This problem involves calculating the final speed of an object undergoing free fall under gravity. We are given the initial state (at rest), the height from which it is dropped, and the acceleration due to gravity.
We can use the principles of kinematics to solve this problem. The relevant equation that connects final velocity ($v$), initial velocity ($u$), acceleration ($a$), and displacement ($s$ or $h$ in this case) is:
$ v^2 = u^2 + 2as $
In this specific scenario:
Identify Given Values:
Select the Appropriate Kinematic Equation:
The equation $v^2 = u^2 + 2gh$ relates the variables involved.
Substitute Values and Calculate:
Substitute the known values into the equation:
$ v^2 = (0 \text{ m/s})^2 + 2 \times (10 \text{ m/s}^2) \times (20 \text{ m}) $
$ v^2 = 0 + 400 \text{ m}^2/\text{s}^2 $
$ v^2 = 400 \text{ m}^2/\text{s}^2 $
Find the Final Speed:
Take the square root of both sides to find $v$:
$ v = \sqrt{400 \text{ m}^2/\text{s}^2} $
$ v = 20 \text{ m/s} $
The speed with which the ball hits the ground is 20 m/s.
Who among the following was the first to conclude that in vacuum all objects fall with the same acceleration g and reach the ground at the same time?
Who among the following is credited with postulating three laws of planetary motion?
When did Henry Cavendish report the measurement of the gravitational constant with the mass and density of the Earth?
Which of the following law states that, "The force between two objects is directly proportional to the product of their masses?"
Which of the following statements about the movement of planets is true?
A. A planet's orbit is elliptical with the Sun at one of two focal points.
B. The orbit of a planet is circular with the sun in the center.
C. The orbit of a planet is elliptical with another planet in one of the two center-points.
D. The orbit of a planet is circular with another planet in the center.