UBC 663

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0.14 UTI
0.0
CN
0.12
Cdens
0.75
CC3
0.25
Clit
0.52
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.52 Likely unique

Overview

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UBC 663 is a sparse, very loose 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, very young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Very young

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 182.722 -63.635 0.393 -5.713 -0.032 –
Li et al. 2025 182.773 -63.626 0.361 -5.724 -0.053 –
Almeida et al. 2025 182.746 -63.631 – – – –
Dias et al. 2021 182.746 -63.631 0.38 -5.721 -0.039 –
Cantat-Gaudin et al. 2020 182.773 -63.626 0.361 -5.724 -0.053 –

💡 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 2.27 0.96 – 18 0.153 – – –
Almeida et al. 2025 2.72 1.35 – 7 – 375 – –
Dias et al. 2021 2.72 1.35 – 7 0.105 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 517 48.0 182.52 -63.8 0.41 -5.68 0.02 – 0.53

💡 Note: The % column shows the percentage of members that UBC 663 shares with each listed object.

Visualization

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