NGC 129
(MWSC 53; FoF 171)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
6.6 [arcmin]
- 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
NGC 129 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young 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.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 7.606 | 60.207 | 0.527 | -2.594 | -1.178 | -46.798 |
| Li et al. | 2025 | 7.607 | 60.213 | 0.511 | -2.605 | -1.096 | β |
| Wei et al. | 2025 | 7.762 | 60.355 | 0.515 | -2.498 | -1.128 | β |
| Almeida et al. | 2025 | 7.573 | 60.223 | β | β | β | β |
| Hunt & Reffert | 2024 | 7.59 | 60.206 | 0.525 | -2.586 | -1.177 | -48.212 |
| Cavallo et al. | 2024 | 7.608 | 60.208 | 0.527 | β | β | β |
| Hunt & Reffert | 2023 | 7.59 | 60.206 | 0.525 | -2.586 | -1.177 | -48.212 |
| Almeida et al. | 2023 | 7.55 | 60.243 | β | β | β | β |
| Just et al. | 2023 | 7.533 | 60.199 | β | β | β | β |
| Jaehnig et al. | 2021 | 7.604 | 60.208 | 0.538 | -2.595 | -1.105 | β |
| Rain et al. | 2021 | 7.607 | 60.213 | 0.511 | -2.605 | -1.096 | β |
| Dias et al. | 2021 | 7.573 | 60.223 | 0.513 | -2.604 | -1.096 | -38.787 |
| Cantat-Gaudin et al. | 2020 | 7.607 | 60.213 | 0.511 | -2.605 | -1.096 | β |
| SΓ‘nchez et al. | 2020 | 7.5 | 60.218 | β | -2.676 | -1.158 | β |
| Cantat-Gaudin & Anders | 2020 | 7.607 | 60.213 | 0.511 | -2.605 | -1.096 | β |
| Liu & Pang | 2019 | 7.591 | 60.218 | 0.507 | -2.593 | -1.115 | β |
| Soubiran et al. | 2018 | 7.607 | 60.213 | β | β | β | -37.89 |
| Cantat-Gaudin et al. | 2018 | 7.607 | 60.213 | 0.511 | -2.605 | -1.096 | β |
| Loktin & Popova | 2017 | 7.5 | 60.218 | β | 0.49 | -0.256 | -38.0 |
| Kharchenko et al. | 2016 | 7.533 | 60.199 | β | β | β | β |
| Dias et al. | 2014 | 7.5 | 60.218 | β | -1.23 | -0.51 | β |
| Kharchenko et al. | 2013 | 7.542 | 60.203 | β | -2.2 | -1.16 | -38.0 |
| Gozha et al. | 2012 | 7.5 | 60.218 | β | β | β | β |
| Kharchenko et al. | 2012 | 7.542 | 60.203 | β | -2.34 | -1.29 | -38.03 |
| Piskunov et al. | 2008 | 7.499 | 60.221 | β | β | β | β |
| Kharchenko et al. | 2007 | 7.5 | 60.22 | β | 0.27 | β | -43.21 |
| Piskunov et al. | 2007 | 7.499 | 60.221 | β | β | β | β |
| van den Bergh | 2006 | 7.5 | 60.217 | β | β | β | β |
| Kharchenko et al. | 2005 | 7.5 | 60.22 | β | -0.92 | -0.48 | -43.21 |
| Kharchenko et al. | 2003 | 7.47 | 60.22 | β | -1.77 | -0.92 | β |
| Chen et al. | 2003 | 7.569 | 60.164 | β | -1.86 | -1.7 | -36.8 |
| Dias et al. | 2002 | 7.5 | 60.218 | β | -1.23 | -0.51 | -37.36 |
| Dambis | 1999 | 7.5 | 60.218 | β | β | β | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.77 | 1.13 | β | 528 | 0.246 | β | β | β |
| Wei et al. | 2025 | 1.98 | 1.51 | β | 110 | 0.500 | 5981 | 0.68 | β |
| Almeida et al. | 2025 | 1.80 | 1.74 | β | 72 | β | 1846 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2588* | β | β |
| Cavallo et al. | 2024 | 1.89 | 1.80 | β | 102 | 0.410 | β | β | β |
| Hunt & Reffert | 2023 | 1.77 | 1.74 | 1.93 | 105 | β | β | β | β |
| Almeida et al. | 2023 | 1.72 | 1.85 | β | 92 | 0.002 | 1577* | 0.54 | β |
| Just et al. | 2023 | β | β | β | 94 | β | 103 | β | β |
| Jaehnig et al. | 2021 | 1.84* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.85 | 1.67 | β | 76 | β | β | β | 0 |
| Dias et al. | 2021 | 1.80 | 1.74 | β | 72 | 0.248 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.91 | 1.51 | β | 129 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.85 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 977 | -2.000 | β | β | β |
| Soubiran et al. | 2018 | 1.85 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.85 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.62 | 1.70 | β | 76 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.69 | 1.68 | β | 94 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.69 | 1.68 | β | 94 | β | β | β | β |
| Gozha et al. | 2012 | 1.62 | β | β | 77 | -0.460 | 1023 | β | β |
| Kharchenko et al. | 2012 | 1.69 | 1.68 | β | 94 | β | β | β | β |
| Piskunov et al. | 2008 | 1.62 | 1.71 | β | 74 | β | 964* | β | β |
| Piskunov et al. | 2007 | 1.62 | 1.71 | β | 74 | β | 205 | β | β |
| van den Bergh | 2006 | 1.62 | 1.71 | β | 78 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.62 | 1.71 | β | 74 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.64 | 1.71 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.62 | β | β | 70 | β | β | β | β |
| Dias et al. | 2002 | 1.62 | 1.70 | β | 77 | β | β | β | β |
| Dambis | 1999 | 1.56 | 1.57 | β | 89 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.