VDB 80
(vdBergh 80)
0.83
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
14.8 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
VDB 80 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 97.712 | -9.599 | 1.013 | -3.254 | 0.48 | 37.033 |
| Almeida et al. | 2025 | 97.747 | -9.621 | â | â | â | â |
| Alfonso et al. | 2024 | 97.635 | -9.548 | 0.976 | -3.258 | 0.736 | â |
| Hunt & Reffert | 2024 | 97.731 | -9.633 | 1.001 | -3.25 | 0.569 | 35.818 |
| Celli et al. | 2024 | 97.739 | -9.625 | â | â | â | â |
| Cavallo et al. | 2024 | 97.43 | -9.628 | 1.003 | â | â | â |
| Hunt & Reffert | 2023 | 97.731 | -9.633 | 1.001 | -3.25 | 0.569 | 35.818 |
| Almeida et al. | 2023 | 97.762 | -9.612 | â | â | â | â |
| He et al. | 2022 | 97.795 | -9.583 | 1.029 | -3.227 | 0.459 | â |
| Dias et al. | 2021 | 97.747 | -9.621 | 1.026 | -3.285 | 0.481 | â |
| Cantat-Gaudin et al. | 2020 | 97.739 | -9.625 | 1.025 | -3.298 | 0.418 | â |
| Cantat-Gaudin & Anders | 2020 | 97.739 | -9.625 | 1.025 | -3.298 | 0.418 | â |
| Cantat-Gaudin et al. | 2018 | 97.739 | -9.625 | 1.025 | -3.298 | 0.418 | â |
| Loktin & Popova | 2017 | 97.71 | -9.654 | â | -3.45 | -11.64 | â |
| Bukowiecki et al. | 2011 | 97.696 | -9.656 | â | â | â | â |
| Dias et al. | 2002 | 97.708 | -9.655 | â | -3.45 | -11.64 | 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 | 0.95 | 1.99 | 2.56 | 6 | -0.144 | 249 | 0.72 | â |
| Almeida et al. | 2025 | 0.95 | 1.73 | â | 6 | â | 280 | â | â |
| Alfonso et al. | 2024 | 0.91 | 1.50 | â | 10 | -0.141 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 217(1) | â | â |
| Celli et al. | 2024 | â | â | â | 6 | â | 129 | â | â |
| Cavallo et al. | 2024 | 1.29 | 1.99 | â | 9 | -0.270 | â | â | â |
| Hunt & Reffert | 2023 | 0.95 | 2.00 | 2.56 | 6 | â | â | â | â |
| Almeida et al. | 2023 | 0.94 | 2.11 | â | 9 | -0.053 | 249(1) | 0.72 | â |
| He et al. | 2022 | â | 2.40 | â | 6 | â | â | â | â |
| Dias et al. | 2021 | 0.95 | 1.73 | â | 6 | -0.148 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.91 | 1.53 | â | 6 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.95 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.95 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.15 | 3.76 | â | 14 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 336 | â | â |
| Bukowiecki et al. | 2011 | 2.37(1) | 2.88 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 2.10 | 1.89 | â | 5 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P338, along with CWNU_201.
Cavallo et al. (2024)
Wood sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.