Reasons for the seasons - Rebecca Kaplan
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0:14 - 0:15When I was a kid,
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0:15 - 0:16my understanding of the seasons
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0:16 - 0:18was that December and January were cold
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0:18 - 0:20and covered with snow,
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0:20 - 0:22April and May were bursting with flowers,
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0:22 - 0:25July and August were hot and sunshiny,
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0:25 - 0:29and September and October were a kaleidoscope of colorful leaves.
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0:29 - 0:30It was just the way the world worked,
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0:30 - 0:32and it was magical.
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0:32 - 0:33If you had told me back then
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0:33 - 0:35that one-third of Earth's population
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0:35 - 0:37had never seen snow
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0:37 - 0:41or that July 4th was most definitely not a beach day,
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0:41 - 0:42I would have thought you were crazy.
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0:42 - 0:45But in reality, seasonal change with four distinct seasons
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0:45 - 0:48only happens in two regions on the planet.
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0:48 - 0:49And, even in those two,
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0:49 - 0:51the seasons are reversed.
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0:51 - 0:52But why?
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0:52 - 0:53A lot of people have heard of an astronomer
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0:53 - 0:55called Johannes Kepler
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0:55 - 0:57and how he proved that planetary orbits are elliptical
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0:57 - 1:00and that the sun is not at the center of the orbit.
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1:00 - 1:02It was a big deal when he figured this out
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1:02 - 1:03several hundred years ago.
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1:03 - 1:06His discovery solved a lot of mathematical problems
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1:06 - 1:07that astronomers were having
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1:07 - 1:09with planetary orbit measurements.
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1:09 - 1:12While it's true that our orbit's not perfectly circular,
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1:12 - 1:14those pictures in our science books,
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1:14 - 1:16on TV, and in the movies
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1:16 - 1:17give an exaggerated impression
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1:17 - 1:19of how elongated our orbit is.
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1:19 - 1:23In fact, Earth's orbit is very nearly a perfect circle.
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1:23 - 1:26However, because Earth's orbit is technically an ellipse,
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1:26 - 1:27even though it doesn't look like one,
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1:27 - 1:30and the sun isn't quite exactly at the center,
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1:30 - 1:31it means that our distance from the sun
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1:31 - 1:33does change through the year.
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1:33 - 1:34Ah-ha!
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1:34 - 1:38So, winter happens when the Earth is further away from the sun!
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1:38 - 1:39Well, no, not so fast.
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1:39 - 1:41The Earth is actually closer to the sun
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1:41 - 1:43in January than we are in July
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1:43 - 1:46by 5 million kilometers.
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1:46 - 1:48January is smack-dab in the middle
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1:48 - 1:50of the coldest season of the year
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1:50 - 1:51for those of us up north.
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1:51 - 1:52Still not convinced?
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1:52 - 1:54How about this:
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1:54 - 1:56Summer and winter occur simultaneously
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1:56 - 1:57on the surface of our planet.
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1:57 - 1:59When it's winter in Connecticut,
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1:59 - 2:00it's summer in New Zealand.
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2:00 - 2:02So, if it's not the distance from the sun,
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2:02 - 2:03what else could it be?
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2:03 - 2:05Well, we need to also need to know
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2:05 - 2:06that the Earth doesn't sit straight up.
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2:06 - 2:08It actually tilts.
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2:08 - 2:09And that axial tilt of the Earth
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2:09 - 2:12is one of the main reasons for the seasons.
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2:12 - 2:14The Earth spins on an axis
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2:14 - 2:17that's tilted 23.5 degrees from vertical.
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2:17 - 2:20At the same time, the Earth revolves around the sun
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2:20 - 2:23with the axis always pointing in the same direction in space.
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2:23 - 2:24Together with the tilt,
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2:24 - 2:26the spinning and revolving causes the number
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2:26 - 2:28of hours of daylight in a region to change
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2:28 - 2:29as the year goes by,
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2:29 - 2:31with more hours in summer
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2:31 - 2:33and fewer in winter.
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2:33 - 2:36So, when the sun is shining on the Earth, it warms up.
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2:36 - 2:38After the sun sets, it has time to cool down.
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2:38 - 2:39So, in the summer,
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2:39 - 2:42any location that's about 40 degrees north of the equator,
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2:42 - 2:44like Hartford, Connecticut,
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2:44 - 2:46will get 15 hours of daylight each day
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2:46 - 2:48and 9 hours of darkness.
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2:48 - 2:50It warms up for longer than it cools.
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2:50 - 2:52This happens day after day,
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2:52 - 2:54so there is an overall warming effect.
