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02 01 Fisika Dasar 1 - Besaran Dan Satuan

36:35EnglishTranscribed Jul 28, 2026
0:01

Welcome to the online lecture series of

0:02

Basic Physics 1.

0:04

In this video, we will discuss a

0:07

topic regarding quantities and units.

0:12

Physics is a basic science and is the

0:15

root of several fields of science such as

0:17

chemistry, astronomy, and even biology.

0:20

Physics is also the basis of

0:22

technology and industry.

0:24

Developments in both of these areas

0:27

are marked by developments

0:29

in physics itself.

0:32

In general, in physics, we

0:34

always try to understand

0:36

existing natural phenomena. To then

0:39

look for a pattern related to the

0:41

phenomenon.

0:43

Then, with the help of

0:45

mathematical language,

0:46

we can engineer this

0:48

into a technology that can be

0:50

applied to various fields.

0:53

For example, the

0:55

following phenomena such as waterfalls and rainbows,

0:58

lightning, and even swimming fish,

1:01

have inspired various

1:03

technological discoveries that we

1:05

enjoy today. Starting from automotive,

1:08

electronic devices,

1:10

health,

1:11

and others.

1:13

Therefore, understanding

1:15

basic physics is important for those of us who will

1:18

enter the industrial world.

1:21

One part of basic physics that is

1:23

important to understand is

1:26

quantities and units.

1:28

Well, let's discuss more

1:30

about these quantities and units.

1:34

Physics is an experimental science.

1:37

As discussed previously,

1:39

we want to understand a natural phenomenon

1:42

and then engineer it so that it can be

1:45

beneficial for human life.

1:48

Well, in

1:49

relation to this, in

1:51

physics, if we want to understand a

1:54

system, whether its nature, phenomena, or

1:57

anything else,

1:58

then we have to disturb the

2:00

system and then

2:03

observe how it responds.

2:06

Let's see here, let's say there is a

2:08

system.

2:10

I would like to know what

2:12

the characteristics of the system are.

2:16

What are its characteristics?

2:18

Suppose I want to know

2:21

what its size is,

2:24

what its

2:26

thermal properties are, etc. So the

2:29

way I do it is by giving a disturbance in the form of

2:32

measurement.

2:34

So,

2:36

from this disturbance, the system will

2:39

respond which is the

2:41

measurement result.

2:43

In relation to measurement results, there are

2:45

two important things we need to know,

2:48

namely

2:49

what we are measuring, namely the

2:52

quantity,

2:54

and

2:55

how much quantity we are measuring. This means that

2:59

the results can later be compared with

3:02

others. That is the unit.

3:07

Well, now

3:08

we return to defining

3:11

quantities and units.

3:13

So, in a measurement we

3:16

obtain a result,

3:18

the quantity is

3:20

to describe what we measure,

3:23

and the unit is to determine the quantity

3:26

of what we measure.

3:31

Now, there are a few important things

3:34

regarding

3:35

this measurement.

3:37

Often we don't realize how

3:40

many very precise measurements

3:43

make modern life

3:46

possible.

3:47

For example,

3:49

every component of a mobile phone,

3:51

from the chip, memory, microphone to the

3:55

camera, is

3:56

highly dependent on a series of

3:58

infrastructures consisting of

4:02

process device materials and

4:04

scientific principles that are measurable and carefully tested

4:06

.

4:08

All of this is

4:10

to ensure

4:11

that

4:13

the phone can make calls,

4:16

send texts or access the internet.

4:19

This unit and precision have become the

4:21

cornerstone of human civilization in the modern era.

4:25

Without clear standards or references,

4:26

it is certain that our civilization could be

4:29

destroyed in an instant.

4:31

That is the importance of

4:34

these quantities and units.

4:38

So it is

4:40

necessary to have a

4:42

standard unit that applies

4:45

forever

4:49

and for everyone.

4:51

So it applies globally.

4:54

Therefore

4:56

we need an agreement on the standards

4:59

we will use.

5:02

Here we use what is called the

5:05

metric system or international system.

5:10

There are seven main quantities or

5:13

basic quantities that we need to know.

5:16

Yes, namely length

5:19

in meters,

5:21

mass in kilograms,

5:24

time in seconds, electric

5:26

current in amperes, temperature

5:29

in Kelvin, light intensity

5:32

in candela

5:34

and amount of substance in moles.

5:38

Each of these quantities

5:42

has a

5:44

standard unit, such as what the

5:46

reference is.

