NGC 2243
(Melotte 46; Collinder 98; MWSC 880; OCL 644; ESO 426 16; FSR 1296; FoF 3)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Nm (P>50%)
1336
Core radius and density
1.4 [pc], 29 [pc-2]
- 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 2243 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, well below 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, age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 97.393 | -31.283 | 0.227 | -1.263 | 5.5 | 60.162 |
| Otto et al. | 2026 | 97.396 | -31.283 | â | -1.28 | 5.49 | 59.9 |
| Li et al. | 2025 | 97.395 | -31.282 | 0.211 | -1.279 | 5.488 | â |
| Guerco et al. | 2025 | 97.4 | -31.3 | 0.22 | -1.24 | 5.5 | 60.0 |
| Hu & Soubiran | 2025 | 97.39 | -31.281 | â | â | â | â |
| Carrasco-Varela et al. | 2025 | 97.539 | -31.317 | â | â | â | â |
| Almeida et al. | 2025 | 97.392 | -31.283 | â | â | â | â |
| Hunt & Reffert | 2024 | 97.396 | -31.283 | 0.223 | -1.267 | 5.494 | 59.993 |
| Cavallo et al. | 2024 | 97.39 | -31.281 | 0.221 | â | â | â |
| Rain et al. | 2024 | 97.393 | -31.284 | 0.222 | -1.263 | 5.493 | â |
| Hunt & Reffert | 2023 | 97.396 | -31.283 | 0.223 | -1.267 | 5.494 | 59.993 |
| Angelo et al. | 2023 | 97.383 | -31.285 | â | -1.26 | 5.5 | â |
| Just et al. | 2023 | 97.387 | -31.284 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 97.395 | -31.282 | â | â | â | â |
| Jaehnig et al. | 2021 | 97.396 | -31.284 | 0.241 | -1.287 | 5.498 | â |
| Netopil et al. | 2022 | 97.392 | -31.283 | â | â | â | 60.02 |
| Rain et al. | 2021 | 97.395 | -31.282 | 0.211 | -1.279 | 5.488 | â |
| Dias et al. | 2021 | 97.392 | -31.283 | 0.217 | -1.282 | 5.489 | 59.611 |
| Spina et al. | 2021 | 97.394 | -31.282 | 0.216 | -1.285 | 5.494 | â |
| Cantat-Gaudin et al. | 2020 | 97.395 | -31.282 | 0.211 | -1.279 | 5.488 | â |
| Donor et al. | 2020 | 97.392 | -31.285 | â | -1.28 | 5.5 | 59.8 |
| Cantat-Gaudin & Anders | 2020 | 97.395 | -31.282 | 0.211 | -1.279 | 5.488 | â |
| Liu & Pang | 2019 | 97.385 | -31.279 | 0.257 | -1.261 | 5.493 | â |
| Soubiran et al. | 2018 | 97.395 | -31.282 | â | â | â | 59.63 |
| Bica et al. | 2019 | 97.397 | -31.283 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 97.395 | -31.282 | 0.211 | -1.279 | 5.488 | â |
| Dias et al. | 2018 | â | â | â | -2.41 | 4.61 | â |
| Loktin & Popova | 2017 | 97.395 | -31.282 | â | -0.49 | 4.02 | 55.0 |
| Sampedro et al. | 2017 | 97.392 | -31.283 | â | -0.54 | 3.36 | â |
| Kharchenko et al. | 2016 | 97.387 | -31.284 | â | â | â | â |
| Netopil et al. | 2016 | 97.392 | -31.283 | â | â | â | â |
| Dias et al. | 2014 | 97.392 | -31.283 | â | -0.48 | 4.02 | â |
| Kharchenko et al. | 2013 | 97.392 | -31.285 | â | -2.81 | 4.09 | 55.0 |
| Gozha et al. | 2012 | 97.392 | -31.283 | â | â | â | â |
| Bukowiecki et al. | 2011 | 97.388 | -31.278 | â | â | â | â |
| Kharchenko et al. | 2007 | 97.39 | -31.28 | â | 0.04 | â | â |
| Ahumada & Lapasset | 2007 | 97.4 | -31.283 | â | â | â | â |
| van den Bergh | 2006 | 97.392 | -31.283 | â | â | â | â |
| Chen et al. | 2003 | 97.449 | -31.287 | â | â | â | â |
| Dias et al. | 2002 | 97.392 | -31.283 | â | -0.49 | 4.02 | 59.84 |
