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 emission nebula with an H II region located in the constellation Sagittarius. Discovered by Giovanni Hodierna in 1654, it is one of only two star-forming nebulae faintly visible to the naked eye from mid-northern latitudes [6] [7] (the other being the Orion Nebula).
Located approximately 4,000–6,000 light-years from Earth, the nebula spans 110 by 50 light-years (appearing as 90' by 40' in Earth's sky). While appearing pink in long-exposure photographs, it typically appears gray when viewed through binoculars or telescopes due to the human eye's limited color sensitivity in low-light conditions. The nebula contains the young open cluster NGC 6530 within its structure. [8]
The Lagoon Nebula features several distinctive structures, including:
Observations in 2006 revealed four Herbig–Haro objects within the Hourglass structure, providing direct evidence of ongoing star formation through accretion processes. [3]
M8 was discovered in 1654
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