Melotte 243

(Collinder 455; NGC 7654; MWSC 3725; M 52; OCL 260; FoF 526)

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1.0 UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 143.0 [N/pc2]
  • 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¸
Melotte 243 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.

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 99999– 351.192 61.592 0.608 -1.899 -1.184 -25.876
Wei et al. 2025 351.184 61.588 0.61 -1.893 -1.199 –
Almeida et al. 2025 351.203 61.587 – – – –
Hunt & Reffert 2024 351.19 61.599 0.606 -1.895 -1.191 -23.905
Cavallo et al. 2024 351.206 61.591 0.607 – – –
Hunt & Reffert 2023 351.19 61.599 0.606 -1.895 -1.191 -23.905
Just et al. 2023 351.169 61.633 – – – –
Jaehnig et al. 2021 351.208 61.591 0.625 -1.933 -1.128 –
Rain et al. 2021 351.195 61.59 0.596 -1.938 -1.131 –
Dias et al. 2021 351.203 61.587 0.597 -1.936 -1.132 -32.09
Cantat-Gaudin et al. 2020 351.195 61.59 0.596 -1.938 -1.131 –
Cantat-Gaudin & Anders 2020 351.195 61.59 0.596 -1.938 -1.131 –
Liu & Pang 2019 351.182 61.586 0.595 -1.931 -1.134 –
Soubiran et al. 2018 351.195 61.59 – – – -32.09
Bica et al. 2019 351.139 61.589 – – – –
Cantat-Gaudin et al. 2018 351.195 61.59 0.596 -1.938 -1.131 –
Loktin & Popova 2017 351.195 61.593 – -0.204 -0.851 -40.0
Kharchenko et al. 2016 351.169 61.633 – – – –
Dias et al. 2014 351.2 61.593 – -0.89 -1.0 –
Kharchenko et al. 2013 351.177 61.637 – -0.23 -3.5 -40.0
Gozha et al. 2012 351.2 61.593 – – – –
Kharchenko et al. 2012 351.177 61.637 – -0.17 -3.41 -40.0
Piskunov et al. 2008 351.185 61.586 – – – –
Kharchenko et al. 2007 351.19 61.59 – 0.17 – -40.0
van den Bergh 2006 351.2 61.583 – – – –
Kharchenko et al. 2005 351.19 61.59 – -1.72 -2.16 -40.0
Kharchenko et al. 2003 351.15 61.62 – -1.23 -1.38 –
Chen et al. 2003 351.117 61.649 – -2.0 -1.78 -35.5
Dias et al. 2002 351.2 61.593 – -0.89 -1.0 -32.98
Dambis 1999 351.2 61.593 – – – –

💡 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– 1.45 2.02 1.7 79 -0.087 2541 0.27 0.0
Wei et al. 2025 3.43 2.52 – 63 -0.250 2541 0.27 –
Almeida et al. 2025 1.50 2.01 – 52 – 4884 – –
Hunt & Reffert 2024 – – – – – 5581(1) – –
Cavallo et al. 2024 1.70 1.99 – 145 0.530 – – –
Hunt & Reffert 2023 1.56 1.95 1.70 84 – – – –
Just et al. 2023 – – – 79 – 337 – –
Jaehnig et al. 2021 1.58(1) – – – – – – –
Rain et al. 2021 1.60 1.77 – 158 – – – 0
Dias et al. 2021 1.50 2.01 – 52 0.075 – – –
Cantat-Gaudin et al. 2020 1.65 1.85 – 155 – – – –
Cantat-Gaudin & Anders 2020 1.60 – – – – – – –
Liu & Pang 2019 – – – 380 -0.750 – – –
Soubiran et al. 2018 1.60 – – – – – – –
Cantat-Gaudin et al. 2018 1.60 – – – – – – –
Loktin & Popova 2017 1.45 1.99 – 59 – – – –
Kharchenko et al. 2016 1.35 2.02 – 79 – – – –
Kharchenko et al. 2013 1.35 2.02 – 79 – – – –
Gozha et al. 2012 1.40 – – 158 – 155 – –
Kharchenko et al. 2012 1.35 2.02 – 79 – – – –
Piskunov et al. 2008 1.42 2.02 – 69 – – – –
van den Bergh 2006 1.42 2.02 – 58 – – – –
Kharchenko et al. 2005 1.42 2.02 – 69 – – – –
Kharchenko et al. 2003 1.42 2.02 – – – – – –
Chen et al. 2003 1.42 – – 50 – – – –
Dias et al. 2002 1.40 1.77 – 158 – – – –
Dambis 1999 1.45 2.02 – 71 – – – –

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

Visualization

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