Berkeley 5
(OCL 331; MWSC 142)
Summary
Berkeley 5 is a rich, very dense object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is poorly studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 26.95 | 62.933 | – | 0.11 | -2.78 | – |
| Kharchenko et al. (2012) | 26.925 | 62.933 | – | 0.11 | -2.78 | – |
| Cantat-Gaudin et al. (2018) | 26.928 | 62.935 | 0.088 | -1.61 | 0.764 | – |
| Bica et al. (2019) | 26.928 | 62.946 | – | – | – | – |
| Cantat-Gaudin et al. (2020) | 26.928 | 62.935 | 0.088 | -1.61 | 0.764 | – |
| UCC | 26.931 | 62.941 | 0.13 | -1.599 | 0.677 | -98.399 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.3, Dist=6200.0, Age=8.9 |
| Kharchenko et al. (2012) | e_bv=1.399, distance=6000, log_age=8.83 |
| Cantat-Gaudin et al. (2018) | dmode=8555.1 |
| Cantat-Gaudin et al. (2020) | AVNN=3.46, DistPc=7079.0, AgeNN=9.06 |
Search coordinates in Bayestar19
