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Mars2501 [29]
2 years ago
7

A tennis ball is dropped from 1.20 m above the ground. It rebounds to a height of 1.00 m. (a) with what velocity does it hit the

ground?
Physics
1 answer:
pashok25 [27]2 years ago
4 0

Answer:

The velocity at which it hits the ground is 4.8497 \frac{m}{s}.

Given:

Height of the ball = 1.2 meter

To find:

The velocity does it hit the ground = ?

Formula used:

v^{2}  = u^{2} + 2as

Where v = final velocity of the ball

u = initial velocity of the ball

a = acceleration due to gravity = 9.8 \frac{m}{s^{2} }

s = distance travelled by the ball = 1.2 meter

Solution:

A tennis ball is dropped from 1.20 m above the ground.

According to kinematic equation of motion,

v^{2}  = u^{2} + 2as

Where v = final velocity of the ball

u = initial velocity of the ball = 0 \frac{m}{s}

a = acceleration due to gravity = 9.8 \frac{m}{s^{2} }

s = distance travelled by the ball = 1.2 meter

Thus,

v^{2} = 0 + 2 × 9.8 × 1.2

v^{2} = 23.52

v = 4.8497 \frac{m}{s}

Hence, the velocity at which it hits the ground is 4.8497 \frac{m}{s}.


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Mars has two moons, Phobos and Deimos. Phobos orbits Mars at a distance of 9380 km from Mars's center, while Deimos orbits at 23
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Answer:

The ratio is   \frac{T_1}{T_2}  = 3.965

Explanation:

From the question we are told that

   The  radius of Phobos orbit is  R_2 =  9380 km

    The radius  of Deimos orbit is  R_1  =  23500 \  km

Generally from Kepler's third law

    T^2 =  \frac{ 4 *  \pi^2 *  R^3}{G * M  }

Here M is the mass of Mars which is constant

        G is the gravitational  constant

So we see that \frac{ 4 *  \pi^2  }{G * M  } =  constant

   

    T^2 = R^3   *  constant      

=>  [\frac{T_1}{T_2} ]^2 =  [\frac{R_1}{R_2} ]^3

Here T_1 is the period of Deimos

and  T_1 is the period of  Phobos

So

      [\frac{T_1}{T_2} ] =  [\frac{R_1}{R_2} ]^{\frac{3}{2}}

=>    \frac{T_1}{T_2}  =  [\frac{23500 }{9380} ]^{\frac{3}{2}}]

=>    \frac{T_1}{T_2}  = 3.965

   

8 0
2 years ago
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