NGC 5800
(ESO 223 11; MWSC 2265)
Summary
NGC 5800 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 225.446 | -51.918 | – | -1.94 | -0.91 | – |
| Kharchenko et al. (2012) | 225.446 | -51.917 | – | -4.17 | 0.83 | – |
| Bica et al. (2019) | 225.455 | -51.934 | – | – | – | – |
| UCC | 225.471 | -51.937 | 0.235 | -7.206 | -3.42 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.06, Dist=1170.0, Age=9.2 |
| Kharchenko et al. (2012) | e_bv=0.541, distance=4844, log_age=9.25 |
Search coordinates in Bayestar19