NGC 2428

(MWSC 1297; FoF 1412)

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0.90 UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 7.9 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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NGC 2428 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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

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 – 114.835 -16.551 0.721 -3.299 2.485 53.583
Li et al. 2025 114.831 -16.55 0.706 -3.316 2.461 –
Hu & Soubiran 2025 114.823 -16.552 – – – –
Almeida et al. 2025 114.823 -16.554 – – – –
Hunt & Reffert 2024 114.852 -16.534 0.721 -3.298 2.492 51.722
Cavallo et al. 2024 114.823 -16.552 0.722 – – –
Hunt & Reffert 2023 114.852 -16.534 0.721 -3.298 2.492 51.722
Almeida et al. 2023 114.822 -16.55 – – – –
Just et al. 2023 114.827 -16.516 – – – –
Tarricq et al. 2022 114.813 -16.533 0.708 -3.296 2.49 –
Dias et al. 2021 114.823 -16.554 0.712 -3.309 2.461 52.788
Cantat-Gaudin et al. 2020 114.831 -16.55 0.706 -3.316 2.461 –
SΓ‘nchez et al. 2020 114.838 -16.528 – -3.2 2.417 –
Cantat-Gaudin & Anders 2020 114.831 -16.55 0.706 -3.316 2.461 –
Liu & Pang 2019 114.808 -16.521 0.715 -3.293 2.429 –
Soubiran et al. 2018 114.831 -16.55 – – – 52.88
Bica et al. 2019 114.828 -16.521 – – – –
Cantat-Gaudin et al. 2018 114.831 -16.55 0.706 -3.316 2.461 –
Loktin & Popova 2017 114.825 -16.518 – -2.895 0.322 47.3
Kharchenko et al. 2016 114.827 -16.516 – – – –
Dias et al. 2014 114.838 -16.528 – -3.05 1.9 47.35
Kharchenko et al. 2013 114.832 -16.518 – -1.72 0.87 47.3
Piskunov et al. 2008 114.847 -16.533 – – – –
Kharchenko et al. 2005 114.85 -16.53 – -2.02 1.12 –

πŸ’‘ 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
Li et al. 2025 1.28 0.38 – 853 -0.152 – – –
Hu & Soubiran 2025 – – – – -0.160* – – –
Almeida et al. 2025 1.26 0.32 – 743 – 408 – –
Hunt & Reffert 2024 – – – – – 687* – –
Cavallo et al. 2024 1.33 0.19 – 794 0.400 – – –
Hunt & Reffert 2023 1.28 0.12 0.43 944 – – – –
Almeida et al. 2023 1.30 0.27 – 773 -0.030 461* 0.55 –
Just et al. 2023 – – – 412 – 21 – –
Tarricq et al. 2022 1.29 – – 741 – – – –
Dias et al. 2021 1.26 0.32 – 743 -0.043 – – –
Cantat-Gaudin et al. 2020 1.32 0.32 – 724 – – – –
Cantat-Gaudin & Anders 2020 1.36 – – – – – – –
Liu & Pang 2019 – – – 447 0.250 – – –
Soubiran et al. 2018 1.36 – – – – – – –
Cantat-Gaudin et al. 2018 1.36 – – – – – – –
Loktin & Popova 2017 1.89 0.15 – 562 – – – –
Kharchenko et al. 2016 1.41 0.58 – 412 – – – –
Kharchenko et al. 2013 1.41 0.58 – 412 -0.145 – – –
Piskunov et al. 2008 2.10 0.16 – 479 – – – –
Kharchenko et al. 2005 2.10 0.16 – 479 – – – –

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

Visualization

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