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To ASTRONOMY….. and beyond!
What we will be discovering:

 Structures of the solar system
 The Sun-Earth-Moon System
 The Planets and their Moons
 Asteroids, Comets, and Meteoroids
 Stars and Galaxies
Axis and Period of Rotation
Axis of Rotation               Period of Rotation

 an imaginary line that        The time it takes for one
  runs through the center        rotation around the axis
  of the planet. (The planet     to occur. (one day)
  rotates around this line.)
Period of Revolution and Ellipse
Period of Revolution           Ellipse

 The time it takes a planet    Oval shaped. (example:
  to move completely             Earth’s orbit around the
  around the sun. (one year)     sun is an oval or ellipse.)
                                ALL planets have
                                 elliptical orbits around
                                 the sun (Kepler’s first
                                 law)
AU’s and LY’s
Astronomical Unit          Light Year

 The average distance      The distance that light
  from Earth to the Sun.     travels in a vacuum in one
 1 AU = 149,600,000km       Julian year. (365.25 days)
                            Typically used to measure
                             distances on a galactic
                             scale.
                            1 ly = apx 10 trillion km
Now, because I know you’re interested…

              Revolution and Rotation
                   periods of the planets:
              Planet    P of rotation   P of revolution
              Mercury   59 days         88 days
              Venus     243 days        255 days
              Earth     24 hours        365 days
              Mars      24 hours        687 days
              Jupiter   10 hours        11.9 years
              Saturn    11 hours        29.5 years
              Uranus    17 hours        84 years
              Neptune   16 hours        165 years
The reason for the seasons!
 The yearly cycle of the seasons is caused
  by the tilt of Earth’s axis as it revolves
  around the sun.
 Depending on which hemisphere is tilted
  towards the sun, they will be experiencing
  summer and the one tilted away will be
  experiencing winter.
 The equator always experiences warm
  weather because it’s always tilted toward
  the sun!
Earth + Revolution = Seasons
The Equinoxes

 The earth experiences 2 equinoxes- one
  in March and one in September.
 An equinox is when neither end of the
  Earth’s axis is tilted toward the sun,
  therefore, both hemispheres are receiving
  an equal amount of sunlight and energy!
 Day and night are equal in length during
  the actual equinox (March 21 and
  September 22)
The Solstices

 The solstices are the times of year when
  the direct sunlight is farthest north or
  south of the equator.
 The summer solstice occurs for us on
  June 21 (this is the winter solstice for the
  southern hemisphere)
 The winter solstice occurs for us on
  December 21 (this is the summer solstice
  for the southern hemisphere)

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Notes revolution rotation

  • 2. What we will be discovering:  Structures of the solar system  The Sun-Earth-Moon System  The Planets and their Moons  Asteroids, Comets, and Meteoroids  Stars and Galaxies
  • 3. Axis and Period of Rotation Axis of Rotation Period of Rotation  an imaginary line that  The time it takes for one runs through the center rotation around the axis of the planet. (The planet to occur. (one day) rotates around this line.)
  • 4. Period of Revolution and Ellipse Period of Revolution Ellipse  The time it takes a planet  Oval shaped. (example: to move completely Earth’s orbit around the around the sun. (one year) sun is an oval or ellipse.)  ALL planets have elliptical orbits around the sun (Kepler’s first law)
  • 5. AU’s and LY’s Astronomical Unit Light Year  The average distance  The distance that light from Earth to the Sun. travels in a vacuum in one  1 AU = 149,600,000km Julian year. (365.25 days)  Typically used to measure distances on a galactic scale.  1 ly = apx 10 trillion km
  • 6. Now, because I know you’re interested… Revolution and Rotation periods of the planets: Planet P of rotation P of revolution Mercury 59 days 88 days Venus 243 days 255 days Earth 24 hours 365 days Mars 24 hours 687 days Jupiter 10 hours 11.9 years Saturn 11 hours 29.5 years Uranus 17 hours 84 years Neptune 16 hours 165 years
  • 7. The reason for the seasons!  The yearly cycle of the seasons is caused by the tilt of Earth’s axis as it revolves around the sun.  Depending on which hemisphere is tilted towards the sun, they will be experiencing summer and the one tilted away will be experiencing winter.  The equator always experiences warm weather because it’s always tilted toward the sun!
  • 8. Earth + Revolution = Seasons
  • 9. The Equinoxes  The earth experiences 2 equinoxes- one in March and one in September.  An equinox is when neither end of the Earth’s axis is tilted toward the sun, therefore, both hemispheres are receiving an equal amount of sunlight and energy!  Day and night are equal in length during the actual equinox (March 21 and September 22)
  • 10. The Solstices  The solstices are the times of year when the direct sunlight is farthest north or south of the equator.  The summer solstice occurs for us on June 21 (this is the winter solstice for the southern hemisphere)  The winter solstice occurs for us on December 21 (this is the summer solstice for the southern hemisphere)

Editor's Notes

  1. Period of revolution, ellipse, astronomical unit
  2. astronomical unit (potentially do lab on page 464)