NGC 2430
Summary
NGC 2430 is a sparse, 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: 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 |
|---|---|---|---|---|---|---|
| Piskunov et al. (2008) | 114.894 | -16.348 | – | – | – | – |
| Kharchenko et al. (2012) | 114.916 | -16.38 | – | -2.74 | 2.09 | – |
| Loktin & Popova (2017) | 114.915 | -16.375 | – | -0.818 | 1.064 | 2.8 |
| UCC | 114.9 | -16.412 | 0.261 | -2.496 | 2.273 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Piskunov et al. (2008) | E(B-V)=0.17, Dist=650, logt=8.68, logMA=1.241 |
| Kharchenko et al. (2012) | e_bv=0.167, distance=707, log_age=7.7, metallicity=0.13 |
| Loktin & Popova (2017) | E(B-V)=0.0, Dist=1905, logt=8.91 |
Search coordinates in Bayestar19