Globular Cluster NGC 1851 in the Southern Constellation Columba

C73 · globular cluster

NGC 1851

NGC 1851 is a relatively massive globular cluster located in the southern constellation of Columba.

RA05h 14m 06sDec−40° 02' 48"

Image: NASA/JPL-Caltech/SSC. Source: JPL via images.nasa.gov.

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Identity & coordinates

Identification

Primary designation
C73
All designations
C73 · NGC 1851
Object type
Globular Cluster
Constellation
Col
Best viewing
Winter

Coordinates & physical

Right ascension (J2000)
05h 14m 06s
Declination (J2000)
−40° 02' 48"
Apparent magnitude (V)
Distance
III

Visibility tonight

V

The science

NGC 1851 is a relatively massive globular cluster located in the southern constellation of Columba. Astronomer John Dreyer described it as not very bright but very large, round, well resolved, and clearly consisting of stars. It is located 39.5 kilolight-years from the Sun, and 54.1 kilolight-years from the Galactic Center. The cluster is following a highly eccentric orbit through the galaxy, with an eccentricity of about 0.7.

Summary adapted from Wikipedia · CC-BY-SA-4.0

VII

References

Wikipedia title resolved via designation — fell back to an alternate catalog designation.

1 merge conflict resolved
  • coordinates: SIMBAD missing → NED used