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Three identical point mass each of mass ...

Three identical point mass each of mass 1kg lie in the x-y plane at point (0,0), (0,0.2m) and (0.2m, 0). The net gravitational force on the mass at the origin is

A

`1.67xx10^(-9)(hati+hatj)N`

B

`3.34xx10^(-10)(hati+hatj)N`

C

`1.67xx10^(-9)(hati-hatj)N`

D

`3.34xx10^(-10)(hati+hatj)N`

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The correct Answer is:
To solve the problem of finding the net gravitational force on the mass at the origin due to the other two masses, we can follow these steps: ### Step 1: Identify the positions of the masses We have three identical point masses, each with a mass of 1 kg, located at: - Mass A at (0, 0) (the origin) - Mass B at (0, 0.2 m) - Mass C at (0.2 m, 0) ### Step 2: Calculate the gravitational force exerted on the mass at the origin by Mass B The gravitational force \( F \) between two point masses is given by the formula: \[ F = \frac{G \cdot m_1 \cdot m_2}{r^2} \] Where: - \( G = 6.67 \times 10^{-11} \, \text{N m}^2/\text{kg}^2 \) (gravitational constant) - \( m_1 = 1 \, \text{kg} \) (mass at the origin) - \( m_2 = 1 \, \text{kg} \) (mass B) - \( r \) is the distance between the two masses, which is \( 0.2 \, \text{m} \). Calculating the force due to Mass B: \[ F_B = \frac{6.67 \times 10^{-11} \cdot 1 \cdot 1}{(0.2)^2} = \frac{6.67 \times 10^{-11}}{0.04} = 1.6675 \times 10^{-9} \, \text{N} \] This force acts in the negative y-direction (downward). ### Step 3: Calculate the gravitational force exerted on the mass at the origin by Mass C Now, we calculate the gravitational force exerted by Mass C: - The distance \( r \) between the mass at the origin and Mass C is also \( 0.2 \, \text{m} \). Calculating the force due to Mass C: \[ F_C = \frac{6.67 \times 10^{-11} \cdot 1 \cdot 1}{(0.2)^2} = \frac{6.67 \times 10^{-11}}{0.04} = 1.6675 \times 10^{-9} \, \text{N} \] This force acts in the negative x-direction (to the left). ### Step 4: Determine the net gravitational force on the mass at the origin The net gravitational force \( \vec{F}_{net} \) on the mass at the origin is the vector sum of the forces due to Mass B and Mass C: \[ \vec{F}_{net} = \vec{F}_B + \vec{F}_C \] Expressing this in vector form: \[ \vec{F}_{net} = -1.6675 \times 10^{-9} \hat{j} - 1.6675 \times 10^{-9} \hat{i} \] ### Step 5: Final Result Thus, the net gravitational force on the mass at the origin is: \[ \vec{F}_{net} = -1.6675 \times 10^{-9} \hat{i} - 1.6675 \times 10^{-9} \hat{j} \, \text{N} \]

To solve the problem of finding the net gravitational force on the mass at the origin due to the other two masses, we can follow these steps: ### Step 1: Identify the positions of the masses We have three identical point masses, each with a mass of 1 kg, located at: - Mass A at (0, 0) (the origin) - Mass B at (0, 0.2 m) - Mass C at (0.2 m, 0) ...
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