FSR 0284
(MWSC 3431)
0.73
UTI
0.58
CN
0.77
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.58 Moderately populated
- Cdens 0.77 Dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0284 is a moderately populated, dense object of high 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, 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.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 314.129 | 49.358 | 0.315 | -2.493 | -3.511 | â |
| Almeida et al. | 2025 | 314.136 | 49.364 | â | â | â | â |
| Hunt & Reffert | 2024 | 314.137 | 49.358 | 0.322 | -2.488 | -3.549 | â |
| Cavallo et al. | 2024 | 314.113 | 49.351 | 0.322 | â | â | â |
| Hunt & Reffert | 2023 | 314.137 | 49.358 | 0.322 | -2.488 | -3.549 | â |
| Just et al. | 2023 | 314.121 | 49.364 | â | â | â | â |
| Dias et al. | 2021 | 314.136 | 49.364 | 0.307 | -2.495 | -3.498 | â |
| Cantat-Gaudin et al. | 2020 | 314.141 | 49.362 | 0.312 | -2.503 | -3.504 | â |
| Cantat-Gaudin & Anders | 2020 | 314.141 | 49.362 | 0.312 | -2.503 | -3.504 | â |
| Cantat-Gaudin et al. | 2018 | 314.141 | 49.362 | 0.312 | -2.503 | -3.504 | â |
| Kharchenko et al. | 2016 | 314.121 | 49.364 | â | â | â | â |
| Dias et al. | 2014 | 314.117 | 49.369 | â | -5.38 | 0.97 | â |
| Kharchenko et al. | 2013 | 314.125 | 49.367 | â | -2.71 | -3.22 | â |
| Froebrich et al. | 2007 | 314.117 | 49.369 | â | â | â | â |
| Dias et al. | 2002 | 314.117 | 49.369 | â | -2.71 | -3.22 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.69 | 2.68 | â | 15 | â | 106 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 577* | â | â |
| Cavallo et al. | 2024 | 2.73 | 3.31 | â | 66 | -0.390 | â | â | â |
| Hunt & Reffert | 2023 | 2.90 | 3.09 | 1.32 | 44 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 596 | â | 104 | â | â |
| Dias et al. | 2021 | 2.69 | 2.68 | â | 15 | 0.002 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.21 | 2.74 | â | 76 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.94 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.94 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.89 | 2.13 | â | 596 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.89 | 2.13 | â | 596 | â | â | â | â |
| Dias et al. | 2002 | 1.89 | 2.13 | â | 596 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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