NGC 2394
0.12
UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.16
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
2.7 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.25 Low quality
- Clit 0.16 Rarely studied
- Cdup 1.0 Unique
Overview
NGC 2394 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.
(*): The parallax distance estimate (~3.96 kpc) differs significantly from the median photometric distance (~0.94 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 112.145 | 7.101 | 0.253 | -1.039 | -0.577 | â |
| Dias et al. | 2018 | â | â | â | -2.61 | -0.17 | â |
| Loktin & Popova | 2017 | 112.14 | 7.087 | â | -6.02 | -4.569 | â |
| Sampedro et al. | 2017 | 112.15 | 7.087 | â | â | â | â |
| Dias et al. | 2014 | 112.15 | 7.087 | â | -0.27 | -0.83 | â |
| Bukowiecki et al. | 2011 | 112.158 | 7.161 | â | â | â | â |
| Dias et al. | 2002 | 112.15 | 7.087 | â | -0.27 | -0.83 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.94 | 0.41 | â | 891 | â | 88 | â | â |
| Loktin & Popova | 2017 | 2.48 | 0.13 | â | 832 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 88 | â | â |
| Bukowiecki et al. | 2011 | 0.94(1) | 0.41 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 0.94 | 0.41 | â | 891 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Cantat-Gaudin & Anders (2020)
Flagged as non-existent in the Revised NGC. Sparse CMD-based estimates exist, but it is considered an asterism in recent compilations. More details in Appendix A of the article.