NGC 5381
(Ruprecht 109; VDBH 156; MWSC 2196; OCL 915; vdBergh-Hagen 156; ESO 133 11)
0.93
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.83
Clit
1.0
Cdup
Stellar density (N50/rad)
38.3 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.83 Well-studied
- Cdup 1.0 Unique
Overview
NGC 5381 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 210.222 | -59.576 | 0.389 | -6.062 | -2.924 | -38.09 |
| Li et al. | 2025 | 210.205 | -59.578 | 0.379 | -6.034 | -2.932 | β |
| Hu & Soubiran | 2025 | 210.226 | -59.581 | β | β | β | β |
| Almeida et al. | 2025 | 210.196 | -59.582 | β | β | β | β |
| Hunt & Reffert | 2024 | 210.22 | -59.578 | 0.39 | -6.073 | -2.919 | -29.414 |
| Cavallo et al. | 2024 | 210.226 | -59.581 | 0.39 | β | β | β |
| Hunt & Reffert | 2023 | 210.22 | -59.578 | 0.39 | -6.073 | -2.919 | -29.414 |
| Just et al. | 2023 | 210.153 | -59.602 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 210.205 | -59.578 | β | β | β | β |
| Dias et al. | 2021 | 210.196 | -59.582 | 0.379 | -6.034 | -2.921 | -38.379 |
| Cantat-Gaudin et al. | 2020 | 210.205 | -59.578 | 0.379 | -6.034 | -2.932 | β |
| SΓ‘nchez et al. | 2020 | 210.171 | -59.587 | β | -6.161 | -2.888 | β |
| Cantat-Gaudin & Anders | 2020 | 210.205 | -59.578 | 0.379 | -6.034 | -2.932 | β |
| Soubiran et al. | 2018 | 210.205 | -59.578 | β | β | β | -38.61 |
| Bica et al. | 2019 | 210.151 | -59.594 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 210.205 | -59.578 | 0.379 | -6.034 | -2.932 | β |
| Kharchenko et al. | 2016 | 210.153 | -59.602 | β | β | β | β |
| Tadross | 2014 | 210.171 | -59.587 | β | β | β | β |
| Dias et al. | 2014 | 210.171 | -59.587 | β | -1.77 | -4.92 | β |
| Kharchenko et al. | 2013 | 210.165 | -59.605 | β | -5.45 | 0.7 | β |
| Dias et al. | 2002 | 210.171 | -59.587 | β | -1.77 | -4.92 | β |
| Lynga | 1987 | 210.154 | -59.562 | β | β | β | β |
| van den Bergh & Hagen | 1975 | 209.275 | -59.317 | β | β | β | β |
| Sulentic et al. | 1973 | 210.138 | -59.554 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 2.34 | 1.615 | 1.58 | 447 | 0.187 | 2563 | β | 0 |
| Li et al. | 2025 | 2.34 | 1.47 | β | 533 | 0.254 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.160(5) | β | β | β |
| Almeida et al. | 2025 | 2.07 | 1.61 | β | 504 | β | 2055 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 4167(1) | β | β |
| Cavallo et al. | 2024 | 2.02 | 1.53 | β | 646 | 0.220 | β | β | β |
| Hunt & Reffert | 2023 | 2.32 | 1.63 | 1.58 | 253 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 447 | β | 218 | β | β |
| Jadhav & Subramaniam | 2021 | 2.34 | 1.62 | β | 355 | β | 3071 | β | 0(1) |
| Dias et al. | 2021 | 2.07 | 1.61 | β | 504 | 0.154 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.34 | 1.62 | β | 355 | β | β | β | β |
| Kounkel et al. | 2020 | 2.61 | 1.90 | β | 389 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.45 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.45 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.45 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.95 | 1.97 | β | 447 | β | β | β | β |
| Tadross | 2014 | 1.17 | 0.19 | β | 1600 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.95 | 1.97 | β | 447 | β | β | β | β |
| Dias et al. | 2002 | 2.63 | 1.45 | β | 251 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).