Melotte 238
(Collinder 444; NGC 7209; MWSC 3585; OCL 215; FoF 2055)
0.97
UTI
0.86
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
10.8 [N/pc2]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 238 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 | 99999â | 331.227 | 46.51 | 0.817 | 2.296 | 0.267 | -19.21 |
| Li et al. | 2025 | 331.224 | 46.508 | 0.82 | 2.255 | 0.283 | â |
| Wei et al. | 2025 | 331.229 | 46.49 | 0.821 | 2.304 | 0.278 | â |
| Almeida et al. | 2025 | 331.229 | 46.495 | â | â | â | â |
| Hunt & Reffert | 2024 | 331.228 | 46.531 | 0.816 | 2.294 | 0.265 | -20.812 |
| Cavallo et al. | 2024 | 331.199 | 46.505 | 0.816 | â | â | â |
| Hunt & Reffert | 2023 | 331.228 | 46.531 | 0.816 | 2.294 | 0.265 | -20.812 |
| Almeida et al. | 2023 | 331.192 | 46.521 | â | â | â | â |
| Cordoni et al. | 2023 | 331.229 | 46.495 | 0.824 | 2.264 | 0.292 | â |
| Just et al. | 2023 | 331.22 | 46.548 | â | â | â | â |
| He et al. | 2022 | 331.241 | 46.507 | 0.816 | 2.298 | 0.258 | â |
| Tarricq et al. | 2022 | 331.258 | 46.522 | 0.811 | 2.309 | 0.258 | â |
| Jaehnig et al. | 2021 | 331.281 | 46.508 | 0.847 | 2.293 | 0.313 | â |
| Rain et al. | 2021 | 331.224 | 46.508 | 0.82 | 2.255 | 0.283 | â |
| Dias et al. | 2021 | 331.229 | 46.495 | 0.824 | 2.264 | 0.292 | -18.188 |
| Cantat-Gaudin et al. | 2020 | 331.224 | 46.508 | 0.82 | 2.255 | 0.283 | â |
| Cantat-Gaudin & Anders | 2020 | 331.224 | 46.508 | 0.82 | 2.255 | 0.283 | â |
| Liu & Pang | 2019 | 331.255 | 46.494 | 0.819 | 2.275 | 0.296 | â |
| Bossini et al. | 2019 | 331.224 | 46.508 | â | â | â | â |
| Soubiran et al. | 2018 | 331.224 | 46.508 | â | â | â | -18.42 |
| Bica et al. | 2019 | 331.288 | 46.498 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 331.224 | 46.508 | 0.82 | 2.255 | 0.283 | â |
| Loktin & Popova | 2017 | 331.275 | 46.483 | â | -0.416 | 0.878 | -9.7 |
| Kharchenko et al. | 2016 | 331.22 | 46.548 | â | â | â | â |
| Dias et al. | 2014 | 331.279 | 46.483 | â | 0.04 | -0.16 | â |
| Kharchenko et al. | 2013 | 331.225 | 46.552 | â | -0.97 | 3.79 | -9.7 |
| Gozha et al. | 2012 | 331.279 | 46.483 | â | â | â | â |
| Kharchenko et al. | 2012 | 331.225 | 46.552 | â | -0.97 | 3.79 | -9.7 |
| Piskunov et al. | 2008 | 331.314 | 46.474 | â | â | â | â |
| Kharchenko et al. | 2007 | 331.27 | 46.48 | â | 0.25 | â | -9.7 |
| Piskunov et al. | 2007 | 331.314 | 46.474 | â | â | â | â |
| van den Bergh | 2006 | 331.325 | 46.483 | â | â | â | â |
| Kharchenko et al. | 2005 | 331.32 | 46.48 | â | 2.49 | 1.62 | â |
| Kharchenko et al. | 2003 | 331.27 | 46.46 | â | 2.76 | 1.04 | â |
| Chen et al. | 2003 | 331.265 | 46.487 | â | â | â | â |
| Dias et al. | 2002 | 331.279 | 46.483 | â | 0.04 | -0.16 | -18.63 |
đĄ 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 | 99999â | 1.17 | 0.52 | 0.56 | 426 | 0.048 | 784 | 0.4 | 0.0 |
| Li et al. | 2025 | 1.18 | 0.44 | â | 541 | 0.245 | â | â | â |
| Wei et al. | 2025 | 1.32 | 0.38 | â | 550 | 0.500 | 1222 | 0.40 | â |
| Almeida et al. | 2025 | 1.15 | 0.61 | â | 494 | â | 784 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1250(1) | â | â |
| Cavallo et al. | 2024 | 1.22 | 0.69 | â | 339 | 0.200 | â | â | â |
| Hunt & Reffert | 2023 | 1.17 | 0.39 | 0.56 | 396 | â | â | â | â |
| Almeida et al. | 2023 | 1.18 | 0.70 | â | 422 | 0.048 | 1087(1) | 0.50 | â |
| Cordoni et al. | 2023 | 1.14 | 0.61 | â | 494 | 0.146 | 1489 | 0.29 | 0.00 |
| Just et al. | 2023 | â | â | â | 426 | â | 153 | â | â |
| He et al. | 2022 | â | 0.85 | â | 251 | â | â | â | â |
| Tarricq et al. | 2022 | 1.12 | â | â | 457 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.18(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.18 | 0.53 | â | 339 | â | â | â | 0 |
| Dias et al. | 2021 | 1.15 | 0.61 | â | 494 | 0.146 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.15 | 0.53 | â | 427 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.18 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 525 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 1.17 | 0.55 | â | 341 | 0.070 | â | â | â |
| Soubiran et al. | 2018 | 1.18 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.18 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.20 | 0.49 | â | 412 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.25 | 0.50 | â | 426 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.25 | 0.50 | â | 426 | -0.120 | â | â | â |
| Gozha et al. | 2012 | 1.17 | â | â | 414 | -0.030 | 275 | â | â |
| Kharchenko et al. | 2012 | 1.25 | 0.50 | â | 426 | -0.120 | â | â | â |
| Piskunov et al. | 2008 | 1.17 | 0.50 | â | 447 | â | 398(1) | â | â |
| Piskunov et al. | 2007 | 1.17 | 0.50 | â | 447 | â | 129 | â | â |
| van den Bergh | 2006 | 1.17 | 0.53 | â | 417 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.17 | 0.50 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.17 | 0.53 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.17 | 0.52 | â | 410 | -0.120(1) | â | â | â |
| Dias et al. | 2002 | 1.17 | 0.52 | â | 414 | -0.120 | â | â | â |
(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. Gold sample.
Cavallo et al. (2024)
Gold sample.