Platais 10
(MWSC 2150; HIP 67014 Group; OCSN 253)
0.85
UTI
0.64
CN
1.0
Cdens
0.62
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
44.7 [arcmin]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Platais 10 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Low mass
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 | 205.132 | -59.271 | 4.179 | -30.326 | -10.145 | -16.819 |
| Li et al. | 2025 | 205.22 | -59.271 | 4.158 | -30.591 | -10.215 | â |
| Almeida et al. | 2025 | 205.009 | -59.404 | â | â | â | â |
| Alfonso et al. | 2024 | 205.833 | -59.234 | 4.104 | -30.038 | -10.599 | â |
| Hunt & Reffert | 2024 | 205.279 | -59.156 | 4.134 | -29.312 | -10.788 | -15.328 |
| Cavallo et al. | 2024 | 207.372 | -58.923 | 4.141 | â | â | â |
| Hunt & Reffert | 2023 | 205.279 | -59.156 | 4.134 | -29.312 | -10.788 | -15.328 |
| Qin et al. | 2023 | 205.36 | -59.21 | 4.15 | -30.28 | -10.7 | -16.97 |
| Just et al. | 2023 | 205.279 | -59.222 | â | â | â | â |
| He et al. | 2022 | 205.502 | -59.258 | 4.175 | -30.316 | -10.335 | â |
| Tarricq et al. | 2022 | 205.326 | -59.189 | 4.184 | -30.155 | -10.404 | â |
| Dias et al. | 2021 | 205.009 | -59.404 | 4.141 | -30.632 | -10.241 | -16.049 |
| Cantat-Gaudin et al. | 2020 | 205.22 | -59.271 | 4.158 | -30.591 | -10.215 | â |
| Cantat-Gaudin & Anders | 2020 | 205.22 | -59.271 | 4.158 | -30.591 | -10.215 | â |
| Bossini et al. | 2019 | 205.22 | -59.271 | â | â | â | â |
| Soubiran et al. | 2018 | 205.22 | -59.271 | â | â | â | -16.83 |
| Bica et al. | 2019 | 205.861 | -59.13 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 205.22 | -59.271 | 4.158 | -30.591 | -10.215 | â |
| Yen et al. | 2018 | 205.461 | -59.13 | 4.02 | -30.51 | -10.52 | â |
| Kharchenko et al. | 2016 | 205.279 | -59.222 | â | â | â | â |
| Dias et al. | 2014 | 205.867 | -59.122 | â | -3.26 | -4.01 | â |
| Kharchenko et al. | 2013 | 205.29 | -59.225 | â | -29.9 | -10.7 | -8.0 |
| Gozha et al. | 2012 | 205.867 | -59.122 | â | â | â | â |
| Piskunov et al. | 2008 | 205.414 | -59.206 | â | â | â | â |
| Kharchenko et al. | 2007 | 205.86 | -59.12 | â | 2.0 | â | -8.0 |
| van den Bergh | 2006 | 205.867 | -59.122 | â | â | â | â |
| Kharchenko et al. | 2005 | 205.42 | -59.21 | â | -29.1 | -10.73 | -8.0 |
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 | 0.22 | 0.39 | â | 133 | -0.167 | â | â | â |
| Almeida et al. | 2025 | 0.24 | 0.42 | â | 206 | â | 21 | â | â |
| Alfonso et al. | 2024 | 0.24 | 0.22 | â | 81 | -0.053 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 43* | â | â |
| Cavallo et al. | 2024 | 0.25 | 0.84 | â | 91 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.24 | 0.28 | 0.69 | 124 | â | â | â | â |
| Qin et al. | 2023 | 0.21 | 0.03 | â | 447 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 219 | â | 30 | â | â |
| He et al. | 2022 | â | 0.50 | â | 112 | â | â | â | â |
| Tarricq et al. | 2022 | 0.24 | â | â | 112 | â | â | â | â |
| Dias et al. | 2021 | 0.24 | 0.42 | â | 206 | -0.053 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.24 | 0.22 | â | 110 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.24 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.24 | 0.28 | â | 92 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.24 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.24 | â | â | â | â | â | â | â |
| Yen et al. | 2018 | 0.23 | 0.29 | â | 195 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.25 | 0.24 | â | 219 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.25 | 0.24 | â | 219 | â | â | â | â |
| Gozha et al. | 2012 | 0.25 | â | â | 100 | â | 1479 | â | â |
| Piskunov et al. | 2008 | 0.25 | 0.25 | â | 158 | â | â | â | â |
| van den Bergh | 2006 | 0.25 | â | â | 100 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.25 | 0.25 | â | 158 | â | 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.
Cavallo et al. (2024)
Gold sample.