FSR 0953
(MWSC 835; FoF 926)
0.91
UTI
0.78
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- 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
FSR 0953 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 and mass parameters (see Parameters). It is very 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 | β | 94.767 | 14.15 | 0.348 | -0.122 | -2.856 | 20.551 |
| Li et al. | 2025 | 94.762 | 14.15 | 0.331 | -0.134 | -2.877 | β |
| Almeida et al. | 2025 | 94.768 | 14.145 | β | β | β | β |
| Zhang et al. | 2024 | 94.759 | 14.146 | β | β | β | β |
| Hunt & Reffert | 2024 | 94.759 | 14.146 | 0.346 | -0.113 | -2.855 | 20.666 |
| Cavallo et al. | 2024 | 94.766 | 14.145 | 0.346 | β | β | β |
| Hunt & Reffert | 2023 | 94.759 | 14.146 | 0.346 | -0.113 | -2.855 | 20.666 |
| Just et al. | 2023 | 94.751 | 14.131 | β | β | β | β |
| Dias et al. | 2021 | 94.768 | 14.145 | 0.333 | -0.142 | -2.892 | β |
| Cantat-Gaudin et al. | 2020 | 94.762 | 14.15 | 0.331 | -0.134 | -2.877 | β |
| SΓ‘nchez et al. | 2020 | 94.758 | 14.148 | β | 0.059 | -2.542 | β |
| Cantat-Gaudin & Anders | 2020 | 94.762 | 14.15 | 0.331 | -0.134 | -2.877 | β |
| Liu & Pang | 2019 | 94.762 | 14.163 | 0.322 | -0.146 | -2.844 | β |
| Soubiran et al. | 2018 | 94.762 | 14.15 | β | β | β | 14.02 |
| Bica et al. | 2019 | 94.76 | 14.149 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 94.762 | 14.15 | 0.331 | -0.134 | -2.877 | β |
| Kharchenko et al. | 2016 | 94.751 | 14.131 | β | β | β | β |
| Dias et al. | 2014 | 94.758 | 14.148 | β | 0.54 | -0.64 | β |
| Kharchenko et al. | 2013 | 94.759 | 14.13 | β | -0.21 | 2.92 | β |
| Froebrich et al. | 2007 | 94.758 | 14.148 | β | β | β | β |
| Dias et al. | 2002 | 94.758 | 14.148 | β | 0.54 | -0.64 | β |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.72 | 2.11 | β | 507 | 0.133 | β | β | β |
| Almeida et al. | 2025 | 2.29 | 2.10 | β | 512 | β | 564 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.368* | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 836* | β | β |
| Cavallo et al. | 2024 | 2.75 | 2.26 | β | 389 | 0.210 | β | β | β |
| Hunt & Reffert | 2023 | 2.66 | 1.91 | 1.25 | 530 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 562 | β | 17 | β | β |
| Dias et al. | 2021 | 2.29 | 2.10 | β | 512 | -0.121 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.57 | 1.48 | β | 646 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.78 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 676 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 2.78 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.78 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.73 | 1.49 | β | 562 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.73 | 1.49 | β | 562 | β | β | β | β |
| Dias et al. | 2002 | 1.73 | 1.49 | β | 562 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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