Melotte 59
(Collinder 125; NGC 2324; MWSC 1084; OCL 542; FSR 1089; FoF 372)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
24.4 [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 59 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 106.034 | 1.045 | 0.214 | -0.328 | -0.086 | 45.015 |
| Li et al. | 2025 | 106.033 | 1.046 | 0.191 | -0.309 | -0.094 | â |
| Hu & Soubiran | 2025 | 106.03 | 1.043 | â | â | â | â |
| Almeida et al. | 2025 | 106.029 | 1.046 | â | â | â | â |
| Zhang et al. | 2024 | 106.035 | 1.047 | â | â | â | â |
| Hunt & Reffert | 2024 | 106.035 | 1.047 | 0.216 | -0.322 | -0.089 | 46.4 |
| Cavallo et al. | 2024 | 106.03 | 1.043 | 0.216 | â | â | â |
| Hunt & Reffert | 2023 | 106.035 | 1.047 | 0.216 | -0.322 | -0.089 | 46.4 |
| Just et al. | 2023 | 106.036 | 1.04 | â | â | â | â |
| Jaehnig et al. | 2021 | 106.043 | 1.05 | 0.217 | -0.324 | -0.11 | â |
| Rain et al. | 2021 | 106.033 | 1.046 | 0.191 | -0.309 | -0.094 | â |
| Dias et al. | 2021 | 106.029 | 1.046 | 0.189 | -0.308 | -0.096 | 43.948 |
| Cantat-Gaudin et al. | 2020 | 106.033 | 1.046 | 0.191 | -0.309 | -0.094 | â |
| Donor et al. | 2020 | 106.043 | 1.038 | â | -0.31 | -0.11 | 42.2 |
| Cantat-Gaudin & Anders | 2020 | 106.033 | 1.046 | 0.191 | -0.309 | -0.094 | â |
| Liu & Pang | 2019 | 106.034 | 1.034 | 0.252 | -0.36 | -0.049 | â |
| Soubiran et al. | 2018 | 106.033 | 1.046 | â | â | â | 41.76 |
| Bica et al. | 2019 | 106.033 | 1.044 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 106.033 | 1.046 | 0.191 | -0.309 | -0.094 | â |
| Loktin & Popova | 2017 | 106.035 | 1.046 | â | -4.199 | -0.59 | 41.8 |
| Kharchenko et al. | 2016 | 106.036 | 1.04 | â | â | â | â |
| Dias et al. | 2014 | 106.029 | 1.045 | â | -2.6 | 1.35 | â |
| Kharchenko et al. | 2013 | 106.042 | 1.038 | â | -2.74 | 0.35 | 41.8 |
| Gozha et al. | 2012 | 106.029 | 1.045 | â | â | â | â |
| Kharchenko et al. | 2007 | 106.03 | 1.04 | â | 0.09 | â | â |
| van den Bergh | 2006 | 106.05 | 1.05 | â | â | â | â |
| Chen et al. | 2003 | 106.056 | 0.999 | â | -1.7 | -2.77 | 41.8 |
| Dias et al. | 2002 | 106.029 | 1.045 | â | -2.6 | 1.35 | 41.81 |
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 | 3.88 | 0.705 | 0.34 | 479 | -0.182 | 2979 | â | 1.0 |
| Li et al. | 2025 | 4.03 | 0.67 | â | 592 | -0.174 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Almeida et al. | 2025 | 3.70 | 0.77 | â | 564 | â | 1467 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.257(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3409(1) | â | â |
| Cavallo et al. | 2024 | 3.45 | 0.54 | â | 759 | -0.130 | â | â | â |
| Hunt & Reffert | 2023 | 4.42 | 0.16 | 0.34 | 600 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 479 | â | 2979 | â | â |
| Jaehnig et al. | 2021 | 4.61(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 4.54 | 0.78 | â | 447 | â | â | â | 1 |
| Dias et al. | 2021 | 3.70 | 0.77 | â | 564 | -0.216 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.21 | 0.40 | â | 537 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.190 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.54 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1000 | -2.000 | â | â | â |
| Soubiran et al. | 2018 | 4.54 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.54 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.92 | 0.38 | â | 439 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.84 | 0.74 | â | 479 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.84 | 0.74 | â | 479 | -0.170 | â | â | â |
| Gozha et al. | 2012 | 3.80 | â | â | 447 | -0.170 | â | â | â |
| van den Bergh | 2006 | 3.81 | 0.40 | â | 427 | â | â | â | â |
| Chen et al. | 2003 | 3.81 | â | â | 420 | â | â | â | â |
| Dias et al. | 2002 | 3.80 | 0.78 | â | 447 | -0.170 | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.