5:49

Of course, this Sir has undergone a

5:52

process of change

5:55

in order to achieve the goal of being

5:59

valid forever for

6:01

everyone.

6:04

Well, now let's look at one

6:06

example of

6:08

how the definition of

6:11

units

6:12

has changed.

6:17

We take the case of units of

6:21

meters for the length quantity.

6:24

So,

6:32

where does the 1 meter that we know today, which is our benchmark for measuring anything, come from? How

6:35

can people say that 1 meter?

6:37

Well, there is a history to this.

6:40

Initially here we see that

6:44

1 meter was

6:46

originally

6:48

defined as

6:50

1 per 10 million

6:53

of the distance along the Earth's surface

6:56

between the

6:58

North Pole

6:59

and the equator passing through the

7:04

Paris meridian.

7:08

Of course,

7:09

with conditions like this,

7:12

it is certain that

7:16

there is imprecision, there is uncertainty

7:19

in the value. Why? Because the benchmark is too

7:22

big

7:23

.

7:25

Yes, it's time to recalculate or

7:28

people want to double check that they have to

7:31

make such a trip. So

7:34

a simpler prototype was made

7:38

to describe

7:41

1 meter.

7:43

Here is the prototype.

7:46

However,

7:47

we know that when we make an

7:50

item as a benchmark, the

7:52

item will definitely

7:54

experience changes,

7:56

both physically and chemically.

7:58

So,

8:00

we try to change the object

8:04

into an

8:05

object that is resistant to

8:07

these changes. Here,

8:09

it is changed

8:11

by

8:13

converting the material into platinum

8:15

iridium and storing it in

8:17

certain conditions.

8:20

So, the length of this rod shows

8:23

one meter.

8:25

However, in order to achieve the goal at

8:27

the beginning, do not let anything change,

8:30

accept it forever,

8:32

then try to define one meter

8:36

through

8:38

physical phenomena, namely here

8:41

after the discovery of the laser,

8:43

the definition of one meter is

8:46

1,650,763.73

8:51

times the

8:53

wavelength of the red-orange light spectrum

8:56

from a krypton atom

8:59

in a vacuum like this.

9:03

Then,

9:05

as time went by,

9:07

the definition changed again.

9:10

Now associated with the speed of

9:13

light.

9:15

Yes, here.

9:17

Then, in 2019, there was a

9:20

redefinition of all

9:23

units, for one meter it was linked

9:26

to

9:28

existing natural constants.

9:32

So, try to ensure that the value

9:36

does not depend on time

9:39

and does not depend on

9:41

where. Well, here is the

9:44

final definition related to the speed of

9:47

light as well.

9:53

So, in relation to the redefinition,

9:57

here we see that

9:58

these are the

10:00

seven

10:02

basic units in SI:

10:05

kilogram,

10:07

meter, second, ampere, kelvin, mole and

10:11

candela,

10:12

whose definitions are

10:15

ultimately linked to the

10:17

constants

10:19

that

10:21

exist in nature, whose values ​​are

10:23

fixed. For example

10:26

here there is um

10:28

kilogram associated with Planck's constant

10:32

um mass

10:33

associated

10:35

sorry, meter associated with the speed of

10:37

light

10:39

here there is

10:40

um second with frequency

10:44

ampere with charge

10:47

um kelvin with um

10:51

Boltzmann's constant and others

10:53

here there are.

10:55

You can read more details about

10:57

this redefinition of basic units.

11:02

Well, now

11:05

in reality

11:09

not all places, not all conditions

11:12

always use units

11:15

in the international system.

11:18

There are some places and conditions that

11:20

use other forms of units

11:25

that are considered more suitable.

11:27

For example, in the United States the

11:29

British Engineering System is more often used

11:31

.

11:33

Maybe we often hear that

11:35

when we read data or read news

11:39

from America, they

11:41

define, for example, length in

11:43

feet, mass in pounds,

11:47

temperature not in Kelvin, Celsius

11:49

but in Fahrenheit, like that, right?

11:53

Well, this is an

11:55

example.

11:56

Or in industry we often

11:58

find

12:00

quantities that are not in the

12:05

basic quantities in SI.

12:06

Often it is its

12:08

derivatives

12:09

that are used to

12:12

best describe the condition of a system.

12:15

For example,

12:18

if we play or we

12:21

see a machine, we often

12:24

read the

12:26

term horsepower.

12:29

This is just a conversion

12:32

that one horsepower is equal to

12:35

745.7

12:36

watts.

12:38

Why use horsepower?

