Saurer 5
Summary
Saurer 5 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, above the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
This object shares a significant percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 294.879 | 25.645 | – | -6.11 | 5.06 | – |
| Kharchenko et al. (2012) | 294.896 | 25.652 | – | -1.41 | -3.17 | – |
| Loktin & Popova (2017) | 294.885 | 25.652 | – | -1.397 | -4.444 | – |
| Bica et al. (2019) | 294.883 | 25.642 | – | – | – | – |
| UCC | 294.868 | 25.638 | 0.072 | -2.266 | -4.37 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.15, Dist=8329.0, Age=9.05 |
| Kharchenko et al. (2012) | e_bv=1.208, distance=5276, log_age=8.87 |
| Loktin & Popova (2017) | E(B-V)=0.677, Dist=2106, logt=8.4 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3858 | 68.0 | 294.87 | 25.64 | 0.07 | -2.15 | -4.26 | -75.92 | 0.41 |