FSR 1698
(MWSC 2289)
0.63
UTI
0.52
CN
0.31
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
5.8 [arcmin]
- CN 0.52 Moderately populated
- Cdens 0.31 Loose
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1698 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Relatively close
Moderate extinction
Massive
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 | 230.233 | -59.622 | 0.285 | -3.923 | -3.585 | 51.426 |
| Almeida et al. | 2025 | 230.234 | -59.627 | â | â | â | â |
| Hunt & Reffert | 2024 | 230.233 | -59.622 | 0.289 | -3.901 | -3.576 | 51.566 |
| Cavallo et al. | 2024 | 230.251 | -59.607 | 0.29 | â | â | â |
| Hunt & Reffert | 2023 | 230.233 | -59.622 | 0.289 | -3.901 | -3.576 | 51.566 |
| Just et al. | 2023 | 230.228 | -59.618 | â | â | â | â |
| Dias et al. | 2021 | 230.234 | -59.627 | 0.248 | -4.028 | -3.531 | â |
| Kharchenko et al. | 2016 | 230.228 | -59.618 | â | â | â | â |
| Dias et al. | 2014 | 230.242 | -59.628 | â | -6.07 | -4.12 | â |
| Kharchenko et al. | 2013 | 230.241 | -59.62 | â | -5.19 | -2.3 | â |
| Froebrich et al. | 2007 | 230.242 | -59.628 | â | â | â | â |
| Dias et al. | 2002 | 230.242 | -59.628 | â | -6.07 | -4.12 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.12 | 2.91 | â | 14 | â | 1022 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1130* | â | â |
| Cavallo et al. | 2024 | 2.90 | 3.16 | â | 32 | 0.570 | â | â | â |
| Hunt & Reffert | 2023 | 3.07 | 3.23 | 2.33 | 12 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 363 | â | 199 | â | â |
| Dias et al. | 2021 | 3.12 | 2.91 | â | 14 | 0.228 | â | â | â |
| Kharchenko et al. | 2016 | 1.56 | 2.71 | â | 363 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.56 | 2.71 | â | 363 | â | â | â | â |
| Dias et al. | 2002 | 1.56 | 2.71 | â | 363 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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