NGC 2362
(MWSC 1173; FoF 671)
0.95
UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.4 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 2362 is a very rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Relatively close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 109.68 | -24.953 | 0.767 | -2.778 | 2.987 | 34.408 |
| Li et al. | 2025 | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | β |
| Almeida et al. | 2025 | 109.672 | -24.949 | β | β | β | β |
| Hunt & Reffert | 2024 | 109.672 | -24.952 | 0.774 | -2.763 | 2.974 | 42.196 |
| Celli et al. | 2024 | 109.671 | -24.954 | β | β | β | β |
| Cavallo et al. | 2024 | 109.693 | -24.967 | 0.778 | β | β | β |
| Hunt & Reffert | 2023 | 109.672 | -24.952 | 0.774 | -2.763 | 2.974 | 42.196 |
| Just et al. | 2023 | 109.674 | -24.958 | β | β | β | β |
| Jaehnig et al. | 2021 | 109.673 | -24.933 | 0.786 | -2.783 | 2.916 | β |
| Rain et al. | 2021 | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | β |
| Dias et al. | 2021 | 109.672 | -24.949 | 0.743 | -2.779 | 2.95 | β |
| Cantat-Gaudin et al. | 2020 | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | β |
| SΓ‘nchez et al. | 2020 | 109.671 | -24.955 | β | -2.688 | 2.931 | β |
| Cantat-Gaudin & Anders | 2020 | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | β |
| Liu & Pang | 2019 | 109.666 | -24.931 | 0.748 | -2.769 | 2.952 | β |
| Dias et al. | 2019 | 109.671 | 24.954 | 0.742 | -2.791 | 2.953 | 28.86 |
| Soubiran et al. | 2018 | 109.671 | -24.954 | β | β | β | 28.86 |
| Cantat-Gaudin et al. | 2018 | 109.671 | -24.954 | 0.742 | -2.791 | 2.953 | β |
| Loktin & Popova | 2017 | 109.68 | -24.96 | β | -3.539 | 1.159 | 29.5 |
| Kharchenko et al. | 2016 | 109.674 | -24.958 | β | β | β | β |
| Dias et al. | 2014 | 109.671 | -24.955 | β | -2.81 | 2.23 | β |
| Kharchenko et al. | 2013 | 109.68 | -24.96 | β | -2.6 | 2.34 | 29.5 |
| Gozha et al. | 2012 | 109.671 | -24.955 | β | β | β | β |
| Piskunov et al. | 2008 | 109.66 | -24.984 | β | β | β | β |
| Kharchenko et al. | 2007 | 109.66 | -24.95 | β | 0.25 | β | 25.33 |
| Piskunov et al. | 2007 | 109.66 | -24.984 | β | β | β | β |
| van den Bergh | 2006 | 109.65 | -24.983 | β | β | β | β |
| Kharchenko et al. | 2005 | 109.66 | -24.99 | β | -2.25 | 2.47 | 25.33 |
| Kharchenko et al. | 2003 | 109.66 | -24.99 | β | -2.36 | 2.64 | β |
| Chen et al. | 2003 | 109.729 | -24.951 | β | -2.29 | 3.03 | 42.2 |
| Dias et al. | 2002 | 109.671 | -24.955 | β | -2.29 | 3.03 | 36.43 |
| Dambis | 1999 | 109.671 | -24.955 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.03 | 0.32 | β | 9 | -0.344 | β | β | β |
| Almeida et al. | 2025 | 1.23 | 0.43 | β | 14 | β | 547 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 389* | β | β |
| Celli et al. | 2024 | β | β | β | 6 | β | 592 | β | β |
| Cavallo et al. | 2024 | 1.19 | 0.30 | β | 5 | 0.030 | β | β | β |
| Hunt & Reffert | 2023 | 1.22 | 0.38 | 1.35 | 7 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 4 | β | 362 | β | β |
| Jaehnig et al. | 2021 | 1.27* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.30 | 0.31 | β | 5 | β | β | β | 0 |
| Dias et al. | 2021 | 1.23 | 0.43 | β | 14 | -0.104 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.34 | 0.37 | β | 6 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.30 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 8 | 0.500 | β | β | β |
| Dias et al. | 2019 | 1.28 | 0.53 | β | 7 | -1.112 | β | β | β |
| Soubiran et al. | 2018 | 1.30 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.30 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.39 | 0.30 | β | 8 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.38 | 0.52 | β | 4 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.38 | 0.52 | β | 4 | β | β | β | β |
| Gozha et al. | 2012 | 1.48 | β | β | 5 | β | 1000 | β | β |
| Piskunov et al. | 2008 | 1.39 | 0.31 | β | 4 | β | 319* | β | β |
| Piskunov et al. | 2007 | 1.39 | 0.31 | β | 4 | β | 71 | β | β |
| van den Bergh | 2006 | 1.39 | 0.31 | β | 8 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.39 | 0.31 | β | 4 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.39 | 0.31 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.39 | β | β | 0 | β | β | β | β |
| Dias et al. | 2002 | 1.48 | 0.31 | β | 5 | β | β | β | β |
| Dambis | 1999 | 1.28 | 0.34 | β | 10 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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