FSR 1212
(MWSC 1115)
0.74
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
1.2 [arcmin]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1212 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Very distant
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 106.947 | -14.145 | 0.163 | -0.339 | 0.486 | â |
| Hu & Soubiran | 2025 | 106.943 | -14.143 | â | â | â | â |
| Hunt & Reffert | 2024 | 106.944 | -14.151 | 0.137 | -0.366 | 0.528 | â |
| Cavallo et al. | 2024 | 106.943 | -14.143 | 0.124 | â | â | â |
| Hunt & Reffert | 2023 | 106.944 | -14.151 | 0.137 | -0.366 | 0.528 | â |
| Just et al. | 2023 | 106.904 | -14.148 | â | â | â | â |
| Perren et al. | 2022 | 106.941 | -14.145 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 106.941 | -14.145 | 0.216 | -0.246 | 0.314 | â |
| Cantat-Gaudin & Anders | 2020 | 106.941 | -14.145 | 0.216 | -0.246 | 0.314 | â |
| Cantat-Gaudin et al. | 2018 | 106.941 | -14.145 | 0.216 | -0.246 | 0.314 | â |
| Kharchenko et al. | 2016 | 106.904 | -14.148 | â | â | â | â |
| Kharchenko et al. | 2013 | 106.909 | -14.15 | â | 0.93 | 0.57 | â |
| Froebrich et al. | 2007 | 106.946 | -14.149 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.400* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1056* | â | â |
| Cavallo et al. | 2024 | 7.45 | 1.64 | â | 1514 | -0.110 | â | â | â |
| Hunt & Reffert | 2023 | 6.62 | 1.87 | 2.07 | 929 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 447 | â | 119 | â | â |
| Perren et al. | 2022 | 10.05 | 2.05 | â | 1259 | -0.120 | 5000 | 0.51 | â |
| Cantat-Gaudin et al. | 2020 | 9.68 | 1.54 | â | 1380 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.07 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.07 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.78 | 2.39 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.78 | 2.39 | â | 447 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.