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Messier 9: Difference between revisions
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(Created page with "Messier 9 or M9 (also designated NGC 6333) is a globular cluster in the constellation of Ophiuchus. It was discovered by Charles Messier in 1764.M9 is one of the nearer gl...") |
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The total luminosity of this cluster is around 120,000 times that of the Sun, the absolute magnitude being -8.04. The brightest individual stars in M9 are of apparent magnitude 13.5, making them visible in moderately sized telescopes. There have been 13 variable stars found in M9.Nearby, at about 80' to the northeast of M9 is the dimmer globular cluster NGC 6356, while at about 80' to the southeast is the globular NGC 6342.<ref>[http://en.wikipedia.org/wiki/Messier_9 Messier 9]</ref> | The total luminosity of this cluster is around 120,000 times that of the Sun, the absolute magnitude being -8.04. The brightest individual stars in M9 are of apparent magnitude 13.5, making them visible in moderately sized telescopes. There have been 13 variable stars found in M9.Nearby, at about 80' to the northeast of M9 is the dimmer globular cluster NGC 6356, while at about 80' to the southeast is the globular NGC 6342.<ref>[http://en.wikipedia.org/wiki/Messier_9 Messier 9]</ref> | ||
==References==<references/>Found in HGS Manual on Page 108 Found in HGS Manual on Page 115 [[Category: Ascension]][[Category: HGS Manual]] | |||
==References== | |||
<references/> | |||
Found in HGS Manual on Page 108 Found in HGS Manual on Page 115 | |||
[[Category: Ascension]][[Category: HGS Manual]] | |||