FSR 0224
(MWSC 3335)
0.66
UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
3.2 [arcmin]
- CN 0.26 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0224 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
High extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 306.341 | 40.207 | 0.573 | -3.167 | -4.33 | 61.526 |
| Almeida et al. | 2025 | 306.351 | 40.224 | â | â | â | â |
| Hunt & Reffert | 2024 | 306.339 | 40.22 | 0.574 | -3.162 | -4.327 | 19.226 |
| Cavallo et al. | 2024 | 306.33 | 40.198 | 0.58 | â | â | â |
| Hunt & Reffert | 2023 | 306.339 | 40.22 | 0.574 | -3.162 | -4.327 | 19.226 |
| Almeida et al. | 2023 | 306.352 | 40.225 | â | â | â | â |
| Just et al. | 2023 | 306.34 | 40.223 | â | â | â | â |
| Dias et al. | 2021 | 306.351 | 40.224 | 0.566 | -3.242 | -4.373 | â |
| Kharchenko et al. | 2016 | 306.34 | 40.223 | â | â | â | â |
| Kharchenko et al. | 2013 | 306.345 | 40.226 | â | -5.25 | -7.05 | â |
| Froebrich et al. | 2007 | 306.337 | 40.227 | â | â | â | â |
| Dias et al. | 2002 | 306.337 | 40.227 | â | -5.25 | -7.05 | 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 | 1.71 | 3.06 | â | 5 | â | 152 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 292* | â | â |
| Cavallo et al. | 2024 | 1.64 | 3.13 | â | 11 | 1.050 | â | â | â |
| Hunt & Reffert | 2023 | 1.68 | 3.51 | 2.42 | 4 | â | â | â | â |
| Almeida et al. | 2023 | 1.65 | 3.28 | â | 5 | 0.040 | 177* | 0.77 | â |
| Just et al. | 2023 | â | â | â | 1012 | â | 60 | â | â |
| Dias et al. | 2021 | 1.71 | 3.06 | â | 5 | 0.242 | â | â | â |
| Kharchenko et al. | 2016 | 1.43 | 2.19 | â | 1012 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.43 | 2.19 | â | 1012 | â | â | â | â |
| Dias et al. | 2002 | 1.43 | 2.19 | â | 1012 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Silver sample.