FSR 1484
(MWSC 1677)
0.79
UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
3.5 [arcmin]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1484 is a moderately populated, very dense object of 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, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is 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 | 142.458 | -50.705 | 0.424 | -5.13 | 3.603 | 12.395 |
| Almeida et al. | 2025 | 142.452 | -50.689 | â | â | â | â |
| Hunt & Reffert | 2024 | 142.447 | -50.7 | 0.42 | -5.129 | 3.617 | 10.076 |
| Cavallo et al. | 2024 | 142.466 | -50.707 | 0.426 | â | â | â |
| Hunt & Reffert | 2023 | 142.447 | -50.7 | 0.42 | -5.129 | 3.617 | 10.076 |
| Almeida et al. | 2023 | 142.463 | -50.687 | â | â | â | â |
| Just et al. | 2023 | 142.44 | -50.679 | â | â | â | â |
| Dias et al. | 2021 | 142.452 | -50.689 | 0.412 | -5.166 | 3.55 | â |
| Cantat-Gaudin et al. | 2020 | 142.452 | -50.697 | 0.406 | -5.154 | 3.537 | â |
| Cantat-Gaudin & Anders | 2020 | 142.452 | -50.697 | 0.406 | -5.154 | 3.537 | â |
| Bica et al. | 2019 | 142.447 | -50.679 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 142.452 | -50.697 | 0.406 | -5.154 | 3.537 | â |
| Kharchenko et al. | 2016 | 142.44 | -50.679 | â | â | â | â |
| Kharchenko et al. | 2013 | 142.446 | -50.682 | â | -3.86 | 9.24 | â |
| Froebrich et al. | 2007 | 142.446 | -50.682 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.00 | 2.46 | â | 367 | â | 239 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 679* | â | â |
| Cavallo et al. | 2024 | 2.37 | 3.24 | â | 174 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 2.18 | 2.88 | 1.43 | 231 | â | â | â | â |
| Almeida et al. | 2023 | 2.07 | 2.83 | â | 262 | 0.052 | 263* | 0.72 | â |
| Just et al. | 2023 | â | â | â | 442 | â | 67 | â | â |
| Dias et al. | 2021 | 2.00 | 2.46 | â | 367 | 0.165 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.37 | 2.25 | â | 437 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.30 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.30 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.85 | 2.58 | â | 442 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.85 | 2.58 | â | 442 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.