Basel 1
(MWSC 2996; Apriamaswili 1; OCL 77)
0.82
UTI
0.71
CN
0.87
Cdens
1.0
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
92
Core radius and density
1.7 [pc], 4.3 [pc-2]
- CN 0.71 Moderately populated
- Cdens 0.87 Dense
- CC3 1.0 Very high quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
Basel 1 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 282.03 | -5.875 | 0.525 | -0.074 | -4.52 | 22.16 |
| Li et al. | 2025 | 282.036 | -5.876 | 0.525 | -0.079 | -4.509 | â |
| Almeida et al. | 2025 | 282.04 | -5.885 | â | â | â | â |
| Hunt & Reffert | 2024 | 282.027 | -5.87 | 0.523 | -0.045 | -4.494 | 22.172 |
| Cavallo et al. | 2024 | 282.034 | -5.883 | 0.524 | â | â | â |
| Hunt & Reffert | 2023 | 282.027 | -5.87 | 0.523 | -0.045 | -4.494 | 22.172 |
| Just et al. | 2023 | 282.031 | -5.866 | â | â | â | â |
| Dias et al. | 2021 | 282.04 | -5.885 | 0.53 | -0.082 | -4.521 | 24.096 |
| Cantat-Gaudin et al. | 2020 | 282.036 | -5.876 | 0.525 | -0.079 | -4.509 | â |
| Cantat-Gaudin & Anders | 2020 | 282.036 | -5.876 | 0.525 | -0.079 | -4.509 | â |
| Soubiran et al. | 2018 | 282.036 | -5.876 | â | â | â | 22.69 |
| Bica et al. | 2019 | 282.033 | -5.847 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 282.036 | -5.876 | 0.525 | -0.079 | -4.509 | â |
| Dias et al. | 2018 | â | â | â | -0.67 | -2.32 | â |
| Dib et al. | 2018 | 282.037 | -5.865 | â | â | â | â |
| Loktin & Popova | 2017 | 282.03 | -5.865 | â | 0.959 | -8.817 | â |
| Sampedro et al. | 2017 | 282.05 | -5.85 | â | -0.76 | -2.63 | â |
| Joshi et al. | 2016 | 282.037 | -5.865 | â | â | â | â |
| Kharchenko et al. | 2016 | 282.031 | -5.866 | â | â | â | â |
| Dias et al. | 2014 | 282.05 | -5.85 | â | -1.07 | -3.24 | â |
| Kharchenko et al. | 2013 | 282.037 | -5.865 | â | 0.36 | -5.53 | â |
| Bukowiecki et al. | 2011 | 282.038 | -5.862 | â | â | â | â |
| van den Bergh | 2006 | 282.05 | -5.85 | â | â | â | â |
| Dias et al. | 2002 | 282.05 | -5.85 | â | -1.07 | -3.24 | â |
| Lynga | 1987 | 282.037 | -5.838 | â | â | â | â |
đĄ 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 | 99999â | 1.75 | 1.59 | 1.155 | 136 | 0.102 | 404 | â | â |
| Li et al. | 2025 | 1.58 | 1.46 | â | 222 | 0.139 | â | â | â |
| Almeida et al. | 2025 | 1.52 | 1.59 | â | 178 | â | 261 | â | â |
| Hunt & Reffert | 2024 | 1.75 | 1.57 | 1.15 | 210 | â | 547(1) | â | â |
| Cavallo et al. | 2024 | 1.71 | 2.21 | â | 89 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 1.75 | 1.57 | 1.16 | 210 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 136 | â | 144 | â | â |
| Dias et al. | 2021 | 1.52 | 1.59 | â | 178 | 0.102 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.85 | 1.24 | â | 229 | â | â | â | â |
| Kounkel et al. | 2020 | 1.91 | 1.91 | â | 186 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.80 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.80 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.80 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.60 | â | â | 136 | â | â | â | â |
| Loktin & Popova | 2017 | 2.19 | 1.54 | â | 77 | â | â | â | â |
| Joshi et al. | 2016 | 1.60 | 1.71 | â | 136 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.60 | 1.71 | â | 136 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.60 | 1.71 | â | 136 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 1587 | â | â |
| Bukowiecki et al. | 2011 | 2.12(1) | 1.70 | â | 141 | â | â | â | â |
| van den Bergh | 2006 | 2.18 | 1.51 | â | 78 | â | â | â | â |
| Dias et al. | 2002 | 2.18 | 1.52 | â | 78 | â | â | â | â |
| Lynga | 1987 | 1.46 | 2.18 | â | 58 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P268, along with HSC_269.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.133, e_all=0.1903.