12:40

This is to illustrate

12:42

how the

12:44

engine performs compared

12:46

to horsepower. We know that

12:49

before the steam engine existed by James Watt,

12:53

which was used as a

12:55

term for an engine for a vehicle or

12:58

anything using horse power.

13:01

When it was converted to a machine, then

13:03

people wanted to see how

13:05

its capabilities compared to the

13:07

previous, which was a

13:09

horse, something like that.

13:11

Another one is suppose this has

13:12

RPM.

13:13

We often hear

13:15

RPM

13:17

when talking about engine speed

13:19

and so on.

13:21

This is

13:22

rotation or revolution per minute,

13:25

revolutions per minute.

13:27

That is to describe

13:30

how many times a machine can rotate

13:32

in one minute.

13:35

Then another example is when

13:38

you build a factory or

13:40

are in an industrial area,

13:42

you must have heard of the

13:45

noise level.

13:46

Well, here we can see there is a table

13:49

here.

13:50

A table that we can easily

13:52

imagine the value of because it is

13:55

scaled

13:57

in tens like this.

14:00

So if it's 130,

14:02

40, it's easy to imagine

14:05

the comparison. Well, this is

14:07

in decibels, it's about the level of

14:09

sound intensity.

14:10

We often talk

14:13

about sound intensity. Well, it is

14:15

differentiated by level, yes. If

14:17

that's the level.

14:19

In decibels it is a

14:21

logarithmic scale of the ratio between the

14:23

intensity of

14:24

a place and

14:26

its threshold intensity.

14:27

So for intensity itself, the unit

14:29

is

14:30

watts per square meter.

14:32

So we can differentiate between

14:33

sound intensity and sound intensity level.

14:37

Don't let it happen that we often get

14:38

the terms mixed up. Another example is

14:41

we talk about mass

14:43

and weight.

14:45

In Indonesia, we make it the same. Suppose

14:47

how much do you weigh?

14:49

Oh, 50 kg. Well, that's

14:52

wrong.

14:53

Because weight is a

14:55

force. The unit is Newton.

14:59

If the kilogram is mass.

15:02

Yes, so often

15:04

physically we are wrong actually. So

15:06

by learning this,

15:08

you will definitely be able to improve how you

15:10

define the terms for

15:13

unit quantities.

15:16

Well, then

15:18

we here

15:20

often encounter

15:23

diverse values. So, the

15:27

measured quantities

15:30

in real life have a

15:33

very wide range.

15:35

From the very big to the

15:36

very small. Like

15:40

in the

15:42

real world, there are objects that are

15:44

very small, there are objects that are

15:45

very large. That's a huge

15:48

scale of scope.

15:50

Therefore

15:52

we need some

15:54

help to accommodate values

15:57

that are either too large or too small

16:00

to be easily written in

16:03

standard decimal notation.

16:05

Example.

16:06

We are talking about electrical power

16:10

in watts.

16:14

We can talk about this electrical power

16:17

on a large scale or a small scale.

16:20

For example,

16:22

we are talking about the electrical power

16:24

generated by a

16:26

geothermal power plant.

16:28

This is an example at the

16:30

Wayang Windu Geothermal Power Plant.

16:33

Or on a smaller scale, we are talking

16:36

about the electrical power of a

16:41

medical device implanted into the body.

16:44

An example of this is a pacemaker.

16:48

Of course the power value must be very

16:50

different.

16:53

For power plants, the

16:55

value is 227

16:58

million watts.

17:00

For

17:02

pacemakers, the value is

17:03

0.0001

17:06

watts.

17:08

So, to accommodate values ​​like

17:11

this which have too many zeros,

17:15

we can use something called

17:17

scientific notation.

17:20

Besides simplifying the writing method,

17:23

it also makes it easier for us to

17:25

imagine

17:28

the scale.

17:30

So it's time for us to see what the

17:32

order of magnitude is.

17:36

Yes, this is clear, right? This is 10^6,

17:39

this is 10^-4. Of course this is a

17:42

very large value and this is a very

17:44

small value.

17:45

Apart from that, in this concept we also

17:48

know something called a prefix. So

17:52

this value of 10 to the power has its

17:54

own name.

17:57

The term

17:58

is called a prefix. For example,

18:00

I can change these two values ​​to something

18:03

like this.

18:05

So 10^6 is called mega, so 27

18:09

MW.

18:11

I changed the one below to 100 *

18:14

10^-6.

18:16

-6 to micro.

