GLIMPSE 17
(Mercer 17)
Summary
GLIMPSE 17 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.4) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 287.331 | 8.197 | – | – | – | – |
| UCC | 287.27 | 8.115 | 0.124 | -2.142 | -4.542 | 40.509 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| MCM 17 | 60.0 | 287.31 | 8.17 | 0.11 | -2.15 | -4.52 | 50.86 | 0.08 |