Lecture Five Flashcards

(11 cards)

0
Q

What is Newton’s second law of motion?

A

Force = mass x acceleration

OR – Force = rate of change in momentum

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
1
Q

What is Newton’s first law of motion?

A

An object moves at constant velocity unless a net force acts to change its speed or direction

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Newton’s third law of motion?

A

For every force, there is always an equal and opposite reaction force

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Why do objects move at constant velocity if no force acts on them?

A

Conservation of momentum:

  • The total momentum of interacting objects cannot change unless an external force is acting on them.
  • Interacting objects exchange momentum through equal and opposite forces.
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

What keeps a planet rotating and orbiting the Sun?

A

Conservation of Angular Momentum:

  • Angular momentum = mass x velocity x radius
  • The angular momentum of an object cannot change unless an external twisting force (torque) is acting on it.
  • Earth experiences no twisting force as it orbits the Sun, so its rotation and orbit will continue indefinitely.
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Types of energy?

A

Kinetic - motion
Radiative - light
Potential - stored

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

What is thermal energy?

A

The collective kinetic energy of many particles. It depends on temperature and density.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

What is temperature?

A

the average kinetic energy of the many particles in a substance

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Gravitation potential energy on earth depends on:

A
  • object’s mass (m)
  • strength of gravity (g)
  • distance object could potentially fall
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Conservation of mass-energy

A

Mass itself is a form of potential energy: E= 2 mc
When the Sun shines it loses mass
Concentrated energy can spontaneously turn into particles (for example, in particle accelerators).

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Conservation of energy

A
  • Energy can be neither created nor destroyed
  • It can change form or be exchanged between objects
  • The total energy content of the universe was determined in the Big Bang and remains the same today
How well did you know this?
1
Not at all
2
3
4
5
Perfectly