SlideShare uma empresa Scribd logo
1 de 103
Chapter 20 – Planetary Motion What would happen if the Earth’s orbit changed?
[object Object],[object Object],[object Object],[object Object],[object Object]
 
[object Object],[object Object]
Constellations
2. “ Wanderers ” moved about the stars – other  planets  in their orbits
C. Early 1500’s – Nicolaus  Copernicus  –  Earth and other planets orbit the sun ( heliocentric model ) in the same  direction and each planet takes a  different amount of time to orbit the sun.
 
 
[object Object],[object Object]
 
2. Developed  three  laws to help understand planetary orbits around the sun: ,[object Object],b. Each planet moves so that an imaginary line drawn from the sun to the planet sweeps out equal areas in equal periods of time.
 
c. The ratio of the  period of   rotation squared   “ T” of any two planets revolving about the sun is equal to the ratio of the cubes of their  mean distance “R” from the sun.
E. Late 1700’s – Issac  Newton  – Developed Law of Inertia (an object’s motion will not change unless the object is acted upon by an outside force). Also, orbits are a result of a planet’s tendency to move in a straight line ( direction ), and the  gravity  of the sun and other celestial bodies (ex: moon).
 
 
 
[object Object],[object Object],[object Object],[object Object],[object Object]
 
B. Period of  Rotation  – movement of planet  around its axis  = 1 day (day and night cycle); Ex. earth=24 hours; Mercury=59 earth days; Pluto=6 earth days.
 
[object Object],[object Object],[object Object]
[object Object],[object Object],[object Object]
 
b. The side of the planet tilted  away  from the sun, is receiving  less direct  sunlight and shorter days (winter). c. During the period of revolution where the earth is not tilted   towards or away from sun are autumn and spring.
 
d. Any planet that is tilted on its axis will have  seasons . e. These changes of the seasons are marked by specific dates: i.  Summer  solstice (June 20/21) – the sun appears at its highest point in the sky.  Longest  day of the year ii.  Winter  solstice (December 21/22) – the N. Hemisphere is at full tilt away from sun.  Shortest  day of the year.
iii.  Autumnal equinox  – (day and night equal) September 22/23 iv.  Vernal equinox  – (day and night equal) March 20/21
 
2.  Retrograde rotation  occurs when planets rotate from east to west; normal rotation direction is west to east. Ex.  Venus .
 
Review Questions ,[object Object],The earth is tilted toward the sun.
2. Why is it necessary that we have an  extra day every four years? (hint: think about the period of revolution for the earth) Because is takes 365.26 days for the earth to orbit the sun.
3. Describe how living conditions on earth might change if the earth’s axis were straight up and down instead of tilted. There would not be a change of seasons.
4. What two factors dictate the elliptical orbit pattern of all the planets? What would happen to the orbit of the planets if the sun were to shrink? Inertia and gravity The force of gravity would be less therefore the orbit would increase.
[object Object],[object Object],[object Object],[object Object],[object Object]
 
C. Slowly changes over time and  completely  reverses  the field after a period of time. D. Importance of the magnetic field: a. Is important for  navigation  around  the planet. b. Shields earth from  cosmic radiation
 
E. Field creates the  magnetosphere  – area of space that is affected by the magnetic field. Begins 1000km in earth’s atmosphere and extends 64,000km into space on side facing sun and millions of kilometers into space on side of earth facing away from the sun (due to  solar wind , blowing the sphere out into space)
 
 
F.  Van Allen  Radiation Belts  1. The inner part of the magnetosphere where charged particles of  solar winds  are trapped.
 
[object Object],[object Object]
 
3. When these particles interact with the upper atmosphere layer it creates  aurora   (giving off light). Ex.  northern lights
 
 
 
IV. The  Moon , our most important satellite A.  ¼  the size of earth,  1/6  less  gravit y.
 
B. 384,403km away from earth. This was determined when astronauts placed a small  mirror  on the moon and a laser was bounced off the mirror from earth. The time to travel to the moon was timed and used to determine the distance, based on the  speed of light .
 
C. Moon and earth are composed of the mostly the  same material , which suggests they formed around the same time.
D. Temperature range of the moon is  100  degrees Celsius during the day and  –175  degrees Celsius at night.
 
