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NGC 3132 (also known as the Eight-Burst Nebula,[2] the Southern Ring Nebula,[2] or Caldwell 74) is a bright and extensively studied planetary nebula in the constellation Vela. Its distance from Earth is estimated at about 613 pc. or 2,000 light-years.[2]

NGC 3132
Emission nebula
Planetary nebula
View in near-infrared by NIRCam
Observation data: J2000.0 epoch
Right ascension10h 07m 01.7640s[1]
Declination−40° 26 11.060[1]
Distance2,000[2] ly
Apparent magnitude (V)9.87[1]
Apparent dimensions (V)62 × 43[3]
ConstellationVela
Physical characteristics
Radius0.4 ly[2] ly
DesignationsEight-Burst Nebula,[2] Southern Ring Nebula,[2] Caldwell 74
See also: Lists of nebulae

The Southern Ring Nebula was selected as one of the five cosmic objects observed by the James Webb Space Telescope as part of the release of its first official science images on July 12, 2022.[4]


Planetary nebula nucleus (PNN)


Images of NGC 3132 reveal two stars close together within the nebulosity, one of 10th magnitude, the other 16th. The central star of the planetary nebula is a white dwarf, and is the fainter of the two stars. This hot central star of about 100,000 K has now blown off its outer layers and is making the nebula fluoresce brightly from the emission of its intense ultraviolet radiation.[5]


See also



References


  1. "NGC 3132". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-01-03.
  2. "Fast Facts – Planetary Nebula NGC 3132". Hubble Heritage Project. Space Telescope Science Institute. Retrieved 2007-10-06.
  3. "Results for NGC 3132". NGC/IC Project Database. Archived from the original on 2012-05-20. Retrieved 2011-01-09.
  4. Garner, Rob (2022-07-08). "NASA Shares List of Cosmic Targets for Webb Telescope's 1st Images". NASA. Retrieved 2022-07-08.
  5. Monreal-Ibero, Ana; Walsh, Jeremy R. (2020). "The MUSE view of the planetary nebula NGC 3132". Astronomy and Astrophysics. 634: A47. arXiv:1912.02847. Bibcode:2020A&A...634A..47M. doi:10.1051/0004-6361/201936845. S2CID 208857629.



На других языках


[de] NGC 3132

NGC 3132 ist ein Planetarischer Nebel im Sternbild Segel des Schiffs am Südsternhimmel. Er ist etwa 2000 Lichtjahre von der Sonne entfernt, hat einen Durchmesser von fast einem halben Lichtjahr und expandiert mit einer Geschwindigkeit von rund 15 Kilometern pro Sekunde. NGC 3132 hat eine Flächenausdehnung von 1,47' und eine scheinbare Helligkeit von 9,2 mag. In manchen Publikationen[7] wird er aufgrund seiner Ähnlichkeit zu M57 auch als Südlicher Ringnebel bezeichnet.
- [en] NGC 3132

[ru] NGC 3132

NGC 3132 — планетарная туманность в созвездии Паруса.



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