UBC 285

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0.65 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 285 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 184.717 -65.425 0.564 -6.246 -0.694 -2.597
Li et al. 2025 184.671 -65.42 0.568 -6.242 -0.711 –
Hunt & Reffert 2024 184.675 -65.442 0.558 -6.248 -0.676 -9.067
Cavallo et al. 2024 184.747 -65.42 0.563 – – –
Hunt & Reffert 2023 184.675 -65.442 0.558 -6.248 -0.676 -9.067
Cantat-Gaudin et al. 2020 184.671 -65.42 0.568 -6.242 -0.711 –
Castro-Ginard et al. 2020 184.695 -65.419 0.568 -6.232 -0.713 –

💡 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 1.69 0.55 – 233 0.144 – – –
Hunt & Reffert 2024 – – – – – 592* – –
Cavallo et al. 2024 1.68 0.57 – 288 0.130 – – –
Hunt & Reffert 2023 1.68 0.52 0.64 259 – – – –
Cantat-Gaudin et al. 2020 1.64 0.45 – 62 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 13337 36.2 184.75 -65.42 0.56 -6.23 -0.66 -16.13 0.0

💡 Note: The % column shows the percentage of members that UBC 285 shares with each listed object.

Visualization

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