Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 3  ·  NGC 5272
Globular cluster M3, RalfThielenPicart
Globular cluster M3
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Globular cluster M3

Globular cluster M3, RalfThielenPicart
Globular cluster M3
Powered byPixInsight

Globular cluster M3

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Description

Messier 3 (M3, NGC 5272) is one of the most outstanding globular clusters. It consists of about half a million stars.
At a distance of 33,900 light years, M3 is further from us than the center of our galaxy. Nevertheless, it seems to have a visual brightness of 6.2 mag; its absolute brightness is -8.93 Mag. Its luminosity is 300,000 times that of our sun. Under very favorable visibility conditions, M3 can even be seen in the night sky with the naked eye. Even in small telescopes, M3 is a fascinating object. Its apparent diameter is 18 minutes of arc, so its real linear diameter corresponds to about 180 light years. Other photographic investigations allow a conclusion to be drawn that the diameter is approx. 20 arc minutes or, in real terms, approx. 200 light years. According to the website "SEDS Messier", the gravity of M3 dominates a spherical volume with a diameter of 760 light years. Members of the globular cluster that exceed the limit of this spherical volume are "forced" to leave M3 by the gravitational forces of the Milky Way. M3 is moving towards us at a speed of 147.6 km / s.

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Globular cluster M3, RalfThielenPicart