OCSN 65

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0.58 UTI
0.81
CN
1.0
Cdens
1.0
CC3
0.35
Clit
0.82
Cdup
Stellar density (N50/rad) 16.4 [N/pc2]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.35 Poorly studied
  • Cdup 0.82 Very likely unique

Overview

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OCSN 65 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Liu et al. (2025)
Classified as primordial binary cluster 321 along with Theia_13, and of multiple system 3 along with ASCC_18, Sigma_Orionis, CWNU_1054 and Theia_13.

Palma et al. (2025)
Part of multiple system G229, along with OCSN_56, Theia_13, CWNU_1072, Sigma_Orionis, CWNU_1088, ASCC_18 and OCSN_68.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 83.789 -1.805 2.366 -1.311 0.921 27.08
Liu et al. 2025 83.76 -2.16 2.36 -1.26 0.93 33.16
Zhang et al. 2024 83.764 -2.155 – – – –
Hunt & Reffert 2024 83.764 -2.155 2.365 -1.258 0.93 33.161
Cavallo et al. 2024 83.749 -1.836 2.362 – – –
Hunt & Reffert 2023 83.764 -2.155 2.365 -1.258 0.93 33.161
Qin et al. 2023 83.88 -1.79 2.37 -1.34 0.93 26.34

💡 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– 0.46 0.475 0.58 14 -0.162 52 – –
Liu et al. 2025 0.48 0.14 – 19 – – – –
Zhang et al. 2024 – – – – -0.133(1) – – –
Hunt & Reffert 2024 – – – – – 52(1) – –
Cavallo et al. 2024 0.44 0.85 – 5 -0.190 – – –
Hunt & Reffert 2023 0.41 0.36 0.58 13 – – – –
Qin et al. 2023 0.52 0.59 – 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 6 17.6 83.34 -1.63 2.41 -0.07 -0.24 28.06 0.69
OCSN 194 14.5 83.32 -1.64 2.42 -0.06 -0.25 28.06 0.02
OCSN 61 0.4 84.06 -0.59 2.56 -1.03 -0.63 29.9 0.52

💡 Note: The % column shows the percentage of members that OCSN 65 shares with each listed object.

Visualization

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