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Try This!  How did our solar system form? Solar System Formation  Early universe – hot cloud of mostly hydrogen and helium  Gases clump to form nebula.

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Presentation on theme: "Try This!  How did our solar system form? Solar System Formation  Early universe – hot cloud of mostly hydrogen and helium  Gases clump to form nebula."— Presentation transcript:

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2 Try This!  How did our solar system form?

3 Solar System Formation  Early universe – hot cloud of mostly hydrogen and helium  Gases clump to form nebula and gravity begins to concentrate mass  Stars are created through nuclear fusion - huge amounts of light and heat!

4 Solar System Origin (4.56 b.y.a.) ROTATING NEBULA THEORY Gravitational contraction and rotation of interstellar gas Planetary disk with central bulge Gravity causes sun to form Fusion and proto-sun Planets form from debris left

5 Evidence for Rotating Nebula Theory 1.The solar system is all the same age approx. 2.The planets all rotate in the same direction and on the same plane http://www.youtube.com/watch?v=xt9Bvc8s_d0 Hubble video 9 minutes

6 We Can Also Look and see solar systems forming elsewhere…. Close-up of “Protoplanets" in Orion

7 What’s in our solar system?

8 TERRESTRIAL PLANETS Density (mass/volume) = 4.0 - 5.5 g/cm 3 Earth is 149 597 871 km from the sun = 1 AU (astronomical unit) The Inner Planets: solid/rocky

9 The Asteroid Belt  Not all solar material formed planets!  Asteroids orbit between Mars and Jupiter  Source of majority of meteorites that fall to Earth  Most get pulled into Jupiter due to its large gravity

10 Stony meteorites  95 % of falls  They are called meteorites if the hit the Earth’s surface  Most burn up in the atmosphere and are called meteors or “shooting stars”

11 Meteoroid, Meteor, Meteorite… http://upload.wikimedia.org/wikipedia/commons/6/6 3/Meteoroid_meteor_meteorite.gif http://www.youtube.com/watch?v=4S6KatI7M3A

12 Captured a greater amount of the lighter materials of the initial solar cloud Density = 0.6 – 1.7 g/cm 3 The Gas Giant Planets

13 Kuiper Belt  Disk of debris at the edge of our Solar System  Pluto is a KB Object (sorry!)  Source of some comets

14 Pluto? considered a dwarf planet – not a true planet  Pluto ranges from 30 – 40 AU’s from the SUN (30 to 40 times farther from the SUN than Earth is!)  It has 3 moons  Frozen and rocky

15 Comets… frozen snowballs Dust tail – white, “smoke,” reflects sun. 600,000 to 6 million miles long tail – Solar UV breaks down CO gas, making them glow blue for of millions of miles

16  The planets don’t ever all line up like this, but it shows their order and relative size  Earth is 1/1,000,000 the volume of the Sun

17 Try This! Planetary Preview – Complete the table Name of PlanetWhat I knowWhat I wonderWhat I learned

18 Jigsaw “The Universe and Its Stars” A. The origin of the universe B. Measuring distances in space C. The Birth of Stars, including our Sun D. Stars: Old Age, Death and New Life E. Galaxies and our Home: The Milky Way F. Dark Energy and the Expansion of the Universe


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