VDB 85
(vdBergh 85)
0.74
UTI
0.65
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
4.6 [arcmin]
- CN 0.65 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
VDB 85 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 101.742 | 1.348 | 0.553 | -0.98 | 0.38 | 28.859 |
| Almeida et al. | 2025 | 101.729 | 1.333 | â | â | â | â |
| Zhang et al. | 2024 | 101.72 | 1.324 | â | â | â | â |
| Hunt & Reffert | 2024 | 101.72 | 1.324 | 0.54 | -0.958 | 0.395 | -1.147 |
| Celli et al. | 2024 | 101.718 | 1.32 | â | â | â | â |
| Cavallo et al. | 2024 | 101.796 | 1.354 | 0.546 | â | â | â |
| Hunt & Reffert | 2023 | 101.72 | 1.324 | 0.54 | -0.958 | 0.395 | -1.147 |
| Dias et al. | 2021 | 101.729 | 1.333 | 0.55 | -0.973 | 0.345 | â |
| Cantat-Gaudin et al. | 2020 | 101.718 | 1.32 | 0.552 | -1.0 | 0.328 | â |
| Cantat-Gaudin & Anders | 2020 | 101.718 | 1.32 | 0.552 | -1.0 | 0.328 | â |
| Cantat-Gaudin et al. | 2018 | 101.718 | 1.32 | 0.552 | -1.0 | 0.328 | â |
| Dias et al. | 2002 | 101.725 | 1.333 | â | 0.17 | 1.23 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.72 | 1.21 | â | 13 | â | 199 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.225* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 317* | â | â |
| Celli et al. | 2024 | â | â | â | 4 | â | 127 | â | â |
| Cavallo et al. | 2024 | 2.01 | 1.21 | â | 35 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 1.68 | 0.99 | 2.16 | 45 | â | â | â | â |
| Dias et al. | 2021 | 1.72 | 1.21 | â | 13 | -0.055 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.69 | 1.35 | â | 4 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.72 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.72 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.64 | 5.95 | â | 71 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Bronze sample.