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
N50 (P>50% members)
1336
Stellar density (N50/rad)
50.7 [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 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 |
| 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 |
| Loktin & Popova | 2017 | 97.395 | -31.282 | â | -0.49 | 4.02 | 55.0 |
| Kharchenko et al. | 2016 | 97.387 | -31.284 | 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 | 3136 | -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 | â | â | â | â | 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 |
| 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 |
| 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 |
| 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.
Rain et al. (2021)
Best fit with log(t)=9.5