NGC 7058
(MWSC 3501; FoF 2419; OCSN 242)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
29.0 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7058 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very 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, age, and metallicity parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 320.47 | 50.816 | 2.73 | 7.445 | 2.753 | -19.437 |
| Wei et al. | 2025 | 320.551 | 50.841 | 2.742 | 7.465 | 2.768 | â |
| Almeida et al. | 2025 | 320.432 | 50.823 | â | â | â | â |
| Alfonso et al. | 2024 | 320.523 | 50.818 | 2.71 | 7.439 | 2.737 | â |
| Hunt & Reffert | 2024 | 320.409 | 50.83 | 2.737 | 7.429 | 2.805 | -20.468 |
| Cavallo et al. | 2024 | 320.501 | 50.814 | 2.732 | â | â | â |
| Hunt & Reffert | 2023 | 320.409 | 50.83 | 2.737 | 7.429 | 2.805 | -20.468 |
| Qin et al. | 2023 | 320.45 | 50.82 | 2.73 | 7.42 | 2.83 | -19.08 |
| He et al. | 2022 | 320.365 | 50.767 | 2.742 | 7.442 | 2.763 | â |
| Dias et al. | 2021 | 320.432 | 50.823 | 2.73 | 7.4 | 2.894 | -16.614 |
| Cantat-Gaudin et al. | 2020 | 320.448 | 50.822 | 2.73 | 7.432 | 2.889 | â |
| Donor et al. | 2020 | 320.423 | 50.82 | â | 7.41 | 2.76 | -19.1 |
| Cantat-Gaudin & Anders | 2020 | 320.448 | 50.822 | 2.73 | 7.432 | 2.889 | â |
| Liu & Pang | 2019 | 320.418 | 50.829 | 2.729 | 7.444 | 2.901 | â |
| Bossini et al. | 2019 | 320.448 | 50.822 | â | â | â | â |
| Soubiran et al. | 2018 | 320.448 | 50.822 | â | â | â | -16.78 |
| Bica et al. | 2019 | 320.405 | 50.834 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 320.448 | 50.822 | 2.73 | 7.432 | 2.889 | â |
| Dias et al. | 2014 | 320.471 | 50.818 | â | -2.1 | -4.63 | â |
| Piskunov et al. | 2008 | 320.472 | 50.819 | â | â | â | â |
| Kharchenko et al. | 2005 | 320.47 | 50.82 | â | 7.33 | 3.18 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Wei et al. | 2025 | 0.37 | 0.03 | â | 57 | 0.500 | 173 | 0.37 | â |
| Almeida et al. | 2025 | 0.36 | 0.14 | â | 208 | â | 32 | â | â |
| Alfonso et al. | 2024 | 0.35 | 0.18 | â | 79 | 0.115 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 274* | â | â |
| Cavallo et al. | 2024 | 0.38 | 0.57 | â | 21 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.36 | 0.13 | 0.68 | 70 | â | â | â | â |
| Qin et al. | 2023 | 0.46 | 0.40 | â | 50 | â | â | â | â |
| He et al. | 2022 | â | 0.55 | â | 50 | â | â | â | â |
| Dias et al. | 2021 | 0.36 | 0.14 | â | 208 | 0.116 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.35 | 0.18 | â | 41 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | 0.030 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.36 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 41 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 0.36 | 0.26 | â | 40 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.36 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.36 | â | â | â | â | â | â | â |
| Piskunov et al. | 2008 | 0.40 | 0.19 | â | 224 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.40 | 0.19 | â | 224 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.