 
E. Topography of the moon consists of  craters  (made by meter strikes),  highlands  (extinct volcanoes),  rills  (cracks, either from lava flow or cracks  created from moonquakes)
F. Rotation around axis is around  27   days  and revolution around earth is around  27 days . The  same side  of the moon is ALWAYS facing earth because its rate of  rotation  is equal to its  revolution .
[object Object],[object Object]
 
 
 
 
G. The Moon appears to move west across the sky (because of the rotation of the earth) but actually moves  eastward   (retrograde rotation).  You can observe the moon relative to stars and you will observe the eastward motion of the earth.
V. Outcome of movements of earth, moon and sun A.  Phases  of the moon - The phases are the result of what  sunlight  is reflected by the moon.
 
 
 
[object Object],[object Object],[object Object]
 
 
2. When the moon is  new , the  moon  is  between the earth and the sun, no light is  reflected.
 
 
 
3. A  waxing  moon is the phase where  more  of the moon is gradually seen over two weeks.
 
4. A  waning moon  is the phase where  less of the moon gradually disappears over two weeks.
 
B.  Eclipses  – As the moon and earth revolve together around the sun, sometimes one of the celestial objects  block the suns rays . There are two types.
[object Object],[object Object]
Solar Eclipse
 
Solar Eclipse Paths
 
2.  Lunar Eclipse  – When the earth is between the  sun and the full moon , causing the earth’s shadow to fall on the moon (looks dark and coppery color, due to the bending of light waves). Label the bodies below: sun, moon, earth
 
 
a. If you are in the  inner shadow  of an eclipse it is called the  umbra
b. If you are in the  outer   shadow  of an eclipse it is called the  penumbra.
3. Tides – Caused by the  gravitational  pull between the  earth  and the  moon . a. Moon pulls on earth through the orbit, causing the rise and fall of the oceans.
b. Tides go between high and low every  6 hours . There is a 50 minutes delay each day due to the moon  rising  50 minutes later each day.
c. The sides of the earth in a direct  line with the moon experience high tides , while the sides of the earth at 90 degrees with the moon experience  low tides
 
d. Full moon and new moons result in higher tides ( spring tides ) because the moon and sun are in  direct line  with the earth,  increasing   the gravitational pull . First quarter and last quarter of the moon phases are the high tides that are  lower  than usual (neap tides) because the moon and sun are at 90o with the earth, there is  less gravitational pull
 
Review Questions ,[object Object],[object Object]
Position of sun, earth and moon at full moon.
2. Why does the lunar eclipse occur either two weeks before or after the total solar eclipse?
What did you Learn? Copy and answer the questions ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]

Mais conteúdo relacionado

Mais procurados

Ch 1 -keplers laws of motion
Ch 1 -keplers laws of motionCh 1 -keplers laws of motion
Ch 1 -keplers laws of motioncphsastronomy
 
Kepler's laws of planetary motion
Kepler's laws of planetary motionKepler's laws of planetary motion
Kepler's laws of planetary motionKumar
 
Keplar's laws of planetary motion Class 11 physics
 Keplar's laws of planetary motion Class 11 physics Keplar's laws of planetary motion Class 11 physics
Keplar's laws of planetary motion Class 11 physicsDevangSPSingh
 
Physics Powerpoint Presentation- Keplers laws of planetary motion
Physics Powerpoint Presentation- Keplers laws of planetary motionPhysics Powerpoint Presentation- Keplers laws of planetary motion
Physics Powerpoint Presentation- Keplers laws of planetary motionKendriya Vidyalaya
 
Keplers Laws
Keplers LawsKeplers Laws
Keplers Lawseliseb
 
9.4 - Orbital Motion & Kepler's third law
9.4 - Orbital Motion & Kepler's third law9.4 - Orbital Motion & Kepler's third law
9.4 - Orbital Motion & Kepler's third lawsimonandisa
 
Johannes kepler nomination
Johannes kepler nominationJohannes kepler nomination
Johannes kepler nominationdom vin
 
Ch 1 -the powers of ten
Ch 1 -the powers of tenCh 1 -the powers of ten
Ch 1 -the powers of tencphsastronomy
 
Keplers laws of planetry motion
Keplers laws of planetry motionKeplers laws of planetry motion
Keplers laws of planetry motionAlokKumar1221
 
