NGC 1333

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0.48 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.39
Clit
0.68
Cdup
Core radius and density 0.8 [pc], 25 [pc-2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.39 Poorly studied
  • Cdup 0.68 Likely unique

Overview

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NGC 1333 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 moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.

Note: This is likely a unique object, which shares a moderate 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 188 along with HSC_1250, and as primordial binary cluster 305 along with OC_0279, and of multiple system 52 along with HSC_1250 and OC_0279.

Palma et al. (2025)
Part of multiple system G108, along with OC_0279 and HSC_1250.

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.96 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.3838, e_all=0.2388.

Lada & Lada (2003)
Embedded cluster within âˆŧ2 Kpc of the Sun.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 52.278 31.27 3.376 7.389 -9.286 10.82
Liu et al. 2025 52.33 31.36 3.37 6.84 -9.71 21.02
Alfonso et al. 2024 52.256 31.263 3.315 7.368 -9.253 –
Cavallo et al. 2024 52.342 31.35 3.378 – – –
Hunt & Reffert 2023 52.328 31.358 3.372 6.836 -9.711 21.016
He et al. 2022 58.508 32.516 3.523 6.203 -9.731 –
Spina et al. 2021 52.297 31.31 3.305 7.352 -9.962 –
Cantat-Gaudin et al. 2020 52.297 31.31 3.344 7.425 -9.865 –
Zhong et al. 2020 52.297 31.31 – 7.425 -9.865 15.904
Cantat-Gaudin & Anders 2020 52.297 31.31 3.344 7.425 -9.865 –
Soubiran et al. 2018 52.297 31.31 – – – 1.92
Cantat-Gaudin et al. 2018 52.297 31.31 3.344 7.425 -9.865 –
Joshi et al. 2016 52.23 31.37 – – – –
Lada & Lada 2003 53.034 31.517 – – – –

💡 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– 0.3 2.35 1.38 11 0.132 79 – –
Liu et al. 2025 0.33 0.44 – 17 – – – –
Alfonso et al. 2024 0.30 2.12 – 11 0.132 – – –
Cavallo et al. 2024 0.42 3.28 – 13 0.320 – – –
Hunt & Reffert 2023 0.29 2.58 1.38 5 – – – –
He et al. 2022 – 0.85 – 18 – – – –
Spina et al. 2021 0.30 – – 11 – – – –
Cantat-Gaudin et al. 2020 0.30 2.12 – 11 – – – –
Kounkel et al. 2020 0.32 3.53 – 7 – – – –
Zhong et al. 2020 0.30(1) – – – -0.050 – – –
Cantat-Gaudin & Anders 2020 0.30 – – – – – – –
Soubiran et al. 2018 0.30 – – – – – – –
Cantat-Gaudin et al. 2018 0.30 – – – – – – –
Joshi et al. 2016 0.32 3.91 – 6 – – – –
Lada & Lada 2003 0.32 – – – – 79 – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 223 60.6 52.24 31.28 3.38 7.41 -9.59 8.45 0.0
NGC 1333NE 31.9 52.29 31.34 3.36 6.82 -9.82 30.81 0.5
NGC 1333SW 28.7 52.28 31.32 3.36 6.82 -9.77 16.54 0.49
CWWDL 14545 17.5 51.33 30.95 3.37 8.08 -8.19 9.62 0.03
HSC 1250 15.6 52.44 31.08 3.39 7.54 -8.24 9.46 0.0

💡 Note: The % column shows the percentage of members that NGC 1333 shares with each listed object.

Visualization

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