Berkeley 96
(MWSC 3630; OCL 232; FSR 0359)
- CN 0.63 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
(*): The parallax distance estimate (~4.37 kpc) differs significantly from the median photometric distance (~3.20 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 337.476 | 55.41 | 0.229 | -3.525 | -3.039 | – |
| Almeida et al. | 2025 | 337.479 | 55.397 | – | – | – | – |
| Hunt & Reffert | 2024 | 337.473 | 55.412 | 0.227 | -3.529 | -3.019 | – |
| Cavallo et al. | 2024 | 337.489 | 55.433 | 0.226 | – | – | – |
| Hunt & Reffert | 2023 | 337.473 | 55.412 | 0.227 | -3.529 | -3.019 | – |
| Just et al. | 2023 | 337.464 | 55.401 | – | – | – | – |
| Jaehnig et al. | 2021 | 337.475 | 55.409 | 0.265 | -3.562 | -3.01 | – |
| Rain et al. | 2021 | 337.478 | 55.408 | 0.252 | -3.503 | -2.994 | – |
| Dias et al. | 2021 | 337.479 | 55.397 | 0.235 | -3.487 | -2.988 | – |
| Cantat-Gaudin et al. | 2020 | 337.478 | 55.408 | 0.252 | -3.503 | -2.994 | – |
| Dias et al. | 2019 | 337.454 | 55.396 | 0.242 | -3.511 | -2.976 | 1.75 |
| Bica et al. | 2019 | 337.461 | 55.41 | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 337.478 | 55.408 | 0.252 | -3.503 | -2.994 | – |
| Loktin & Popova | 2017 | 337.47 | 55.405 | – | -0.613 | -0.274 | – |
| Kharchenko et al. | 2016 | 337.464 | 55.401 | – | – | – | – |
| Kharchenko et al. | 2013 | 337.47 | 55.405 | – | -4.49 | -3.6 | – |
| Kharchenko et al. | 2012 | 337.47 | 55.405 | – | -4.49 | -3.6 | – |
| Dias et al. | 2002 | 337.454 | 55.396 | – | -2.86 | -1.31 | – |
| Dambis | 1999 | 337.454 | 55.396 | – | – | – | – |
💡 Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.98 | 1.85 | – | 18 | – | 227 | – | – |
| Hunt & Reffert | 2024 | – | – | – | – | – | 741* | – | – |
| Cavallo et al. | 2024 | 3.48 | 1.77 | – | 41 | 0.120 | – | – | – |
| Hunt & Reffert | 2023 | 4.31 | 1.90 | 1.61 | 20 | – | – | – | – |
| Just et al. | 2023 | – | – | – | 10 | – | 216 | – | – |
| Jaehnig et al. | 2021 | 3.69* | – | – | – | – | – | – | – |
| Rain et al. | 2021 | 3.56 | 0.53 | – | 40 | – | – | – | 0 |
| Dias et al. | 2021 | 2.98 | 1.85 | – | 18 | -0.094 | – | – | – |
| Cantat-Gaudin et al. | 2020 | 3.58 | 1.43 | – | 37 | – | – | – | – |
| Dias et al. | 2019 | 3.20 | 1.61 | – | 19 | -0.930 | – | – | – |
| Cantat-Gaudin et al. | 2018 | 3.56 | – | – | – | – | – | – | – |
| Loktin & Popova | 2017 | 3.12 | 1.88 | – | 8 | – | – | – | – |
| Kharchenko et al. | 2016 | 3.20 | 2.11 | – | 10 | – | – | – | – |
| Kharchenko et al. | 2013 | 3.20 | 2.11 | – | 10 | – | – | – | – |
| Kharchenko et al. | 2012 | 3.20 | 2.11 | – | 10 | – | – | – | – |
| Dias et al. | 2002 | 3.18 | 1.67 | – | 40 | – | – | – | – |
| Dambis | 1999 | 3.16 | 1.97 | – | 6 | – | – | – | – |
💡 Note: The parameters are sometimes
transformed from their original values to match the format of the
columns shown here, see FAQ.
The columns DAv, Bfr, BSS correspond to differential
extinction, binary fraction, and blue stragglers, respectively.
BSS values can be listed as fractions or integers.
(*): indicates that this parameter is
assigned more than one value in the corresponding reference.
Almeida et al. (2025): Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024): Gold sample.