Trumpler 8
(Collinder 167; NGC 2479; MWSC 1380; OCL 623; ESO 561 01; FSR 1271)
0.96
UTI
0.78
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
23.2 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 8 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is very well-studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 118.768 | -17.735 | 0.607 | -4.318 | 1.097 | 40.212 |
| Li et al. | 2025 | 118.762 | -17.732 | 0.626 | -4.318 | 1.053 | β |
| Hu & Soubiran | 2025 | 118.765 | -17.73 | β | β | β | β |
| Almeida et al. | 2025 | 118.755 | -17.731 | β | β | β | β |
| Hunt & Reffert | 2024 | 118.772 | -17.734 | 0.611 | -4.326 | 1.097 | 34.536 |
| Cavallo et al. | 2024 | 118.765 | -17.731 | 0.612 | β | β | β |
| Hunt & Reffert | 2023 | 118.772 | -17.734 | 0.611 | -4.326 | 1.097 | 34.536 |
| Almeida et al. | 2023 | 118.751 | -17.747 | β | β | β | β |
| Just et al. | 2023 | 118.779 | -17.727 | β | β | β | β |
| Dias et al. | 2021 | 118.755 | -17.731 | 0.623 | -4.334 | 1.059 | 40.969 |
| Cantat-Gaudin et al. | 2020 | 118.762 | -17.732 | 0.626 | -4.318 | 1.053 | β |
| SΓ‘nchez et al. | 2020 | 118.775 | -17.71 | β | -4.324 | 1.111 | β |
| Donor et al. | 2020 | 118.785 | -17.73 | β | -4.3 | 1.09 | 41.6 |
| Cantat-Gaudin & Anders | 2020 | 118.762 | -17.732 | 0.626 | -4.318 | 1.053 | β |
| Bica et al. | 2019 | 118.777 | -17.715 | β | β | β | β |
| Loktin & Popova | 2017 | 118.77 | -17.738 | β | -6.64 | 3.632 | 38.17 |
| Kharchenko et al. | 2016 | 118.779 | -17.727 | β | β | β | β |
| Dias et al. | 2014 | 118.775 | -17.71 | β | -2.94 | -1.33 | β |
| Kharchenko et al. | 2013 | 118.785 | -17.73 | β | -7.14 | 4.72 | β |
| Piskunov et al. | 2008 | 118.763 | -17.712 | β | β | β | β |
| Kharchenko et al. | 2005 | 118.77 | -17.71 | β | -0.94 | 1.93 | β |
| Kharchenko et al. | 2003 | 118.74 | -17.7 | β | -1.89 | 0.57 | β |
| Dias et al. | 2002 | 118.775 | -17.71 | β | -2.94 | -1.33 | 38.17 |
π‘ 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 | 99999β | 1.52 | 0.26 | 0.47 | 1035 | -0.035 | 392 | 0.54 | β |
| Li et al. | 2025 | 1.56 | 0.24 | β | 1217 | -0.040 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.150(5) | β | β | β |
| Almeida et al. | 2025 | 1.50 | 0.26 | β | 1219 | β | 390 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 678(1) | β | β |
| Cavallo et al. | 2024 | 1.51 | 0.19 | β | 1349 | -0.020 | β | β | β |
| Hunt & Reffert | 2023 | 1.52 | 0.10 | 0.47 | 1309 | β | β | β | β |
| Almeida et al. | 2023 | 1.56 | 0.07 | β | 1262 | 0.066 | 395(1) | 0.54 | β |
| Just et al. | 2023 | β | β | β | 1035 | β | 258 | β | β |
| Dias et al. | 2021 | 1.50 | 0.26 | β | 1219 | -0.104 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.56 | 0.15 | β | 977 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.030 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.53 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.64 | 0.57 | β | 589 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.36 | 0.26 | β | 1035 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.36 | 0.26 | β | 1035 | β | β | β | β |
| Piskunov et al. | 2008 | 1.20 | 0.31 | β | 977 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.20 | 0.31 | β | 977 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.67 | 0.31 | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.58 | 0.16 | β | 1000 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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