Trumpler 32
(Collinder 372; MWSC 2873; Harvard 19; OCL 55)
0.92
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Nm (P>50%)
1002
Core radius and density
1.1 [pc], 36 [pc-2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Trumpler 32 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is 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 | 274.294 | -13.349 | 0.578 | -1.028 | 1.161 | 16.012 |
| Li et al. | 2025 | 274.294 | -13.349 | 0.578 | -1.052 | 1.158 | â |
| Hu & Soubiran | 2025 | 274.301 | -13.343 | â | â | â | â |
| Almeida et al. | 2025 | 274.301 | -13.351 | â | â | â | â |
| Hunt & Reffert | 2024 | 274.292 | -13.356 | 0.579 | -1.039 | 1.16 | 18.996 |
| Cavallo et al. | 2024 | 274.302 | -13.343 | 0.579 | â | â | â |
| Hunt & Reffert | 2023 | 274.292 | -13.356 | 0.579 | -1.039 | 1.16 | 18.996 |
| Almeida et al. | 2023 | 274.298 | -13.332 | â | â | â | â |
| Just et al. | 2023 | 274.29 | -13.331 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 274.294 | -13.349 | â | â | â | â |
| Dias et al. | 2021 | 274.301 | -13.351 | 0.578 | -1.052 | 1.152 | 17.222 |
| Cantat-Gaudin et al. | 2020 | 274.294 | -13.349 | 0.578 | -1.052 | 1.158 | â |
| Cantat-Gaudin & Anders | 2020 | 274.294 | -13.349 | 0.578 | -1.052 | 1.158 | â |
| Soubiran et al. | 2018 | 274.294 | -13.349 | â | â | â | 16.52 |
| Bica et al. | 2019 | 274.296 | -13.362 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 274.294 | -13.349 | 0.578 | -1.052 | 1.158 | â |
| Dib et al. | 2018 | 274.297 | -13.33 | â | â | â | â |
| Loktin & Popova | 2017 | 274.335 | -13.346 | â | -0.809 | -4.314 | â |
| Sampedro et al. | 2017 | 274.375 | -13.35 | â | -1.79 | 0.5 | â |
| Joshi et al. | 2016 | 274.297 | -13.33 | â | â | â | â |
| Kharchenko et al. | 2016 | 274.29 | -13.331 | â | â | â | â |
| Dias et al. | 2014 | 274.375 | -13.35 | â | -0.91 | -0.34 | â |
| Kharchenko et al. | 2013 | 274.297 | -13.33 | â | 0.64 | -3.6 | â |
| Morales et al. | 2013 | 274.375 | -13.35 | â | â | â | â |
| van den Bergh | 2006 | 274.375 | -13.35 | â | â | â | â |
| Dias et al. | 2002 | 274.375 | -13.35 | â | -0.91 | -0.34 | â |
| Lynga | 1987 | 274.407 | -13.351 | 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 | 1.62 | 2.43 | 2.07 | 647 | -0.008 | 1422 | 0.62 | 0 |
| Li et al. | 2025 | 1.76 | 2.53 | â | 754 | 0.150 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.160(5) | â | â | â |
| Almeida et al. | 2025 | 1.56 | 2.48 | â | 647 | â | 975 | â | â |
| Hunt & Reffert | 2024 | 1.61 | 2.18 | 2.07 | 764 | â | 4914(1) | â | â |
| Cavallo et al. | 2024 | 1.40 | 2.64 | â | 813 | -0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.61 | 2.18 | 2.07 | 764 | â | â | â | â |
| Almeida et al. | 2023 | 1.60 | 2.43 | â | 748 | 0.079 | 1422(1) | 0.62 | â |
| Just et al. | 2023 | â | â | â | 624 | â | 1750 | â | â |
| Jadhav & Subramaniam | 2021 | 1.61 | 1.32 | â | 1349 | â | 891 | â | 0(1) |
| Dias et al. | 2021 | 1.56 | 2.48 | â | 647 | -0.008 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.61 | 1.32 | â | 1349 | â | â | â | â |
| Kounkel et al. | 2020 | 1.73 | 2.49 | â | 794 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.65 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.65 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.62 | â | â | 624 | â | â | â | â |
| Loktin & Popova | 2017 | 1.94 | 2.99 | â | 457 | â | â | â | â |
| Joshi et al. | 2016 | 1.62 | 2.43 | â | 624 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.62 | 2.43 | â | 624 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.62 | 2.43 | â | 624 | â | â | â | â |
| Morales et al. | 2013 | 1.72 | â | â | 300 | â | â | â | â |
| van den Bergh | 2006 | 1.72 | 2.02 | â | 302 | â | â | â | â |
| Dias et al. | 2002 | 1.72 | 2.02 | â | 302 | 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 P557, along with OC_0030.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.87 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.87 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1523, e_all=0.1734.
Morales et al. (2013)
Classified as morphological type 'OC1' (totally exposed cluster still physically associated with gas). Morphological flag: exposed cluster, without submm emission.