Keplers law for planetary motion.ppt
Keplers law for planetary motion.pptKeplers law for planetary motion.ppt
Keplers law for planetary motion.pptDEPARTMENT OF PHYSICS
 
Early model of the Universe
Early model of the UniverseEarly model of the Universe
Early model of the UniverseJerome Bigael
 
Chapter 22outline
Chapter 22outlineChapter 22outline
Chapter 22outlinejmchenry071
 

Mais procurados (20)

Ch 1 -keplers laws of motion
Ch 1 -keplers laws of motionCh 1 -keplers laws of motion
Ch 1 -keplers laws of motion
 
Kepler's laws of planetary motion
Kepler's laws of planetary motionKepler's laws of planetary motion
Kepler's laws of planetary motion
 
Kepler laws Notes
Kepler laws NotesKepler laws Notes
Kepler laws Notes
 
Keplar's laws of planetary motion Class 11 physics
 Keplar's laws of planetary motion Class 11 physics Keplar's laws of planetary motion Class 11 physics
Keplar's laws of planetary motion Class 11 physics
 
Keplers law
Keplers lawKeplers law
Keplers law
 
Physics Powerpoint Presentation- Keplers laws of planetary motion
Physics Powerpoint Presentation- Keplers laws of planetary motionPhysics Powerpoint Presentation- Keplers laws of planetary motion
Physics Powerpoint Presentation- Keplers laws of planetary motion
 
Johannes kepler
Johannes keplerJohannes kepler
Johannes kepler
 
Keplers Laws
Keplers LawsKeplers Laws
Keplers Laws
 
9.4 - Orbital Motion & Kepler's third law
9.4 - Orbital Motion & Kepler's third law9.4 - Orbital Motion & Kepler's third law
9.4 - Orbital Motion & Kepler's third law
 
Keplers laws
Keplers lawsKeplers laws
Keplers laws
 
Johannes kepler
Johannes keplerJohannes kepler
Johannes kepler
 
Johannes kepler nomination
Johannes kepler nominationJohannes kepler nomination
Johannes kepler nomination
 
Johannes Kepler
Johannes KeplerJohannes Kepler
Johannes Kepler
 
Ch 1 -the powers of ten
Ch 1 -the powers of tenCh 1 -the powers of ten
Ch 1 -the powers of ten
 
Keplers laws of planetry motion
Keplers laws of planetry motionKeplers laws of planetry motion
Keplers laws of planetry motion
 
Planetarymotion
PlanetarymotionPlanetarymotion
Planetarymotion
 
Keplers law for planetary motion.ppt
Keplers law for planetary motion.pptKeplers law for planetary motion.ppt
Keplers law for planetary motion.ppt
 
keepar law Deepak singh rajput
keepar law Deepak singh rajputkeepar law Deepak singh rajput
keepar law Deepak singh rajput
 
Early model of the Universe
Early model of the UniverseEarly model of the Universe
Early model of the Universe
 
Chapter 22outline
Chapter 22outlineChapter 22outline
Chapter 22outline
 

Destaque

Chapter 14 – water resources
Chapter 14 – water resourcesChapter 14 – water resources
Chapter 14 – water resourcesAnnie cox
 
Heating of the earth - 2
Heating of the earth - 2Heating of the earth - 2
Heating of the earth - 2Annie cox
 
Chapter 22 – astronomical technology
Chapter 22 – astronomical technologyChapter 22 – astronomical technology
Chapter 22 – astronomical technologyAnnie cox
 
Chapter 16 – the atmosphere and weather
Chapter 16 – the atmosphere and weatherChapter 16 – the atmosphere and weather
Chapter 16 – the atmosphere and weatherAnnie cox
 
Atmosphere lesson
Atmosphere lessonAtmosphere lesson
Atmosphere lessonAnnie cox
 
Air pressure
Air pressureAir pressure
Air pressureAnnie cox
 
Heating of the earth
Heating of the earthHeating of the earth
Heating of the earthAnnie cox
 
Air pressure
Air pressureAir pressure
Air pressureAnnie cox
 
Chapter 14 – water resources
Chapter 14 – water resourcesChapter 14 – water resources
Chapter 14 – water resourcesAnnie cox
 
Chapter 6 maps
Chapter 6  mapsChapter 6  maps
Chapter 6 mapsAnnie cox
 
Chapter 19 – formation of the universe
Chapter 19 – formation of the universeChapter 19 – formation of the universe
Chapter 19 – formation of the universeAnnie cox
 
