Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  Iris Nebula  ·  NGC 7023  ·  VdB139
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NGC7023 The Iris Nebula, Denis Janky
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NGC7023 The Iris Nebula

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NGC7023 The Iris Nebula, Denis Janky
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NGC7023 The Iris Nebula

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Description

The Iris Nebula resides in the constellation Cepheus, and is a fine visual and photographic object. It was originally discovered on October 18, 1794 by William Herschel.

This nebula is contained within our Milky Way Galaxy and is an example of a reflection nebula. It is anchored by the young, blue central star catalogued as HD200775 (or V380 Cep). The nebula is composed of dust that has remained after the formation of HD200775, and this dust is being illuminated by light from the star. The faint red filaments near the center are caused by ultraviolet radiation from the star that has ionized hydrogen gas.

The central star is very young (approximately 6400 years old), and it’s radius is estimated to be about 8.71 times that of the Sun. It has an apparent magnitude of 7.34, which is just beyond reach of naked eye visibility for most observers and sky conditions.

Distance estimates to the nebula range from 1300 to just over 1700 light years. The span of the blue region of the nebula is approximately six light years.

There is a star cluster on the west side of the nebula known as Collinder 427. It can be seen in the upper right region of this image, roughly centered within the dark ear-shaped region.

There are many splendid images of this nebula, and many are taken with small, wide field telescopes that show the full expanse of the surrounding dust cloud. The current image is a narrow field closeup, and so only exhibits the bright central region and a portion of the darker surrounding material.

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NGC7023 The Iris Nebula, Denis Janky