California nebula


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California nebula

(NGC 1499) An emission nebula – an H II region – that lies in the constellation Perseus and is ionized by the star Xi (ξ) Persei.
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A far more challenging target toward the northwest, the Taurus Molecular Cloud 1 (TMC-1) can be found just north of the Hyades and extends westward past the California Nebula (NGC 1499) and the Pleiades (M45).
The California Nebula, NGC 1499, in Perseus is a large HII region--around 2x1[degrees];
California Nebula (right) The California Nebula (NGC 1499), taken on October 11, 1996.
The H-beta will also work on a few other similarly dim objects, like the California Nebula, but it's certainly not a general-use filter.
Perseus is also the home to the large diffuse emission nebula NGC 1499, the California Nebula.
Located in Perseus, the California Nebula is a challenge to observe visually in any telescope, and long exposures are required to photograph its entirety.
Even rather dim M76, the Little Dumbbell Nebula, and NGC 1499, the elusive California Nebula, get considerable attention.
NGC 1499, the California Nebula, along with variable and multiple stars, so in many ways this is also a general purpose atlas.
The Zeta ([zeta]) Persei Association (also called Perseus OB2) and its neighbor the California Nebula (NGC 1499) are roughly 1,000 light-years distant.
The California Nebula (NGC 1499) in Perseus displays faint wisps of gases that extend far beyond the familiar boundaries of this well-known object.
The bright complex in Perseus at upper right includes the California Nebula, though the state gets a noteworthy border revision because of the faint nebulosity recorded here.
I had first seen the California Nebula almost 30 years ago in a fine, low-power telescope, but you typically need a nebula filter to pick out this 21/4[degrees]-long glow visually.

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