Melotte 83
(Collinder 176; NGC 2539; MWSC 1439; OCL 611; FoF 2043)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
37.3 [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 83 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 | 122.662 | -12.833 | 0.756 | -2.323 | -0.546 | 28.683 |
| Li et al. | 2025 | 122.658 | -12.834 | 0.754 | -2.331 | -0.584 | β |
| Hu & Soubiran | 2025 | 122.668 | -12.834 | β | β | β | β |
| Almeida et al. | 2025 | 122.657 | -12.835 | β | β | β | β |
| Hunt & Reffert | 2024 | 122.664 | -12.827 | 0.758 | -2.326 | -0.543 | 28.626 |
| Cavallo et al. | 2024 | 122.668 | -12.834 | 0.759 | β | β | β |
| Hunt & Reffert | 2023 | 122.664 | -12.827 | 0.758 | -2.326 | -0.543 | 28.626 |
| Almeida et al. | 2023 | 122.646 | -12.864 | β | β | β | β |
| Just et al. | 2023 | 122.663 | -12.838 | β | β | β | β |
| Tarricq et al. | 2022 | 122.637 | -12.844 | 0.763 | -2.326 | -0.538 | β |
| Jaehnig et al. | 2021 | 122.649 | -12.827 | 0.784 | -2.338 | -0.572 | β |
| Rain et al. | 2021 | 122.658 | -12.834 | 0.754 | -2.331 | -0.584 | β |
| Dias et al. | 2021 | 122.657 | -12.835 | 0.76 | -2.332 | -0.592 | 29.24 |
| Cantat-Gaudin et al. | 2020 | 122.658 | -12.834 | 0.754 | -2.331 | -0.584 | β |
| SΓ‘nchez et al. | 2020 | 122.654 | -12.818 | β | -2.384 | -0.686 | β |
| Cantat-Gaudin & Anders | 2020 | 122.658 | -12.834 | 0.754 | -2.331 | -0.584 | β |
| Liu & Pang | 2019 | 122.664 | -12.843 | 0.762 | -2.319 | -0.58 | β |
| Soubiran et al. | 2018 | 122.658 | -12.834 | β | β | β | 29.18 |
| Bica et al. | 2019 | 122.669 | -12.826 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 122.658 | -12.834 | 0.754 | -2.331 | -0.584 | β |
| Loktin & Popova | 2017 | 122.655 | -12.84 | β | -2.115 | -2.223 | 26.1 |
| Kharchenko et al. | 2016 | 122.663 | -12.838 | β | β | β | β |
| Dias et al. | 2014 | 122.654 | -12.818 | β | -3.2 | -1.24 | β |
| Kharchenko et al. | 2013 | 122.67 | -12.84 | β | -2.28 | -1.91 | 26.1 |
| Gozha et al. | 2012 | 122.654 | -12.818 | β | β | β | β |
| Piskunov et al. | 2008 | 122.666 | -12.84 | β | β | β | β |
| Kharchenko et al. | 2007 | 122.65 | -12.82 | β | 0.5 | β | 26.12 |
| Piskunov et al. | 2007 | 122.666 | -12.84 | β | β | β | β |
| van den Bergh | 2006 | 122.675 | -12.833 | β | β | β | β |
| Kharchenko et al. | 2005 | 122.67 | -12.84 | β | -3.37 | -1.87 | 26.12 |
| Kharchenko et al. | 2003 | 122.67 | -12.84 | β | -4.0 | -1.77 | β |
| Chen et al. | 2003 | 122.921 | -13.246 | β | -2.5 | -1.22 | 29.3 |
| Dias et al. | 2002 | 122.654 | -12.818 | β | -3.2 | -1.24 | 28.89 |
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 | 1.28 | 0.25 | 0.33 | 562 | 0.072 | 1786 | 0.44 | 0.0 |
| Li et al. | 2025 | 1.20 | 0.25 | β | 851 | -0.148 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.130(5) | β | β | β |
| Almeida et al. | 2025 | 1.24 | 0.21 | β | 764 | β | 1367 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2026(1) | β | β |
| Cavallo et al. | 2024 | 1.33 | 0.33 | β | 661 | 0.210 | β | β | β |
| Hunt & Reffert | 2023 | 1.21 | 0.08 | 0.33 | 1076 | β | β | β | β |
| Almeida et al. | 2023 | 1.24 | 0.14 | β | 776 | -0.005 | 1152(1) | 0.44 | β |
| Just et al. | 2023 | β | β | β | 543 | β | 989 | β | β |
| Tarricq et al. | 2022 | 1.20 | β | β | 708 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.27(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.28 | 0.25 | β | 372 | β | β | β | 0 |
| Dias et al. | 2021 | 1.24 | 0.21 | β | 764 | 0.015 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.23 | 0.11 | β | 692 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.28 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 912 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 1.28 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.28 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.39 | 0.26 | β | 379 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.23 | 0.45 | β | 543 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.23 | 0.45 | β | 543 | 0.130 | β | β | β |
| Gozha et al. | 2012 | 1.36 | β | β | 372 | 0.130 | 2455 | β | β |
| Piskunov et al. | 2008 | 1.36 | 0.25 | β | 562 | β | 5483(1) | β | β |
| Piskunov et al. | 2007 | 1.36 | 0.25 | β | 562 | β | 1786 | β | β |
| van den Bergh | 2006 | 1.36 | 0.25 | β | 372 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.36 | 0.25 | β | 562 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.37 | 0.25 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.36 | 0.25 | β | 370 | 0.130(1) | β | β | β |
| Dias et al. | 2002 | 1.36 | 0.25 | β | 372 | 0.130 | 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.