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NGC 5882

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Small planetary nebula in the constellation Lupus
NGC 5882
Emission nebula
Planetary nebula
A Hubble Space Telescope (HST) image of NGC 5882.
Credit: HST/NASA/ESA.
Observation data: J2000 epoch
Right ascension15 16 49.95679
Declination−45° 38′ 58.6109″
Distance7.7 kly (2.4 kpcly
Apparent dimensions (V)13–14
ConstellationLupus
DesignationsESO 274-7, IC 1108, NGC 5882
See also: Lists of nebulae

NGC 5882 is a small planetary nebula in the southern constellation of Lupus, positioned about 1.5° to the southwest of the star Epsilon Lupi. It was discovered by English astronomer John Herschel on July 2, 1834 from the Cape of Good Hope observatory. John L. E. Dreyer described it as "very small, round, quite sharp". It is located at a distance of approximately 7.7 kilolight-years from the Sun.

This nebular region consists of the cast-off outer atmosphere of an aging star. It is roughly elliptical in shape with several clumps of ionized material, and is surrounded by a larger region of low-level emission that extends for three times the nominal diameter of the main nebula. The nebula is expanding with an average velocity of 12.5 km/s. It consists of two shells: the inner shell is elliptical and measures 11″ × 6″, while the more rapidly expanding outer shell is rounder with a diameter of 15″. The inner shell has what appears to be multiple bubble-like shapes. The clumps in the outer shell may be the result of instabilities.

The elemental abundances of the nebula are very similar to those in the Sun, except for a times two enrichment of nitrogen. The latter suggests that the central star did not go through second dredge-up. The central star has an apparent visual magnitude of 13.43. It shines with 830 times the luminosity of the Sun and has 22.7% of the Sun's radius. It is displaced slightly from the center of symmetry for the nebula.

References

  1. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ Stanghellini, Letizia; et al. (December 2008), "The Magellanic Cloud Calibration of the Galactic Planetary Nebula Distance Scale", The Astrophysical Journal, 689 (1): 194–202, arXiv:0807.1129, Bibcode:2008ApJ...689..194S, doi:10.1086/592395, S2CID 119257242
  3. ^ Pottasch, S. R.; et al. (August 2004). "Abundances of Planetary Nebulae IC 418, IC 2165 and NGC 5882". Astronomy and Astrophysics. 423 (2): 593–605. Bibcode:2004A&A...423..593P. doi:10.1051/0004-6361:20040413.
  4. ^ O'Meara, Stephen James (April 8, 2013). Deep-Sky Companions: Southern Gems. Cambridge University Press. p. 279. ISBN 9781139851541.
  5. "NGC 5882". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-02-25.
  6. Sinnott, Roger W.; Perryman, Michael A. C. (1997). Millennium Star Atlas. Vol. 2. Sky Publishing Corporation and the European Space Agency. p. 948. ISBN 0-933346-83-2.
  7. Seligman, Courtney. "New General Catalogue objects: NGC 5850 - 5899". cseligman.com. Retrieved 2020-09-20.
  8. ^ Corradi, Romano L. M.; et al. (October 2000). "Knots in the Outer Shells of the Planetary Nebulae IC 2553 and NGC 5882". The Astrophysical Journal. 542 (2): 861–869. arXiv:astro-ph/0003238. Bibcode:2000ApJ...542..861C. doi:10.1086/317041. S2CID 18811052.

External links

  • Media related to NGC 5882 at Wikimedia Commons
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