| Emission nebula | |
|---|---|
 Spitzer Space Telescope photo of the nebula | |
| Observation data | |
| Distance | 2,400 ly |
| Constellation | Cepheus |
| See also:Lists of nebulae | |
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TheElephant's Trunk Nebula is a concentration ofinterstellar gas and dust within the much larger ionized gas regionIC 1396 located in the constellationCepheus about 2,400light years away from Earth.[1] The piece of thenebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star (HD 206267) that is just to the east of IC 1396A. (In the Spitzer Space Telescope view shown, the massive star is just to the left of the edge of the image.) The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.[citation needed]
The Elephant's Trunk Nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards ofstars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.[citation needed]
The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk Nebula. This pressure has triggered the current generation of protostars.[2][3]
Media related toElephant's Trunk Nebula at Wikimedia Commons
