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FISIKA Kelas 11 - Gelombang Cahaya | GIA Academy

26:12EnglishTranscribed Jul 28, 2026
0:00

[music]

0:08

[music]

0:18

Hello friends, welcome back

0:20

to the Gia Academy YouTube channel. I hope my

0:23

friends are always healthy and keep up their

0:25

spirits.

0:28

At night when we use a

0:30

car and turn on the lights, we

0:33

can see that the light from the car lights

0:35

travels straight in the direction of the

0:37

light source. At other times, just

0:40

after the rain, sometimes we can

0:42

see colorful lights in the sky

0:45

called rainbows. So, what is

0:47

the process by which a rainbow

0:49

is formed? We will study the

0:51

symptoms of light in

0:53

this video.

0:56

So, in this video we will learn

0:58

about light waves. Keep watching

1:01

the video, okay?

1:04

So, friends, light is a form of

1:06

energy in the form of

1:08

electromagnetic waves with a wavelength of

1:10

around 380

1:12

to 750 nm. These light waves

1:16

do not require a medium to propagate

1:19

so that light can propagate in a

1:21

vacuum. That is why

1:23

sunlight can reach the earth even though it

1:26

passes through the vacuum of outer

1:28

space at a speed of 300 million m/s.

1:34

As an electromagnetic wave,

1:36

light has the following properties.

1:39

First, light can be reflected or

1:41

[music] reflection. can be

1:44

refracted, experience mixing or

1:47

interference,

1:49

experience bending, diffraction, can be

1:52

broken down, dispersed, and experience

1:55

polarization.

1:59

So, these are the six properties of light

2:01

that we will discuss in

2:04

this video. Reflection, refraction, interference,

2:08

diffraction, dispersion, [music]

2:11

and polarization. Come on, let's discuss them one by one

2:13

.

2:16

We start from the reflection of light or

2:18

reflection. Light reflection is the

2:21

reversal of the direction of light because it hits

2:23

a surface. The process of

2:26

light reflection follows the law of reflection, namely the

2:29

incident [musical] ray, the normal line, and the

2:31

reflected ray lie on one

2:33

flat plane. The angle of incidence is the same as the

2:35

angle of reflection. The

2:39

second property is the refraction of light or

2:41

refraction. Refraction of light is

2:44

the bending of the direction of light propagation because it

2:46

passes through the boundary plane of two

2:48

different propagation media. The process of refraction of

2:51

light follows the law of refraction

2:53

stated by Willbrad Snellius,

2:56

a

2:58

Dutch physicist. Snelius put forward the law

3:00

of refraction as follows. The incident ray, the

3:03

normal line, and the refracted ray lie

3:05

on one plane. The ratio

3:08

between the sine of the angle of incidence and the sine of the

3:10

angle of refraction is constant.

3:14

We can write Senelius' second law

3:16

in the following equation. Sin

3:19

theta 1/ sin theta 2 = n2/n1

3:23

[music] = n21 n1v1 = n2v2

3:29

n1 lambda 1 = n2 lambda2 with theta 1

3:34

angle of incidence theta 2 angle of refraction n1 n2

3:37

refractive index of medium v1 v2 speed of

3:41

light wave in

3:44

lambda 1 lambda 2 wavelength of

3:46

light in meters.

3:50

According to Snelius, when light is refracted

3:52

in a medium of different densities, what

3:54

will happen is that the light

3:56

coming from the less dense medium [music]

3:58

to the denser medium is refracted

4:01

closer to the normal line. Rays

4:03

coming from a denser medium to a

4:05

less dense medium are refracted

4:07

[music] away from the normal line. Remember,

4:10

distance to closeness brings you closer, closeness to

4:12

distance brings you further away. Meanwhile, incident rays

4:15

that are perpendicular to the boundary plane are not

4:17

refracted, but are transmitted. The

4:21

next property of light is interference.

4:24

Light interference is a combination

4:27

of two coherent light waves

4:29

, which have the same frequency and

4:31

amplitude, while the

4:33

phase difference remains the same.

4:37

Interference is of two types.

4:39

First, maximum or

4:42

constructive interference, which is interference that

4:44

reinforces each other. The properties of

4:47

this interference are that it produces a

4:49

bright pattern if the waves are

4:51

in phase or the phase difference is 0 degrees or an

4:54

integer multiple of 360 [music]

4:57

degrees. Second interference,

5:00

minimum or destructive interference.

