that will go to a high-latitude site in Mars' northern hemisphere. Upon landing, it will expose buried ice by scraping away the soil. After collecting a sample of icy soil, Phoenix will analyze its qualities as a possible habitat for microbial life.

Says Bandfield, "The take-home message for the Phoenix lander is that the THEMIS results show a lot of patchiness in the ground ice, and this should continue down to smaller and smaller scales."

Phoenix, he adds, "may find ground ice is shallower and much easier to reach in some spots than in others."

Source: Arizona State University

Explore further: Video gives astronaut's-eye view inside NASA's Orion spacecraft

add to favorites email to friend print save as pdf

Related Stories

Comet 67P/Churyumov-Gerasimenko in living color

Dec 12, 2014

Rosetta's OSIRIS team have produced a color image of Comet 67P/Churyumov-Gerasimenko as it would be seen by the human eye. As anticipated, the comet turns out to be very grey indeed, with only slight, subtle ...

Recommended for you

SDO captures images of two mid-level flares

Dec 19, 2014

The sun emitted a mid-level flare on Dec. 18, 2014, at 4:58 p.m. EST. NASA's Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts ...

Why is Venus so horrible?

Dec 19, 2014

Venus sucks. Seriously, it's the worst. The global temperature is as hot as an oven, the atmospheric pressure is 90 times Earth, and it rains sulfuric acid. Every part of the surface of Venus would kill you ...

Image: Christmas wrapping the Sentinel-3A antenna

Dec 19, 2014

The moment a team of technicians, gowned like hospital surgeons, wraps the Sentinel-3A radar altimeter in multilayer insulation to protect it from the temperature extremes found in Earth orbit.

Video: Flying over Becquerel

Dec 19, 2014

This latest release from the camera on ESA's Mars Express is a simulated flight over the Becquerel crater, showing large-scale deposits of sedimentary material.

User comments : 0

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.