Nowadays, NGC 6229 is a widely discussed topic that has sparked the interest of many people around the world. Since its emergence, NGC 6229 has generated controversy and debate, provoking conflicting opinions among experts and society in general. In this article, we will thoroughly explore everything related to NGC 6229, from its origin to its current implications, in order to provide a global and complete vision that allows a thorough understanding of this topic that is so relevant today.
NGC 6229 | |
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![]() NGC 6229 as seen through the Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Class | VII |
Constellation | Hercules |
Right ascension | 16h 46m 58.8s |
Declination | +47° 31′ 40″ |
Apparent magnitude (V) | 9.4 |
Apparent dimensions (V) | 4.50' |
Physical characteristics | |
Absolute magnitude | -8.06 |
Metallicity | = -1.13±0.06[1] dex |
Other designations | GCL 47 |
NGC 6229 is a globular cluster located in the constellation Hercules. It is designated as GC(v)B in the galaxy morphological classification scheme and was discovered by the British astronomer William Herschel on 12 May 1787. NGC 6229 is located at about 100,000 light years away from Earth.[2][3][4][5]
It is an intermediate-metallicity globular cluster with two distinct generations of stars, and may be the remnant core of a spheroidal dwarf galaxy.[1]