原版英语RAZ 教案The Sun.pdf

上传人:qq****8 文档编号:96930406 上传时间:2024-04-06 格式:PDF 页数:13 大小:1.97MB
返回 下载 相关 举报
原版英语RAZ 教案The Sun.pdf_第1页
第1页 / 共13页
原版英语RAZ 教案The Sun.pdf_第2页
第2页 / 共13页
点击查看更多>>
资源描述

《原版英语RAZ 教案The Sun.pdf》由会员分享,可在线阅读,更多相关《原版英语RAZ 教案The Sun.pdf(13页珍藏版)》请在taowenge.com淘文阁网|工程机械CAD图纸|机械工程制图|CAD装配图下载|SolidWorks_CaTia_CAD_UG_PROE_设计图分享下载上搜索。

1、www.readinga-The SunA Reading AZ Level V Leveled BookWord Count:1,631The Sun Visit www.readinga- for thousands of books and materials.Written by Ned JensenLEVELED BOOK VWritten by Ned JensenThe Sun The SunLevel V Leveled Book Learning AZWritten by Ned JensenIllustrated by Craig FrederickAll rights r

2、eserved.www.readinga-Photo Credits:Front cover:courtesy of ESA/NASA/SOHO;back cover,pages 1,3,11(all),16,21:Jupiterimages Corporation;page 4:PaulPaladin/123RF;pages 5,17:ArtToday;page 6:courtesy of NASA Solarsystem Collection;page 9:iS Cheng;page 10:Corbis;page 12:REUTERS/Chip East;page 13:The SOHO-

3、EIT Consortium/ESA/NASA;pages 15,19:Learning A-Z;page 18:Hemis/Alamy;page 20:Elena Elisseeva/D;page 22:courtesy of NASA/JPL-Caltech/Harvard-Smithsonian CfAwww.readinga-CorrelationLEVEL VR4040Fountas&PinnellReading RecoveryDRA34Table of ContentsIntroduction.4 Just Another Star.6Where the Sun Gets Its

4、 Energy .7Action on the Surface .10From Sun to Earth.13The Sun and Us .16The Suns Death.22Conclusion .22Glossary .23Explore More .24Index .24IntroductionThe Sun is a huge ball of flaming gas at the center of our solar system.Its just one of billions of stars in the galaxy,but life on Earth couldnt s

5、urvive without it.The Sun controls Earths heat,light,and weather.Scientists know a lot about the Sun and how it affects Earths inhabitants.Scientists are always learning more and finding new ways to harness the power of the Sun.The Sun is a raging storm of activity.Solar eclipseThe Sun Level V56The

6、Suns far-reaching gravity prevents Earth and its seven sister planets from flying off their elliptical orbits into the vast universe.Earth makes one complete orbit around the Sun every 365 days,or once every year.If Earths orbit slowed down,it would become a doomed fireball and crash into the Sun.If

7、 Earths orbit speeded up,it would break free of the Suns gravity and become a block of ice floating through space.Without the Sun,Earth would be a dark,frozen wasteland void of life.Just Another StarThe Sun is just one of billions of stars in the Milky Way galaxy.The Milky Way is made up of a huge c

8、ollection of stars.Compared to billions of other stars,the Sun is small.Some astronomers call it the yellow runt.All stars,including the Sun,are classified by color,size,and brightness.The biggest stars are the hypergiants,which can be more than 1,500 times the size of Earths Sun.The smallest stars

9、are the very hot white dwarf stars.In between these giant and dwarf stars are the yellow stars,such as our Sun.They are the most common type of stars found in the Milky Way.Our Sun and solar system are just a tiny part of the Milky Way.Our solar systemPlanets in orbit around the SunMercuryEarthJupit

10、erUranusSunVenusMarsSaturnNeptuneDo You Know?The Sun is so enormous that 1.3 million Earths could fit inside it.The Sun Level V78CoreRadiation zonePhotosphereParts of the SunSolar FlareConvection zoneCoronaWhere the Sun Gets Its EnergyEarths Sun started producing energy shortly after it began formin

