HSC 2042

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0.24 UTI
0.26
CN
0.08
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.8 [pc], 0.4 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.08 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2042 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 130.065 -32.684 0.495 -5.562 3.196 –
Hu & Soubiran 2025 130.105 -32.731 – – – –
Hunt & Reffert 2024 130.056 -32.672 0.505 -5.545 3.2 63.134
Cavallo et al. 2024 130.105 -32.731 0.503 – – –
Hunt & Reffert 2023 130.056 -32.672 0.505 -5.545 3.2 63.134

💡 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– 1.91 0.7 0.94 349 -0.025 109 – –
Hu & Soubiran 2025 – – – – -0.160(5) – – –
Hunt & Reffert 2024 1.91 0.70 0.94 349 – 109(1) – –
Cavallo et al. 2024 1.75 0.63 – 1072 0.110 – – –
Hunt & Reffert 2023 1.91 0.70 0.94 348 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3011 96.2 130.08 -32.7 0.5 -5.56 3.2 – 0.05

💡 Note: The % column shows the percentage of members that HSC 2042 shares with each listed object.

Visualization

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