Newton’s law of universal gravitation

In the subject of Newton’s law, was learned that every object which is initially rest becomes moves, or any object that initially moves becomes rest if there is “something” that moves or stops the object. Something is called “force”. Why does the fruit fall or move towards the surface of the earth after it is released from the stem? Newton’s law states that if the fruit moves, there must be a force acting on the fruit. The force that causes fruit or any object to fall towards the surface of the earth is called the force of gravity.

The problem of falling objects involving the force of gravity, which you are studying right now, has been thought of and studied by Isaac Newton, a British scientist. This problem that Newton thought had existed since ancient Greece. There are two basic problems that have been investigated by the Greeks, long before Newton was born. The question that is always questioned is why things always fall to the surface of the earth and how the planets move, including the sun and moon. The Greeks at that time saw the problem of falling objects and planetary movements as two different things. Thus it continued until Newton’s time. So what Newton produced was built on the work of people before him. What distinguishes Newton and the people before he is that Newton saw the problem of falling objects and planetary motion caused by one thing only and must obey the same law. In other words, Newton argued that the force that causes objects to fall to the surface of the ground is the same force, which causes the moon to move around the earth.

The relationship between the force of gravity with distance and mass

When formulating the law of gravity, Newton compared the acceleration of fruit falling near the surface of the earth with the centripetal acceleration of the moon when circling the earth. According to Newton, the acceleration experienced by falling fruit and the centripetal acceleration experienced by the moon circling the earth is caused by the same force, the earth’s gravitational force. Newton argues that the acceleration of the moon when it orbits the earth is proportional to 1/r2 where r = the distance between the center of the earth and the center of the moon = 3.84 x 10 8 m and the acceleration of falling fruit is proportional to 1/R2, where R = distance between the center of the earth and fruit center. The fruit is near the surface of the earth so that R = RF, where RE = radius of earth = 6.37 x 106 m. Thus, the comparison between moon acceleration (aM) and fruit acceleration (g):

Newton's law of universal gravitation 1

So the centripetal acceleration of the moon:

aM = (2.75 x 10-4)(g) = (2.75 x 10-4)(9.8 m/s2) = 2.7 x 10-3 m/s2

Newton also calculated the centripetal acceleration of the moon in a different way. It is known that the lunar orbital period or the time month to do one revolution = 27.3 days = 2.36 x 106 seconds. The length of the path traversed by the moon = the circumference of the lunar orbit = 2 (3.14) (r) where r = the distance between the center of the moon and the center of the earth. The centripetal acceleration of Moon:

Newton's law of universal gravitation 2

The centripetal acceleration of the moon obtained in this calculation is almost the same as the results of previous calculations. Newton’s Second Law states that force is proportional to acceleration (F = m a). The above calculations show that acceleration is proportional to 1/r2 or acceleration is inversely proportional to the square of the distance (r2). Thus it can be concluded that the gravitational force is proportional to 1/r2 or the gravitational force is inversely proportional to the square of the distance. Mathematically:

Newton's law of universal gravitation 3

In addition to investigating the relationship between gravitational forces and the distance between objects, Newton also investigated the relationship between the gravitational force and the mass of objects. Newton’s Third Law states that if there is an action force there is a reaction force. The action force and reaction force have the same magnitude and opposite directions (F-action = -F reaction, a negative sign indicates that the direction of the force is opposite). If the earth’s gravitational force attracts the fruit, the gravitational force of the fruit also attracts the earth. Earth’s gravitational force works on the fruit, whereas the gravitational force of the fruit works on the earth. Likewise the gravitational force between the earth and the moon. Earth’s gravitational force with fruit’s gravitational force or gravitational force with the moon’s gravitational force is a reaction force. Because force is proportional to mass (F = m a) and because the force of action and the force of reaction have the same magnitude, the gravitational force between two objects must be proportional to the mass of the two objects. Mathematically:

Newton's law of universal gravitation 3a

Newton’s law of universal gravitation

Newton’s law of universal gravitation states that every object in the universe attracts one another, where the attraction between objects is proportional to their mass and inversely proportional to the square of their distance. If two objects with masses of m1 and m2 are separated by distance r then the magnitude of the gravitational force between the two objects is:

Newton's law of universal gravitation 4

G = gravitational constant (6.673 x 10-11 Nm2/ kg2). G is measured by experiment.

Newton's law of universal gravitation 5

F12 is the gravitational force applied to m1 at m2 while F21 is the gravitational force applied to m2 at m1. F12 works at m2 and pulls m2 towards m1, while F21 works at m1 and pulls m1 towards m2. F21 and F12 have the same magnitude and opposite direction. So F21 and F12 are pairs of action-reaction. r is the distance between the center of m1 and the center of m2. The center of m1 is located in the center of the object, as is the center of m2. If r is stated in km then it is first converted to meters (international system unit).

Sample problem 1 (gravitational force between 2 particles)

Calculate the gravitational force between two students, each with a mass of 30 kg and 40 kg and a distance of 1 meter.

