NGC 2312
Summary
NGC 2312 is a poorly populated, very loose object of very 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 8 years.
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) | 104.696 | 10.295 | – | -3.54 | -2.32 | – |
| Kharchenko et al. (2012) | 104.7 | 10.28 | – | -0.9 | -2.8 | – |
| Loktin & Popova (2017) | 104.7 | 10.295 | – | -0.568 | -0.725 | – |
| UCC | 104.707 | 10.319 | 0.265 | -0.997 | -1.223 | 72.472 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.16, Dist=2245.0, Age=8.52 |
| Kharchenko et al. (2012) | e_bv=0.208, distance=2436, log_age=8.81 |
| Loktin & Popova (2017) | E(B-V)=0.071, Dist=3058, logt=8.86 |
Search coordinates in Bayestar19