Melotte 183
(Collinder 354; VDBH 254; NGC 6475; MWSC 2739; M 7; OCL 1028; vdBergh-Hagen 254; ESO 394 09; FoF 2404; OCSN 240)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
117.0 [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
Melotte 183 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near 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 age parameter (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 268.471 | -34.831 | 3.578 | 3.075 | -5.397 | -14.533 |
| Nizovkina et al. | 2025 | 268.476 | -34.828 | â | â | â | â |
| Li et al. | 2025 | 268.447 | -34.841 | 3.572 | 3.099 | -5.426 | â |
| Wei et al. | 2025 | 268.469 | -34.841 | 3.579 | 3.07 | -5.403 | â |
| Almeida et al. | 2025 | 268.397 | -34.88 | â | â | â | â |
| Alfonso et al. | 2024 | 268.477 | -34.81 | 3.539 | 3.075 | -5.389 | â |
| Hunt & Reffert | 2024 | 268.476 | -34.828 | 3.583 | 3.08 | -5.366 | -14.55 |
| Cavallo et al. | 2024 | 268.483 | -34.784 | 3.583 | â | â | â |
| Hunt & Reffert | 2023 | 268.476 | -34.828 | 3.583 | 3.08 | -5.366 | -14.55 |
| Almeida et al. | 2023 | 268.421 | -34.872 | â | â | â | â |
| Qin et al. | 2023 | 268.45 | -34.82 | 3.58 | 3.06 | -5.38 | -14.24 |
| He et al. | 2022 | 268.446 | -34.793 | 3.584 | 3.033 | -5.37 | â |
| Tarricq et al. | 2022 | 268.434 | -34.879 | 3.591 | 3.067 | -5.404 | â |
| Jaehnig et al. | 2021 | 268.466 | -34.782 | 3.599 | 3.097 | -5.316 | â |
| Rain et al. | 2021 | 268.447 | -34.841 | 3.572 | 3.099 | -5.426 | â |
| Dias et al. | 2021 | 268.397 | -34.88 | 3.567 | 3.105 | -5.399 | -14.591 |
| Cantat-Gaudin et al. | 2020 | 268.447 | -34.841 | 3.572 | 3.099 | -5.426 | â |
| Cantat-Gaudin & Anders | 2020 | 268.447 | -34.841 | 3.572 | 3.099 | -5.426 | â |
| Liu & Pang | 2019 | 268.475 | -34.804 | 3.593 | 3.105 | -5.313 | â |
| Bossini et al. | 2019 | 268.447 | -34.841 | â | â | â | â |
| Soubiran et al. | 2018 | 268.447 | -34.841 | â | â | â | -14.84 |
| Bica et al. | 2019 | 268.466 | -34.807 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 268.447 | -34.841 | 3.572 | 3.099 | -5.426 | â |
| Yen et al. | 2018 | 268.373 | -34.656 | 3.45 | 3.15 | -5.51 | â |
| Loktin & Popova | 2017 | 268.455 | -34.794 | â | 1.67 | -3.6 | -12.6 |
| Kharchenko et al. | 2016 | 268.431 | -34.781 | â | â | â | â |
| Dias et al. | 2014 | 268.462 | -34.793 | â | -3.19 | -4.08 | â |
| Kharchenko et al. | 2013 | 268.44 | -34.78 | â | 2.58 | -4.98 | -12.6 |
| Gozha et al. | 2012 | 268.462 | -34.793 | â | â | â | â |
| Piskunov et al. | 2008 | 268.451 | -34.789 | â | â | â | â |
| Kharchenko et al. | 2007 | 268.45 | -34.79 | â | 1.2 | â | -14.21 |
| Piskunov et al. | 2007 | 268.451 | -34.789 | â | â | â | â |
| van den Bergh | 2006 | 268.45 | -34.783 | â | â | â | â |
| Kharchenko et al. | 2005 | 268.45 | -34.79 | â | 2.83 | -5.14 | -14.21 |
| Kharchenko et al. | 2003 | 268.47 | -34.8 | â | 2.82 | -5.26 | â |
| Chen et al. | 2003 | 268.476 | -34.812 | â | â | â | â |
| Dias et al. | 2002 | 268.462 | -34.793 | â | 1.67 | -3.6 | -14.78 |
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 | 0.285 | 0.31 | 0.65 | 224 | 0.030 | 791 | 0.285 | 1.0 |
| Nizovkina et al. | 2025 | 0.24(4) | 0.21(4) | â | 292(4) | -0.044(4) | â | â | â |
| Li et al. | 2025 | 0.27 | 0.26 | â | 341 | 0.047 | â | â | â |
| Wei et al. | 2025 | 0.37 | 0.66 | â | 68 | 0.000 | 1247 | 0.14 | â |
| Almeida et al. | 2025 | 0.28 | 0.38 | â | 273 | â | 993 | â | â |
| Alfonso et al. | 2024 | 0.29 | 0.30 | â | 271 | 0.020 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2379(1) | â | â |
| Cavallo et al. | 2024 | 0.27 | 0.95 | â | 126 | -0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.27 | 0.21 | 0.65 | 171 | â | â | â | â |
| Almeida et al. | 2023 | 0.27 | 0.20 | â | 465 | 0.114 | 791(1) | 0.43 | â |
| Qin et al. | 2023 | 0.32 | 0.37 | â | 200 | â | â | â | â |
| He et al. | 2022 | â | 0.50 | â | 141 | â | â | â | â |
| Tarricq et al. | 2022 | 0.28 | â | â | 224 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.28(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.28 | 0.31 | â | 295 | â | â | â | 1 |
| Dias et al. | 2021 | 0.28 | 0.38 | â | 273 | 0.019 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.29 | 0.30 | â | 224 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.28 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 186 | -0.250 | â | â | â |
| Bossini et al. | 2019 | 0.28 | 0.15 | â | 300 | 0.070 | â | â | â |
| Soubiran et al. | 2018 | 0.28 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.28 | â | â | â | â | â | â | â |
| Yen et al. | 2018 | 0.30 | 0.48 | â | 195 | â | â | â | â |
| Loktin & Popova | 2017 | 0.30 | 0.32 | â | 299 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.30 | 0.68 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.30 | 0.68 | â | 178 | 0.140 | â | â | â |
| Gozha et al. | 2012 | 0.30 | â | â | 299 | 0.140 | 661 | â | â |
| Piskunov et al. | 2008 | 0.30 | 0.31 | â | 166 | â | 735(1) | â | â |
| Piskunov et al. | 2007 | 0.30 | 0.31 | â | 166 | â | 436 | â | â |
| van den Bergh | 2006 | 0.30 | 0.31 | â | 302 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.30 | 0.31 | â | 166 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.28 | 0.31 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.30 | 0.32 | â | 290 | 0.030(1) | â | â | â |
| Dias et al. | 2002 | 0.30 | 0.32 | â | 299 | 0.140 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.