NGC 3572

(MWSC 1906)

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0.95 UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members) 122
Radius (P>50% members) 3.7 [arcmin]
C3 classification AA
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
NGC 3572 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is very well-studied in the literature.

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for NGC 3572 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 167.655 -60.311 0.381 -6.245 1.904 -4.918
Almeida et al. 2025 167.633 -60.302 – – – –
Hunt & Reffert 2024 167.625 -60.28 0.373 -6.253 1.949 -4.931
Celli et al. 2024 167.64 -60.294 – – – –
Cavallo et al. 2024 167.639 -60.302 0.371 – – –
Hunt & Reffert 2023 167.625 -60.28 0.373 -6.253 1.949 -4.931
Just et al. 2023 167.596 -60.246 – – – –
Jaehnig et al. 2021 167.646 -60.293 0.409 -6.204 1.921 –
Rain et al. 2021 167.64 -60.294 0.376 -6.261 1.893 –
Dias et al. 2021 167.633 -60.302 0.383 -6.266 1.904 –
Cantat-Gaudin et al. 2020 167.64 -60.294 0.376 -6.261 1.893 –
Cantat-Gaudin & Anders 2020 167.64 -60.294 0.376 -6.261 1.893 –
Soubiran et al. 2018 167.64 -60.294 – – – 0.92
Cantat-Gaudin et al. 2018 167.64 -60.294 0.376 -6.261 1.893 –
Loktin & Popova 2017 167.595 -60.248 – -4.37 -0.96 -8.0
Kharchenko et al. 2016 167.596 -60.246 – – – –
Dias et al. 2014 167.596 -60.248 – -4.3 -0.88 –
Kharchenko et al. 2013 167.602 -60.25 – -9.19 2.31 -8.0
Gozha et al. 2012 167.596 -60.248 – – – –
Piskunov et al. 2008 167.612 -60.243 – – – –
Kharchenko et al. 2007 167.59 -60.25 – 0.11 – -8.47
van den Bergh 2006 167.6 -60.25 – – – –
Kharchenko et al. 2005 167.61 -60.25 – -10.55 1.25 -9.5
Kharchenko et al. 2003 167.61 -60.25 – -9.7 -1.02 –
Dias et al. 2002 167.596 -60.248 – -4.37 -0.96 -4.0
Dambis 1999 167.596 -60.248 – – – –

💡 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– 2.26 1.21 1.5 8 -0.054 502 – 0.0
Almeida et al. 2025 2.28 1.44 – 6 – 659 – –
Hunt & Reffert 2024 – – – – – 502(1) – –
Celli et al. 2024 – – – 5 – 543 – –
Cavallo et al. 2024 2.24 1.42 – 4 -0.180 – – –
Hunt & Reffert 2023 2.42 1.29 1.50 5 – – – –
Just et al. 2023 – – – 8 – 162 – –
Jaehnig et al. 2021 2.46(1) – – – – – – –
Rain et al. 2021 2.47 1.18 – 8 – – – 0
Dias et al. 2021 2.28 1.44 – 6 0.071 – – –
Cantat-Gaudin et al. 2020 2.45 1.53 – 5 – – – –
Cantat-Gaudin & Anders 2020 2.47 – – – – – – –
Soubiran et al. 2018 2.47 – – – – – – –
Cantat-Gaudin et al. 2018 2.47 – – – – – – –
Loktin & Popova 2017 2.00 1.20 – 8 – – – –
Kharchenko et al. 2016 2.00 1.13 – 8 – – – –
Kharchenko et al. 2013 2.00 1.13 – 8 – – – –
Gozha et al. 2012 2.00 – – 8 – 427 – –
Piskunov et al. 2008 2.00 1.05 – 8 – – – –
van den Bergh 2006 2.00 1.21 – 8 – – – –
Kharchenko et al. 2005 2.00 1.05 – 8 – – – –
Kharchenko et al. 2003 2.00 1.15 – – – – – –
Dias et al. 2002 2.00 1.21 – 8 – – – –
Dambis 1999 2.40 1.36 – 3 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 227 16.4 167.49 -60.31 0.37 -6.22 1.85 -28.47 0.15
Hogg 10 14.8 167.68 -60.41 0.39 -6.2 1.79 -10.87 0.82

💡 Note: The % column shows the percentage of members that NGC 3572 shares with each listed object.

Visualization
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NGC 3572 UCC
NGC 3572 HUNT23
NGC 3572 CANTAT20
Galactocentric position diagram