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Messier 28

Coordinates:Sky map18h 24m 32.89s, −24° 52′ 11.4″
From Wikipedia, the free encyclopedia
Globular cluster in the constellation of Sagittarius
For other uses, seeM28.
Messier 28
Globular cluster Messier 28 in Sagittarius
Observation data (J2000epoch)
ClassIV[1]
ConstellationSagittarius
Right ascension18h 24m 32.89s[2]
Declination–24° 52′ 11.4″[2]
Distance18.26 ± 0.98 kly (5.6 ± 0.3 kpc)[3]
Apparent magnitude (V)6.8[4]
Apparent dimensions (V)11′.2[5]
Physical characteristics
Mass5.51×105[6] M
Radius30 ly[7]
VHB15.55 ± 0.10[8]
Metallicity[Fe/H] = –1.32[6]dex
Estimated age12.0 Gyr[9]
Notable featuresContains first pulsar discovered in a globular[10]
Other designationsGCl 94, M 28,NGC 6626[2]
See also:Globular cluster,List of globular clusters

Messier 28 orM28, also known asNGC 6626, is aglobular cluster of stars in the center-west ofSagittarius. It was discovered by French astronomerCharles Messier in 1764.[11][a] He briefly described it as a "nebula containing no star... round, seen with difficulty in 312-foot telescope;Diam 2."[12]

In the sky it is less than a degree to the northwest of the 3rdmagnitude starKaus Borealis (LambdaSgr). 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 18,300light-years away fromEarth.[3] It is about551000 M[6] and its metallicity (averaging −1.32 which means more than 10 times less than our own star), coherency and preponderence of olderstellar evolution objects, support its dating to very roughly 12 billion years old.[9] 18RR Lyrae typevariable stars have been found within.

It bore the first discovery of amillisecond pulsar in a globular cluster – PSR B1821–24. This was using theLovell Telescope atJodrell Bank Observatory, England.[10] A total of 11 further of these have since been detected in it withthe telescope atGreen Bank Observatory,West Virginia. As of 2011, these number the third-most in a cluster tied to the Milky Way, followingTerzan 5 and47 Tucanae.[13]

Gallery

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  • Messier 28 taken by Hubble.[14]
    Messier 28 taken byHubble.[14]
  • 2.5' view of M28 taken by Hubble Space Telescope.
    2.5' view of M28 taken by Hubble Space Telescope.
  • Messier 28 on 2MASS; wide angle
    Messier 28 on2MASS; wide angle
  • Map showing location of M28
    Map showing location of M28

See also

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References and footnotes

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References

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  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.
  2. ^abc"M 28".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2006-11-16.
  3. ^abOliveira, 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.
  4. ^"Messier 28".SEDS Messier Catalog. Retrieved21 July 2024.
  5. ^abInglis, 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.
  6. ^abcBoyles, 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.
  7. ^Fromtrigonometry: radius = distance × sin( diameter_angle / 2 ) = 30 ly
  8. ^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
  9. ^abKoleva, 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
  10. ^ab"JBO - Stars".Jodrell Bank Observatory. Retrieved2007-06-01.
  11. ^abcThompson, Robert Bruce; Thompson, Barbara Fritchman (2007),Illustrated Guide to Astronomical Wonders, Diy Science,O'Reilly Media, Inc., p. 402,ISBN 978-0596526856.
  12. ^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
  13. ^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
  14. ^"Nebulous, but no nebula".www.spacetelescope.org. Retrieved11 March 2019.

Footnotes

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  1. ^On July 27

External links

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Wikimedia Commons has media related toMessier 28.


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Painting of Charles Messier, creator of the Messier catalog
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