October 5, 2010
After completing its primary mission to map the infrared sky, NASA's Wide-field Infrared Survey Explorer (WISE) has reached the expected end of its onboard supply of frozen coolant. Although WISE has "warmed up," NASA has decided the mission will still continue. WISE will now focus on our nearest neighbors — the asteroids and comets traveling together with our solar system's planets around the Sun.
"Two of our four infrared detectors still work even at warmer temperatures, so we can use those bands to continue our hunt for asteroids and comets," said Amy Mainzer of NASA's Jet Propulsion Laboratory in Pasadena, California. Mainzer is the principal investigator of the new phase of the mission, now known as the NEOWISE Post-Cryogenic Mission. A cryogen is a coolant used to make the detectors more sensitive. In WISE's case, the cryogen was frozen hydrogen.
WISE launched December 14, 2009, from Vandenberg Air Force Station in California aboard a Delta II launch vehicle. Its 16-inch infrared telescope scans the skies from an Earth-circling orbit crossing the poles. It has already snapped more than 1.8 million pictures at four infrared wavelengths. Currently, the survey has covered the sky about 1.5 times, producing a vast catalog containing hundreds of millions of objects from near-Earth asteroids to cool stars called brown dwarfs to distant, luminous galaxies.
To date, WISE has discovered 19 comets and more than 33,500 asteroids, including 120 near-Earth objects, which are those bodies with orbits that pass relatively close to Earth's path around the Sun. More discoveries regarding objects outside our solar system, such as the brown dwarfs and luminous galaxies, are expected.
"The science data collected by WISE will be used by the scientific community for decades," said Jaya Bajpayee from the Astrophysics Division of NASA's Science Mission Directorate at the agency's headquarters in Washington, D.C. "It will also provide a sky map for future observatories like NASA's James Webb Space Telescope."
The NEOWISE Post-Cryogenic Mission is designed to complete the survey of the solar system and finish the second survey of the rest of the sky at its new warmer temperature of about -334° Fahrenheit (-203° Celsius) using its two shortest wavelength detectors. The survey extension will last 1 to 4 months, depending on early results.
NEOWISE also will keep on observing other targets, such as the closest brown dwarfs to the Sun. In addition, data from the second sky scan will help identify objects that have moved in the sky since WISE first detected them. This allows astronomers to pick out the brown dwarfs closest to our Sun. The closer the object is, the more it will appear to move from our point of view.
The WISE science team now is analyzing millions of objects captured in the images, including many never seen before. A first batch of WISE data, covering more than half the sky, will be released to the astronomical community in spring 2011, with the rest to follow about 1 year later.
"WISE has provided a guidebook to the universe with thousands of targets worth viewing with a large telescope," said Edward Wright from the University of California, Los Angeles. "We're working on figuring out just how far away the brown dwarfs are, and how luminous the galaxies are."