HSC 1722

Click to load Aladin Lite
0.28 UTI
0.45
CN
0.12
Cdens
0.75
CC3
0.06
Clit
0.96
Cdup
Core radius and density 3.2 [pc], 0.6 [pc-2]
  • CN 0.45 Poorly populated
  • Cdens 0.12 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 0.96 Unique

Overview

â„šī¸
HSC 1722 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Liu et al. (2025)
Classified as primordial binary cluster 205 along with HSC_1723, and of multiple system 58 along with HSC_1723, HSC_1721 and NGC_2311.

Palma et al. (2025)
Part of multiple system G128, along with HSC_1723 and HSC_1721.

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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.568 -4.75 0.429 -1.758 0.754 –
Liu et al. 2025 104.54 -4.75 0.43 -1.77 0.76 –
Hunt & Reffert 2024 104.541 -4.754 0.428 -1.769 0.756 –
Cavallo et al. 2024 104.593 -4.727 0.426 – – –
Hunt & Reffert 2023 104.541 -4.754 0.428 -1.769 0.756 –

💡 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– 2.1 1.185 2.08 58 0.150 351 – –
Liu et al. 2025 4.63 0.56 – 13 – – – –
Hunt & Reffert 2024 2.10 1.19 2.08 57 – 351(1) – –
Cavallo et al. 2024 2.01 1.18 – 79 0.150 – – –
Hunt & Reffert 2023 2.10 1.19 2.08 58 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 2311 4.4 104.45 -4.61 0.45 -1.31 1.0 32.11 0.9

💡 Note: The % column shows the percentage of members that HSC 1722 shares with each listed object.

Visualization

â„šī¸