MCM 52
Summary
MCM 52 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 20 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 |
|---|---|---|---|---|---|---|
| Mercer et al. (2005) | 216.264 | -60.46 | – | – | – | – |
| UCC | 216.212 | -60.446 | 0.331 | -6.5 | -2.304 | -27.239 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19