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How far from earth must a body be along ...

How far from earth must a body be along a line towards the sun so that the sun's gravitational pull on it balances that of the earth . Distance between sun and earth's centre is `1.5 xx 10^(10)` km . Mass of the sun is `3.24 xx 10^(5)` times mass of the earth .

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To find the distance from the Earth where the gravitational pull of the Earth and the Sun on a body is balanced, we can follow these steps: ### Step 1: Define the variables Let: - \( M_e \) = mass of the Earth - \( M_s \) = mass of the Sun - \( d \) = distance from the Earth to the Sun = \( 1.5 \times 10^{10} \) km - \( x \) = distance from the Earth to the point where the gravitational forces balance ### Step 2: Set up the gravitational force equations The gravitational force exerted by the Earth on the body is given by: \[ F_e = \frac{G M_e m}{x^2} \] where \( m \) is the mass of the body and \( G \) is the gravitational constant. The gravitational force exerted by the Sun on the body is given by: \[ F_s = \frac{G M_s m}{(d - x)^2} \] ### Step 3: Set the forces equal to each other For the forces to balance, we set \( F_e = F_s \): \[ \frac{G M_e m}{x^2} = \frac{G M_s m}{(d - x)^2} \] ### Step 4: Simplify the equation We can cancel \( G \) and \( m \) from both sides: \[ \frac{M_e}{x^2} = \frac{M_s}{(d - x)^2} \] ### Step 5: Substitute the mass of the Sun Given that \( M_s = 3.24 \times M_e \), we substitute this into the equation: \[ \frac{M_e}{x^2} = \frac{3.24 M_e}{(d - x)^2} \] ### Step 6: Cancel \( M_e \) We can cancel \( M_e \) from both sides: \[ \frac{1}{x^2} = \frac{3.24}{(d - x)^2} \] ### Step 7: Cross-multiply Cross-multiplying gives: \[ (d - x)^2 = 3.24 x^2 \] ### Step 8: Expand and rearrange Expanding the left side: \[ d^2 - 2dx + x^2 = 3.24 x^2 \] Rearranging gives: \[ d^2 - 2dx + x^2 - 3.24 x^2 = 0 \] \[ d^2 - 2dx - 2.24 x^2 = 0 \] ### Step 9: Solve the quadratic equation This is a quadratic equation in \( x \): \[ -2.24 x^2 - 2dx + d^2 = 0 \] Using the quadratic formula \( x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a} \): Here, \( a = -2.24 \), \( b = -2d \), and \( c = d^2 \). ### Step 10: Calculate the values Substituting \( d = 1.5 \times 10^{10} \) km into the formula will yield the value of \( x \).
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