FSR 0977
(MWSC 895; Riddle 1; Teutsch J0631.9+1151)
0.90
UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
14.1 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0977 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 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 | 99999â | 97.977 | 11.873 | 0.439 | 0.704 | -1.542 | 24.799 |
| Li et al. | 2025 | 97.974 | 11.865 | 0.453 | 0.721 | -1.533 | â |
| Hu & Soubiran | 2025 | 97.985 | 11.859 | â | â | â | â |
| Almeida et al. | 2025 | 97.975 | 11.857 | â | â | â | â |
| Zhang et al. | 2024 | 97.968 | 11.868 | â | â | â | â |
| Hunt & Reffert | 2024 | 97.968 | 11.868 | 0.448 | 0.684 | -1.546 | 23.756 |
| Cavallo et al. | 2024 | 97.985 | 11.859 | 0.446 | â | â | â |
| Hunt & Reffert | 2023 | 97.968 | 11.868 | 0.448 | 0.684 | -1.546 | 23.756 |
| Almeida et al. | 2023 | 97.974 | 11.861 | â | â | â | â |
| Just et al. | 2023 | 97.957 | 11.847 | â | â | â | â |
| Dias et al. | 2021 | 97.975 | 11.857 | 0.44 | 0.7 | -1.528 | 23.464 |
| Cantat-Gaudin et al. | 2020 | 97.974 | 11.865 | 0.453 | 0.721 | -1.533 | â |
| Cantat-Gaudin & Anders | 2020 | 97.974 | 11.865 | 0.453 | 0.721 | -1.533 | â |
| Soubiran et al. | 2018 | 97.974 | 11.865 | â | â | â | 23.72 |
| Bica et al. | 2019 | 97.972 | 11.844 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 97.974 | 11.865 | 0.453 | 0.721 | -1.533 | â |
| Kharchenko et al. | 2016 | 97.957 | 11.847 | â | â | â | â |
| Dias et al. | 2014 | 97.963 | 11.844 | â | -1.11 | 2.18 | â |
| Kharchenko et al. | 2013 | 97.965 | 11.845 | â | 3.15 | 0.25 | â |
| Froebrich et al. | 2007 | 97.963 | 11.844 | â | â | â | â |
| Dias et al. | 2002 | 97.963 | 11.844 | â | 3.15 | 0.25 | 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 | 1.92 | 1.595 | 2.38 | 661 | -0.149 | 148 | 0.81 | â |
| Li et al. | 2025 | 1.77 | 1.37 | â | 952 | -0.176 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.140(5) | â | â | â |
| Almeida et al. | 2025 | 1.78 | 1.50 | â | 920 | â | 91 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.189(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 382(1) | â | â |
| Cavallo et al. | 2024 | 2.14 | 1.69 | â | 661 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 2.00 | 1.60 | 2.38 | 618 | â | â | â | â |
| Almeida et al. | 2023 | 1.78 | 1.59 | â | 851 | -0.147 | 200(1) | 0.81 | â |
| Just et al. | 2023 | â | â | â | 479 | â | 96 | â | â |
| Dias et al. | 2021 | 1.78 | 1.50 | â | 920 | -0.151 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.19 | 1.00 | â | 851 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.07 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.07 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.07 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.92 | 1.81 | â | 479 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.92 | 1.81 | â | 479 | â | â | â | â |
| Dias et al. | 2002 | 1.92 | 1.81 | â | 479 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.