Melotte 224
(Collinder 406; NGC 6830; MWSC 3191; OCL 125)
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
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 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 | β |
| Wei et al. | 2025 | 297.715 | 23.087 | 0.43 | -3.198 | -5.777 | β |
| Almeida et al. | 2025 | 297.724 | 23.101 | β | β | β | β |
| 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 | β | β | β |
| Hunt & Reffert | 2023 | 297.722 | 23.098 | 0.415 | -3.196 | -5.759 | -1.175 |
| Almeida et al. | 2023 | 297.725 | 23.098 | β | β | β | β |
| Just et al. | 2023 | 297.744 | 23.097 | β | β | β | β |
| Jaehnig et al. | 2021 | 297.717 | 23.098 | 0.456 | -3.204 | -5.758 | β |
| Rain et al. | 2021 | 297.718 | 23.101 | 0.424 | -3.213 | -5.766 | β |
| Dias et al. | 2021 | 297.724 | 23.101 | 0.426 | -3.215 | -5.752 | β |
| Cantat-Gaudin et al. | 2020 | 297.718 | 23.101 | 0.424 | -3.213 | -5.766 | β |
| SΓ‘nchez et al. | 2020 | 297.746 | 23.1 | β | -3.154 | -5.753 | β |
| Cantat-Gaudin & Anders | 2020 | 297.718 | 23.101 | 0.424 | -3.213 | -5.766 | β |
| Bossini et al. | 2019 | 297.718 | 23.101 | β | β | β | β |
| Soubiran et al. | 2018 | 297.718 | 23.101 | β | β | β | 2.62 |
| Bica et al. | 2019 | 297.743 | 23.095 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 297.718 | 23.101 | 0.424 | -3.213 | -5.766 | β |
| Loktin & Popova | 2017 | 297.75 | 23.1 | β | 0.316 | -7.392 | -30.9 |
| Kharchenko et al. | 2016 | 297.744 | 23.097 | β | β | β | β |
| Dias et al. | 2014 | 297.746 | 23.1 | β | -3.1 | -6.34 | β |
| Kharchenko et al. | 2013 | 297.75 | 23.1 | β | -0.86 | -4.0 | -30.9 |
| Gozha et al. | 2012 | 297.746 | 23.1 | β | β | β | β |
| Piskunov et al. | 2008 | 297.743 | 23.095 | β | β | β | β |
| Kharchenko et al. | 2007 | 297.75 | 23.1 | β | 0.17 | β | -30.9 |
| van den Bergh | 2006 | 297.75 | 23.1 | β | β | β | β |
| Kharchenko et al. | 2005 | 297.75 | 23.1 | β | -0.04 | -2.7 | β |
| Kharchenko et al. | 2003 | 297.76 | 23.08 | β | 0.07 | -5.86 | β |
| Dias et al. | 2002 | 297.746 | 23.1 | β | 0.89 | -2.76 | -30.9 |
| Dambis | 1999 | 297.746 | 23.1 | β | β | β | β |
π‘ 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 | 99999β | 2.03 | 1.57 | 1.74 | 86 | 0.240 | 1180 | 0.445 | 0.0 |
| Li et al. | 2025 | 1.85 | 1.57 | β | 236 | 0.054 | β | β | β |
| Wei et al. | 2025 | 2.49 | 1.66 | β | 71 | 0.500 | 2058 | 0.31 | β |
| Almeida et al. | 2025 | 2.04 | 1.75 | β | 107 | β | 642 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1871(1) | β | β |
| Cavallo et al. | 2024 | 2.39 | 1.88 | β | 69 | 0.590 | β | β | β |
| Hunt & Reffert | 2023 | 2.14 | 1.75 | 1.74 | 59 | β | β | β | β |
| Almeida et al. | 2023 | 2.02 | 1.86 | β | 53 | 0.159 | 699(1) | 0.58 | β |
| Just et al. | 2023 | β | β | β | 127 | β | 330 | β | β |
| Jaehnig et al. | 2021 | 2.19(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.21 | 1.49 | β | 100 | β | β | β | 0 |
| Dias et al. | 2021 | 2.04 | 1.75 | β | 107 | 0.280 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.38 | 1.44 | β | 162 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.21 | β | β | β | β | β | β | β |
| Bossini et al. | 2019 | 2.37 | 1.51 | β | 101 | 0.220 | β | β | β |
| Soubiran et al. | 2018 | 2.21 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.21 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.65 | 1.54 | β | 39 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.84 | 1.68 | β | 127 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.84 | 1.68 | β | 127 | β | β | β | β |
| Gozha et al. | 2012 | 1.64 | β | β | 37 | β | 1660 | β | β |
| Piskunov et al. | 2008 | 1.64 | 1.55 | β | 33 | β | β | β | β |
| van den Bergh | 2006 | 1.64 | 1.55 | β | 37 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.64 | 1.55 | β | 33 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.64 | 1.55 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.64 | 1.55 | β | 37 | 0.240 | β | β | β |
| Dambis | 1999 | 1.61 | 1.76 | β | 100 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.