Cygnus-X: The Cool Swan Glowing in Flight
This new view of the Cygnus-X star-formation region by Herschel highlights chaotic networks of dust and gas that point to sites of massive star formation. The image combines far-infrared data acquired at 70 micron (corresponding to the blue channel); 160 micron (corresponding to the green channel); and 250 micron (corresponding to the red channel). The observations were made on May 24, 2010, and December 18, 2010. North is to the lower-right and east to the upper-right.
Herschel is a European Space Agency cornerstone mission, with science instruments provided by consortia of European institutes and with important participation by NASA. NASA's Herschel Project Office is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA.
- May 10, 2012
- ESA/PACS/SPIRE/Martin Hennemann & Frdrique Motte, Laboratoire AIM Paris-Saclay, CEA/Irfu CNRS/INSU Univ. Paris Diderot, France
- Subject | Milky Way
- Nebula Type Star Formation
- Lightyears 4,700
|Telescope||Spectral Band||Color Assigment||Wavelength|
|Herschel (PACS)||Infrared||Blue||70.0 µm|
|Herschel (PACS)||Infrared||Green||160.0 µm|
|Herschel (SPIRE)||Millimeter||Red||250.0 µm|