Six stars of equal mass m are moving about the centre of mass of the system such they are always on the vertices of a regular hexagon of side length a. Their common time period will be
2π√4√3a3Gm(5√3+4)
→F=−→F1+−→F2+−→F3+−→F4+−→F5
|−→F2|=|−→F5| and |−→F2|=|−→F4|
→F=−→F3+2F2cos30∘+2F1cos60∘
F3=Gm24a2; F2=Gm23a2; F1=Gm2a2
F=Gm2a2(54+1√3)=mω2a
ω=√Gma3(54+1√3); T=2π√4√3a3Gm(5√3+4)