PIA14092: Nebulae: Not as Close as They Appear
 Mission:  Wide-field Infrared Survey Explorer (WISE)
 Instrument:  WISE Telescope
 Product Size:  5500 x 2830 pixels (w x h)
 Produced By:  IPAC-Caltech
 Full-Res TIFF:  PIA14092.tif (46.7 MB)
 Full-Res JPEG:  PIA14092.jpg (1.215 MB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

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This latest image from NASA's Wide-field Infrared Survey Explorer, or WISE, shows three different nebulae located in the constellation of Perseus. NGC 1491 is seen on the right side of the image, SH 2-209 is on the left side and BFS 34 lies in between. The picture covers an area on the sky equal to 8 full moons.

It is easy to think that celestial objects like the three in this image are located at the same distance from Earth, as if they were placed on the dome of a planetarium. In reality, objects that appear close together on the sky can actually be quite far apart. In this case, NGC 1491 and BFS 34 are part of the same cloud complex located at a distance of about 10,700 light-years away in the Perseus arm of the Milky Way Galaxy. SH 2-209 is farther away at about 16,000 light-years distance, located in the outer arm of the Milky Way. NGC 1491 can be seen in visible light with an optical telescope. In contrast, SH 2-209 disappears completely in visible light, obscured by dust.

Although they are not structurally associated with each other, the nebulae do have much in common. All three are members of the same "family" of objects called HII regions by astronomers. HII regions are created when ultraviolet radiation from hot stars ionizes the surrounding gas, causing it to glow in visible light. The surrounding dust is also heated by this radiation and we see it glow in infrared light. These regions are well known for being places where new stars are born. In this image, the star cluster [BDS2003] 65 is developing within the SH 2-206 nebula. The bright spot in the center of BFS 34 nebula is the growing star cluster [BDS2003] 63.

Color in this image represents specific wavelengths of infrared light. Blue and cyan (blue-green) represent wavelengths of 3.4 and 4.6 microns, respectively. In this image, most of the light emitted at these wavelengths is from hot stars. Green and red represent 12- and 22-micron light, which is mainly from warm dust.

JPL manages the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate, Washington. The principal investigator, Edward Wright, is at UCLA. The mission was competitively selected under NASA's Explorers Program managed by the Goddard Space Flight Center, Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory, Logan, Utah, and the spacecraft was built by Ball Aerospace & Technologies Corp., Boulder, Colo. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA.

More information is online at http://www.nasa.gov/wise and http://wise.astro.ucla.edu.

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