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NGC 7662

Coordinates:Sky map23h 25m 54s, +42° 32′ 6″
From Wikipedia, the free encyclopedia
Planetary nebula in the constellation Andromeda
"Blue Snowball" redirects here. For the microphone product, seeBlue Microphones.
NGC 7662
Emission nebula
Planetary nebula
Observation data:J2000epoch
Right ascension23h 25m 53.832s[1]
Declination+42° 32′ 05.84″[1]
Distance5,730 ± 340[1] ly
Apparent magnitude (V)8.3[2]
Apparent dimensions (V)32″ × 28″[2]
ConstellationAndromeda
Physical characteristics
Radius0.8[citation needed] ly
DesignationsPK 106-17 1, GCRV 14695, PN ARO 20, Blue Snowball Nebula, Snowball Nebula,Caldwell 22[3]
See also:Lists of nebulae

NGC 7662 is aplanetary nebula located in the northernconstellationAndromeda. It is known as theBlue Snowball Nebula,Snowball Nebula, andCaldwell 22. This nebula was discovered October 6, 1784 by the German-born English astronomerWilliam Herschel. In theNew General Catalogue it is described as a "magnificent planetary or annular nebula, very bright, pretty small inangular size, round, blue, variable nucleus". The object has anapparent visual magnitude of 8.3 and spans an angular size of32″ × 28″.[2]Parallax measurements give a distance estimate of 5,730 ± 340 ly (1,757 ± 103 pc).[1]

NGC 7662 is a popular planetary nebula for casual observers. A small telescope will reveal a star-like object with slight nebulosity. A 6" telescope with amagnification around 100x will reveal a slightly bluish disk, while telescopes with aprimary mirror at least 16" in diameter may reveal slight color and brightness variations in the interior.[4]

Hubble Space Telescope image of NGC 7662[5]

This nebula has an elliptical shape with a triple-shell structure. The brightest is the main shell, which spans12″ × 18″. This is surrounded by a fainter outer shell, which has an elliptical form. Both shells are enclosed by a faint, circular halo,[6] some134″ in diameter. The two shells can be modeled asprolate spheroids, with the inner shell having the greater elongation, amajor axis tilt of 50° to the line of sight, and a hull thickness of~2.5″.[7] Several knots and a jet-like structure are visible, which displayemission lines and low ionization. Based on the expansion rate, the estimated age of the nebula is 3,080 years.[6]

The central star of the planetary nebula is asubdwarf O star with aspectral type of sdO.[8] The best fit model for this star gives aneffective temperature of 100 kK, with 5,250 times theluminosity of the Sun[6] and 60.5% of theSun's mass.[7]X-ray emission from the nebula is being generated by thestellar wind from this star striking previously ejected matter.[2]

See also

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References

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  1. ^abcdBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  2. ^abcdO'Meara, Stephen James (2016).Deep-Sky Companions: The Caldwell Objects. Cambridge University Press. pp. 105–108.ISBN 9781316033531.
  3. ^"NGC 7662".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2007-04-10.
  4. ^Burnham, Robert (2013).Burnham's Celestial Handbook, An Observer's Guide to the Universe Beyond the Solar System. Vol. 1. Dover Publications. p. 157.ISBN 9780486319025.
  5. ^"Hubble picture of NGC 7662". The Hubble European Space Agency Information Centre. 2007-09-27.
  6. ^abcBarría, D.; Kimeswenger, S. (October 2018)."HST/WFPC2 imaging analysis and cloudy modelling of the multiple-shell planetary nebulae NGC 3242, NGC 6826, and NGC 7662".Monthly Notices of the Royal Astronomical Society.480 (2):1626–1638.arXiv:1807.01787.Bibcode:2018MNRAS.480.1626B.doi:10.1093/mnras/sty1796.
  7. ^abGuerrero, Martín A.; et al. (October 2004). "Physical Structure of Planetary Nebulae. II. NGC 7662".The Astronomical Journal.128 (4):1705–1710.arXiv:astro-ph/0407029.Bibcode:2004AJ....128.1705G.doi:10.1086/423913.S2CID 7142085.
  8. ^González-Santamaría, I.; et al. (2021). "Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity".Astronomy & Astrophysics.656: A51.arXiv:2109.12114.Bibcode:2021A&A...656A..51G.doi:10.1051/0004-6361/202141916.S2CID 237940344.

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