Pozzo 1
(FoF 2394)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
28.9 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Pozzo 1 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a large percentage of members with 6 later reported entries. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 122.385 | -47.332 | 2.888 | -6.407 | 9.606 | 15.219 |
| Li et al. | 2025 | 122.374 | -47.335 | 2.853 | -6.516 | 9.53 | â |
| Wei et al. | 2025 | 122.367 | -47.364 | 2.916 | -6.48 | 9.724 | â |
| Almeida et al. | 2025 | 122.331 | -47.301 | â | â | â | â |
| Alfonso et al. | 2024 | 122.315 | -47.379 | 2.796 | -6.298 | 9.359 | â |
| Hunt & Reffert | 2024 | 122.375 | -47.354 | 2.847 | -6.364 | 9.437 | 14.001 |
| Celli et al. | 2024 | 122.374 | -47.335 | â | â | â | â |
| Cavallo et al. | 2024 | 122.33 | -47.389 | 2.845 | â | â | â |
| Hunt & Reffert | 2023 | 122.375 | -47.354 | 2.847 | -6.364 | 9.437 | 14.001 |
| Almeida et al. | 2023 | 122.344 | -47.315 | â | â | â | â |
| Cordoni et al. | 2023 | 122.331 | -47.301 | 2.855 | -6.475 | 9.587 | â |
| He et al. | 2022 | 122.494 | -46.623 | 2.847 | -6.549 | 9.497 | â |
| Rain et al. | 2021 | 122.374 | -47.335 | 2.853 | -6.516 | 9.53 | â |
| Dias et al. | 2021 | 122.331 | -47.301 | 2.855 | -6.475 | 9.587 | 18.69 |
| Cantat-Gaudin et al. | 2020 | 122.374 | -47.335 | 2.853 | -6.516 | 9.53 | â |
| Cantat-Gaudin & Anders | 2020 | 122.374 | -47.335 | 2.853 | -6.516 | 9.53 | â |
| Liu & Pang | 2019 | 122.246 | -47.391 | 2.778 | -6.331 | 9.279 | â |
| Dias et al. | 2019 | 122.375 | -47.335 | 2.853 | -6.516 | 9.53 | 19.189 |
| Monteiro & Dias | 2019 | 122.374 | -47.335 | â | -6.544 | 9.568 | 2.062 |
| Bossini et al. | 2019 | 122.374 | -47.335 | â | â | â | â |
| Soubiran et al. | 2018 | 122.374 | -47.335 | â | â | â | 18.67 |
| Cantat-Gaudin et al. | 2018 | 122.374 | -47.335 | 2.853 | -6.516 | 9.53 | â |
| Dias et al. | 2014 | 122.383 | -47.337 | â | -2.14 | 3.77 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.31 | 0.20 | â | 13 | -0.144 | â | â | â |
| Wei et al. | 2025 | 0.25 | 1.16 | â | 7 | 0.500 | 575 | 0.49 | â |
| Almeida et al. | 2025 | 0.34 | 0.16 | â | 12 | â | 350 | â | â |
| Alfonso et al. | 2024 | 0.33 | 0.07 | â | 12 | -0.069 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 138* | â | â |
| Celli et al. | 2024 | â | â | â | 10 | â | 343 | â | â |
| Cavallo et al. | 2024 | 0.35 | 0.70 | â | 5 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.35 | 0.35 | 0.98 | 9 | â | â | â | â |
| Almeida et al. | 2023 | 0.34 | 0.27 | â | 13 | -0.042 | 610* | 0.23 | â |
| Cordoni et al. | 2023 | 0.34 | 0.16 | â | 12 | -0.069 | 754 | 0.21 | 0.00 |
| He et al. | 2022 | â | 0.20 | â | 11 | â | â | â | â |
| Rain et al. | 2021 | 0.35 | 0.22 | â | 14 | â | â | â | 0 |
| Dias et al. | 2021 | 0.34 | 0.16 | â | 12 | -0.069 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.33 | 0.07 | â | 10 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.35 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 7 | 0.500 | â | â | â |
| Dias et al. | 2019 | 0.34 | 0.25 | â | 12 | -0.323 | â | â | â |
| Monteiro & Dias | 2019 | 0.35 | 0.24 | â | 14 | 0.037 | â | â | â |
| Bossini et al. | 2019 | 0.32 | 0.16 | â | 13 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.35 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.35 | â | â | â | 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: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.