OC 0470
0.60
UTI
0.7
CN
1.0
Cdens
1.0
CC3
0.16
Clit
1.0
Cdup
Nm (P>50%)
90
Core radius and density
0.6 [pc], 16 [pc-2]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.16 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
OC 0470 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is rarely studied in the literature.
Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 117.342 | -46.366 | 2.549 | -4.712 | 9.06 | 17.631 |
| Liu et al. | 2025 | 117.38 | -46.37 | 2.54 | -4.68 | 8.97 | 15.1 |
| Wei et al. | 2025 | 117.913 | -46.329 | 2.542 | -4.727 | 9.015 | â |
| Swiggum et al. | 2024 | 117.375 | -46.368 | 2.54 | -4.684 | 8.975 | 17.974 |
| Hunt & Reffert | 2024 | 117.375 | -46.368 | 2.54 | -4.684 | 8.975 | 15.103 |
| Cavallo et al. | 2024 | 117.462 | -46.684 | 2.539 | â | â | â |
| Hunt & Reffert | 2023 | 117.375 | -46.368 | 2.54 | -4.684 | 8.975 | 15.103 |
| Hao et al. | 2022 | 117.367 | -46.354 | 2.561 | -4.673 | 9.011 | 21.25 |
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 | 0.385 | 0.515 | 0.86 | 7 | 0.250 | 378 | 0.53 | â |
| Liu et al. | 2025 | 0.46 | 0.14 | â | 13 | â | â | â | â |
| Wei et al. | 2025 | 0.23 | 1.62 | â | 6 | 0.500 | 378 | 0.53 | â |
| Swiggum et al. | 2024 | 0.39 | â | â | 7 | â | 381 | â | â |
| Hunt & Reffert | 2024 | 0.38 | 0.26 | 0.86 | 7 | â | 198(1) | â | â |
| Cavallo et al. | 2024 | 0.40 | 0.77 | â | 4 | -0.250 | â | â | â |
| Hunt & Reffert | 2023 | 0.38 | 0.26 | 0.86 | 7 | â | â | â | â |
| Hao et al. | 2022 | â | 2.13 | â | 8 | 0.250 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Liu et al. (2025)
Classified as primordial binary cluster 88 along with CWNU_1069, and of multiple system 29 along with HSC_2056 and CWNU_1069.
Palma et al. (2025)
Part of multiple system G27, along with CWNU_1069 and HSC_2056.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.98 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).