5:03

This means that these interferences weaken each other

5:05

.

5:07

This interference produces a dark pattern that

5:09

occurs if the waves are 180 degrees out of phase

5:13

or an odd number of 180

5:16

degrees.

5:19

There are several experiments to investigate

5:21

light interference patterns. First,

5:23

Thomas or Fresnel's experiment to

5:26

test double slit interference. In

5:29

his experiment, Thomas Yang demonstrated

5:31

a light source that illuminates two

5:34

parallel slits separated by a distance

5:37

D, thus producing two

5:39

coherent beams of light with a deviation angle theta. The

5:42

interference pattern is observed on a screen at

5:45

a distance L from the slit and has a

5:48

regular pattern, namely a bright pattern for

5:50

maximum interference results and a dark pattern

5:53

for minimum interference results. In

5:56

the center of the screen there is a

5:58

central light. The distance from the center light to light or

6:01

dark to n is denoted by Yn.

6:06

From the double slit experiment,

6:08

we can calculate the

6:10

following quantities. In the bright pattern, the

6:12

equation d sin theta = n lambda or

6:16

dn/l

6:18

= n lambda applies. The number n indicates the order

6:22

or number of brightness with the provisions 0

6:24

for the central brightness, one for the first brightness

6:27

and so on. Meanwhile, in the

6:29

dark pattern the equation applies d sin theta = n -

6:34

1/2 * lambda or dn/l [music]

6:38

= n - 1/2 * lambda. The number n

6:43

indicates the order or number of darks starting

6:46

with the first dark n = 1, the second dark,

6:50

n = 2, and so on. As

6:53

we have discussed previously,

6:55

the quantities for

6:57

this double slit interference equation are D

7:00

is the slit distance in meters, theta is the

7:03

deviation angle, N is the interference order,

7:07

[music] lambda is the wavelength in

7:09

meters, L is the distance from the slit to the screen,

7:12

also in meters. and Yn is

7:15

the distance from the center light to light or dark

7:18

to N in meters. The

7:22

second interference pattern experiment is

7:25

interference in thin layers.

7:29

We can observe the interference phenomenon in thin layers in

7:32

soap bubbles exposed to sunlight

7:34

or thin layers of kerosene

7:36

spilled on water, producing

7:39

certain colors of light. The

7:41

interference pattern in a thin layer occurs

7:44

when a ray with an angle of incidence I

7:47

hits a thin layer with a thickness of D

7:49

and a refractive index of N.

7:51

[music]

7:51

so that the ray experiences reflection and

7:54

refraction with a refractive angle of R so that

7:56

we can see the pattern of light colors

7:58

.

8:01

The difference in optical path length

8:03

and the change in the phase of the reflected light

8:06

causes

8:08

maximum and minimum interference to occur. At

8:11

maximum interference or bright pattern the

8:14

equation 2nd cos r = m - 1/2 * lambda applies.

8:20

Meanwhile, in the minimum interference or

8:23

dark pattern, the 2nd cos [music] r = m

8:28

lambda applies with the thickness of the thin layer

8:31

in meters. R refractive angle [music] n

8:34

refractive index of thin film lambda

8:38

wavelength of light in air in

8:40

meters. Lambda 0 wavelength of light

8:44

in a thin layer is in meters and

8:47

m is the interference order.

8:51

And the last interference pattern experiment

8:54

is Newton's ring interference.

8:57

Newton's rings are dark circular lines

8:59

resulting from the

9:01

interference of light by reflection from two

9:03

different planes, namely a convex PL lens

9:07

and a parallel plane mirror.

9:09

This Newton's ring interference pattern occurs when light

9:12

comes in a perpendicular direction to an

9:15

optical system consisting of a

9:17

flat convex lens or plan convex lens

9:20

with a large radius R placed

9:23

on a parallel plane glass producing a

9:26

pattern of dark and light circular lines with a

9:28

small radius R [music] and

9:31

having an air layer thickness D

9:33

between the glass surface and the lens.

9:37

The equation resulting from the

9:39

Newton's ring interference pattern

9:42

is for the bright circle pattern NR²

9:44

[music]

9:45

= m - 1/2 * lambda r. Dark circle pattern

9:50

NR² = m lambda r. And to

9:54

calculate the thickness of the air layer

9:56

between the glass surface and the lens in the

9:59

bright pattern, D = m - 1/2 * lambda/2.

