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Deep Impact Team Reports First Evidence of Cometary Ice
02.03.2006

Three small areas of water ice on the surface of Tempel 1
The three small areas of water ice on the surface of Tempel 1 appear in this image, taken by an instrument aboard NASA's Deep Impact spacecraft.

Comet Tempel 1, target of last year's July 4 cosmic collision, contains small amounts of surface water ice. These results, reported by members of NASA's Deep Impact team in an advanced online edition of Science, offer the first definitive evidence of surface ice on any comet

"We have known for a long time that water ice exists in comets, but this is the first evidence of water ice on comets," said Jessica Sunshine, Deep Impact co-investigator and lead author of the Science article.

"Understanding a comet's water cycle and supply is critical to understanding these bodies as a system and as a possible source that delivered water to Earth," she said. "Add the large organic component in comets and you have two of the key ingredients for life."

The findings help satisfy one of the major goals of the Deep Impact mission: Find out what is on the inside -- and outside -- of a comet. Since the July 4 encounter, the Deep Impact team has reported a few key findings. These include an abundance of organic matter in Tempel 1's interior as well as its likely origins -- the region of the solar system now occupied by Uranus and Neptune.

According to the new research in Science, the comet's surface features three pockets of thin ice. The area the ice covers is small. The surface area of Tempel 1 is roughly 45 square miles or 1.2 billion square feet. The ice, however, covers roughly 300,000 square feet. And only 6 percent of that area consists of pure water ice. The rest is dust.

"It's like a seven-acre skating rink of snowy dirt," said Peter Schultz, professor of geological sciences at Brown University, Deep Impact co-investigator and co-author on the Science paper.

Sunshine, Schultz and the rest of the team arrived at their findings by analyzing data captured by an infrared spectrometer, an optical instrument that uses light to determine the composition of matter.

Based on this spectral data, it appears that the surface ice used to be inside Tempel 1 but became exposed over time. The team reports that jets -- occasional blasts of dust and vapor -- may send this surface ice, as well as interior ice, to the coma, or tail, of Tempel 1.

"So we know we're looking at a geologically active body whose surface is changing over time," Schultz said. "Now we can begin to understand how and why these jets erupt."

 

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