Artist impression of the NEOWISE mission.
Credit: JPL/NASA
After two years of operations, the NEOWISE space mission is consistently beating ground-based telescopes in its fraction of detected possibly dangerous asteroids to Earth.
While overall near-Earth NEOWISE asteroid discoveries are tiny — this NASA site says NEOWISE found 34 in its second year — 13 of those asteroids have orbits that bring them really close to Earth, putting them in the “potentially hazardous” category. As a fraction of discoveries, NEOWISE’s haul of potentially hazardous asteroids exceeds ground-based surveys by a factor of three, a new paper says.
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The paper (available on Arxiv and set to publish in the Astronomical Journal) was released just before its investigators find out if the successor mission to NEOWISE will be approved. Called NEOCam or Near-Earth Object Camera, the mission is one of five being considered for NASA’s next round of lower-cost Discovery-class missions. A decision is expected in September, with the selected mission launching in 2021.
Meanwhile, NEOWISE is still going strong as it enters its third and likely final year of operations in Earth orbit, according to status updates on the website. In 2017 it is expected to enter an orbital zone too sunny for observations.
NEOWISE took a series of images of Comet PanSTARRS 2012 K1 in May 2014.
Credit: NASA/JPL-Caltech
“As of mid-June 2016, NEOWISE has completed its fifth coverage of the entire sky and is beginning the sixth pass,” the website says, adding that 541 near-Earth objects and 99 comets have been surveyed so far (among more than 20,000 solar system objects).
The investigators are now reprocessing the mission data to seek asteroids and comets at even fainter magnitudes. They’re also cataloging the asteroid and comet properties they have to deliver to NASA’s Planetary Data SystemPlanetary Data System.
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NEOWISE comes from a base telescope has already endured a two-year hibernation and subsequent restart since the first mission, the Wide-field Infrared Survey Explorer (WISE), launched in 2009.
WISE scanned the sky in four infrared wavelengths until its coolant ran out in 2010. NEOWISE began as a four-month mission scanning the sky in 2011 using the two shortest wavelength detectors. NEOWISE went into hibernation in 2011, then was brought out again in 2013.
NEOWISE caught Comet C/2013 UQ4 (Catalina)’s high activity after reaching the closest point of its orbit to the sun in 2013.
Credit: NASA/JPL-Caltech
Among NEOWISE’s major contributions to asteroid science is refining the size of many known asteroids. In its second year alone, 84% of the 207 near-Earth asteroids NEOWISE observed were missing precise diameters and albedos (brightness) until it did measurements.
“Using visible wavelengths of light, it is difficult to tell if an asteroid is big and dark, or bright and small, because both combinations reflect the same amount of light,” Carrie Nugent, a NEOWISE scientist at the California Institute of Technology, explained in a 2015 NASA press release.
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“But when you look at an asteroid in the infrared with NEOWISE, the amount of infrared light corresponds with how big the asteroid is, and with some thermal models on a computer, you can figure out how big the asteroids are.”
The new paper summarizing NEOWISE’s second year was led by Nugent and co-authored by NEOWISE principal investigator Amy Mainzer. Both were unavailable for interviews before this article’s publication date due to work on a large project, they told Discovery News.
Originally published on Discovery News.
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