Melotte 158
(Collinder 322; VDBH 209; NGC 6259; MWSC 2511; OCL 996; vdBergh-Hagen 209; ESO 277 22)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1891
Stellar density (N50/rad)
76.0 [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 158 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, 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.
Note: This object shares a very small percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 255.194 | -44.68 | 0.42 | -1.038 | -2.895 | -34.401 |
| Wei et al. | 2025 | 255.193 | -44.686 | 0.422 | -1.039 | -2.899 | β |
| Almeida et al. | 2025 | 255.197 | -44.675 | β | β | β | β |
| Hunt & Reffert | 2024 | 255.193 | -44.677 | 0.424 | -1.047 | -2.893 | -35.597 |
| Cavallo et al. | 2024 | 255.2 | -44.681 | 0.424 | β | β | β |
| Hunt & Reffert | 2023 | 255.193 | -44.677 | 0.424 | -1.047 | -2.893 | -35.597 |
| Just et al. | 2023 | 255.214 | -44.69 | β | β | β | β |
| Jaehnig et al. | 2021 | 255.205 | -44.687 | 0.44 | -1.009 | -2.893 | β |
| Rain et al. | 2021 | 255.195 | -44.678 | 0.408 | -1.015 | -2.892 | β |
| Dias et al. | 2021 | 255.197 | -44.675 | 0.415 | -1.012 | -2.882 | -36.049 |
| Cantat-Gaudin et al. | 2020 | 255.195 | -44.678 | 0.408 | -1.015 | -2.892 | β |
| SΓ‘nchez et al. | 2020 | 255.188 | -44.655 | β | -0.994 | -2.857 | β |
| Cantat-Gaudin & Anders | 2020 | 255.195 | -44.678 | 0.408 | -1.015 | -2.892 | β |
| Soubiran et al. | 2018 | 255.195 | -44.678 | β | β | β | -32.84 |
| Bica et al. | 2019 | 255.174 | -44.657 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 255.195 | -44.678 | 0.408 | -1.015 | -2.892 | β |
| Loktin & Popova | 2017 | 255.195 | -44.656 | β | -4.431 | -8.397 | -33.7 |
| Kharchenko et al. | 2016 | 255.214 | -44.69 | β | β | β | β |
| Dias et al. | 2014 | 255.188 | -44.655 | β | 0.94 | -1.93 | β |
| Kharchenko et al. | 2013 | 255.225 | -44.69 | β | -1.87 | -5.27 | -33.7 |
| Gozha et al. | 2012 | 255.187 | -44.655 | β | β | β | β |
| Kharchenko et al. | 2007 | 255.19 | -44.65 | β | 0.12 | β | β |
| van den Bergh | 2006 | 255.175 | -44.667 | β | β | β | β |
| Chen et al. | 2003 | 255.176 | -44.671 | β | β | β | β |
| Dias et al. | 2002 | 255.188 | -44.655 | β | 1.04 | -1.88 | -34.66 |
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 | 1.85 | 1.88 | 1.28 | 265 | 0.020 | 4946 | 0.23 | 0.0 |
| Wei et al. | 2025 | 3.95 | 1.88 | β | 576 | 0.500 | 4835 | 0.23 | β |
| Almeida et al. | 2025 | 1.81 | 2.11 | β | 329 | β | 5056 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 17779(1) | β | β |
| Cavallo et al. | 2024 | 1.67 | 2.74 | β | 234 | -0.400 | β | β | β |
| Hunt & Reffert | 2023 | 2.17 | 2.34 | 1.28 | 164 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 299 | β | 323 | β | β |
| Jaehnig et al. | 2021 | 2.26(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.29 | 1.52 | β | 214 | β | β | β | 0 |
| Dias et al. | 2021 | 1.81 | 2.11 | β | 329 | 0.149 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.31 | 1.87 | β | 269 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.29 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.29 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.29 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.18 | 1.47 | β | 265 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.85 | 2.00 | β | 299 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.85 | 2.00 | β | 299 | 0.020 | β | β | β |
| Gozha et al. | 2012 | 1.03 | β | β | 217 | 0.020 | β | β | β |
| van den Bergh | 2006 | 1.03 | 1.55 | β | 219 | β | β | β | β |
| Chen et al. | 2003 | 1.03 | 1.54 | β | 210 | 0.020(1) | β | β | β |
| Dias et al. | 2002 | 1.03 | 1.54 | β | 217 | 0.020 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.