Riddle 4
(MWSC 167)
0.91
UTI
0.55
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
1.8 [arcmin]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Riddle 4 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
High 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 | 31.862 | 60.259 | 0.345 | -0.791 | -0.491 | -44.579 |
| Li et al. | 2025 | 31.862 | 60.26 | 0.339 | -0.757 | -0.451 | â |
| Almeida et al. | 2025 | 31.858 | 60.263 | â | â | â | â |
| Hunt & Reffert | 2024 | 31.85 | 60.262 | 0.354 | -0.806 | -0.499 | -25.266 |
| Celli et al. | 2024 | 31.862 | 60.26 | â | â | â | â |
| Cavallo et al. | 2024 | 31.83 | 60.27 | 0.352 | â | â | â |
| Hunt & Reffert | 2023 | 31.85 | 60.262 | 0.354 | -0.806 | -0.499 | -25.266 |
| Just et al. | 2023 | 31.848 | 60.269 | â | â | â | â |
| Dias et al. | 2021 | 31.858 | 60.263 | 0.349 | -0.764 | -0.474 | â |
| Cantat-Gaudin et al. | 2020 | 31.862 | 60.26 | 0.339 | -0.757 | -0.451 | â |
| Cantat-Gaudin & Anders | 2020 | 31.862 | 60.26 | 0.339 | -0.757 | -0.451 | â |
| Dias et al. | 2019 | 31.846 | 60.257 | 0.337 | -0.761 | -0.523 | -30.388 |
| Soubiran et al. | 2018 | 31.862 | 60.26 | â | â | â | -34.08 |
| Cantat-Gaudin et al. | 2018 | 31.862 | 60.26 | 0.339 | -0.757 | -0.451 | â |
| Loktin & Popova | 2017 | 31.845 | 60.257 | â | 0.414 | -1.534 | â |
| Kharchenko et al. | 2016 | 31.848 | 60.269 | â | â | â | â |
| Kharchenko et al. | 2013 | 31.86 | 60.271 | â | 1.01 | -1.1 | â |
| Kharchenko et al. | 2012 | 31.86 | 60.271 | â | 1.01 | -1.1 | â |
| Kronberger et al. | 2006 | 31.845 | 60.257 | â | â | â | â |
| Dias et al. | 2002 | 31.846 | 60.257 | â | 9.08 | -6.01 | 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 | 2.23 | 2.99 | â | 535 | -0.126 | â | â | â |
| Almeida et al. | 2025 | 2.64 | 3.04 | â | 11 | â | 328 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 819* | â | â |
| Celli et al. | 2024 | â | â | â | 27 | â | 392 | â | â |
| Cavallo et al. | 2024 | 3.03 | 3.04 | â | 35 | 0.690 | â | â | â |
| Hunt & Reffert | 2023 | 2.69 | 3.29 | 0.76 | 15 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 22 | â | 11 | â | â |
| Dias et al. | 2021 | 2.64 | 3.04 | â | 11 | -0.109 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.08 | 3.01 | â | 27 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.72 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 2.27 | 2.29 | â | 21 | -1.623 | â | â | â |
| Soubiran et al. | 2018 | 2.72 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.72 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.80 | 2.13 | â | 219 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.20 | 3.25 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.20 | 3.25 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.20 | 3.25 | â | 22 | â | â | â | â |
| Dias et al. | 2002 | 2.80 | 3.41 | â | 40 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.