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Asked in GUJCET 2022 · Bohr's rules in other systems
Given: m=6×10²⁴ kg, v=3×10⁴ m s⁻¹, r=1.5×10¹¹ m.
Idea: Bohr's condition mvr=(nh)/(2π) applied to the earth gives n=(2π mvr)/h.
mvr=6×10²⁴×3×10⁴×1.5×10¹¹=2.7×10⁴⁰ kg m² s⁻¹.
n=(2×3.14×2.7×10⁴⁰)/(6.625×10⁻³⁴)=2.56×10⁷⁴≈2.6×10⁷⁴.
A quantum number this large means neighbouring allowed orbits are indistinguishable, which is why quantisation is never noticed for planets.
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