Chapter 17 – meteorology
Chapter 17 – meteorologyChapter 17 – meteorology
Chapter 17 – meteorologyAnnie cox
 
Chapter 21 stars
Chapter 21   starsChapter 21   stars
Chapter 21 starsAnnie cox
 
Planetary motionmodule15
Planetary motionmodule15Planetary motionmodule15
Planetary motionmodule15Kella Boatner
 
Brahe and kepler
Brahe and keplerBrahe and kepler
Brahe and keplerjoverba
 
Presentation Siebesma - (Extreme Precipitation, Present and Future
Presentation Siebesma - (Extreme Precipitation, Present and FuturePresentation Siebesma - (Extreme Precipitation, Present and Future
Presentation Siebesma - (Extreme Precipitation, Present and FutureTU Delft Climate Institute
 
Population Data Workbench - Meteorology Data Query
Population Data Workbench - Meteorology Data QueryPopulation Data Workbench - Meteorology Data Query
Population Data Workbench - Meteorology Data QueryYoosook Lee
 
Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...
Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...
Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...University of the Highlands and Islands
 

Destaque (20)

Chapter 14 – water resources
Chapter 14 – water resourcesChapter 14 – water resources
Chapter 14 – water resources
 
Heating of the earth - 2
Heating of the earth - 2Heating of the earth - 2
Heating of the earth - 2
 
Chapter 22 – astronomical technology
Chapter 22 – astronomical technologyChapter 22 – astronomical technology
Chapter 22 – astronomical technology
 
Chapter 16 – the atmosphere and weather
Chapter 16 – the atmosphere and weatherChapter 16 – the atmosphere and weather
Chapter 16 – the atmosphere and weather
 
Atmosphere lesson
Atmosphere lessonAtmosphere lesson
Atmosphere lesson
 
Air pressure
Air pressureAir pressure
Air pressure
 
Heating of the earth
Heating of the earthHeating of the earth
Heating of the earth
 
Air pressure
Air pressureAir pressure
Air pressure
 
Chapter 14 – water resources
Chapter 14 – water resourcesChapter 14 – water resources
Chapter 14 – water resources
 
Chapter 6 maps
Chapter 6  mapsChapter 6  maps
Chapter 6 maps
 
Chapter 19 – formation of the universe
Chapter 19 – formation of the universeChapter 19 – formation of the universe
Chapter 19 – formation of the universe
 
Chapter 17 – meteorology
Chapter 17 – meteorologyChapter 17 – meteorology
Chapter 17 – meteorology
 
Chapter 21 stars
Chapter 21   starsChapter 21   stars
Chapter 21 stars
 
Planetary motionmodule15
Planetary motionmodule15Planetary motionmodule15
Planetary motionmodule15
 
2(1) environmental archaeology
2(1) environmental archaeology2(1) environmental archaeology
2(1) environmental archaeology
 
Brahe and kepler
Brahe and keplerBrahe and kepler
Brahe and kepler
 
UNIT 3 POPULATION ECOLOGY (1)
UNIT 3 POPULATION ECOLOGY (1)UNIT 3 POPULATION ECOLOGY (1)
UNIT 3 POPULATION ECOLOGY (1)
 
Presentation Siebesma - (Extreme Precipitation, Present and Future
Presentation Siebesma - (Extreme Precipitation, Present and FuturePresentation Siebesma - (Extreme Precipitation, Present and Future
Presentation Siebesma - (Extreme Precipitation, Present and Future
 
Population Data Workbench - Meteorology Data Query
Population Data Workbench - Meteorology Data QueryPopulation Data Workbench - Meteorology Data Query
Population Data Workbench - Meteorology Data Query
 
Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...
Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...
Hydroclimatology of Sariz Creek Watershed, Located In Seyhan Basin, And Simul...
 

