Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  B161  ·  IC 1396  ·  LBN 452  ·  LBN 455  ·  LDN  ·  LDN 1099  ·  LDN 1105  ·  LDN 1110  ·  LDN 1111  ·  LDN 1112  ·  Sh2-131  ·  VdB142
IC1396 Elephant Trunk, Jerry Macon
Powered byPixInsight

IC1396 Elephant Trunk

IC1396 Elephant Trunk, Jerry Macon
Powered byPixInsight

IC1396 Elephant Trunk

Equipment

Loading...

Acquisition details

Loading...

Description

The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth. The piece of the nebula 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. 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.

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 of stars, 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.

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. (Wikipedia)

Comments

Sky plot

Sky plot

Histogram

IC1396 Elephant Trunk, Jerry Macon