Melotte 85
(Collinder 179; NGC 2548; MWSC 1454; M 48; OCL 584; FSR 1217; FoF 2362)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
29.2 [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 85 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a 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 | 99999â | 123.389 | -5.732 | 1.298 | -1.282 | 1.045 | 8.104 |
| Li et al. | 2025 | 123.412 | -5.726 | 1.289 | -1.313 | 1.029 | â |
| Almeida et al. | 2025 | 123.4 | -5.719 | â | â | â | â |
| Alfonso et al. | 2024 | 123.402 | -5.698 | 1.261 | -1.293 | 1.04 | â |
| Zhang et al. | 2024 | 123.455 | -5.77 | â | â | â | â |
| Hunt & Reffert | 2024 | 123.455 | -5.77 | 1.291 | -1.294 | 1.037 | 8.026 |
| Cavallo et al. | 2024 | 123.361 | -5.709 | 1.294 | â | â | â |
| Hunt & Reffert | 2023 | 123.455 | -5.77 | 1.291 | -1.294 | 1.037 | 8.026 |
| Almeida et al. | 2023 | 123.364 | -5.741 | â | â | â | â |
| Just et al. | 2023 | 123.428 | -5.767 | â | â | â | â |
| He et al. | 2022 | 123.401 | -5.737 | 1.301 | -1.282 | 1.042 | â |
| Tarricq et al. | 2022 | 123.385 | -5.74 | 1.306 | -1.28 | 1.043 | â |
| Jaehnig et al. | 2021 | 123.384 | -5.732 | 1.321 | -1.294 | 0.999 | â |
| Rain et al. | 2021 | 123.412 | -5.726 | 1.289 | -1.313 | 1.029 | â |
| Dias et al. | 2021 | 123.4 | -5.719 | 1.284 | -1.323 | 1.039 | 8.792 |
| Cantat-Gaudin et al. | 2020 | 123.412 | -5.726 | 1.289 | -1.313 | 1.029 | â |
| Cantat-Gaudin & Anders | 2020 | 123.412 | -5.726 | 1.289 | -1.313 | 1.029 | â |
| Liu & Pang | 2019 | 123.36 | -5.723 | 1.283 | -1.31 | 1.012 | â |
| Soubiran et al. | 2018 | 123.412 | -5.726 | â | â | â | 8.85 |
| Bica et al. | 2019 | 123.44 | -5.774 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 123.412 | -5.726 | 1.289 | -1.313 | 1.029 | â |
| Loktin & Popova | 2017 | 123.435 | -5.75 | â | -3.73 | 2.13 | 41.5 |
| Kharchenko et al. | 2016 | 123.428 | -5.767 | â | â | â | â |
| Dias et al. | 2014 | 123.429 | -5.75 | â | -3.73 | 2.13 | â |
| Kharchenko et al. | 2013 | 123.435 | -5.77 | â | -1.25 | 1.3 | 41.5 |
| Gozha et al. | 2012 | 123.429 | -5.75 | â | â | â | â |
| Piskunov et al. | 2008 | 123.425 | -5.749 | â | â | â | â |
| Kharchenko et al. | 2007 | 123.43 | -5.75 | â | 0.73 | â | 41.5 |
| Piskunov et al. | 2007 | 123.425 | -5.749 | â | â | â | â |
| van den Bergh | 2006 | 123.425 | -5.75 | â | â | â | â |
| Kharchenko et al. | 2005 | 123.43 | -5.75 | â | -0.78 | 1.55 | â |
| Kharchenko et al. | 2003 | 123.42 | -5.78 | â | -0.66 | 1.76 | â |
| Chen et al. | 2003 | 123.452 | -5.784 | â | -0.5 | 0.93 | 5.0 |
| Dias et al. | 2002 | 123.429 | -5.75 | â | -3.73 | 2.13 | 7.7 |
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 | 0.77 | 0.1 | 0.43 | 490 | 0.032 | 1016 | 0.45 | 0.0 |
| Li et al. | 2025 | 0.73 | 0.12 | â | 593 | -0.040 | â | â | â |
| Almeida et al. | 2025 | 0.75 | 0.12 | â | 521 | â | 906 | â | â |
| Alfonso et al. | 2024 | 0.77 | 0.15 | â | 490 | 0.032 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.081(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1476(1) | â | â |
| Cavallo et al. | 2024 | 0.77 | 0.10 | â | 417 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 0.73 | 0.10 | 0.43 | 379 | â | â | â | â |
| Almeida et al. | 2023 | 0.75 | 0.13 | â | 518 | -0.002 | 920(1) | 0.45 | â |
| Just et al. | 2023 | â | â | â | 525 | â | 1016 | â | â |
| He et al. | 2022 | â | 0.15 | â | 447 | â | â | â | â |
| Tarricq et al. | 2022 | 0.76 | â | â | 407 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.76(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.76 | 0.09 | â | 398 | â | â | â | 0 |
| Dias et al. | 2021 | 0.75 | 0.12 | â | 521 | 0.032 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.77 | 0.15 | â | 389 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.76 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 661 | -0.250 | â | â | â |
| Soubiran et al. | 2018 | 0.76 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.76 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.77 | 0.10 | â | 361 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.79 | 0.13 | â | 525 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.79 | 0.13 | â | 525 | 0.080 | â | â | â |
| Gozha et al. | 2012 | 0.77 | â | â | 398 | 0.080 | 1122 | â | â |
| Piskunov et al. | 2008 | 0.77 | 0.09 | â | 562 | â | 2366(1) | â | â |
| Piskunov et al. | 2007 | 0.77 | 0.09 | â | 562 | â | 986 | â | â |
| van den Bergh | 2006 | 0.77 | 0.09 | â | 363 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.77 | 0.09 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.77 | 0.09 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.77 | 0.10 | â | 360 | 0.080(1) | â | â | â |
| Dias et al. | 2002 | 0.77 | 0.09 | â | 398 | 0.080 | 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: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.