18:19

Well,

18:20

we will learn about

18:22

scientific notation and prefixes.

18:25

Okay, now let's look at

18:29

scientific notation.

18:32

Well, in general,

18:33

scientific notation is written in the form

18:37

A multiplied by 10^B.

18:41

Where A is a real number.

18:45

So the value can be from

18:49

minus to positive.

18:53

Can be commas, can be whole numbers.

18:55

While B is an integer.

18:58

Of course it can be positive and negative.

19:01

For example, we can see here.

19:05

Suppose

19:06

10

19:09

thousand.

19:10

We convert it into

19:13

scientific notation form. Here we can

19:16

see it becomes

19:18

1 * 10 ^ 4. Where from?

19:21

We want to make this one in front,

19:23

okay? That means this one

19:26

moved here.

19:28

Meanwhile, we change the zero to 10 to the

19:32

power of 10. This means there are 1 2 3 4.

19:36

This means there are 10 ^ 4.

19:40

Another example.

19:43

75 million.

19:46

Suppose

19:48

I want the front number in

19:50

scientific notation

19:51

to be 75.

19:54

So this is 75. The

19:56

remainder is that we have 1

19:59

2 3 4 5 6 zeros. So this is 10 ^ 6.

20:06

Now, what if I don't want the front number to be

20:09

75, but I want it to be

20:12

7.5, for example this one.

20:16

So 7.5

20:20

means 75, but the comma is here, right?

20:24

So

20:26

what is the number after the comma here?

20:30

1 2 3 4 5 6 7. So this means 10 ^ 7.

20:37

Or maybe this was 10 ^ 6 initially, right?

20:40

If a comma moves back

20:42

here, then the exponent increases by one.

20:45

If there is a zero added to

20:47

the right, the exponent will reduce by one.

20:51

Another example.

20:52

0.001.

20:55

So the example here is that we want

20:57

to keep the number one in front here.

21:01

This means that there is

21:03

no comma behind the number one,

21:05

right? This means that the comma must

21:08

be moved until it disappears. How

21:11

to do?

21:12

We shift this comma 1

21:15

2

21:16

3 times. So this is 10 to the power of

21:18

minus 3.

21:20

Another example here, let's say

21:23

0.000009.

21:27

How do you get here?

21:30

So, for

21:31

example, if I want this to be 9,

21:34

that means there is no comma before 9, right

21:36

here, right.

21:37

This means the comma must be removed, we

21:39

move 1 2 3 4 5 6 times. That means

21:43

this is minus 6.

21:46

Yes.

21:48

Another example is this 0.00025,

21:51

meaning

21:52

if I want the front to be 25, there is no

21:54

comma behind it,

21:56

meaning we remove the comma 1 2 3 4 5.

22:02

What if I want it to be 0,

22:05

sorry, 2.5, like this. That means the comma is

22:08

between 2 and 5, right? This means we

22:09

shift the comma to between 2 and 5.

22:13

This means 1 2 3 4 times. If it means something

22:17

like this.

22:19

If it's 0.25, you should be able to

22:21

define it too. Like that, yeah.

22:25

So, now that you have a

22:28

form of scientific notation, how do you

22:30

operate it?

22:32

There are several properties.

22:35

If you multiply like this,

22:37

it means that if you multiply the

22:41

scientific notation form, then

22:45

multiply the front part as usual

22:47

A times C

22:49

, so the exponent becomes the sum.

22:54

For example, suppose

22:56

I have

22:57

eee suppose here there is

23:00

2

23:02

times 10 to the power of 3

23:05

I want to multiply it

23:09

by suppose this is 3 times 10 to the power of

23:14

minus 2 suppose that

23:17

means the result is

23:20

2 times 3 first 6

23:23

multiplied by 10 to the power of what? The power is

23:26

added

23:27

3 plus minus 2

23:31

then the result is 6

23:33

times 10 to the power of 3 plus minus 2 is

23:37

1

23:40

that is yes

23:41

next

23:42

division

23:45

we divide the front number first then the

23:48

power becomes a subtraction form

23:55

for example I have for example

23:57

eee 12 times 10 to the power of

24:02

6 divided by

24:05

4 times 10 to the power of minus 3 for example yes

24:11

means the result is the same as

24:13

12 divided by 4

24:16

times 10 to the power of 6 minus minus 3

24:18

the result is the same as

24:23

meaning

24:24

3 times 10 to the power of 6 minus minus 3

24:29

nine like that yes

24:34

finally

24:36

if the power yes for example here the power of

24:41

A times 10 to the power of B are all

24:43

raised to the power of K

24:45

then

24:46

raise the power first the power of the

24:47

front number then the

24:49

power is

24:51

multiplied for example for example

24:55

2 times 10 to the power of 5

25:00

squared is equal to meaning

25:03

2 squared multiplied by

25:06

10

25:07

^ 5

25:10

^ 2 yes multiply 2 is equal to

25:13

4 * 10 ^ 10

25:17

Well, that's how to write

25:21

the conversion into scientific notation and

25:24

operate it. We will

25:26

encounter many values ​​like this

25:29

in the following sections.

