NGC 7380
0.90
UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.7 [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 7380 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 341.851 | 58.109 | 0.346 | -2.486 | -2.187 | -66.519 |
| Li et al. | 2025 | 341.817 | 58.125 | 0.333 | -2.517 | -2.144 | â |
| Almeida et al. | 2025 | 341.8 | 58.148 | â | â | â | â |
| Hunt & Reffert | 2024 | 341.921 | 58.099 | 0.342 | -2.464 | -2.194 | -80.095 |
| Celli et al. | 2024 | 341.817 | 58.125 | â | â | â | â |
| Cavallo et al. | 2024 | 341.855 | 58.112 | 0.347 | â | â | â |
| Hunt & Reffert | 2023 | 341.921 | 58.099 | 0.342 | -2.464 | -2.194 | -80.095 |
| Jaehnig et al. | 2021 | 341.842 | 58.087 | 0.355 | -2.79 | -2.226 | â |
| Rain et al. | 2021 | 341.817 | 58.125 | 0.333 | -2.517 | -2.144 | â |
| Dias et al. | 2021 | 341.8 | 58.148 | 0.331 | -2.499 | -2.134 | â |
| Cantat-Gaudin et al. | 2020 | 341.817 | 58.125 | 0.333 | -2.517 | -2.144 | â |
| Cantat-Gaudin & Anders | 2020 | 341.817 | 58.125 | 0.333 | -2.517 | -2.144 | â |
| Dias et al. | 2019 | 341.837 | 58.132 | 0.304 | -2.624 | -2.044 | -51.118 |
| Cantat-Gaudin et al. | 2018 | 341.817 | 58.125 | 0.333 | -2.517 | -2.144 | â |
| Loktin & Popova | 2017 | 341.835 | 58.132 | â | -1.023 | -0.321 | -34.1 |
| Dias et al. | 2014 | 341.837 | 58.132 | â | -1.31 | -4.46 | â |
| Gozha et al. | 2012 | 341.837 | 58.132 | â | â | â | â |
| Piskunov et al. | 2008 | 341.765 | 58.116 | â | â | â | â |
| Kharchenko et al. | 2007 | 341.83 | 58.13 | â | 0.25 | â | -34.13 |
| Piskunov et al. | 2007 | 341.765 | 58.116 | â | â | â | â |
| van den Bergh | 2006 | 341.775 | 58.117 | â | â | â | â |
| Kharchenko et al. | 2005 | 341.77 | 58.12 | â | -3.08 | -1.66 | -34.13 |
| Chen et al. | 2003 | 341.783 | 58.099 | â | -1.74 | -2.52 | -39.0 |
| Dias et al. | 2002 | 341.837 | 58.132 | â | -1.74 | -2.52 | -42.09 |
| Dambis | 1999 | 341.837 | 58.132 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.25 | 0.93 | â | 791 | 0.143 | â | â | â |
| Almeida et al. | 2025 | 2.39 | 1.85 | â | 10 | â | 357 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1306* | â | â |
| Celli et al. | 2024 | â | â | â | 4 | â | 811 | â | â |
| Cavallo et al. | 2024 | 2.45 | 1.80 | â | 9 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 2.70 | 1.85 | 2.25 | 9 | â | â | â | â |
| Jaehnig et al. | 2021 | 2.82* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.77 | 1.86 | â | 12 | â | â | â | 0 |
| Dias et al. | 2021 | 2.39 | 1.85 | â | 10 | -0.062 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.73 | 1.59 | â | 4 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.77 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 1.81 | 1.61 | â | 22 | -2.028 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.77 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.22 | 1.87 | â | 12 | â | â | â | â |
| Gozha et al. | 2012 | 2.22 | â | â | 12 | -0.420 | 4467 | â | â |
| Piskunov et al. | 2008 | 2.22 | 1.86 | â | 5 | â | 2729* | â | â |
| Piskunov et al. | 2007 | 2.22 | 1.86 | â | 5 | â | 451 | â | â |
| van den Bergh | 2006 | 2.22 | 1.86 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.22 | 1.86 | â | 5 | â | â | â | â |
| Chen et al. | 2003 | 2.22 | â | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 2.22 | 1.87 | â | 12 | â | â | â | â |
| Dambis | 1999 | 2.56 | 1.74 | â | 13 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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