Trumpler 22
(Collinder 283; VDBH 161; MWSC 2226; OCL 920; vdBergh-Hagen 161; ESO 134 06)
0.92
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.9
Clit
1.0
Cdup
Nm (P>50%)
215
Core radius and density
2.5 [pc], 5.4 [pc-2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.9 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 22 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near 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 age, metallicity, 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 | 217.796 | -61.165 | 0.402 | -5.142 | -2.687 | -40.732 |
| Li et al. | 2025 | 217.783 | -61.169 | 0.386 | -5.12 | -2.683 | â |
| Almeida et al. | 2025 | 217.794 | -61.155 | â | â | â | â |
| Hunt & Reffert | 2024 | 217.807 | -61.182 | 0.41 | -5.147 | -2.688 | -40.212 |
| Cavallo et al. | 2024 | 217.793 | -61.17 | 0.41 | â | â | â |
| Hunt & Reffert | 2023 | 217.807 | -61.182 | 0.41 | -5.147 | -2.688 | -40.212 |
| Just et al. | 2023 | 217.72 | -61.162 | â | â | â | â |
| Dias et al. | 2021 | 217.794 | -61.155 | 0.386 | -5.136 | -2.713 | -43.17 |
| Cantat-Gaudin et al. | 2020 | 217.783 | -61.169 | 0.386 | -5.12 | -2.683 | â |
| Cantat-Gaudin & Anders | 2020 | 217.783 | -61.169 | 0.386 | -5.12 | -2.683 | â |
| Bossini et al. | 2019 | 217.783 | -61.169 | â | â | â | â |
| Soubiran et al. | 2018 | 217.783 | -61.169 | â | â | â | -43.03 |
| Bica et al. | 2019 | 217.743 | -61.169 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 217.783 | -61.169 | 0.386 | -5.12 | -2.683 | â |
| Dias et al. | 2018 | â | â | â | -4.87 | -2.77 | â |
| Dib et al. | 2018 | 217.732 | -61.165 | â | â | â | â |
| Loktin & Popova | 2017 | 217.755 | -61.168 | â | -1.131 | -4.299 | -38.46 |
| Sampedro et al. | 2017 | 217.758 | -61.167 | â | -4.51 | -4.46 | â |
| Joshi et al. | 2016 | 217.732 | -61.165 | â | â | â | â |
| Kharchenko et al. | 2016 | 217.72 | -61.162 | â | â | â | â |
| Dias et al. | 2014 | 217.758 | -61.167 | â | -4.63 | -4.9 | â |
| Kharchenko et al. | 2013 | 217.732 | -61.165 | â | -5.06 | -4.2 | â |
| Morales et al. | 2013 | 217.758 | -61.167 | â | â | â | â |
| Piskunov et al. | 2008 | 217.743 | -61.169 | â | â | â | â |
| van den Bergh | 2006 | 217.75 | -61.167 | â | â | â | â |
| Kharchenko et al. | 2005 | 217.75 | -61.17 | â | -5.05 | -1.68 | â |
| Kharchenko et al. | 2003 | 217.78 | -61.15 | â | -5.71 | -3.39 | â |
| Dias et al. | 2002 | 217.758 | -61.167 | â | -4.63 | -4.9 | -38.46 |
| Lynga | 1987 | 217.809 | -61.167 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 216.85 | -60.95 | 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 | 1.75 | 1.67 | 0.77 | 95 | -0.060 | 627 | â | â |
| Li et al. | 2025 | 2.11 | 1.86 | â | 122 | 0.158 | â | â | â |
| Almeida et al. | 2025 | 2.21 | 1.90 | â | 65 | â | 1035 | â | â |
| Hunt & Reffert | 2024 | 2.27 | 1.76 | 0.77 | 95 | â | 1830(1) | â | â |
| Cavallo et al. | 2024 | 1.80 | 1.71 | â | 398 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 2.27 | 1.76 | 0.77 | 95 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 313 | â | 122 | â | â |
| Dias et al. | 2021 | 2.21 | 1.90 | â | 65 | 0.275 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.44 | 1.78 | â | 32 | â | â | â | â |
| Kounkel et al. | 2020 | 2.28 | 2.44 | â | 63 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.41 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 2.36 | 1.83 | â | 24 | -0.170 | â | â | â |
| Soubiran et al. | 2018 | 2.41 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.41 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.61 | â | â | 313 | â | â | â | â |
| Loktin & Popova | 2017 | 1.53 | 1.62 | â | 95 | â | â | â | â |
| Joshi et al. | 2016 | 1.61 | 1.58 | â | 313 | â | 219 | â | â |
| Kharchenko et al. | 2016 | 1.61 | 1.58 | â | 313 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.61 | 1.58 | â | 313 | â | â | â | â |
| Morales et al. | 2013 | 1.52 | â | â | 89 | â | â | â | â |
| Piskunov et al. | 2008 | 1.52 | 1.64 | â | 129 | â | â | â | â |
| van den Bergh | 2006 | 1.52 | 1.64 | â | 89 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.52 | 1.64 | â | 129 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.52 | 1.64 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.52 | 1.64 | â | 89 | -0.170 | â | â | â |
| Lynga | 1987 | 1.70 | 1.67 | â | 110 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P482, along with HSC_2649.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.4495, e_all=0.058.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg45' along with Hogg 17, NGC 5617 and Pismis 19.
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.