Berkeley 100
(MWSC 3727; OCL 264)
0.80
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
10.8 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 100 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~6.08 kpc) differs significantly from the median photometric distance (~4.30 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 351.484 | 63.779 | 0.165 | -3.267 | -1.475 | -65.069 |
| Hunt & Reffert | 2024 | 351.489 | 63.78 | 0.173 | -3.265 | -1.459 | -45.808 |
| Cavallo et al. | 2024 | 351.502 | 63.784 | 0.172 | β | β | β |
| Hunt & Reffert | 2023 | 351.489 | 63.78 | 0.173 | -3.265 | -1.459 | -45.808 |
| Just et al. | 2023 | 351.468 | 63.775 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 351.485 | 63.781 | 0.123 | -3.372 | -1.557 | β |
| SΓ‘nchez et al. | 2020 | 351.492 | 63.78 | β | -3.207 | -1.595 | β |
| Cantat-Gaudin & Anders | 2020 | 351.485 | 63.781 | 0.123 | -3.372 | -1.557 | β |
| Bica et al. | 2019 | 351.491 | 63.782 | β | β | β | β |
| Kharchenko et al. | 2016 | 351.468 | 63.775 | β | β | β | β |
| Dias et al. | 2014 | 351.492 | 63.78 | β | -2.47 | -0.26 | β |
| Kharchenko et al. | 2013 | 351.477 | 63.778 | β | -1.25 | -2.58 | β |
| Kharchenko et al. | 2012 | 351.477 | 63.778 | β | -1.25 | -2.58 | β |
| Dias et al. | 2002 | 351.492 | 63.78 | β | -1.25 | -2.58 | β |
π‘ 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 4.305 | 3.6 | 2.15 | 70 | -0.350 | 536 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1052(1) | β | β |
| Cavallo et al. | 2024 | 5.45 | 3.60 | β | 282 | -0.350 | β | β | β |
| Hunt & Reffert | 2023 | 4.84 | 3.10 | 2.15 | 225 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 27 | β | 19 | β | β |
| Cantat-Gaudin et al. | 2020 | 6.08 | 2.48 | β | 1230 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 6.58 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.70 | 3.75 | β | 27 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.70 | 3.75 | β | 27 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.70 | 3.75 | β | 27 | β | β | β | β |
| Dias et al. | 2002 | 3.77 | 3.10 | β | 112 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.