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gregori [183]
3 years ago
15

A ball with an initial velocity of 5 m/s rolls off a horizontal table with a height of 1.0

Physics
1 answer:
Dmitry [639]3 years ago
8 0

Answer:

Approximately 0.45\; \rm s, assuming that air resistance is negligible and that g = 9.81\; \rm m\cdot s^{-2}.

Explanation:

The ball starts to fall the moment it rolls of the edge of the table.

  • Let h_{0} denote the initially height of this ball.
  • Let v_{0} denote the initial vertical velocity of this ball.

Assume that gravity is the only force acting on the ball during its fall (that is, there's no air resistance to slow the ball down.) The vertical acceleration of this ball during the fall would be constantly equal to (-g) (negative because the ball is accelerating downwards.)

The following SUVAT equation would give the height h of this ball at time t:

\displaystyle h = \frac{1}{2}\, (-g)\cdot t^{2} + v_{0} \cdot t + h_{0}.

Since the table is horizontal, the vertical velocity of this ball would be 0 the moment it rolls of the edge. In other words: v_{0} = 0\; \rm m\cdot s^{-1}.

The initial height of this ball when it rolls of the table is h_{0} = 1.0\; \rm m, same as the height of the table.

Hence, the height h of this ball at time t would be:

\begin{aligned}h &= \frac{1}{2}\, (-g)\cdot t^{2} + v_{0} \cdot t + h_{0} \\ &= \frac{1}{2}\, (-g) \cdot t^{2} + h_{0}\end{aligned}.

At t = 0\; \rm s, the height of this ball would be 1.0\; \rm m. The ball would be on the ground by the time h = 0\; \rm m, Set the right-hand side of this equation to 0 and solve for the time t at which the ball is on the ground:

\displaystyle \frac{1}{2}\, (-g) \cdot t^{2} + h_{0} = 0.

\displaystyle \frac{1}{2}\, (-g) \cdot t^{2} = - h_{0}.

\displaystyle t = \sqrt{\frac{2\, h_{0}}{g}}.

Substitute in the values h_{0} = 1.0\; \rm m and g = 9.81\; \rm m\cdot s^{-2}:

\begin{aligned} t &= \sqrt{\frac{2\, h_{0}}{g}} \\ &= \sqrt{\frac{1.0\; \rm m}{9.81\; \rm m\cdot s^{-2}}} \\ &\approx0.45\; \rm s\end{aligned}.

In other words, the ball would be in the air for approximately 0.45\; \rm s. (The initial horizontal velocity of this ball does not affect the duration of this fall.)

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Answer: 5.06\times10^{9}

At sea level, there is one standard atmospheric pressure which is equal to 101.325 kilopascals.

The pressure of faintest sound that a human ear can hear is 20 micro-pascals.

taking the ratio of two:

\frac {101.325 kilopascals. }{20 micropascals} = \frac {101.325 \times 10^{3}Pa}{20 \times 10^{-6}Pa}

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Calculate the force of gravity between planet X and planet y if both planets are 3.75 X 10^11 m apart, planet X has a mass of 1.
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So, the force of gravity that the asteroid and the planet have on each other approximately \boxed{\sf{2.9 \times 10^{17} \: N}}

<h3>Introduction</h3>

Hi ! Now, I will help to discuss about the gravitational force between two objects. The force of gravity is not affected by the radius of an object, but radius between two object. Moreover, if the object is a planet, the radius of the planet is only to calculate the "gravitational acceleration" on the planet itself,does not determine the gravitational force between the two planets. For the gravitational force between two objects, it can be calculated using the following formula :

\boxed{\sf{\bold{F = G \times \frac{m_1 \times m_2}{r^2}}}}

With the following condition :

  • F = gravitational force (N)
  • G = gravity constant ≈ \sf{6.67 \times 10^{-11}} N.m²/kg²
  • \sf{m_1} = mass of the first object (kg)
  • \sf{m_2} = mass of the second object (kg)
  • r = distance between two objects (m)

<h3>Problem Solving</h3>

We know that :

  • G = gravity constant ≈ \sf{6.67 \times 10^{-11}} N.m²/kg²
  • \sf{m_X} = mass of the planet X = \sf{1.55 \times 10^{22}} kg.
  • \sf{m_Y} = mass of the planet Y = \sf{3.95 \times 10^{28}} kg.
  • r = distance between two objects = \sf{3.75 \times 10^{11}} m.

What was asked :

  • F = gravitational force = ... N

Step by step :

\sf{F = G \times \frac{m_X \times m_Y}{r^2}}

\sf{F = 6.67 \cdot 10^{-11} \times \frac{1.55 \cdot 10^{22} \cdot 3.95 \times 10^{28}}{(3.75 \times 10^{11})^2}}

\sf{F \approx \frac{40.84 \times 10^{-11 + 22 + 28}}{14.0625 \times 10^{22}}}

\sf{F \approx 2.9 \times 10^{39 - 22}}

\sf{F \approx 2.9 \times 10^{17} \: N}

<h3>Conclusion</h3>

So, the force of gravity that the asteroid and the planet have on each other approximately

\boxed{\sf{2.9 \times 10^{17} \: N}}

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