原版英语RAZ 教案(S) Our Solar System_DS.pdf
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1、Our Solar SystemA Reading AZ Level S Leveled BookWord Count:1,766Visit www.readinga- for thousands of books and materials.www.readinga-Written by Bruce D.CooperLEVELED BOOK SOur Solar System Written by Bruce D.Cooperwww.readinga-Our Solar System 28NotesOur Solar SystemLevel S Leveled Book Learning A
2、ZWritten by Bruce D.CooperDigital image manipulationby Randy GatesAll rights reserved.www.readinga-CorrelationLEVEL SO3434Fountas&PinnellReading RecoveryDRAPhoto Credits:Front cover,title page,pages 4,7,10:courtesy of NASA/JPL;back cover:courtesy of SDO/AIA;page 3:courtesy of NASA/ESA/The Hubble Her
3、itage Team(STScI/AURA);page 5:courtesy of Solar&Heliospheric Observatory/Extreme Ultraviolet Imaging Telescope/NASA/Goddard Space Flight Center;page 6:courtesy of SOHO(ESA&NASA)/EIT Consortium;page 8:courtesy of NASA/Johns Hopkins University Applied Physics Laboratory/Arizona State University/Carneg
4、ie Institution of Washington.Image reproduced courtesy of Science/AAAS;pages 9,13:courtesy of NASA/JPL/USGS;page 11:courtesy of NASA/GSFC/GOES/NOAA;pages 12,17,21:courtesy of NASA;page 14:courtesy of NASA and The Hubble Heritage Team(STScI/AURA);page 15:courtesy of NASA/JPL-Caltech/University of Ari
5、zona;page 16:courtesy of NASA,ESA,and E.Karkoschka(University of Arizona);page 18:courtesy of NASA/JPL/Space Science Institute;page 19:courtesy of NASA,ESA,and the Hubble Heritage Team(STScI/AURA);page 20:courtesy of Erich Karkoschka(University of Arizona)and NASA;page 22:courtesy of NASA,ESA,and M.
6、Buie(Southwest Research Institute);page 23:courtesy of ESA-AOES Medialab;page 24:WIYN/NOAO/AURA/NSF/epa/Corbis;page 25(center):courtesy of ESA/LFI&HFI Consortia;page 25(right):courtesy of ESA D.Ducros27NotesOur Solar System Level S3Table of ContentsIntroduction .4The Sun.6Mercury.8Venus .9Earth.11Th
7、e Moon .13Mars .14Jupiter .16Saturn .18Uranus.20Neptune .21Pluto and Other Dwarf Planets .22Asteroids.23Comets .24Conclusion .25Glossary .2626Glossaryatmosphere(n.)a layer of gases surrounding a planet,star,or moon(p.12)diameter(n.)the length of a straight line through the center of an object(p.23)f
8、ossil fuels(n.)sources of energy such as coal,oil,and natural gas that were made by the decomposition of plants and animals over millions of years(p.6)gravitational pull(n.)the force of attraction that tends to draw objects together(p.13)meteor(n.)a meteoroid that enters Earths atmosphere(p.23)meteo
9、rite(n.)a meteoroid that actually lands on Earth(p.23)meteoroid(n.)a comet,asteroid,or dust particle floating in space (p.23)orbit(n.)the path of an object revolving around another object(p.8)orbits(v.)to revolve around another object(p.4)4IntroductionOur Solar System is made up of the Sun,eight off
10、icial planets,several dwarf planets,and hundreds of planetary satellites,or moons.It also contains comets,asteroids,and clouds of gas.The Sun is the center of the Solar System.Everything else in the Solar System goes around,or orbits,the Sun.Mercury,Venus,Earth,and Mars are the inner,rocky planets.T
11、hey are made of hard materials.The outer planets are Jupiter,Saturn,Uranus,and Neptune.They are known as the gas giants and are made mostly of gases.The outer planets are hundreds of times larger than Earth.SunJupiterSaturnNeptuneUranusPlutoEarthMoonVenusMarsMercuryOur Solar System Level S25Conclusi
12、onHumans have always wondered,“whats happening out there in space?”For centuries,we could only guess.New rockets,space probes,satellites,and telescopes show us whats happening in our Solar System every day.These tools have helped scientists to discover new planets,re-count moons,and see stars being
