Berkeley 88
Summary
Berkeley 88 is a moderately populated, very dense object of low C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
This object shares a significant percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 305.4 | 48.083 | – | -2.49 | -4.02 | – |
| Kharchenko et al. (2012) | 305.332 | 48.14 | – | -2.49 | -4.02 | – |
| UCC | 305.308 | 48.141 | 0.116 | -3.973 | -4.659 | -68.164 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.88, Dist=6319.0, Age=9.2 |
| Kharchenko et al. (2012) | e_bv=1.208, distance=5038, log_age=8.815 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3863 | 72.3 | 305.3 | 48.14 | 0.11 | -3.96 | -4.65 | -68.16 | 0.06 |