11、gestimated to be about 4.5 billion years ago.The Sun started as a gigantic cloud of gas and dust.It began collapsing into a huge ball under the force of gravity.As more and more dust and gas were packed into the giant ball,the pressure around the hydrogen gas at the center increased.This pressure pr

12、oduced extremely high temperatures that triggered a reaction at the center,or core,of the ball.The fuel in the Sun has kept this reaction going since it started.The energy-producing reaction in the core is called a thermonuclear reaction.A combustible gas called hydrogen makes up about 70 percent of

13、 Earths Sun.Most of the remaining gas is helium.Hydrogen gas is the fuel that produces the Suns energy.In a thermonuclear reaction,tiny hydrogen atoms combine to form larger helium atoms.This process is called fusion.When the hydrogen atoms fuse,they release bits of energy.As trillions upon trillion

14、s of hydrogen atoms fuse and release energy,the overall effect is the release of huge amounts of energy.Heliumabout30%Hydrogenabout70%metals made from hydrogen through fusion0.1%HeliumHydrogenextreme heatHydrogenFusion ProcessDo You Know?The Sun is so hot that its surface temperature can reach 6,000

15、C(11,000F).Compare that to the temperature of boiling water,which is 100C(212F),and you get an idea of just how hot the Sun is.Its 60 times hotter!The Sun Level V910The energy slowly makes its way from deep in the Suns core to its surface.It takes hundreds of thousands of years for particles of ener

16、gy to travel more than six million miles(9.7 million km)from the core to the surface.Along the way,the particles lose much of their energy,and the remaining energy that reaches the Suns surface is in the form of visible light energy,which is the light we see from Earth.Action on the Surface From Ear

17、th,the Sun may look like a gentle,glowing ball,but scientists know that the surface is actually raging with activity.Energy is constantly bubbling to the surface,much like a pot of boiling soup.While the Suns surface is always a storm of activity,there are times when it is more active than others.In

18、 fact,the Suns activity seems to occur in eleven-year cycles.Action seen on the Suns surface,or photosphere,and in the coronaSolar telescopes such as one on Kitt Peak in Arizona allow scientists to take a closer look at the Sun.The Sun Level V1112During active times,scientists observe dark spots mov

19、ing across the Suns surface.These areas,called sunspots,are cooler than the surrounding gases.They occur where magnetic energy bursts to the surface.Other solar activities take place during the high points in the Suns cycle.The most violent are solar flares,which are large loops of energy shooting h

20、igh above the Suns surface.Some of these flares reach heights of more than 100,000 miles.One of the largest solar flares recorded erupted in 1946 and arched 140,000 miles high.While solar flares are shooting from the surface,the Suns corona,or the halo of light around the Sun,becomes very active.Str

21、angely,even though the corona is far above the surface of the Sun,it is much hotter than the surface.The corona reaches temperatures over two million degrees Celsius(3.6 million F).When the corona is active,it ejects huge masses of radiation.This increased activity of the corona sends waves of high-

22、energy particles sweeping toward Earth.The radiation threatens to disable satellites orbiting Earth that control radio,television,and cell phone communication,as well as electrical power.In 1989,a massive solar explosion knocked out a power grid on Earth,leaving almost seven million people in the Un

23、ited States and Canada without electricity.Do You Know?Remember,the Sun is a giant ball and sends energy out in all directions.Only a tiny fraction of the Suns energy reaches Earth.Most of it goes off into space.EarthMassive blackouts can be caused by solar explosions.Solar flareSunThe Sun Level V13

24、14From Sun to EarthMost people think that heat from the Sun warms the Earth.But heat has to travel through matter to get from one place to another.So while the Suns energy travels through the vacuum of space,that energy doesnt heat space.Energy from the Sun travels to Earth as electromagnetic waves

