Find the value of I , the orbital angular momentum quantum number, for the moon when it is a . a distance of 3 . 6 9 × 1 0 8 m from earth. The extremely large value obtained implies that it is impossible to tell the difference between adjacent quantized orbits for macroscopic objects. I
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Find the value of I , the orbital angular momentum quantum number, for the moon when it is a . a distance of 3 . 6 9 × 1 0 8 m from earth. The extremely large value obtained implies that it is impossible to tell the difference between adjacent quantized orbits for macroscopic objects. I
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Asked by: Govind Prajapati
Created at: 2025-11-14 01:20:28
Asked by: Govind Prajapati
Created at: 2025-11-14 01:20:28
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# Orbital Angular Momentum Quantum Number (\( l \)) for the Moon
We are to find the orbital angular momentum quantum number (\( l \)) for the Moon when it is at a distance of \( r = 3.69 \times 10^8 \) m from Earth.
## Step 1: Classical Angular Momentum
The **classical angular momentum** of the Moon in its orbit is:
\[
L = m v r
\]
Where:
- \( m \) = mass of Moon (\( 7.35 \times 10^{22 \) kg)
- \( v \) = orbital speed of Moon
- \( r \) = orbital radius (\(3.69 \times 10^8 \) m)
The Moon’s average orbital speed is about \( v = 1.02 \times 103 \) m/s.
Plug in values:
\[
L = (7.35 \times 10^{22} \text{ kg}) \cdot (1.02 \times 10^3 \text{ m/s}) \cdot (3.69 \times 10^8 \text{ m})
\]
\[
L \approx 2.77 \times 10^{34} \text{ kg m}^2/\text{s}
\]
## Step 2: Quantization of Angular Momentum
In quantum mechanics, the angular momentum is quantized:
\[
L = \sqrt{l(l+1)} \hbar
\]
For very large \( l \), \( \sqrt{l(l+1)} \approx l \). Thus,
\[
l \approx \frac{L}{\hbar}
\]
Where \( \hbar = 1.055 \times 10^{-34} \) J·s.
## Step 3: Calculate \( l \)
\[
l \approx \frac{2.77 \times 10^{34}}{1.055 \times 10^{-34}}
\]
\[
l \approx 2.63 \times 10^{68}
\]
## Step 4: Interpretation
- The quantum number \( l \) for the Moon is **enormously large**: \( \approx 2.6 \times 10^{68} \).
- The difference between adjacent quantum levels (\( \Delta l = 1 \)) is completely unobservable for such macroscopic systems.
---
**Summary Table**
| Quantity | Value |
|------------------|----------------------------|
| Distance \( r \) | \( 3.69 \times 10^8 \) m |
| Mass \( m \) | \( 7.35 \times 10^{22} \) kg|
| Speed \( v \) | \( 1.02 \times 10^3 \) m/s |
| \( \hbar \) | \( 1.055 \times 10^{-34} \) J·s |
| Quantum \( l \) | \( \approx 2.6 \times 10^{68} \) |
---
## Conclusion
**The orbital angular momentum quantum number \( l \) for the Moon is approximately \( 2.6 \times 10^{68} \). For macroscopic objects, the quantization of angular momentum is indistinguishable from a continuum.**
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