Press Release

“THOR” Mars Mission to Seek Underground Water

By SpaceRef Editor
January 26, 2006
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“THOR” Mars Mission to Seek Underground Water
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A bold, new robotic mission to Mars proposes to make the first exploration of subsurface water ice in a potentially habitable zone.

THOR, a low-cost mission designed for NASA’s Mars Scout program, aims to send a projectile at high speed into the martian surface while observing the impact and its aftermath. The mission is led by Arizona State University in Tempe, in partnership with the Jet Propulsion Laboratory (JPL).

Planned for launch in 2011, THOR (Tracing Habitability, Organics, and Resources) will use a direct approach to excavating material from beneath the surface of Mars: blasting it out.

“The mission’s goal is to expose snow and ice in a previously unexplored part of Mars — the deep subsurface. We’ll do this by blowing a crater at least 30 feet deep in the martian ground,” says THOR’s principal investigator Phil Christensen of Arizona State University’s Mars Space Flight Facility.

Besides finding underground water, he says, THOR will also look for organic compounds, including methane, which Earth-based telescopes and other Mars spacecraft have detected in the martian atmosphere.

The proposed THOR mission will use a two-part spacecraft consisting of an impactor probe and an observer craft. The impactor is a simple projectile made of pure Arizona copper. The observer spacecraft will carry it until shortly before reaching Mars. After being released from the observer, the impactor will streak through the martian atmosphere to an impact site lying between 30° and 60° latitude, in either the northern or southern hemisphere.

“In many areas of Mars’ middle latitudes, we see tantalizing evidence of dust-covered layers of snow or ice,” says Christensen. “THOR will aim for this material.” The suspected ice-rich layers were deposited during the past 50,000 to 1 million years, as the martian climate changed due to orbital variations.

According to the mission plan, when the impactor slams into the ground, it will dig a crater more than 30 feet (10 meters) deep. The observer spacecraft will study the debris plume jetting from the impact site.

The observer’s instruments will include a visible-light camera and an infrared spectrometer. In addition to studying the plume, the spectrometer’s role is to search the martian atmosphere for organic materials and gases such as methane.

In the past, Christensen notes, Mars has been studied using flyby and orbiter spacecraft, and with landers. While highly valuable, such missions have only scratched the surface, he says. “The time has come to take martian studies a step further — and deeper.”

Christensen adds, “This unexplored region of Mars may provide chemical and mineral clues to tell us about habitable areas on the planet.”

“The THOR mission plans to use a straightforward, low-risk approach to reach the martian subsurface,” says JPL’s David Spencer, study lead engineer for THOR. Spencer is the former mission manager for Deep Impact, the comet mission that pioneered the impact technique. Comparing the two missions, Spencer says, “With such a large target region on Mars, delivering THOR¹s impactor will be less challenging than the Deep Impact comet encounter.”

Christensen sees THOR’s scientific value continuing far beyond the impact. “THOR’s crater will remain a test-site for all current Mars spacecraft and those in years to come,” he says. Moreover, he points out, “the crater might also be visited on the ground by a future Mars rover, sometime in the next decade.”

NASA’s Mars Scouts are competitively proposed missions designed to advance the goals of NASA’s Mars exploration program. The Mars Scout Program is managed by JPL for NASA’s Office of Space Science, Washington.

SpaceRef staff editor.