Pismis 5

(MWSC 1516)

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0.92 UTI
0.85
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 40.6 [N/pc2]
  • CN 0.85 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Pismis 5 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption, age, and mass parameters (see Parameters). It is very well-studied in the literature.

Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.

Liu et al. (2025)
Classified as primordial binary cluster 57 along with CWNU_102, and as primordial binary cluster 131 along with DBSB_19, and of multiple system 23 along with OC_0467, DBSB_19 and CWNU_102.

Palma et al. (2025)
Part of multiple system G68, along with CWNU_102, DBSB_19 and OC_0467.

Cavallo et al. (2024)
Gold sample.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 129.409 -39.619 1.055 -5.475 4.255 19.644
Liu et al. 2025 129.41 -39.58 1.07 -5.48 4.27 12.03
Almeida et al. 2025 129.373 -39.645 – – – –
Alfonso et al. 2024 129.397 -39.969 1.029 -5.561 3.981 –
Hunt & Reffert 2024 129.414 -39.584 1.065 -5.476 4.27 12.031
Celli et al. 2024 129.407 -39.603 – – – –
Cavallo et al. 2024 129.396 -39.631 1.065 – – –
Hunt & Reffert 2023 129.414 -39.584 1.065 -5.476 4.27 12.031
Almeida et al. 2023 129.369 -39.646 – – – –
Just et al. 2023 129.41 -39.577 – – – –
He et al. 2022 129.494 -40.213 1.082 -5.555 3.762 –
Richer et al. 2021 129.413 -39.583 1.02 -5.469 4.268 –
Dias et al. 2021 129.373 -39.645 1.038 -5.493 4.267 –
Cantat-Gaudin et al. 2020 129.407 -39.603 1.026 -5.494 4.275 –
SΓ‘nchez et al. 2020 129.408 -39.583 – -5.488 4.154 –
Cantat-Gaudin & Anders 2020 129.407 -39.603 1.026 -5.494 4.275 –
Cantat-Gaudin et al. 2018 129.407 -39.603 1.026 -5.494 4.275 –
Loktin & Popova 2017 129.405 -39.583 – -4.9 2.84 –
Kharchenko et al. 2016 129.41 -39.577 – – – –
Dias et al. 2014 129.408 -39.583 – -4.88 2.9 –
Kharchenko et al. 2013 129.415 -39.58 – -6.96 4.25 –
Bukowiecki et al. 2011 129.417 -39.577 – – – –
van den Bergh 2006 129.408 -39.584 – – – –
Dias et al. 2002 129.408 -39.583 – -4.9 2.84 –
Dambis 1999 129.408 -39.584 – – – –

πŸ’‘ 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 99999– 0.92 1.48 2.1 10 -0.043 228 0.67 –
Liu et al. 2025 1.66 0.58 – 10 – – – –
Almeida et al. 2025 0.92 1.39 – 8 – 180 – –
Alfonso et al. 2024 0.93 1.48 – 10 -0.034 – – –
Hunt & Reffert 2024 – – – – – 298(1) – –
Celli et al. 2024 – – – 10 – 276 – –
Cavallo et al. 2024 0.93 1.76 – 2 -0.290 – – –
Hunt & Reffert 2023 0.91 1.59 2.10 4 – – – –
Almeida et al. 2023 0.91 1.59 – 10 -0.051 332(1) 0.67 –
Just et al. 2023 – – – 20 – 7 – –
He et al. 2022 – 1.35 – 4 – – – –
Richer et al. 2021 – 2.27 – 10 – – – –
Dias et al. 2021 0.92 1.39 – 8 -0.034 – – –
Cantat-Gaudin et al. 2020 0.94 1.48 – 10 – – – –
Cantat-Gaudin & Anders 2020 0.95 – – – – – – –
Cantat-Gaudin et al. 2018 0.95 – – – – – – –
Loktin & Popova 2017 0.87 1.31 – 16 – – – –
Kharchenko et al. 2016 0.70 2.58 – 20 – – – –
Kharchenko et al. 2013 0.70 2.58 – 20 – – – –
Bukowiecki et al. 2012 – – – – – 132 – –
Bukowiecki et al. 2011 1.01(1) 2.14 – 13 – – – –
van den Bergh 2006 0.87 1.30 – 16 – – – –
Dias et al. 2002 0.87 1.31 – 16 – – – –
Dambis 1999 0.89 1.71 – 50 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2221 13.1 129.43 -40.23 1.06 -5.62 3.77 21.57 0.41
OC 0460 6.9 129.4 -39.59 1.07 -5.51 4.31 11.45 0.0

πŸ’‘ Note: The % column shows the percentage of members that Pismis 5 shares with each listed object.

Visualization

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