NGC 7281
(MWSC 3624)
0.86
UTI
0.56
CN
0.73
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
6.1 [arcmin]
- CN 0.56 Moderately populated
- Cdens 0.73 Moderately dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7281 is a moderately populated, moderately dense object of very 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, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 336.274 | 57.895 | 0.427 | -2.083 | -1.276 | -26.713 |
| Li et al. | 2025 | 336.259 | 57.869 | 0.432 | -2.123 | -1.238 | â |
| Almeida et al. | 2025 | 336.279 | 57.871 | â | â | â | â |
| Hunt & Reffert | 2024 | 336.261 | 57.834 | 0.419 | -2.076 | -1.305 | -26.703 |
| Cavallo et al. | 2024 | 336.442 | 57.953 | 0.422 | â | â | â |
| Hunt & Reffert | 2023 | 336.261 | 57.834 | 0.419 | -2.076 | -1.305 | -26.703 |
| Just et al. | 2023 | 336.26 | 57.817 | â | â | â | â |
| Dias et al. | 2021 | 336.279 | 57.871 | 0.438 | -2.122 | -1.227 | â |
| Cantat-Gaudin et al. | 2020 | 336.259 | 57.869 | 0.432 | -2.123 | -1.238 | â |
| Cantat-Gaudin & Anders | 2020 | 336.259 | 57.869 | 0.432 | -2.123 | -1.238 | â |
| Bossini et al. | 2019 | 336.259 | 57.869 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 336.259 | 57.869 | 0.432 | -2.123 | -1.238 | â |
| Loktin & Popova | 2017 | 336.255 | 57.817 | â | -1.347 | -0.571 | â |
| Kharchenko et al. | 2016 | 336.26 | 57.817 | â | â | â | â |
| Dias et al. | 2014 | 336.325 | 57.817 | â | -2.13 | -3.19 | â |
| Kharchenko et al. | 2013 | 336.265 | 57.82 | â | -1.56 | -2.44 | â |
| Kharchenko et al. | 2012 | 336.265 | 57.82 | â | -1.56 | -2.44 | â |
| Piskunov et al. | 2008 | 336.315 | 57.815 | â | â | â | â |
| Piskunov et al. | 2007 | 336.315 | 57.815 | â | â | â | â |
| Kharchenko et al. | 2005 | 336.33 | 57.82 | â | -0.46 | -2.41 | â |
| Kharchenko et al. | 2003 | 336.28 | 57.84 | â | 1.29 | -4.39 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.98 | 1.65 | â | 22 | -0.045 | â | â | â |
| Almeida et al. | 2025 | 2.01 | 1.71 | â | 27 | â | 238 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 515* | â | â |
| Cavallo et al. | 2024 | 2.47 | 1.67 | â | 78 | 0.520 | â | â | â |
| Hunt & Reffert | 2023 | 2.20 | 1.60 | 1.16 | 68 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 72 | â | 131 | â | â |
| Dias et al. | 2021 | 2.01 | 1.71 | â | 27 | 0.064 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.25 | 1.44 | â | 35 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.17 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 2.38 | 1.51 | â | 30 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.17 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.01 | 0.94 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.60 | 1.55 | â | 72 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.60 | 1.55 | â | 72 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.60 | 1.55 | â | 72 | â | â | â | â |
| Piskunov et al. | 2008 | 1.62 | 1.55 | â | 72 | â | 312* | â | â |
| Piskunov et al. | 2007 | 1.62 | 1.55 | â | 72 | â | 40 | â | â |
| Kharchenko et al. | 2005 | 1.62 | 1.55 | â | 72 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.83 | 1.24 | â | â | 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.
Cavallo et al. (2024)
Gold sample.