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Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

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Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All
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Page 1: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Newton’s LawsPhysics 113 Goderya

Chapter(s): 5Learning Outcomes: All

Page 2: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Force

Force: It is a push or a pull.

Force has both magnitude and direction.

Force exist in a variety of situations.

Page 3: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Types of Forces

• Contact Forces: Force is due to physical contact between the bodies. Example mechanical forces.

• Field Force: No physical contact is necessary to experience the force. Examples are Gravitational, Electrical, Magnetic, and Nuclear Forces.

Page 4: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

A New Era of Science

Mathematics as a tool for understanding physics

Page 5: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Isaac Newton (1643 - 1727)

• Building on the results of Galileo and Kepler

Major achievements:

1. Invented Calculus as a necessary tool to solve mathematical problems related to motion

• Adding physics interpretations to the mathematical descriptions of astronomy by Copernicus, Galileo and Kepler

2. Discovered the three laws of motion

3. Discovered the universal law of mutual gravitation

Page 6: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

A New Era of Science

Mathematics as a tool for understanding physics

Page 7: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Isaac Newton (1643 - 1727)

• Building on the results of Galileo and Kepler

Major achievements:

1. Invented Calculus as a necessary tool to solve mathematical problems related to motion

• Adding physics interpretations to the mathematical descriptions of astronomy by Copernicus, Galileo and Kepler

2. Discovered the three laws of motion

3. Discovered the universal law of mutual gravitation

Page 8: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Newton’s Laws of Motion (1)

1. A body continues at rest or in uniform motion in a straight line unless acted upon by some net force.

An astronaut floating in space will continue to float forever in a straight line unless some external force is accelerating him/her.

Page 9: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Newton’s Laws of Motion (2)

2. The acceleration a of a body is inversely proportional to its mass m, directly proportional to the net force F, and in the same direction as the net force.

a = F/m F = m a

Page 10: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Newton’s Laws of Motion (3)

3. To every action, there is an equal and opposite reaction.

The same force that is accelerating the boy forward, is accelerating the skateboard backward.

M = 70 kg

m = 1 kg

v = 7 m/s

V = ?

Page 11: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

The Universal Law of Gravity

• Any two bodies are attracting each other through gravitation, with a force proportional to the product of their masses and inversely proportional to the square of their distance:

F = - G Mm

r2

(G is the Universal constant of gravity.)

Page 12: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Gravity and Distance: The Inverse-Square Law

Inverse-square law• relates the intensity of an effect to the inverse-

square of the distance from the cause• in equation form: intensity = 1/distance2

• for increases in distance, there are decreases in force

• even at great distances, force approaches but never reaches zero

Page 13: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Inverse-Square Law

Page 14: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Inverse-Square Law

Page 15: Newton’s Laws Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

Universal Gravitation

Universal gravitation• everything attracts everything else

example: Earth is round because of gravitation—all parts of Earth have been pulled in, making the surface equidistant from the center

• The universe is expanding and accelerating outward.


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