NGC 7082
(MWSC 3517; OCL 209; FoF 2070)
0.93
UTI
0.9
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
10.2 [arcmin]
- CN 0.9 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7082 is a very rich, very dense object of high C3 quality. Its parallax locates it at a relatively 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 metallicity parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 322.19 | 47.107 | 0.728 | -0.298 | -1.172 | -11.84 |
| Li et al. | 2025 | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | â |
| Wei et al. | 2025 | 322.16 | 47.099 | 0.738 | -0.28 | -1.175 | â |
| Almeida et al. | 2025 | 322.18 | 47.099 | â | â | â | â |
| Hunt & Reffert | 2024 | 322.165 | 47.101 | 0.729 | -0.291 | -1.184 | -10.947 |
| Cavallo et al. | 2024 | 322.182 | 47.098 | 0.729 | â | â | â |
| Hunt & Reffert | 2023 | 322.165 | 47.101 | 0.729 | -0.291 | -1.184 | -10.947 |
| Almeida et al. | 2023 | 322.187 | 47.104 | â | â | â | â |
| Just et al. | 2023 | 322.194 | 47.106 | â | â | â | â |
| Tarricq et al. | 2022 | 322.128 | 47.107 | 0.732 | -0.3 | -1.181 | â |
| Jaehnig et al. | 2021 | 322.175 | 47.106 | 0.765 | -0.29 | -1.108 | â |
| Rain et al. | 2021 | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | â |
| Dias et al. | 2021 | 322.18 | 47.099 | 0.732 | -0.297 | -1.1 | -15.075 |
| Cantat-Gaudin et al. | 2020 | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | â |
| Cantat-Gaudin & Anders | 2020 | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | â |
| Liu & Pang | 2019 | 322.196 | 47.102 | 0.726 | -0.281 | -1.119 | â |
| Soubiran et al. | 2018 | 322.186 | 47.103 | â | â | â | -24.85 |
| Bica et al. | 2019 | 322.347 | 47.081 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | â |
| Loktin & Popova | 2017 | 322.32 | 47.127 | â | -1.9 | -2.32 | -9.1 |
| Kharchenko et al. | 2016 | 322.194 | 47.106 | â | â | â | â |
| Dias et al. | 2014 | 322.321 | 47.127 | â | -1.9 | -2.32 | â |
| Kharchenko et al. | 2013 | 322.2 | 47.11 | â | -1.03 | -2.12 | -9.1 |
| Gozha et al. | 2012 | 322.321 | 47.127 | â | â | â | â |
| Kharchenko et al. | 2012 | 322.2 | 47.11 | â | -1.03 | -2.12 | -9.1 |
| Piskunov et al. | 2008 | 322.244 | 47.125 | â | â | â | â |
| Kharchenko et al. | 2007 | 322.32 | 47.13 | â | 0.35 | â | -9.1 |
| Piskunov et al. | 2007 | 322.244 | 47.125 | â | â | â | â |
| van den Bergh | 2006 | 322.25 | 47.133 | â | â | â | â |
| Kharchenko et al. | 2005 | 322.24 | 47.13 | â | -1.56 | -3.55 | -9.1 |
| Kharchenko et al. | 2003 | 322.2 | 47.1 | â | -1.88 | -2.84 | â |
| Chen et al. | 2003 | 322.307 | 47.124 | â | â | â | â |
| Dias et al. | 2002 | 322.321 | 47.127 | â | -1.9 | -2.32 | -9.1 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.22 | 0.80 | â | 201 | -0.043 | â | â | â |
| Wei et al. | 2025 | 1.39 | 0.55 | â | 100 | 0.500 | 942 | 0.49 | â |
| Almeida et al. | 2025 | 1.28 | 1.01 | â | 136 | â | 1044 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1174* | â | â |
| Cavallo et al. | 2024 | 1.32 | 0.72 | â | 288 | 0.410 | â | â | â |
| Hunt & Reffert | 2023 | 1.30 | 0.74 | 0.57 | 147 | â | â | â | â |
| Almeida et al. | 2023 | 1.29 | 0.98 | â | 168 | 0.028 | 847* | 0.46 | â |
| Just et al. | 2023 | â | â | â | 100 | â | 407 | â | â |
| Tarricq et al. | 2022 | 1.30 | â | â | 65 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.31* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.32 | 0.71 | â | 170 | â | â | â | 0 |
| Dias et al. | 2021 | 1.28 | 1.01 | â | 136 | -0.015 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.34 | 0.79 | â | 62 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.32 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 132 | -0.250 | â | â | â |
| Soubiran et al. | 2018 | 1.32 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.32 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.44 | 0.73 | â | 171 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.30 | 0.74 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.30 | 0.74 | â | 100 | -0.010 | â | â | â |
| Gozha et al. | 2012 | 1.44 | â | â | 171 | -0.010 | 3981 | â | â |
| Kharchenko et al. | 2012 | 1.30 | 0.74 | â | 100 | -0.010 | â | â | â |
| Piskunov et al. | 2008 | 1.44 | 0.74 | â | 81 | â | 1589* | â | â |
| Piskunov et al. | 2007 | 1.44 | 0.74 | â | 81 | â | 441 | â | â |
| van den Bergh | 2006 | 1.44 | 0.74 | â | 170 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.44 | 0.74 | â | 81 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.44 | 0.74 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.44 | 0.73 | â | 170 | -0.010* | â | â | â |
| Dias et al. | 2002 | 1.44 | 0.73 | â | 171 | -0.010 | â | â | â |
(*): 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.
Cavallo et al. (2024)
Gold sample.