FSR 0985
(SAI 62; MWSC 786)
0.81
UTI
0.59
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
1.8 [arcmin]
- CN 0.59 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0985 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 92.957 | 7.017 | 0.453 | -0.474 | -0.94 | 51.522 |
| Almeida et al. | 2025 | 92.941 | 7.011 | â | â | â | â |
| Zhang et al. | 2024 | 92.952 | 7.021 | â | â | â | â |
| Hunt & Reffert | 2024 | 92.952 | 7.021 | 0.453 | -0.478 | -0.941 | â |
| Cavallo et al. | 2024 | 92.952 | 7.018 | 0.451 | â | â | â |
| Hunt & Reffert | 2023 | 92.952 | 7.021 | 0.453 | -0.478 | -0.941 | â |
| Almeida et al. | 2023 | 92.945 | 7.008 | â | â | â | â |
| Just et al. | 2023 | 92.932 | 7.021 | â | â | â | â |
| Dias et al. | 2021 | 92.941 | 7.011 | 0.448 | -0.39 | -0.911 | â |
| Cantat-Gaudin et al. | 2020 | 92.953 | 7.02 | 0.462 | -0.433 | -0.904 | â |
| Cantat-Gaudin & Anders | 2020 | 92.953 | 7.02 | 0.462 | -0.433 | -0.904 | â |
| Bica et al. | 2019 | 92.953 | 7.026 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 92.953 | 7.02 | 0.462 | -0.433 | -0.904 | â |
| Kharchenko et al. | 2016 | 92.932 | 7.021 | â | â | â | â |
| Kharchenko et al. | 2013 | 92.94 | 7.02 | â | -0.64 | -3.84 | â |
| Glushkova et al. | 2010 | 92.954 | 7.023 | â | â | â | â |
| Froebrich et al. | 2007 | 92.954 | 7.025 | â | â | â | 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 | 1.92 | 1.54 | â | 231 | â | 193 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.335* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 337* | â | â |
| Cavallo et al. | 2024 | 2.36 | 1.56 | â | 324 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 2.03 | 1.18 | 0.92 | 236 | â | â | â | â |
| Almeida et al. | 2023 | 1.95 | 1.46 | â | 391 | -0.122 | 245* | 0.70 | â |
| Just et al. | 2023 | â | â | â | 316 | â | 226 | â | â |
| Dias et al. | 2021 | 1.92 | 1.54 | â | 231 | -0.091 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.14 | 1.18 | â | 257 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.04 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.04 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.45 | 2.45 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.45 | 2.45 | â | 316 | â | â | â | â |
| Glushkova et al. | 2010 | 2.63 | 1.71 | â | 398 | 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: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.