Trumpler 33
(Collinder 378; MWSC 2910; OCL 34; ESO 590 20; FoF 2212)
0.95
UTI
0.77
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
6.6 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 33 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 276.151 | -19.715 | 0.688 | 0.492 | 0.511 | -4.359 |
| Li et al. | 2025 | 276.159 | -19.711 | 0.677 | 0.435 | 0.449 | â |
| Almeida et al. | 2025 | 276.164 | -19.712 | â | â | â | â |
| Hunt & Reffert | 2024 | 276.158 | -19.709 | 0.682 | 0.52 | 0.502 | -3.987 |
| Cavallo et al. | 2024 | 276.142 | -19.743 | 0.687 | â | â | â |
| Hunt & Reffert | 2023 | 276.158 | -19.709 | 0.682 | 0.52 | 0.502 | -3.987 |
| Almeida et al. | 2023 | 276.169 | -19.72 | â | â | â | â |
| Just et al. | 2023 | 276.164 | -19.721 | â | â | â | â |
| Tarricq et al. | 2022 | 276.151 | -19.726 | 0.699 | 0.536 | 0.528 | â |
| Dias et al. | 2021 | 276.164 | -19.712 | 0.682 | 0.423 | 0.447 | â |
| Cantat-Gaudin et al. | 2020 | 276.159 | -19.711 | 0.677 | 0.435 | 0.449 | â |
| Cantat-Gaudin & Anders | 2020 | 276.159 | -19.711 | 0.677 | 0.435 | 0.449 | â |
| Liu & Pang | 2019 | 276.151 | -19.716 | 0.688 | 0.509 | 0.526 | â |
| Dias et al. | 2019 | 276.175 | -19.717 | 0.699 | 0.458 | 0.511 | -4.64 |
| Soubiran et al. | 2018 | 276.159 | -19.711 | â | â | â | -3.71 |
| Bica et al. | 2019 | 276.164 | -19.719 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 276.159 | -19.711 | 0.677 | 0.435 | 0.449 | â |
| Loktin & Popova | 2017 | 276.18 | -19.718 | â | 2.656 | -6.093 | -3.8 |
| Kharchenko et al. | 2016 | 276.164 | -19.721 | â | â | â | â |
| Dias et al. | 2014 | 276.175 | -19.717 | â | -0.43 | -1.55 | -16.2 |
| Kharchenko et al. | 2013 | 276.172 | -19.72 | â | -3.0 | -1.85 | -3.8 |
| Gozha et al. | 2012 | 276.175 | -19.717 | â | â | â | â |
| Piskunov et al. | 2008 | 276.173 | -19.724 | â | â | â | â |
| van den Bergh | 2006 | 276.175 | -19.717 | â | â | â | â |
| Kharchenko et al. | 2005 | 276.18 | -19.72 | â | -4.69 | -0.92 | â |
| Dias et al. | 2002 | 276.175 | -19.717 | â | -0.43 | -1.55 | -16.2 |
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 | 1.33 | 1.44 | â | 72 | -0.041 | â | â | â |
| Almeida et al. | 2025 | 1.41 | 1.50 | â | 49 | â | 126 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 925* | â | â |
| Cavallo et al. | 2024 | 1.18 | 1.56 | â | 95 | -0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.36 | 1.41 | 1.29 | 52 | â | â | â | â |
| Almeida et al. | 2023 | 1.33 | 1.49 | â | 69 | 0.061 | 313* | 0.56 | â |
| Just et al. | 2023 | â | â | â | 69 | â | 36 | â | â |
| Tarricq et al. | 2022 | 1.39 | â | â | 65 | â | â | â | â |
| Dias et al. | 2021 | 1.41 | 1.50 | â | 49 | 0.145 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.45 | 1.22 | â | 58 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.42 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 29 | 0.250 | â | â | â |
| Dias et al. | 2019 | 1.49 | 1.30 | â | 27 | -0.013 | â | â | â |
| Soubiran et al. | 2018 | 1.42 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.42 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.80 | 1.17 | â | 43 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.28 | 1.55 | â | 69 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.28 | 1.55 | â | 69 | -1.544 | â | â | â |
| Gozha et al. | 2012 | 1.75 | â | â | 48 | â | 107 | â | â |
| Piskunov et al. | 2008 | 1.75 | 1.12 | â | 69 | â | â | â | â |
| van den Bergh | 2006 | 1.75 | 1.12 | â | 48 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.75 | 1.12 | â | 69 | â | â | â | â |
| Dias et al. | 2002 | 1.75 | 1.11 | â | 48 | -1.544 | 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.