The Cygnus-X star-forming region is located 4,600 light-years from Earth and
spans more than 600 light-years. It contains 10 times as much gas as the
Orion Nebula - enough to make over three million Suns. This infrared photograph from the Spitzer Space Telescope reveals more than a thousand protostars in the earliest stages of forming. Light of 3.6 microns is color-coded blue: 4.5-micron light is blue-green; 8.0-micron light is green; and 24-micron light is red.
Credit: NASA/JPL-Caltech/J. Hora (CfA) High Resolution Image (jpg) Low Resolution Image (jpg)
A bubbling cauldron of star birth is highlighted in this new image from
NASA's Spitzer Space Telescope. Infrared light that we can't see with our
eyes has been color-coded, such that the shortest wavelengths are shown in
blue and the longest in red. The middle wavelength range is green. Credit: NASA / JPL-Caltech / J. Hora (CfA) High Resolution Image (jpg) Low Resolution Image (jpg)
The top left box shows AFGL 2636, which is a bright-rimmed shell of material, carved out by winds and radiation from massive stars. These massive stars are located near the tip of the pillar in the center of the
region. The inner region is glowing red due to gas that has been ionized by
the massive stars. Spitzer has revealed a cluster of young stars with planet-forming disks in the central region, and embryonic stars embedded in the rim around the cavity. The situation is similar in the top right image, a region called DR22. The lower left and right images show clouds that are so thick to appear dark even to the dust-piercing, infrared eyes of Spitzer.
Young stars, visible as red points, are buried in these dark clouds. They are red because they are heating up surrounding dust, causing it to glow at longer infrared wavelengths. The red orb in the lower right image surrounds what is thought to be a star called a luminous blue variable, visible as the blue central point. This is a more evolved massive star that, after periods of instability, cast off a shell of material (red) from its outer layers. The bright object below the dark cloud in the lower right image is the tip of a large pillar, called DR 15, which is being eroded by winds and radiation from a large number of massive stars located above it. Credit: NASA / JPL-Caltech / J. Hora (CfA) High Resolution Image (jpg) Low Resolution Image (jpg)