NGC 7129
(MWSC 3549)
0.79
UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
79
Core radius and density
0.4 [pc], 61 [pc-2]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
NGC 7129 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. 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 | 99999â | 325.728 | 66.113 | 1.129 | -1.758 | -3.419 | -0.16 |
| Almeida et al. | 2025 | 325.782 | 66.134 | â | â | â | â |
| Alfonso et al. | 2024 | 325.723 | 66.135 | 1.079 | -1.818 | -3.45 | â |
| Hunt & Reffert | 2024 | 325.741 | 66.123 | 1.097 | -1.773 | -3.46 | -17.652 |
| Celli et al. | 2024 | 325.74 | 66.114 | â | â | â | â |
| Cavallo et al. | 2024 | 325.691 | 66.169 | 1.095 | â | â | â |
| Hunt & Reffert | 2023 | 325.741 | 66.123 | 1.097 | -1.773 | -3.46 | -17.652 |
| Just et al. | 2023 | 325.72 | 66.107 | â | â | â | â |
| He et al. | 2022 | 325.764 | 66.125 | 1.133 | -1.727 | -3.413 | â |
| Dias et al. | 2021 | 325.782 | 66.134 | 1.075 | -1.759 | -3.442 | â |
| Cantat-Gaudin et al. | 2020 | 325.74 | 66.114 | 1.086 | -1.759 | -3.267 | â |
| Cantat-Gaudin & Anders | 2020 | 325.74 | 66.114 | 1.086 | -1.759 | -3.267 | â |
| Cantat-Gaudin et al. | 2018 | 325.74 | 66.114 | 1.086 | -1.759 | -3.267 | â |
| Dias et al. | 2018 | â | â | â | -1.47 | -1.38 | â |
| Loktin & Popova | 2017 | 325.725 | 66.107 | â | 0.128 | -1.309 | â |
| Joshi et al. | 2016 | 325.725 | 66.11 | â | â | â | â |
| Kharchenko et al. | 2016 | 325.72 | 66.107 | â | â | â | â |
| Tadross | 2014 | 325.746 | 66.113 | â | â | â | â |
| Kharchenko et al. | 2013 | 325.725 | 66.11 | â | -1.41 | -3.97 | â |
| Kharchenko et al. | 2012 | 325.725 | 66.11 | â | -1.48 | -3.92 | â |
| Bukowiecki et al. | 2011 | 325.733 | 66.108 | â | â | â | â |
| Bica et al. | 2003 | 325.728 | 66.1 | â | â | â | â |
| Dias et al. | 2002 | 325.746 | 66.113 | â | -1.62 | -3.08 | â |
| Lynga | 1987 | 325.328 | 66.09 | â | â | â | â |
| Sulentic et al. | 1973 | 325.317 | 66.098 | 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 | 0.905 | 2.49 | 2.45 | 14 | 0.128 | 96 | â | â |
| Almeida et al. | 2025 | 0.89 | 2.20 | â | 6 | â | 93 | â | â |
| Alfonso et al. | 2024 | 0.87 | 1.78 | â | 20 | 0.128 | â | â | â |
| Hunt & Reffert | 2024 | 0.91 | 2.30 | 2.45 | 10 | â | 313(1) | â | â |
| Celli et al. | 2024 | â | â | â | 21 | â | 96 | â | â |
| Cavallo et al. | 2024 | 1.43 | 2.14 | â | 52 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.91 | 2.30 | 2.45 | 10 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 14 | â | 1 | â | â |
| He et al. | 2022 | â | 2.75 | â | 6 | â | â | â | â |
| Dias et al. | 2021 | 0.89 | 2.20 | â | 6 | 0.128 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.88 | 1.78 | â | 21 | â | â | â | â |
| Kounkel et al. | 2020 | 1.01 | 2.32 | â | 11 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.90 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.90 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.72 | 2.49 | â | 525 | â | â | â | â |
| Joshi et al. | 2016 | 1.05 | 4.43 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.05 | 4.43 | â | 14 | â | â | â | â |
| Tadross | 2014 | 1.07 | 3.06 | â | 120 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.05 | 4.43 | â | 14 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 105 | â | â |
| Kharchenko et al. | 2012 | 0.65 | 4.10 | â | 45 | â | â | â | â |
| Bukowiecki et al. | 2011 | 0.32(1) | 3.38 | â | 20 | â | â | â | â |
| Dias et al. | 2002 | 1.07 | 3.06 | â | 120 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as genetic pair P232, along with HSC_814.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Wood sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.06 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.06 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1872, e_all=0.1887.
Bica et al. (2003)
Classified as infrared cluster (IRC).