Physics exam #3

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/13

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 2:35 AM on 4/10/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

14 Terms

1
New cards

Uniform Circular Motion

When something moves in a circle, its velocity is always changing direction.

Even if the speed stays the same, the direction changes → so it is accelerating.

2
New cards

Centripetal acceleration

Everything moving in a circle is constantly being pulled toward the center.

Example:

  • car going around a curve

  • planet orbiting sun

  • ball on a string

3
New cards

Direction of velocity

Velocity points along the edge of the circle, not toward the center.

Think:

velocity → sideways
force → inward

4
New cards

Centripetal force equations

Fc​=mv²/r​

where

  • m = mass

  • v = velocity

  • r = radius of circle

5
New cards

centrifugal force?

There is NO centrifugal force

That is a fake force people feel in rotating frames.

In physics problems:

centripetal force exists
centrifugal force does NOT

6
New cards

What provides centripetal force?

Situation

Force causing circular motion

ball on string

tension

car turning

friction

planet orbit

gravity

roller coaster

normal force

The equation F=mv²/r tells you how much force is required, not what type of force it is.

7
New cards

Cars Turning (Highway Curves)

When a car turns, it wants to go straight because of inertia.

Something must pull it toward the center.

On a flat road, that force is:

FRICTION

8
New cards

Flat curve

Friction provides centripetal force.

So:

Ff=mv²/r

If friction is too small → car skids outward.

This is why roads get dangerous when wet

9
New cards

Banked Curves

  • NASCAR tracks

  • highway ramps

The tilt allows the normal force to help provide centripetal force.

Meaning:

You don't rely completely on friction.

There is one special speed where:

  • friction = 0

  • normal force provides all centripetal force

v=√rgtan⁡θ

Where

  • r = radius

  • g = gravity

  • θ = angle of bank

10
New cards

Gravity

The same force that pulls apples down keeps the moon in orbit.

Gravity acts between any two objects with mass

11
New cards

Newton's Law of Universal Gravitation

F= G * m1​m2​​/r²

where

  • G = gravitational constant

  • m1,m2= masses

  • r = distance between centers

12
New cards

value of G

G=6.67×10^-11 Nm2/kg2

It is VERY small.

Meaning gravity between normal objects is tiny.

Example:
Two people standing next to each other technically attract each other gravitationally — but it's unbelievably small.

13
New cards

Difference between G and g

Big G

Universal gravitational constant

G=6.67×10^−11

Used in:

F=G * m1m2/r2

Little g

Acceleration due to Earth's gravity

g=9.8 m/s2

Used in:

F=mg

14
New cards