
M9 · globular cluster
Messier 9
Messier 9 or M9 is a globular cluster in the constellation of Ophiuchus.
Identity & coordinates
Identification
- Primary designation
- M9
- All designations
- M9 · NGC 6333
- Object type
- Globular Cluster
- Constellation
- Ophiuchus
- Best viewing
- Summer
Coordinates & physical
- Right ascension (J2000)
- 17h 19m 11s
- Declination (J2000)
- −18° 30' 58"
- Apparent magnitude (V)
- —
- Distance
- —
Visibility tonight
The science
Messier 9 or M9 is a globular cluster in the constellation of Ophiuchus. It is positioned in the southern part of the constellation to the southwest of Eta Ophiuchi, and lies atop a dark cloud of dust designated Barnard 64. The cluster was discovered by French astronomer Charles Messier on June 3, 1764, who described it as a "nebula without stars". In 1783, English astronomer William Herschel was able to use his reflector to resolve individual stars within the cluster. He estimated the cluster to be 7–8′ in diameter with stars densely packed near the center.
Summary adapted from Wikipedia · CC-BY-SA-4.0
References
- SIMBAD Not resolved
- NED Fetched May 8, 2026 View in NED ↗
- Wikipedia Fetched May 8, 2026 Read full article ↗
Wikipedia title resolved via designation — fell back to an alternate catalog designation.
1 merge conflict resolved
- coordinates: SIMBAD missing → NED used



