Lesson 4 Flashcards

1
Q

Define speed.

A

Speed is the rate at which an object moves (ex. 100 km/h)

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2
Q

Define velocity.

A

The speed travelled in a given direction (ex. 100 km/h due east)

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3
Q

Define acceleration.

A

It is the change in velocity (ex. 9.8 m/s^2 downward)

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4
Q

What did the Copernican revolution spark for sir Isaac Newton?

A

The discovery of the laws of motion and gravity

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5
Q

Do all falling objects accelerate at the same rate?

A

Yes; everything on earth accelerates at 9.8m/s
- this means that if a falling object takes 1 second to reach the ground, it was falling at 9.8m/s, it it took 2 seconds, it was falling at 9.8m/s x 2, etc

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6
Q

What does net force change?

A

It changes the momentum of an object (which generally means acceleration, i.e. velocity)

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7
Q

What is a force?

A

it is a vector quantity (its direction matters)

- multiple forces can be applied to an object in different directions

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8
Q

What is weight? What is mass? Are they the same thing?

A

Weight = the force that acts upon an object (mass x gravity)
Mass = the amount of matter an object has
Weight does not equal mass

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9
Q

What is momentum?

A

mass x velocity

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10
Q

How can weight change?

A

In the amount of gravity that is acting on an object and the motion of the object (particularly acceleration)
- ex. a 100kg object on earth moving downward will be 100kg on the moon if it is moving upwards

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11
Q

What is angular momentum?

A

The rotational momentum of a spinning object

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12
Q

What is net force?

A

The direction an object will go when all other forces are also applied (like a tug of war between a strong guy and a 5 year old)

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13
Q

What is weightless free fall?

A

When the effects of acceleration are more powerful than the effects of gravity

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14
Q

What does the law of conservation state?

A

a quantity cannot be created or destroyed, it can only be exchanged for something else

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15
Q

What does acceleration upwards cause?

A

More gravity therefore more weight

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16
Q

What does acceleration downwards cause?

A

Less gravity therefore less weight

17
Q

What were Newton’s Laws of Motion? (3)

A
  1. an object moves at a constant velocity unless a net force acts to change its speed or direction
  2. Force = mass x acceleration
  3. for every force, there is always an equal and opposite reaction force
18
Q

What are the three laws of conservation? (3)

A
  1. Law of Conservation of momentum:
    - the total momentum of interacting objects cannot change unless an external force is acting on them
  2. Law of Conservation of angular momentum:
    - angular momentum = mass x velocity x radius of angular movement
    - as radius decreases, velocity increases and as radius increases, velocity decreases
  3. Law of Conservation of energy:
    - energy is conserved but can be exchanged with objects and with other forms of energy
    - the total amount of energy of the universe was determined in the big bang and remains the same
19
Q

What are the three basic categories of energy?

A
  1. kinetic energy (movement)
  2. radiative energy (light and gravity)
  3. potential energy (stored energy like electricity)
20
Q

What are the 4 types of forces?

A
  1. gravitational
  2. electromagnetic
  3. weak
  4. strong
    - these forces interact to create different kinds of energies
21
Q

What are the three subcategories of energy?

A

a. thermal energy: collective kinetic energy of the many particles in a substance (C, F or K)
b. gravitational potential energy: how gravity interacts with an object that has mass
- in space, an object has more gravitational energy when it is spread out than when it contracts
b. i. mass: a form of potential energy
- E=MC^2
- a small amount of mass can produce a large amount of energy

22
Q

Describe the universal law of gravity?

A

Every mass attracts every other mass

  • attraction is directly proportional to the product of their masses
  • attraction is inversely proportional to the square of the distance between their centres
23
Q

What can Newton’s third law help astronomers to do?

A

Estimate the mass of distant objects

24
Q

What effects do gravity have on orbits?

A
  • total orbital energy (gravitational and kinetic) remain constant if there is no external force
  • orbits can gain or lose energy by having a gravitational encounter or by experiencing friction or atmospheric drag
25
Q

What happens if an object gains enough orbital energy?

A

It can escape bound orbit to unbound orbit (escape velocity)

26
Q

What is the escape velocity from earth?

A

11 km/s from sea level

27
Q

How does the moon’s gravity affect earth?

A
  • the shape of earth is bulged due to the moon’s gravitational pull
  • it causes water to change tides
  • the rotation of the earth is affected (it is slowed down due to the gravity of the moon pulling on earth)
28
Q

What is the size of the tide affected by? Which phase is associated with which tide?

A

The size of the tides is affected by the phase of the moon (where the moon is in relation to the sun)

  • a spring tide (highest tide) is associated with new and full moons
  • a neap tide (lowest tide) is associated with the first and third quarter
29
Q

What is tidal friction?

A

Friction with the rotating earth pulls the tidal bulges slightly ahead of the earth-moon line

30
Q

What does tidal friction have an effect on?

A

The length of a day

- it increases by 1 second every 50,000 years

31
Q

Is the rate of acceleration of an object dependent on its mass?

A

NO