Globular cluster
Messier 9
Also M9 · NGC 6333
A globular cluster: hundreds of thousands of very old stars in a tight ball, orbiting the Milky Way's centre.
Measured
- Distance
- 27,070 light-years
- Size
- about 68 light-years across (approximate)
- Constellation
- Ophiuchus
- Position (J2000)
- RA 17h 19m 12s, Dec −18.52°
How far, from the Sun
27,100 light-years. To cross it:
- Light27,100 years
- Voyager 1's speed481 million years
- Driving at 100 km/h292 billion years
Voyager 1 at the speed it moved outward over the year to 2026-10-25 (JPL Horizons). Driving: nonstop, never refuelling.
Facts
- It is one of the globular clusters closest to the Milky Way's centre, dimmed by dust in front of it.
How it was found
- Messier discovered it in 1764.
Where this comes from
- Baumgardt & Vasiliev 2021, MNRAS 505, 5957 (8.3 kpc; the distances in public/sky/galaxy/globulars.json)
- This research has made use of the SIMBAD database, CDS, Strasbourg, France (Wenger et al. 2000, A&AS 143, 9).
- This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier).
Every catalogue Ouranos draws is credited on the credits page.