Q.If the law of gravitation, instead of being inverse-square law, becomes an inverse-cube law- (Note: more than one of the given options may be correct.)
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Start your 14-day free trial to unlock the full solution →Under an inverse-cube force law, closed elliptical orbits become impossible (Bertrand's theorem restricts closed orbits to inverse-square and Hooke's-law forces), so planets can no longer trace ellipses — option (A) is correct. Circular orbits remain mathematically possible for any power law (just unstable, not impossible) — so (B) is false. Near Earth's surface, the field is still nearly uniform over a hand-thrown stone's tiny trajectory regardless of the force law's form, so motion stays parabolic — option (C) is correct. The shell theorem (zero field inside a uniform shell) is special to the inverse-square law and fails for inverse-cube — so (D) is false.
(A) Elliptical orbits
Stable, closed orbits (ones that retrace the same path every revolution) exist only for very special force laws — a result known as Bertrand's theorem, which shows this happens only for the inverse-square law (, giving Kepler's ellipses) and Hooke's law (). For an inverse-cube law, the effective radial potential no longer has the right shape to produce a stable closed elliptical path — orbits instead spiral in or spiral out. So planets will not have elliptic orbits under an inverse-cube law. (A) is correct.
(B) Circular orbits
A circular orbit only requires that the gravitational force at radius supply exactly the centripetal force needed for that radius:
This equation has a valid solution for every — a circular orbit is mathematically possible at any radius. What changes under the inverse-cube law is stability: a small radial nudge doesn't oscillate back (as it does for inverse-square orbits) but instead grows, so the orbit is unstable, not impossible. Since option (B) claims circular orbits are not possible (rather than merely unstable), it is false.
(C) Projectile motion near Earth's surface …
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