25、called radiant energy,which only turn into heat when they are absorbed by matter.Examples of radiant energy include visible light,infrared light,and ultraviolet waves.About half of the radiant energy we get from the Sun is in the form of visible light.The rest is in the form of infrared and ultravio

26、let light,which humans cannot see.Radiant energy travels fast300,000 km per second(186,000 mi per second).At that speed,you could go around Earth about eight times in one second.Thats really flying!But even going that fast,it takes energy leaving the Sun eight minutes to make the trip to Earth.Earth

27、s atmosphere and clouds reflect much of the radiant energy from the Sun before it reaches the surface.When radiant energy gets through,the atmosphere absorbs some of it,heating the air.The energy also hits the surface of the Earth and is absorbed by the land,water,and other matter.When the radiant e

28、nergy is absorbed,it changes to heat as the visible light or infrared waves agitate the molecules in the matter struck by the waves.Do You Know?The Sun is 150 million kilometers(93 million miles)from Earth.That is the same distance as traveling around Earth at the equator more than 3,700 times.SunEa

29、rthAbout 51 percent of the radiant energy from the Sun is absorbed by Earths atmosphere and surface.SunEarths surfaceatmospherecloudcloudreflected by surface 4%reflected by atmosphere 6%reflected by clouds 20%absorbed by clouds and atmosphere 19%energy fromSun100%The Sun Level V1516The Sun and UsJus

30、t about all of the energy we use as humans can be linked to the Sun.The energy we get from food comes from plants that use sunlight to grow.So when you eat an apple or a plate of spinach,youre eating the Suns energy.The coal,gasoline,and oil we burn for energy comes from the Sun,too.All of these sou

31、rces of fuel are from plants that grew long,long ago by using energy from the Sun.Even the energy we get from the wind comes from the Sun.Uneven heating of the Earths surface by the Sun is what makes the air surrounding Earth move.In essence,the Sun moves sailboats and spins the blades of wind gener

32、ators.Windmills turn using wind created by the uneven heating of Earths surface.Which Cup Is Warmer?Earths surface heats unequally.Land absorbs the Suns radiant energy better than water.Dark surfaces absorb energy while light-colored surfaces reflect energy.Materials:flat black paint small paintbrus

33、h two 16 oz.tin cans(remove labels)water thermometerSteps:1 Paint the outside of one can with black paint.2 After allowing the paint to dry,fill the black can about halfway with water.3 Fill the unpainted can with an equal amount of water.4 Place both cans of water in the sunlight for two hours.5 Af

34、ter two hours,use a thermometer to tell which cup of water is the warmest.Try ThisThe Sun Level V1718Scientists have found ways to capture the Suns energy and use it to heat homes and make electricity.Solar cells absorb energy from the Sun and change it into electricity.Solar cells are used on calcu

35、lators.They are also placed on large panels attached to satellites in space.Cities and homes use solar energy for heat in colder months.Solar collectors are used to produce heat.They are made of black pipes filled with water.The black pipes absorb radiant energy from the Sun.The radiant energy chang

36、es to heat and warms the water in the pipes.The water then flows through pipes into a building.Heat radiates out from the water in the pipes and heats the air in the building.Solar furnaces are used to produce very hot temperatures.They are made of curved mirrors that focus energy from the Sun onto

37、a very small area.The concentrated energy is changed to heat and can reach temperatures of thousands of degrees.The very hot temperatures are used to make new materials and to destroy harmful waste products.Scientists are even planning a solar furnace that will float in space and send focused solar

38、energy back to Earth.Do You Know?In Germany there is a solar energy power plant that can make enough electricity to power almost 2,000 homes.An area bigger than 37 football fields is covered with 33,500 large solar panels.This power plant uses only solar energy,and it does not pollute the air or wat

