UBC 492

Click to load Aladin Lite
0.00 UTI
0.45
CN
0.6
Cdens
0.75
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.6 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
UBC 492 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

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

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 148.715 -50.928 0.422 -6.847 5.054 11.126
Li et al. 2025 148.736 -50.951 0.39 -6.86 4.997 –
Almeida et al. 2025 148.733 -50.949 – – – –
Dias et al. 2021 148.733 -50.949 0.395 -6.874 5.035 –
Cantat-Gaudin et al. 2020 148.736 -50.951 0.39 -6.86 4.997 –
Castro-Ginard et al. 2020 148.74 -50.951 0.393 -6.87 5.023 –

💡 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 2.11 1.04 – 280 0.147 – – –
Almeida et al. 2025 2.25 1.41 – 112 – 212 – –
Dias et al. 2021 2.25 1.41 – 112 0.288 – – –
Cantat-Gaudin et al. 2020 2.63 1.26 – 59 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Collinder 213 100.0 148.69 -50.92 0.42 -6.85 5.05 11.13 0.63

💡 Note: The % column shows the percentage of members that UBC 492 shares with each listed object.

Visualization

â„šī¸