| Lynga | 1987 | 97.449 | -31.287 | â | â | â | â |
| Sulentic et al. | 1973 | 97.437 | -31.284 | 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 | 4.17 | 0.16 | 0.35 | 3183 | -0.460 | 4401 | 0.16 | 8 |
| Otto et al. | 2026 | â | â | â | 4365 | -0.460(15) | â | â | â |
| Li et al. | 2025 | 4.03 | 0.24 | â | 3136 | -0.386 | â | â | â |
| Guerco et al. | 2025 | â | â | â | 4370 | -0.480 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.380(5) | â | â | â |
| Carrasco-Varela et al. | 2025 | 4.00 | 0.27 | â | 3443 | -0.450 | â | â | 6(1) |
| Almeida et al. | 2025 | 4.00 | 0.27 | â | 3443 | â | 3681 | â | â |
| Hunt & Reffert | 2024 | 3.95 | 0.03 | 0.35 | 2748 | â | 5121(1) | â | â |
| Cavallo et al. | 2024 | 2.91 | 0.67 | â | 3890 | -0.940 | â | â | â |
| Rain et al. | 2024 | 4.08 | 0.00 | â | 3426 | â | 9279 | 0.16 | â |
| Hunt & Reffert | 2023 | 3.95 | 0.03 | 0.35 | 2748 | â | â | â | â |
| Angelo et al. | 2023 | 3.80 | 0.32 | â | 3548 | -0.470 | 13(1) | â | â |
| Just et al. | 2023 | â | â | â | 1365 | â | 1832 | â | â |
| Spina et al. | 2022 | â | â | â | â | -0.460 | â | â | â |
| Jadhav & Subramaniam | 2021 | 3.72 | 0.02 | â | 4365 | â | 7576 | â | 8(1) |
| Jaehnig et al. | 2021 | 4.29(1) | â | â | â | â | â | â | â |
| Netopil et al. | 2022 | 3.53(1) | â | â | 4786 | -0.460(1) | â | â | â |
| Rain et al. | 2021 | 4.17 | 0.16 | â | 1072 | â | â | â | 14 |
| Dias et al. | 2021 | 4.00 | 0.27 | â | 3443 | -0.482 | â | â | â |
| Spina et al. | 2021 | 4.34 | â | â | 4365 | -0.472(20) | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.72 | 0.02 | â | 4365 | â | â | â | â |
| Kounkel et al. | 2020 | 4.51 | 0.35 | â | 1698 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.460 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.17 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 3390 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 4.17 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.17 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 4.88 | 0.19 | â | 1076 | â | â | â | â |
| Kharchenko et al. | 2016 | 4.45 | 0.20 | â | 1365 | â | â | â | â |
| Netopil et al. | 2016 | 10.51 | â | â | 3230 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.45 | 0.20 | â | 1365 | -0.490 | â | â | â |
| Gozha et al. | 2012 | 4.46 | â | â | 1076 | -0.490 | â | â | â |
| Bukowiecki et al. | 2011 | 4.45(1) | 0.00 | â | 1413 | â | â | â | â |
| Paunzen et al. | 2010 | â | â | â | â | -0.570 | â | â | â |
| Ahumada & Lapasset | 2007 | â | 0.16 | â | 1072 | â | â | â | 9 |
| van den Bergh | 2006 | 4.46 | 0.16 | â | 1072 | â | â | â | â |
| Chen et al. | 2003 | 4.46 | 0.16 | â | 1070 | -0.440(1) | â | â | â |
| Dias et al. | 2002 | 4.46 | 0.16 | â | 1076 | -0.420 | â | â | â |
| Lynga | 1987 | 3.58 | 0.00 | â | 6026 | -0.550 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Rain et al. (2024)
This cluster hosts only a few BSSs. Those offset from the ZAMS are consistent with binary evolution, with some appearing as evolved binaries, though not yet classified as YSSs.
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1102, e_all=0.1768.
Rain et al. (2021)
Best fit with log(t)=9.5