39、er.Solar cells collect energy from the Sun.1000 kw solar furnace in Odeillo,FranceThe Sun Level V1920Passive solar homes have special features to collect energy from the Sun.These homes have large windows that face the south in the parts of the world north of the equator.They face north in areas sou

40、th of the equator.During the colder winter months when the Sun is lower in the sky,sunlight passes through the windows and changes to heat when it is absorbed by walls inside the house.This house takes advantage of solar energy with windows facing south.Solar Cooker Make your own solar cooker at hom

41、e!Materials:black construction paperscissorswhite foam cup2 rubber bandsshoeboxsealable plastic baggie23 slices of applealuminum foilnewspaper/styrofoamSteps:1 Cut a strip of black construction paper to fit the inside of the foam cup.2 Place the apple slices inside the baggie and seal it.3 Cut a hol

42、e in the lid of the shoebox that is big enough to fit the cup through.4 Place the cup in the box and surround it with shredded pieces of newspaper or pieces of styrofoam.Use the rubber bands to secure the shoebox lid.5 Use the foil to make a funnel around the cup as shown in the picture.Keep the foi

43、l smooth,making sure the shiny side faces inward.6 Line the foam cup with the construction paper and place the baggie with apples inside.7 Aim the foil funnel toward the sun and wait 12 hours.Remove the cup and eat your baked apple.Question:What caused your solar cooker to get hot?Try ThisThe Sun Le

44、vel V2122As important as the Sun is to our survival,it also poses dangers to humans.We are learning more and more about how solar energy damages our skin.A skin cancer,called melanoma,is caused by overexposure to the Suns harmful ultraviolet rays.Years of exposure and severe sunburns can damage skin

45、 cells.It is important to wear sunscreen and clothing that covers your skin when you are out in the Sun,especially for long periods of time.The Suns DeathEach day fusion changes more and more of the Suns hydrogen fuel into helium.Scientists estimate that the Sun has about five billion years of fuel

46、left before it will begin to cool down and eventually die.Do You Know?Never look directly into the Sun.The Suns powerful rays can burn the cornea,the sensitive area of your eyes that makes it possible for you to see.Damage to the cornea can cause blindness.Even sunglasses cant completely protect you

47、r eyes from the Sun.Ring Nebula what Earths Sun could look like when it diesConclusionWe depend on the Sun for our survival.It is the source of most of the energy we use every day.Scientists are working hard to better understand the Sun and its energy.Satellites orbiting Earth collect data from the

48、Sun.Better solar telescopes being developed on Earth are aimed at the Sun to collect data.As we understand the Sun better and find new ways to use its energy,we will grow even more dependent on the power of the Sun.The Sun Level V2324Glossaryfusion blending of atoms that results in the release of en

49、ergy(p.8)matter a substance that takes up space and has weight(p.13)orbit a path taken by a body,such as the Earth,around another body,such as the Sun(p.5)radiant energy energy traveling in electromagnetic waves,such as infrared,visible light,or radio waves(p.13)radiation process of giving off energ

50、y in the form of rays,such as light or heat(p.12)solar cells structures made from silicon or plastic that absorb light energy from the Sun and turn it into electricity(p.17)solar flares sudden energy bursts that appear as large bright loops on the Suns surface(p.11)sunspots cooler,dark spots on the

展开阅读全文
相关资源
相关搜索

当前位置:首页 > 教育专区 > 高考资料

本站为文档C TO C交易模式,本站只提供存储空间、用户上传的文档直接被用户下载,本站只是中间服务平台,本站所有文档下载所得的收益归上传人(含作者)所有。本站仅对用户上传内容的表现方式做保护处理,对上载内容本身不做任何修改或编辑。若文档所含内容侵犯了您的版权或隐私,请立即通知淘文阁网,我们立即给予删除!客服QQ:136780468 微信:18945177775 电话:18904686070

工信部备案号:黑ICP备15003705号© 2020-2023 www.taowenge.com 淘文阁