FSR 0850
(MWSC 662; FoF 77; LISC 0122)
0.78
UTI
0.79
CN
0.81
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
218
Core radius and density
2.5 [pc], 4.1 [pc-2]
- CN 0.79 Rich
- Cdens 0.81 Dense
- CC3 0.75 High quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0850 is a rich, 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 age, metallicity, and mass parameters (see Parameters). It is 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 | 99999â | 86.261 | 24.744 | 0.444 | 1.263 | -2.528 | 18.599 |
| Hu & Soubiran | 2025 | 86.273 | 24.761 | â | â | â | â |
| Almeida et al. | 2025 | 86.266 | 24.744 | â | â | â | â |
| Zhang et al. | 2024 | 86.241 | 24.745 | â | â | â | â |
| Hunt & Reffert | 2024 | 86.241 | 24.745 | 0.447 | 1.248 | -2.524 | 15.209 |
| Cavallo et al. | 2024 | 86.274 | 24.761 | 0.446 | â | â | â |
| Hunt & Reffert | 2023 | 86.241 | 24.745 | 0.447 | 1.248 | -2.524 | 15.209 |
| Almeida et al. | 2023 | 86.278 | 24.753 | â | â | â | â |
| Just et al. | 2023 | 86.271 | 24.739 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 86.257 | 24.74 | â | â | â | â |
| Dias et al. | 2021 | 86.266 | 24.744 | 0.441 | 1.296 | -2.57 | 16.987 |
| Cantat-Gaudin et al. | 2020 | 86.257 | 24.74 | 0.438 | 1.301 | -2.555 | â |
| Zhong et al. | 2020 | 86.257 | 24.74 | â | 1.301 | -2.555 | 17.289 |
| Cantat-Gaudin & Anders | 2020 | 86.257 | 24.74 | 0.438 | 1.301 | -2.555 | â |
| Liu & Pang | 2019 | 86.269 | 24.76 | 0.461 | 1.237 | -2.491 | â |
| Dias et al. | 2019 | 86.312 | 24.754 | 0.456 | 1.286 | -2.518 | 19.37 |
| Soubiran et al. | 2018 | 86.257 | 24.74 | â | â | â | 19.24 |
| Cantat-Gaudin et al. | 2018 | 86.257 | 24.74 | 0.438 | 1.301 | -2.555 | â |
| Dib et al. | 2018 | 86.28 | 24.738 | â | â | â | â |
| Sampedro et al. | 2017 | 86.312 | 24.754 | â | -1.07 | 0.58 | â |
| Kharchenko et al. | 2016 | 86.271 | 24.739 | â | â | â | â |
| Kharchenko et al. | 2013 | 86.28 | 24.738 | â | 0.07 | -3.88 | -17.0 |
| Camargo et al. | 2012 | 86.312 | 24.754 | â | â | â | â |
| Froebrich et al. | 2007 | 86.312 | 24.754 | â | â | â | â |
| Dias et al. | 2002 | 86.312 | 24.754 | â | 0.07 | -3.88 | 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 | 2.04 | 1.74 | 2.28 | 263 | -0.160 | 513 | 0.62 | 0 |
| Hu & Soubiran | 2025 | â | â | â | â | -0.160(5) | â | â | â |
| Almeida et al. | 2025 | 1.92 | 1.78 | â | 219 | â | 470 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.278(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.04 | 1.57 | 2.28 | 376 | â | 1172(1) | â | â |
| Cavallo et al. | 2024 | 2.07 | 1.72 | â | 537 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 2.04 | 1.57 | 2.28 | 377 | â | â | â | â |
| Almeida et al. | 2023 | 1.89 | 1.71 | â | 377 | -0.099 | 513(1) | 0.62 | â |
| Deng & Li | 2023 | 1.91 | 1.76 | â | 500 | -0.136 | â | â | â |
| Just et al. | 2023 | â | â | â | 20 | â | 139 | â | â |
| Jadhav & Subramaniam | 2021 | 2.23 | 1.29 | â | 468 | â | 881 | â | 0(1) |
| Dias et al. | 2021 | 1.92 | 1.78 | â | 219 | -0.086 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.23 | 1.29 | â | 468 | â | â | â | â |
| Kounkel et al. | 2020 | 2.25 | 1.80 | â | 263 | â | â | â | â |
| Zhong et al. | 2020 | 2.14(1) | 1.51 | â | 9000 | -0.185 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.14 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1150 | -0.500 | â | â | â |
| Dias et al. | 2019 | 1.86 | 1.51 | â | 37 | -0.881 | â | â | â |
| Soubiran et al. | 2018 | 2.14 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.14 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.84 | â | â | 20 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.84 | 1.77 | â | 20 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.84 | 1.77 | â | 20 | â | â | â | â |
| Camargo et al. | 2012 | 2.75 | 2.18 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 1.84 | 1.77 | â | 20 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.91 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.91 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1287, e_all=0.2437.