Berkeley 96
(MWSC 3630; OCL 232; FSR 0359)
Summary
Berkeley 96 is a moderately populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 337.454 | 55.396 | – | – | – | – |
| Dias et al. (2002) | 337.454 | 55.396 | – | -2.86 | -1.31 | – |
| Kharchenko et al. (2012) | 337.47 | 55.405 | – | -4.49 | -3.6 | – |
| Kharchenko et al. (2013) | 337.47 | 55.405 | – | -4.49 | -3.6 | – |
| Kharchenko et al. (2016) | 337.464 | 55.401 | – | – | – | – |
| Loktin & Popova (2017) | 337.47 | 55.405 | – | -0.613 | -0.274 | – |
| Cantat-Gaudin et al. (2018) | 337.478 | 55.408 | 0.252 | -3.503 | -2.994 | – |
| Bica et al. (2019) | 337.461 | 55.41 | – | – | – | – |
| Dias et al. (2019) | 337.454 | 55.396 | 0.242 | -3.511 | -2.976 | 1.75 |
| Cantat-Gaudin et al. (2020) | 337.478 | 55.408 | 0.252 | -3.503 | -2.994 | – |
| Dias et al. (2021) | 337.479 | 55.397 | 0.235 | -3.487 | -2.988 | – |
| Rain et al. (2021) | 337.478 | 55.408 | 0.252 | -3.503 | -2.994 | – |
| Jaehnig et al. (2021) | 337.475 | 55.409 | 0.265 | -3.562 | -3.01 | – |
| Just et al. (2023) | 337.464 | 55.401 | – | – | – | – |
| Hunt & Reffert (2023) | 337.473 | 55.412 | 0.227 | -3.529 | -3.019 | – |
| Cavallo et al. (2024) | 337.489 | 55.433 | 0.226 | – | – | – |
| Hunt & Reffert (2024) | 337.473 | 55.412 | 0.227 | -3.529 | -3.019 | – |
| Almeida et al. (2025) | 337.479 | 55.397 | – | – | – | – |
| UCC | 337.476 | 55.41 | 0.229 | -3.525 | -3.039 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.634, DM0=12.5, log_age_=6.8 |
| Dias et al. (2002) | E(B-V)=0.54, Dist=3180.0, Age=7.6 |
| Kharchenko et al. (2012) | E(B-V)=0.681, d=3200.0, logt=7.0 |
| Kharchenko et al. (2013) | E(B-V)=0.681, d=3200.0, logt=7.0 |
| Kharchenko et al. (2016) | E(B-V)=0.681, d=3200.0, logt=7.0 |
| Loktin & Popova (2017) | E(B-V)=0.605, Dist=3122, logt=6.911 |
| Cantat-Gaudin et al. (2018) | dmode=3560.6 |
| Dias et al. (2019) | E(B-V)=0.52, Dist=3196, logAge=7.268, Z=0.006 |
| Cantat-Gaudin et al. (2020) | AVNN=1.43, DistPc=3573.0, AgeNN=7.57 |
| Dias et al. (2021) | Av=1.854, Dist=2984, logage=7.256, [Fe/H]=-0.094 |
| Rain et al. (2021) | E(B-V)=0.17, Dist=3560.6, log(Age)=7.6, NBSS=0 |
| Jaehnig et al. (2021) | dmode=3.689 |
| Just et al. (2023) | logt=7.0, logmt=2.335 |
| Hunt & Reffert (2023) | AV50=1.904, diffAV50=1.613, MOD50=13.171, logAge50=7.31 |
| Cavallo et al. (2024) | AV50=1.77, dMod50=12.71, logAge50=7.61, [Fe/H]50=0.12 |
| Hunt & Reffert (2024) | MassJ=740.554, MassTot=811.051 |
| Almeida et al. (2025) | AV=1.854, Dist=2984, logAge=7.256, MassRk=226.8 |
Search coordinates in Bayestar19