| Emission nebula | |
|---|---|
| Planetary nebula | |
 Hubble Space Telescope image of NGC 3918. Credit: ESA/Hubble and NASA. | |
| Observation data:J2000.0epoch | |
| Right ascension | 11h 50m 17.7s[1] |
| Declination | −57° 10′ 56.9″[1] |
| Distance | 4 900 ly |
| Apparent magnitude (V) | 8.5 |
| Apparent dimensions (V) | 8 to 10 arcsec |
| Constellation | Centaurus |
| Physical characteristics | |
| Radius | 0.095-0.12 ly |
| Designations | He2-74 / Hen 2-74 / Sa2-81 / PK 294+4.1 / PN G294.6+04.7 / ESO 170-1[1] |
| See also:Lists of nebulae | |
NGC 3918 is a brightplanetary nebula in theconstellationCentaurus, nicknamed the "Blue Planetary" or "The Southerner". It is thebrightest of the far southern planetary nebulae. This nebula was discovered by SirJohn Herschel in March 1834 and is easily visible through small telescopes. The round or even slightly oval diameter is telescopically between 8 and 10arcsec, though deep images extends this to about 19 or 20 arcsec. More surprising is the beautiful rich blue colour that looks much like the coloured images ofNeptune taken byVoyager 2 in 1989.
Spectroscopy reveals NGC 3918 is approaching us at 17±3.0 kilometres per second, while the nebulosity is expanding at around 24 kilometres per second. The central star is 14.6 visible light magnitude, and remains invisible to optical observers, as it is obscured by the sheer brightness of the surrounding nebula.[2]
The distance is estimated at 1.5kpc (4 900light-years).
Media related toNGC 3918 at Wikimedia Commons
