Emission nebula | |
---|---|
Planetary nebula | |
Observation data: J2000.0 epoch | |
Right ascension | 19h 05m 55.6s[1] |
Declination | −05° 59′ 32.9″[1] |
Distance | 6,500 ly (2,000[2] pc) |
Apparent magnitude (V) | 11.9[3] |
Apparent dimensions (V) | 0.43′ |
Constellation | Aquila |
Physical characteristics | |
Radius | 0.4 ly |
Absolute magnitude (V) | 0.4 |
Designations | Glowing Eye Nebula, GSC 05140-03497, PK 029-05 1, PN Th 1-J, CSI-06-19031, HD 177656, PMN J1905-0559, PN Sa 2-382, EM* CDS 1043, HuLo 1, PN ARO 101, PN G029.2-05.9, GCRV 11549, IRAS 19032-0604, PN VV' 477, SCM 227, GSC2 S3002210353, 2MASX J19055556-0559327, PN VV 219, UCAC2 29903231 |
NGC 6751, also known as the Glowing Eye Nebula,[2] is a planetary nebula in the constellation Aquila. It is estimated to be about 6,500 light-years (2.0 kiloparsecs) away.[2]
NGC 6751 was discovered by the astronomer Albert Marth on 20 July 1863.[4] John Louis Emil Dreyer, the compiler of the New General Catalogue, described the object as "pretty bright, small".[4] The object was assigned a duplicate designation, NGC 6748.[4][5]
The nebula was the subject of the winning picture in the 2009 Gemini School Astronomy Contest, in which Australian high school students competed to select an astronomical target to be imaged by Gemini.
NGC 6751 is an easy telescopic target for deep-sky observers because its location is immediately southeast of the extremely red-colored cool carbon star V Aquilae.