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The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these.

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Presentation on theme: "The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these."— Presentation transcript:

1 The Sun & The Solar System

2 Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these layers except the core has a unique name as a part of the sun

3 Structure of the Sun (continued) Core = Center of the Sun, comparable to the inner core on Earth Radiative Zone = Layer surrounding the core, similar to the Earth’s outer core Convective Zone = Similar to the Earth’s mantle

4 Structure of the Sun (continued) Photosphere = The surface of the sun. Equivalent to the Earth’s crust. The photosphere is what we see from Earth. Chromosphere = The Sun’s atmosphere. The uppermost part is known as the corona

5 Sunspots Sunspots are cool, dark areas of gasses in the photosphere caused by magnetic fields Sunspot cycles are variations in the number of sunspots which occur on average every 11 years

6 Formation of the Solar System The Solar Nebular Theory The Big Bang describes the origin of the universe After the Big Bang, clouds of gas and dust formed solar nebulas This is the same way all new stars are formed Gravity caused the gas and dust to begin to condense, collide, and heat up When the temperature gets hot enough, fusion begins; the sun was born ~5 billion years ago

7 Kepler’s Laws of the Solar System Johannes Kepler (1571-1630) developed the mathematical calculations which explain planetary motion 1 st Law = Planets circle the sun in elliptical orbits 2 nd Law = Planets travel at different speeds at different points in their orbit 3 rd Law = Describes the relationship between a planet’s distance from the sun and the amount of time it takes to complete a revolution around the sun

8 The Inner Planets (The terrestrial planets) Mercury: One Year = 88 days One Day = 59 Earth days Venus: One Year = 225 days One Day = 243 Earth days Venus rotates on its axis opposite all the other planets. This is known as retrograde rotation.

9 The Inner Planets (continued) Earth: The only planet with liquid water Extremely active geology (plate tectonics) Mars: One Year = 687 days One Day = One Earth day The largest volcano in the solar system is on Mars. The name of the volcano is Olympus Mons

10 The Outer Planets (the gas giants) Jupiter: The largest planet, mass is twice all the other planets combined One Year = 12 Earth years One Day = 9 hours and 50 minutes, rotates fastest Moons include Io, Europa, Ganymede, & Callisto; collectively known as the Galilean moons Saturn: Complex ring system, has the most moons One Year = 29.5 Earth years; One Day = 10.66 hours

11 The Outer Planets (continued) Uranus: One Year = 84 Earth years; One Day = 17 hours Green color caused by methane in the atmosphere Neptune: One Year = 165 Earth years; One Day = 16 hours Bluish-green color with white “clouds” of frozen methane Pluto: No longer considered a planet; One Year = 250 Earth years; One Day = 6 Earth days; Discovered by accident in 1930

12 Other Celestial Bodies Asteroids = Fragments of rock which orbit the sun Asteroids are made of the same materials the planets are composed of Most asteroids exist in a belt between Mars and Jupiter Comet = A body of rock, dust, methane, ammonia, and ice which orbits the sun in long ellipses Comets have a head and a tail Comets lose mass as they orbit the sun, ice melts when the comet is near the sun

13 Other Celestial Bodies (continued) Meteoroids = small bits of rock and metal which move randomly through the solar system Comets leave behind the smallest meteoroids Asteroids which collide can break up into larger meteoroids Meteor = a meteoroid which enters the Earth’s atmosphere5 Meteorite = any part of a meteor which remains after it hits the Earth’s surface


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