FSR 1284
(MWSC 1176)
0.85
UTI
0.59
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.59 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1284 is a moderately populated, very dense 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 near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity 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 | 109.992 | -24.535 | 0.392 | -0.958 | 1.381 | 59.665 |
| Li et al. | 2025 | 109.992 | -24.535 | 0.392 | -0.983 | 1.357 | â |
| Almeida et al. | 2025 | 109.986 | -24.525 | â | â | â | â |
| Hunt & Reffert | 2024 | 109.992 | -24.538 | 0.391 | -0.95 | 1.386 | 59.669 |
| Cavallo et al. | 2024 | 109.989 | -24.521 | 0.393 | â | â | â |
| Hunt & Reffert | 2023 | 109.992 | -24.538 | 0.391 | -0.95 | 1.386 | 59.669 |
| Almeida et al. | 2023 | 109.986 | -24.524 | â | â | â | â |
| Just et al. | 2023 | 109.989 | -24.528 | â | â | â | â |
| Dias et al. | 2021 | 109.986 | -24.525 | 0.391 | -0.995 | 1.358 | â |
| Cantat-Gaudin et al. | 2020 | 109.992 | -24.535 | 0.392 | -0.983 | 1.357 | â |
| Cantat-Gaudin & Anders | 2020 | 109.992 | -24.535 | 0.392 | -0.983 | 1.357 | â |
| Soubiran et al. | 2018 | 109.992 | -24.535 | â | â | â | 42.2 |
| Cantat-Gaudin et al. | 2018 | 109.992 | -24.535 | 0.392 | -0.983 | 1.357 | â |
| Kharchenko et al. | 2016 | 109.989 | -24.528 | â | â | â | â |
| Kharchenko et al. | 2013 | 109.995 | -24.53 | â | -2.01 | 6.06 | â |
| Froebrich et al. | 2007 | 110.004 | -24.526 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.28 | 1.01 | â | 762 | -0.055 | â | â | â |
| Almeida et al. | 2025 | 2.25 | 1.08 | â | 778 | â | 201 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 356* | â | â |
| Cavallo et al. | 2024 | 2.98 | 1.12 | â | 490 | 0.700 | â | â | â |
| Hunt & Reffert | 2023 | 2.41 | 0.52 | 1.06 | 769 | â | â | â | â |
| Almeida et al. | 2023 | 2.32 | 1.05 | â | 762 | -0.045 | 195* | 0.67 | â |
| Just et al. | 2023 | â | â | â | 1396 | â | 63 | â | â |
| Dias et al. | 2021 | 2.25 | 1.08 | â | 778 | -0.076 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.33 | 0.84 | â | 589 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.38 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.38 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.38 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.94 | 0.64 | â | 1396 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.94 | 0.64 | â | 1396 | 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.