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Section 4.2

Mark Lubrick · 1,274 words · 6 min read

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0:00the next thing we want to consider is

0:01the idea of seasons and why we have

0:04because there's actually quite a bit of

0:06misconception around it most commonly

0:09people think we have different seasons

0:11because of the different distance we are

0:13from the Sun and now it's true that we

0:16do vary our distance from the Sun but

0:19it's not by a very large amount it's

0:21only about 3% and well for thus those of

0:25us in North America we're actually

0:27closer to the Sun during our winter than

0:30during our summer so clearly that's not

0:33the case so what's the reason well it's

0:36because of the tilt of our axis of

0:39rotation

0:40remember that's that big metal spike if

0:42we jabbed it through the earth and we're

0:44rotating spike that's the thing we're

0:47rotating about well you can see that's

0:51our big metal spike in the image right

0:52here and it's tilted at about 23.5

0:56degrees so that means how we are facing

1:00the Sun changes from time to time if

1:04we're in the summer for North America

1:06our part of the planet is actually

1:10tilted more towards the Sun and then in

1:12our winter we are actually tilted away

1:14from the Sun and thus it's the opposite

1:17and the other side of the planet well we

1:21also have these vernal equinox autumn

1:24equinoxes the idea is that equinoxes for

1:27equal and in fact remember vernal

1:29equinox was where we defined our zero

1:32point for our right ascension so it's

1:36important idea it's that time of day a

1:38year that March 21st where the Sun is it

1:41gives us an idea a zero point for where

1:43to compare and the reason these are

1:45equal or equinoxes in the name is

1:47because you can see that tilt doesn't

1:50matter in this case the tilt doesn't

1:53actually go towards or away from the Sun

1:55so both both the north and south

1:58hemisphere are getting the same amount

2:01of sunlight at these two times great

2:05well let's keep going why does that

2:08really account for the seasons again I

2:09mean we're tilted towards the Sun

2:11well that has a couple different effects

2:15for one thing the angle of the sunlight

2:17is actually different in those two

2:19different times in our summer the

2:21sunlight is coming more directly on us

2:24in fact let's go back to that image for

2:26a second and you can see it be more

2:29directed at us

2:30whereas here you'd be more or again

2:33leaning away if you will and so the

2:35sunlight actually gets spread out over a

2:37bigger angle the same amount of sunrays

2:39being spread out over a larger area

2:41means it's not gonna heat up as much so

2:44in the winter the Sun that gets more

2:46spread up and that's not as effective

2:48but even more than that the sun's

2:51position if we were going back to the

2:53idea of the celestial sphere we could

2:56think of how the Sun is rotating around

2:57us I remember of course it's not

2:59actually rotating around us we're

3:01rotating relative to it but where it

3:03would appear in the sky changes

3:05throughout the year for us in North

3:09America during the summer months is much

3:11higher up and thus as it goes around

3:15due to our rotation let's just go the

3:18proper way of explaining it if we think

3:20of how it seems to go across the sky due

3:23to Earth's rotation well during the

3:26summer it has further to travel so it's

3:28out longer we have a day with more

3:31sunlight by the time we're in the winter

3:35the Sun is much lower

3:37from our perspective and thus it's not

3:39out for as long so not only is the

3:42sunlight more direct but it's also out

3:44for longer and that's why in the summer

3:46it's warmer nothing to do with the

3:48distance from us to the Sun again we're

3:51actually further in the summer it's all

3:54about how we are tilted relative to

3:57orbiting around the Sun now the strength

4:01of this effect depends on where you are

4:04if you're in the northern hemisphere of

4:06course versus the southern hemisphere

4:08it's completely different our summer

4:09their winter the opposite but even how

4:14much you notice the seasons really

4:16depends on where you are and if you look

4:18at this image right here you can see

4:21where this is the two different times

4:22one we're tota towards the Sun one will

4:24toss it away

4:25but if you look at see the equator the

4:28effects are not gonna be as strong the

4:31sunlight still gonna be fairly direct in

4:33both of these cases and this amount of

4:36sunlight is gonna be very similar so

4:38they won't notice the seasonal change as

4:40drastically as someone who is very far

4:43north in fact if you were say really far

4:45north you can get to certain times of

4:47the year where the Sun won't go down

4:49it's so high up in the sky it won't go

4:52down for months and months and once at a

4:55time so you might have six months of

4:57sunlight six months of darkness

4:58depending on where you are it really

5:01depends on how far north and south on

5:04our planet you are and how big of an

5:07effect you notice from season to season

5:11of course there is a couple real-world

5:14complications your book points to and I

5:16felt like it would be important to talk

5:17about them for one thing when people

5:19talk about how long the days are well

5:21our days are actually longer than

5:24science would normally predict I mean if

5:27you take all the things into account no

5:28science will get it right but if you're

5:31just looking at where the Sun is in the

5:34sky from one time to another our days

5:38would seem longer and it's because of

5:40this idea of a refraction refraction is

5:42the bending of light when it travels

5:44from one medium to another

5:46and if you've ever gone to the beach or

5:49had your legs in water you'll probably

5:52notice it it when you look down it looks

5:54like your legs kind of get cut off in a

5:55weird way it's because the light bends

5:57when it was into the water so this same

6:01thing happens in our atmosphere and what

6:03ends up happening is as say the Sun is

6:05setting some of the light gets bent and

6:08so we actually see that sunlight for

6:10longer than you would predict also we

6:15talk about summer solstice is when we'd

6:17have the most sunlight on us summer

6:20solstice for us in North America around

6:22June 21st we get the longest day of

6:26sunlight I mean the days of course are

6:28still the same length but the amount of

6:30sunlight we have in that day is the

6:32longest yet it's usually not the warmest

6:35day of the year I mean June 21st is not

6:37the day you're picturing going ah that's

6:38gonna be the war

6:39they usually sound like july/august is

6:41when you really are starting to enjoy

6:43the beach why well because the earth

6:48actually has to heat up sure we have

6:49tons of sunlight and it's very direct

6:52and out for long on the summer solstice

6:54but we still have the world is a little

6:58cold all that sunlight hitting the

7:01ground hitting the water especially if

7:03you're at like a lake that water's gonna

7:05take a while to warm up so summer

7:08solstice will not be the warmest day of

7:10the year but it will be the day that has

7:12the most sunlight for those of us in

7:14North America

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