Trumpler 2
(Collinder 29; MWSC 219; OCL 365; FoF 2297)
0.96
UTI
0.8
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
15.3 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 2 is a rich, very dense object of very high C3 quality. Its parallax locates it at a 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 age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 39.247 | 55.927 | 1.445 | 1.531 | -5.406 | -7.248 |
| Li et al. | 2025 | 39.232 | 55.905 | 1.431 | 1.583 | -5.352 | â |
| Wei et al. | 2025 | 39.281 | 55.886 | 1.454 | 1.524 | -5.406 | â |
| Almeida et al. | 2025 | 39.239 | 55.894 | â | â | â | â |
| Alfonso et al. | 2024 | 38.967 | 55.958 | 1.397 | 1.462 | -5.223 | â |
| Zhang et al. | 2024 | 39.305 | 55.926 | â | â | â | â |
| Hunt & Reffert | 2024 | 39.305 | 55.926 | 1.455 | 1.54 | -5.411 | -8.322 |
| Cavallo et al. | 2024 | 38.956 | 55.889 | 1.448 | â | â | â |
| Hunt & Reffert | 2023 | 39.305 | 55.926 | 1.455 | 1.54 | -5.411 | -8.322 |
| Almeida et al. | 2023 | 39.267 | 55.895 | â | â | â | â |
| Just et al. | 2023 | 39.356 | 55.948 | â | â | â | â |
| He et al. | 2022 | 39.34 | 55.914 | 1.449 | 1.525 | -5.381 | â |
| Tarricq et al. | 2022 | 39.217 | 55.927 | 1.434 | 1.553 | -5.375 | â |
| Jaehnig et al. | 2021 | 39.255 | 55.934 | 1.456 | 1.56 | -5.302 | â |
| Rain et al. | 2021 | 39.232 | 55.905 | 1.431 | 1.583 | -5.352 | â |
| Dias et al. | 2021 | 39.239 | 55.894 | 1.435 | 1.581 | -5.343 | -3.99 |
| Cantat-Gaudin et al. | 2020 | 39.232 | 55.905 | 1.431 | 1.583 | -5.352 | â |
| Cantat-Gaudin & Anders | 2020 | 39.232 | 55.905 | 1.431 | 1.583 | -5.352 | â |
| Liu & Pang | 2019 | 39.222 | 55.966 | 1.441 | 1.574 | -5.323 | â |
| Bossini et al. | 2019 | 39.232 | 55.905 | â | â | â | â |
| Soubiran et al. | 2018 | 39.232 | 55.905 | â | â | â | -4.12 |
| Bica et al. | 2019 | 39.281 | 55.934 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 39.232 | 55.905 | 1.431 | 1.583 | -5.352 | â |
| Loktin & Popova | 2017 | 39.225 | 55.915 | â | 1.375 | -1.757 | -27.5 |
| Kharchenko et al. | 2016 | 39.356 | 55.948 | â | â | â | â |
| Dias et al. | 2014 | 39.221 | 55.915 | â | 0.11 | -3.49 | â |
| Kharchenko et al. | 2013 | 39.367 | 55.95 | â | 0.78 | -4.0 | -27.5 |
| Gozha et al. | 2012 | 39.221 | 55.915 | â | â | â | â |
| Kharchenko et al. | 2012 | 39.367 | 55.95 | â | 0.69 | -4.07 | -27.5 |
| Piskunov et al. | 2008 | 39.211 | 55.919 | â | â | â | â |
| Kharchenko et al. | 2007 | 39.22 | 55.92 | â | 0.5 | â | -27.5 |
| Piskunov et al. | 2007 | 39.211 | 55.919 | â | â | â | â |
| van den Bergh | 2006 | 39.225 | 55.917 | â | â | â | â |
| Kharchenko et al. | 2005 | 39.22 | 55.92 | â | 1.4 | -5.57 | -39.0 |
| Kharchenko et al. | 2003 | 39.22 | 55.92 | â | 0.72 | -5.6 | â |
| Chen et al. | 2003 | 39.31 | 55.971 | â | 1.36 | -5.13 | 2.4 |
| Dias et al. | 2002 | 39.221 | 55.915 | â | 0.11 | -3.49 | 2.4 |
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 | 0.66 | 0.85 | â | 342 | 0.052 | â | â | â |
| Wei et al. | 2025 | 1.08 | 1.36 | â | 68 | 0.000 | 726 | 0.35 | â |
| Almeida et al. | 2025 | 0.68 | 1.10 | â | 238 | â | 423 | â | â |
| Alfonso et al. | 2024 | 0.71 | 0.86 | â | 177 | 0.139 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.144* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 702* | â | â |
| Cavallo et al. | 2024 | 0.72 | 1.20 | â | 66 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 0.65 | 0.86 | 1.10 | 90 | â | â | â | â |
| Almeida et al. | 2023 | 0.67 | 1.19 | â | 106 | -0.042 | 498* | 0.47 | â |
| Just et al. | 2023 | â | â | â | 84 | â | 110 | â | â |
| He et al. | 2022 | â | 1.20 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.70 | â | â | 112 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.69* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.68 | 0.93 | â | 91 | â | â | â | 0 |
| Dias et al. | 2021 | 0.68 | 1.10 | â | 238 | 0.140 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.71 | 0.86 | â | 112 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.68 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 81 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 0.74 | 0.95 | â | 92 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.68 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.68 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.66 | 1.02 | â | 136 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.67 | 1.00 | â | 84 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.67 | 1.00 | â | 84 | â | â | â | â |
| Gozha et al. | 2012 | 0.72 | â | â | 89 | â | 427 | â | â |
| Kharchenko et al. | 2012 | 0.67 | 1.00 | â | 84 | â | â | â | â |
| Piskunov et al. | 2008 | 0.65 | 0.99 | â | 85 | â | 160* | â | â |
| Piskunov et al. | 2007 | 0.65 | 0.99 | â | 85 | â | 61 | â | â |
| van den Bergh | 2006 | 0.65 | 0.99 | â | 148 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.65 | 0.99 | â | 85 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.65 | 0.99 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.65 | â | â | 140 | -0.450* | â | â | â |
| Dias et al. | 2002 | 0.72 | 1.24 | â | 89 | 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: good fit.
Cavallo et al. (2024)
Gold sample.