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Contains:  IC 1396
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Elephant's Trunk nebula - My very first SHO image ;-)

Technical card

Resolution: 2468x3175

Dates:May 9, 2017May 10, 2017May 15, 2017

Frames:
Baader Ha 2" 7nm: 22x600" -20C bin 1x1
Baader Planetarium O3 1.25" 8.5nm: 21x600" -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 22x600" -20C bin 1x1

Integration: 10.8 hours

Darks: ~22

Flats: ~21

Bias: ~100

Avg. Moon age: 15.60 days

Avg. Moon phase: 93.35%

Astrometry.net job: 1582130

RA center: 323.838 degrees

DEC center: 57.612 degrees

Pixel scale: 1.217 arcsec/pixel

Orientation: -88.339 degrees

Field radius: 0.680 degrees

Locations: Nürnberg, Nürnberg, Bayern, Germany

Description

Object description (wikipedia.org):

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 west of IC 1396A. (In the Figure above, 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.

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.

Comments

Author

superelch
Thomas Richter
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Elephant's Trunk nebula - My very first SHO image ;-), 





    
        

            Thomas Richter