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Section 2.1 b

Mark Lubrick · 1,121 words · 6 min read

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0:00what does this mean if the Sun is

0:02actually rotating or seeming to rotate

0:05around us or at least is moving relative

0:07to the Stars

0:09well how we see the Sun where it's lined

0:12up relative to the Stars behind it

0:16changes throughout the year and I mean

0:19this would be very difficult to see

0:21during the day because the stars are not

0:23visible because the Sun is so bright but

0:25if you extrapolate it out knowing where

0:27it was the Sun would seem to line up in

0:29front of a different set of stars

0:32throughout the year and this might be

0:34familiar to many of you it's the so

0:36called zodiac the zodiac where the Sun

0:39seems to appear relative to us when we

0:42look at the Sun where it would be lined

0:44up with the Stars does change out

0:46through the year as it does a full as we

0:48sorry do a full 360 around the Sun so it

0:53seems to line up and that's where the

0:54zodiac comes from where the Sun would be

0:57in front of what stars and this is

0:59something we're going to talk about more

1:01in a later chapter when we talk about

1:03astrology and in essence why it actually

1:05makes no sense but we'll get there a

1:08little bit later now another thing

1:10that's important to note is that all the

1:13planets and even the moon all seem to

1:15orbit very close to this ecliptic as

1:18well so if we look at this image right

1:21here you can see the ecliptic visit has

1:23been superimposed on top of it this line

1:25right here and you can see all of the

1:27planets and the moon morrow Saturn all

1:29of these ones are very close to the

1:31ecliptic and this is not a coincidence

1:33what we find is when we look at our

1:35solar system is in essence that is very

1:38flat all of the planets orbiting the Sun

1:41all orbit on a very similar plane but we

1:46also have to talk about constellations

1:47in general because they're actually kind

1:50of important for astronomy we actually

1:52divide the sky that celestial sphere

1:55into 88 different constellations and now

1:58they're not all the same size but this

2:01is a very rough way of organizing the

2:05sky and actually being able to give

2:07directions now what do I mean by that

2:09well if the sky is divided into 88

2:12constellations

2:13and I say well this is in the Orion

2:16constellation I know the rough part of

2:19the sky that that relates to I don't

2:21know exactly where in the sky that is

2:23but it tells me a rough direction your

2:26book talks about the idea of comparing

2:28this to the States I like how it divides

2:30it into States well sure if I say it's

2:34in California I don't know exactly where

2:36that is

2:37but it gives me a pretty good idea it's

2:39a very similar thing here by referring

2:42to what constellation something's in I

2:45get a rough idea of what portion of the

2:47sky it is in and in the next video we're

2:50gonna see a more specific way of

2:52dividing it in and actually giving

2:53coordinate system but this gives you a

2:55rough idea of where in the sky something

2:57is so these constellations are still

2:59useful even if they often look nothing

3:01like what they're supposed to in fact

3:03that's not an accident either if you

3:06look at your book it describes the idea

3:08that some of these were just named after

3:10famous things so they didn't necessarily

3:12look like the objects they were named

3:15after but one last point worth noting is

3:20that these constellations aren't

3:23groupings of stars like most people seem

3:25to think many of these constellations

3:27have stars that are nowhere near each

3:29other if you look at the Big Dipper this

3:32is an actual image of how far the stars

3:34would be they are nowhere near each

3:36other it just so happens the stars

3:38appear in the same direction when we

3:40look into night sky from our perspective

3:42on earth if someone was looking from a

3:44different planet a different solar

3:45system they would see very very

3:47different constellations and so these

3:50constellations are not actual groupings

3:52of stars they are just in the same

3:54general direction what is this whole

3:57idea of angular size let's take a look

4:01at some demonstrations of this actually

4:03because angular size is an important

4:05concept it is the angle and objects

4:08takes up when you're looking from one

4:10side to the other let's jump to some

4:15examples so angular size it says this

4:20angular size of an object depends on how

4:22big the object is and how far away it is

4:24from us well let's think for a second if

4:26that makes it

4:27here's my pan my nice chewed-up and I

4:31don't know why I always chew on it well

4:34my pen is a fixed size it's not gonna

4:36change I'm not magic this pen is a pen

4:39what happens as I move it towards the

4:41camera seems to be getting bigger it's

4:45not but all that's happening is this

4:48angular size is changing as its distance

4:52from us the viewer changes so angular

4:56size and let's use my cell phone we're

5:02going to use this as a demonstration of

5:03angular size right here again angular

5:05size is if I was looking at the angle

5:09would actually take something here let's

5:10demonstrate let's say I am someone

5:12standing right here so this is me the

5:15angular size of my phone from this

5:17perspective would literally just be the

5:20angle it takes up when looking from one

5:22side to the other so this we could

5:27define as the angular size I can even

5:29give it a fancy simulator and that's

5:31just the size this object takes up from

5:33this perspective what happens if I move

5:36my phone relative so I'm still standing

5:38here

5:38go paper two-dimensional me now my phone

5:42has moved closer

5:52okay now the angular size has changed

5:56the angular size would be this distance

5:58Peter - I could even call it if I wanted

6:01to nothing changed I'm still at the same

6:03spot this phone is still the same size

6:06phone it's just because of its relative

6:09position it now seems larger to me which

6:12again is the very long way of doing this

6:14demonstration I did right here but

6:18hopefully that actually demonstrates the

6:22idea and please ask questions if not

6:25this is a concept were going to come

6:27back to especially when we started

6:29looking at our Sun and Moon combination

6:32angular size becomes very important and

6:34a whole explanation of why you get into

6:36Clips actually

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