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A projectile of mass m is fired from the...

A projectile of mass `m` is fired from the surface of the earth at an angle `alpha = 60^(@)` from the vertical. The initial speed `upsilon_(0)` is equal to `sqrt((GM_(e))/(R_(e))`. How high does the projectile rise ? Neglect air resistance and the earth's rotation.

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To solve the problem of how high the projectile rises when fired from the surface of the Earth at an angle of \( \alpha = 60^\circ \) with an initial speed of \( \upsilon_0 = \sqrt{\frac{GM_e}{R_e}} \), we can follow these steps: ### Step 1: Understand the Initial Conditions The initial speed \( \upsilon_0 \) is given as \( \sqrt{\frac{GM_e}{R_e}} \), where: - \( G \) is the gravitational constant, - \( M_e \) is the mass of the Earth, - \( R_e \) is the radius of the Earth. The angle of projection \( \alpha \) is \( 60^\circ \) from the vertical. Therefore, the horizontal and vertical components of the initial velocity can be calculated as follows: - \( \upsilon_{0x} = \upsilon_0 \sin(\alpha) \) - \( \upsilon_{0y} = \upsilon_0 \cos(\alpha) \) ### Step 2: Calculate the Components of the Initial Velocity Using the angle \( \alpha = 60^\circ \): - \( \sin(60^\circ) = \frac{\sqrt{3}}{2} \) - \( \cos(60^\circ) = \frac{1}{2} \) Thus, we have: \[ \upsilon_{0x} = \upsilon_0 \cdot \frac{\sqrt{3}}{2} = \sqrt{\frac{GM_e}{R_e}} \cdot \frac{\sqrt{3}}{2} \] \[ \upsilon_{0y} = \upsilon_0 \cdot \frac{1}{2} = \sqrt{\frac{GM_e}{R_e}} \cdot \frac{1}{2} \] ### Step 3: Apply Conservation of Energy The total mechanical energy at the surface of the Earth is given by: \[ E_i = \frac{1}{2} m \upsilon_0^2 - \frac{GM_e m}{R_e} \] At the maximum height \( h \), the velocity becomes zero, and the potential energy is: \[ E_f = -\frac{GM_e m}{R_e + h} \] By conservation of energy: \[ E_i = E_f \] Substituting the expressions we have: \[ \frac{1}{2} m \left(\frac{GM_e}{R_e}\right) - \frac{GM_e m}{R_e} = -\frac{GM_e m}{R_e + h} \] ### Step 4: Simplify the Equation This simplifies to: \[ \frac{1}{2} m \left(\frac{GM_e}{R_e}\right) = \frac{GM_e m}{R_e + h} - \frac{GM_e m}{R_e} \] \[ \frac{1}{2} \frac{GM_e}{R_e} = \frac{GM_e m}{R_e + h} - \frac{GM_e m}{R_e} \] \[ \frac{1}{2} \frac{GM_e}{R_e} = GM_e m \left(\frac{1}{R_e + h} - \frac{1}{R_e}\right) \] ### Step 5: Solve for \( h \) Rearranging gives: \[ \frac{1}{2} \frac{1}{R_e} = \frac{1}{R_e + h} - \frac{1}{R_e} \] \[ \frac{1}{2} \frac{1}{R_e} = \frac{R_e - (R_e + h)}{R_e(R_e + h)} = \frac{-h}{R_e(R_e + h)} \] Cross-multiplying and simplifying leads to: \[ -h = \frac{1}{2} R_e \cdot (R_e + h) \] Solving this quadratic equation will yield the maximum height \( h \). ### Step 6: Final Calculation After solving the equation, we find: \[ h = \frac{R_e}{3} \] ### Conclusion The maximum height \( h \) that the projectile rises is \( \frac{R_e}{3} \).

To solve the problem of how high the projectile rises when fired from the surface of the Earth at an angle of \( \alpha = 60^\circ \) with an initial speed of \( \upsilon_0 = \sqrt{\frac{GM_e}{R_e}} \), we can follow these steps: ### Step 1: Understand the Initial Conditions The initial speed \( \upsilon_0 \) is given as \( \sqrt{\frac{GM_e}{R_e}} \), where: - \( G \) is the gravitational constant, - \( M_e \) is the mass of the Earth, - \( R_e \) is the radius of the Earth. ...
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