FSR 1172
(MWSC 1023)
0.72
UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Stellar density (N50/rad)
5.3 [N/pc2]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1172 is a moderately populated, 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, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 103.905 | -11.028 | 0.406 | -0.453 | -0.288 | 31.564 |
| Almeida et al. | 2025 | 103.919 | -11.033 | â | â | â | â |
| Hunt & Reffert | 2024 | 103.904 | -11.031 | 0.408 | -0.422 | -0.286 | 31.564 |
| Cavallo et al. | 2024 | 103.885 | -11.03 | 0.408 | â | â | â |
| Hunt & Reffert | 2023 | 103.904 | -11.031 | 0.408 | -0.422 | -0.286 | 31.564 |
| Just et al. | 2023 | 103.901 | -11.028 | â | â | â | â |
| Dias et al. | 2021 | 103.919 | -11.033 | 0.373 | -0.539 | -0.217 | â |
| Cantat-Gaudin et al. | 2020 | 103.909 | -11.035 | 0.39 | -0.486 | -0.247 | â |
| Cantat-Gaudin & Anders | 2020 | 103.909 | -11.035 | 0.39 | -0.486 | -0.247 | â |
| Cantat-Gaudin et al. | 2018 | 103.909 | -11.035 | 0.39 | -0.486 | -0.247 | â |
| Kharchenko et al. | 2016 | 103.901 | -11.028 | â | â | â | â |
| Kharchenko et al. | 2013 | 103.908 | -11.03 | â | -0.94 | 3.06 | â |
| Froebrich et al. | 2007 | 103.908 | -11.019 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.37 | 1.94 | 0.58 | 212 | 0.129 | 67 | â | â |
| Almeida et al. | 2025 | 2.09 | 2.02 | â | 149 | â | 62 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 249(1) | â | â |
| Cavallo et al. | 2024 | 2.37 | 1.74 | â | 275 | 0.410 | â | â | â |
| Hunt & Reffert | 2023 | 2.43 | 1.90 | 0.58 | 126 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 631 | â | 67 | â | â |
| Dias et al. | 2021 | 2.09 | 2.02 | â | 149 | -0.153 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.52 | 1.71 | â | 112 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.38 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.38 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.29 | 1.94 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.29 | 1.94 | â | 631 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P308, along with CWNU_1438.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.