NGC 7031
(Collinder 430; FSR 0294; MWSC 3466; OCL 210)
0.92
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.91
Clit
1.0
Cdup
Stellar density (N50/rad)
39.9 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.91 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7031 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age 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 | 99999β | 316.809 | 50.863 | 0.721 | -1.251 | -4.274 | 2.419 |
| Hunt & Reffert | 2024 | 316.803 | 50.866 | 0.713 | -1.243 | -4.281 | 12.045 |
| Cavallo et al. | 2024 | 316.811 | 50.859 | 0.722 | β | β | β |
| Hunt & Reffert | 2023 | 316.803 | 50.866 | 0.713 | -1.243 | -4.281 | 12.045 |
| Just et al. | 2023 | 316.77 | 50.872 | β | β | β | β |
| Tarricq et al. | 2022 | 316.813 | 50.882 | 0.716 | -1.248 | -4.283 | β |
| Richer et al. | 2021 | 316.81 | 50.863 | 0.669 | -1.213 | -4.216 | β |
| Cantat-Gaudin et al. | 2020 | 316.809 | 50.87 | 0.704 | -1.242 | -4.205 | β |
| SΓ‘nchez et al. | 2020 | 316.8 | 50.875 | β | -1.291 | -4.396 | β |
| Cantat-Gaudin & Anders | 2020 | 316.809 | 50.87 | 0.704 | -1.242 | -4.205 | β |
| Soubiran et al. | 2018 | 316.809 | 50.87 | β | β | β | -4.16 |
| Bica et al. | 2019 | 316.833 | 50.834 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 316.809 | 50.87 | 0.704 | -1.242 | -4.205 | β |
| Loktin & Popova | 2017 | 316.8 | 50.875 | β | -0.68 | -1.207 | 0.2 |
| Kharchenko et al. | 2016 | 316.77 | 50.872 | β | β | β | β |
| Dias et al. | 2014 | 316.8 | 50.875 | β | -2.87 | -4.77 | β |
| Kharchenko et al. | 2013 | 316.774 | 50.875 | β | -1.95 | -4.01 | 0.2 |
| Gozha et al. | 2012 | 316.8 | 50.875 | β | β | β | β |
| Kharchenko et al. | 2012 | 316.774 | 50.875 | β | -1.95 | -4.01 | 0.24 |
| Bukowiecki et al. | 2011 | 316.754 | 50.879 | β | β | β | β |
| Froebrich et al. | 2007 | 316.688 | 50.857 | β | β | β | β |
| van den Bergh | 2006 | 316.803 | 50.882 | β | β | β | β |
| Dias et al. | 2002 | 316.8 | 50.875 | β | -2.87 | -4.77 | 0.24 |
| Lynga | 1987 | 316.833 | 50.834 | β | β | β | β |
| Sulentic et al. | 1973 | 316.829 | 50.835 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 1.1 | 2.6 | 2.78 | 141 | 0.730 | 377 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1403(1) | β | β |
| Cavallo et al. | 2024 | 1.72 | 3.23 | β | 31 | 0.730 | β | β | β |
| Hunt & Reffert | 2023 | 1.32 | 3.23 | 2.78 | 23 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 158 | β | 48 | β | β |
| Tarricq et al. | 2022 | 1.40 | β | β | 186 | β | β | β | β |
| Richer et al. | 2021 | β | 1.46 | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.45 | 2.14 | β | 155 | β | β | β | β |
| Kounkel et al. | 2020 | 1.33 | 2.59 | β | 112 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.36 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 1.36 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.36 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 0.94 | 2.80 | β | 157 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.10 | 2.60 | β | 158 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.10 | 2.60 | β | 158 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 377 | β | β |
| Gozha et al. | 2012 | 0.90 | β | β | 137 | β | β | β | β |
| Kharchenko et al. | 2012 | 1.10 | 2.60 | β | 158 | β | β | β | β |
| Bukowiecki et al. | 2011 | 0.87(1) | 2.18 | β | 141 | β | β | β | β |
| van den Bergh | 2006 | 0.90 | 2.68 | β | 138 | β | β | β | β |
| Dias et al. | 2002 | 0.90 | 2.69 | β | 137 | β | β | β | β |
| Lynga | 1987 | 1.00 | 2.49 | β | 56 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.64 (50th percentile).