FSR 0942
(SAI 59; MWSC 729; FoF 681)
0.91
UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
20.3 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0942 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, old 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 91.496 | 13.667 | 0.307 | -0.441 | 0.08 | 31.74 |
| Hu & Soubiran | 2025 | 91.482 | 13.661 | β | β | β | β |
| Zhang et al. | 2024 | 91.506 | 13.67 | β | β | β | β |
| Hunt & Reffert | 2024 | 91.506 | 13.67 | 0.311 | -0.428 | 0.078 | 44.572 |
| Cavallo et al. | 2024 | 91.482 | 13.661 | 0.314 | β | β | β |
| Hunt & Reffert | 2023 | 91.506 | 13.67 | 0.311 | -0.428 | 0.078 | 44.572 |
| Just et al. | 2023 | 91.487 | 13.661 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 91.487 | 13.667 | 0.277 | -0.412 | 0.092 | β |
| SΓ‘nchez et al. | 2020 | 91.496 | 13.664 | β | -0.408 | 0.021 | β |
| Donor et al. | 2020 | 91.496 | 13.66 | β | -0.46 | 0.22 | 29.3 |
| Cantat-Gaudin & Anders | 2020 | 91.487 | 13.667 | 0.277 | -0.412 | 0.092 | β |
| Liu & Pang | 2019 | 91.493 | 13.675 | 0.3 | -0.346 | 0.084 | β |
| Soubiran et al. | 2018 | 91.487 | 13.667 | β | β | β | 31.88 |
| Bica et al. | 2019 | 91.51 | 13.668 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 91.487 | 13.667 | 0.277 | -0.412 | 0.092 | β |
| Loktin & Popova | 2017 | 91.5 | 13.659 | β | -0.434 | -0.506 | β |
| Kharchenko et al. | 2016 | 91.487 | 13.661 | β | β | β | β |
| Dias et al. | 2014 | 91.496 | 13.664 | β | -3.92 | -2.28 | β |
| Kharchenko et al. | 2013 | 91.495 | 13.66 | β | -0.98 | -1.77 | β |
| Glushkova et al. | 2010 | 91.497 | 13.664 | β | β | β | β |
| Froebrich et al. | 2007 | 91.492 | 13.668 | β | β | β | β |
| Dias et al. | 2002 | 91.496 | 13.664 | β | -3.92 | -2.28 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 3.16 | 1.935 | 2.22 | 1000 | -0.255 | 844 | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.230(5) | β | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.379(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1352(1) | β | β |
| Cavallo et al. | 2024 | 3.16 | 2.51 | β | 501 | 0.310 | β | β | β |
| Hunt & Reffert | 2023 | 2.90 | 2.06 | 2.22 | 574 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1000 | β | 337 | β | β |
| Cantat-Gaudin et al. | 2020 | 3.40 | 1.73 | β | 724 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.280 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.27 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 1100 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 3.27 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.27 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.61 | 1.87 | β | 316 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.08 | 2.00 | β | 1000 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.08 | 2.00 | β | 1000 | β | β | β | β |
| Glushkova et al. | 2010 | 2.00 | 1.83 | β | 1000 | β | β | β | β |
| Dias et al. | 2002 | 2.00 | 1.83 | β | 1000 | -0.290 | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.