FSR 0902
(MWSC 832)
0.70
UTI
0.67
CN
1.0
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Stellar density (N50/rad)
8.5 [N/pc2]
- CN 0.67 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0902 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~1.96 kpc) differs significantly from the median photometric distance (~1.24 kpc).
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 94.578 | 20.549 | 0.509 | 0.45 | -2.649 | 18.882 |
| Zhang et al. | 2024 | 94.578 | 20.562 | â | â | â | â |
| Hunt & Reffert | 2024 | 94.578 | 20.562 | 0.513 | 0.443 | -2.625 | 8.103 |
| Cavallo et al. | 2024 | 94.617 | 20.556 | 0.514 | â | â | â |
| Hunt & Reffert | 2023 | 94.578 | 20.562 | 0.513 | 0.443 | -2.625 | 8.103 |
| Just et al. | 2023 | 94.567 | 20.542 | â | â | â | â |
| Bica et al. | 2019 | 94.586 | 20.528 | â | â | â | â |
| Kharchenko et al. | 2016 | 94.567 | 20.542 | â | â | â | â |
| Kharchenko et al. | 2013 | 94.575 | 20.54 | â | -0.51 | -5.5 | â |
| Froebrich et al. | 2007 | 94.579 | 20.528 | â | â | â | â |
| Dias et al. | 2002 | 94.579 | 20.528 | â | 2.28 | -5.23 | 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 | 1.23 | 1.54 | 14 | -0.131 | 216 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.182(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 346(1) | â | â |
| Cavallo et al. | 2024 | 1.62 | 1.43 | â | 11 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 1.81 | 1.31 | 1.54 | 5 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 14 | â | 86 | â | â |
| Kharchenko et al. | 2016 | 1.24 | 1.23 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.24 | 1.23 | â | 14 | â | â | â | â |
| Dias et al. | 2002 | 1.24 | 1.23 | â | 14 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G118, along with HSC_1504, NGC_2175, Pismis_27 and UBC_1303.
Cavallo et al. (2024)
Gold sample.