FSR 0968
(MWSC 785)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
4.8 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0968 is a rich, 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, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 92.843 | 11.86 | 0.377 | -0.426 | -1.178 | 52.95 |
| Li et al. | 2025 | 92.843 | 11.863 | 0.382 | -0.356 | -1.158 | â |
| Almeida et al. | 2025 | 92.849 | 11.853 | â | â | â | â |
| Zhang et al. | 2024 | 92.835 | 11.869 | â | â | â | â |
| Hunt & Reffert | 2024 | 92.835 | 11.869 | 0.375 | -0.439 | -1.18 | 52.957 |
| Cavallo et al. | 2024 | 92.842 | 11.856 | 0.376 | â | â | â |
| Hunt & Reffert | 2023 | 92.835 | 11.869 | 0.375 | -0.439 | -1.18 | 52.957 |
| Almeida et al. | 2023 | 92.845 | 11.853 | â | â | â | â |
| Just et al. | 2023 | 92.833 | 11.872 | â | â | â | â |
| Dias et al. | 2021 | 92.849 | 11.853 | 0.377 | -0.373 | -1.149 | â |
| Cantat-Gaudin et al. | 2020 | 92.843 | 11.863 | 0.382 | -0.356 | -1.158 | â |
| Cantat-Gaudin & Anders | 2020 | 92.843 | 11.863 | 0.382 | -0.356 | -1.158 | â |
| Bossini et al. | 2019 | 92.843 | 11.863 | â | â | â | â |
| Bica et al. | 2019 | 92.834 | 11.86 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 92.843 | 11.863 | 0.382 | -0.356 | -1.158 | â |
| Kharchenko et al. | 2016 | 92.833 | 11.872 | â | â | â | â |
| Kharchenko et al. | 2013 | 92.841 | 11.871 | â | -0.4 | -1.8 | â |
| Froebrich et al. | 2007 | 92.838 | 11.861 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.34 | 1.41 | â | 70 | -0.057 | â | â | â |
| Almeida et al. | 2025 | 2.39 | 1.64 | â | 18 | â | 199 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.257* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 663* | â | â |
| Cavallo et al. | 2024 | 2.25 | 1.57 | â | 47 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 2.35 | 1.39 | 0.63 | 59 | â | â | â | â |
| Almeida et al. | 2023 | 2.25 | 1.54 | â | 45 | -0.157 | 214* | 0.61 | â |
| Just et al. | 2023 | â | â | â | 331 | â | 173 | â | â |
| Dias et al. | 2021 | 2.39 | 1.64 | â | 18 | -0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.67 | 1.04 | â | 83 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.43 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 2.43 | 1.17 | â | 82 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.43 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.19 | 0.97 | â | 331 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.19 | 0.97 | â | 331 | 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.
Cavallo et al. (2024)
Gold sample.