Trumpler 10
(MWSC 1567; FoF 2411; OCSN 276)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
28.6 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 10 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption and mass parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 131.917 | -42.48 | 2.298 | -12.405 | 6.563 | 21.166 |
| Li et al. | 2025 | 131.943 | -42.566 | 2.287 | -12.532 | 6.527 | â |
| Wei et al. | 2025 | 131.791 | -42.382 | 2.3 | -12.353 | 6.574 | â |
| Almeida et al. | 2025 | 132.009 | -42.604 | â | â | â | â |
| Alfonso et al. | 2024 | 132.013 | -42.65 | 2.281 | -12.468 | 6.584 | â |
| Hunt & Reffert | 2024 | 131.937 | -42.534 | 2.295 | -12.38 | 6.571 | 19.995 |
| Cavallo et al. | 2024 | 131.888 | -42.452 | 2.297 | â | â | â |
| Hunt & Reffert | 2023 | 131.937 | -42.534 | 2.295 | -12.38 | 6.571 | 19.995 |
| Qin et al. | 2023 | 131.93 | -42.5 | 2.3 | -12.63 | 6.52 | 20.82 |
| Just et al. | 2023 | 131.868 | -42.396 | â | â | â | â |
| He et al. | 2022 | 136.687 | -47.103 | 2.327 | -13.098 | 6.25 | â |
| Jaehnig et al. | 2021 | 131.986 | -42.547 | 2.294 | -12.375 | 6.492 | â |
| Rain et al. | 2021 | 131.943 | -42.566 | 2.287 | -12.532 | 6.527 | â |
| Dias et al. | 2021 | 132.009 | -42.604 | 2.282 | -12.529 | 6.517 | 21.984 |
| Cantat-Gaudin et al. | 2020 | 131.943 | -42.566 | 2.287 | -12.532 | 6.527 | â |
| Cantat-Gaudin & Anders | 2020 | 131.943 | -42.566 | 2.287 | -12.532 | 6.527 | â |
| Liu & Pang | 2019 | 131.83 | -42.447 | 2.255 | -12.354 | 6.5 | â |
| Dias et al. | 2019 | 131.975 | -42.45 | 2.263 | -12.385 | 6.465 | 20.183 |
| Bossini et al. | 2019 | 131.943 | -42.566 | â | â | â | â |
| Soubiran et al. | 2018 | 131.943 | -42.566 | â | â | â | 22.43 |
| Cantat-Gaudin et al. | 2018 | 131.943 | -42.566 | 2.287 | -12.532 | 6.527 | â |
| Loktin & Popova | 2017 | 131.97 | -42.45 | â | -6.558 | 7.674 | 32.17 |
| Kharchenko et al. | 2016 | 131.868 | -42.396 | â | â | â | â |
| Dias et al. | 2014 | 131.975 | -42.45 | â | -4.59 | 3.75 | â |
| Kharchenko et al. | 2013 | 131.872 | -42.4 | â | -12.0 | 6.9 | 15.0 |
| Gozha et al. | 2012 | 131.975 | -42.45 | â | â | â | â |
| Piskunov et al. | 2008 | 131.913 | -42.448 | â | â | â | â |
| Kharchenko et al. | 2007 | 131.97 | -42.45 | â | 0.75 | â | 15.0 |
| Piskunov et al. | 2007 | 131.913 | -42.448 | â | â | â | â |
| van den Bergh | 2006 | 131.925 | -42.45 | â | â | â | â |
| Kharchenko et al. | 2005 | 131.92 | -42.45 | â | -11.9 | 6.05 | 15.0 |
| Kharchenko et al. | 2003 | 131.88 | -42.48 | â | -11.79 | 6.24 | â |
| Chen et al. | 2003 | 131.905 | -42.504 | â | -13.4 | 7.04 | 21.5 |
| Dias et al. | 2002 | 131.975 | -42.45 | â | -12.06 | 6.6 | 32.17 |
| Dambis | 1999 | 131.975 | -42.45 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.42 | 0.09 | 0.54 | 35 | 0.072 | 653 | 0.53 | 0.0 |
| Li et al. | 2025 | 0.45 | 0.17 | â | 48 | 0.156 | â | â | â |
| Wei et al. | 2025 | 0.39 | 0.02 | â | 50 | 0.250 | 725 | 0.53 | â |
| Almeida et al. | 2025 | 0.43 | 0.19 | â | 57 | â | 653 | â | â |
| Alfonso et al. | 2024 | 0.43 | 0.00 | â | 40 | 0.045 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 715(1) | â | â |
| Cavallo et al. | 2024 | 0.45 | 0.41 | â | 17 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 0.42 | 0.08 | 0.54 | 37 | â | â | â | â |
| Qin et al. | 2023 | 0.44 | 0.06 | â | 71 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 24 | â | 16 | â | â |
| He et al. | 2022 | â | 0.30 | â | 40 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.44(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.43 | 0.09 | â | 35 | â | â | â | 0 |
| Dias et al. | 2021 | 0.43 | 0.19 | â | 57 | 0.043 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.43 | 0.00 | â | 32 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.43 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 50 | 0.250 | â | â | â |
| Dias et al. | 2019 | 0.44 | 0.16 | â | 42 | 0.223 | â | â | â |
| Bossini et al. | 2019 | 0.37 | 0.14 | â | 55 | -0.120 | â | â | â |
| Soubiran et al. | 2018 | 0.43 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.43 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.42 | 0.11 | â | 35 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.42 | 0.09 | â | 24 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.42 | 0.09 | â | 24 | â | â | â | â |
| Gozha et al. | 2012 | 0.42 | â | â | 35 | -0.130 | 490 | â | â |
| Piskunov et al. | 2008 | 0.42 | 0.09 | â | 24 | â | 746(1) | â | â |
| Piskunov et al. | 2007 | 0.42 | 0.09 | â | 24 | â | 406 | â | â |
| van den Bergh | 2006 | 0.42 | 0.09 | â | 35 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.42 | 0.09 | â | 24 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.36 | 0.09 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.42 | â | â | 30 | â | â | â | â |
| Dias et al. | 2002 | 0.42 | 0.11 | â | 35 | -0.130 | â | â | â |
| Dambis | 1999 | 0.36 | 0.11 | â | 32 | â | â | â | â |
(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.
Cavallo et al. (2024)
Gold sample.