Semelhante a Chapter 20 planetary motion

Semelhante a Chapter 20 planetary motion (20)

Astronomy - Notes
Astronomy - NotesAstronomy - Notes
Astronomy - Notes
 
Earth moon sun notes
Earth moon sun notesEarth moon sun notes
Earth moon sun notes
 
Astronomy nc 2014
Astronomy nc 2014Astronomy nc 2014
Astronomy nc 2014
 
Ch 23
Ch 23Ch 23
Ch 23
 
Astronomy- Motion, eclipses, tides, moon
Astronomy- Motion, eclipses, tides, moonAstronomy- Motion, eclipses, tides, moon
Astronomy- Motion, eclipses, tides, moon
 
12.1 earth, moon, sun
12.1 earth, moon, sun12.1 earth, moon, sun
12.1 earth, moon, sun
 
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
 
Chap 14 solar system
Chap 14  solar systemChap 14  solar system
Chap 14 solar system
 
The Cycles of the Moon
The Cycles of the MoonThe Cycles of the Moon
The Cycles of the Moon
 
Unit1.Planet Earth
Unit1.Planet EarthUnit1.Planet Earth
Unit1.Planet Earth
 
Chapter 1
Chapter 1Chapter 1
Chapter 1
 
Earth and Space
Earth and SpaceEarth and Space
Earth and Space
 
Astronomy by jatin
Astronomy by jatinAstronomy by jatin
Astronomy by jatin
 
Astronomy by jatin
Astronomy by jatinAstronomy by jatin
Astronomy by jatin
 
Astronomy by jatin
Astronomy by jatinAstronomy by jatin
Astronomy by jatin
 
Astronomy by jatin
Astronomy by jatinAstronomy by jatin
Astronomy by jatin
 
Astronomy by jatin
Astronomy by jatinAstronomy by jatin
Astronomy by jatin
 
Ch15 the solar system
Ch15 the solar systemCh15 the solar system
Ch15 the solar system
 
Earth's Motions
Earth's MotionsEarth's Motions
Earth's Motions
 
Solar system
Solar systemSolar system
Solar system
 

Mais de Annie cox

Unit 2 post assessment
Unit 2 post assessmentUnit 2 post assessment
Unit 2 post assessmentAnnie cox
 
Chapter 2 current issues
Chapter 2  current issuesChapter 2  current issues
Chapter 2 current issuesAnnie cox
 
Chapter 18 – air pollution and global changes
Chapter 18 – air pollution and global changesChapter 18 – air pollution and global changes
Chapter 18 – air pollution and global changesAnnie cox
 
Chapter 15 – water quality and pollution
Chapter 15 – water quality and pollutionChapter 15 – water quality and pollution
Chapter 15 – water quality and pollutionAnnie cox
 
Chapter 13 – oceans and beaches
Chapter 13 – oceans and beachesChapter 13 – oceans and beaches
Chapter 13 – oceans and beachesAnnie cox
 
Double sidedeqnws
Double sidedeqnwsDouble sidedeqnws
Double sidedeqnwsAnnie cox
 
Double sidedeqnws
Double sidedeqnwsDouble sidedeqnws
Double sidedeqnwsAnnie cox
 
Chapter 17 – meteorology
Chapter 17 – meteorologyChapter 17 – meteorology
Chapter 17 – meteorologyAnnie cox
 
Moduel 5 topic 3
Moduel 5 topic 3Moduel 5 topic 3
Moduel 5 topic 3Annie cox
 
Moduel 5 topic 3
Moduel 5 topic 3Moduel 5 topic 3
Moduel 5 topic 3Annie cox
 
Module 5 topic 2 2nd
Module 5 topic 2   2ndModule 5 topic 2   2nd
Module 5 topic 2 2ndAnnie cox
 
Module 5 topic 2
Module 5 topic 2Module 5 topic 2
Module 5 topic 2Annie cox
 
Module 5 topic 1 2nd
Module 5 topic 1   2ndModule 5 topic 1   2nd
Module 5 topic 1 2ndAnnie cox
 
Module 5 topic 1
Module 5 topic 1Module 5 topic 1
Module 5 topic 1Annie cox
 
Module 4 topic 1 2nd
Module 4 topic 1   2ndModule 4 topic 1   2nd
Module 4 topic 1 2ndAnnie cox
 

Mais de Annie cox (17)

Unit 2 post assessment
Unit 2 post assessmentUnit 2 post assessment
Unit 2 post assessment
 
Chapter 2 current issues
Chapter 2  current issuesChapter 2  current issues
Chapter 2 current issues
 
Chapter 18 – air pollution and global changes
Chapter 18 – air pollution and global changesChapter 18 – air pollution and global changes
Chapter 18 – air pollution and global changes
 
