NGC 381
(MWSC 105; FoF 2128)
0.92
UTI
0.84
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
7.7 [arcmin]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 381 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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
Moderate 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 | â | 17.095 | 61.585 | 0.852 | 1.588 | -2.301 | -24.323 |
| Li et al. | 2025 | 17.094 | 61.586 | 0.847 | 1.602 | -2.263 | â |
| Hu & Soubiran | 2025 | 17.099 | 61.588 | â | â | â | â |
| Wei et al. | 2025 | 17.074 | 61.599 | 0.851 | 1.606 | -2.342 | â |
| Almeida et al. | 2025 | 17.089 | 61.594 | â | â | â | â |
| Zhang et al. | 2024 | 17.104 | 61.584 | â | â | â | â |
| Hunt & Reffert | 2024 | 17.104 | 61.584 | 0.856 | 1.6 | -2.318 | -21.94 |
| Cavallo et al. | 2024 | 17.099 | 61.588 | 0.853 | â | â | â |
| Hunt & Reffert | 2023 | 17.104 | 61.584 | 0.856 | 1.6 | -2.318 | -21.94 |
| Almeida et al. | 2023 | 17.098 | 61.6 | â | â | â | â |
| Just et al. | 2023 | 17.097 | 61.576 | â | â | â | â |
| He et al. | 2022 | 17.09 | 61.586 | 0.855 | 1.599 | -2.33 | â |
| Tarricq et al. | 2022 | 17.109 | 61.578 | 0.859 | 1.6 | -2.347 | â |
| Jaehnig et al. | 2021 | 17.101 | 61.586 | 0.878 | 1.609 | -2.261 | â |
| Rain et al. | 2021 | 17.094 | 61.586 | 0.847 | 1.602 | -2.263 | â |
| Dias et al. | 2021 | 17.089 | 61.594 | 0.845 | 1.6 | -2.257 | â |
| Cantat-Gaudin et al. | 2020 | 17.094 | 61.586 | 0.847 | 1.602 | -2.263 | â |
| Cantat-Gaudin & Anders | 2020 | 17.094 | 61.586 | 0.847 | 1.602 | -2.263 | â |
| Liu & Pang | 2019 | 17.085 | 61.597 | 0.854 | 1.599 | -2.254 | â |
| Bossini et al. | 2019 | 17.094 | 61.586 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 17.094 | 61.586 | 0.847 | 1.602 | -2.263 | â |
| Loktin & Popova | 2017 | 17.085 | 61.583 | â | -1.213 | -1.246 | -22.0 |
| Kharchenko et al. | 2016 | 17.097 | 61.576 | â | â | â | â |
| Dias et al. | 2014 | 17.079 | 61.583 | â | -0.22 | 0.11 | â |
| Kharchenko et al. | 2013 | 17.107 | 61.579 | â | 0.22 | -2.07 | -22.0 |
| Gozha et al. | 2012 | 17.079 | 61.584 | â | â | â | â |
| Kharchenko et al. | 2012 | 17.107 | 61.579 | â | 0.22 | -2.07 | -22.0 |
| Piskunov et al. | 2008 | 17.083 | 61.596 | â | â | â | â |
| Kharchenko et al. | 2007 | 17.08 | 61.58 | â | 0.1 | â | -22.0 |
| van den Bergh | 2006 | 17.083 | 61.584 | â | â | â | â |
| Kharchenko et al. | 2005 | 17.08 | 61.6 | â | 0.81 | -1.51 | -22.0 |
| Kharchenko et al. | 2003 | 17.07 | 61.58 | â | -0.16 | -0.39 | â |
| Chen et al. | 2003 | 17.061 | 61.587 | â | â | â | â |
| Dias et al. | 2002 | 17.079 | 61.583 | â | -0.22 | 0.11 | -29.76 |
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 | 1.07 | 1.13 | â | 591 | -0.027 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.090* | â | â | â |
| Wei et al. | 2025 | 2.63 | 1.56 | â | 501 | 0.500 | 655 | 0.39 | â |
| Almeida et al. | 2025 | 1.10 | 1.38 | â | 427 | â | 455 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.134* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 808* | â | â |
| Cavallo et al. | 2024 | 1.17 | 1.19 | â | 562 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 1.11 | 1.23 | 0.80 | 237 | â | â | â | â |
| Almeida et al. | 2023 | 1.12 | 1.44 | â | 353 | -0.011 | 369* | 0.51 | â |
| Just et al. | 2023 | â | â | â | 708 | â | 82 | â | â |
| He et al. | 2022 | â | 1.50 | â | 251 | â | â | â | â |
| Tarricq et al. | 2022 | 1.14 | â | â | 427 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.14* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.14 | 1.24 | â | 316 | â | â | â | 0 |
| Dias et al. | 2021 | 1.10 | 1.38 | â | 427 | 0.105 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.17 | 0.93 | â | 380 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.14 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 363 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 1.27 | 1.04 | â | 500 | 0.070 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.14 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.09 | 1.05 | â | 362 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.20 | 1.05 | â | 708 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.20 | 1.05 | â | 708 | 0.070 | â | â | â |
| Gozha et al. | 2012 | 1.15 | â | â | 320 | 0.020 | 33 | â | â |
| Kharchenko et al. | 2012 | 1.20 | 1.05 | â | 708 | 0.070 | â | â | â |
| Piskunov et al. | 2008 | 1.06 | 1.05 | â | 589 | â | â | â | â |
| van den Bergh | 2006 | 1.15 | 1.24 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.06 | 1.05 | â | 589 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.05 | 1.05 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.15 | 1.24 | â | 320 | 0.070* | â | â | â |
| Dias et al. | 2002 | 1.15 | 1.24 | â | 320 | 0.070 | â | â | â |
(*): 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.