Theia 2488

Click to load Aladin Lite
0.12 UTI
0.39
CN
0.95
Cdens
0.5
CC3
0.25
Clit
0.26
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 0.95 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.26 Possibly duplicate

Overview

â„šī¸
Theia 2488 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 58.971 57.178 0.294 0.197 -0.679 -48.603
Hu & Soubiran 2025 58.996 57.167 – – – –
Hunt & Reffert 2024 58.978 57.188 0.289 0.165 -0.666 -49.278
Cavallo et al. 2024 58.996 57.167 0.293 – – –
Hunt & Reffert 2023 58.978 57.188 0.289 0.165 -0.666 -49.278

💡 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
Hu & Soubiran 2025 – – – – -0.140* – – –
Hunt & Reffert 2024 – – – – – 348* – –
Cavallo et al. 2024 2.81 1.59 – 575 -0.090 – – –
Hunt & Reffert 2023 3.12 1.42 0.96 521 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2703 74.4 58.98 57.19 0.3 0.21 -0.68 -54.5 0.36

💡 Note: The % column shows the percentage of members that Theia 2488 shares with each listed object.

Visualization

â„šī¸