Melotte 23
(Collinder 47; NGC 1528; MWSC 353; OCL 397; FoF 2138)
0.97
UTI
0.87
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
31.5 [N/pc2]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 23 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively 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 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 | 63.877 | 51.21 | 0.966 | 2.138 | -2.278 | -12.626 |
| Li et al. | 2025 | 63.878 | 51.218 | 0.948 | 2.181 | -2.246 | β |
| Almeida et al. | 2025 | 63.862 | 51.229 | β | β | β | β |
| Zhang et al. | 2024 | 63.906 | 51.195 | β | β | β | β |
| Hunt & Reffert | 2024 | 63.906 | 51.195 | 0.964 | 2.149 | -2.304 | -12.024 |
| Cavallo et al. | 2024 | 63.836 | 51.233 | 0.967 | β | β | β |
| Hunt & Reffert | 2023 | 63.906 | 51.195 | 0.964 | 2.149 | -2.304 | -12.024 |
| Almeida et al. | 2023 | 63.853 | 51.242 | β | β | β | β |
| Cordoni et al. | 2023 | 63.862 | 51.229 | 0.945 | 2.182 | -2.25 | β |
| Just et al. | 2023 | 63.836 | 51.19 | β | β | β | β |
| He et al. | 2022 | 63.859 | 51.219 | 0.972 | 2.128 | -2.298 | β |
| Tarricq et al. | 2022 | 63.89 | 51.221 | 0.986 | 2.133 | -2.273 | β |
| Jaehnig et al. | 2021 | 63.867 | 51.211 | 0.984 | 2.18 | -2.218 | β |
| Rain et al. | 2021 | 63.878 | 51.218 | 0.948 | 2.181 | -2.246 | β |
| Dias et al. | 2021 | 63.862 | 51.229 | 0.945 | 2.182 | -2.25 | -9.533 |
| Cantat-Gaudin et al. | 2020 | 63.878 | 51.218 | 0.948 | 2.181 | -2.246 | β |
| SΓ‘nchez et al. | 2020 | 63.846 | 51.215 | β | 2.227 | -2.174 | β |
| Cantat-Gaudin & Anders | 2020 | 63.878 | 51.218 | 0.948 | 2.181 | -2.246 | β |
| Liu & Pang | 2019 | 63.874 | 51.216 | 0.958 | 2.161 | -2.232 | β |
| Bossini et al. | 2019 | 63.878 | 51.218 | β | β | β | β |
| Soubiran et al. | 2018 | 63.878 | 51.218 | β | β | β | -9.62 |
| Bica et al. | 2019 | 63.852 | 51.229 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 63.878 | 51.218 | 0.948 | 2.181 | -2.246 | β |
| Loktin & Popova | 2017 | 63.84 | 51.216 | β | -2.074 | 1.13 | -9.2 |
| Kharchenko et al. | 2016 | 63.836 | 51.19 | β | β | β | β |
| Dias et al. | 2014 | 63.846 | 51.215 | β | 0.9 | -1.08 | β |
| Kharchenko et al. | 2013 | 63.847 | 51.19 | β | 1.2 | -1.38 | -9.2 |
| Gozha et al. | 2012 | 63.846 | 51.215 | β | β | β | β |
| Kharchenko et al. | 2012 | 63.847 | 51.19 | β | 1.2 | -1.38 | -9.15 |
| Piskunov et al. | 2008 | 63.829 | 51.214 | β | β | β | β |
| Kharchenko et al. | 2007 | 63.84 | 51.22 | β | 0.44 | β | -10.3 |
| Piskunov et al. | 2007 | 63.829 | 51.214 | β | β | β | β |
| van den Bergh | 2006 | 63.85 | 51.217 | β | β | β | β |
| Kharchenko et al. | 2005 | 63.84 | 51.22 | β | 1.67 | -2.46 | β |
| Kharchenko et al. | 2003 | 63.85 | 51.2 | β | 2.02 | -1.39 | β |
| Chen et al. | 2003 | 63.827 | 51.285 | β | 1.81 | -2.44 | -10.3 |
| Dias et al. | 2002 | 63.846 | 51.215 | β | 0.9 | -1.08 | -16.9 |
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 | 0.97 | 0.81 | 1.02 | 355 | 0.007 | 770 | 0.38 | 0.0 |
| Li et al. | 2025 | 0.94 | 0.90 | β | 470 | -0.043 | β | β | β |
| Almeida et al. | 2025 | 0.97 | 1.00 | β | 385 | β | 892 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.131(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1346(1) | β | β |
| Cavallo et al. | 2024 | 1.05 | 0.90 | β | 437 | 0.460 | β | β | β |
| Hunt & Reffert | 2023 | 0.98 | 0.92 | 1.02 | 209 | β | β | β | β |
| Almeida et al. | 2023 | 0.99 | 1.15 | β | 347 | 0.007 | 925(1) | 0.46 | β |
| Cordoni et al. | 2023 | 0.97 | 1.00 | β | 385 | 0.117 | 1075 | 0.30 | 0.00 |
| Just et al. | 2023 | β | β | β | 355 | β | 184 | β | β |
| He et al. | 2022 | β | 1.20 | β | 251 | β | β | β | β |
| Tarricq et al. | 2022 | 1.04 | β | β | 309 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.01(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.02 | 0.78 | β | 389 | β | β | β | 0 |
| Dias et al. | 2021 | 0.97 | 1.00 | β | 385 | 0.117 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.07 | 0.82 | β | 295 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.02 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 288 | 0.250 | β | β | β |
| Bossini et al. | 2019 | 0.99 | 0.79 | β | 394 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 1.02 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.02 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 0.80 | 0.82 | β | 344 | β | β | β | β |
| Kharchenko et al. | 2016 | 0.95 | 0.78 | β | 355 | β | β | β | β |
| Kharchenko et al. | 2013 | 0.95 | 0.78 | β | 355 | β | β | β | β |
| Gozha et al. | 2012 | 1.09 | β | β | 398 | -0.130 | 479 | β | β |
| Kharchenko et al. | 2012 | 0.95 | 0.78 | β | 355 | β | β | β | β |
| Piskunov et al. | 2008 | 0.78 | 0.74 | β | 269 | β | 647(1) | β | β |
| Piskunov et al. | 2007 | 0.78 | 0.74 | β | 269 | β | 239 | β | β |
| van den Bergh | 2006 | 0.78 | 0.81 | β | 372 | β | β | β | β |
| Kharchenko et al. | 2005 | 0.78 | 0.74 | β | 269 | β | β | β | β |
| Kharchenko et al. | 2003 | 0.78 | 0.81 | β | β | β | β | β | β |
| Chen et al. | 2003 | 0.78 | β | β | 360 | β | β | β | β |
| Dias et al. | 2002 | 1.09 | 0.81 | β | 398 | 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.
Cavallo et al. (2024)
Gold sample.