Basic equation of celestial mechanics:
dθ2d2u+u=mh2u2−f(1/u) (1)
Equation of lemniscate,
r2=a2cos2θ (2)
Put r=1/u in equation (2), we get
u21=a2cos2θ
⇒u=a1sec2θ (3)
Differentiating equation (3) with respect to θ , we get
dθdu=a1×2sec2θ1×sec2θ×tan2θ×2
⇒dθdu=a1sec2θ1/2tan2θ (4)
Again differentiating the above equation
dθ2d2u=a1(sec1/22θtan22θ+2sec5/22θ) (5)
Adding equation (3) and (5) we get
dθ2d2u+u=a1[sec1/22θ{tan22θ+1}+2sec5/22θ]
⇒dθ2d2u+u=a1[3sec5/22θ]
=3×a1×r5a5 from eq. (3) and (2)
=3a4r−5 (6)
Substituting value of equation (6) in (1)
3a4r−5=mh2r−2−f(r)
⇒f(r)=r7−3a4mh2
∴ The force f(r) will make a particle describe lemniscate shaped orbit.
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