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Chapter 5 h

Mark Lubrick · 1,171 words · 6 min read

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0:00there's a few properties of light that

0:02we can look at and firstly is the idea

0:04of reflection when light hits a surface

0:07it can reflect or bounce off of that

0:10surface and that's why in this image

0:12right here we get this nice beautiful

0:14dual image of the mountains you can see

0:18it's like a mirror image of the

0:19mountains reflected in the water light

0:21it's coming off the water towards us and

0:24we see the same image of the mountain

0:27again but some of that light will also

0:31actually pass through into the water

0:34some reflects off but some will go into

0:37the water and when it does it will

0:39refract or bend meaning light going into

0:43the water won't follow a straight line

0:45it would actually Bend when it passes

0:47into the water and that's true whether

0:50we're talking to water or if it was

0:52going from air to glass when it passes

0:55from one material to another light will

0:57actually refract or bend and one case of

1:02this is when we'd look at the light

1:04going to represent specifically white

1:07light when we look at the light coming

1:09from the Sun it's called white light and

1:12that's because it considered and

1:13consists of all the colors of the

1:16rainbow but when we see it we see white

1:19light I mean you shouldn't be staring at

1:21the Sun ever but if you see the light

1:22coming from it it looks white we don't

1:24see all different colors however if we

1:27take that light and we put it through a

1:30prism the dip we will actually see that

1:33it is made up of all the colors of a

1:35rainbow and what happens is when the

1:38light goes into the prism it refracts or

1:41bends you can see here's a nice example

1:43of it it doesn't follow a straight path

1:45it bends at the border between our

1:48medium here and the prism well

1:51the strange thing is the different

1:55colors will actually Bend different

1:58amounts because of their different

1:59wavelengths so red light and blue light

2:02or violet or yellow or green all Bend at

2:06slightly different angles

2:08and then when it comes out the other

2:11side of the prism it will Bend again and

2:13again all the different colors will pen

2:15slightly different and what happens is

2:17we get the white light dispersed

2:20dispersed into all the different colors

2:23so white light made up of all the colors

2:26we can use this prism to split it into

2:28all the different colors and see them

2:30and we see a nice beautiful rainbow of

2:33colors in fact this is why we see

2:36rainbows in the case of a rainbow the

2:39raindrops are acting as our prisms and

2:43now technically there's a little other

2:44complication and the fact that the light

2:46actually bends and like hits the back

2:49surface of the raindrop and then comes

2:51back but the idea is still the same the

2:53raindrop acts as a prism and takes the

2:56white light from the Sun and splits it

2:58into all the colors of the rainbow quite

3:01literally the rainbow in this case so we

3:04get this nice beautiful rainbow because

3:06the light is being split into all of its

3:09component covers because sunlight

3:11actually has it all in there but in

3:15science we can also use this because

3:18what will I use is a so-called

3:19spectrometer a spectrometer to study the

3:23spectrums of light so what we do is take

3:27white light and we can split it into the

3:29different colors and that to do that we

3:32use a spectrometer or and this whole

3:35process is called spectroscopy we're

3:37studying the spectrum of colors and

3:39really what you're doing is taking a

3:41light source say hey maybe this light

3:44from the Sun and we put it through this

3:46narrow slit the reason we're doing that

3:48is because we're narrowing it down to

3:49one beam of light put that through a

3:52prism and it splits it into our spectrum

3:55of colors and this is the simple setup

3:57of a spectrometer right here now what

4:01we're seeing right here when we see all

4:03of the colors in a rainbow is can tell

4:05called a continuous spectrum we're gonna

4:07see we get different type of spectra

4:09different types of these spectrums

4:11depending on what is our light source

4:13for a continuous spectrum what we have

4:16is some kind of hot dense gas or solid

4:20that would give a can

4:22tenuous spectrum of colors all the way

4:24from red through violet

4:26often we think of blue as the follower

4:29side but technically it's violet if we

4:31think of Roy G before remembering the

4:33colors but if we see all of the colors

4:36it's considered a continuous spectrum

4:38because you can see it's all the colors

4:40continuously with no breaks and that is

4:43once again when you have say a hot dense

4:48gas or a solid giving off the light but

4:53what can also happen is if we instead

4:56use for the light source a gas a

5:01low-density gas that we heat up what we

5:04find is we get a so-called emission

5:07spectrum emission spectrum or emission

5:10line spectrum and it looks like this or

5:13something like this anyway where we only

5:16get certain lines of color against a

5:19black background we are missing many of

5:21those lines we don't have all of the

5:23colors of rainbow we just get some lines

5:26against this background and now the

5:30thing is the spectrum we get depends on

5:34what the gas is made up of and we

5:37actually find each gas each atom of gas

5:40each element of gas whether we're using

5:42hydrogen or helium they would be very

5:45different they would each have their own

5:47unique pattern you can think of this

5:49like a barcode each element has its own

5:52unique pattern its own unique barcode so

5:56if you took gas that you had no idea

5:59what it was and if you were able to heat

6:01up this low-density gas run it through

6:03spectroscope or spectrometer we'd be

6:06able to determine what it is just by

6:08matching up the barcode against one that

6:10we know is we've mapped these all out in

6:12the lab and seen what they look like so

6:14we know all the different elements what

6:16their pattern should look like and again

6:19each one is unique that's kind of the

6:22neat thing about it so this is an

6:23emission spectrum where we don't have

6:26all of the continuous spectrum just

6:28certain lines within it and again each

6:33element has its own unique pattern and

6:35you can see

6:36this shows a little bit better they

6:38aren't gonna have all the colors in a

6:39rainbow different elements have their

6:41own unique little barcode if you will

6:44and you can compare that against a

6:45continuous spectrum where all the colors

6:47are there there whereas this is just

6:50certain lines so yeah already a very

6:54useful idea we can determine what the

6:57elements of a gas are

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