13、born and being swallowed.They have also given us the first full-sky survey map of our universe and a direct view at the Sun.What will they show us next about our Solar System and beyond?In July 2010,after a year-long mapping mission,the orbiting Planck Telescope of the European Space Agency(ESA)deli
14、vered its first full-sky survey of our universe.Plancks mission is to measure radiation left over from the ancient beginnings of our universe so that scientists can study how it was formed.As Planck sweeps the sky,it also measures the temperatures,density of matter,speed,and movement of galaxies.24C
15、ometsComets are composed of ice and dust and are like large dirty snowballs in space.They have very oval-shaped orbits.For part of that orbit,they come close to the Sun,and then they swing far out into space.Some comets orbit the Sun in less than 200 years.The most famous of these is Halleys Comet.I
16、t returns every seventy-six years.Other comets take thousands of years to complete an orbit.Comet Hyakutake,which passed close to the Earth in 1996,will return in about 9,000 years.The comet NEAT,photographed by the WIYN telescope at Kitt Peak National Observatory in Arizona,was discovered in 2001 b
17、y the Near Earth Asteroid Tracking system.Our Solar System Level S5To get an idea of the size of things in our Solar System,imagine that Earth is a grape.If the Earth were the size of a grape,the Moon would be the size of a green pea.The Sun would be as big as a ball that an adult man could stand in
18、.Jupiter,the largest planet,would be the size of a grapefruit,while Saturn,the second largest planet,would be the size of an orange.Uranus and Neptune would be the size of lemons.Approximate size of Earth for comparisonThe diameter of Earth is approximately 13,000 kilometers(8,100 miles).The Suns di
19、ameter is approximately 1.4 million kilometers(870,000 miles).How many times larger is the Suns diameter than the Earths?6The SunThe Sun is a huge ball of burning gas that sends energy far out into the Solar System.The Sun plays a very important part in our daily lives,providing energy that supports
20、 all life on Earth.The Sun causes seasons,climate,ocean currents,air circulation,and weather.Without the Suns energy,plants could not grow and make food.Also,there would be no gas,oil,or coal,which are Earths fossil fuels.Fossil fuels are formed over millions of years from dead plant and animal life
21、.The temperature of the Suns surface is approximately 6,000 degrees Celsius(10,832 degrees Fahrenheit).The Suns core is approximately 15,000,000 degrees Celsius(27,000,032 degrees Fahrenheit).Our Solar System Level S23AsteroidsAsteroids are rocky,metallic objects orbiting the Sun.They range in size
22、from a few feet in diameter to hundreds of miles in diameter.Most asteroids are found between Mars and Jupiter.Some have orbits that cross the Earths path,and in the past,some have even crashed into Earth.Asteroids and other smaller objects that enter Earths atmosphere are called meteoroids.If they
23、survive the trip and land on the ground,they are called meteorites.If they burn up before landing,they are called meteors.Among the best evidence of an asteroid hitting Earth is the Barringer Crater near Winslow,Arizona.Satellites monitor impact tests during research into ways to prevent asteroids f
24、rom colliding with Earth.Our Solar System Level S7The Sun is just one of billions of stars.It has been around for about 4.6 billion years.It will keep producing energy for another 5 billion years.Before it dies,it will swell up and swallow many of the inner planets.Then it will shrink into a much sm
25、aller ball.Relative sizes of the objects in our Solar SystemSunJupiterSaturnUranusNeptunePlutoMercuryEarthVenusMars22What Would You Weigh?Gravity is different on each planet,and gravity determines how much you weigh.If you weigh 70 lbs.on Earth,then you would weigh:On Mercury 27 lbs.On Venus 63 lbs.
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