UBC 609

Click to load Aladin Lite
0.18 UTI
0.0
CN
0.09
Cdens
0.38
CC3
0.31
Clit
0.84
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 0.84 Very likely unique

Overview

â„šī¸
UBC 609 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Massive Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 65.226 53.046 0.224 0.459 -0.726 –
Almeida et al. 2025 65.263 53.226 – – – –
Celli et al. 2024 65.262 53.069 – – – –
Dias et al. 2021 65.263 53.226 0.192 0.471 -0.642 -49.94
Cantat-Gaudin et al. 2020 65.262 53.069 0.198 0.474 -0.667 –
Castro-Ginard et al. 2020 65.217 53.187 0.199 0.478 -0.654 –

💡 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 3.90 2.58 – 5 – 2216 – –
Celli et al. 2024 – – – 6 – 2887 – –
Dias et al. 2021 3.90 2.58 – 5 -0.248 – – –
Cantat-Gaudin et al. 2020 3.65 2.38 – 6 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Mayer 2 16.0 65.0 53.16 0.25 0.31 -0.72 -25.2 0.06

💡 Note: The % column shows the percentage of members that UBC 609 shares with each listed object.

Visualization

â„šī¸