Melotte 179
(Collinder 349; IC 4665; MWSC 2689; OCL 85; FoF 2432; OCSN 206)
0.97
UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
33.1 [N/pc2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 179 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age 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 | 266.568 | 5.576 | 2.897 | -0.851 | -8.533 | -15.003 |
| Li et al. | 2025 | 266.554 | 5.615 | 2.868 | -0.909 | -8.52 | â |
| Wei et al. | 2025 | 266.518 | 5.622 | 2.904 | -0.864 | -8.532 | â |
| Almeida et al. | 2025 | 266.554 | 5.58 | â | â | â | â |
| Alfonso et al. | 2024 | 266.597 | 5.595 | 2.855 | -0.838 | -8.521 | â |
| Zhang et al. | 2024 | 266.532 | 5.635 | â | â | â | â |
| Hunt & Reffert | 2024 | 266.532 | 5.635 | 2.867 | -0.881 | -8.532 | -17.295 |
| Cavallo et al. | 2024 | 266.588 | 5.56 | 2.877 | â | â | â |
| Hunt & Reffert | 2023 | 266.532 | 5.635 | 2.867 | -0.881 | -8.532 | -17.295 |
| Almeida et al. | 2023 | 266.671 | 5.502 | â | â | â | â |
| Qin et al. | 2023 | 266.47 | 5.7 | 2.88 | -0.89 | -8.54 | -14.74 |
| Just et al. | 2023 | 266.558 | 5.694 | â | â | â | â |
| He et al. | 2022 | 266.512 | 5.597 | 2.9 | -0.87 | -8.555 | â |
| Jaehnig et al. | 2021 | 266.543 | 5.658 | 2.909 | -0.942 | -8.494 | â |
| Rain et al. | 2021 | 266.554 | 5.615 | 2.868 | -0.909 | -8.52 | â |
| Dias et al. | 2021 | 266.554 | 5.58 | 2.86 | -0.896 | -8.504 | -14.142 |
| Cantat-Gaudin et al. | 2020 | 266.554 | 5.615 | 2.868 | -0.909 | -8.52 | â |
| Cantat-Gaudin & Anders | 2020 | 266.554 | 5.615 | 2.868 | -0.909 | -8.52 | â |
| Liu & Pang | 2019 | 266.438 | 5.681 | 2.896 | -0.905 | -8.477 | â |
| Bossini et al. | 2019 | 266.554 | 5.615 | â | â | â | â |
| Soubiran et al. | 2018 | 266.554 | 5.615 | â | â | â | -14.4 |
| Bica et al. | 2019 | 266.551 | 5.665 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 266.554 | 5.615 | 2.868 | -0.909 | -8.52 | â |
| Loktin & Popova | 2017 | 266.58 | 5.717 | â | -0.86 | -8.1 | -12.2 |
| Kharchenko et al. | 2016 | 266.558 | 5.694 | â | â | â | â |
| Dias et al. | 2014 | 266.575 | 5.717 | â | 1.45 | -4.95 | â |
| Kharchenko et al. | 2013 | 266.565 | 5.695 | â | -0.6 | -8.0 | -12.2 |
| Gozha et al. | 2012 | 266.575 | 5.717 | â | â | â | â |
| Piskunov et al. | 2008 | 266.577 | 5.716 | â | â | â | â |
| Kharchenko et al. | 2007 | 266.58 | 5.72 | â | 1.0 | â | -10.26 |
| Piskunov et al. | 2007 | 266.577 | 5.716 | â | â | â | â |
| van den Bergh | 2006 | 266.575 | 5.717 | â | â | â | â |
| Kharchenko et al. | 2005 | 266.58 | 5.72 | â | -0.57 | -7.4 | -10.26 |
| Kharchenko et al. | 2003 | 266.53 | 5.66 | â | -0.3 | -6.76 | â |
| Chen et al. | 2003 | 266.55 | 5.708 | â | -0.99 | -7.77 | -13.0 |
| Dias et al. | 2002 | 266.575 | 5.717 | â | -0.86 | -8.1 | -15.95 |
| Dambis | 1999 | 266.575 | 5.717 | â | â | â | â |
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 | 0.35 | 0.53 | 0.98 | 42 | -0.004 | 255 | 0.5 | 0.0 |
| Li et al. | 2025 | 0.35 | 0.56 | â | 42 | 0.057 | â | â | â |
| Wei et al. | 2025 | 0.43 | 0.87 | â | 41 | 0.000 | 285 | 0.21 | â |
| Almeida et al. | 2025 | 0.33 | 0.71 | â | 53 | â | 190 | â | â |
| Alfonso et al. | 2024 | 0.35 | 0.45 | â | 35 | -0.004 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.019(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 251(1) | â | â |
| Cavallo et al. | 2024 | 0.36 | 0.94 | â | 22 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 0.34 | 0.56 | 0.98 | 33 | â | â | â | â |
| Almeida et al. | 2023 | 0.31 | 0.51 | â | 204 | 0.112 | 308(1) | 0.79 | â |
| Qin et al. | 2023 | 0.46 | 0.71 | â | 28 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 43 | â | 56 | â | â |
| He et al. | 2022 | â | 0.90 | â | 35 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.34(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.35 | 0.37 | â | 38 | â | â | â | 0 |
| Dias et al. | 2021 | 0.33 | 0.71 | â | 53 | -0.005 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.35 | 0.45 | â | 33 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.35 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 33 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 0.31 | 0.40 | â | 38 | -0.030 | â | â | â |
| Soubiran et al. | 2018 | 0.35 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.35 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.35 | 0.54 | â | 43 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.35 | 0.53 | â | 43 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.35 | 0.53 | â | 43 | -0.030 | â | â | â |
| Gozha et al. | 2012 | 0.35 | â | â | 43 | -0.030 | 479 | â | â |
| Piskunov et al. | 2008 | 0.35 | 0.53 | â | 43 | â | 259(1) | â | â |
| Piskunov et al. | 2007 | 0.35 | 0.53 | â | 43 | â | 140 | â | â |
| van den Bergh | 2006 | 0.35 | 0.53 | â | 43 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.35 | 0.53 | â | 43 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.35 | 0.53 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.35 | â | â | 40 | â | â | â | â |
| Dias et al. | 2002 | 0.35 | 0.54 | â | 43 | -0.030 | â | â | â |
| Dambis | 1999 | 0.33 | 0.60 | â | 40 | â | 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.