Trumpler 36
(Collinder 414; IC 1311; FSR 0214; Dolidze 2; MWSC 3270; MWSC 3271; OCL 173; OCL 174)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.2 [arcmin]
- 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 36 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Very distant
Moderate extinction
Very massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 302.7 | 41.177 | 0.133 | -3.324 | -5.075 | -61.41 |
| Li et al. | 2025 | 302.697 | 41.177 | 0.124 | -3.364 | -5.047 | â |
| Hu & Soubiran | 2025 | 302.696 | 41.177 | â | â | â | â |
| Carrasco-Varela et al. | 2025 | 302.846 | 41.196 | â | â | â | â |
| Almeida et al. | 2025 | 302.693 | 41.174 | â | â | â | â |
| Hunt & Reffert | 2024 | 302.698 | 41.182 | 0.128 | -3.325 | -5.084 | -61.446 |
| Cavallo et al. | 2024 | 302.696 | 41.177 | 0.125 | â | â | â |
| Hunt & Reffert | 2023 | 302.698 | 41.182 | 0.128 | -3.325 | -5.084 | -61.446 |
| Just et al. | 2023 | 302.694 | 41.175 | â | â | â | â |
| Jaehnig et al. | 2021 | 302.697 | 41.18 | 0.134 | -3.356 | -5.056 | â |
| Rain et al. | 2021 | 302.697 | 41.177 | 0.124 | -3.364 | -5.047 | â |
| Dias et al. | 2021 | 302.693 | 41.174 | 0.131 | -3.366 | -5.048 | -61.041 |
| Cantat-Gaudin et al. | 2020 | 302.697 | 41.177 | 0.124 | -3.364 | -5.047 | â |
| Cantat-Gaudin & Anders | 2020 | 302.697 | 41.177 | 0.124 | -3.364 | -5.047 | â |
| Soubiran et al. | 2018 | 302.697 | 41.177 | â | â | â | -8.41 |
| Bica et al. | 2019 | 302.686 | 41.165 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 302.697 | 41.177 | 0.124 | -3.364 | -5.047 | â |
| Kharchenko et al. | 2016 | 302.694 | 41.175 | â | â | â | â |
| Dias et al. | 2014 | 302.475 | 41.367 | â | -0.16 | -6.16 | â |
| Kharchenko et al. | 2013 | 302.698 | 41.178 | â | -3.61 | -2.92 | -63.2 |
| Gozha et al. | 2012 | 302.575 | 41.217 | â | â | â | â |
| Froebrich et al. | 2007 | 302.7 | 41.179 | â | â | â | â |
| van den Bergh | 2006 | 302.575 | 41.217 | â | â | â | â |
| Dias et al. | 2002 | 302.575 | 41.217 | â | 0.59 | -6.51 | -63.15 |
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 | 6.54 | 1.79 | â | 1070 | -0.046 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.240* | â | â | â |
| Carrasco-Varela et al. | 2025 | 5.89 | 1.55 | â | 1406 | 0.050 | â | â | 0.01* |
| Almeida et al. | 2025 | 6.69 | 1.55 | â | 1406 | â | 5517 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 14882* | â | â |
| Cavallo et al. | 2024 | 5.30 | 2.05 | â | 1549 | -0.610 | â | â | â |
| Hunt & Reffert | 2023 | 7.88 | 1.81 | 0.96 | 962 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1413 | â | 8995 | â | â |
| Jaehnig et al. | 2021 | 7.54* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 6.51 | 0.87 | â | 1585 | â | â | â | 5 |
| Dias et al. | 2021 | 6.69 | 1.55 | â | 1406 | 0.143 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 6.17 | 1.34 | â | 912 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 6.51 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 6.51 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 6.51 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 5.89 | 1.42 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.89 | 1.42 | â | 1413 | -0.300 | â | â | â |
| Gozha et al. | 2012 | 6.03 | â | â | 1585 | -0.300 | â | â | â |
| van den Bergh | 2006 | 5.33 | 2.36 | â | 417 | â | â | â | â |
| Dias et al. | 2002 | 6.03 | 0.87 | â | 1585 | -0.300 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.