Berkeley 16
(NGC 1798; FSR 0705; MWSC 483; OCL 410; Dolidze 48)
Summary
Berkeley 16 is a very rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 77.912 | 47.692 | – | 0.9 | -0.16 | -2.0 |
| Froebrich et al. (2007) | 77.929 | 47.695 | – | – | – | – |
| Kharchenko et al. (2012) | 77.91 | 47.695 | – | -1.9 | -2.44 | – |
| Kharchenko et al. (2013) | 77.91 | 47.695 | – | -1.9 | -2.44 | – |
| Kharchenko et al. (2016) | 77.899 | 47.695 | – | – | – | – |
| Loktin & Popova (2017) | 77.91 | 47.693 | – | -0.671 | -0.866 | -2.0 |
| Cantat-Gaudin et al. (2018) | 77.914 | 47.691 | 0.178 | 0.913 | -0.318 | – |
| Bica et al. (2019) | 77.898 | 47.689 | – | – | – | – |
| Soubiran et al. (2018) | 77.914 | 47.691 | – | – | – | 2.66 |
| Donor et al. (2020) | 77.91 | 47.695 | – | 0.83 | -0.31 | 2.7 |
| Cantat-Gaudin et al. (2020) | 77.914 | 47.691 | 0.178 | 0.913 | -0.318 | – |
| Dias et al. (2021) | 77.918 | 47.69 | 0.174 | 0.915 | -0.297 | 2.413 |
| Rain et al. (2021) | 77.914 | 47.691 | 0.178 | 0.913 | -0.318 | – |
| Jaehnig et al. (2021) | 77.915 | 47.692 | 0.21 | 0.906 | -0.295 | – |
| Just et al. (2023) | 77.899 | 47.695 | – | – | – | – |
| Hunt & Reffert (2023) | 77.908 | 47.689 | 0.204 | 0.792 | -0.37 | 1.626 |
| Cavallo et al. (2024) | 77.891 | 47.696 | 0.206 | – | – | – |
| Hunt & Reffert (2024) | 77.908 | 47.689 | 0.204 | 0.792 | -0.37 | 1.626 |
| Zhang et al. (2024) | 77.908 | 47.689 | – | – | – | – |
| Almeida et al. (2025) | 77.918 | 47.69 | – | – | – | – |
| Hu & Soubiran (2025) | 77.891 | 47.697 | – | – | – | – |
| UCC | 77.913 | 47.691 | 0.203 | 0.81 | -0.366 | 2.458 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.47, Dist=3470.0, Age=9.25, [Fe/H]=-0.12 |
| Kharchenko et al. (2012) | E(B-V)=0.312, d=5247.0, logt=9.3, [Fe/H]=-0.03 |
| Kharchenko et al. (2013) | E(B-V)=0.312, d=5247.0, logt=9.3, [Fe/H]=-0.03 |
| Kharchenko et al. (2016) | E(B-V)=0.312, d=5247.0, logt=9.3 |
| Loktin & Popova (2017) | E(B-V)=0.312, Dist=4153, logt=8.99 |
| Cantat-Gaudin et al. (2018) | dmode=4834.5 |
| Soubiran et al. (2018) | dmode=4834.5 |
| Donor et al. (2020) | Fe/H=-0.27 |
| Cantat-Gaudin et al. (2020) | AVNN=1.12, DistPc=5124.0, AgeNN=9.22 |
| Dias et al. (2021) | Av=1.635, Dist=4832, logage=9.137, [Fe/H]=-0.1 |
| Rain et al. (2021) | E(B-V)=0.47, Dist=4834.5, log(Age)=9.25, NBSS=27 |
| Jaehnig et al. (2021) | dmode=4.947 |
| Just et al. (2023) | logt=9.3, logmt=3.195 |
| Hunt & Reffert (2023) | AV50=1.472, diffAV50=1.572, MOD50=13.093, logAge50=8.965 |
| Cavallo et al. (2024) | AV50=1.63, dMod50=12.96, logAge50=9.19, [Fe/H]50=-0.31 |
| Hunt & Reffert (2024) | MassJ=3352.44, MassTot=3377.31 |
| Zhang et al. (2024) | [Fe/H]ANN=-0.3631, [Fe/H]MCMC=-0.0082 |
| Almeida et al. (2025) | AV=1.635, Dist=4832, logAge=9.137, MassRk=1887.7 |
| Hu & Soubiran (2025) | MA22=-0.25, MA23f=-0.43, MA23g=-0.37, MZ23=-0.52, MK24=-0.35, MF24=-0.34 |
Search coordinates in Bayestar19