NGC 2360
(Melotte 64; Collinder 134; MWSC 1165; OCL 589; FSR 1225; FoF 2083)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1227
Stellar density (N50/rad)
86.2 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 2360 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with 2 later reported entries. 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 | 109.44 | -15.631 | 0.917 | 0.376 | 5.628 | 27.693 |
| Malhotra et al. | 2026 | 109.441 | -15.639 | â | â | â | â |
| Li et al. | 2025 | 109.443 | -15.631 | 0.902 | 0.383 | 5.603 | â |
| Hu & Soubiran | 2025 | 109.436 | -15.633 | â | â | â | â |
| Wei et al. | 2025 | 109.44 | -15.635 | 0.918 | 0.382 | 5.63 | â |
| Almeida et al. | 2025 | 109.44 | -15.63 | â | â | â | â |
| Hunt & Reffert | 2024 | 109.441 | -15.644 | 0.917 | 0.385 | 5.629 | 27.246 |
| Cavallo et al. | 2024 | 109.436 | -15.633 | 0.916 | â | â | â |
| Hunt & Reffert | 2023 | 109.441 | -15.644 | 0.917 | 0.385 | 5.629 | 27.246 |
| Almeida et al. | 2023 | 109.438 | -15.628 | â | â | â | â |
| Angelo et al. | 2023 | 109.463 | -15.629 | â | 0.39 | 5.63 | â |
| Cordoni et al. | 2023 | 109.44 | -15.63 | 0.9 | 0.389 | 5.608 | â |
| Just et al. | 2023 | 109.419 | -15.638 | â | â | â | â |
| He et al. | 2022 | 109.435 | -15.635 | 0.918 | 0.389 | 5.634 | â |
| Tarricq et al. | 2022 | 109.44 | -15.639 | 0.924 | 0.376 | 5.63 | â |
| Jadhav & Subramaniam | 2021 | 109.443 | -15.631 | â | â | â | â |
| Jaehnig et al. | 2021 | 109.444 | -15.637 | 0.931 | 0.363 | 5.591 | â |
| Rain et al. | 2021 | 109.443 | -15.631 | 0.902 | 0.383 | 5.603 | â |
| Dias et al. | 2021 | 109.44 | -15.63 | 0.9 | 0.389 | 5.608 | 28.386 |
| Cantat-Gaudin et al. | 2020 | 109.443 | -15.631 | 0.902 | 0.383 | 5.603 | â |
| Cantat-Gaudin & Anders | 2020 | 109.443 | -15.631 | 0.902 | 0.383 | 5.603 | â |
| Liu & Pang | 2019 | 109.442 | -15.626 | 0.903 | 0.393 | 5.595 | â |
| Soubiran et al. | 2018 | 109.443 | -15.631 | â | â | â | 28.3 |
| Bica et al. | 2019 | 109.455 | -15.654 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 109.443 | -15.631 | 0.902 | 0.383 | 5.603 | â |
| Loktin & Popova | 2017 | 109.425 | -15.641 | â | -1.792 | 6.032 | 25.5 |
| Kharchenko et al. | 2016 | 109.419 | -15.638 | â | â | â | â |
| Dias et al. | 2014 | 109.429 | -15.642 | â | -1.51 | 5.27 | â |
| Kharchenko et al. | 2013 | 109.425 | -15.64 | â | -2.3 | 6.6 | 25.5 |
| Gozha et al. | 2012 | 109.429 | -15.642 | â | â | â | â |
| Bukowiecki et al. | 2011 | 109.433 | -15.631 | â | â | â | â |
| Piskunov et al. | 2008 | 109.422 | -15.637 | â | â | â | â |
| Kharchenko et al. | 2007 | 109.42 | -15.64 | â | 0.25 | â | 25.47 |
| Piskunov et al. | 2007 | 109.422 | -15.637 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 109.425 | -15.65 | â | â | â | â |
| van den Bergh | 2006 | 109.425 | -15.633 | â | â | â | â |
| Kharchenko et al. | 2005 | 109.42 | -15.64 | â | -2.62 | 4.89 | 25.47 |
| Kharchenko et al. | 2003 | 109.44 | -15.63 | â | -2.6 | 4.82 | â |
| Chen et al. | 2003 | 109.436 | -15.63 | â | 3.51 | 8.07 | 27.2 |
| Dias et al. | 2002 | 109.429 | -15.642 | â | -3.51 | 8.07 | 27.28 |
| Lynga | 1987 | 109.431 | -15.633 | â | â | â | â |
| Sulentic et al. | 1973 | 109.409 | -15.646 | â | â | â | â |