10:05

In the dark pattern, D = M * lambda/2 where

10:10

D is the thickness of the air, r is the

10:13

radius of the ring. Both are in units of

10:16

meters, N. The refractive index of a plan convex lens is

10:19

lambda, the wavelength of light

10:22

is in meters, the interference order is m, and

10:25

r is the radius of the lens in

10:28

meters. The

10:31

next characteristic of light [music] is

10:33

diffraction. Light diffraction is

10:36

the phenomenon of bending or deflection of the

10:38

direction of light propagation when it passes through a

10:41

narrow gap or grating so that the

10:43

light waves appear to widen at the

10:46

edge of the gap. In diffraction, interference also occurs,

10:49

forming

10:52

dark and light lines on the screen.

10:55

Based on the medium or gap it

10:57

passes through, diffraction can be divided

11:00

into three types. First,

11:02

single slit diffraction. In single slit diffraction

11:05

, incident light with a

11:07

wavelength of lambda enters a

11:10

single slit with a width of D, experiences

11:13

wave bending and forms a

11:15

deviation angle of theta. [music] The incoming light

11:18

falls directly on the screen, forming a

11:20

pattern of dark and light. The distance between the

11:23

slit and the screen is denoted by L

11:26

and the distance from the center light to light or

11:28

dark to N is Yn. So we can

11:32

calculate the magnitude of this diffraction.

11:35

For dark patterns the equation d sin

11:38

theta = n lambda or dn/l

11:42

= n lambda applies. Where n represents the order

11:46

or number of the dark pattern. Meanwhile, in the

11:48

bright pattern, the equation d sin theta

11:51

= n - 1/2 * lambda or dn/l

11:57

= n - 1/2 * lambda [music] applies, where n

12:02

is the order or number of the bright pattern.

12:06

All the quantities in

12:08

this single-slit diffraction equation are the same as the quantities for

12:11

double-slit interference in the

12:14

previous discussion. It's just that the formula for the

12:17

light and dark patterns is reversed.

12:19

Why is that? In single slit diffraction

12:22

it appears that the central bright band is

12:24

wider than the slit width. The

12:27

other bright [musical] bands become narrower

12:29

as they move further from the central light.

12:32

But the width of the dark band is almost constant.

12:34

Therefore, if d sin theta = n lambda,

12:38

what occurs in single slit diffraction

12:41

is minimum interference or

12:43

dark bands. The

12:46

second type of diffraction is

12:49

grating diffraction. A grating is a barrier that

12:51

has many gaps with

12:53

the same width and distance between the gaps

12:56

. A beam of light

12:59

passed through a grating produces a

13:01

sharper bright band

13:03

than double-slit interference

13:05

and single-slit diffraction. [music]

13:07

Some equations that we can

13:09

use to find the magnitude of the

13:11

diffraction grating are first we can

13:14

calculate the grating constant or the distance between the

13:17

slits with the equation D = 1/n. N

13:22

represents the number of lines per cm.

13:25

Next is the equation for calculating the

13:27

magnitude of the light and dark patterns.

13:30

Where the equation is the same as the

13:32

equation for double slit interference.

13:35

In light patterns, the equation d sin

13:38

theta = dyn/

13:42

n lambda applies. And in the dark pattern, d

13:45

sin theta = dn/l

13:48

= n - 1/2 * lambda.

13:54

And the last type of diffraction is

13:56

diffraction of resolving power in optical instruments. The

13:59

resolving power of an optical instrument is the ability of an

14:01

optical instrument to produce separate images

14:04

of two adjacent objects.

14:06

If an optical instrument has a

14:09

diaphragm diameter D, [music] then two

14:11

light sources S1 and S2 can still be

14:15

separated precisely on the screen

14:17

to form images S1 A' and S2' [music]

14:21

with resolving power DM'. The intersection of the two

14:25

lights at the lens diaphragm

14:27

will form a separation angle or

14:30

minimum resolution angle theta M and the distance of the object

14:33

from the lens is L. So, to

14:36

calculate the resolving power of this optical tool

14:38

, we can use the

14:40

following equation. DM = 1.22

14:44

l/d.

14:46

And to calculate the minimum resolution angle

14:48

is theta M = 1.22

14:52

lambda/d. where L is the distance of the object

14:56

from the lens and D is the aperture diameter of

14:59

both optical instruments in meters.

15:03

Until [music] here, friends can

15:04

understand it, okay?

15:07

Next we will discuss the

15:09

fifth property of light, namely dispersion.

