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
Stellar density (N50/rad) 15.3 [N/pc2]
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 MOCAMOCA 🔍 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.

Palma et al. (2025)
Part of multiple system G154, along with NGC_3590, ASCC_65, HSC_2406 and UBC_659.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg44' along with Hogg 10.

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 – – – –
Bukowiecki et al. 2011 167.6 -60.246 – – – –
Piskunov et al. 2008 167.612 -60.243 – – – –
Kharchenko et al. 2007 167.59 -60.25 – 0.11 – -8.47
Ahumada & Lapasset 2007 167.6 -60.25 – – – –
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 1.23 1.5 8 -0.054 522 – 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 1.20 – 8 – – – 0
Dias et al. 2021 2.28 1.44 – 6 0.071 – – –
Cantat-Gaudin et al. 2020 2.45 1.53 – 5 – – – –
Kounkel et al. 2020 2.48 1.30 – 18 – – – –
Cantat-Gaudin & Anders 2020 2.47 – – – – – – –
Soubiran et al. 2018 2.47 – – – – – – –
Cantat-Gaudin et al. 2018 2.47 – – – – – – –
Loktin & Popova 2017 2.00 1.22 – 8 – – – –
Kharchenko et al. 2016 2.00 1.15 – 8 – – – –
Kharchenko et al. 2013 2.00 1.15 – 8 – – – –
Bukowiecki et al. 2012 – – – – – 730 – –
Gozha et al. 2012 2.00 – – 8 – 427 – –
Bukowiecki et al. 2011 2.04(1) 1.07 – 10 – – – –
Piskunov et al. 2008 2.00 1.07 – 8 – – – –
Ahumada & Lapasset 2007 – 1.23 – 8 – – – 0
van den Bergh 2006 2.00 1.23 – 8 – – – –
Kharchenko et al. 2005 2.00 1.07 – 8 – – – –
Kharchenko et al. 2003 2.00 1.17 – – – – – –
Dias et al. 2002 2.00 1.23 – 8 – – – –
Dambis 1999 2.40 1.39 – 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 0.77

💡 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