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
C3 classification AB
Number of members (P>50%) 360
Radius (P>50% members) 10.8 [arcmin]
  • CN 0.85 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
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 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.

Close Moderate extinction Near-solar metallicity Very young

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

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for Pismis 5 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 129.409 -39.619 1.055 -5.475 4.255 19.644
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 –
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 –
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] Bfr BSS
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* – –
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* 0.67 –
Just et al. 2023 – – – 20 – 7 – –
He et al. 2022 – 1.35 – 4 – – – –
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 – – – –
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 – – – –

(*): Indicates that this parameter is assigned more than one value 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
ℹ️
Pismis 5 UCC
Pismis 5 HUNT23
Pismis 5 CANTAT20
Galactocentric position diagram