Melotte 54
(Collinder 119; NGC 2301; FSR 1071; MWSC 1000; OCL 540; FoF 2215)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1134
Stellar density (N50/rad)
85.6 [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 54 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a 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, 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 | 102.938 | 0.469 | 1.143 | -1.37 | -2.191 | 25.091 |
| Li et al. | 2025 | 102.943 | 0.465 | 1.135 | -1.367 | -2.179 | β |
| Wei et al. | 2025 | 102.942 | 0.475 | 1.153 | -1.356 | -2.189 | β |
| Almeida et al. | 2025 | 102.951 | 0.472 | β | β | β | β |
| Alfonso et al. | 2024 | 102.942 | 0.477 | 1.111 | -1.357 | -2.188 | β |
| Zhang et al. | 2024 | 102.937 | 0.462 | β | β | β | β |
| Hunt & Reffert | 2024 | 102.937 | 0.462 | 1.149 | -1.368 | -2.185 | 25.8 |
| Cavallo et al. | 2024 | 102.957 | 0.476 | 1.148 | β | β | β |
| Hunt & Reffert | 2023 | 102.937 | 0.462 | 1.149 | -1.368 | -2.185 | 25.8 |
| Almeida et al. | 2023 | 102.947 | 0.469 | β | β | β | β |
| Just et al. | 2023 | 102.938 | 0.467 | β | β | β | β |
| He et al. | 2022 | 102.948 | 0.474 | 1.151 | -1.361 | -2.181 | β |
| Tarricq et al. | 2022 | 102.944 | 0.454 | 1.15 | -1.355 | -2.193 | β |
| Jaehnig et al. | 2021 | 102.943 | 0.461 | 1.169 | -1.336 | -2.183 | β |
| Rain et al. | 2021 | 102.943 | 0.465 | 1.135 | -1.367 | -2.179 | β |
| Dias et al. | 2021 | 102.951 | 0.472 | 1.135 | -1.369 | -2.188 | 25.732 |
| Cantat-Gaudin et al. | 2020 | 102.943 | 0.465 | 1.135 | -1.367 | -2.179 | β |
| SΓ‘nchez et al. | 2020 | 102.938 | 0.46 | β | -1.383 | -2.002 | β |
| Cantat-Gaudin & Anders | 2020 | 102.943 | 0.465 | 1.135 | -1.367 | -2.179 | β |
| Liu & Pang | 2019 | 102.965 | 0.464 | 1.132 | -1.364 | -2.18 | β |
| Soubiran et al. | 2018 | 102.943 | 0.465 | β | β | β | 26.53 |
| Bica et al. | 2019 | 102.93 | 0.476 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 102.943 | 0.465 | 1.135 | -1.367 | -2.179 | β |
| Loktin & Popova | 2017 | 102.945 | 0.46 | β | -0.052 | -1.181 | 39.6 |
| Kharchenko et al. | 2016 | 102.938 | 0.467 | β | β | β | β |
| Dias et al. | 2014 | 102.937 | 0.46 | β | -0.83 | -2.76 | β |
| Kharchenko et al. | 2013 | 102.945 | 0.465 | β | -0.71 | -4.07 | 39.6 |
| Gozha et al. | 2012 | 102.938 | 0.46 | β | β | β | β |
| Piskunov et al. | 2008 | 102.939 | 0.459 | β | β | β | β |
| Kharchenko et al. | 2007 | 102.94 | 0.46 | β | 0.25 | β | 39.65 |
| Piskunov et al. | 2007 | 102.939 | 0.459 | β | β | β | β |
| Froebrich et al. | 2007 | 102.846 | 0.561 | β | β | β | β |
| van den Bergh | 2006 | 102.95 | 0.467 | β | β | β | β |
| Kharchenko et al. | 2005 | 102.94 | 0.46 | β | -1.5 | -4.35 | 62.0 |
| Kharchenko et al. | 2003 | 102.93 | 0.46 | β | -1.4 | -5.01 | β |
| Chen et al. | 2003 | 102.962 | 0.448 | β | -2.31 | -3.31 | 21.2 |
| Dias et al. | 2002 | 102.938 | 0.46 | β | -0.83 | -2.76 | 13.54 |
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 | 0.86 | 0.1 | 0.53 | 185 | 0.060 | 418 | 0.44 | 0.0 |
| Li et al. | 2025 | 0.85 | 0.18 | β | 259 | 0.050 | β | β | β |
| Wei et al. | 2025 | 0.86 | 0.17 | β | 98 | 0.250 | 1127 | 0.53 | β |
| Almeida et al. | 2025 | 0.85 | 0.23 | β | 185 | β | 1055 | β | β |
| Alfonso et al. | 2024 | 0.86 | 0.08 | β | 272 | 0.059 | β | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.102(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1498(1) | β | β |
| Cavallo et al. | 2024 | 0.86 | 0.23 | β | 145 | 0.190 | β | β | β |
| Hunt & Reffert | 2023 | 0.82 | 0.12 | 0.53 | 139 | β | β | β | β |
| Almeida et al. | 2023 | 0.83 | 0.25 | β | 202 | -0.031 | 725(1) | 0.35 | β |
| Just et al. | 2023 | β | β | β | 224 | β | 33 | β | β |
| He et al. | 2022 | β | 0.40 | β | 79 | β | β | β | β |
| Tarricq et al. | 2022 | 0.83 | β | β | 209 | β | β | β | β |
| Jaehnig et al. | 2021 | 0.86(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 0.86 | 0.09 | β | 158 | β | β | β | 0 |
| Dias et al. | 2021 | 0.85 | 0.23 | β | 185 | 0.057 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 0.86 | 0.08 | β | 214 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 0.86 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 98 | 0.250 | β | β | β |
| Soubiran et al. | 2018 | 0.86 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 0.86 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 0.87 | 0.10 | β | 163 | β | β | β | β |
| Kharchenko et al. | 2016 | 0.81 | 0.19 | β | 224 | β | β | β | β |
| Kharchenko et al. | 2013 | 0.81 | 0.19 | β | 224 | 0.060 | β | β | β |
| Gozha et al. | 2012 | 0.87 | β | β | 158 | 0.060 | 112 | β | β |
| Piskunov et al. | 2008 | 0.86 | 0.09 | β | 204 | β | 94(1) | β | β |
| Piskunov et al. | 2007 | 0.86 | 0.09 | β | 204 | β | 38 | β | β |
| van den Bergh | 2006 | 0.87 | 0.09 | β | 166 | β | β | β | β |
| Kharchenko et al. | 2005 | 0.86 | 0.09 | β | 204 | β | β | β | β |
| Kharchenko et al. | 2003 | 0.87 | 0.09 | β | β | β | β | β | β |
| Chen et al. | 2003 | 0.87 | 0.09 | β | 160 | 0.060(1) | β | β | β |
| Dias et al. | 2002 | 0.87 | 0.09 | β | 158 | 0.060 | 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.