NGC 7063
(Collinder 435; MWSC 3507; OCL 192; FoF 2274; LISC 3389)
0.96
UTI
0.78
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Nm (P>50%)
187
Core radius and density
1.5 [pc], 7.7 [pc-2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7063 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below 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, metallicity, and mass parameters (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 | 321.103 | 36.504 | 1.492 | 1.516 | -2.543 | -1.911 |
| Malhotra et al. | 2026 | 321.126 | 36.496 | â | â | â | â |
| Li et al. | 2025 | 321.122 | 36.507 | 1.477 | 1.524 | -2.482 | â |
| Almeida et al. | 2025 | 321.103 | 36.499 | â | â | â | â |
| Alfonso et al. | 2024 | 321.123 | 36.511 | 1.464 | 1.513 | -2.524 | â |
| Zhang et al. | 2024 | 321.117 | 36.489 | â | â | â | â |
| Hunt & Reffert | 2024 | 321.117 | 36.489 | 1.492 | 1.533 | -2.548 | -2.175 |
| Cavallo et al. | 2024 | 321.114 | 36.507 | 1.493 | â | â | â |
| Hunt & Reffert | 2023 | 321.117 | 36.489 | 1.492 | 1.533 | -2.548 | -2.175 |
| Almeida et al. | 2023 | 321.108 | 36.491 | â | â | â | â |
| Cordoni et al. | 2023 | 321.103 | 36.499 | 1.483 | 1.524 | -2.453 | â |
| Just et al. | 2023 | 321.129 | 36.492 | â | â | â | â |
| He et al. | 2022 | 321.116 | 36.488 | 1.493 | 1.506 | -2.524 | â |
| Tarricq et al. | 2022 | 321.107 | 36.478 | 1.493 | 1.512 | -2.524 | â |
| Jaehnig et al. | 2021 | 321.138 | 36.511 | 1.507 | 1.525 | -2.461 | â |
| Rain et al. | 2021 | 321.122 | 36.507 | 1.477 | 1.524 | -2.482 | â |
| Richer et al. | 2021 | 321.106 | 36.487 | 1.489 | 1.544 | -2.466 | â |
| Dias et al. | 2021 | 321.103 | 36.499 | 1.483 | 1.524 | -2.453 | 5.945 |
| Cantat-Gaudin et al. | 2020 | 321.122 | 36.507 | 1.477 | 1.524 | -2.482 | â |
| Zhong et al. | 2020 | 321.122 | 36.507 | â | 1.524 | -2.482 | 0.197 |
| Cantat-Gaudin & Anders | 2020 | 321.122 | 36.507 | 1.477 | 1.524 | -2.482 | â |
| Liu & Pang | 2019 | 321.117 | 36.49 | 1.479 | 1.505 | -2.454 | â |
| Bossini et al. | 2019 | 321.122 | 36.507 | â | â | â | â |
| Soubiran et al. | 2018 | 321.122 | 36.507 | â | â | â | 4.43 |
| Bica et al. | 2019 | 321.069 | 36.504 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 321.122 | 36.507 | 1.477 | 1.524 | -2.482 | â |
| Dias et al. | 2018 | â | â | â | -1.21 | -2.78 | â |
| Dib et al. | 2018 | 321.135 | 36.495 | â | â | â | â |
| Loktin & Popova | 2017 | 321.09 | 36.487 | â | -0.088 | -0.715 | â |
| Sampedro et al. | 2017 | 321.087 | 36.487 | â | â | â | â |
| Joshi et al. | 2016 | 321.135 | 36.495 | â | â | â | â |
| Kharchenko et al. | 2016 | 321.129 | 36.492 | â | â | â | â |
| Dias et al. | 2014 | 321.087 | 36.487 | â | -1.07 | -2.53 | â |
| Kharchenko et al. | 2013 | 321.135 | 36.495 | â | 0.77 | -2.4 | â |
| Bukowiecki et al. | 2011 | 321.121 | 36.528 | â | â | â | â |
| Piskunov et al. | 2008 | 321.087 | 36.49 | â | â | â | â |
| Piskunov et al. | 2007 | 321.087 | 36.49 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 321.1 | 36.483 | â | â | â | â |
| van den Bergh | 2006 | 321.1 | 36.483 | â | â | â | â |
| Kharchenko et al. | 2005 | 321.09 | 36.49 | â | 1.24 | -2.83 | â |
| Kharchenko et al. | 2003 | 321.1 | 36.49 | â | 1.56 | -2.76 | â |
| Dias et al. | 2002 | 321.087 | 36.487 | â | -1.07 | -2.53 | â |
| Lynga | 1987 | 321.13 | 36.497 | â | â | â | â |
| Sulentic et al. | 1973 | 321.106 | 36.491 | 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 | 0.66 | 0.285 | 0.47 | 102 | -0.009 | 147 | 0.465 | 0 |
| Malhotra et al. | 2026 | 0.67 | 0.35 | â | 75 | -0.090 | â | â | â |
