Melotte 161
(Collinder 324; VDBH 213; NGC 6281; MWSC 2530; OCL 1003; vdBergh-Hagen 213; ESO 332 19; FoF 2332; OCSN 238)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
122.6 [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 161 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 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 | 99999â | 256.184 | -37.955 | 1.884 | -1.884 | -4.045 | -5.322 |
| Li et al. | 2025 | 256.179 | -37.948 | 1.873 | -1.856 | -4.017 | â |
| Wei et al. | 2025 | 256.181 | -37.95 | 1.885 | -1.902 | -4.044 | â |
| Almeida et al. | 2025 | 256.181 | -37.952 | â | â | â | â |
| Alfonso et al. | 2024 | 256.182 | -37.946 | 1.845 | -1.888 | -4.044 | â |
| Hunt & Reffert | 2024 | 256.189 | -37.941 | 1.885 | -1.881 | -4.05 | -5.662 |
| Cavallo et al. | 2024 | 256.195 | -37.947 | 1.886 | â | â | â |
| Hunt & Reffert | 2023 | 256.189 | -37.941 | 1.885 | -1.881 | -4.05 | -5.662 |
| Qin et al. | 2023 | 256.17 | -37.95 | 1.88 | -1.9 | -4.06 | -4.8 |
| Just et al. | 2023 | 256.16 | -37.98 | â | â | â | â |
| He et al. | 2022 | 256.18 | -37.946 | 1.884 | -1.902 | -4.051 | â |
| Tarricq et al. | 2022 | 256.205 | -37.938 | 1.888 | -1.899 | -4.049 | â |
| Jaehnig et al. | 2021 | 256.191 | -37.955 | 1.91 | -1.833 | -4.039 | â |
| Rain et al. | 2021 | 256.179 | -37.948 | 1.873 | -1.856 | -4.017 | â |
| Dias et al. | 2021 | 256.181 | -37.952 | 1.876 | -1.871 | -4.005 | -6.415 |
| Cantat-Gaudin et al. | 2020 | 256.179 | -37.948 | 1.873 | -1.856 | -4.017 | â |
| Cantat-Gaudin & Anders | 2020 | 256.179 | -37.948 | 1.873 | -1.856 | -4.017 | â |
| Liu & Pang | 2019 | 256.169 | -37.943 | 1.882 | -1.897 | -3.989 | â |
| Soubiran et al. | 2018 | 256.179 | -37.948 | â | â | â | -5.0 |
| Bica et al. | 2019 | 256.166 | -37.945 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 256.179 | -37.948 | 1.873 | -1.856 | -4.017 | â |
| Loktin & Popova | 2017 | 256.17 | -37.986 | â | -6.478 | -3.407 | -15.4 |
| Kharchenko et al. | 2016 | 256.16 | -37.98 | â | â | â | â |
| Dias et al. | 2014 | 256.171 | -37.985 | â | -2.27 | -2.71 | â |
| Kharchenko et al. | 2013 | 256.17 | -37.98 | â | -2.96 | -3.75 | -15.4 |
| Gozha et al. | 2012 | 256.171 | -37.985 | â | â | â | â |
| Piskunov et al. | 2008 | 256.155 | -37.989 | â | â | â | â |
| Kharchenko et al. | 2007 | 256.17 | -37.99 | â | 0.45 | â | -15.43 |
| Piskunov et al. | 2007 | 256.155 | -37.989 | â | â | â | â |
| van den Bergh | 2006 | 256.175 | -37.983 | â | â | â | â |
| Kharchenko et al. | 2005 | 256.17 | -37.99 | â | -2.96 | -3.75 | -15.43 |
| Kharchenko et al. | 2003 | 256.17 | -37.95 | â | -3.33 | -3.85 | â |
| Chen et al. | 2003 | 256.173 | -37.987 | â | â | â | â |
| Dias et al. | 2002 | 256.171 | -37.985 | â | -2.14 | -2.97 | -5.58 |
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 | 0.52 | 0.46 | 0.8 | 316 | 0.043 | 214 | 0.46 | 0.0 |
| Li et al. | 2025 | 0.53 | 0.43 | â | 472 | 0.144 | â | â | â |
| Wei et al. | 2025 | 0.62 | 0.57 | â | 275 | 0.250 | 1061 | 0.46 | â |
| Almeida et al. | 2025 | 0.52 | 0.63 | â | 328 | â | 988 | â | â |
| Alfonso et al. | 2024 | 0.54 | 0.30 | â | 648 | 0.044 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1414(1) | â | â |
| Cavallo et al. | 2024 | 0.53 | 0.82 | â | 186 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 0.50 | 0.37 | 0.80 | 274 | â | â | â | â |
| Qin et al. | 2023 | 0.66 | 0.62 | â | 224 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 316 | â | 26 | â | â |
| He et al. | 2022 | â | 0.75 | â | 282 | â | â | â | â |
| Tarricq et al. | 2022 | 0.53 | â | â | 513 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.52(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.53 | 0.43 | â | 309 | â | â | â | 0 |
| Dias et al. | 2021 | 0.52 | 0.63 | â | 328 | 0.042 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.54 | 0.30 | â | 513 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.53 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 269 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 0.53 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.53 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.50 | 0.46 | â | 313 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.51 | 0.60 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.51 | 0.60 | â | 316 | 0.000 | â | â | â |
| Gozha et al. | 2012 | 0.48 | â | â | 314 | 0.000 | 162 | â | â |
| Piskunov et al. | 2008 | 0.49 | 0.46 | â | 324 | â | 214(1) | â | â |
| Piskunov et al. | 2007 | 0.49 | 0.46 | â | 324 | â | 101 | â | â |
| van den Bergh | 2006 | 0.48 | 0.46 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.49 | 0.46 | â | 324 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.48 | 0.46 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.48 | 0.46 | â | 310 | 0.000(1) | â | â | â |
| Dias et al. | 2002 | 0.48 | 0.46 | â | 314 | 0.000 | 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. Gold sample.
Cavallo et al. (2024)
Gold sample.