Berkeley 10
(FSR 0623; MWSC 290; OCL 370; FoF 630)
Summary
Berkeley 10 is a rich, very dense object of very 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) | 54.883 | 66.486 | – | -2.11 | -0.5 | – |
| Froebrich et al. (2007) | 54.925 | 66.495 | – | – | – | – |
| Kharchenko et al. (2012) | 54.9 | 66.49 | – | -1.93 | -0.96 | – |
| Kharchenko et al. (2013) | 54.9 | 66.49 | – | -1.72 | -1.22 | – |
| Kharchenko et al. (2016) | 54.886 | 66.488 | – | – | – | – |
| Loktin & Popova (2017) | 54.885 | 66.486 | – | -2.837 | -2.97 | – |
| Cantat-Gaudin et al. (2018) | 54.894 | 66.486 | 0.372 | -1.47 | 1.047 | – |
| Bica et al. (2019) | 54.874 | 66.49 | – | – | – | – |
| Soubiran et al. (2018) | 54.894 | 66.486 | – | – | – | -36.29 |
| Liu & Pang (2019) | 54.89 | 66.486 | 0.368 | -1.426 | 1.036 | – |
| Cantat-Gaudin et al. (2020) | 54.894 | 66.486 | 0.372 | -1.47 | 1.047 | – |
| Dias et al. (2021) | 54.888 | 66.49 | 0.368 | -1.464 | 1.053 | -36.134 |
| Just et al. (2023) | 54.886 | 66.488 | – | – | – | – |
| Hunt & Reffert (2023) | 54.885 | 66.489 | 0.398 | -1.497 | 1.005 | -32.448 |
| Cavallo et al. (2024) | 54.895 | 66.488 | 0.396 | – | – | – |
| Hunt & Reffert (2024) | 54.885 | 66.489 | 0.398 | -1.497 | 1.005 | -32.448 |
| Almeida et al. (2025) | 54.888 | 66.49 | – | – | – | – |
| UCC | 54.895 | 66.484 | 0.387 | -1.497 | 1.01 | -36.462 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.75, Dist=1700.0, Age=9.06, [Fe/H]=-0.49 |
| Kharchenko et al. (2012) | E(B-V)=0.799, d=2201.0, logt=8.825, [Fe/H]=-0.49 |
| Kharchenko et al. (2013) | E(B-V)=0.799, d=2201.0, logt=8.81, [Fe/H]=-0.49 |
| Kharchenko et al. (2016) | E(B-V)=0.799, d=2201.0, logt=8.81 |
| Loktin & Popova (2017) | E(B-V)=0.841, Dist=2535, logt=8.67 |
| Cantat-Gaudin et al. (2018) | dmode=2496.5 |
| Soubiran et al. (2018) | dmode=2496.5 |
| Liu & Pang (2019) | Age=0.692, Z=0.5 |
| Cantat-Gaudin et al. (2020) | AVNN=1.94, DistPc=2365.0, AgeNN=9.08 |
| Dias et al. (2021) | Av=2.595, Dist=2004, logage=8.902, [Fe/H]=-0.1 |
| Just et al. (2023) | logt=8.81, logmt=2.734 |
| Hunt & Reffert (2023) | AV50=2.802, diffAV50=1.198, MOD50=11.866, logAge50=8.531 |
| Cavallo et al. (2024) | AV50=3.14, dMod50=11.99, logAge50=8.55, [Fe/H]50=0.04 |
| Hunt & Reffert (2024) | MassJ=2288.05, MassTot=2308.57 |
| Almeida et al. (2025) | AV=2.595, Dist=2004, logAge=8.902, MassRk=1156.4 |
Search coordinates in Bayestar19