25:36

So,

25:38

after we got to know about

25:40

scientific notation, we also got to know

25:43

here what is called a prefix or prefix.

25:46

So, the multiplication factors 10^

25:50

have their own names, their

25:52

own prefixes.

25:53

Which is the prefix for the unit.

25:56

Suppose I have a quantity

26:01

that is measured, the result is, for example,

26:05

I get 10^-9

26:09

m

26:11

or, for example, eh, don't, for example, 2 *

26:15

10^-9

26:16

m.

26:18

So

26:19

10^-9 is nano. But I

26:21

mentioned earlier that the value is the same

26:23

as

26:24

2 nm.

26:27

So

26:28

this exponent value is changed to the

26:31

nano prefix or I measure I have a value

26:35

for example

26:37

emm

26:38

7 * 10^

26:42

9

26:43

watts of

26:45

electrical power, right.

26:47

So in what form should I write it

26:51

? 5 in front of it is

26:53

giga watt. like that.

26:57

Yes, so just change it.

27:00

Roughly, yes, later the values ​​that

27:02

you need to understand are quite a few parts, maybe

27:05

kilo, mega, giga, nano, micro, milli.

27:09

That's what we'll use often later.

27:14

Well,

27:15

in

27:16

physics we often encounter

27:20

many symbols. These symbols are used

27:23

to describe

27:25

both quantities, prefixes and

27:29

other things.

27:31

Well,

27:32

these symbols, apart from using the

27:35

alphabet

27:37

that we know

27:38

A, B, C, D, E to Z,

27:41

also use the Greek alphabet.

27:46

Well, here is an

27:48

example

27:50

of the

27:52

Greek alphabet.

27:55

Yes, starting from alpha,

27:58

beta,

28:00

gamma, delta,

28:02

to omega.

28:05

Surely you are already familiar

28:08

with some of the

28:10

letters here, right?

28:11

But there are also parts that are not. Well,

28:13

here the example

28:15

is given that the letter on the left

28:18

is the capital letter, the letter

28:20

on the right is the lower case letter. Maybe

28:22

we meet lowercase letters more often

28:24

.

28:26

Well, some examples that you are probably

28:29

familiar with include the first one,

28:32

lambda.

28:34

We often use the lowercase lambda

28:36

in the

28:37

wave concept to represent eh

28:40

as a symbol for wavelength.

28:43

Another example is

28:45

rho.

28:46

If rho is roughly what

28:48

we are talking about in terms of

28:50

density, density, right?

28:54

Another one that we may

28:55

encounter frequently is

28:57

omega.

28:58

Both capital and lower case letters

29:00

.

29:01

Where do

29:03

you find the capital omega?

29:04

This is the unit for

29:06

electrical resistance, right? For example, if

29:08

there is a 7 ohm resistor, that's omega, right?

29:13

Where are the lowercase letters? We can

29:14

meet this small letter omega in

29:17

the concept of waves as well

29:19

or the concept of rotational motion regarding

29:21

angular velocity or

29:24

angular frequency. That's how it is. So I

29:26

hope you are starting to get familiar with

29:30

this Greek alphabet. How to

29:33

write it and how to

29:35

read it. Also what symbol is he.

29:40

Okay, now that we know some

29:42

basic concepts

29:44

we will move on to the

29:47

physics part.

29:48

So,

29:49

as an introduction,

29:53

we will get to know

29:54

what is called idealization and modeling.

29:58

So

29:59

various physical systems can be

30:01

simplified into a model.

30:04

What for?

30:05

To avoid

30:06

overly complicated analysis.

30:09

For example, a simple thing

30:11

is actually complicated physically.

30:14

For example, you throw a ball.

30:17

If you throw a ball, let's say it

30:19

's a baseball.

30:24

So what happened there? First,

30:26

there are several physical phenomena,

30:28

namely, first the ball rotates.

