Emission nebula | |
---|---|
H II region | |
![]() The Lagoon Nebula as imaged by the Vera C. Rubin Observatory in very high-resolution, taken on May 28, 2025.[1][a] | |
Observation data: J2000 epoch | |
Right ascension | 18h 03m 37s[2] |
Declination | −24° 23′ 12″[2] |
Distance | 4,100[3] ly (1,250 pc) |
Apparent magnitude (V) | 4.6[4] |
Apparent dimensions (V) | 90 × 40 arcmins[4] |
Constellation | Sagittarius |
Physical characteristics | |
Radius | 55 × 20 ly |
Designations | Sharpless 25, RCW 146, Gum 72 M8 contains: NGC 6523, NGC 6530,[2] Hourglass nebula[5] |
The Lagoon Nebula (catalogued as Messier 8 or M8, NGC 6523, Sharpless 25, RCW 146, and Gum 72) is a giant interstellar cloud in the constellation Sagittarius. It is classified as an emission nebula and has an H II region.
The Lagoon Nebula was discovered by Giovanni Hodierna in 1654[6][7] and is one of only two star-forming nebulae faintly visible to the eye from mid-northern latitudes. Seen with binoculars, it appears as a distinct cloud-like patch with a definite core. Within the nebula is the open cluster NGC 6530.[8]
M8 was discovered in 1654
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