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2:54 - 2:56Remember this fact for later!
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2:56 - 2:58In the winter, the opposite happens.
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2:58 - 3:00There are many more hours of cooling time
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3:00 - 3:01than warming time,
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3:01 - 3:05and day after day, this results in a cooling effect.
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3:05 - 3:07The interesting thing is, as you move north,
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3:07 - 3:10the number of daylight hours in summer increases.
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3:10 - 3:13So, Juneau, Alaska would get about 19 hours of daylight
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3:13 - 3:18on the same summer day that Tallahassee, Florida gets about 14.
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3:18 - 3:20In fact, in the summertime at the North Pole,
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3:20 - 3:23the sun never sets.
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3:23 - 3:26OK, then, it's all about daylight hours, I've got it!
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3:26 - 3:29Well, no, there's another important piece to this puzzle.
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3:29 - 3:31If daylight hours were the only thing
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3:31 - 3:33that determined average temperature,
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3:33 - 3:35wouldn't the North Pole be the hottest place
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3:35 - 3:36on Earth in northern summer
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3:36 - 3:38because it receives 24 hours of daylight
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3:38 - 3:41in the months surrounding the summer solstice?
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3:41 - 3:42But it's the North Pole.
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3:42 - 3:43There's still icebergs in the water
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3:43 - 3:45and snow on the ground.
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3:45 - 3:46So, what's going on?
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3:46 - 3:47The Earth is a sphere
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3:47 - 3:50and so the amount of solar energy an area receives
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3:50 - 3:52changes based on how high the sun is in the sky,
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3:52 - 3:54which, as you know, changes during the day
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3:54 - 3:56between sunrise and sunset.
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3:56 - 3:59But, the maximum height also changes during the year,
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3:59 - 4:01with the greatest solar height during the summer months
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4:01 - 4:04and highest of all at noon on the summer solstice,
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4:04 - 4:06which is June 21st in the northern hemisphere
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4:06 - 4:09and December 21st in the southern hemisphere.
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4:09 - 4:11This is because as the Earth revolves,
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4:11 - 4:13the northern hemisphere ends up tilted away
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4:13 - 4:15from the sun in the winter
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4:15 - 4:16and toward the sun in summer,
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4:16 - 4:18which puts the sun more directly overhead
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4:18 - 4:20for longer amounts of time.
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4:20 - 4:23Remember those increased summer time daylight hours?
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4:23 - 4:26And solar energy per square kilometer increases
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4:26 - 4:28as the sun gets higher in the sky.
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4:28 - 4:30So, when the sun's at an angle,
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4:30 - 4:32the amount of energy delivered
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4:32 - 4:35to each square of the sunlit area is less.
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4:35 - 4:38Therefore, even though the North Pole is getting 24 hours
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4:38 - 4:39of daylight to warm up,
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4:39 - 4:42the sunlight it receives is very spread out
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4:42 - 4:45and delivers less energy than a place further south,
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4:45 - 4:47where the sun is higher in the sky
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4:47 - 4:49because it's more tilted toward the sun.
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4:49 - 4:51Besides, the North Pole has a lot to make up for.
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4:51 - 4:54It was cooling down without any sunlight at all
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4:54 - 4:55for 6 months straight.
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4:55 - 4:58So, as the seasons change, wherever you are,
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4:58 - 5:01you can now appreciate not just the beauty of each new season
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5:01 - 5:02but the astronomical complexity
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5:02 - 5:05that brings them to you.
- Title:
- Reasons for the seasons - Rebecca Kaplan
- Description:
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View full lesson: http://ed.ted.com/lessons/reasons-for-the-seasons-rebecca-kaplan
Why do some regions experience full-time heat while others are reckoning with frigid temperatures and snow? And why are the seasons reversed in the two hemispheres? Rebecca Kaplan explains how the shape of the Earth's orbit around the Sun and the Earth's tilt on its axis affect the amount of sunlight each region receives.
Lesson by Rebecca Kaplan, animation by Marc Christoforidis.
- Video Language:
- English
- Team:
- closed TED
- Project:
- TED-Ed
- Duration:
- 05:21
Jessica Ruby approved English subtitles for Reasons for the seasons - Rebecca Kaplan | ||
Jessica Ruby accepted English subtitles for Reasons for the seasons - Rebecca Kaplan | ||
Jessica Ruby edited English subtitles for Reasons for the seasons - Rebecca Kaplan | ||
Andrea McDonough edited English subtitles for Reasons for the seasons - Rebecca Kaplan | ||
Andrea McDonough added a translation |