Melotte 93
(Collinder 200; VDBH 50; NGC 2670; MWSC 1554; OCL 764; vdBergh-Hagen 50; ESO 210 05; FoF 694)
0.92
UTI
0.83
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
35.3 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 93 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate 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 | 131.388 | -48.797 | 0.666 | -5.356 | 3.667 | 19.38 |
| Li et al. | 2025 | 131.386 | -48.801 | 0.647 | -5.379 | 3.621 | β |
| Wei et al. | 2025 | 131.401 | -48.803 | 0.657 | -5.37 | 3.723 | β |
| Almeida et al. | 2025 | 131.375 | -48.81 | β | β | β | β |
| Hunt & Reffert | 2024 | 131.369 | -48.791 | 0.666 | -5.36 | 3.678 | 14.814 |
| Cavallo et al. | 2024 | 131.374 | -48.812 | 0.668 | β | β | β |
| Hunt & Reffert | 2023 | 131.369 | -48.791 | 0.666 | -5.36 | 3.678 | 14.814 |
| Almeida et al. | 2023 | 131.395 | -48.783 | β | β | β | β |
| Just et al. | 2023 | 131.388 | -48.817 | β | β | β | β |
| Tarricq et al. | 2022 | 131.404 | -48.801 | 0.661 | -5.349 | 3.692 | β |
| Jaehnig et al. | 2021 | 131.386 | -48.796 | 0.681 | -5.379 | 3.599 | β |
| Rain et al. | 2021 | 131.386 | -48.801 | 0.647 | -5.379 | 3.621 | β |
| Dias et al. | 2021 | 131.375 | -48.81 | 0.651 | -5.381 | 3.606 | β |
| Cantat-Gaudin et al. | 2020 | 131.386 | -48.801 | 0.647 | -5.379 | 3.621 | β |
| SΓ‘nchez et al. | 2020 | 131.375 | -48.8 | β | -5.356 | 3.635 | β |
| Cantat-Gaudin & Anders | 2020 | 131.386 | -48.801 | 0.647 | -5.379 | 3.621 | β |
| Liu & Pang | 2019 | 131.375 | -48.795 | 0.653 | -5.392 | 3.606 | β |
| Soubiran et al. | 2018 | 131.386 | -48.801 | β | β | β | 5.15 |
| Bica et al. | 2019 | 131.385 | -48.8 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 131.386 | -48.801 | 0.647 | -5.379 | 3.621 | β |
| Loktin & Popova | 2017 | 131.37 | -48.8 | β | -6.15 | 5.74 | 17.2 |
| Kharchenko et al. | 2016 | 131.388 | -48.817 | β | β | β | β |
| Dias et al. | 2014 | 131.375 | -48.8 | β | -6.15 | 5.74 | β |
| Kharchenko et al. | 2013 | 131.392 | -48.82 | β | -11.95 | 6.2 | 17.2 |
| Gozha et al. | 2012 | 131.375 | -48.8 | β | β | β | β |
| Piskunov et al. | 2008 | 131.364 | -48.799 | β | β | β | β |
| van den Bergh | 2006 | 131.375 | -48.8 | β | β | β | β |
| Kharchenko et al. | 2005 | 131.37 | -48.8 | β | -11.97 | 4.86 | β |
| Kharchenko et al. | 2003 | 131.38 | -48.78 | β | -11.05 | 3.98 | β |
| Dias et al. | 2002 | 131.375 | -48.8 | β | -6.15 | 5.74 | 17.2 |
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 | 1.41 | 1.33 | 1.81 | 114 | 0.277 | 682 | 0.435 | 0.0 |
| Li et al. | 2025 | 1.21 | 1.16 | β | 253 | -0.254 | β | β | β |
| Wei et al. | 2025 | 2.44 | 1.46 | β | 407 | 0.250 | 1054 | 0.34 | β |
| Almeida et al. | 2025 | 1.47 | 1.31 | β | 93 | β | 802 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1147(1) | β | β |
| Cavallo et al. | 2024 | 1.56 | 1.25 | β | 191 | 0.620 | β | β | β |
| Hunt & Reffert | 2023 | 1.41 | 1.50 | 1.81 | 105 | β | β | β | β |
| Almeida et al. | 2023 | 1.39 | 1.42 | β | 125 | 0.148 | 562(1) | 0.53 | β |
| Just et al. | 2023 | β | β | β | 138 | β | 28 | β | β |
| Tarricq et al. | 2022 | 1.46 | β | β | 123 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.47(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.48 | 1.33 | β | 49 | β | β | β | 0 |
| Dias et al. | 2021 | 1.47 | 1.31 | β | 93 | 0.304 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.51 | 1.08 | β | 102 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.48 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 63 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 1.48 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.48 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.19 | 1.33 | β | 49 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.29 | 1.35 | β | 138 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.29 | 1.35 | β | 138 | β | β | β | β |
| Gozha et al. | 2012 | 1.19 | β | β | 49 | β | 44 | β | β |
| Piskunov et al. | 2008 | 1.19 | 1.33 | β | 126 | β | β | β | β |
| van den Bergh | 2006 | 1.19 | 1.33 | β | 49 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.19 | 1.33 | β | 126 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.12 | 1.05 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.19 | 1.33 | β | 49 | 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. Gold sample.
Cavallo et al. (2024)
Gold sample.