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What must the separation be between a 5....

What must the separation be between a 5.2 kg particle and a 2.4 kg particle for their gravitational attraction to have a magnitude of `2.3 xx 10^(-12)` N?

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To find the separation between a 5.2 kg particle and a 2.4 kg particle for their gravitational attraction to have a magnitude of \(2.3 \times 10^{-12}\) N, we can use Newton's law of gravitation. The formula for gravitational force is given by: \[ F_g = \frac{G \cdot M_1 \cdot M_2}{R^2} \] Where: - \(F_g\) is the gravitational force, - \(G\) is the gravitational constant (\(6.67 \times 10^{-11} \, \text{N m}^2/\text{kg}^2\)), - \(M_1\) is the mass of the first particle (5.2 kg), - \(M_2\) is the mass of the second particle (2.4 kg), - \(R\) is the separation between the two masses. ### Step-by-Step Solution: 1. **Identify the known values**: - \(M_1 = 5.2 \, \text{kg}\) - \(M_2 = 2.4 \, \text{kg}\) - \(F_g = 2.3 \times 10^{-12} \, \text{N}\) - \(G = 6.67 \times 10^{-11} \, \text{N m}^2/\text{kg}^2\) 2. **Rearrange the formula to solve for \(R\)**: \[ R^2 = \frac{G \cdot M_1 \cdot M_2}{F_g} \] Therefore, \[ R = \sqrt{\frac{G \cdot M_1 \cdot M_2}{F_g}} \] 3. **Substitute the known values into the equation**: \[ R = \sqrt{\frac{(6.67 \times 10^{-11}) \cdot (5.2) \cdot (2.4)}{2.3 \times 10^{-12}}} \] 4. **Calculate the numerator**: \[ (6.67 \times 10^{-11}) \cdot (5.2) \cdot (2.4) = 8.33976 \times 10^{-10} \] 5. **Calculate \(R^2\)**: \[ R^2 = \frac{8.33976 \times 10^{-10}}{2.3 \times 10^{-12}} = 3.628 \times 10^{2} \] 6. **Take the square root to find \(R\)**: \[ R = \sqrt{3.628 \times 10^{2}} \approx 19.03 \, \text{m} \] 7. **Final answer**: The separation \(R\) must be approximately \(19 \, \text{m}\).
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Knowledge Check

  • Assuming a particle to have the form of a sphere and to absorb all incident light, the radius (in mm) of a particle for which its gravitational attraction to the Sun is Counterbalanced by the force that light exerts on it is------. The power of light radiated by the sun equals P=4xx10^(26)W and the density of the particle is r=1.0 g//cm^(3) . Use G=(20)/(3)xx10^(-11)Nm^(2)//kg^(2) , pi=(25)/(8) and mass of the sun =2xx10^(30)kg

    A
    `0.8`
    B
    `0.6`
    C
    `0.1`
    D
    `0.4`
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