Collinder 85
(NGC 2186; MWSC 787; OCL 498; FoF 17)
0.91
UTI
0.78
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
48.9 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 85 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. 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 | 99999β | 93.031 | 5.45 | 0.432 | 0.375 | -1.96 | 43.369 |
| Li et al. | 2025 | 93.031 | 5.453 | 0.413 | 0.415 | -1.993 | β |
| Almeida et al. | 2025 | 93.022 | 5.452 | β | β | β | β |
| Zhang et al. | 2024 | 93.028 | 5.451 | β | β | β | β |
| Hunt & Reffert | 2024 | 93.028 | 5.451 | 0.422 | 0.383 | -1.944 | 43.378 |
| Cavallo et al. | 2024 | 93.021 | 5.457 | 0.426 | β | β | β |
| Hunt & Reffert | 2023 | 93.028 | 5.451 | 0.422 | 0.383 | -1.944 | 43.378 |
| Just et al. | 2023 | 93.03 | 5.464 | β | β | β | β |
| Jaehnig et al. | 2021 | 93.031 | 5.457 | 0.437 | 0.423 | -1.998 | β |
| Rain et al. | 2021 | 93.031 | 5.453 | 0.413 | 0.415 | -1.993 | β |
| Dias et al. | 2021 | 93.022 | 5.452 | 0.412 | 0.405 | -1.967 | β |
| Cantat-Gaudin et al. | 2020 | 93.031 | 5.453 | 0.413 | 0.415 | -1.993 | β |
| SΓ‘nchez et al. | 2020 | 93.033 | 5.454 | β | 0.527 | -2.038 | β |
| Cantat-Gaudin & Anders | 2020 | 93.031 | 5.453 | 0.413 | 0.415 | -1.993 | β |
| Liu & Pang | 2019 | 93.047 | 5.462 | 0.426 | 0.409 | -1.967 | β |
| Soubiran et al. | 2018 | 93.031 | 5.453 | β | β | β | 21.98 |
| Bica et al. | 2019 | 93.035 | 5.455 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 93.031 | 5.453 | 0.413 | 0.415 | -1.993 | β |
| Loktin & Popova | 2017 | 93.03 | 5.454 | β | 0.168 | 0.487 | 20.2 |
| Kharchenko et al. | 2016 | 93.03 | 5.464 | β | β | β | β |
| Dias et al. | 2014 | 93.033 | 5.454 | β | -0.23 | -2.79 | β |
| Kharchenko et al. | 2013 | 93.037 | 5.463 | β | 0.03 | -0.12 | 20.2 |
| Gozha et al. | 2012 | 93.033 | 5.454 | β | β | β | β |
| Piskunov et al. | 2008 | 93.021 | 5.459 | β | β | β | β |
| van den Bergh | 2006 | 93.025 | 5.467 | β | β | β | β |
| Kharchenko et al. | 2005 | 93.03 | 5.46 | β | 1.61 | -0.29 | β |
| Kharchenko et al. | 2003 | 93.03 | 5.46 | β | 1.57 | -0.86 | β |
| Dias et al. | 2002 | 93.033 | 5.454 | β | -0.23 | -2.79 | 20.15 |
π‘ 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 | 99999β | 2.07 | 0.82 | 1.21 | 158 | -0.153 | 262 | β | 0.0 |
| Li et al. | 2025 | 2.12 | 0.88 | β | 279 | -0.071 | β | β | β |
| Almeida et al. | 2025 | 2.03 | 1.06 | β | 149 | β | 418 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.297(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 674(1) | β | β |
| Cavallo et al. | 2024 | 2.15 | 0.93 | β | 269 | 0.000 | β | β | β |
| Hunt & Reffert | 2023 | 2.11 | 0.60 | 1.21 | 344 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 158 | β | 106 | β | β |
| Jaehnig et al. | 2021 | 2.29(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.26 | 0.84 | β | 200 | β | β | β | 0 |
| Dias et al. | 2021 | 2.03 | 1.06 | β | 149 | -0.153 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.25 | 0.65 | β | 251 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.26 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 933 | -0.500 | β | β | β |
| Soubiran et al. | 2018 | 2.26 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.26 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.71 | 0.82 | β | 65 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.45 | 0.81 | β | 158 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.45 | 0.81 | β | 158 | β | β | β | β |
| Gozha et al. | 2012 | 1.45 | β | β | 200 | β | 35 | β | β |
| Piskunov et al. | 2008 | 1.45 | 0.81 | β | 120 | β | β | β | β |
| van den Bergh | 2006 | 1.45 | 0.84 | β | 55 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.45 | 0.81 | β | 120 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.45 | 0.68 | β | β | β | β | β | β |
| Dias et al. | 2002 | 2.70 | 0.84 | β | 200 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.