Melotte 243
(Collinder 455; NGC 7654; MWSC 3725; M 52; OCL 260; FoF 526)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1216
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
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 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 | â |
| Almeida et al. | 2025 | 351.203 | 61.587 | â | â | â | â |
| 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 | â | â | â |
| Hunt & Reffert | 2023 | 351.19 | 61.599 | 0.606 | -1.895 | -1.191 | -23.905 |
| Just et al. | 2023 | 351.169 | 61.633 | â | â | â | â |
| Jaehnig et al. | 2021 | 351.208 | 61.591 | 0.625 | -1.933 | -1.128 | â |
| Rain et al. | 2021 | 351.195 | 61.59 | 0.596 | -1.938 | -1.131 | â |
| 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 | â |
| Cantat-Gaudin & Anders | 2020 | 351.195 | 61.59 | 0.596 | -1.938 | -1.131 | â |
| Liu & Pang | 2019 | 351.182 | 61.586 | 0.595 | -1.931 | -1.134 | â |
| Soubiran et al. | 2018 | 351.195 | 61.59 | â | â | â | -32.09 |
| Bica et al. | 2019 | 351.139 | 61.589 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 351.195 | 61.59 | 0.596 | -1.938 | -1.131 | â |
| Loktin & Popova | 2017 | 351.195 | 61.593 | â | -0.204 | -0.851 | -40.0 |
| Kharchenko et al. | 2016 | 351.169 | 61.633 | â | â | â | â |
| Dias et al. | 2014 | 351.2 | 61.593 | â | -0.89 | -1.0 | â |
| Kharchenko et al. | 2013 | 351.177 | 61.637 | â | -0.23 | -3.5 | -40.0 |
| Gozha et al. | 2012 | 351.2 | 61.593 | â | â | â | â |
| Kharchenko et al. | 2012 | 351.177 | 61.637 | â | -0.17 | -3.41 | -40.0 |
| Piskunov et al. | 2008 | 351.185 | 61.586 | â | â | â | â |
| Kharchenko et al. | 2007 | 351.19 | 61.59 | â | 0.17 | â | -40.0 |
| van den Bergh | 2006 | 351.2 | 61.583 | â | â | â | â |
| Kharchenko et al. | 2005 | 351.19 | 61.59 | â | -1.72 | -2.16 | -40.0 |
| Kharchenko et al. | 2003 | 351.15 | 61.62 | â | -1.23 | -1.38 | â |
| Chen et al. | 2003 | 351.117 | 61.649 | â | -2.0 | -1.78 | -35.5 |
| Dias et al. | 2002 | 351.2 | 61.593 | â | -0.89 | -1.0 | -32.98 |
| Dambis | 1999 | 351.2 | 61.593 | â | â | â | â |
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 | 1.45 | 2.02 | 1.7 | 79 | -0.087 | 2541 | 0.27 | 0.0 |
| Wei et al. | 2025 | 3.43 | 2.52 | â | 63 | -0.250 | 2541 | 0.27 | â |
| Almeida et al. | 2025 | 1.50 | 2.01 | â | 52 | â | 4884 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 5581(1) | â | â |
| Cavallo et al. | 2024 | 1.70 | 1.99 | â | 145 | 0.530 | â | â | â |
| Hunt & Reffert | 2023 | 1.56 | 1.95 | 1.70 | 84 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 79 | â | 337 | â | â |
| Jaehnig et al. | 2021 | 1.58(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.60 | 1.77 | â | 158 | â | â | â | 0 |
| Dias et al. | 2021 | 1.50 | 2.01 | â | 52 | 0.075 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.65 | 1.85 | â | 155 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.60 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 380 | -0.750 | â | â | â |
| Soubiran et al. | 2018 | 1.60 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.60 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.45 | 1.99 | â | 59 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.35 | 2.02 | â | 79 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.35 | 2.02 | â | 79 | â | â | â | â |
| Gozha et al. | 2012 | 1.40 | â | â | 158 | â | 155 | â | â |
| Kharchenko et al. | 2012 | 1.35 | 2.02 | â | 79 | â | â | â | â |
| Piskunov et al. | 2008 | 1.42 | 2.02 | â | 69 | â | â | â | â |
| van den Bergh | 2006 | 1.42 | 2.02 | â | 58 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.42 | 2.02 | â | 69 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.42 | 2.02 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.42 | â | â | 50 | â | â | â | â |
| Dias et al. | 2002 | 1.40 | 1.77 | â | 158 | â | â | â | â |
| Dambis | 1999 | 1.45 | 2.02 | â | 71 | â | 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.