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Sharpless 176, James E.
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Sharpless 176

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Sharpless 176, James E.
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Sharpless 176

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Description

Sharpless 176 (Sh2-176) is a faint planetary nebula with a hydrogen-rich central star. It was discovered to be a planetary nebula by F. Sabbadin et al in 1977 (Astronomy & Astrophysics, "Sharpless 176: A Large, Nearby Planetary Nebula", March 1977). It is approximately 490 light-years away with estimates for its age ranging from 24,000 to over 180,000 years old based on the computed kinematics (expansion rate and nebular diameter). Expanding at 19 km/sec, Sh2-176 has been estimated to span 3.1 to over 22 light-years across depending on the source. Its asymmetricity is believed to be the result of bow shocks involving the interstellar medium and the nebula itself where the brighter portion of the nebula represents the interaction of the nebula with the interstellar medium as it travels through space.  The central star associated with Sh2-176 is a blue subdwarf with a magnitude of 18.74.  (ImagingDeepSpace.com)

Imaged over several nights:  Oct 5, 8-10 and 12, 2022.

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