NGC 3132
| Nebula | |
|---|---|
 | |
| Observation data: J2000.0 epoch | |
| Right ascension | 10h 07m 01.7640s[1] |
| Declination | −40° 26′ 11.060″[1] |
| Distance | 2,000 ly[2] ly |
| Apparent magnitude (V) | 9.87[1] |
| Apparent dimensions (V) | 1′.4 × 0′.9[citation needed] |
| Constellation | Vela |
| Physical characteristics | |
| Radius | 0.2 ly[2] ly |
| Absolute magnitude (V) | - |
| Designations | Eight-burst Nebula,[1] Southern Ring Nebula[2] |
NGC 3132 (Eight-burst Nebula / Southern Ring Nebula) is a bright and extensively studied planetary nebula in the constellation Vela. From the available spectroscopic data, presently the observed gas shell is expanding at about 24 kms-1.
Distance is estimated to be about 550 kpc. or 2,000 light years from Earth.
Planetary nebula nucleus (PNN)
Images of NGC 3132 reveal within the nebulosity two stars close together, one of 10th magnitude, the other 16th. The central planetary nebula nucleus (PNN) or white dwarf central star is the fainter of these two stars. This hot central star of about 100,000 K has now blown off its layers and is making the nebula fluoresce brightly from the emission of its intense ultraviolet radiation.
References
- ^ a b c d "SIMBAD Astronomical Database". Results for NGC 3132. Retrieved 2007-01-03.
- ^ a b c "Fast Facts - Planetary Nebula NGC 3132". Space Telescope Science Institute. Retrieved 2007-10-06.
External links
Wikimedia Commons has media related to NGC 3132.