HSC 1057
0.53
UTI
0.52
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
1.7 [arcmin]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 1057 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a large* distance, above 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 was recently reported in the literature.
(*): The parallax distance estimate (~6.57 kpc) differs significantly from the median photometric distance (~4.71 kpc).
Note: This object shares a large 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 | 30.722 | 64.42 | 0.152 | -0.748 | -0.018 | -63.033 |
| Hu & Soubiran | 2025 | 30.774 | 64.437 | â | â | â | â |
| Hunt & Reffert | 2024 | 30.72 | 64.42 | 0.141 | -0.764 | -0.009 | -63.334 |
| Cavallo et al. | 2024 | 30.774 | 64.437 | 0.148 | â | â | â |
| Hunt & Reffert | 2023 | 30.72 | 64.42 | 0.141 | -0.764 | -0.009 | -63.334 |
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 | -0.160* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 746* | â | â |
| Cavallo et al. | 2024 | 3.96 | 2.33 | â | 661 | -0.800 | â | â | â |
| Hunt & Reffert | 2023 | 5.45 | 2.23 | 1.49 | 329 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.