Messier 26, also known as NGC 6694, is an open cluster of stars in the southern constellation of Scutum. It was discovered by Charles Messier in 1764.[a] This 8th magnitude cluster is a challenge to find in ideal skies with typical binoculars, where it can be, with any modern minimum 3-inch (76 mm) aperture device. It is south-southwest of the open cluster Messier 11 and is 14′ across.[3] About 25 stars are visible in a telescope with a 150–200 mm (6–8 in) aperture.[6]
| Messier 26 | |
|---|---|
 Open cluster Messier 26 Credit: Hillary Mathis, Vanessa Harvey, REU program/NOIRLab/NSF/AURA | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 18h 45m 18.0s[1] |
| Declination | −09° 23′ 00″[1] |
| Distance | 5,160 ly (1,582 pc)[2] |
| Apparent magnitude (V) | 8.0[3] |
| Apparent dimensions (V) | 14′[3] |
| Physical characteristics | |
| Radius | 11 ly[4] |
| Estimated age | 85.3[1] million years |
| Other designations | Messier 26, NGC 6694,[5] Cr 389, C 1842-094 |
| Associations | |
| Constellation | Scutum |
M26 spans a linear size of 22[4] light years across with a tidal radius of 25 light-years,[7] and is at a distance of 5,160[2] light years from the Earth. The brightest star is of magnitude 11[6] and the age of this cluster has been calculated to be 85.3[1] million years. It includes one known spectroscopic binary system.[8]
An interesting feature of M26 is a region of low star density near the nucleus. A hypothesis was that it was caused by an obscuring cloud of interstellar matter between us and the cluster, but a paper by James Cuffey suggested that this is not possible and that it really is a "shell of low stellar space density".[9] In 2015, Michael Merrifield of the University of Nottingham said that there is, as yet, no clear explanation for the phenomenon.[10]
Gallery edit
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Map showing the location of M26 (Roberto Mura)
See also edit
Footnotes and references edit
Footnotes edit
- ^ On June 20
References edit
- ^ a b c d Wu, Zhen-Yu; et al. (November 2009), "The orbits of open clusters in the Galaxy", Monthly Notices of the Royal Astronomical Society, 399 (4): 2146–2164, arXiv:0909.3737, Bibcode:2009MNRAS.399.2146W, doi:10.1111/j.1365-2966.2009.15416.x, S2CID 6066790.
- ^ a b Kharchenko, N. V.; et al. (2005), "Astrophysical parameters of Galactic open clusters", Astronomy and Astrophysics, 438 (3): 1163–1173, arXiv:astro-ph/0501674, Bibcode:2005A&A...438.1163K, doi:10.1051/0004-6361:20042523, S2CID 9079873.
- ^ a b c Thompson, Robert; Thompson, Barbara (2007), Illustrated Guide to Astronomical Wonders: From Novice to Master Observer, DIY science, O'Reilly Media, Inc., p. 431, ISBN 978-0596526856
- ^ a b Kharchenko, N. V.; et al. (March 2009), "Shape parameters of Galactic open clusters", Astronomy and Astrophysics, 495 (3): 807–818, arXiv:0812.3542, Bibcode:2009A&A...495..807K, doi:10.1051/0004-6361/200810407, S2CID 2196805.
- ^ "M 26". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved November 15, 2018.
- ^ a b Burnham, Robert (1978), Burnham's Celestial Handbook: An Observer's Guide to the Universe Beyond the Solar System, Dover books on astronomy, vol. 3, Courier Corporation, p. 1756, ISBN 978-0486236735
- ^ Piskunov, A. E.; et al. (January 2008), "Tidal radii and masses of open clusters", Astronomy and Astrophysics, 477 (1): 165–172, Bibcode:2008A&A...477..165P, doi:10.1051/0004-6361:20078525.
- ^ Mermilliod, J. -C.; et al. (October 2007), "Red giants in open clusters. XIII. Orbital elements of 156 spectroscopic binaries", Astronomy and Astrophysics, 473 (3): 829–845, Bibcode:2007A&A...473..829M, doi:10.1051/0004-6361:20078007.
- ^ Cuffey, James (1940). "The Galactic Clusters NGC 6649 and NGC 6694". Astrophysical Journal. 92: 303. Bibcode:1940ApJ....92..303C. doi:10.1086/144220.
- ^ Merrifield, Michael (Oct 2, 2015). "M26 - Open Cluster". Deep Sky Videos. University of Nottingham/University of Sheffield. Retrieved March 29, 2016.
External links edit
- Messier 26, SEDS Messier pages
- Messier 26 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
