Deep Impact Overview: By The Numbers

To Strike a Comet: Astronomers Eager for Deep Impact’s Cosmic Collision
An artist's concept of Deep Impact's arrival at its target comet. The combination Flyby/Impactor spacecraft is expected to reach Comet Tempel 1 on July 4, 2005. (Image credit: NASA/Pat Rawlings.)

It's a match six years in the making and the underdog doesn't stand a chance, but that hasn't dampened the excitement of NASA's Deep Impact scientists one bit.

This July 4th, the agency's Impactor spacecraft--an 820-pound copper probe shaped like your typical living room coffee table--will go up against the comet Tempel 1, a massive hunk of rock and ice about the size of Washington D.C.

About the size of a Volkswagen Beetle automobile, Flyby is the larger of the two Deep Impact spacecrafts and will carry two of the mission's three primary research instruments.

Unlike the HRI, the Medium Resolution Instrument (MRI) will be able to take wide-angle shots of the entire comet. It has a maximum resolution of about 30 feet and will serve as HRI's backup. The MRI's wide field of view will be crucial for guiding Flyby spacecraft safely towards Tempel 1, especially during the last few days of the approach.

The final research instrument, the Impactor Targeting Sensor (ITS), is located on the Impactor spacecraft. The ITS is nearly identical to Flyby's MRI and will be used to guide Impactor to Tempel 1 during the final approach. It will also take pictures of the comet until the moment of impact.

Impactor's task is a difficult one. From a distance of more than half a million miles, it must aim for a sunny, well-lit spot on Tempel 1 that is less than 4 miles in diameter, all while zipping along at 23,000 miles per hour itself.

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Staff Writer

Ker Than is a science writer and children's book author who joined Space.com as a Staff Writer from 2005 to 2007. Ker covered astronomy and human spaceflight while at Space.com, including space shuttle launches, and has authored three science books for kids about earthquakes, stars and black holes. Ker's work has also appeared in National Geographic, Nature News, New Scientist and Sky & Telescope, among others. He earned a bachelor's degree in biology from UC Irvine and a master's degree in science journalism from New York University. Ker is currently the Director of Science Communications at Stanford University.