Melotte 81
(Collinder 171; NGC 2509; MWSC 1410; OCL 630; ESO 561 07; FSR 1282; FoF 588)
0.98
UTI
0.88
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
29.9 [N/pc2]
- CN 0.88 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 81 is a 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, old cluster, but with a large variance across recent sources for the absorption, 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 | 120.202 | -19.057 | 0.371 | -2.72 | 0.798 | 60.613 |
| Li et al. | 2025 | 120.201 | -19.056 | 0.363 | -2.708 | 0.764 | β |
| Hu & Soubiran | 2025 | 120.201 | -19.058 | β | β | β | β |
| Almeida et al. | 2025 | 120.2 | -19.058 | β | β | β | β |
| Hunt & Reffert | 2024 | 120.201 | -19.058 | 0.373 | -2.72 | 0.804 | 58.708 |
| Cavallo et al. | 2024 | 120.201 | -19.058 | 0.374 | β | β | β |
| Hunt & Reffert | 2023 | 120.201 | -19.058 | 0.373 | -2.72 | 0.804 | 58.708 |
| Almeida et al. | 2023 | 120.2 | -19.058 | β | β | β | β |
| Just et al. | 2023 | 120.189 | -19.048 | β | β | β | β |
| Dias et al. | 2021 | 120.2 | -19.058 | 0.364 | -2.708 | 0.766 | 61.087 |
| Cantat-Gaudin et al. | 2020 | 120.201 | -19.056 | 0.363 | -2.708 | 0.764 | β |
| SΓ‘nchez et al. | 2020 | 120.2 | -19.052 | β | -2.759 | 0.752 | β |
| Cantat-Gaudin & Anders | 2020 | 120.201 | -19.056 | 0.363 | -2.708 | 0.764 | β |
| Liu & Pang | 2019 | 120.198 | -19.056 | 0.369 | -2.712 | 0.771 | β |
| Soubiran et al. | 2018 | 120.201 | -19.056 | β | β | β | 60.83 |
| Bica et al. | 2019 | 120.193 | -19.056 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 120.201 | -19.056 | 0.363 | -2.708 | 0.764 | β |
| Loktin & Popova | 2017 | 120.195 | -19.05 | β | -6.133 | 2.19 | β |
| Kharchenko et al. | 2016 | 120.189 | -19.048 | β | β | β | β |
| Dias et al. | 2014 | 120.2 | -19.052 | β | -2.64 | 1.81 | β |
| Kharchenko et al. | 2013 | 120.195 | -19.05 | β | -3.82 | 4.24 | β |
| Dias et al. | 2002 | 120.2 | -19.052 | β | -2.64 | 1.81 | β |
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 | 2.46 | 0.32 | 0.16 | 1514 | -0.021 | 1194 | 0.89 | β |
| Li et al. | 2025 | 2.50 | 0.35 | β | 1468 | 0.057 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.100(5) | β | β | β |
| Almeida et al. | 2025 | 2.41 | 0.33 | β | 1514 | β | 935 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2169(1) | β | β |
| Cavallo et al. | 2024 | 2.18 | 0.61 | β | 1479 | -0.230 | β | β | β |
| Hunt & Reffert | 2023 | 2.42 | 0.12 | 0.16 | 1644 | β | β | β | β |
| Almeida et al. | 2023 | 2.83 | 0.06 | β | 1400 | 0.426 | 1453(1) | 0.89 | β |
| Just et al. | 2023 | β | β | β | 1585 | β | 255 | β | β |
| Dias et al. | 2021 | 2.41 | 0.33 | β | 1514 | 0.082 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.50 | 0.23 | β | 1514 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.55 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 2290 | -0.500 | β | β | β |
| Soubiran et al. | 2018 | 2.55 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.55 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.25 | 0.14 | β | 1288 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.71 | 0.32 | β | 1585 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.71 | 0.32 | β | 1585 | β | β | β | β |
| Dias et al. | 2002 | 0.91 | 0.46 | β | 7943 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.