NGC 2428
(MWSC 1297; FoF 1412)
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
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
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 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 | β |
| Hu & Soubiran | 2025 | 114.823 | -16.552 | β | β | β | β |
| Almeida et al. | 2025 | 114.823 | -16.554 | β | β | β | β |
| 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 | β | β | β |
| Hunt & Reffert | 2023 | 114.852 | -16.534 | 0.721 | -3.298 | 2.492 | 51.722 |
| Almeida et al. | 2023 | 114.822 | -16.55 | β | β | β | β |
| Just et al. | 2023 | 114.827 | -16.516 | β | β | β | β |
| Tarricq et al. | 2022 | 114.813 | -16.533 | 0.708 | -3.296 | 2.49 | β |
| 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 | β |
| SΓ‘nchez et al. | 2020 | 114.838 | -16.528 | β | -3.2 | 2.417 | β |
| Cantat-Gaudin & Anders | 2020 | 114.831 | -16.55 | 0.706 | -3.316 | 2.461 | β |
| Liu & Pang | 2019 | 114.808 | -16.521 | 0.715 | -3.293 | 2.429 | β |
| Soubiran et al. | 2018 | 114.831 | -16.55 | β | β | β | 52.88 |
| Bica et al. | 2019 | 114.828 | -16.521 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 114.831 | -16.55 | 0.706 | -3.316 | 2.461 | β |
| Loktin & Popova | 2017 | 114.825 | -16.518 | β | -2.895 | 0.322 | 47.3 |
| Kharchenko et al. | 2016 | 114.827 | -16.516 | β | β | β | β |
| Dias et al. | 2014 | 114.838 | -16.528 | β | -3.05 | 1.9 | 47.35 |
| Kharchenko et al. | 2013 | 114.832 | -16.518 | β | -1.72 | 0.87 | 47.3 |
| Piskunov et al. | 2008 | 114.847 | -16.533 | β | β | β | β |
| Kharchenko et al. | 2005 | 114.85 | -16.53 | β | -2.02 | 1.12 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.28 | 0.38 | β | 853 | -0.152 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.160* | β | β | β |
| Almeida et al. | 2025 | 1.26 | 0.32 | β | 743 | β | 408 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 687* | β | β |
| Cavallo et al. | 2024 | 1.33 | 0.19 | β | 794 | 0.400 | β | β | β |
| Hunt & Reffert | 2023 | 1.28 | 0.12 | 0.43 | 944 | β | β | β | β |
| Almeida et al. | 2023 | 1.30 | 0.27 | β | 773 | -0.030 | 461* | 0.55 | β |
| Just et al. | 2023 | β | β | β | 412 | β | 21 | β | β |
| Tarricq et al. | 2022 | 1.29 | β | β | 741 | β | β | β | β |
| Dias et al. | 2021 | 1.26 | 0.32 | β | 743 | -0.043 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.32 | 0.32 | β | 724 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.36 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 447 | 0.250 | 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 | 1.89 | 0.15 | β | 562 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.41 | 0.58 | β | 412 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.41 | 0.58 | β | 412 | -0.145 | β | β | β |
| Piskunov et al. | 2008 | 2.10 | 0.16 | β | 479 | β | β | β | β |
| Kharchenko et al. | 2005 | 2.10 | 0.16 | β | 479 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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