Theia 128

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0.25 UTI
0.25
CN
0.31
Cdens
0.62
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.0 [pc], 1.6 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.31 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 128 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Palma et al. (2025)
Classified as optical pair P571, along with Theia_546.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.98 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 108.651 -7.682 1.996 -8.461 2.171 22.953
Cavallo et al. 2024 108.684 -7.639 1.994 – – –
Hunt & Reffert 2023 108.653 -7.694 1.992 -8.399 2.23 31.15
Kounkel & Covey 2019 109.804 -7.695 1.489 – – 6.74

💡 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– 0.5 0.4 0.46 45 0.270 – – –
Cavallo et al. 2024 0.50 0.40 – 38 0.270 – – –
Hunt & Reffert 2023 0.48 0.15 0.46 96 – – – –
Kounkel & Covey 2019 0.67 0.63 – 45 – – – –

Visualization

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