FSR 0222
(MWSC 3314)
0.53
UTI
0.76
CN
0.54
Cdens
0.75
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
140
Core radius and density
2.2 [pc], 2.7 [pc-2]
- CN 0.76 Rich
- Cdens 0.54 Moderately dense
- CC3 0.75 High quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0222 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by very 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 mass parameters (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.09 kpc) differs significantly from the median photometric distance (~1.24 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 305.037 | 40.796 | 0.323 | -2.248 | -4.846 | -24.381 |
| Hunt & Reffert | 2024 | 305.049 | 40.807 | 0.316 | -2.234 | -4.848 | -24.805 |
| Cavallo et al. | 2024 | 305.004 | 40.784 | 0.313 | â | â | â |
| He et al. | 2023 | 305.045 | 40.8 | 0.304 | -2.248 | -4.837 | -23.2 |
| Hunt & Reffert | 2023 | 305.049 | 40.807 | 0.316 | -2.234 | -4.848 | -24.805 |
| Just et al. | 2023 | 305.027 | 40.83 | â | â | â | â |
| Dib et al. | 2018 | 305.032 | 40.833 | â | â | â | â |
| Joshi et al. | 2016 | 305.032 | 40.833 | â | â | â | â |
| Kharchenko et al. | 2016 | 305.027 | 40.83 | â | â | â | â |
| Kharchenko et al. | 2013 | 305.032 | 40.833 | â | -2.77 | -6.64 | -2.0 |
| Froebrich et al. | 2007 | 305.021 | 40.836 | â | â | â | â |
| Dias et al. | 2002 | 305.021 | 40.836 | â | 2.94 | -5.65 | 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 | 1.24 | 5.26 | 2.79 | 16 | 0.250 | 679 | â | â |
| Hunt & Reffert | 2024 | 2.78 | 5.49 | 2.79 | 1057 | â | 1284(1) | â | â |
| Cavallo et al. | 2024 | 3.60 | 5.14 | â | 562 | 0.250 | â | â | â |
| He et al. | 2023 | 3.55 | 7.25 | â | 158 | â | â | â | â |
| Hunt & Reffert | 2023 | 2.78 | 5.49 | 2.79 | 1057 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 16 | â | 74 | â | â |
| Dib et al. | 2018 | 1.24 | â | â | 16 | â | â | â | â |
| Joshi et al. | 2016 | 1.24 | 5.26 | â | 16 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.24 | 5.26 | â | 16 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.24 | 5.26 | â | 16 | â | â | â | â |
| Dias et al. | 2002 | 1.24 | 5.26 | â | 16 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.06 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.06 (50th percentile).