Ferrero 10
(MWSC 1059)
0.14
UTI
0.41
CN
0.04
Cdens
0.38
CC3
0.25
Clit
0.51
Cdup
Nm (P>50%)
41
Core radius and density
7.8 [pc], 0.2 [pc-2]
- CN 0.41 Poorly populated
- Cdens 0.04 Very loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 0.51 Likely unique
Overview
Ferrero 10 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.
(*): The parallax distance estimate (~2.28 kpc) differs significantly from the median photometric distance (~4.85 kpc).
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 105.194 | -3.051 | 0.438 | -1.286 | 0.638 | 83.927 |
| Bica et al. | 2019 | 105.113 | -3.012 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -1.41 | 0.3 | â |
| Loktin & Popova | 2017 | 105.12 | -3.009 | â | -0.422 | 0.191 | â |
| Sampedro et al. | 2017 | 105.112 | -3.01 | â | 1.64 | 5.26 | â |
| Dias et al. | 2016 | 105.112 | -3.01 | â | 0.22 | 5.57 | â |
| Dias et al. | 2014 | 105.112 | -3.01 | â | 0.22 | 5.57 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 4.85 | 1.08 | â | 550 | â | â | â | â |
| Loktin & Popova | 2017 | 4.85 | 1.08 | â | 550 | â | â | â | â |
MOCA

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). Asterisms reported by amateur astronomers in the web. Asterisms and clusters by L. Ferrero.