UBC 240
0.62
UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
4.9 [arcmin]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 240 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 121.315 | -33.021 | 0.391 | -1.905 | 2.287 | 91.042 |
| Li et al. | 2025 | 121.312 | -33.036 | 0.363 | -1.911 | 2.281 | â |
| Hunt & Reffert | 2024 | 121.305 | -32.999 | 0.395 | -1.914 | 2.309 | â |
| Cavallo et al. | 2024 | 121.305 | -33.015 | 0.393 | â | â | â |
| Hunt & Reffert | 2023 | 121.305 | -32.999 | 0.395 | -1.914 | 2.309 | â |
| Cantat-Gaudin et al. | 2020 | 121.312 | -33.036 | 0.363 | -1.911 | 2.281 | â |
| Castro-Ginard et al. | 2020 | 121.321 | -33.038 | 0.366 | -1.907 | 2.283 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.16 | 0.88 | â | 630 | -0.054 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 376* | â | â |
| Cavallo et al. | 2024 | 2.31 | 1.58 | â | 191 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 2.34 | 1.12 | 1.05 | 197 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.61 | 1.05 | â | 135 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.