Celestial hemisphere:  Northern  ·  Constellation: Perseus (Per)  ·  Contains:  NGC 1579  ·  Sh2-222
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NGC 1579, Gary Imm
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NGC 1579

Getting plate-solving status, please wait...
NGC 1579, Gary Imm
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NGC 1579

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Description

This object is an emission nebula located 2000 light years away in the constellation of Perseus at a declination of +35 degrees. This object spans 10 arc-minutes in our apparent view, which corresponds to a diameter of 5 light years.

The nebula is nicknamed the Northern Trifid Nebula. Trifid is Latin for "split into three parts", referring to the dark lanes "trisecting" the nebula. The Northern Trifid Nebula is smaller than the better known Trifid Nebula and lies much farther north in the sky.

NGC1579 is illuminated by the central reflected light of the orange star near the center of the nebula. This star, named LkHα 101, is a hot star almost 10,000 times more luminous and 15 times more massive than the Sun, but it is heavily obscured by dust. It lies within a small, young star cluster, together with dozens of sibling stars that are also newly formed.

Per its nickname, prominent dark dust lanes extend throughout the nebula. This nebula will not likely have a long life, since powerful stellar winds emanating from the stars will eventually blow the gas and dust away, leaving just stars behind.

I desperately tried numerous times to construct a true narrowband image using additional OIII and SII subs, but those signals were just too dim to made a decent image.

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