FSR 0952
Summary
FSR 0952 is a poorly populated, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 13 years.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 92.562 | 13.013 | – | -2.79 | -1.23 | – |
| Froebrich et al. (2007) | 92.562 | 13.013 | – | – | – | – |
| Kharchenko et al. (2012) | 92.573 | 13.017 | – | -1.16 | -1.84 | – |
| UCC | 92.547 | 13.053 | 0.238 | -0.525 | -0.633 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.625, Dist=1994.0, Age=9.105 |
| Kharchenko et al. (2012) | e_bv=0.625, distance=1994, log_age=9.105 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 2471 | 79.3 | 92.57 | 12.9 | 0.25 | -0.49 | -0.65 | – | 0.25 |