15:12

Light dispersion is the process of breaking down

15:15

white or polychromatic light into

15:17

colored or monochromatic light.

15:20

Dispersion occurs when light passes through

15:22

mediums with different refractive indices. In the

15:25

following image we can see that

15:27

white light passing through a prism

15:30

is broken down into a spectrum of colors, namely

15:32

red, orange, yellow, green,

15:37

blue, indigo and violet. This

15:40

shows that white light is actually a

15:42

combination of the

15:44

seven colors mentioned above, called

15:47

polychromatic light. Meanwhile, light that

15:49

only consists of one color is called

15:52

monochromatic light.

15:55

In the event of light dispersion by a

15:57

prism, a dispersion angle is formed which

15:59

is the width of the [music] spectrum

16:01

produced by the prism, the size of which

16:03

depends on the difference between the [music]

16:05

deviation angles of the purple and

16:08

red colors. The magnitude of this dispersion angle can be

16:11

calculated using the equation pi = nu -

16:15

nm * beta where pi is the

16:18

dispersion angle, nu is the refractive index of violet light, NM is the

16:23

refractive index of red light, and beta is the

16:26

peak angle or refractive angle of the prism.

16:30

And the last property of light is

16:32

polarization. Light polarization is the

16:35

phenomenon of partial absorption of the direction of

16:38

vibration of light waves. Light can be

16:41

polarized due to the following events:

16:43

reflection, refraction, and reflection,

16:46

double refraction or twin refraction,

16:49

selective absorption, scattering. And

16:52

this is an illustration of the path of

16:55

light polarization.

16:58

In light polarization, we can

16:59

determine the intensity of transmitted light

17:02

using two

17:04

polaroids. The first Polaroid [music]

17:06

is called a polarizer which functions

17:09

to pass polarized light with a

17:12

vibration direction according to the easy axis P1. The

17:15

second polaroid is called an analyzer, which

17:18

functions to analyze the light

17:20

passed through the polarizer. When

17:23

the analyzer is rotated, then [music]

17:25

when the easy axis P2 is parallel to the

17:28

easy axis of the polarizer P1, the brightest light will be seen

17:31

. Next, the light

17:34

will dim and will appear dark when

17:36

P1 and P2 are perpendicular to each other. If the angle

17:40

formed between P1 and P2 is

17:43

theta, then the intensity of light

17:45

passed through the analyzer is I2 = I1

17:50

cos² theta = 1/2 I0 [music] cos² theta

17:55

with I0 the initial light intensity I1

17:59

the intensity of the polarized light coming out

18:01

of the polarizer and I2 the intensity of the

18:04

polarized light coming out of

18:07

the analyzer all three in

18:10

watts/m².

18:13

So, friends, that was

18:15

our entire discussion about the

18:17

properties of light, namely reflection

18:20

, refraction, refraction,

18:23

combination, interference, bending,

18:25

[music]

18:26

diffraction, dispersion, and

18:29

polarization. Friends can

18:31

understand it, right?

18:34

So that friends understand better, let's

18:36

solve the following example problem. The

18:40

first question, it is known that the

18:42

wavelength of the incident double-slit interference is

18:44

7,500 [music]

18:47

angstroms which we convert to meters

18:50

to 7.5 * 10^ -7 m. Slit width 0.2

18:56

mm = 2 * 10^ -4 m. The distance from the slit to the screen is

19:01

1 m and the distance from the center light to the

19:04

outermost light is 7.5 cm. This means yn = 7.5

19:10

cm = 7.5 * 10^ -2 m. The question is the number of

19:17

bright lines on the screen or n? Well,

19:20

we know the equation used to

19:22

solve the problem of the light pattern in

19:24

double slit interference is dn/l

19:28

= n lambda. Then we enter all the

19:31

quantity values ​​that have been converted

19:33

to meters. 2 * 10^ -4 * 7.5 *

19:39

10^ -2/1

19:42

= n * 7.5 * 10^ -7. We do the

19:47

arithmetic operation until we get n = 15/7.5

19:52

* 10^1 = 20. So the number of bright lines

19:57

on the screen is 20. The correct answer is

20:00

D.

20:02

Second question. It is known that the wavelength

20:05

incident on the thin membrane is 589.3

20:10

nm. We don't need to convert

20:13

to meters because the answer choices

20:15

in the question are also in nanometers.

20:18

The refractive index of soapy water is n = 1.33.

