UBC 385

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0.00 UTI
0.35
CN
1.0
Cdens
1.0
CC3
0.38
Clit
0.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.38 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
UBC 385 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young 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.

Close Moderate extinction Near-solar metallicity Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 317.944 60.023 1.176 -2.531 -3.506 -17.856
Li et al. 2025 317.94 60.092 1.178 -2.53 -3.468 –
Alfonso et al. 2024 318.434 59.506 1.116 -2.553 -3.558 –
Celli et al. 2024 317.94 60.092 – – – –
He et al. 2022 317.952 60.014 1.187 -2.521 -3.517 –
Cantat-Gaudin et al. 2020 317.94 60.092 1.178 -2.53 -3.468 –
Castro-Ginard et al. 2020 317.945 60.077 1.18 -2.538 -3.466 –

💡 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 0.74 1.33 – 11 -0.140 – – –
Alfonso et al. 2024 0.87 1.20 – 41 0.010 – – –
Celli et al. 2024 – – – 20 – 142 – –
He et al. 2022 – 1.55 – 8 – – – –
Cantat-Gaudin et al. 2020 0.87 1.20 – 19 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Riddle 6 100.0 318.03 59.9 1.17 -2.53 -3.51 -23.22 0.65
OC 0158 14.3 318.24 59.51 1.16 -2.54 -3.51 -24.65 0.02
CWNU 1192 5.7 318.54 59.41 1.16 -2.51 -3.5 -25.37 0.02

💡 Note: The % column shows the percentage of members that UBC 385 shares with each listed object.

Visualization

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