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Trifid Nebula

Coordinates:Sky map18h 02m 23s, −23° 01′ 48″
From Wikipedia, the free encyclopedia
(Redirected fromSh 2-30)
Emission nebula in the constellation Sagittarius
Trifid Nebula
Emission nebula
H II region
reflection nebula anddark nebula
The Trifid Nebula as imaged by theVera C. Rubin Observatory in very high-resolution, taken on May 28, 2025[1]
Observation data:J2000epoch
Right ascension18h 02m 23s[2]
Declination−23° 01′ 48″[2]
Distance4100±200[3] ly   (1,260±70 pc)
Apparent magnitude (V)+6.3[2]
Apparent dimensions (V)28arcmins
ConstellationSagittarius
Physical characteristics
Radius21 ly
Notable featuresa
DesignationsM20,NGC 6514,[2]Sharpless 30,RCW 147, Gum 76
See also:Lists of nebulae

TheTrifid Nebula (catalogued asMessier 20 orM20 and asNGC 6514) is anH II region in the north-west ofSagittarius in astar-forming region in theMilky Way'sScutum–Centaurus Arm.[4] It was discovered byCharles Messier on June 5, 1764.[5] Its name means 'three-lobe'. The object is an unusual combination of anopen cluster ofstars, anemission nebula (the relatively dense, reddish-pink portion), areflection nebula (the mainlyNNE blue portion), and adark nebula (the apparent 'gaps' in the former that cause the trifurcated appearance, also designatedBarnard 85). Viewed through a smalltelescope, the Trifid Nebula is a bright and peculiar object, and is thus a perennial favorite of amateur astronomers.[6]

The most massive star that has formed in this region is HD 164492A, anO7.5III star with a mass more than 20 times themass of the Sun.[7]This star is surrounded by a cluster of approximately 3100 young stars.[8]

Characteristics

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The Trifid Nebula was the subject of an investigation by astronomers using theHubble Space Telescope in 1997, using filters that isolate emission fromhydrogenatoms,ionizedsulfur atoms, and doubly ionizedoxygen atoms. The images were combined into a false-color composite picture to suggest how the nebula might look to the eye.

The close-up images show a dense cloud of dust and gas, which is astellar nursery full of embryonic stars. This cloud is aboutly away from the nebula's central star. Astellar jet protrudes from the head of the cloud and is about0.75 ly long. The jet's source is a young stellar object deep within the cloud. Jets are the exhaust gasses of star formation and radiation from the nebula's central star makes the jet glow.

The images also showed a finger-like stalk to the right of the jet. It points from the head of the dense cloud directly toward the star that powers the Trifid Nebula. This stalk is a prominent example ofevaporating gaseous globules, or 'EGGs'. The stalk has survived because its tip is a knot of gas that is dense enough to resist being eaten away by the powerful radiation from the star.

In January 2005,NASA'sSpitzer Space Telescope discovered 30 embryonic stars and 120 newborn stars not seen invisible light images.

It is centered about4100 ly fromEarth. Itsapparent magnitude is 6.3.

Details and features

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  • The Trifid Nebula. The outlined area is enlarged right.
    The Trifid Nebula. The outlined area is enlarged right.
  • Hubble image of a stellar jet in the Trifid Nebula
    Hubble image of a stellar jet in the Trifid Nebula
  • This video sequence compares a new view of the Trifid Nebula in infrared light, from the VVV VISTA survey with a more familiar visible-light view from a small telescope.
  • The Trifid Nebula
    The Trifid Nebula
  • Trifid Nebula close-up
    Trifid Nebula close-up
  • Widefield image of the Trifid Nebula next to Lagoon Nebula
    Widefield image of the Trifid Nebula next toLagoon Nebula
  • Trifid Nebula seen at different wavelengths
    Trifid Nebula seen at differentwavelengths

See also

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References

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  1. ^"Trifid and Lagoon (Image)". NSF–DOE Vera C. Rubin Observatory. 2025. Retrieved2025-06-26.
  2. ^abcd"NGC 6514".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2006-11-16.
  3. ^Kuhn, Michael A.; Hillenbrand, Lynne A.; Sills, Alison; Feigelson, Eric D.; Getman, Konstantin V. (2018)."Kinematics in Young Star Clusters and Associations with Gaia DR2".The Astrophysical Journal.870 (1): 32.arXiv:1807.02115.Bibcode:2019ApJ...870...32K.doi:10.3847/1538-4357/aaef8c.S2CID 119328315.
  4. ^Cambrésy, L.; et al. (2011). "Variation of the extinction law in the Trifid nebula".Astronomy & Astrophysics.527: A141.arXiv:1101.1089.Bibcode:2011A&A...527A.141C.doi:10.1051/0004-6361/201015863.S2CID 39501333.
  5. ^Messier 20
  6. ^"Trifid Nebula: A Massive Star Factory".Science Daily. August 26, 2009. Retrieved2010-07-06.
  7. ^Rho, J.; et al. (2004). "Chandra Observation of the Trifid Nebula: X-Ray Emission from the O Star Complex and Actively Forming Pre-Main-Sequence Stars".Astrophysical Journal.607 (2):904–912.arXiv:astro-ph/0401377.Bibcode:2004ApJ...607..904R.doi:10.1086/383081.S2CID 119090269.
  8. ^Kuhn, M. A.; et al. (2015). "The Spatial Structure of Young Stellar Clusters. II. Total Young Stellar Populations".Astrophysical Journal.802 (1): 60.arXiv:1501.05300.Bibcode:2015ApJ...802...60K.doi:10.1088/0004-637X/802/1/60.S2CID 119309858.

External links

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Wikimedia Commons has media related toTrifid Nebula.
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Painting of Charles Messier, creator of the Messier catalog
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