| Liu et al. | 2025 | 0.76 | 0.11 | â | 89 | â | â | â | â |
| Li et al. | 2025 | 0.67 | 0.36 | â | 89 | 0.035 | â | â | â |
| Almeida et al. | 2025 | 0.66 | 0.37 | â | 150 | â | 147 | â | â |
| Alfonso et al. | 2024 | 0.66 | 0.23 | â | 86 | -0.009 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.231(1) | â | â | â |
| Hunt & Reffert | 2024 | 0.63 | 0.13 | 0.47 | 147 | â | 318(1) | â | â |
| Cavallo et al. | 2024 | 0.65 | 0.27 | â | 182 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.63 | 0.13 | 0.47 | 148 | â | â | â | â |
| Almeida et al. | 2023 | 0.66 | 0.33 | â | 154 | 0.002 | 131(1) | 0.53 | â |
| Cordoni et al. | 2023 | 0.66 | 0.37 | â | 150 | -0.009 | 244 | 0.40 | 0(1) |
| Deng & Li | 2023 | 0.55 | 0.32 | â | 300 | -0.105 | â | â | â |
| Just et al. | 2023 | â | â | â | 90 | â | 24 | â | â |
| He et al. | 2022 | â | 0.40 | â | 71 | â | â | â | â |
| Tarricq et al. | 2022 | 0.65 | â | â | 102 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.66(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.66 | 0.32 | â | 186 | â | â | â | 0 |
| Richer et al. | 2021 | â | 0.38 | â | 98 | â | â | â | â |
| Dias et al. | 2021 | 0.66 | 0.37 | â | 150 | -0.009 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.66 | 0.23 | â | 98 | â | â | â | â |
| Kounkel et al. | 2020 | 0.65 | 0.34 | â | 123 | â | â | â | â |
| Zhong et al. | 2020 | 0.66(1) | 0.33 | â | 8274 | -0.072 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.66 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 52 | -0.250 | â | â | â |
| Bossini et al. | 2019 | 0.66 | 0.33 | â | 188 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.66 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.66 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 0.69 | â | â | 90 | â | â | â | â |
| Loktin & Popova | 2017 | 0.70 | 0.29 | â | 105 | â | â | â | â |
| Joshi et al. | 2016 | 0.69 | 0.28 | â | 90 | â | 151 | â | â |
| Kharchenko et al. | 2016 | 0.69 | 0.28 | â | 90 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.69 | 0.28 | â | 90 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 711 | â | â |
| Bukowiecki et al. | 2011 | 0.70(1) | 0.41 | â | 79 | â | â | â | â |
| Piskunov et al. | 2008 | 0.69 | 0.28 | â | 120 | â | 102(1) | â | â |
| Piskunov et al. | 2007 | 0.69 | 0.28 | â | 120 | â | 27 | â | â |
| Ahumada & Lapasset | 2007 | â | 0.28 | â | 95 | â | â | â | 0 |
| van den Bergh | 2006 | 0.69 | 0.28 | â | 95 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.69 | 0.28 | â | 120 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.69 | 0.28 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.69 | 0.29 | â | 95 | â | â | â | â |
| Lynga | 1987 | 0.66 | 0.22 | â | 141 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Malhotra et al. (2026)
Lowest/Highest stellar mass in the catalogue with a mass-ratio estimate: 0.34/4.12 Msun
Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 295 along with UPK_113.
Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P238, along with UPK_113.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Richer et al. (2021)
The expected number of WDs is 1.8, 0 WD candidates found, and 1 WD candidate found in the wide search.
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1001, e_all=0.0562.
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=8.274, Av=0.326, [Fe/H]=0.000 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108).
Ahumada & Lapasset (2007)
Only the photoelectric data of (1961PUSNO..17..343H) were examined.