Bohr Orbit Radius and Energy — From Intuition to Formula
Imagine an electron trapped near a nucleus. It wants to fall in because of the electric attraction, but if it moved like a classical planet it would spiral inward, radiating energy and crashing. Bohr’s genius was to say: no, the electron can only live in certain allowed orbits — and in those orbits it does not radiate. That’s the starting point.
Why would orbits be fixed? Bohr borrowed an idea from waves. If you tie a string in a loop, only certain wavelengths fit smoothly around it. Similarly, the electron’s wave nature means its orbit must contain an integer number of wavelengths. That integer is n, the principal quantum number (n=1,2,3,…). The smallest orbit (n=1) is the ground state; larger n means higher energy, farther out.
Radius of the nth orbit
For a hydrogen-like atom (one electron, nuclear charge +Ze), the Coulomb force provides the centripetal force:
r2kZe2=rmv2
where k=4πε01 and m is the electron mass. Bohr’s quantization condition says the angular momentum is an integer multiple of ℏ=h/2π:
mvr=nℏ
Solve these two equations together. From the second, v=nℏ/(mr). Substitute into the first:
r2kZe2=rm(mrnℏ)2=mr3n2ℏ2
Multiply both sides by r3 and rearrange:
r=kmZe2n2ℏ2
Define the Bohr radius a0=kme2ℏ2≈0.529A˚ (the radius of the n=1 orbit for hydrogen, Z=1). Then:
rn=Zn2a0
The radius grows as n2 — the n=2 orbit is four times larger than n=1, n=3 is nine times larger, and so on. For higher Z, the stronger pull shrinks all orbits by 1/Z.
Energy of the nth orbit
Total energy = kinetic + potential. For a Coulomb force, K=21mv2 and U=−rkZe2 (negative because the force is attractive; zero at infinity). Using the force equation kZe2/r2=mv2/r, we get mv2=kZe2/r, so:
K=21rkZe2,U=−rkZe2
Hence:
E=K+U=−21rkZe2
Now substitute rn from above:
En=−21(n2/Z)a0kZe2=−2a0kZ2e2⋅n21
The constant 2a0ke2 is the Rydberg energy Ry≈13.6eV. So:
En=−n2Z2(13.6eV)
For hydrogen (Z=1): E1=−13.6 eV, E2=−3.4 eV, E3=−1.51 eV, … approaching zero as n→∞.
The negative sign means the electron is bound. The most negative energy (deepest well) is the ground state n=1. As n increases, energy becomes less negative — the electron is less tightly bound. At n=∞, E=0, the atom is ionized.
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