FSR 1443
0.31
UTI
0.0
CN
0.11
Cdens
0.25
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.11 Very loose
- CC3 0.25 Low quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1443 is a sparse, very loose object of low 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 metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 129.85 | -47.357 | 0.249 | -3.514 | 4.311 | â |
| Hu & Soubiran | 2025 | 129.841 | -47.348 | â | â | â | â |
| Almeida et al. | 2025 | 129.857 | -47.356 | â | â | â | â |
| Hunt & Reffert | 2024 | 129.853 | -47.353 | 0.286 | -3.474 | 4.465 | 36.624 |
| Cavallo et al. | 2024 | 129.841 | -47.348 | 0.288 | â | â | â |
| Hunt & Reffert | 2023 | 129.853 | -47.353 | 0.286 | -3.474 | 4.465 | 36.624 |
| Almeida et al. | 2023 | 129.858 | -47.355 | â | â | â | â |
| Dias et al. | 2021 | 129.857 | -47.356 | 0.221 | -3.562 | 4.144 | 37.746 |
| Dias et al. | 2014 | 129.858 | -47.357 | â | -2.1 | 2.55 | â |
| Froebrich et al. | 2007 | 129.858 | -47.357 | â | â | â | â |
| Dias et al. | 2002 | 129.858 | -47.357 | â | -4.12 | 8.37 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.220* | â | â | â |
| Almeida et al. | 2025 | 3.30 | 1.82 | â | 505 | â | 583 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 340* | â | â |
| Cavallo et al. | 2024 | 3.42 | 1.10 | â | 708 | 0.940 | â | â | â |
| Hunt & Reffert | 2023 | 3.05 | 1.46 | 1.58 | 484 | â | â | â | â |
| Almeida et al. | 2023 | 3.00 | 1.80 | â | 420 | -0.120 | 192* | 0.70 | â |
| Dias et al. | 2021 | 3.30 | 1.82 | â | 505 | -0.019 | â | â | â |
| Dias et al. | 2002 | 1.86 | 1.42 | â | 589 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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