20:23

Since what occurs is the first bright pattern

20:25

, the interference order

20:28

is 1 and the refraction angle is perpendicular

20:31

to the thin film, [music] so r = 0

20:34

degrees. What is asked in this question

20:37

is the thickness of the membrane or d. To

20:40

answer this, we recall the

20:42

thin film interference equation in the

20:45

bright pattern, namely 2nd cos r = m - 1/2 *

20:51

lambda. So to find the value of d =

20:54

[music] m - 1/2 * lambda/2n

20:59

cos r. We plug in the known values ​​of the quantities

21:02

in the equation. D = 1 - 1/2 *

21:07

589.3/2

21:11

* 1.33

21:14

* 1 and we do the arithmetic operation

21:17

until we get D = 110.8

21:21

nm. [music] So the thickness of the soap water film

21:24

is 110.8

21:27

nm. The correct answer is A.

21:31

Next question. It is known that the radius of the circle of

21:33

Newton's ring is small R = 1 mm =

21:38

1 * 10^ -3 m. The radius of the convex plane or

21:44

r is 4 m. And the refractive index of the lens n =

21:49

1. Because the pattern that occurs is the

21:51

first light, then m = 1. [music]

21:54

What is asked is the wavelength of light

21:57

or lambda. We know this problem is

21:59

related to

22:01

Newton's ring interference whose bright circle pattern equation

22:04

is NR² = m - 1/2 * lambda

22:10

r. So to find lambda we

22:13

can enter the value of the

22:14

known quantity. 1 * 10^ -3^ 2 = 1 - 1/2 *

22:23

lambda * 4. Lambda = 1 * 10^ -6/2.

22:29

Lambda = 5 * 10^ -7 m = 5,000 angstroms.

22:35

So the correct answer is C.

22:39

Fourth question. It is known that a grating in

22:42

the fraction of 1500 lines/cm is passed by a

22:46

beam of light from a lamp which

22:49

produces a bright pattern of n = 1. If the

22:52

first order deviation angle is 30

22:55

degrees, we are asked to determine the

22:58

wavelength of light from the lamp.

23:00

In grating diffraction, the equation

23:02

used is d sin theta = n lambda

23:07

with d = 1/n. [music]

23:09

So the equation becomes 1/n sin theta

23:13

= n lambda. We enter the value of the

23:16

known quantity. 1/1500

23:19

sin 30 degrees = 1 lambda. So

23:23

we get lambda = 0.0033

23:28

cm = 3.33

23:32

* 10^ -6 m. So, the wavelength of

23:36

light from the lamp is 3.33

23:40

* 10^ -6 m. The correct answer is A.

23:45

Next question. It is known that the refracting angle

23:48

of the prism is 10 degrees. The refractive index of

23:51

red light NM = 1.60

23:55

and violet NU = 1.64.

23:59

This question asks us to determine the size of the

24:01

angle of dispersion in a prism. To

24:04

calculate the angle of dispersion of a prism, we

24:06

use the equation pi = nu - nf * beta.

24:12

Then we enter the known value of the quantity

24:14

. Pi = 1.64

24:18

- 1.60

24:20

* 10 degrees. So we get pi =

24:24

0.04 * 10 degrees = 0.4 degrees. So

24:29

the angle of dispersion of the prism is 0.4

24:32

degrees. The correct answer is D.

24:36

Last question. It is known that the angle between the

24:39

polarizer and analyzer is 60 degrees

24:42

and the initial natural light intensity is 124

24:46

watts/m²

24:48

with I1 only 50%. This means that I1 in

24:52

this case is only 1/2 I0. What is asked

24:55

in the question is the intensity of light

24:58

coming out of the analyzer or I2.

25:01

Well, we can calculate I2 at

25:03

this polarization with the equation I2 = I1

25:08

cos² theta. Since I1 = 1/2,

25:13

then I2 = 1/2 cos² theta. We enter

25:19

known numbers. I2 = 1/2 * 124 *

25:25

cos² 60 degrees. So we get I2 =

25:30

124/2

25:32

* 1/2

25:35

= 15.5 W/m². [music]

25:39

So the intensity of light coming out

25:42

of the analyzer is 15.5 W/m².

25:47

The answer is A.

25:49

Okay, guys. Thus

25:51

our discussion about light waves. Don't

25:54

forget to keep watching about

25:56

light waves. Don't forget to keep watching the

25:58

latest videos on our channel, OK?

26:00

See you in the next video.

26:04

[music]

26:10

Yeah.

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