Alessi 175
0.08
UTI
0.0
CN
0.03
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
18
Core radius and density
5.3 [pc], 0.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Alessi 175 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 108.953 | -0.701 | 0.239 | -0.822 | 0.425 | 86.771 |
| Bica et al. | 2019 | 108.974 | -0.719 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
MOCA

Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.