Q497739
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Key facts
- Right ascension
- 17 13 44.211
- Declination
- −37 ° 06 ′ 15.94 ″
- Distance
- 3400 ± 500 ly (1040 ± 160 pc )
- Apparent magnitude v
- 7.1B
- Apparent dimensions v
- >3′.0
- Constellation
- Scorpius
- Radius
- >1.5 ± 0.2 ly ly
- Absolute magnitude v
- -3.0B , − 0.3
- Notable features
- Dual chemistry, hot central star
- Designations
- Bipolar Nebula, Bug Nebula, PK 349+01 1, Butterfly Nebula, Sharpless 6, RCW 124, Gum 60, Caldwell 69
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 741
- Image
- NGC 6302 Hubble 2009.full.jpg
Show 8 more facts
- Commons category
- NGC 6302
- catalog code
- WEB 14231
- spectral class
- Ne...
- time of discovery or invention
- 1880-00-00
- apparent magnitude
- 7.1
- right ascension
- 258.4347458
- declination
- -37.1030417
- radial velocity
- -35.7
Sources (1)
via Wikidata · CC0
~7 min read
Article
NGC 6302 (also known as the Bug Nebula, Butterfly Nebula, or Caldwell 69) is a bipolar type planetary nebula in the constellation Scorpius. The structure in this planetary nebula is among the most complex ever seen in any planetary nebulae. The spectrum of Butterfly Nebula shows that its central star is one of the hottest stars known, with a surface temperature in excess of 250,000 degrees Celsius. This implies that the star from which it formed must have been very large in order to become this hot.
The central star, a white dwarf, was identified in 2009, using the upgraded Wide Field Camera 3 on board the Hubble Space Telescope. The star has a current mass of around 0.64 solar masses. The star is surrounded by a dense equatorial disc composed of gas and dust. This dense disc is postulated to have caused the star's outflows to form the bipolar structure seen in the Nebula. similar to an hourglass. This bipolar structure shows features such as ionization walls, knots and sharp edges to the lobes.