Trumpler 16
0.89
UTI
0.84
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Nm (P>50%)
332
Core radius and density
2.5 [pc], 8.8 [pc-2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Trumpler 16 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 massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (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 | 161.256 | -59.715 | 0.403 | -6.889 | 2.586 | -0.073 |
| Almeida et al. | 2025 | 161.25 | -59.694 | â | â | â | â |
| Hunt & Reffert | 2024 | 161.265 | -59.697 | 0.402 | -6.908 | 2.606 | -2.885 |
| Celli et al. | 2024 | 161.253 | -59.7 | â | â | â | â |
| Cavallo et al. | 2024 | 161.236 | -59.736 | 0.403 | â | â | â |
| Hunt & Reffert | 2023 | 161.265 | -59.697 | 0.402 | -6.908 | 2.606 | -2.885 |
| Jaehnig et al. | 2021 | 161.236 | -59.708 | 0.416 | -6.88 | 2.556 | â |
| Rain et al. | 2021 | 161.253 | -59.7 | 0.389 | -6.864 | 2.509 | â |
| Dias et al. | 2021 | 161.25 | -59.694 | 0.39 | -6.903 | 2.521 | â |
| Cantat-Gaudin et al. | 2020 | 161.253 | -59.7 | 0.389 | -6.864 | 2.509 | â |
| Cantat-Gaudin & Anders | 2020 | 161.253 | -59.7 | 0.389 | -6.864 | 2.509 | â |
| Cantat-Gaudin et al. | 2018 | 161.253 | -59.7 | 0.389 | -6.864 | 2.509 | â |
| Dias et al. | 2018 | â | â | â | -7.08 | 2.3 | â |
| Loktin & Popova | 2017 | 161.295 | -59.717 | â | -6.94 | 1.41 | -25.0 |
| Sampedro et al. | 2017 | 161.292 | -59.717 | â | -6.36 | 1.15 | â |
| Dias et al. | 2014 | 161.292 | -59.717 | â | -6.94 | 1.41 | â |
| Gozha et al. | 2012 | 161.292 | -59.717 | â | â | â | â |
| Piskunov et al. | 2008 | 161.287 | -59.713 | â | â | â | â |
| Kharchenko et al. | 2007 | 161.29 | -59.72 | â | 0.12 | â | -25.0 |
| Ahumada & Lapasset | 2007 | 161.25 | -59.717 | â | â | â | â |
| van den Bergh | 2006 | 161.3 | -59.717 | â | â | â | â |
| Kharchenko et al. | 2005 | 161.29 | -59.72 | â | -11.1 | 4.02 | -25.0 |
| Kharchenko et al. | 2003 | 161.26 | -59.72 | â | -10.36 | 5.24 | â |
| Dias et al. | 2002 | 161.292 | -59.717 | â | -6.94 | 1.41 | -22.78 |
| Dambis | 1999 | 161.292 | -59.717 | â | â | â | â |
| Lynga | 1987 | 161.269 | -59.709 | â | â | â | -16.0 |
| van den Bergh & Hagen | 1975 | 160.8 | -59.45 | 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 | 2.4 | 1.53 | 2.3 | 6 | 0.224 | 1114 | â | 0 |
| Almeida et al. | 2025 | 2.08 | 1.51 | â | 5 | â | 574 | â | â |
| Hunt & Reffert | 2024 | 2.38 | 1.67 | 2.30 | 6 | â | 1796(1) | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 1107 | â | â |
| Cavallo et al. | 2024 | 1.49 | 1.53 | â | 21 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 2.38 | 1.67 | 2.30 | 6 | â | â | â | â |
| Jaehnig et al. | 2021 | 2.40(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.40 | 1.14 | â | 1 | â | â | â | 0 |
| Dias et al. | 2021 | 2.08 | 1.51 | â | 5 | 0.348 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.11 | 1.16 | â | 13 | â | â | â | â |
| Kounkel et al. | 2020 | 2.16 | 2.14 | â | 10 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.40 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.40 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.84 | 1.69 | â | 6 | â | â | â | â |
| Gozha et al. | 2012 | 3.90 | â | â | 5 | â | 1122 | â | â |
| Piskunov et al. | 2008 | 2.84 | 1.64 | â | 8 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 1.55 | â | 6 | â | â | â | 0 |
| van den Bergh | 2006 | 2.67 | 1.55 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.84 | 1.64 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2003 | 2.70 | 1.26 | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.90 | 1.14 | â | 1 | â | â | â | â |
| Dambis | 1999 | 2.56 | 1.53 | â | 3 | â | â | â | â |
| Lynga | 1987 | 2.90 | 1.48 | â | 10 | 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)
Part of multiple system G21, along with ASCC_62, Gulliver_52, NGC_3496 and Collinder_228.
Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.44 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.44 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2718, e_all=0.2512.
Ahumada & Lapasset (2007)
The dereddened colour-magnitude diagram was examined (1973A&AS...12..331F). The cluster apparent diameter was taken from (1992AJ....104.1865T).