Eskimo Nebula

NGC 2392
Emission nebula
Planetary nebula
	NGC 2392, the Eskimo Nebula by HST in 1999. ; Credit: NASA/ESA/STScI
Observation data: J2000 epoch
Right ascension	07h 29m 10.7669s
Declination	+20° 54′ 42.488″
Distance	6520±560 ly
Apparent magnitude (V)	10.1
Apparent dimensions (V)	48″; × 48″;
Constellation	Gemini
Physical characteristics
Radius	≥0.34 ly ly
Absolute magnitude (V)	≤0.4
Notable features	–
Designations	NGC 2392, Caldwell 39, PN G197.8+17.3; Central Star: HIP 36369, HD 59088, TYC 1372-1287-1
	See also: Lists of nebulae

The Eskimo Nebula (NGC 2392), also known as the Clown-faced Nebula, Lion Nebula,^[4] or Caldwell 39, is a bipolar^[5] double-shell^[6] planetary nebula (PN). It was discovered by astronomer William Herschel in 1787. The formation resembles a person's head surrounded by a parka hood. It is surrounded by gas that composed the outer layers of a Sun-like star. The visible inner filaments are ejected by a strong wind of particles from the central star. The outer disk contains unusual, light-year-long filaments.

NGC 2392 lies about 6500 light-years away, and is visible with a small telescope in the constellation of Gemini.

Historic data[]

NGC 2392 in 32 inch telescope

The nebula was discovered by William Herschel on January 17, 1787, in Slough, England. He described it as "A star 9th magnitude with a pretty bright middle, nebulosity equally dispersed all around. A very remarkable phenomenon."^[7] NGC 2392 WH IV-45 is included in the Astronomical League's Herschel 400 observing program.

Location[]

NGC 2392 is located just east of δ Geminorum, just south the ecliptic.

Naming controversy[]

On 11 August 2020, the IAU Working Group on Star Names (WGSN),^{[citation needed]} NASA/IPAC Extragalactic Database (NED),^{[citation needed]} and SIMBAD Astronomical Database (CDS) discontinued use of three nicknames that were perceived as offensive - "Eskimo Nebula", "Clown Face Nebula", and "Clownface Nebula" - and strongly recommended the nebula be referred to by its NGC designation in further publications.^[8]^[1]

Notes[]

^{^} Radius = distance × sin(angular size / 2) = ≥2900 ly * sin(48″ / 2) = ≥0.34 ly
^{^} 10.1 apparent magnitude - 5 * (log₁₀(≥880 pc distance) - 1) = ≤0.4 absolute magnitude

References[]

^ Jump up to: ^a ^b ^c ^d ^e "NGC 2392". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-12-22.
^ Gaia Collaboration et al. (2018b): Summary of the contents and survey properties
^ O'Dell, C. R.; Balick, B.; Hajian, A. R.; Henney, W. J.; et al. (2002). "Knots in Nearby Planetary Nebulae". The Astronomical Journal. 123 (6): 3329–3347. Bibcode:2002AJ....123.3329O. doi:10.1086/340726.
^ Deep-Sky Companions: The Caldwell Objects, 2nd Edition, Stephen James O'Meara, 2016, p.181
^ O'dell, C. R.; Balick, B.; Hajian, A. R.; Henney, W. J.; et al. (2003). "Knots in Planetary Nebulae". In S. J. Arthur & W. J. Henney (ed.). Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9–13, 2002. 15. pp. 29–33. Bibcode:2003RMxAC..15...29O.
^ Guerrero, M. A.; Chu, Y.-H.; Gruendl, R. A.; Meixner, M. (2005). "XMM-Newton detection of hot gas in the Eskimo Nebula: Shocked stellar wind or collimated outflows?". Astronomy and Astrophysics. 430 (3): L69–L72. arXiv:astro-ph/0412540. Bibcode:2005A&A...430L..69G. doi:10.1051/0004-6361:200400131.
^ The Scientific Papers of Sir William Herschel by J. L. E. Dreyer, Royal Society, London 1912
^ Talbert, Tricia (11 August 2020). "NASA to Reexamine Nicknames for Cosmic Objects". NASA. Retrieved 11 August 2020.

External links[]

NGC 2392 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
APOD (2003-12-07) – NGC 2392
Eskimo Nebula Lowell Observatory
The Structure & Evolution of the Eskimo Planetary Nebula University of Maryland Astronomy Department
A Kinematic Determination of the Structure of the Double Ring Planetary Nebula NGC 2392, the Eskimo Astrophysical Journal v.362, p.226 October 1990
A Cat's Eye view of the Eskimo from Saturn Maria-Teresa Garc ́ıa-D ́ıaz, Jose-Alberto L ́opez, Wofgang Steffen,Michael G. Richer and Hortensia Riesgo, 2011

Coordinates: 07^h 29^m 10.7669^s, +20° 54′ 42.488″

[simbad-1] Jump up to: ^a ^b ^c ^d ^e "NGC 2392". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-12-22.

[2] Gaia Collaboration et al. (2018b): Summary of the contents and survey properties

[ODelletal2002-3] O'Dell, C. R.; Balick, B.; Hajian, A. R.; Henney, W. J.; et al. (2002). "Knots in Nearby Planetary Nebulae". The Astronomical Journal. 123 (6): 3329–3347. Bibcode:2002AJ....123.3329O. doi:10.1086/340726.

[4] Deep-Sky Companions: The Caldwell Objects, 2nd Edition, Stephen James O'Meara, 2016, p.181

[ODelletal2003-5] O'dell, C. R.; Balick, B.; Hajian, A. R.; Henney, W. J.; et al. (2003). "Knots in Planetary Nebulae". In S. J. Arthur & W. J. Henney (ed.). Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9–13, 2002. 15. pp. 29–33. Bibcode:2003RMxAC..15...29O.

[Guerreroetal2005-6] Guerrero, M. A.; Chu, Y.-H.; Gruendl, R. A.; Meixner, M. (2005). "XMM-Newton detection of hot gas in the Eskimo Nebula: Shocked stellar wind or collimated outflows?". Astronomy and Astrophysics. 430 (3): L69–L72. arXiv:astro-ph/0412540. Bibcode:2005A&A...430L..69G. doi:10.1051/0004-6361:200400131.

[7] The Scientific Papers of Sir William Herschel by J. L. E. Dreyer, Royal Society, London 1912

[8] Talbert, Tricia (11 August 2020). "NASA to Reexamine Nicknames for Cosmic Objects". NASA. Retrieved 11 August 2020.

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