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Contents

   



(Top)
 


1 Gallery  





2 See also  





3 References and footnotes  



3.1  References  





3.2  Footnotes  







4 External links  














Messier 28






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Coordinates: Sky map18h24m32.89s, 24° 52 11.4
 

From Wikipedia, the free encyclopedia
 


Globular cluster Messier 28 in Sagittarius

Observation data (J2000 epoch)

Class

IV[1]

Constellation

Sagittarius

Right ascension

18h24m 32.89s[2]

Declination

–24° 52′ 11.4″[2]

Distance

18.26 ± 0.98 kly (5.6 ± 0.3 kpc)[3]

Apparent magnitude (V)

6.8[4]

Apparent dimensions (V)

11′.2[5]

Physical characteristics

Mass

5.51×105[6] M

Radius

30 ly[7]

VHB

15.55 ± 0.10[8]

Metallicity

 = –1.32[6] dex

Estimated age

12.0 Gyr[9]

Notable features

Contains first pulsar discovered in a globular[10]

Other designations

GCl 94, M 28, NGC 6626[2]

See also: Globular cluster, List of globular clusters

Messier 28orM28, also known as NGC 6626, is a globular cluster of stars in the center-west of Sagittarius. It was discovered by French astronomer Charles Messier in 1764.[11][a] He briefly described it as a "nebula containing no star... round, seen with difficulty in 312-foot telescope; Diam2."[12]

In the sky it is less than a degree to the northwest of the 3rd magnitude star Kaus Borealis (Lambda Sgr). This cluster is faintly visible as a hazy patch with a pair of binoculars[11] and can be readily found in a small telescope with an 8 cm (3.1 in) aperture, showing as a nebulous feature spanning 11.2 arcminutes. Using an aperture of 15 cm (5.9 in), the core becomes visible and a few distinct stars can be resolved, along the periphery. Larger telescopes will provide greater resolution,[5] one of 25 cm (9.8 in) revealing a dense 2′ core, with more density within.[11]

It is about 18,300 light-years away from Earth.[3] It is about 551000 M[6] and its metallicity (averaging −1.32 which means more than 10 times less than our own star), coherency and preponderence of older stellar evolution objects, support its dating to very roughly 12 billion years old.[9]18RR Lyrae type variable stars have been found within.

It bore the first discovery of a millisecond pulsar in a globular cluster – PSR B1821–24. This was using the Lovell TelescopeatJodrell Bank Observatory, England.[10] A total of 11 further of these have since been detected in it with the telescopeatGreen Bank Observatory, West Virginia. As of 2011, these number the third-most in a cluster tied to the Milky Way, following Terzan 5 and 47 Tucanae.[13]

Gallery[edit]

See also[edit]

References and footnotes[edit]

References[edit]

  1. ^ Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin, 849 (849): 11–14, Bibcode:1927BHarO.849...11S.
  • ^ a b c "M 28". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2006-11-16.
  • ^ a b Oliveira, R. A. P.; Ortolani, S.; Barbuy, B.; Kerber, L. O.; Maia, F. F. S.; Bica, E.; Cassisi, S.; Souza, S. O.; Pérez-Villegas, A. (2022). "Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters". Astronomy & Astrophysics. 657: A123. arXiv:2110.13943. Bibcode:2022A&A...657A.123O. doi:10.1051/0004-6361/202141596. S2CID 239998638.
  • ^ "Messier 28". SEDS Messier Catalog. Retrieved 28 April 2022.
  • ^ a b Inglis, Mike (2004), Astronomy of the Milky Way: Observer's guide to the northern sky, Patrick Moore's Practical Astronomy Series, vol. 1, Springer, p. 21, Bibcode:2003amwn.book.....I, ISBN 978-1852337094.
  • ^ a b c Boyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters", The Astrophysical Journal, 742 (1): 51, arXiv:1108.4402, Bibcode:2011ApJ...742...51B, doi:10.1088/0004-637X/742/1/51, S2CID 118649860.
  • ^ From trigonometry: radius = distance × sin( diameter_angle / 2 ) = 30 ly
  • ^ Testa, Vincenzo; et al. (February 2001), "Horizontal-Branch Morphology and Dense Environments: Hubble Space Telescope Observations of Globular Clusters NGC 2298, 5897, 6535, and 6626", The Astronomical Journal, 121 (2): 916–934, Bibcode:2001AJ....121..916T, doi:10.1086/318752
  • ^ a b Koleva, M.; et al. (April 2008), "Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting", Monthly Notices of the Royal Astronomical Society, 385 (4): 1998–2010, arXiv:0801.0871, Bibcode:2008MNRAS.385.1998K, doi:10.1111/j.1365-2966.2008.12908.x, S2CID 17571531
  • ^ a b "JBO - Stars". Jodrell Bank Observatory. Retrieved 2007-06-01.
  • ^ a b c Thompson, Robert Bruce; Thompson, Barbara Fritchman (2007), Illustrated Guide to Astronomical Wonders, Diy Science, O'Reilly Media, Inc., p. 402, ISBN 978-0596526856.
  • ^ Burnham, Robert (1979), Burnham's celestial handbook: an observer's guide to the universe beyond the solar system, Dover books explaining science, vol. 3 (2nd ed.), Dover Publications, p. 1609, ISBN 978-0486236735
  • ^ Bogdanov, Slavko; et al. (April 2011), "Chandra X-ray Observations of 12 Millisecond Pulsars in the Globular Cluster M28", The Astrophysical Journal, 730 (2): 81, arXiv:1101.4944, Bibcode:2011ApJ...730...81B, doi:10.1088/0004-637X/730/2/81, S2CID 118621389
  • ^ "Nebulous, but no nebula". www.spacetelescope.org. Retrieved 11 March 2019.
  • Footnotes[edit]

    1. ^ On July 27

    External links[edit]


  • icon Stars
  • Outer space
  • List

  • M2
  • M3
  • M4
  • M5
  • M6
  • M7
  • M8
  • M9
  • M10
  • M11
  • M12
  • M13
  • M14
  • M15
  • M16
  • M17
  • M18
  • M19
  • M20
  • M21
  • M22
  • M23
  • M24
  • M25
  • M26
  • M27
  • M28
  • M29
  • M30
  • M31
  • M32
  • M33
  • M34
  • M35
  • M36
  • M37
  • M38
  • M39
  • M40
  • M41
  • M42
  • M43
  • M44
  • M45
  • M46
  • M47
  • M48
  • M49
  • M50
  • M51
  • M52
  • M53
  • M54
  • M55
  • M56
  • M57
  • M58
  • M59
  • M60
  • M61
  • M62
  • M63
  • M64
  • M65
  • M66
  • M67
  • M68
  • M69
  • M70
  • M71
  • M72
  • M73
  • M74
  • M75
  • M76
  • M77
  • M78
  • M79
  • M80
  • M81
  • M82
  • M83
  • M84
  • M85
  • M86
  • M87
  • M88
  • M89
  • M90
  • M91
  • M92
  • M93
  • M94
  • M95
  • M96
  • M97
  • M98
  • M99
  • M100
  • M101
  • M102
  • M103
  • Added
  • Painting of Charles Messier, creator of the Messier catalog

    See also

  • Catalogue of Nebulae and Clusters of Stars
  • Herschel 400 Catalogue
  • Index Catalogue
  • New General Catalogue
  • Revised New General Catalogue
  • Commons
  • Portal
  • New General Catalogue 6500 to 6999

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  • List of NGC objects

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Messier_28&oldid=1192500356"

    Categories: 
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