Alessi 94
(UBC 2)
0.63
UTI
0.57
CN
0.34
Cdens
1.0
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
1.7 [N/pc2]
- CN 0.57 Moderately populated
- Cdens 0.34 Loose
- CC3 1.0 Very high quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
Alessi 94 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 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 | 5.376 | 46.544 | 1.782 | -6.411 | -5.094 | -15.837 |
| Li et al. | 2025 | 5.584 | 46.532 | 1.754 | -6.374 | -5.022 | â |
| Wei et al. | 2025 | 5.343 | 46.839 | 1.757 | -2.053 | -5.016 | â |
| Alfonso et al. | 2024 | 6.015 | 46.524 | 1.757 | -6.407 | -5.034 | â |
| Zhang et al. | 2024 | 5.269 | 46.531 | â | â | â | â |
| Cavallo et al. | 2024 | 6.036 | 46.576 | 1.781 | â | â | â |
| Hunt & Reffert | 2023 | 5.269 | 46.531 | 1.781 | -6.365 | -5.083 | -16.817 |
| Tarricq et al. | 2022 | 5.095 | 46.652 | 1.793 | -6.407 | -5.071 | â |
| Cantat-Gaudin et al. | 2020 | 5.584 | 46.532 | 1.754 | -6.374 | -5.022 | â |
| Cantat-Gaudin & Anders | 2020 | 5.584 | 46.532 | 1.754 | -6.374 | -5.022 | â |
| Bica et al. | 2019 | 5.796 | 46.605 | â | â | â | â |
| Castro-Ginard et al. | 2018 | 5.802 | 46.604 | 1.745 | -6.34 | -5.003 | -9.73 |
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 | 0.555 | 0.18 | 0.57 | 209 | 0.077 | 86 | 0.39 | â |
| Li et al. | 2025 | 0.56 | 0.16 | â | 594 | 0.077 | â | â | â |
| Wei et al. | 2025 | 0.65 | 0.43 | â | 275 | 0.250 | 86 | 0.39 | â |
| Alfonso et al. | 2024 | 0.55 | 0.18 | â | 578 | -0.049 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.063(1) | â | â | â |
| Cavallo et al. | 2024 | 0.56 | 0.26 | â | 178 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 0.53 | 0.12 | 0.57 | 184 | â | â | â | â |
| Tarricq et al. | 2022 | 0.55 | â | â | 209 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.55 | 0.18 | â | 200 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.56 | â | â | â | 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)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.