Trumpler 1
(Collinder 15; MWSC 127; OCL 328; FSR 0552)
0.96
UTI
0.79
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
21.3 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 1 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 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 | 23.909 | 61.286 | 0.354 | -1.635 | -0.576 | â |
| Li et al. | 2025 | 23.915 | 61.283 | 0.348 | -1.598 | -0.541 | â |
| Almeida et al. | 2025 | 23.923 | 61.285 | â | â | â | â |
| Hunt & Reffert | 2024 | 23.916 | 61.284 | 0.355 | -1.645 | -0.584 | â |
| Celli et al. | 2024 | 23.915 | 61.283 | â | â | â | â |
| Cavallo et al. | 2024 | 23.856 | 61.282 | 0.355 | â | â | â |
| Hunt & Reffert | 2023 | 23.916 | 61.284 | 0.355 | -1.645 | -0.584 | â |
| Almeida et al. | 2023 | 23.918 | 61.287 | â | â | â | â |
| Just et al. | 2023 | 23.899 | 61.272 | â | â | â | â |
| Jaehnig et al. | 2021 | 23.913 | 61.287 | 0.388 | -1.612 | -0.525 | â |
| Rain et al. | 2021 | 23.915 | 61.283 | 0.348 | -1.598 | -0.541 | â |
| Dias et al. | 2021 | 23.923 | 61.285 | 0.347 | -1.609 | -0.539 | â |
| Cantat-Gaudin et al. | 2020 | 23.915 | 61.283 | 0.348 | -1.598 | -0.541 | â |
| Cantat-Gaudin & Anders | 2020 | 23.915 | 61.283 | 0.348 | -1.598 | -0.541 | â |
| Bossini et al. | 2019 | 23.915 | 61.283 | â | â | â | â |
| Bica et al. | 2019 | 23.9 | 61.298 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 23.915 | 61.283 | 0.348 | -1.598 | -0.541 | â |
| Loktin & Popova | 2017 | 23.925 | 61.284 | â | -0.5 | -0.812 | -65.0 |
| Kharchenko et al. | 2016 | 23.899 | 61.272 | â | â | â | â |
| Dias et al. | 2014 | 23.925 | 61.283 | â | -3.31 | -1.02 | â |
| Kharchenko et al. | 2013 | 23.91 | 61.275 | â | 0.67 | -2.16 | -65.0 |
| Gozha et al. | 2012 | 23.925 | 61.283 | â | â | â | â |
| Kharchenko et al. | 2012 | 23.91 | 61.275 | â | 0.67 | -2.16 | -65.0 |
| Kharchenko et al. | 2007 | 23.92 | 61.28 | â | 0.03 | â | â |
| van den Bergh | 2006 | 23.925 | 61.283 | â | â | â | â |
| Dias et al. | 2002 | 23.925 | 61.283 | â | -3.31 | -1.02 | -65.0 |
| Dambis | 1999 | 23.925 | 61.283 | 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 | 2.57 | 1.805 | 1.03 | 26 | -0.025 | 557 | 0.64 | 0.0 |
| Li et al. | 2025 | 2.54 | 1.75 | â | 47 | -0.039 | â | â | â |
| Almeida et al. | 2025 | 2.42 | 1.84 | â | 22 | â | 345 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 897(1) | â | â |
| Celli et al. | 2024 | â | â | â | 29 | â | 572 | â | â |
| Cavallo et al. | 2024 | 3.16 | 1.62 | â | 40 | 0.720 | â | â | â |
| Hunt & Reffert | 2023 | 2.63 | 1.63 | 1.03 | 28 | â | â | â | â |
| Almeida et al. | 2023 | 2.42 | 1.81 | â | 26 | -0.046 | 557(1) | 0.64 | â |
| Just et al. | 2023 | â | â | â | 13 | â | 24 | â | â |
| Jaehnig et al. | 2021 | 2.58(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.65 | 2.11 | â | 20 | â | â | â | 0 |
| Dias et al. | 2021 | 2.42 | 1.84 | â | 22 | -0.012 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.78 | 1.63 | â | 29 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.65 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 3.30 | 1.78 | â | 33 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.65 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.58 | 1.79 | â | 30 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.40 | 1.81 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.40 | 1.81 | â | 13 | â | â | â | â |
| Gozha et al. | 2012 | 2.56 | â | â | 40 | -0.710 | â | â | â |
| Kharchenko et al. | 2012 | 2.40 | 1.81 | â | 13 | â | â | â | â |
| van den Bergh | 2006 | 2.56 | 1.80 | â | 30 | â | â | â | â |
| Dias et al. | 2002 | 2.47 | 2.11 | â | 20 | â | â | â | â |
| Dambis | 1999 | 2.69 | 1.64 | â | 25 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.