Chapter 15 – water quality and pollution
Chapter 15 – water quality and pollutionChapter 15 – water quality and pollution
Chapter 15 – water quality and pollution
 
Chapter 13 – oceans and beaches
Chapter 13 – oceans and beachesChapter 13 – oceans and beaches
Chapter 13 – oceans and beaches
 
Doubleside
DoublesideDoubleside
Doubleside
 
Double sidedeqnws
Double sidedeqnwsDouble sidedeqnws
Double sidedeqnws
 
Double sidedeqnws
Double sidedeqnwsDouble sidedeqnws
Double sidedeqnws
 
Doubleside
DoublesideDoubleside
Doubleside
 
Chapter 17 – meteorology
Chapter 17 – meteorologyChapter 17 – meteorology
Chapter 17 – meteorology
 
Moduel 5 topic 3
Moduel 5 topic 3Moduel 5 topic 3
Moduel 5 topic 3
 
Moduel 5 topic 3
Moduel 5 topic 3Moduel 5 topic 3
Moduel 5 topic 3
 
Module 5 topic 2 2nd
Module 5 topic 2   2ndModule 5 topic 2   2nd
Module 5 topic 2 2nd
 
Module 5 topic 2
Module 5 topic 2Module 5 topic 2
Module 5 topic 2
 
Module 5 topic 1 2nd
Module 5 topic 1   2ndModule 5 topic 1   2nd
Module 5 topic 1 2nd
 
Module 5 topic 1
Module 5 topic 1Module 5 topic 1
Module 5 topic 1
 
Module 4 topic 1 2nd
Module 4 topic 1   2ndModule 4 topic 1   2nd
Module 4 topic 1 2nd
 

