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Chapter 2 a

Mark Lubrick · 1,187 words · 6 min read

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0:00welcome back this week we're gonna be

0:01starting off with chapter 2 but remember

0:03we already covered 2.1 in the first week

0:06we'll reference some of those ideas I

0:08mean many of the concepts in the course

0:10will build off of previous chapters and

0:12previous ideas but in this case we're

0:15gonna be starting off with 2.2 and let's

0:17get right to it

0:19so astronomies been around for a long

0:23time in some shape or form in fact the

0:25idea of cosmology us trying to study the

0:28universe trying to understand its

0:30structure and its origin it is something

0:32people have been doing since ancient

0:34times

0:34obviously the complexity with which we

0:37do it has changed drastically the

0:38techniques the tools we have to use has

0:41changed drastically

0:42but many early societies did study the

0:46sky for a variety of reasons in some

0:49cases it was simply a religious thing

0:51they thought the events occurring in the

0:54sky above them related to their gods and

0:57might indicate displeasure or at least

0:58tell them to avoid doing certain things

1:00so but many also use it for much more

1:04practical purposes such as calendars

1:06that's what we're actually able to see

1:08in these a lot of these rock formations

1:10were actually calendars meant to line up

1:13with specific things whether it might be

1:16lining up say with the moon's phases to

1:18tell us what time month it is and in

1:20some cases it's to line up with certain

1:23times of year

1:23in fact we'll talk about stonehedge

1:25later on and see that it's an example of

1:27that but often society is needed to know

1:30when say to plant their crops for them

1:33these interests were a matter of

1:34survival knowing when to plant your

1:36crops could mean the difference between

1:38your civilization surviving or not if

1:41you weren't able to make enough food to

1:42feed everyone people are gonna die

1:45so you need to actually be able to

1:46predict what time of year it is and I

1:49mean that sounds maybe like a silly idea

1:50to us now but they didn't have a phone

1:52to look and go oh that's the day I mean

1:55they had to find a some way to predict

1:58growing seasons also a lot of people are

2:02using it for like seafaring if your

2:03culture was trying to travel well if

2:06they didn't have compass they had to use

2:08things like the Stars to try and

2:10navigate so there was a lot of very

2:12practical

2:13reasons they study this guy and started

2:15trying to actually make very simple

2:18instruments to tell them things now

2:23we're going to keep going and look at

2:25some of these early things and early

2:27models or the ideas one thing I want to

2:29mention though right off the bat you're

2:30gonna notice I'm putting a lot of dates

2:32like the birth dates and death dates of

2:34these people like Aristotle here I'm not

2:36gonna expect you to know that I would

2:38not expect you to know that Aristotle

2:40was born in 384 BCE

2:42because well I don't think that's

2:45necessarily an important detail for you

2:47to learn but I wanted to put the dates

2:49in here so you know roughly when this

2:51was occurring again like what kind of

2:53time frame we're looking at so just to

2:56give you an idea of how spaced out event

2:58some of these events are and again how

3:00early on they were like someone like

3:01Aristotle again 384 BCE before Common

3:05Era that's a long long time ago and

3:08thing is Aristotle was nice

3:12representative of his time in terms of

3:15what he believed a lot of the people had

3:18the similar beliefs to him well one

3:21thing Aristotle knew was that the Sun

3:23must be further from us than the moon

3:26they had noticed eclipses remember we

3:29talked about eclipses last week where

3:31the Sun Act he gets blocked by the moon

3:34they had noticed these events in history

3:35so they knew obviously if the moon was

3:38passing in from the Sun it must be

3:40closer to us they also understood the

3:43reason why the moon went through its

3:45phases again something we studied last

3:46week it goes through those phases

3:48because of it going around us and the

3:52sun's light hitting it so they were

3:54aware that it was a sunlight hitting and

3:57lighting the face of the Moon and that

3:58was what was causing it to go through

4:00the various phases but Aristotle also

4:04was able to argue that the earth was

4:06round something that we should all know

4:08for fact as of now and there was a

4:12couple different arguments he used for

4:13that for one thing the Eclipse Eclipse

4:19lunar eclipse in this case before we're

4:22looking at solar was why we knew that

4:24the moon

4:25could become between us and the Sun but

4:27the lunar eclipse remember that is the

4:30shadow of the earth passing across the

4:33moon and since that shadow always has a

4:37circular shape they knew earth was

4:40around because if I mean if you noticed

4:43that one's great you could argue that

4:44the world was flat and just in round

4:47shape and that we were lining it up but

4:49every eclipse every time there was a

4:52lunar eclipse it was circular no matter

4:55what angle was going on no matter what

4:57part of the earth was looking at it so

5:00he was able to from that justify that

5:02Hey look it must be a sphere because

5:05every part of it when it lines and goes

5:08across the moon is actually round so he

5:14was able to argue from that perspective

5:15that it was round but he also actually

5:17looked at the people traveling remember

5:22we talked about the celestial sphere and

5:23the Stars and then above us well what he

5:27said what Aristotle was arguing was that

5:29look if you travel far north the stars

5:33you see can actually change the Stars

5:37you see will change because eyes are

5:40getting higher up on earth you're seeing

5:42further up the celestial sphere you can

5:44actually see different stars remember

5:47you have that Zenith right above you you

5:50can see her to the horizon at 90 degrees

5:53from you that means you're not seeing

5:55the entire sky so as you get farther

5:57north what you would see the stars you

6:00see would be different and that was a

6:01very good argument to that obviously we

6:03must be moving across a curves feet

6:05surface as if it was earth was flat then

6:08we'd all be seeing the same stars so it

6:11was very convincing arguments hopefully

6:14these days well I mean there is still

6:16people who argue this in present day

6:18which is kind of silly

6:21I don't know what the conspiracy would

6:22be that would make us want the world to

6:25be round but there is quite a few

6:27compelling arguments your book lists a

6:30few others as well even I mean one being

6:33hey look we take satellite images in

6:35space and we clearly see it's a global

6:38as the satellites travel around it so

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