Website Lets Users Scout the Red Planet from Home

For those who want to explore Mars but can't wait for a spacecraft to take them there, NASA scientists have reformulated a website that lets the general public search data and images from previous missions.

The website called Marsoweb had been designed to help scientists select possible landing sites for the Mars Exploration Rovers. By making the web pages more user friendly, NASA hopes that space enthusiasts will electronically survey the red planet's terrain for interesting geological features.

However, many Mars lovers already know about the site. About a half million people have visited Marsoweb. "Armchair planetary astronomers probably found it through Google," said Glenn Deardorff, a computer scientists, who has worked on Marsoweb for over four years. In January, the site recorded 26.7 million "hits" when the first rover, Spirit, landed.

Also on display are the candidate landing sites for the Mars Exploration Rover 2003 missions. Laypersons can try to discern the selection process that mission organizers went through. "It isn't easy to find an overlap," Deardorff said, "between something scientifically interesting and a good landing spot from an engineering perspective."

In some ways, Marsoweb is a test bed for the software that will be needed for the High Resolution Imaging Science Experiment (HiRISE), scheduled to go up with the Mars Reconnaissance Orbiter in 2005. HiRISE should be able to view objects on the surface with one-meter resolution, which will allow better identification of geological features. The public will be able to peruse these images and put in requests for follow-up observations. For this reason, NASA is touting HiRISE as "the people's camera."

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Michael Schirber
Contributing Writer

Michael Schirber is a freelance writer based in Lyons, France who began writing for Space.com and Live Science in 2004 . He's covered a wide range of topics for Space.com and Live Science, from the origin of life to the physics of NASCAR driving. He also authored a long series of articles about environmental technology. Michael earned a Ph.D. in astrophysics from Ohio State University while studying quasars and the ultraviolet background. Over the years, Michael has also written for Science, Physics World, and New Scientist, most recently as a corresponding editor for Physics.