This ad will auto close in 10 seconds

Asteroid tracking infrared sensor passes key test

Last Updated: Tuesday, April 16, 2013 - 12:26

Washington: A NASA funded infrared sensor that could improve the agency`s future detecting and tracking of asteroids and comets has passed a critical design test.

The test assessed performance of the Near Earth Object Camera (NEOCam) in an environment that mimicked the temperatures and pressures of deep space. NEOCam is the cornerstone instrument for a proposed new space-based asteroid-hunting telescope.

The sensor could be a vital component to inform plans for the agency`s recently announced initiative to develop the first-ever mission to identify, capture and relocate an asteroid closer to Earth for future exploration by astronauts.

"This sensor represents one of many investments made by NASA`s Discovery Program and its Astrophysics Research and Analysis Program in innovative technologies to significantly improve future missions designed to protect Earth from potentially hazardous asteroids," said Lindley Johnson, program executive for NASA`s Near-Earth Object Program Office in Washington.

Near-Earth objects are asteroids and comets with orbits that come within 28 million miles of Earth`s path around the Sun. Asteroids do not emit visible light, they reflect it. Depending on how reflective an object is, a small, light-colored space rock can look the same as a big, dark one. As a result, data collected with optical telescopes using visible light can be deceiving.

"Infrared sensors are a powerful tool for discovering, cataloging and understanding the asteroid population," said Amy Mainzer, a co-author of the paper and principal investigator for NASA`s NEOWISE mission at the agency`s Jet Propulsion Laboratory (JPL) in Pasadena, Calif.

NEOWISE stands for Near-Earth Object Wide-Field Infrared Survey Explorer.

The NEOCam sensor is designed to be more reliable and significantly lighter in weight for launching aboard space-based telescopes. Once launched, the proposed telescope would be located about four times the distance between Earth and the moon where NEOCam could observe the comings and goings of NEOs every day without the impediments of cloud cover and daylight.

The sensor is the culmination of almost 10 years of scientific collaboration between JPL; the University of Rochester, which facilitated the test; and Teledyne Imaging Sensors of Camarillo, California, which developed the sensor.

Details of the sensor`s design and capabilities are published in an upcoming edition of the Journal of Optical Engineering.


First Published: Tuesday, April 16, 2013 - 12:26
comments powered by Disqus