MCM 62
Summary
MCM 62 is a sparse, very loose object of intermediate 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.
This object shares a moderate percentage of members with a later reported entry.
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) | 236.272 | -54.137 | – | – | – | – |
| UCC | 236.088 | -54.217 | 0.415 | -3.768 | -3.109 | -32.079 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 2728 | 32.0 | 235.97 | -54.31 | 0.43 | -3.7 | -3.19 | -33.99 | 0.35 |