Berkeley 45
(MWSC 3086; OCL 107)
0.90
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
1.8 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 45 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
Distant
High extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 289.779 | 15.715 | 0.246 | -1.357 | -4.577 | 6.164 |
| Almeida et al. | 2025 | 289.777 | 15.714 | β | β | β | β |
| Hunt & Reffert | 2024 | 289.775 | 15.717 | 0.254 | -1.378 | -4.587 | 12.222 |
| Cavallo et al. | 2024 | 289.77 | 15.713 | 0.254 | β | β | β |
| Hunt & Reffert | 2023 | 289.775 | 15.717 | 0.254 | -1.378 | -4.587 | 12.222 |
| Just et al. | 2023 | 289.774 | 15.72 | β | β | β | β |
| Dias et al. | 2021 | 289.777 | 15.714 | 0.224 | -1.328 | -4.534 | β |
| Cantat-Gaudin et al. | 2020 | 289.778 | 15.716 | 0.225 | -1.336 | -4.534 | β |
| SΓ‘nchez et al. | 2020 | 289.8 | 15.717 | β | -1.346 | -4.484 | β |
| Cantat-Gaudin & Anders | 2020 | 289.778 | 15.716 | 0.225 | -1.336 | -4.534 | β |
| Soubiran et al. | 2018 | 289.778 | 15.716 | β | β | β | 6.66 |
| Bica et al. | 2019 | 289.782 | 15.714 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 289.778 | 15.716 | 0.225 | -1.336 | -4.534 | β |
| Kharchenko et al. | 2016 | 289.774 | 15.72 | β | β | β | β |
| Dias et al. | 2014 | 289.8 | 15.717 | β | -0.63 | -3.63 | β |
| Kharchenko et al. | 2013 | 289.78 | 15.722 | β | 0.12 | -3.97 | β |
| Dias et al. | 2002 | 289.8 | 15.717 | β | 0.12 | -3.97 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.51 | 3.05 | β | 553 | β | 1127 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2504* | β | β |
| Cavallo et al. | 2024 | 3.02 | 3.99 | β | 245 | -0.170 | β | β | β |
| Hunt & Reffert | 2023 | 3.70 | 3.63 | 1.79 | 229 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 724 | β | 337 | β | β |
| Dias et al. | 2021 | 3.51 | 3.05 | β | 553 | 0.274 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.33 | 2.88 | β | 617 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.94 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.94 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.94 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.36 | 3.23 | β | 724 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.36 | 3.23 | β | 724 | β | β | β | β |
| Dias et al. | 2002 | 2.35 | 4.34 | β | 398 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.