NGC 7058

(MWSC 3501; FoF 2419; OCSN 242)

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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

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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

Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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 –
Almeida et al. 2025 320.432 50.823 – – – –
Alfonso et al. 2024 320.523 50.818 2.71 7.439 2.737 –
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 – – –
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 –
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 –
Donor et al. 2020 320.423 50.82 – 7.41 2.76 -19.1
Cantat-Gaudin & Anders 2020 320.448 50.822 2.73 7.432 2.889 –
Liu & Pang 2019 320.418 50.829 2.729 7.444 2.901 –
Bossini et al. 2019 320.448 50.822 – – – –
Soubiran et al. 2018 320.448 50.822 – – – -16.78
Bica et al. 2019 320.405 50.834 – – – –
Cantat-Gaudin et al. 2018 320.448 50.822 2.73 7.432 2.889 –
Dias et al. 2014 320.471 50.818 – -2.1 -4.63 –
Piskunov et al. 2008 320.472 50.819 – – – –
Kharchenko et al. 2005 320.47 50.82 – 7.33 3.18 –

💡 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 – 57 0.500 173 0.37 –
Almeida et al. 2025 0.36 0.14 – 208 – 32 – –
Alfonso et al. 2024 0.35 0.18 – 79 0.115 – – –
Hunt & Reffert 2024 – – – – – 274* – –
Cavallo et al. 2024 0.38 0.57 – 21 -0.030 – – –
Hunt & Reffert 2023 0.36 0.13 0.68 70 – – – –
Qin et al. 2023 0.46 0.40 – 50 – – – –
He et al. 2022 – 0.55 – 50 – – – –
Dias et al. 2021 0.36 0.14 – 208 0.116 – – –
Cantat-Gaudin et al. 2020 0.35 0.18 – 41 – – – –
Donor et al. 2020 – – – – 0.030 – – –
Cantat-Gaudin & Anders 2020 0.36 – – – – – – –
Liu & Pang 2019 – – – 41 0.000 – – –
Bossini et al. 2019 0.36 0.26 – 40 0.000 – – –
Soubiran et al. 2018 0.36 – – – – – – –
Cantat-Gaudin et al. 2018 0.36 – – – – – – –
Piskunov et al. 2008 0.40 0.19 – 224 – – – –
Kharchenko et al. 2005 0.40 0.19 – 224 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1124 1.0 324.77 50.26 2.83 7.14 1.77 -16.92 0.03

💡 Note: The % column shows the percentage of members that NGC 7058 shares with each listed object.

Visualization

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