NGC 743
(MWSC 154; FoF 2228)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
8.8 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 743 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 29.618 | 60.119 | 0.911 | -0.057 | -1.74 | -20.46 |
| Li et al. | 2025 | 29.614 | 60.13 | 0.881 | -0.03 | -1.708 | â |
| Almeida et al. | 2025 | 29.618 | 60.132 | â | â | â | â |
| Hunt & Reffert | 2024 | 29.664 | 60.152 | 0.919 | -0.06 | -1.715 | -18.318 |
| Cavallo et al. | 2024 | 29.82 | 60.163 | 0.916 | â | â | â |
| Hunt & Reffert | 2023 | 29.664 | 60.152 | 0.919 | -0.06 | -1.715 | -18.318 |
| Almeida et al. | 2023 | 29.591 | 60.133 | â | â | â | â |
| Just et al. | 2023 | 29.644 | 60.154 | â | â | â | â |
| He et al. | 2022 | 29.697 | 60.12 | 0.917 | -0.075 | -1.727 | â |
| Tarricq et al. | 2022 | 29.589 | 60.106 | 0.89 | -0.072 | -1.685 | â |
| Dias et al. | 2021 | 29.618 | 60.132 | 0.882 | -0.036 | -1.702 | â |
| Cantat-Gaudin et al. | 2020 | 29.614 | 60.13 | 0.881 | -0.03 | -1.708 | â |
| Cantat-Gaudin & Anders | 2020 | 29.614 | 60.13 | 0.881 | -0.03 | -1.708 | â |
| Liu & Pang | 2019 | 29.62 | 60.126 | 0.896 | -0.077 | -1.647 | â |
| Soubiran et al. | 2018 | 29.614 | 60.13 | â | â | â | -18.16 |
| Cantat-Gaudin et al. | 2018 | 29.614 | 60.13 | 0.881 | -0.03 | -1.708 | â |
| Loktin & Popova | 2017 | 29.655 | 60.155 | â | -1.04 | -2.16 | -6.5 |
| Kharchenko et al. | 2016 | 29.644 | 60.154 | â | â | â | â |
| Dias et al. | 2014 | 29.654 | 60.155 | â | -1.04 | -2.16 | â |
| Kharchenko et al. | 2013 | 29.655 | 60.157 | â | -1.81 | -2.77 | -6.5 |
| Kharchenko et al. | 2012 | 29.655 | 60.157 | â | -1.81 | -2.77 | -6.5 |
| Dias et al. | 2002 | 29.654 | 60.155 | â | -1.04 | -2.16 | -6.5 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.03 | 1.54 | â | 42 | 0.155 | â | â | â |
| Almeida et al. | 2025 | 1.06 | 1.80 | â | 110 | â | 225 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 532* | â | â |
| Cavallo et al. | 2024 | 1.16 | 1.79 | â | 35 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 1.04 | 1.48 | 1.95 | 56 | â | â | â | â |
| Almeida et al. | 2023 | 1.04 | 1.77 | â | 67 | 0.001 | 178* | 0.68 | â |
| Just et al. | 2023 | â | â | â | 195 | â | 59 | â | â |
| He et al. | 2022 | â | 1.90 | â | 40 | â | â | â | â |
| Tarricq et al. | 2022 | 1.14 | â | â | 115 | â | â | â | â |
| Dias et al. | 2021 | 1.06 | 1.80 | â | 110 | 0.039 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.17 | 1.40 | â | 100 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.10 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 29 | -0.250 | â | â | â |
| Soubiran et al. | 2018 | 1.10 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.10 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.96 | 2.08 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.10 | 1.40 | â | 195 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.10 | 1.40 | â | 195 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.10 | 1.40 | â | 195 | â | â | â | â |
| Dias et al. | 2002 | 1.62 | 2.94 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.