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QJEEM18Phcf2b: JEE Main 2018 Physics - Class 11 JEEM18Phcf2b Solution: Take the mean distance of the moon and the sun from the earth…

Take the mean distance of the moon and the sun from the earth to be 0.4×1060.4 \times {10^6} km and 150×106150 \times {10^6} km respectively. Their masses are 8×10228 \times {10^{22}} kg and 2×10302 \times {10^{30}} kg respectively. The radius of the earth is 64006400 km. Let ΔF1\Delta {F_1} be the difference in the forces exerted by the moon at the nearest and farthest points on the earth and ΔF2\Delta {F_2} be the difference in the force exerted by the sun at the nearest and farthest points on the earth. Then, the number closest to ΔF1ΔF2{{\Delta {F_1}} \over {\Delta {F_2}}} is :

Multiple Choice Options

  • A 22
  • B 10−2{10^{ - 2}}
  • C 0.60.6
  • D 66

Step-by-Step Verified Solution

As gravitational force of attraction,

F = GMmR2{{GMm} \over {{R^2}}}

∴    \therefore\,\,\,\, Force of attraction berween earth and moon

F1 = GMemr12{{G{M_e}m} \over {r_1^2}}

Force of attraction between earth and sun,

F2 = GMeMsr22{{GMeMs} \over {r_2^2}}

∴    \therefore\,\,\,\, Δ\Delta F1 = −- 2GMemr13{{2G{M_e}m} \over {r_1^3}} Δ\Delta r1

Δ\Delta F2 = −- 2GMe Msr23{{2GMe\,Ms} \over {r_2^3}} Δ\Delta r2

∴    \therefore\,\,\,\, ΔF1ΔF2{{\Delta {F_1}} \over {\Delta {F_2}}} = mΔr1r13×r23Ms Δr2{{m\Delta {r_1}} \over {r_1^3}} \times {{r_2^3} \over {Ms\,\Delta {r_2}}}

= (mMs)(r23r13)(Δr1Δr2)\left( {{m \over {Ms}}} \right)\left( {{{r_2^3} \over {r_1^3}}} \right)\left( {{{\Delta {r_1}} \over {\Delta {r_2}}}} \right)

Δr1=Δr2\Delta {r_1} = \Delta {r_2} = diameter of the earth = 2 Rearth

Given

m = 8 ×\times 1022 kg

Ms = 2 ×\times 1030 kg

r1 = 0.4 ×\times 106 km

r2 = 150 ×\times 106 km

∴    \therefore\,\,\,\, ΔF1ΔF2=(8×10222×1030)(150×1060.4×106)3×1{{\Delta {F_1}} \over {\Delta {F_2}}} = \left( {{{8 \times {{10}^{22}}} \over {2 \times {{10}^{30}}}}} \right){\left( {{{150 \times {{10}^6}} \over {0.4 \times {{10}^6}}}} \right)^3} \times 1

= 2

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