Lagoon Nebula

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Lagoon Nebula
Emission nebula
H II region
Trifid Vera Rubins.png
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]
Distance4,100 [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]
See also: Lists of nebulae

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).

Contents

Characteristics

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]

See also

Notes

  1. The bluish-pink nebula on the upper right is the Trifid Nebula.

References

  1. "Trifid and Lagoon (Image)". NSF–DOE Vera C. Rubin Observatory. 2025. Retrieved 2025-06-26.
  2. 1 2 3 "M 8". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2006-11-15.
  3. 1 2 Arias, J. I.; Barbá, R. H.; Maíz Apellániz, J.; Morrell, N. I.; Rubio, M. (2006). "The infrared Hourglass cluster in M8". Monthly Notices of the Royal Astronomical Society . 366 (3): 739–757. arXiv: astro-ph/0506552 . Bibcode:2006MNRAS.366..739A. doi: 10.1111/j.1365-2966.2005.09829.x . S2CID   13907667.
  4. 1 2 Stoyan, Ronald (2008). Atlas of the Messier Objects: Highlights of the Deep Sky. Cambridge University Press. p. 88. ISBN   978-0-521-89554-5.
  5. "SIMBAD Astronomical Database". Results for Hourglass Nebula. Retrieved 2006-12-22.
  6. Vowler, Faith; Bolles, Dana (12 September 2024). "Messier 8". NASA Science. Archived from the original on 17 March 2025. Retrieved 17 March 2025. M8 was discovered in 1654
  7. Kronberg, Guy McArthur, Hartmut Frommert, Christine. "Messier Object 8". messier.seds.org. Retrieved 11 April 2018.{{cite web}}: CS1 maint: multiple names: authors list (link)
  8. N. F. H. Tothill; Marc Gagné; B. Stecklum; M. A. Kenworthy (2008). "The Lagoon Nebula and its Vicinity". In Bo Reipurth (ed.). Handbook of Star-Forming Regions: Volume 2 The Southern Sky. Astronomical Society of the Pacific. p. 53. ISBN   978-1-58381-671-4.