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Chapter 2 f

Mark Lubrick · 1,285 words · 6 min read

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0:00we're ready to start moving on to the

0:02more recent models of the universe and

0:06how we actually understand the universe

0:07and nicolaus copernicus is one of the

0:10more famous early astronomers he really

0:15helped push forward the idea of the

0:17heliocentric or sun-centered model the

0:21idea that earth is not the center the

0:24Sun is again he was definitely not the

0:26first person to suggest this idea but he

0:29really started getting the conversation

0:30going again you can see it's now been

0:32hundreds and hundreds of years we left

0:34off at about a hundred and forty ad with

0:37Ptolemies model that was very

0:40complicated but did a pretty good job of

0:42describing the motion of objects but by

0:45this point they've started to get more

0:46and more observations that see that his

0:49model still doesn't fit perfectly and so

0:52people like Copernicus we really started

0:54pushing forward the idea of the

0:55heliocentric model and actually he

0:57published a book in the book he wrote

0:59was published the year he died in 1543

1:02and started getting this conversation

1:04going now this model was still a little

1:08flawed they still believe the circle was

1:10a perfect shape and so they said that

1:13sure we were rotating around the Sun but

1:17we were doing so in a perfect circle and

1:19so were the other planets so a bit of a

1:22mistake but it was still pushing forward

1:25a much better way it could describe the

1:26retrograde motion the planets we saw a

1:28much much nicer because that's actually

1:30what was happening so it was a simpler

1:32cleaner model and that was one of its

1:34appeals and it started the conversation

1:36going

1:38of course Galileo Galilee is also very

1:42very famous he was early scientist

1:45really and he studied mechanics

1:47mechanics is really studying the motion

1:49of objects and the forces causing those

1:53motions and he started actually making

1:55some very good observations started

1:58making some great conclusions for one

2:00thing what he found was that when he

2:03studied objects that were moving objects

2:07that were moving say falling through the

2:09air or rolling down a ramp he found that

2:13the

2:13acceleration was the same was a uniform

2:17acceleration an acceleration is the

2:20change of speed or direction so if

2:23something speeding up when your car

2:25speeds up or slows down that's

2:27acceleration when it changes direction

2:29that's technically acceleration as well

2:31so he's found that this acceleration was

2:35uniform for these falling objects

2:37something that is kind of important

2:39we'll talk more about later but he also

2:44found that objects tend to stay either

2:50moving or at rest up tonin everyone kind

2:54of thought the idea was things at rest

2:56was the natural state but he had this

2:57idea that look if you could get slippery

2:59enough surface it would keep sliding and

3:02I mean this idea where I'm not gonna go

3:04into too much right now because we're

3:05gonna see it more in Chapter three when

3:07we started talking about Newton but it

3:09isn't worth no-neck Galileo actually

3:11started talking about these ideas first

3:13so he's much more famous though for what

3:18he did with astronomy because he

3:22actually ended up building a telescope

3:24he wasn't the first person in milled a

3:26telescope but it was neat because he

3:29heard the description of what a

3:30telescope was and from that built one

3:33never actually saw it but built one

3:36himself and he eventually realized he

3:38could turn this towards the skies and

3:39study objects that hadn't been studied

3:42before the objects that were too faint

3:44for the human eye to see he could turn

3:46and look at them and see things in much

3:49more detail he could magnify these

3:51objects and see them as they were much

3:54much closer much larger so this was one

3:57of his very early telescopes and he saw

4:01their idea of things again he was a

4:04proponent of the heliocentric model he

4:07thought hey this makes sense and he said

4:10about trying to prove it again a very

4:13good first early scientist started

4:15trying to prove it and he's noticed a

4:17few things one of the things he saw is

4:19that there was moons orbiting Jupiter

4:22the we'll see talk about these later he

4:25found moon

4:26orbiting Jupiter and right away this was

4:29a bit of a challenge to the earth center

4:31model we had thought everything revolves

4:34around the earth but here he was able to

4:36see something rotating around something

4:38else so he showed there was something

4:42spinning around Jupiter moons it had its

4:45own moon so all of a sudden already and

4:47pointing out main Aerith isn't so

4:48special in fact Juber had more moons

4:51than we did great well he also studied

4:55the moon and what he found was a bit

4:57surprising he saw a lot of craters and

4:59mountains valleys basically a lot of the

5:01features we associate with earth and it

5:04started being clear that maybe earth

5:06wasn't so special these features were on

5:08another object as well and so maybe they

5:11even have a similar history maybe earth

5:14isn't so special isn't it the center of

5:16everything but the true death Knoll -

5:21the geocentric model this idea that

5:25Earth is the center well Galileo studied

5:29the phases of Venus and now just like

5:33our Moon can go through phases Venus can

5:35go through phases remember

5:37Venus or like our Moon was only lit to

5:40us from the Sun the Sun shines light

5:43reflects off the moon and thus we see it

5:45same with Venus we see Venus because of

5:48a reflection of light from the Sun and

5:50so it also goes through phases as we

5:54both orbit the Sun the thing was it

5:57could go through phases if it was

6:00rotating around Earth but not the phases

6:04that Galileo observed Galileo observed

6:08phases of Venus that couldn't be

6:11explained in the geocentric model it was

6:14not possible this was the defining key

6:19observation that showed geocentric model

6:21was wrong it couldn't explain this you

6:25could put as many deference and

6:27epicycles and weird complicated models

6:29as you wanted but this was the end this

6:32couldn't be described so geocentric

6:35model was wrong

6:36heliocentric model was right

6:38and you would think that's when it

6:40should have ended the debate should have

6:43ended unfortunately not unfortunately

6:47the geocentric model was very popular

6:49the Roman Catholic Church was very

6:52powerful and he was actually forced to

6:55go in front of the Inquisition he was

6:59forced to go in front the Inquisition

7:00they told him he had to retract his

7:03claims that he had to say nope that the

7:05earth was the center which he refused to

7:07do and so as a result he was placed

7:10under house arrest for his life he was

7:13locked away in his house also his books

7:18I mean again this was a defining

7:21characteristic showing that no

7:23geocentric model was wrong but still

7:261836

7:27hundreds of years later his books were

7:30still banned by the church because he

7:33was said to have been here ethical his

7:36work was here a C heresy it was against

7:40the teachings now it was in 1992 the

7:45church did admit that they'd handled

7:46this incorrectly but yeah it's worth

7:51noting that this man actually did suffer

7:55for his work he lost his freedoms and he

7:59was right his work was right he was

8:01trying to advance our understanding of

8:03the world and gave up his freedom to do

8:06so so we take these bits of knowledge

8:10for granted we know the earth is not the

8:13center but others had to fight for this

8:15knowledge and for this advancement to

8:17take place it's worth noting that

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