our solar system

11
Our Solar System http://www.youtube.com/watch?v=pUZ 2tfr1bsU

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Page 1: Our Solar System

Our Solar System

http://www.youtube.com/watch?v=pUZ2tfr1bsU

Page 2: Our Solar System

Essential Question

• Why is the solar system arranged the way it is?• Why are the planets, asteroids, Kuiper ice

objects.

Page 3: Our Solar System

Nebula)

Page 4: Our Solar System

Demo:

1. Obtain a water bottle with a cap. Fill it 2/3rds full of water.

2. Pour several pebbles and large gravel pieces into the bottle.3. Obtain a ¼ of a piece of Alka-Seltzer. Quickly place it in the bottle and

put the cap on tight.4. Gently shake the bottle for several seconds then place it upright on the table.

Page 5: Our Solar System

Nebular Hypothesis of the Origin of the Solar System

Page 6: Our Solar System

Step 1. About 5 billion years agoNebulae of gas (hydrogen and helium) and dust a light year across.Due to a nearby supernova explosion (?) it begins to contract As it contracts, it spins faster.Flattens into a disk shape

Page 7: Our Solar System

Step 2:The center contracts and heats up forming a proto-star. The Sun (99% of the mass) formed at the centerSorting: Heavier material (rock an metal) gravitate toward the center.Lighter gas and dust get blown farther out

Page 8: Our Solar System

Step 3:

Repeated collisions caused the smaller pieces of solid material to collide and condense (combine) to form larger, rocky inner planets and asteroid belt .

Page 9: Our Solar System

Step 4:Within a few million years these bodies cooled, cleared their neighborhood and formed into the icy gassy outer planets, etc.

Page 10: Our Solar System

Exit Slip

1. How are the planets in the solar system sorted?

2. Which planets are more dense?

define density:

Page 11: Our Solar System

Earth’s Early History• Bombardment by high velocity meteorites

and comets• generated immense amounts of heat energy

and melted the metals and rock on the young planet.

• The denser materials like iron (Fe) sank into the core of the Earth. • lighter silicates (Si), oxygen (O)

compounds, rise near the surface. • decay of radioactive elements in the Earth, generate heat