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- Messier_14 abstract "Messier 14 (also known as M14 or NGC 6402) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier in 1764.At a distance of about 30,000 light-years, M14 contains several hundreds of thousands of stars. At an apparent magnitude +7.6 it can be easily observed with binoculars. Medium-sized telescopes will show some hint of the individual stars of which the brightest is of magnitude +14.The total luminosity of M14 is in the order of 400,000 times that of the Sun corresponding to an absolute magnitude of -9.12. The shape of the cluster is decidedly elongated. M14 is about 100 light-years across.A respectable total of 70 variable stars is known in M14, many of the W Virginis variety common in globular clusters. In 1938, a nova appeared although this was not discovered until photographic plates from that time were studied in 1964. It is estimated that the nova reached a maximum brightness of magnitude +9.2, over five times brighter than the brightest 'normal' star in the cluster.Slightly over 3° southwest of M14 lies the faint globular cluster NGC 6366.".
- Messier_14 thumbnail Messier_object_014.jpg?width=300.
- Messier_14 wikiPageExternalLink cluster_4.php?ggc=M+14.
- Messier_14 wikiPageExternalLink m014.html.
- Messier_14 wikiPageID "319545".
- Messier_14 wikiPageRevisionID "592476170".
- Messier_14 appmagV "+8.32".
- Messier_14 caption "Messier 14, from 2MASS".
- Messier_14 class "VIII".
- Messier_14 constellation Ophiuchus.
- Messier_14 epoch Epoch_(astronomy).
- Messier_14 hasPhotoCollection Messier_14.
- Messier_14 metalFe "–1.28".
- Messier_14 name "Messier 14".
- Messier_14 names "NGC 6402".
- Messier_14 radiusLy "50.0".
- Messier_14 sizeV "11".
- Messier_14 subject Category:Globular_clusters.
- Messier_14 subject Category:Messier_objects.
- Messier_14 subject Category:NGC_objects.
- Messier_14 subject Category:Objects_within_100_kly_of_Earth.
- Messier_14 subject Category:Ophiuchus_(constellation).
- Messier_14 comment "Messier 14 (also known as M14 or NGC 6402) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier in 1764.At a distance of about 30,000 light-years, M14 contains several hundreds of thousands of stars. At an apparent magnitude +7.6 it can be easily observed with binoculars.".
- Messier_14 label "Cúmulo globular M14".
- Messier_14 label "M 14 (шаровое скопление)".
- Messier_14 label "M14 (amas globulaire)".
- Messier_14 label "M14 (astronomia)".
- Messier_14 label "M14 (天体)".
- Messier_14 label "M14 (球狀星團)".
- Messier_14 label "Messier 14".
- Messier_14 label "Messier 14".
- Messier_14 label "Messier 14".
- Messier_14 label "Messier 14".
- Messier_14 label "Messier 14".
- Messier_14 label "مسييه 14".
- Messier_14 sameAs Messier_14.
- Messier_14 sameAs Messier_14.
- Messier_14 sameAs Μεσιέ_14.
- Messier_14 sameAs Cúmulo_globular_M14.
- Messier_14 sameAs M14_(amas_globulaire).
- Messier_14 sameAs Messier_14.
- Messier_14 sameAs M14_(astronomia).
- Messier_14 sameAs M14_(天体).
- Messier_14 sameAs 메시에_14.
- Messier_14 sameAs Messier_14.
- Messier_14 sameAs Messier_14.
- Messier_14 sameAs Messier_14.
- Messier_14 sameAs m.01vb8_.
- Messier_14 sameAs Q11320.
- Messier_14 sameAs Q11320.
- Messier_14 wasDerivedFrom Messier_14?oldid=592476170.
- Messier_14 depiction Messier_object_014.jpg.
- Messier_14 isPrimaryTopicOf Messier_14.