UBC 631

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0.20 UTI
0.0
CN
0.02
Cdens
0.75
CC3
0.13
Clit
1.0
Cdup
Core radius and density 3.6 [pc], 0.08 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.75 High quality
  • Clit 0.13 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 631 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Almeida et al. (2025)
Mass determination: intermediate 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 99999– 112.709 -14.161 0.193 -1.401 1.641 –
Li et al. 2025 112.709 -14.148 0.195 -1.381 1.633 –
Almeida et al. 2025 112.709 -14.141 – – – –
Dias et al. 2021 112.709 -14.141 0.194 -1.4 1.651 –
Cantat-Gaudin et al. 2020 112.709 -14.148 0.195 -1.381 1.633 –
Castro-Ginard et al. 2020 112.714 -14.144 0.193 -1.387 1.631 –

💡 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] Bfrac BSS
UCC 99999– 4.81 1.505 – 24 -0.103 516 – –
Li et al. 2025 4.80 0.79 – 519 -0.041 – – –
Almeida et al. 2025 4.82 1.56 – 10 – 516 – –
Dias et al. 2021 4.82 1.56 – 10 -0.166 – – –
Kounkel et al. 2020 4.66 1.45 – 39 – – – –

Visualization

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