Pozzo 1

(FoF 2394)

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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

â„šī¸
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

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

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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 –
Wei et al. 2025 122.367 -47.364 2.916 -6.48 9.724 –
Almeida et al. 2025 122.331 -47.301 – – – –
Alfonso et al. 2024 122.315 -47.379 2.796 -6.298 9.359 –
Hunt & Reffert 2024 122.375 -47.354 2.847 -6.364 9.437 14.001
Celli et al. 2024 122.374 -47.335 – – – –
Cavallo et al. 2024 122.33 -47.389 2.845 – – –
Hunt & Reffert 2023 122.375 -47.354 2.847 -6.364 9.437 14.001
Almeida et al. 2023 122.344 -47.315 – – – –
Cordoni et al. 2023 122.331 -47.301 2.855 -6.475 9.587 –
He et al. 2022 122.494 -46.623 2.847 -6.549 9.497 –
Rain et al. 2021 122.374 -47.335 2.853 -6.516 9.53 –
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 –
Cantat-Gaudin & Anders 2020 122.374 -47.335 2.853 -6.516 9.53 –
Liu & Pang 2019 122.246 -47.391 2.778 -6.331 9.279 –
Dias et al. 2019 122.375 -47.335 2.853 -6.516 9.53 19.189
Monteiro & Dias 2019 122.374 -47.335 – -6.544 9.568 2.062
Bossini et al. 2019 122.374 -47.335 – – – –
Soubiran et al. 2018 122.374 -47.335 – – – 18.67
Cantat-Gaudin et al. 2018 122.374 -47.335 2.853 -6.516 9.53 –
Dias et al. 2014 122.383 -47.337 – -2.14 3.77 –

💡 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 – 13 -0.144 – – –
Wei et al. 2025 0.25 1.16 – 7 0.500 575 0.49 –
Almeida et al. 2025 0.34 0.16 – 12 – 350 – –
Alfonso et al. 2024 0.33 0.07 – 12 -0.069 – – –
Hunt & Reffert 2024 – – – – – 138* – –
Celli et al. 2024 – – – 10 – 343 – –
Cavallo et al. 2024 0.35 0.70 – 5 -0.210 – – –
Hunt & Reffert 2023 0.35 0.35 0.98 9 – – – –
Almeida et al. 2023 0.34 0.27 – 13 -0.042 610* 0.23 –
Cordoni et al. 2023 0.34 0.16 – 12 -0.069 754 0.21 0.00
He et al. 2022 – 0.20 – 11 – – – –
Rain et al. 2021 0.35 0.22 – 14 – – – 0
Dias et al. 2021 0.34 0.16 – 12 -0.069 – – –
Cantat-Gaudin et al. 2020 0.33 0.07 – 10 – – – –
Cantat-Gaudin & Anders 2020 0.35 – – – – – – –
Liu & Pang 2019 – – – 7 0.500 – – –
Dias et al. 2019 0.34 0.25 – 12 -0.323 – – –
Monteiro & Dias 2019 0.35 0.24 – 14 0.037 – – –
Bossini et al. 2019 0.32 0.16 – 13 0.000 – – –
Soubiran et al. 2018 0.35 – – – – – – –
Cantat-Gaudin et al. 2018 0.35 – – – – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 254 100.0 122.38 -47.34 2.89 -6.4 9.6 14.61 0.07
CWWDL 14592 4.4 123.01 -46.3 2.79 -6.35 9.19 15.12 0.16
CWWDL 14595 4.4 122.36 -46.77 2.73 -6.23 9.01 16.28 0.1
OC 0478 4.4 122.65 -47.46 2.98 -6.75 9.8 14.78 0.0
CWWDL 14586 4.0 121.61 -48.0 2.74 -6.0 9.04 18.68 0.26
CWWDL 14593 2.1 123.1 -46.18 2.87 -6.51 9.41 15.29 0.11

💡 Note: The % column shows the percentage of members that Pozzo 1 shares with each listed object.

Visualization

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