Berkeley 48
(NGC 6827; MWSC 3186; OCL 120; FSR 0152)
0.88
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
19.6 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 48 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~9.23 kpc) differs significantly from the median photometric distance (~6.47 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 297.221 | 21.214 | 0.108 | -2.453 | -5.465 | -8.165 |
| Almeida et al. | 2025 | 297.22 | 21.214 | β | β | β | β |
| Hunt & Reffert | 2024 | 297.222 | 21.214 | 0.124 | -2.462 | -5.456 | -1.635 |
| Cavallo et al. | 2024 | 297.225 | 21.207 | 0.119 | β | β | β |
| Hunt & Reffert | 2023 | 297.222 | 21.214 | 0.124 | -2.462 | -5.456 | -1.635 |
| Just et al. | 2023 | 297.208 | 21.213 | β | β | β | β |
| Dias et al. | 2021 | 297.22 | 21.214 | 0.095 | -2.408 | -5.465 | β |
| Cantat-Gaudin et al. | 2020 | 297.22 | 21.213 | 0.103 | -2.418 | -5.465 | β |
| SΓ‘nchez et al. | 2020 | 297.221 | 21.215 | β | -2.273 | -5.454 | β |
| Cantat-Gaudin & Anders | 2020 | 297.22 | 21.213 | 0.103 | -2.418 | -5.465 | β |
| Soubiran et al. | 2018 | 297.22 | 21.213 | β | β | β | 23.75 |
| Bica et al. | 2019 | 297.227 | 21.22 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 297.22 | 21.213 | 0.103 | -2.418 | -5.465 | β |
| Kharchenko et al. | 2016 | 297.208 | 21.213 | β | β | β | β |
| Kharchenko et al. | 2013 | 297.213 | 21.215 | β | 1.4 | -12.34 | β |
| Dias et al. | 2002 | 297.221 | 21.215 | β | 1.92 | -5.07 | 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 | 6.47 | 2.595 | 2.33 | 955 | -0.224 | 1632 | β | β |
| Almeida et al. | 2025 | 6.47 | 2.36 | β | 853 | β | 1632 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3054(1) | β | β |
| Cavallo et al. | 2024 | 5.27 | 3.42 | β | 331 | -0.700 | β | β | β |
| Hunt & Reffert | 2023 | 7.04 | 3.18 | 2.33 | 226 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1148 | β | 372 | β | β |
| Dias et al. | 2021 | 6.47 | 2.36 | β | 853 | 0.253 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 5.73 | 1.98 | β | 1288 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 7.59 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 7.59 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 7.59 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 4.19 | 2.77 | β | 1148 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.19 | 2.77 | β | 1148 | β | β | β | β |
| Dias et al. | 2002 | 4.55 | 2.42 | β | 955 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Silver sample.