Luna is a pilot project initially focused on We He-3(He-3, 2p)He-4 cro
ss section measurement within the thermal energy region of the Sun (15
-27 keV). A compact high current 50 kV ion accelerator facility includ
ing a windowless gas target system, a beam calorimeter and four detect
or telescopes has been built, tested and installed underground at Labo
ratori Nazionali del Gran Sasso. In these conditions, thanks to the co
smic ray suppression, we could attain a background level of less than
1 event per week, a rate similar to the one expected from He-3(He-3, 2
p)He-4 at the lower edge of the Sun thermal energy region.