NGC 3324
0.85
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Nm (P>50%)
180
Core radius and density
1.3 [pc], 8.6 [pc-2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
NGC 3324 is a rich, very dense 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, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 159.333 | -58.623 | 0.373 | -7.082 | 2.798 | -21.009 |
| Liu et al. | 2025 | 159.33 | -58.62 | 0.38 | -7.1 | 2.8 | 111.46 |
| Almeida et al. | 2025 | 159.372 | -58.625 | â | â | â | â |
| Hunt & Reffert | 2024 | 159.325 | -58.624 | 0.379 | -7.096 | 2.804 | 111.458 |
| Celli et al. | 2024 | 159.341 | -58.615 | â | â | â | â |
| Cavallo et al. | 2024 | 159.33 | -58.63 | 0.381 | â | â | â |
| Hunt & Reffert | 2023 | 159.325 | -58.624 | 0.379 | -7.096 | 2.804 | 111.458 |
| Jaehnig et al. | 2021 | 159.341 | -58.632 | 0.398 | -7.21 | 3.067 | â |
| Rain et al. | 2021 | 159.341 | -58.615 | 0.356 | -7.112 | 2.782 | â |
| Dias et al. | 2021 | 159.372 | -58.625 | 0.351 | -7.128 | 2.767 | â |
| Cantat-Gaudin et al. | 2020 | 159.341 | -58.615 | 0.356 | -7.112 | 2.782 | â |
| Cantat-Gaudin & Anders | 2020 | 159.341 | -58.615 | 0.356 | -7.112 | 2.782 | â |
| Cantat-Gaudin et al. | 2018 | 159.341 | -58.615 | 0.356 | -7.112 | 2.782 | â |
| Dias et al. | 2018 | â | â | â | -7.59 | 2.92 | â |
| Loktin & Popova | 2017 | 159.33 | -58.641 | â | -7.46 | 3.11 | -7.7 |
| Sampedro et al. | 2017 | 159.333 | -58.642 | â | -4.22 | -0.95 | â |
| Dias et al. | 2014 | 159.333 | -58.642 | â | -5.44 | -1.31 | â |
| Gozha et al. | 2012 | 159.333 | -58.642 | â | â | â | â |
| Bukowiecki et al. | 2011 | 159.312 | -58.621 | â | â | â | â |
| Piskunov et al. | 2008 | 159.318 | -58.639 | â | â | â | â |
| Kharchenko et al. | 2007 | 159.33 | -58.64 | â | 0.16 | â | -8.5 |
| Ahumada & Lapasset | 2007 | 159.325 | -58.65 | â | â | â | â |
| van den Bergh | 2006 | 159.325 | -58.633 | â | â | â | â |
| Kharchenko et al. | 2005 | 159.33 | -58.64 | â | -7.81 | 3.77 | -8.5 |
| Kharchenko et al. | 2003 | 159.31 | -58.62 | â | -12.2 | 5.07 | â |
| Dias et al. | 2002 | 159.333 | -58.642 | â | -7.46 | 3.11 | -8.5 |
| Dambis | 1999 | 159.333 | -58.642 | â | â | â | â |
| Lynga | 1987 | 159.337 | -58.622 | â | â | â | -12.0 |
đĄ 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 | 99999â | 2.42 | 1.45 | 1.69 | 6 | -0.040 | 444 | â | 0 |
| Liu et al. | 2025 | 2.49 | 0.55 | â | 8 | â | â | â | â |
| Almeida et al. | 2025 | 2.49 | 1.64 | â | 6 | â | 416 | â | â |
| Hunt & Reffert | 2024 | 2.40 | 1.90 | 1.69 | 6 | â | 383(1) | â | â |
| Celli et al. | 2024 | â | â | â | 11 | â | 444 | â | â |
| Cavallo et al. | 2024 | 2.04 | 1.30 | â | 8 | -0.040 | â | â | â |
| Hunt & Reffert | 2023 | 2.40 | 1.90 | 1.69 | 6 | â | â | â | â |
| Jaehnig et al. | 2021 | 2.52(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.60 | 1.36 | â | 6 | â | â | â | 0 |
| Dias et al. | 2021 | 2.49 | 1.64 | â | 6 | 0.294 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.39 | 1.19 | â | 11 | â | â | â | â |
| Kounkel et al. | 2020 | 2.62 | 2.28 | â | 2 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.60 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.60 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.30 | 1.45 | â | 6 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 1306 | â | â |
| Gozha et al. | 2012 | 2.32 | â | â | 6 | â | 2692 | â | â |
| Bukowiecki et al. | 2011 | 2.44(1) | 1.58 | â | 10 | â | â | â | â |
| Piskunov et al. | 2008 | 2.30 | 1.45 | â | 5 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 1.39 | â | 6 | â | â | â | 0 |
| van den Bergh | 2006 | 2.32 | 1.39 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.30 | 1.45 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2003 | 2.33 | 1.39 | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.32 | 1.38 | â | 6 | -0.474 | â | â | â |
| Dambis | 1999 | 2.55 | 1.48 | â | 3 | â | â | â | â |
| Lynga | 1987 | 3.30 | 1.36 | â | 2 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 225 along with HSC_2342, and of multiple system 64 along with IC_2581 and HSC_2342.
Palma et al. (2025)
Part of multiple system G151, along with HSC_2358, HSC_2342 and IC_2581.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2022, e_all=0.1851.
Ahumada & Lapasset (2007)
The dereddened colour-magnitude diagram in (1977A&AS...27..145C) was examined. The apparent cluster diameter is also from (1977A&AS...27..145C).