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chapter 6 b

Mark Lubrick · 1,291 words · 6 min read

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0:00now there is generally three main types

0:02of telescopes we're gonna talk about

0:04them a little more but the idea of a

0:06refractor a reflector or kind of a

0:10hybrid of the two a compound which we're

0:12not really gonna talk about the compound

0:13telescope but we're gonna focus on these

0:16refractor and reflector types remember

0:20though we're trying to gather as much

0:21light or radiation as possible and

0:24ideally bring it to a focus so that's

0:27the important thing to keep in mind here

0:31how do we do that well in the case of a

0:37refractor light is actually refracting

0:41through a lens in a case of a reflector

0:46light is reflecting off a mirror so the

0:49names kind of make sense it is important

0:51to remember that we're looking at

0:53objects that are very very far away and

0:56that means the light coming from them

0:58are in essence parallel light rays now

1:01we talked about this in a previous

1:03chapter we talked about how our Sun we

1:05could basically approximate the Rays

1:08coming from it as parallel when we're

1:10looking at things are even further the

1:12light rays really are parallel because

1:13any that didn't start off parallel would

1:16miss us so if the light rays coming from

1:19something hit us and hit even a

1:21relatively large telescope well any

1:24other rays coming in must also be

1:26parallel to those ones because they came

1:29from so far away like this image shows

1:31they would miss us if they were even a

1:34little bit off from being parallel to

1:36each other okay now why is the idea of

1:39parallel light rays important that

1:41relates to the idea of focusing the

1:43light rays remember when we looked at

1:46spectroscopy we saw a light passing

1:48through one medium will Bend well the

1:52light going through a lens will be bent

1:55and focused to a specific point I have

1:59so called focal point at a certain focal

2:02length from the lens I mean not the most

2:04creative names with very apt

2:05descriptions it gets focused to a point

2:07and that's where you get your clear

2:10image so that's the idea of the focus

2:12we're getting a clear

2:13image because of light rays from this

2:15distant object are getting focused to

2:18that point that's where you get your

2:19image in the case of the mirror the

2:21light actually rebounds or reflects off

2:25of the mirror and is also focused to the

2:28focal point at a certain poco length so

2:31the ideas are the same it's just in this

2:33case it's refracting through the lens in

2:35this case it's reflecting off the mirror

2:38which we will see has some important

2:40consequences but the over idea is still

2:42the same light comes in gets focused to

2:45a point because we have these parallel

2:47light rays that being said you might be

2:51asking yourself how do we get an image

2:54then for getting an image like how do we

2:57get an image if all the light is being

2:58focused to a point isn't it all just

3:00blur it on top of each other well we've

3:03added we had a bit of a simplification

3:05in a previous slide we talked about all

3:06the light rays being parallel well

3:09technically the object we're looking at

3:11is not just a dot necessarily I mean

3:14even when we see a star to us it looks

3:16like a dot but technically the light

3:18coming from the top and the light coming

3:19from the bottom will come in at slightly

3:21different angles and of course we're

3:23looking at something even closer the

3:25light gets from the top and the bottom

3:27is different and so this has a nice

3:30demonstration if you're looking at these

3:31rocks the light from this top rock comes

3:34in a slightly different angle than the

3:36light from the bottom Rock and thus

3:38those different rays actually get

3:40focused different the light from the

3:42bottom rock is still parallel to the

3:45rest of the life on the bottom rock so

3:47it all gets focused to a specific point

3:49but the light from the top Rock is gonna

3:51be focused to a different point because

3:53it's at a slightly different angle to

3:55this so light rays from the same thing

3:58are parallel but when you're comparing

4:00the top of an object to the bottom

4:02there's slightly different angles and

4:04gets focused slightly different and so

4:07this is a long way of saying we get an

4:09image it still produces an image just

4:12because each part gets focused to a

4:13slightly different part which is related

4:15to what we were seeing and thus we get

4:17an image one of the odd things though is

4:21that the image will actually be flipped

4:22because of the characteristics of optics

4:25the image would be flipped

4:26and the same basic idea is happening in

4:29our eyes not as this image shows this is

4:32a mirror and it's reflecting but when we

4:34were thought about the previous slide

4:36where shows a refractor with the lights

4:38going through a lens and being focused

4:40well that's what happens with your eyes

4:41your eye is just a lens same with your

4:45glasses if you use glasses your glasses

4:47are just helping focus the light to a

4:49specific point if there's your lens in

4:52your eyes doesn't quite focus it

4:54properly to the right place to be read

4:56and thus you get a blurry image but the

4:58lens in the glasses will help focus it

5:01so that it does actually end up at the

5:03right part and so you can actually see

5:06it but it is kind of funny that it does

5:08get inverted and our brain just flips it

5:11for us so we end up with an image of

5:14whatever we are looking at now again

5:20this show is a basic setup of the

5:22refractor and reflector telescopes what

5:25we have is the light coming in and

5:28either refracting through a lens or

5:31reflecting off the mirror but the thing

5:35is we don't often just stop there what

5:39we want is the image to actually be hot

5:43summer to be viewable in the case of

5:45amateur telescopes usually there's an

5:47eyepiece we want to be able to actually

5:48see a copy of this image at the eyepiece

5:51and so the light even though it might be

5:54focused to a point often what will

5:56happen is it'll be either deflected out

6:00an eyepiece or yeah maybe by secondary

6:03mirror or it just goes to the eyepiece

6:07here in the refractor case the main idea

6:09is we want to be able to actually put

6:10our eye there and see the actual image

6:14because otherwise if it's just focused

6:17within the me and the actual telescope

6:19well great you can't see that and in

6:21this case if it was focused here sure if

6:25you had a nice beautiful image but you

6:26couldn't see it wouldn't be helpful so

6:28often what we actually have is a

6:29secondary mirror that will deflect it to

6:32an eyepiece or other situations and

6:35allude to in a second but one of the

6:38advantages of telescopes right now

6:40again we get this nice focused image we

6:43can see it but many modern telescopes

6:45have a variety of eyepieces that come

6:47with them as well and the thing is each

6:50of these eyepieces allow a slightly

6:52different magnification we have the

6:54light coming in from our image we get

6:56our image and it's focused to a point

6:57but the size the magnification of that

7:00image can be modified by the eyepieces

7:03so when you actually view it so often

7:06with amateur telescopes you're gonna see

7:08they come with a variety of eyepieces so

7:10you can see it at different

7:12magnifications

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