Stellar Gusts From AFGL 2591
AFGL 2591 is located within the Milky Way more than 3,000 light-years from Earth, in the constellation of Cygnus. Over the course of the last few thousand years, it has created a vast expanding nebula larger than 500 times the diameter of our solar system. The star is at least 10 times the size of the Sun, and over 20,000 times as bright, but perhaps only one million years old. The wispy white and blue structure in the expanding nebula to the right of the young star is a huge outflow of gas and dust driven by the infall of material onto the star's surface. Gemini scientists believe that the outflow is likely occurring symmetrically around the star - a second giant-sized expanding nebula to the left of the star is hidden from view by a dense and extensive disk (or torus) of material encircling AFGL 2591.
Credit:International Gemini Observatory
About the Image
Id: | gemini0101a |
Type: | Observation |
Release date: | July 23, 2001, 8 p.m. |
Related releases: | gemini0101 |
Size: | 968 x 900 px |
About the Object
Wallpapers
Coordinates
Position (RA): | 20 29 24.91 |
Position (Dec): | 40° 11' 10.89" |
Field of view: | 1.88 x 1.75 arcminutes |
Orientation: | North is 0.5° left of vertical |
Colors & filters
Band | Wave-length | Tele-scope |
---|---|---|
Infrared J | 1.25 μm | Gemini North NIRI |
Infrared H | 1.64 μm | Gemini North NIRI |
Infrared Kprime | 2.12 μm | Gemini North NIRI |