FSR 0158
(SAI 130; MWSC 3182)
0.90
UTI
0.84
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
14.0 [N/pc2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0158 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is 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 | 296.995 | 26.032 | 0.178 | -2.773 | -5.447 | 6.369 |
| Almeida et al. | 2025 | 296.99 | 26.039 | â | â | â | â |
| Hunt & Reffert | 2024 | 296.989 | 26.041 | 0.186 | -2.789 | -5.458 | 13.715 |
| Celli et al. | 2024 | 296.99 | 26.04 | â | â | â | â |
| Cavallo et al. | 2024 | 296.999 | 26.01 | 0.184 | â | â | â |
| Hunt & Reffert | 2023 | 296.989 | 26.041 | 0.186 | -2.789 | -5.458 | 13.715 |
| Just et al. | 2023 | 297.009 | 26.038 | â | â | â | â |
| Dias et al. | 2021 | 296.99 | 26.039 | 0.131 | -2.737 | -5.407 | â |
| Cantat-Gaudin et al. | 2020 | 296.99 | 26.04 | 0.139 | -2.748 | -5.432 | â |
| Cantat-Gaudin & Anders | 2020 | 296.99 | 26.04 | 0.139 | -2.748 | -5.432 | â |
| Soubiran et al. | 2018 | 296.99 | 26.04 | â | â | â | 5.37 |
| Bica et al. | 2019 | 296.988 | 26.029 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 296.99 | 26.04 | 0.139 | -2.748 | -5.432 | â |
| Kharchenko et al. | 2016 | 297.009 | 26.038 | â | â | â | â |
| Kharchenko et al. | 2013 | 297.015 | 26.04 | â | -3.37 | -4.79 | â |
| Glushkova et al. | 2010 | 296.992 | 26.032 | â | â | â | â |
| Froebrich et al. | 2007 | 296.996 | 26.032 | â | â | â | â |
| Dias et al. | 2002 | 296.996 | 26.032 | â | 0.58 | -6.26 | 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 | 4.505 | 3.97 | 3.1 | 77 | 0.011 | 336 | â | â |
| Almeida et al. | 2025 | 3.73 | 3.97 | â | 77 | â | 476 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 5684(1) | â | â |
| Celli et al. | 2024 | â | â | â | 10 | â | 150 | â | â |
| Cavallo et al. | 2024 | 6.25 | 4.68 | â | 21 | 0.000 | â | â | â |
| Hunt & Reffert | 2023 | 5.28 | 5.12 | 3.10 | 48 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 320 | â | 195 | â | â |
| Dias et al. | 2021 | 3.73 | 3.97 | â | 77 | 0.021 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 6.14 | 4.39 | â | 10 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.96 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.96 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.96 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.77 | 3.74 | â | 320 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.77 | 3.74 | â | 320 | â | â | â | â |
| Glushkova et al. | 2010 | 3.60 | 3.63 | â | 200 | â | â | â | â |
| Dias et al. | 2002 | 2.77 | 3.74 | â | 320 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.
Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.