Chapter 20 planetary motion

  • 1. Chapter 20 – Planetary Motion What would happen if the Earth’s orbit changed?
  • 2.
  • 3.  
  • 4.
  • 6. 2. “ Wanderers ” moved about the stars – other planets in their orbits
  • 7. C. Early 1500’s – Nicolaus Copernicus – Earth and other planets orbit the sun ( heliocentric model ) in the same direction and each planet takes a different amount of time to orbit the sun.
  • 8.  
  • 9.  
  • 10.
  • 11.  
  • 12.
  • 13.  
  • 14. c. The ratio of the period of rotation squared “ T” of any two planets revolving about the sun is equal to the ratio of the cubes of their mean distance “R” from the sun.
  • 15. E. Late 1700’s – Issac Newton – Developed Law of Inertia (an object’s motion will not change unless the object is acted upon by an outside force). Also, orbits are a result of a planet’s tendency to move in a straight line ( direction ), and the gravity of the sun and other celestial bodies (ex: moon).
  • 16.  
  • 17.  
  • 18.  
  • 19.
  • 20.  
  • 21. B. Period of Rotation – movement of planet around its axis = 1 day (day and night cycle); Ex. earth=24 hours; Mercury=59 earth days; Pluto=6 earth days.
  • 22.  
  • 23.
  • 24.
  • 25.  
  • 26. b. The side of the planet tilted away from the sun, is receiving less direct sunlight and shorter days (winter). c. During the period of revolution where the earth is not tilted towards or away from sun are autumn and spring.
  • 27.  
  • 28. d. Any planet that is tilted on its axis will have seasons . e. These changes of the seasons are marked by specific dates: i. Summer solstice (June 20/21) – the sun appears at its highest point in the sky. Longest day of the year ii. Winter solstice (December 21/22) – the N. Hemisphere is at full tilt away from sun. Shortest day of the year.
  • 29. iii. Autumnal equinox – (day and night equal) September 22/23 iv. Vernal equinox – (day and night equal) March 20/21
  • 30.  
  • 31. 2. Retrograde rotation occurs when planets rotate from east to west; normal rotation direction is west to east. Ex. Venus .
  • 32.  
  • 33.
  • 34. 2. Why is it necessary that we have an extra day every four years? (hint: think about the period of revolution for the earth) Because is takes 365.26 days for the earth to orbit the sun.
  • 35. 3. Describe how living conditions on earth might change if the earth’s axis were straight up and down instead of tilted. There would not be a change of seasons.
  • 36. 4. What two factors dictate the elliptical orbit pattern of all the planets? What would happen to the orbit of the planets if the sun were to shrink? Inertia and gravity The force of gravity would be less therefore the orbit would increase.
  • 37.
  • 38.  
  • 39. C. Slowly changes over time and completely reverses the field after a period of time. D. Importance of the magnetic field: a. Is important for navigation around the planet. b. Shields earth from cosmic radiation
  • 40.  
  • 41. E. Field creates the magnetosphere – area of space that is affected by the magnetic field. Begins 1000km in earth’s atmosphere and extends 64,000km into space on side facing sun and millions of kilometers into space on side of earth facing away from the sun (due to solar wind , blowing the sphere out into space)
  • 42.  
  • 43.  
  • 44. F. Van Allen Radiation Belts 1. The inner part of the magnetosphere where charged particles of solar winds are trapped.
  • 45.  
  • 46.
  • 47.  
  • 48. 3. When these particles interact with the upper atmosphere layer it creates aurora (giving off light). Ex. northern lights
  • 49.  
  • 50.  
  • 51.  
  • 52. IV. The Moon , our most important satellite A. ¼ the size of earth, 1/6 less gravit y.
  • 53.  
  • 54. B. 384,403km away from earth. This was determined when astronauts placed a small mirror on the moon and a laser was bounced off the mirror from earth. The time to travel to the moon was timed and used to determine the distance, based on the speed of light .
  • 55.  
  • 56. C. Moon and earth are composed of the mostly the same material , which suggests they formed around the same time.
  • 57. D. Temperature range of the moon is 100 degrees Celsius during the day and –175 degrees Celsius at night.
  • 58.  
  • 59.  
  • 60. E. Topography of the moon consists of craters (made by meter strikes), highlands (extinct volcanoes), rills (cracks, either from lava flow or cracks created from moonquakes)
  • 61. F. Rotation around axis is around 27 days and revolution around earth is around 27 days . The same side of the moon is ALWAYS facing earth because its rate of rotation is equal to its revolution .
  • 62.
  • 63.  
  • 64.  
  • 65.  
  • 66.  
  • 67. G. The Moon appears to move west across the sky (because of the rotation of the earth) but actually moves eastward (retrograde rotation). You can observe the moon relative to stars and you will observe the eastward motion of the earth.
  • 68. V. Outcome of movements of earth, moon and sun A. Phases of the moon - The phases are the result of what sunlight is reflected by the moon.
  • 69.  
  • 70.  
  • 71.  
  • 72.
  • 73.  
  • 74.  
  • 75. 2. When the moon is new , the moon is between the earth and the sun, no light is reflected.
  • 76.  
  • 77.  
  • 78.  
  • 79. 3. A waxing moon is the phase where more of the moon is gradually seen over two weeks.
  • 80.  
  • 81. 4. A waning moon is the phase where less of the moon gradually disappears over two weeks.
  • 82.  
  • 83. B. Eclipses – As the moon and earth revolve together around the sun, sometimes one of the celestial objects block the suns rays . There are two types.
  • 84.
  • 86.  
  • 88.  
  • 89. 2. Lunar Eclipse – When the earth is between the sun and the full moon , causing the earth’s shadow to fall on the moon (looks dark and coppery color, due to the bending of light waves). Label the bodies below: sun, moon, earth
  • 90.  
  • 91.  
  • 92. a. If you are in the inner shadow of an eclipse it is called the umbra
  • 93. b. If you are in the outer shadow of an eclipse it is called the penumbra.
  • 94. 3. Tides – Caused by the gravitational pull between the earth and the moon . a. Moon pulls on earth through the orbit, causing the rise and fall of the oceans.
  • 95. b. Tides go between high and low every 6 hours . There is a 50 minutes delay each day due to the moon rising 50 minutes later each day.
  • 96. c. The sides of the earth in a direct line with the moon experience high tides , while the sides of the earth at 90 degrees with the moon experience low tides
  • 97.  
  • 98. d. Full moon and new moons result in higher tides ( spring tides ) because the moon and sun are in direct line with the earth, increasing the gravitational pull . First quarter and last quarter of the moon phases are the high tides that are lower than usual (neap tides) because the moon and sun are at 90o with the earth, there is less gravitational pull
  • 99.  
  • 100.
  • 101. Position of sun, earth and moon at full moon.
  • 102. 2. Why does the lunar eclipse occur either two weeks before or after the total solar eclipse?
  • 103.