Solution

Newton's law of universal gravitation 7

The magnitude of the gravitational force is so small so that the two objects are not attracted to each other.

Sample problem 2 (gravitational force between 2 particles)

Newton's law of universal gravitation 8

Calculate the total gravitational force experienced by m2 due to the gravitational force applied to m1 at m2 and the gravitational force applied to m3 at m2. The distance between center m1 and m2 is 2 meters and the distance between center m2 and m3 is 1 meter.

Solution:

The force of gravity of m1 at m2:

Newton's law of universal gravitation 9

The force of gravity of m3 at m2:

Newton's law of universal gravitation 10

The total gravitational force experienced by m2:

Fg total = (6.673 – 1.668) x 10-11 N = 5.005 x 10-11 N. In the figure below, the F32 arrow is longer than the F12 arrow. So the direction of the total gravitational force goes to m3.

Newton's law of universal gravitation 11

Sample problem 3 (total gravity force = zero):

Two balls A and B, each with a mass of m and 5m. Both balls have the same diameter. If the gravitational force at a point between ball A and ball B is equal to zero, then the distance of that point from the surface of ball A is …

Newton's law of universal gravitation 12

Pembahasan :

Solution:

The diameter of the ball A and B is 1 meter, so the radius of the ball A and B is 0.5 meters. The distance between the center of the ball A and B is 6 meters.

We place a test particle with mass m at a point located between ball A and ball B.

FA = the gravitational force applied by ball A to the test particle (the direction of gravity towards the ball A).

FB = the gravitational force that is applied by the ball B to the test particle (the direction of gravity towards the ball B).

So that the gravitational force experienced by the test particle is zero then FA = FB (FA and FB have opposite direction).

Newton's law of universal gravitation 13

Use the quadratic formula to determine the value of x

Newton's law of universal gravitation 14

So x = 4.88 meters

4.88 m – 0.5 m = 4.38 m. The gravitational force is zero, 4.38 meters from the surface of ball A. What is the distance from the surface of ball B?

Measurement of universal gravity constant (G)

To find out your body mass, you only need to stand on a scale and then read the scale of your body mass. It’s easy to measure your body mass. Well, how to measure the mass of the earth? There are no giant scales that are used to measure the mass of the earth and if there is no scale we cannot measure the mass of the earth using these scales because the earth is always moving at all times. The mass of the earth is known through calculation after the universal gravitational constant (G) is measured by experiment.

Weight

The weight of an object is the total gravitational force acting on an object due to the gravitational force applied by all objects in the universe on that object. If the object is located above the surface of the earth or the surface of the earth, then we ignore the gravitational force that is carried by other objects in the universe and consider the weight of an object as the gravitational force of the earth acting on the object.

Newton's law of universal gravitation 15

w = weight of object, mE = mass of earth, m = mass of object, RE = radius of earth.

If an object is h above the surface of the earth (objects are above a certain height such as a plane, for example) or objects spaced r above the surface of the earth where r = RE + h then the gravitational force acting on the object or the weight of the object is:

Newton's law of universal gravitation 16

This equation shows that the weight of an object decreases to the square of the distance from the center of the earth. So the farther from the surface of the earth, the weight of objects decreases.

Acceleration of gravity

Based on Newton’s second law we know that the weight of an object is the force that causes the object to experience an acceleration of free fall (gravitational acceleration):

w = m g

Combine both equation w = F g and w = m g :

Newton's law of universal gravitation 17

This equation explains the gravitational acceleration experienced by an object at a certain height above the earth’s surface. Through this equation, known that the acceleration of gravity decreases with increasing altitude and does not depend on the mass of objects falling freely.

Acceleration of gravity of objects located above the earth’s surface or above ground level:

Newton's law of universal gravitation 18

The mass of the earth can be calculated by changing the above equation to:

Newton's law of universal gravitation 19

Calculate the mass of the earth using this equation!

Problems and Solutions

1. Two objects m1 and m2 each with a mass of 6 kg and 9 kg separated by a distance of 5 cm. Object m3 = 1 kg is placed between the two. If the gravitational force experienced by m3 = 0 then the distance m3 from m1 is …

Force of gravity and gravitational field - problems and solutions 1

Gravitational force = 0 if F13 = F23.

Force of gravity and gravitational field - problems and solutions 2

a = -1, b = -20, c = 50

Use quadratic formula:

Force of gravity and gravitational field - problems and solutions 3

Force of gravity and gravitational field - problems and solutions 4

The results cannot be negative. So x = r13 = distance m3 and m1 = 2.25 cm.

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2. Two objects A and B are 60 cm apart. Mass A is 24 kg and mass B is 10 kg. Where is the location of a point that has a strong gravitational field equal to zero?

Force of gravity and gravitational field - problems and solutions 6

Gravitational field = 0 if gA = gB.

Force of gravity and gravitational field - problems and solutions 7

a = 7

b = -1440

c = 43200

Use quadratic formula:

Force of gravity and gravitational field - problems and solutions 8

x = rA = 169.25 cm or

x = rA = 36.46 cm

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