Gaia 1 | |
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![]() Sirius and the Gaia 1 cluster | |
Observation data (J2000epoch) | |
Right ascension | 6h 45m 52.8s[1] |
Declination | −16° 45′ 00″[1] |
Distance | 15 kly (4.6 kpc)[1] |
Apparent dimensions (V) | 13arcmins[1] |
Physical characteristics | |
Mass | 2.2×104[1] M☉ |
Radius | 29 ly[1] |
Estimated age | 6.3 Gyr[1] |
Associations | |
Constellation | Canis Major |
See also:Open cluster,List of open clusters |
Gaia 1 is anopen cluster of stars discovered in 2017 byastronomers using data from theGaia Space Observatory. It is a high-mass and bright cluster, but it remained unseen in priorastronomy due toveiling glare in ordinarytelescopes overwhelmed by the starSirius, which lies 10arcmins west.[2] Itshalf-light radius is about 29 light-years (9 pc), assuming a distance of 15,000 light-years (4,600 pc), and it has an estimated mass of about 22,000 M☉.[1]
Researchers detected the Gaia 1 cluster applying automated"star gauging" to the Gaia observatory's data on star locations.[3] This analysis surprisingly indicated a prominent concentration of stars, previously unknown and uncataloged, adjacent to Sirius. Gaia observed a cluster population of approximately 1,200 stars down to Gaiamagnitude 19. Analysis of2MASS data for those stars shows ared giant branch and a pronouncedred clump that allows theabsolute magnitude of the stars to be deduced and the distance calculated. Fitting the red giant branch also allows the age of the cluster to be calculated at 6.3 billion years.[1]
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