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 | 1.1 | 0.35 | 0.34 | 1000 | -0.083 | 1316 | 0.41 | 0 |
| Malhotra et al. | 2026 | 1.08 | 0.31 | â | 1074 | -0.030 | â | â | â |
| Li et al. | 2025 | 1.02 | 0.41 | â | 1361 | -0.175 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.210(5) | â | â | â |
| Wei et al. | 2025 | 1.11 | 0.49 | â | 1410 | -0.250 | 1589 | 0.30 | â |
| Almeida et al. | 2025 | 1.05 | 0.41 | â | 1268 | â | 1671 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2771(1) | â | â |
| Cavallo et al. | 2024 | 1.09 | 0.35 | â | 1175 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.01 | 0.12 | 0.34 | 1452 | â | â | â | â |
| Almeida et al. | 2023 | 1.04 | 0.40 | â | 1276 | -0.083 | 1327(1) | 0.41 | â |
| Angelo et al. | 2023 | 0.95 | 0.38 | â | 1413 | -0.220 | 8(1) | â | â |
| Cordoni et al. | 2023 | 1.05 | 0.41 | â | 1268 | -0.045 | 1656 | 0.41 | 0(1) |
| Just et al. | 2023 | â | â | â | 447 | â | 543 | â | â |
| He et al. | 2022 | â | 0.55 | â | 891 | â | â | â | â |
| Tarricq et al. | 2022 | 1.09 | â | â | 1000 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 1.12 | 0.39 | â | 1023 | â | 3104 | â | 0(1) |
| Jaehnig et al. | 2021 | 1.07(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.07 | 0.03 | â | 631 | â | â | â | 1 |
| Dias et al. | 2021 | 1.05 | 0.41 | â | 1268 | -0.045 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.12 | 0.39 | â | 1023 | â | â | â | â |
| Kounkel et al. | 2020 | 1.07 | 0.62 | â | 891 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.07 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1410 | -0.250 | â | â | â |
| Soubiran et al. | 2018 | 1.07 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.07 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.89 | 0.35 | â | 592 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.56 | 1.31 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.56 | 1.31 | â | 447 | -0.030 | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 1305 | â | â |
| Gozha et al. | 2012 | 1.89 | â | â | 561 | -0.030 | 1000 | â | â |
| Bukowiecki et al. | 2011 | 1.17(1) | 0.00 | â | 1413 | â | â | â | â |
| Piskunov et al. | 2008 | 1.89 | 0.35 | â | 389 | â | 955(1) | â | â |
| Piskunov et al. | 2007 | 1.89 | 0.35 | â | 389 | â | 255 | â | â |
| Ahumada & Lapasset | 2007 | â | 0.35 | â | 562 | â | â | â | 4 |
| van den Bergh | 2006 | 1.89 | 0.35 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.89 | 0.35 | â | 389 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.89 | 0.35 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.89 | 0.35 | â | 560 | -0.150(1) | â | â | â |
| Dias et al. | 2002 | 1.12 | 0.03 | â | 631 | -0.030 | â | â | â |
| Lynga | 1987 | 1.63 | 0.19 | â | 1288 | -0.130 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Malhotra et al. (2026)
Lowest/Highest stellar mass in the catalogue with a mass-ratio estimate: 0.49/1.81 Msun
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Ahumada & Lapasset (2007)
Stars 51 and 100 are cited as blue stragglers in (1968ApJ...152...83E) and (1994AJ....108.1828M). The last reference also considers stars 1, 69, and 82 (WEBDA numbers) as stragglers. Adopted cluster centre: star 46 (1968ApJ...152...83E).