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chapter 6 i

Mark Lubrick · 877 words · 4 min read

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0:00if we go back to our slide from last

0:03week and look at the electromagnetic

0:04spectrum and how it interacts with our

0:06atmosphere how its absorbed by our

0:08atmosphere a clearer picture starts to

0:10emerge we've got the visible part

0:12remember that goes all the way down and

0:14we can see it on earth whereas the radio

0:16as well we have these optical and radio

0:18windows so we can actually do visible

0:22astronomy and radio astronomy from the

0:24surface of Earth and we said we can do

0:27some infrared as well it's pretty

0:29difficult but some of it gets blocked

0:32but not all Vince it can make it pretty

0:35far down in the atmosphere and so what

0:38they started to try to do early on was

0:41actually try and get higher up in our

0:43atmosphere they did things like trying

0:45to use balloons and actually one of the

0:47early attempts was actually a plane they

0:50put an infrared telescope in a plane and

0:54try to detect infrared rays actually do

0:58infrared astronomy from a plane so it

1:01was kind of a neat way of doing it

1:03and again we're getting a buffs on the

1:05atmosphere some of the interference and

1:08also hopefully that'll help cool things

1:11down a bit because we're getting higher

1:12up in the atmosphere it's gonna be

1:13colder but even better is if we can put

1:16it in space space is incredibly cold so

1:20that idea that we have to make a

1:22telescope and infrared one down to about

1:25a couple Kelvin that's a lot easier in

1:28space because we're not getting the

1:30heating effects we just have to make

1:32sure the actual operating material of

1:36the telescope itself doesn't get heated

1:37so putting it in space is the ideal

1:41solution of course this isn't cheap just

1:45have rockets to launch it into space so

1:47this isn't always the most practical

1:49option and that's why we still do a lot

1:52of observations from Earth because it is

1:55very expensive but it is worth it

1:58especially when we started looking those

1:59parts the spectrum like infrared that

2:01are hard to see from Earth we can get

2:03these spectacular images and study these

2:05objects that are difficult to study

2:06otherwise but it's also nice to try and

2:12do

2:13and visible from space as well again

2:16remember we get that twinkling of the

2:18stars because of the atmosphere and we

2:20try to increase our resolution well in

2:22space we don't have to worry about the

2:24atmosphere limiting our resolution

2:26because there's no atmosphere so putting

2:29a visible telescope in space allows us

2:31to get images of amazing quality only

2:34limited by the size of the telescope

2:36itself and one of the most famous one of

2:39the most significant missions was the

2:41hubble space telescope

2:43this actually was designed to get

2:45visible infrared and ultraviolet

2:47radiation haven't really alluded to this

2:50before but really ultraviolet could also

2:52be used or used the same kind of mirrors

2:55we use for visible so the same basic

2:57setup we use for visible really covers

2:59infrared and ultraviolet again really

3:01the CCDs the detector changes but the

3:04basic setup remains the same for all

3:06three of those now Hubble telescope

3:10again was an incredibly important

3:14mission it was meant to change the way

3:17we used see the universe see objects

3:20we'd never witnessed before in details

3:22we never could

3:23but when Hubble was first launched and

3:26we started to make our images there is a

3:29huge problem

3:30they were blurry it turned out the main

3:35mirror was actually had a design flaw

3:39it was just slightly out of shape by

3:43about one fiftieth the width of a human

3:46hair think about that and if you've got

3:49a hair lying around that's following on

3:50your shoulder look at your hair and

3:52think one-fiftieth the width of that

3:54that's how little misshapen this mirror

3:58was but it meant the images were blurry

4:03they weren't what we had expected this

4:05was a huge blow in terms of what we were

4:08hoping to get from the Hubble Space

4:09Telescope so what they actually ended up

4:12having to do is send some astronauts up

4:14there and basically in essence give it

4:17glasses give it corrective optics to try

4:21to account for this which did actually

4:24work and now the Hubble Space

4:26Telescope's been providing amazing

4:28images ever since since about 1993 it

4:33was fixed and it has been changing our

4:37way of looking at the universe

4:38identifying incredible images Deep Field

4:41images of tons of different galaxies I

4:43mean look at this image all these weird

4:46cool shaped galaxies and it's again

4:51originally was designed poorly

4:53apparently it was meant to save money

4:55they didn't do a full testing of the

4:58optical mirror before launching it oops

5:01but they did end up fixing it and we've

5:05gone spectacular images because again

5:07it's in space so there is no atmosphere

5:09to limit its resolution this mirror is

5:11not actually that big

5:13it's about 2.4 meters compared to some

5:17of the other ones we're talking about

5:18like the Keck that are 10 meters it's

5:20the only 2.4 but because it's in space

5:23you can get much better images it's not

5:25limited by that bad seeing caused by our

5:29atmosphere

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