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Astronomy project#1
The Sun
 The center of our solar system.
 Is medium-hot and yellow.
 Is made up of the two gasses; hydrogen
  and helium.
Layers:
 Chromosphere
 Photosphere
 Convective zone
 Core
 Radiative zone
The Sun
Mercury
 Very hot atmosphere.
 Has no moons.
 Is the first of the inner four planets.
 Is unable to trap heat.
 Closest planet to the sun.
 Rotates the sun in only 88 days.
 36 million miles from the sun.
Mercury
Venus
 Has a very thick atmosphere.
 Has no moons.
 Is about the same size as Earth.
 Is the 2nd of the inner four planets.
 Is the hottest planet.
 Venus is slightly smaller than the Earth
  in diameter – 6%.
 Venus is 67 million miles away from the
  sun.
Venus
Earth
 Is about 4.5 billion years old.
 Astrological name, Terra.
 93 million miles from the sun.
 Has tectonic plates, which allow the
  cruse to recycle itself.
 Orbits the sun once ever 365.25 days.
 Seasons are caused by the tilt.
 Its tilt is about 66°.
Earth
Mars
 Named after the Greek God of War.
 One day is a little over 24 hours.
 Dust storms can cover much of the
  planet for months at a time.
 One year = 687 days.
 Has two moons; Phobos and Diemos.
 Has polar ice caps.
 Has about the same surface area of the
  Earth.
Mars
Jupiter
 5th planet from the sun.
 Largest planet in the solar system.
 Orbits the sun once every 12 years.
 Consists primarily of
  hydrogen, nitrogen, helium, and water.
 Held together by a massive gravity field.
 Rings consist of dust and meteoroids.
 Rings are about 140, 000 km long.
Jupiter
Saturn
   886 million miles from the sun.
   Has a rocky core, primarily consists of
    liquid metallic hydrogen.
   A gas giant, parts of the planet rotate at
    different speeds.
   One rotation at the equator, a “day” takes
    10 hours and 14 minutes. At the poles it
    takes 25 minutes longer.
   Has a massive magnetic field.
   Is visible in the night sky with the naked
    eye.
Saturn
Uranus
   Has 13 rings with 2 being very far from the
    planet.
   The Voyager is the only probe to visit.
   Has a massive axis tilt of roughly 90°.
   Takes 84 years to make one rotation
    around the sun.
   Known to have 27 moons.
   Located between Saturn and Neptune and
    is approximately 1.8 billion miles from the
    sun.
Uranus
Neptune
   Cannot be viewed with the naked eye in
    the sky.
   Orbits the sun once every 165 years.
   Has been visited once by the Voyager 2
    probe in 1989.
   Neptune is the Roman God of the Sea.
   One day is equivalent to 16 hours on Earth.
   Is about 4 times the size of Earth.
   Has an atmosphere of
    hydrogen, helium, methane, and ammonia.
Neptune
Our Moon
   Contains soil materials similar to the crust
    of the Earth.
   2,168 miles in diameter.
   238,000 miles from the Earth on average.
   Rotates clockwise.
   Orbits the Earth once ever 29.5 days.
   Moving away from the Earth 38 millimeters
    a year.
   Has no atmosphere, so the surface does
    not change because of winds and erosion.
Our Moon
Eclipses
 Types of eclipses: solar and lunar
 Solar eclipse: Occurs when the moon
  passes between the Earth and Sun
  therefore blocking the sun. This can only
  occur during the day.
 Lunar eclipse: When Earth is between
  the Moon and Sun causing blockage of
  the moon. This can only occur if it is a
  full moon, at night, AND the sun is in line
  with the Earth and Moon.
Eclipses




    Lunar Eclipse   Solar Eclipse
Gravitational Forces
Rules for Law of Universal Gravitation:
1) The Gravitational Force increases as
   the mass of the object increases.
2) The Gravitational Force decreases as
   distance between the objects increase.
* Gravitational Force is changed by mass.
Gravitational Forces
What Happened To Pluto?
   In 2006, the definition of a planet was
    changed. 3 things decide whether it’s a
    planet or not a planet:
1) It orbits the sun. (yes)
2) It is large enough that its own gravity
     prevents other objects from sharing its
     orbit with the sun. (no)
3) It is large enough that its gravity makes it
     into a spherical shape. (yes)
 * It is not a planet because it is not large
     enough that its own gravity prevents other
     objects from sharing its orbit with the sun.*
What Happened To Pluto?
Tools and Technology
   Telescopes:
      - Used on earth or space
      - 2 types: refracting and reflecting

   Satellites:
      - Used in space
      - Controlled by gravity
      - Example: Sputnik I
      - Communication satellites, scientific satellites
Tools and Technology




  Sputnik satellite   Hubble Space Telescope
Space Objects
   Comets:
     - Icy, glowing, and flying objects
     - Measures from meters to kilometers wide

   Meteoroids:
     - Smaller than asteroids and comets

   Meteors:
     - Passes through the atmosphere

   Meteorites:
     - Passes atmosphere and hits surface
Space Objects



 Comet McNaught    meteoroid




                  Diablo- Canyon
    meteor           meteorite
Fun Facts
 If you put Saturn in water it would float
 We are moving through space at the
  rate of 530 km a second
 The moon is drifting away from earth
 The light hitting the earth right now is
  30,000 years old
 The sun loses up to a billion kilograms a
  second due to solar winds
Thanks for
watching!!!

