FSR 1063
(SAI 66; MWSC 917)
0.75
UTI
0.68
CN
0.85
Cdens
0.75
CC3
0.74
Clit
1.0
Cdup
Nm (P>50%)
86
Core radius and density
1.6 [pc], 4.2 [pc-2]
- CN 0.68 Moderately populated
- Cdens 0.85 Dense
- CC3 0.75 High quality
- Clit 0.74 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1063 is a moderately populated, 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 | 99999β | 98.658 | -0.261 | 0.414 | 0.022 | -1.532 | 49.442 |
| Li et al. | 2025 | 98.654 | -0.265 | 0.393 | 0.057 | -1.541 | β |
| Almeida et al. | 2025 | 98.654 | -0.26 | β | β | β | β |
| Zhang et al. | 2024 | 98.655 | -0.267 | β | β | β | β |
| Hunt & Reffert | 2024 | 98.655 | -0.267 | 0.408 | 0.01 | -1.548 | 49.441 |
| Cavallo et al. | 2024 | 98.64 | -0.243 | 0.407 | β | β | β |
| Hunt & Reffert | 2023 | 98.655 | -0.267 | 0.408 | 0.01 | -1.548 | 49.441 |
| Just et al. | 2023 | 98.651 | -0.266 | β | β | β | β |
| Dias et al. | 2021 | 98.654 | -0.26 | 0.387 | 0.033 | -1.522 | β |
| Cantat-Gaudin et al. | 2020 | 98.654 | -0.265 | 0.393 | 0.057 | -1.541 | β |
| SΓ‘nchez et al. | 2020 | 98.658 | -0.267 | β | 0.169 | -1.538 | β |
| Zhong et al. | 2020 | 98.654 | -0.265 | β | 0.057 | -1.541 | 12.663 |
| Cantat-Gaudin & Anders | 2020 | 98.654 | -0.265 | 0.393 | 0.057 | -1.541 | β |
| Bossini et al. | 2019 | 98.654 | -0.265 | β | β | β | β |
| Soubiran et al. | 2018 | 98.654 | -0.265 | β | β | β | 59.76 |
| Bica et al. | 2019 | 98.658 | -0.265 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 98.654 | -0.265 | 0.393 | 0.057 | -1.541 | β |
| Dias et al. | 2018 | β | β | β | 0.78 | -1.35 | β |
| Sampedro et al. | 2017 | 98.658 | -0.267 | β | -1.34 | -2.56 | β |
| Kharchenko et al. | 2016 | 98.651 | -0.266 | β | β | β | β |
| Dias et al. | 2014 | 98.658 | -0.267 | β | -0.66 | -2.36 | β |
| Kharchenko et al. | 2013 | 98.658 | -0.267 | β | 2.96 | 0.15 | β |
| Glushkova et al. | 2010 | 98.658 | -0.267 | β | β | β | β |
| Froebrich et al. | 2007 | 98.654 | -0.265 | β | β | β | β |
| Dias et al. | 2002 | 98.658 | -0.267 | β | -0.66 | -2.36 | β |
π‘ 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 | 99999β | 2.2 | 1.95 | 1.15 | 324 | -0.058 | 247 | β | β |
| Li et al. | 2025 | 2.00 | 2.20 | β | 355 | -0.163 | β | β | β |
| Almeida et al. | 2025 | 1.89 | 2.19 | β | 187 | β | 247 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.496(1) | β | β | β |
| Hunt & Reffert | 2024 | 2.20 | 2.07 | 1.15 | 167 | β | 402(1) | β | β |
| Cavallo et al. | 2024 | 2.37 | 2.21 | β | 214 | 0.460 | β | β | β |
| Hunt & Reffert | 2023 | 2.20 | 2.07 | 1.15 | 167 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 724 | β | 242 | β | β |
| Dias et al. | 2021 | 1.89 | 2.19 | β | 187 | -0.116 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.38 | 1.77 | β | 110 | β | β | β | β |
| Kounkel et al. | 2020 | 2.44 | 2.16 | β | 324 | β | β | β | β |
| Zhong et al. | 2020 | 2.37(1) | 1.80 | β | 8403 | 0.000 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.37 | β | β | β | β | β | β | β |
| Bossini et al. | 2019 | 2.28 | 1.77 | β | 253 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 2.37 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.37 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.03 | 1.58 | β | 724 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.03 | 1.58 | β | 724 | β | β | β | β |
| Glushkova et al. | 2010 | 1.97 | 1.83 | β | 398 | β | β | β | β |
| Dias et al. | 2002 | 2.03 | 1.58 | β | 724 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.225, e_all=0.0465.