**59.** Radius of the first excited state of Helium ion is given as: \( a_0 \rightarrow \) radius of first stationary state of hydrogen atom. Options: - (1) \( r = \frac{a_0}{2} \) - (2) \( r = \frac{a_0}{4} \) - (3) \( r = 4a_0 \) - (4) \( r = 2a_0 \)

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Published July 8, 2025
Physics
Modern Physics
Atomic Structure
Bohr Model

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Detailed Explanation

Key Ideas to Know

  1. Bohr Radius (a0a_0)
    The radius of the ground state (n=1n = 1) of the hydrogen atom.

  2. Bohr Model for Hydrogen-Like Species
    For any one-electron ion (H, He⁺, Li²⁺ …) the radius of the nthn^{\text{th}} orbit is

    rn=n2a0Zr_n = \frac{n^2 a_0}{Z}

    where
    nn = principal quantum number (1, 2, 3 …)
    ZZ = nuclear charge (1 for H, 2 for He⁺, 3 for Li²⁺ …).

  3. First Excited State
    Means n=2n = 2 (because the ground state is n=1n = 1).


Reasoning Chain a Student Should Follow

  1. Identify Z: For He⁺, Z=2Z = 2.

  2. Identify n: First excited state → n=2n = 2.

  3. Plug into Formula:

    r=(2)2a02r = \frac{(2)^2 a_0}{2}

  4. Simplify:

    r=4a02=2a0r = \frac{4 a_0}{2} = 2a_0

  5. Match Option: Option (4) is the correct one.

Each step is chosen directly from Bohr’s radius formula, tailored to a hydrogen-like ion with higher nuclear charge.

Simple Explanation (ELI5)

Imagine Planets and Orbits

Think of an atom like a mini-solar system. The electron is the planet, and the nucleus is the Sun. For hydrogen, the very first circular path (orbit) has a special size called Bohr radius and we name it a0a_0.

Now, a helium ion (He⁺) is like hydrogen but the Sun is twice as strong (because its charge is +2 instead of +1). When the planet jumps to the next bigger orbit (first excited state), you simply ask:

  1. How big is that orbit for hydrogen?
  2. How does a stronger Sun pull the planet closer?

The math answer says the new size is 2a02a_0. So the helium planet’s first excited circle is exactly twice the Bohr radius.

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Step-by-Step Solution

Step-by-Step Solution

  1. Write Bohr Radius Formula for Hydrogen-Like Ion

rn=n2a0Zr_n = \frac{n^2 a_0}{Z}

  1. Insert Helium Ion Data
    Nuclear charge: Z=2Z = 2
    First excited state: n=2n = 2

  2. Substitute

r=(2)2a02r = \frac{(2)^2 a_0}{2}

  1. Calculate

r=4a02=2a0r = \frac{4a_0}{2} = 2a_0

  1. Select Correct Option
    Option (4) r=2a0r = 2a_0 is correct.

Examples

Example 1

Satellite orbits: Higher gravitational pull (larger mass planet) shrinks orbit radii for the same orbital energy.

Example 2

Electron capture therapy: Heavy nuclei pull electrons closer, influencing transition energies in medical isotope design.

Example 3

Spectroscopy of ionized gases in nebulae: Sizes of orbits dictate emission line wavelengths when single-electron ions transition.

Visual Representation

References

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