Search Menu
Photonics Media Photonics Buyers' Guide Photonics EDU Photonics Spectra BioPhotonics EuroPhotonics Industrial Photonics Photonics Showcase Photonics ProdSpec Photonics Handbook
More News
Email Facebook Twitter Google+ LinkedIn Comments

Gazing outward, growing wiser

Photonics Spectra
Feb 2011
Lynn Savage,

In December, NASA’s Wide-field Infrared Survey Explorer (WISE) celebrated one full year of exploring the universe using four different bands of IR detection. The image here represents just a small fraction of the sky catalogued by the satellite during its operational run.

The image shows three nebulae that are part of the Orion molecular cloud: the Flame nebula, the Horsehead nebula and NGC 2023. The Flame nebula appears to be kindled by the bright blue star to the right of the central cloud. This star, dubbed Alnitak, is the easternmost star in the belt of the constellation Orion. The radiance captured by the satellite’s imagers originates from dust that has been heated by Alnitak.

Image courtesy of NASA.

NGC 2023 can be seen as a bright circle in the lower part of the image. It is a reflection nebula, meaning that the dust is reflecting the visible light of nearby stars. WISE, however, sees the IR glow of the warmed dust itself.

Between NGC 2023 and the Flame, the famous Horsehead nebula appears as a ghostly bump on the lower right of the vertical dust ridge. In visible wavelengths, the Horsehead is easily discerned; again, the IR detectors aboard WISE peer into the cloud to see the glow of the interstellar dust.

WISE incorporates four sensors, each with 1024 x 1024 pixels, recording near-IR bands at 3.4 and 4.6 μm and mid-IR bands at 12 and 22 µm. The near-IR sensors are composed of HgCdTe; the mid-IR ones, Si:As. Blue represents light emitted at 3.4 μm, which comes mainly from hot stars. Relatively cooler objects, such as the dust of the nebulae, are shown as green (4.6 μm) and red (12 μm). The image was made from data collected after WISE (as expected) began to run out of its supply of solid hydrogen cryogen almost nine months into its mission. From August to October 2010, while the cryogen was depleting, the satellite had only three detectors operational, and the 12-μm detector was less sensitive. This turned out to be a good thing, because the less sensitive detector reduced the glare of the Flame portion of the nebula enough to bring out the details in the rest of the image.

The scientific observation of celestial radiation that has reached the vicinity of Earth, and the interpretation of these observations to determine the characteristics of the extraterrestrial bodies and phenomena that have emitted the radiation.
astronomyBasic ScienceFlame nebulaHgCdTeHorsehead nebulaimaginginfraredLighter SideNASANGC 2023Orion Molecular Cloudsatellite imagingSensors & DetectorsSi:Assky catalogueWide-field Infrared Survey Explorer

Terms & Conditions Privacy Policy About Us Contact Us
back to top
Facebook Twitter Instagram LinkedIn YouTube RSS
©2018 Photonics Media, 100 West St., Pittsfield, MA, 01201 USA,

Photonics Media, Laurin Publishing
x Subscribe to Photonics Spectra magazine - FREE!
We use cookies to improve user experience and analyze our website traffic as stated in our Privacy Policy. By using this website, you agree to the use of cookies unless you have disabled them.