Theia 70

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0.48 UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.08
Clit
1.0
Cdup
Stellar density (N50/rad) 6.1 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.08 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 70 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

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

Palma et al. (2025)
Part of multiple system G204, along with Mamajek_2 and HSC_95.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.97 (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– 257.214 -18.019 4.774 -5.655 -11.507 -18.62
Swiggum et al. 2024 257.117 -18.209 4.764 -5.645 -11.39 -15.926
Cavallo et al. 2024 257.315 -17.624 4.762 – – –
Hunt & Reffert 2023 257.117 -18.209 4.764 -5.645 -11.39 -19.68
Kounkel & Covey 2019 257.243 -17.317 4.788 – – 3.511

💡 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– 0.21 0.59 1.16 16 0.190 62 – –
Swiggum et al. 2024 0.21 – – 16 – 62 – –
Cavallo et al. 2024 0.21 0.86 – 15 0.190 – – –
Hunt & Reffert 2023 0.21 0.49 1.16 16 – – – –
Kounkel & Covey 2019 0.21 0.59 – 26 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 2 88.9 257.33 -17.77 4.8 -5.66 -11.39 -16.51 0.07

💡 Note: The % column shows the percentage of members that Theia 70 shares with each listed object.

Visualization

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