NGC 7039
(Collinder 431; MWSC 3474; OCL 203)
0.91
UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
70.5 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7039 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near 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 absorption and age 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 | 317.664 | 45.598 | 1.321 | -0.26 | -2.582 | -7.62 |
| Li et al. | 2025 | 317.663 | 45.597 | 1.293 | -0.32 | -2.542 | â |
| Wei et al. | 2025 | 317.745 | 45.612 | 1.32 | -0.225 | -2.588 | â |
| Almeida et al. | 2025 | 317.662 | 45.595 | â | â | â | â |
| Alfonso et al. | 2024 | 317.696 | 45.577 | 1.287 | -0.239 | -2.6 | â |
| Swiggum et al. | 2024 | 317.653 | 45.582 | 1.318 | -0.24 | -2.626 | -9.628 |
| Hunt & Reffert | 2024 | 317.653 | 45.582 | 1.318 | -0.24 | -2.626 | -7.442 |
| Celli et al. | 2024 | 317.663 | 45.597 | â | â | â | â |
| Cavallo et al. | 2024 | 317.699 | 45.61 | 1.319 | â | â | â |
| Hunt & Reffert | 2023 | 317.653 | 45.582 | 1.318 | -0.24 | -2.626 | -7.442 |
| Almeida et al. | 2023 | 317.655 | 45.586 | â | â | â | â |
| Just et al. | 2023 | 317.757 | 45.73 | â | â | â | â |
| He et al. | 2022 | 317.681 | 45.596 | 1.311 | -0.254 | -2.595 | â |
| Rain et al. | 2021 | 317.663 | 45.597 | 1.293 | -0.32 | -2.542 | â |
| Richer et al. | 2021 | 317.651 | 45.629 | 1.298 | -0.342 | -2.536 | â |
| Dias et al. | 2021 | 317.662 | 45.595 | 1.29 | -0.249 | -2.544 | -8.512 |
| Cantat-Gaudin et al. | 2020 | 317.663 | 45.597 | 1.293 | -0.32 | -2.542 | â |
| Cantat-Gaudin & Anders | 2020 | 317.663 | 45.597 | 1.293 | -0.32 | -2.542 | â |
| Soubiran et al. | 2018 | 317.663 | 45.597 | â | â | â | -10.59 |
| Bica et al. | 2019 | 317.755 | 45.65 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 317.663 | 45.597 | 1.293 | -0.32 | -2.542 | â |
| Loktin & Popova | 2017 | 317.7 | 45.617 | â | -1.316 | -0.227 | -11.6 |
| Kharchenko et al. | 2016 | 317.757 | 45.73 | â | â | â | â |
| Dias et al. | 2014 | 317.7 | 45.617 | â | -2.43 | -2.21 | â |
| Kharchenko et al. | 2013 | 317.763 | 45.733 | â | -3.29 | -0.48 | -11.6 |
| Gozha et al. | 2012 | 317.7 | 45.617 | â | â | â | â |
| Bukowiecki et al. | 2011 | 317.683 | 45.599 | â | â | â | â |
| Piskunov et al. | 2008 | 317.695 | 45.621 | â | â | â | â |
| Kharchenko et al. | 2007 | 317.7 | 45.62 | â | 0.28 | â | -11.6 |
| Ahumada & Lapasset | 2007 | 317.7 | 45.617 | â | â | â | â |
| van den Bergh | 2006 | 317.7 | 45.617 | â | â | â | â |
| Kharchenko et al. | 2005 | 317.7 | 45.62 | â | -1.68 | -4.69 | -11.0 |
| Kharchenko et al. | 2003 | 317.8 | 45.67 | â | -1.87 | -5.14 | â |
| Dias et al. | 2002 | 317.7 | 45.617 | â | -0.48 | -2.99 | -12.2 |
| Lynga | 1987 | 317.805 | 45.659 | â | â | â | â |
| Sulentic et al. | 1973 | 318.05 | 45.653 | 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 | 0.78 | 0.41 | 1.09 | 44 | -0.015 | 314 | 0.55 | 0 |
| Liu et al. | 2025 | 0.81 | 0.15 | â | 15 | â | â | â | â |
| Li et al. | 2025 | 0.68 | 0.38 | â | 13 | -0.052 | â | â | â |
| Wei et al. | 2025 | 0.80 | 1.02 | â | 6 | 0.000 | 815 | 0.70 | â |
| Almeida et al. | 2025 | 0.76 | 0.56 | â | 16 | â | 314 | â | â |
| Alfonso et al. | 2024 | 0.76 | 0.28 | â | 18 | 0.091 | â | â | â |
| Swiggum et al. | 2024 | 0.74 | â | â | 7 | â | 266 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 183(1) | â | â |
| Celli et al. | 2024 | â | â | â | 22 | â | 215 | â | â |
| Cavallo et al. | 2024 | 0.78 | 0.98 | â | 5 | -0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.73 | 0.26 | 1.09 | 7 | â | â | â | â |
| Almeida et al. | 2023 | 0.74 | 0.52 | â | 13 | -0.031 | 218(1) | 0.40 | â |
| Just et al. | 2023 | â | â | â | 452 | â | 793 | â | â |
| He et al. | 2022 | â | 0.10 | â | 8 | â | â | â | â |
| Rain et al. | 2021 | 0.76 | 0.41 | â | 66 | â | â | â | 0 |
| Richer et al. | 2021 | â | 0.82 | â | 12 | â | â | â | â |
| Dias et al. | 2021 | 0.76 | 0.56 | â | 16 | 0.091 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.76 | 0.28 | â | 22 | â | â | â | â |
| Kounkel et al. | 2020 | 0.80 | 0.85 | â | 93 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.76 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 0.76 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.76 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.96 | 0.40 | â | 70 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.55 | 0.70 | â | 452 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.55 | 0.70 | â | 452 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 420 | â | â |
| Gozha et al. | 2012 | 0.95 | â | â | 66 | â | 589 | â | â |
| Bukowiecki et al. | 2011 | 0.82(1) | 0.19 | â | 79 | â | â | â | â |
| Piskunov et al. | 2008 | 0.95 | 0.41 | â | 676 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 0.41 | â | 66 | â | â | â | 0 |
| van den Bergh | 2006 | 0.95 | 0.41 | â | 66 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.95 | 0.41 | â | 676 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.95 | 0.41 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.95 | 0.41 | â | 66 | â | â | â | â |
| Lynga | 1987 | 0.70 | 0.38 | â | 126 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 294 along with OC_0140.
Palma et al. (2025)
Part of multiple system G220, along with OC_0140 and Theia_26.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Ahumada & Lapasset (2007)
According to (1987A&AS...67..545S) there would be two clusters: the first one at 700 pc, and the second one at 1500 pc.