FSR 0931
(MWSC 796)
0.51
UTI
0.76
CN
0.47
Cdens
0.75
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
134
Core radius and density
2.5 [pc], 2.3 [pc-2]
- CN 0.76 Rich
- Cdens 0.47 Loose
- CC3 0.75 High quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0931 is a rich, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 93.349 | 15.938 | 0.577 | -0.489 | -0.981 | â |
| Zhang et al. | 2024 | 93.379 | 15.94 | â | â | â | â |
| Hunt & Reffert | 2024 | 93.379 | 15.94 | 0.58 | -0.504 | -0.978 | â |
| Cavallo et al. | 2024 | 93.332 | 15.936 | 0.58 | â | â | â |
| Hunt & Reffert | 2023 | 93.379 | 15.94 | 0.58 | -0.504 | -0.978 | â |
| Just et al. | 2023 | 93.245 | 15.931 | â | â | â | â |
| Bica et al. | 2019 | 93.282 | 15.946 | â | â | â | â |
| Dib et al. | 2018 | 93.252 | 15.93 | â | â | â | â |
| Joshi et al. | 2016 | 93.252 | 15.93 | â | â | â | â |
| Kharchenko et al. | 2016 | 93.245 | 15.931 | â | â | â | â |
| Kharchenko et al. | 2013 | 93.252 | 15.93 | â | 0.8 | -5.3 | â |
| Froebrich et al. | 2007 | 93.279 | 15.944 | 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 | 1.66 | 1.84 | 1.89 | 25 | 0.021 | 318 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.198(1) | â | â | â |
| Hunt & Reffert | 2024 | 1.62 | 1.43 | 1.89 | 73 | â | 509(1) | â | â |
| Cavallo et al. | 2024 | 1.78 | 1.71 | â | 85 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 1.62 | 1.43 | 1.89 | 73 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 25 | â | 127 | â | â |
| Dib et al. | 2018 | 1.66 | â | â | 25 | â | â | â | â |
| Joshi et al. | 2016 | 1.66 | 1.97 | â | 25 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.66 | 1.97 | â | 25 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.66 | 1.97 | â | 25 | 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 P117, along with FSR_0923.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.60 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.60 (50th percentile).