30:32

Yes, it rotates about

30:34

its axis.

30:35

So the ball doesn't stay in

30:38

position.

30:39

Then

30:40

and he there are complex shapes. what

30:42

this means is that this ball may not be

30:44

100% a

30:46

perfect ball shape, there are dents on the

30:48

sides,

30:49

there are seams here, it's

30:52

quite a complex shape.

30:54

Then don't forget that there

30:56

must be a factor of air friction and

30:59

wind.

31:01

He exerts a force on the ball,

31:03

either as a drag

31:06

or

31:07

eh, making the ball

31:11

move in a complicated way.

31:13

Yes.

31:14

Then there is also the gravitational force that

31:17

works depending on the height.

31:20

Because

31:22

the higher the ball is from a reference point,

31:25

for example the ground surface, the

31:27

gravitational force will actually

31:30

decrease.

31:33

So here it is seen that there are many

31:36

phenomena that need to be taken into account.

31:39

But

31:41

in this fundamental physics in particular

31:46

we utilize idealization and

31:48

modeling. So we assume the conditions are

31:51

ideal

31:53

so that

31:55

we can model the system in a

31:57

simple way. Like what?

31:59

Like this.

32:02

Okay.

32:04

We assume or idealize. What is the

32:07

ideal?

32:08

Assumption. Yes, firstly, the ball that

32:12

has a

32:15

complex shape, there are dents, there are

32:17

seams, we consider it as a

32:19

point or particle object.

32:22

So if the object is a point or particle,

32:25

we don't need to or we won't be

32:28

able to see its rotational motion.

32:32

This means that

32:33

the direction of the ball's movement is only

32:37

this green arrow.

32:38

There is no direction in which the ball rotates.

32:41

One.

32:42

So, we can eliminate the

32:45

rotational motion factor.

32:47

The second is

32:49

idealization, we ignore air friction.

32:52

So what?

32:54

One of the forces at work is missing.

32:58

There is no air friction force.

33:00

Here, okay?

33:01

Third, we assume that the

33:04

gravitational force acting on the ball is

33:06

constant. So, even though the ball changes

33:08

height, the

33:10

gravitational force remains the same value.

33:14

So that in the end this system

33:17

becomes very simple and we can

33:20

analyze it much more easily.

33:23

Of course,

33:27

as you study physics more

33:29

advancedly,

33:31

these factors will start to come

33:32

into play. So that when we

33:35

encounter a real case

33:38

,

33:39

we can get results that are

33:42

close to reality.

33:45

But of course,

33:47

this simplification

33:50

usually doesn't change the

33:53

real value very much. That's how it is

33:56

.

33:59

Besides talking about

34:01

idealization and modeling, we also need to

34:04

talk more about a reference point.

34:09

So, later in defining

34:11

several quantities in physics,

34:13

we must have a common reference point

34:16

. So that

34:19

later we can easily

34:21

analyze, to identify

34:25

physical quantities, especially later

34:27

in motion.

34:29

The frame of reference we use is

34:31

a Cartesian coordinate system

34:34

, yes. There are actually many

34:36

coordinate systems, yes.

34:38

There are Cartesian, there are polar, there are cylindrical,

34:41

and there are spherical. Let's just use the

34:43

simplest one.

34:45

For example, let's say I have

34:48

coordinates in two dimensions, namely

34:52

Cartesian, there are two x-axis and y-axis

34:55

which are perpendicular to each other.

34:57

Suppose there is a ball at point A.

35:02

In two-dimensional Cartesian coordinates,

35:04

I can define this object to be

35:06

at positions

35:08

xA

35:09

and yA, so the points are xA,yA.

35:16

For three dimensions,

35:18

we add one more axis,

35:21

besides x,

35:22

y, there is also z.

35:26

Suppose there is a ball at point B, then

35:29

I can determine its position on each

35:33

axis,

35:34

at xB with respect to the x-axis, with respect to the

35:37

z-axis at zB, with respect to the y-axis

35:40

at yB. This means the position is

35:43

xB,yB,zB.

35:47

Well,

35:48

later this framework or coordinate system

35:50

is what we will use

35:53

while

35:55

studying

35:57

some parts of basic physics.

36:02

OK,

36:03

so far you have learned

36:06

a little about quantities and units.

36:10

You can look for various

36:13

other explanations in various sources,

36:16

both books

36:17

and

36:19

other videos.

36:22

Okay, that's it for

36:23

this video.

36:26

Happy learning and see you in the

36:29

next video.

36:31

Thank You.

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