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M 14 (globular cluster)

The globular cluster M 14 (also known as M 14 or NGC 6402 ) is a globular star cluster in the constellation Ophiuchus .

Ball cluster M 14
Star cluster
Messier object 014.jpg
Research history
DiscovererCharles Messier
opening date1764
DesignationsNGC 6402 , M 14
Observational data
( Age J2000.0 )
Type ofGlobular cluster
Right ascension
Declination
Distance30 300 St. years (9300 pc )
Visible magnitude (V)7.6
Visible Dimensions (V)11,0 ′
ConstellationOphiuchus
physical characteristics
ClassVIII
Radius50 St. years
Absolute magnitude (V)

Content

  • 1 Discovery History
  • 2 Interesting features
  • 3 Observations
    • 3.1 Neighbors in the sky from the Messier catalog
    • 3.2 Sequence of observation at the Messier Marathon
  • 4 Images
  • 5 See also
  • 6 notes
  • 7 References

Discovery History

It was discovered by Charles Messier in 1764 .

Interesting features

Located at a distance of 30,300 light-years , M 14 contains several hundred thousand stars. The total luminosity M 14 is 400 thousand times greater than the solar luminosity , which corresponds to an absolute magnitude of −9.12 m . M 14 extends 100 light-years across.

About 70 variable stars are known in the cluster, many of which belong to the Virgo class W , typical of globular clusters. In 1938, a new one appeared in the cluster, although it was not seen until 1964 when the photographic plates of that time were studied. According to estimates, the new one reached a maximum of +9.2 stellar magnitude, which is 5 times brighter than the brightest “normal” star in the cluster.

Observations

 
M 14 in Ophiuchus constellation

This globular cluster lies in the summer constellation part of Ophiuchus poor with landmarks and finding an object, even with good binoculars or a telescope finder, is not an easy task. M 14 is located just south of the middle of the segment connecting ν and σ Ophiuchus. With binoculars, the cluster is barely noticeable. The cluster is allowed to stars on the periphery only in a telescope with an aperture of 200 mm or more.

About 3 ° southwest of M 14 (next to the 4.5m star) is a very dim globular cluster NGC 6366 .

Neighbors in the Sky from Messier Catalog

  • M 10 and M 12 - (to the west - closer to the center of Ophiuchus) a pair of rather bright and different clusters;
  • M 9 - (on the southern outskirts of Ophiuchus) less concentrated and not so rich;
  • M 11 - (in the east, in the Shield) one of the most beautiful open clusters of the summer sky.

Sequence of Observation at the Messier Marathon

... M 4 → M 29 → M 14 → M 9 → M 71 ...

Images

 
 

Gal. Longitude 21.3239 °
Gal. Latitude + 14.8044 °
Distance 30 300 St. years

See also

  • List of Messier objects
  • New General Catalog


Notes

  1. ↑ Harris W. E. A catalog of parameters for globular clusters in the Milky Way // Astron. J. / J. G. III - IOP Publishing , 1996. - Vol. 112, Iss. 4. - P. 1487. - ISSN 0004-6256 ; 1538-3881 - doi: 10.1086 / 118116
    <a href=" https://wikidata.org/wiki/Track:Q28739659 "> </a> <a href=" https://wikidata.org/wiki/Track:Q6234745 "> </a> <a href = " https://wikidata.org/wiki/Track:Q2915886 "> </a> <a href=" https://wikidata.org/wiki/Track:Q669166 "> </a> <a href = " https://wikidata.org/wiki/Track:Q28739509 "> </a>

Links

  • SEDS Messier pages on M 14



Source - https://ru.wikipedia.org/w/index.php?title=M_14_(spherical cluster )&oldid = 91239705


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