UBC 487

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0.64 UTI
0.37
CN
1.0
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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UBC 487 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 and metallicity parameters (see Parameters). It is moderately studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 139.681 -51.6 0.525 -5.784 4.158 –
Li et al. 2025 139.691 -51.6 0.499 -5.812 4.14 –
Almeida et al. 2025 139.748 -51.603 – – – –
Hunt & Reffert 2024 139.681 -51.588 0.528 -5.787 4.181 –
Celli et al. 2024 139.691 -51.6 – – – –
Cavallo et al. 2024 139.705 -51.609 0.53 – – –
Hunt & Reffert 2023 139.681 -51.588 0.528 -5.787 4.181 –
Dias et al. 2021 139.748 -51.603 0.476 -5.806 4.127 –
Cantat-Gaudin et al. 2020 139.691 -51.6 0.499 -5.812 4.14 –
Castro-Ginard et al. 2020 139.716 -51.6 0.499 -5.807 4.126 –

💡 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 1.62 1.84 – 128 -0.045 – – –
Almeida et al. 2025 1.85 1.94 – 19 – 297 – –
Hunt & Reffert 2024 – – – – – 298* – –
Celli et al. 2024 – – – 26 – 205 – –
Cavallo et al. 2024 1.91 1.38 – 123 0.650 – – –
Hunt & Reffert 2023 1.81 1.99 1.58 24 – – – –
Dias et al. 2021 1.85 1.94 – 19 0.194 – – –
Cantat-Gaudin et al. 2020 1.83 1.39 – 26 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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