Globular cluster
Messier 107
Also M107 · NGC 6171
A globular cluster: tens of thousands of very old stars in a tight ball, orbiting the Milky Way's centre.
Measured
- Distance
- 18,360 light-years
- Size
- about 54 light-years across (approximate)
- Constellation
- Ophiuchus
- Position (J2000)
- RA 16h 32m 32s, Dec −13.05°
How far, from the Sun
18,400 light-years. To cross it:
- Light18,400 years
- Voyager 1's speed326 million years
- Driving at 100 km/h198 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 holds about 61,200 times the Sun's mass in stars (Baumgardt's globular cluster database).
How it was found
- Helen Sawyer Hogg added it to Messier's list in 1947; Pierre Méchain had discovered it in 1782.
Where this comes from
- Baumgardt & Vasiliev 2021, MNRAS 505, 5957 (5.63 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.