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Astronomy project#1

  • 2. The Sun  The center of our solar system.  Is medium-hot and yellow.  Is made up of the two gasses; hydrogen and helium. Layers:  Chromosphere  Photosphere  Convective zone  Core  Radiative zone
  • 4. Mercury  Very hot atmosphere.  Has no moons.  Is the first of the inner four planets.  Is unable to trap heat.  Closest planet to the sun.  Rotates the sun in only 88 days.  36 million miles from the sun.
  • 6. Venus  Has a very thick atmosphere.  Has no moons.  Is about the same size as Earth.  Is the 2nd of the inner four planets.  Is the hottest planet.  Venus is slightly smaller than the Earth in diameter – 6%.  Venus is 67 million miles away from the sun.
  • 8. Earth  Is about 4.5 billion years old.  Astrological name, Terra.  93 million miles from the sun.  Has tectonic plates, which allow the cruse to recycle itself.  Orbits the sun once ever 365.25 days.  Seasons are caused by the tilt.  Its tilt is about 66°.
  • 10. Mars  Named after the Greek God of War.  One day is a little over 24 hours.  Dust storms can cover much of the planet for months at a time.  One year = 687 days.  Has two moons; Phobos and Diemos.  Has polar ice caps.  Has about the same surface area of the Earth.
  • 11. Mars
  • 12. Jupiter  5th planet from the sun.  Largest planet in the solar system.  Orbits the sun once every 12 years.  Consists primarily of hydrogen, nitrogen, helium, and water.  Held together by a massive gravity field.  Rings consist of dust and meteoroids.  Rings are about 140, 000 km long.
  • 14. Saturn  886 million miles from the sun.  Has a rocky core, primarily consists of liquid metallic hydrogen.  A gas giant, parts of the planet rotate at different speeds.  One rotation at the equator, a “day” takes 10 hours and 14 minutes. At the poles it takes 25 minutes longer.  Has a massive magnetic field.  Is visible in the night sky with the naked eye.
  • 16. Uranus  Has 13 rings with 2 being very far from the planet.  The Voyager is the only probe to visit.  Has a massive axis tilt of roughly 90°.  Takes 84 years to make one rotation around the sun.  Known to have 27 moons.  Located between Saturn and Neptune and is approximately 1.8 billion miles from the sun.
  • 18. Neptune  Cannot be viewed with the naked eye in the sky.  Orbits the sun once every 165 years.  Has been visited once by the Voyager 2 probe in 1989.  Neptune is the Roman God of the Sea.  One day is equivalent to 16 hours on Earth.  Is about 4 times the size of Earth.  Has an atmosphere of hydrogen, helium, methane, and ammonia.
  • 20. Our Moon  Contains soil materials similar to the crust of the Earth.  2,168 miles in diameter.  238,000 miles from the Earth on average.  Rotates clockwise.  Orbits the Earth once ever 29.5 days.  Moving away from the Earth 38 millimeters a year.  Has no atmosphere, so the surface does not change because of winds and erosion.
  • 22. Eclipses  Types of eclipses: solar and lunar  Solar eclipse: Occurs when the moon passes between the Earth and Sun therefore blocking the sun. This can only occur during the day.  Lunar eclipse: When Earth is between the Moon and Sun causing blockage of the moon. This can only occur if it is a full moon, at night, AND the sun is in line with the Earth and Moon.
  • 23. Eclipses Lunar Eclipse Solar Eclipse
  • 24. Gravitational Forces Rules for Law of Universal Gravitation: 1) The Gravitational Force increases as the mass of the object increases. 2) The Gravitational Force decreases as distance between the objects increase. * Gravitational Force is changed by mass.
  • 26. What Happened To Pluto?  In 2006, the definition of a planet was changed. 3 things decide whether it’s a planet or not a planet: 1) It orbits the sun. (yes) 2) It is large enough that its own gravity prevents other objects from sharing its orbit with the sun. (no) 3) It is large enough that its gravity makes it into a spherical shape. (yes) * It is not a planet because it is not large enough that its own gravity prevents other objects from sharing its orbit with the sun.*
  • 28. Tools and Technology  Telescopes: - Used on earth or space - 2 types: refracting and reflecting  Satellites: - Used in space - Controlled by gravity - Example: Sputnik I - Communication satellites, scientific satellites
  • 29. Tools and Technology Sputnik satellite Hubble Space Telescope
  • 30. Space Objects  Comets: - Icy, glowing, and flying objects - Measures from meters to kilometers wide  Meteoroids: - Smaller than asteroids and comets  Meteors: - Passes through the atmosphere  Meteorites: - Passes atmosphere and hits surface
  • 31. Space Objects Comet McNaught meteoroid Diablo- Canyon meteor meteorite
  • 32. Fun Facts  If you put Saturn in water it would float  We are moving through space at the rate of 530 km a second  The moon is drifting away from earth  The light hitting the earth right now is 30,000 years old  The sun loses up to a billion kilograms a second due to solar winds