Berkeley 86
(OCL 167; MWSC 3316; FoF 2183)
Summary
Berkeley 86 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is very well-studied in the literature.
This object shares a very small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 305.05 | 38.69 | – | – | – | – |
| Dias et al. (2002) | 305.1 | 38.7 | – | -4.56 | -5.56 | -25.54 |
| Chen et al. (2003) | 305.095 | 38.743 | – | -3.8 | -4.11 | -19.3 |
| Piskunov et al. (2008) | 305.098 | 38.693 | – | – | – | – |
| Kharchenko et al. (2012) | 305.052 | 38.69 | – | -4.4 | -2.17 | – |
| Loktin & Popova (2017) | 305.1 | 38.7 | – | -4.56 | -5.56 | -19.3 |
| Cantat-Gaudin et al. (2018) | 305.084 | 38.688 | 0.558 | -3.447 | -5.402 | – |
| Bica et al. (2019) | 305.087 | 38.663 | – | – | – | – |
| Dias et al. (2019) | 305.1 | 38.7 | 0.572 | -3.51 | -5.497 | -3.733 |
| Liu & Pang (2019) | 305.058 | 38.711 | 0.563 | -3.468 | -5.507 | – |
| Cantat-Gaudin et al. (2020) | 305.084 | 38.688 | 0.558 | -3.447 | -5.402 | – |
| Dias et al. (2021) | 305.104 | 38.706 | 0.561 | -3.437 | -5.406 | – |
| Rain et al. (2021) | 305.084 | 38.688 | 0.558 | -3.447 | -5.402 | – |
| Jaehnig et al. (2021) | 305.062 | 38.689 | 0.586 | -3.456 | -5.454 | – |
| Hunt & Reffert (2023) | 305.077 | 38.68 | 0.563 | -3.453 | -5.469 | -42.479 |
| Cavallo et al. (2024) | 305.084 | 38.702 | 0.565 | – | – | – |
| Celli et al. (2024) | 305.084 | 38.688 | – | – | – | – |
| Hunt & Reffert (2024) | 305.077 | 38.68 | 0.563 | -3.453 | -5.469 | -42.479 |
| Almeida et al. (2025) | 305.104 | 38.706 | – | – | – | – |
| UCC | 305.081 | 38.707 | 0.562 | -3.441 | -5.433 | -0.477 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.996, DM0=9.48, log_age_=6.4 |
| Dias et al. (2002) | E(B-V)=0.898, Dist=1112.0, Age=7.116 |
| Chen et al. (2003) | HDis=1112, Age=0.01 |
| Piskunov et al. (2008) | E(B-V)=0.9, Dist=1112, logt=6.96, logMA=1.864 |
| Kharchenko et al. (2012) | e_bv=0.958, distance=1653, log_age=6.8 |
| Loktin & Popova (2017) | E(B-V)=0.898, Dist=1112, logt=7.116 |
| Cantat-Gaudin et al. (2018) | dmode=1703.1 |
| Dias et al. (2019) | E(B-V)=0.79, Dist=1861, logAge=7.192, Z=0.026 |
| Liu & Pang (2019) | Age=0.005, Z=0.5 |
| Cantat-Gaudin et al. (2020) | AVNN=2.77, DistPc=1621.0, AgeNN=7.04 |
| Dias et al. (2021) | Av=2.59, Dist=1719, logage=6.775, [Fe/H]=0.18 |
| Rain et al. (2021) | E(B-V)=0.89, Dist=1703.1, log(Age)=7.11, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.702 |
| Hunt & Reffert (2023) | AV50=2.548, diffAV50=1.124, MOD50=11.159, logAge50=6.575 |
| Cavallo et al. (2024) | AV50=2.42, dMod50=11.2, logAge50=6.75, [Fe/H]50=0.32 |
| Celli et al. (2024) | Age=11.0, Mc=180.1 |
| Hunt & Reffert (2024) | MassJ=317.198, MassTot=317.198 |
| Almeida et al. (2025) | AV=2.59, Dist=1719, logAge=6.775, MassRk=242.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 2501 | 0.9 | 305.47 | 38.74 | 0.56 | -3.28 | -5.68 | – | 0.04 |