Melotte 224

(Collinder 406; NGC 6830; MWSC 3191; OCL 125)

Click to load Aladin Lite
0.96 UTI
0.82
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 22.3 [N/pc2]
  • CN 0.82 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

ℹ️
Melotte 224 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below 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. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 297.716 23.097 0.429 -3.202 -5.767 1.201
Li et al. 2025 297.718 23.101 0.424 -3.213 -5.766 –
Wei et al. 2025 297.715 23.087 0.43 -3.198 -5.777 –
Almeida et al. 2025 297.724 23.101 – – – –
Hunt & Reffert 2024 297.722 23.098 0.415 -3.196 -5.759 -1.175
Cavallo et al. 2024 297.717 23.1 0.42 – – –
Hunt & Reffert 2023 297.722 23.098 0.415 -3.196 -5.759 -1.175
Almeida et al. 2023 297.725 23.098 – – – –
Just et al. 2023 297.744 23.097 – – – –
Jaehnig et al. 2021 297.717 23.098 0.456 -3.204 -5.758 –
Rain et al. 2021 297.718 23.101 0.424 -3.213 -5.766 –
Dias et al. 2021 297.724 23.101 0.426 -3.215 -5.752 –
Cantat-Gaudin et al. 2020 297.718 23.101 0.424 -3.213 -5.766 –
SΓ‘nchez et al. 2020 297.746 23.1 – -3.154 -5.753 –
Cantat-Gaudin & Anders 2020 297.718 23.101 0.424 -3.213 -5.766 –
Bossini et al. 2019 297.718 23.101 – – – –
Soubiran et al. 2018 297.718 23.101 – – – 2.62
Bica et al. 2019 297.743 23.095 – – – –
Cantat-Gaudin et al. 2018 297.718 23.101 0.424 -3.213 -5.766 –
Loktin & Popova 2017 297.75 23.1 – 0.316 -7.392 -30.9
Kharchenko et al. 2016 297.744 23.097 – – – –
Dias et al. 2014 297.746 23.1 – -3.1 -6.34 –
Kharchenko et al. 2013 297.75 23.1 – -0.86 -4.0 -30.9
Gozha et al. 2012 297.746 23.1 – – – –
Piskunov et al. 2008 297.743 23.095 – – – –
Kharchenko et al. 2007 297.75 23.1 – 0.17 – -30.9
van den Bergh 2006 297.75 23.1 – – – –
Kharchenko et al. 2005 297.75 23.1 – -0.04 -2.7 –
Kharchenko et al. 2003 297.76 23.08 – 0.07 -5.86 –
Dias et al. 2002 297.746 23.1 – 0.89 -2.76 -30.9
Dambis 1999 297.746 23.1 – – – –

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– 2.03 1.57 1.74 86 0.240 1180 0.445 0.0
Li et al. 2025 1.85 1.57 – 236 0.054 – – –
Wei et al. 2025 2.49 1.66 – 71 0.500 2058 0.31 –
Almeida et al. 2025 2.04 1.75 – 107 – 642 – –
Hunt & Reffert 2024 – – – – – 1871(1) – –
Cavallo et al. 2024 2.39 1.88 – 69 0.590 – – –
Hunt & Reffert 2023 2.14 1.75 1.74 59 – – – –
Almeida et al. 2023 2.02 1.86 – 53 0.159 699(1) 0.58 –
Just et al. 2023 – – – 127 – 330 – –
Jaehnig et al. 2021 2.19(1) – – – – – – –
Rain et al. 2021 2.21 1.49 – 100 – – – 0
Dias et al. 2021 2.04 1.75 – 107 0.280 – – –
Cantat-Gaudin et al. 2020 2.38 1.44 – 162 – – – –
Cantat-Gaudin & Anders 2020 2.21 – – – – – – –
Bossini et al. 2019 2.37 1.51 – 101 0.220 – – –
Soubiran et al. 2018 2.21 – – – – – – –
Cantat-Gaudin et al. 2018 2.21 – – – – – – –
Loktin & Popova 2017 1.65 1.54 – 39 – – – –
Kharchenko et al. 2016 1.84 1.68 – 127 – – – –
Kharchenko et al. 2013 1.84 1.68 – 127 – – – –
Gozha et al. 2012 1.64 – – 37 – 1660 – –
Piskunov et al. 2008 1.64 1.55 – 33 – – – –
van den Bergh 2006 1.64 1.55 – 37 – – – –
Kharchenko et al. 2005 1.64 1.55 – 33 – – – –
Kharchenko et al. 2003 1.64 1.55 – – – – – –
Dias et al. 2002 1.64 1.55 – 37 0.240 – – –
Dambis 1999 1.61 1.76 – 100 – – – –

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

Visualization

ℹ️