FSR 1051
(MWSC 1003)
0.76
UTI
0.62
CN
1.0
Cdens
0.5
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
9.1 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1051 is a moderately populated, very dense object of intermediate 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 well-studied in the literature.
(*): The parallax distance estimate (~2.53 kpc) differs significantly from the median photometric distance (~1.89 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 103.046 | 3.657 | 0.395 | -0.781 | -2.641 | 36.992 |
| Almeida et al. | 2025 | 103.043 | 3.664 | â | â | â | â |
| Zhang et al. | 2024 | 103.048 | 3.653 | â | â | â | â |
| Hunt & Reffert | 2024 | 103.048 | 3.653 | 0.384 | -0.772 | -2.632 | 36.989 |
| Cavallo et al. | 2024 | 103.043 | 3.64 | 0.384 | â | â | â |
| Hunt & Reffert | 2023 | 103.048 | 3.653 | 0.384 | -0.772 | -2.632 | 36.989 |
| Just et al. | 2023 | 103.028 | 3.657 | â | â | â | â |
| Dias et al. | 2021 | 103.043 | 3.664 | 0.406 | -0.765 | -2.655 | â |
| Cantat-Gaudin et al. | 2020 | 103.046 | 3.662 | 0.399 | -0.761 | -2.639 | â |
| Zhong et al. | 2020 | 103.046 | 3.662 | â | -0.761 | -2.639 | 41.86 |
| Cantat-Gaudin & Anders | 2020 | 103.046 | 3.662 | 0.399 | -0.761 | -2.639 | â |
| Soubiran et al. | 2018 | 103.046 | 3.662 | â | â | â | 37.17 |
| Bica et al. | 2019 | 103.061 | 3.644 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 103.046 | 3.662 | 0.399 | -0.761 | -2.639 | â |
| Kharchenko et al. | 2016 | 103.028 | 3.657 | â | â | â | â |
| Kharchenko et al. | 2013 | 103.035 | 3.655 | â | 0.13 | -1.92 | â |
| Froebrich et al. | 2007 | 103.054 | 3.642 | â | â | â | â |
| Dias et al. | 2002 | 103.054 | 3.642 | â | 0.13 | -1.92 | 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 | 1.89 | 1.44 | 2.08 | 537 | -0.066 | 162 | â | â |
| Almeida et al. | 2025 | 1.89 | 1.70 | â | 432 | â | 162 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.043(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 312(1) | â | â |
| Cavallo et al. | 2024 | 1.80 | 1.88 | â | 457 | -0.350 | â | â | â |
| Hunt & Reffert | 2023 | 2.29 | 1.84 | 2.08 | 327 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 617 | â | 83 | â | â |
| Dias et al. | 2021 | 1.89 | 1.70 | â | 432 | -0.089 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.48 | 1.44 | â | 257 | â | â | â | â |
| Zhong et al. | 2020 | 1.18 | 1.35 | â | 8790 | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.33 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.33 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.33 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.18 | 1.35 | â | 617 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.18 | 1.35 | â | 617 | â | â | â | â |
| Dias et al. | 2002 | 1.18 | 1.35 | â | 617 | 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)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.