The latest NASA "Image of the Day" image.

Decorating the Sky
This mosaic image taken by NASA's Wide-field Infrared Survey Explorer, or WISE, features three nebulae that are part of the giant Orion Molecular Cloud--the Flame nebula, the Horsehead nebula and NGC 2023.
This mosaic image taken by NASA's Wide-field Infrared Survey Explorer, or WISE, features three nebulae that are part of the giant Orion Molecular Cloud--the Flame nebula, the Horsehead nebula and NGC 2023.
Despite its  name, there is no fire roaring in the Flame nebula. What makes this  nebula shine is the bright blue star seen to the right of the central  cloud. This star, Alnitak, is the easternmost star in Orion's belt. Wind  and radiation from Alnitak blasts away electrons from the gas in the  Flame nebula, causing it to become ionized and glow in visible light.  The infrared glow seen by WISE is from dust warmed by Alnitak's  radiation. 
The famous Horsehead nebula appears in this image as a faint  bump on the lower right side of the vertical dust ridge. In visible  light, this nebula is easily recognizable as a dramatic silhouette in  the shape of a horse's head. It is classified as a dark nebula because  the dense cloud blocks out the visible light of the glowing gas behind  it. WISE's infrared detectors can peer into the cloud to see the glow of  the dust itself. A third nebula, NGC 2023, can be seen as a bright  circle in the lower half of the image. NGC 2023 is classified as a  reflection nebula, meaning that the dust is reflecting the visible light  of nearby stars. 
But here WISE sees the infrared glow of the warmed  dust itself. Color in this image represents specific infrared  wavelengths. Blue represents light emitted at 3.4-micron wavelengths,  mainly from hot stars. Relatively cooler objects, such as the dust of  the nebulae, appear green and red. Green represents 4.6-micron light and  red represents 12-micron light. This image was made from data collected  after WISE began to run out of its supply of solid hydrogen cryogen in  August 2010. Cryogen is a coolant used to make infrared detectors more  sensitive. WISE mapped the entire sky by July using four infrared  detectors, but during the period from August to October 2010, while the  cryogen was depleting, WISE had only three detectors operational, and  the 12-micron detector was less sensitive. 
This turned out to be a good  thing in the case of this image, because the less-sensitive detector  reduced the glare of the Flame portion of the nebula enough to bring out  details of the rest of the nebula.
 Image Credit: NASA/JPL-Caltech/UCLA
Δευτέρα, 27 Δεκέμβριος 2010 7:00:00 πμ
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