IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth. There 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.

Telescope: Astro Physics 175EDF f8.3
Mount: Astro Physics 3600GTO “El Capitan”
Camera: SBIG STT8300
Guider: SBIG FW8G OAG(Guided Filter Wheel)

H-alpha: 17×20 mins = 340 mins, OIII: 29×20 mins = 580 mins, SII: 31×20 mins = 620 mins

Total Imaging Time: 25h 40m

Data Imaged remotely over 10 nights during October & November 2015.
Data acquisition & Processing by David Churchill.

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