- Mercer 3
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Mercer 3 Observation data (J2000 epoch) Constellation Scutum Right ascension 18h 18m 30s[1] Declination −16° 58′ 36″[1] Distance 13–26 kly (4–8 kpc[1]) Apparent magnitude (V) not visible Apparent dimensions (V) 39″ (half-light diameter)[1] Physical characteristics Mass 2–3 × 105 M☉ Radius 2–5 ly Estimated age 12 Gyr[1] See also: Globular cluster, List of globular clusters Mercer 3 is a heavily obscured globular cluster embedded in the disk of the Milky Way galaxy.[1] It was discovered in 2008 in the data obtained by 2MASS and GLIMPSE infrared surveys. The cluster is located in the Scutum constellation. It had avoided detection for such a long time due to the extremely strong foreground extinction in its direction reaching 24 magnitudes in the visible light. Mercer 3 is probably situated at the distance from 4 to 8 kpc from the Sun and has a half-light radius of 0.7–1.5 pc.[1]
Mercer 3 is an old globular cluster having the age of about 12 billion years. The mass of cluster is estimated at 2–3 hundred thousand solar masses.[1]
References
Stellar systems Bound Galaxy · Dwarf galaxy · Star cluster ( Globular cluster · Open cluster ) · Star system ( Binary star · Multiple star system )Unbound Visual grouping Categories:- Globular clusters
- Scutum constellation
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