the outer planets p. 575

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The Outer Planets p. 575

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The Outer Planets p. 575. The Inner Planets to Scale. 3,031 mi 7,521 mi 7,926 mi 4,222 mi. 5.4 g/cm3 5.2 g/cm3 5.5 g/cm3 3.9 g/cm^3. The Outer Planets to Scale. 88,700 mi 75,000 mi 31,700 mi 30,200 mi. - PowerPoint PPT Presentation

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Page 1: The Outer Planets p. 575

The Outer Planetsp. 575

Page 2: The Outer Planets p. 575

The Inner Planets to Scale

3,031 mi 7,521 mi 7,926 mi 4,222 mi

5.4 g/cm3 5.2 g/cm3 5.5 g/cm3 3.9 g/cm^3

Page 3: The Outer Planets p. 575

The Outer Planets to Scale

88,700 mi 75,000 mi 31,700 mi 30,200 mi

1.3 g/cm3 0.7 g/cm3 1.3 g/cm3 1.6 g/cm3

Page 4: The Outer Planets p. 575

Outer Planet Similarities• All are tens of thousands of miles across

– Much larger than the inner planets

• All are made of gas - hydrogen and helium– No rocky surface like the inner planets– Call GAS GIANTS– All have many moons and is surrounded by

rings

• All are not very dense (b/c made of gas)• Why do the outer planets share these

similarities?• Why don’t the outer planets have more in

common with the inner planets?

Page 5: The Outer Planets p. 575

Jupiter• Largest planet and most

massive planet• Its mass is 2 ½ times all the

planets combined.• Colorful cloud bands• Thick atmosphere of

hydrogen and helium• Rapid rotation (9h50m)• -250°F at cloud tops• Pressure at core is approx.

30 million X greater than earth’s pressure.

• Has 63+ moons (Io, Europa, Ganymede, and Callisto

Page 6: The Outer Planets p. 575

Great Red Spot

• Hurricane-like storm, fueled by heat inside of Jupiter

• Large enough to cover 3 Earths

• Discovered by Galileo nearly 400 years ago– Why can it last so long

compared with hurricanes on the Earth? No land to weaken it.

Page 7: The Outer Planets p. 575

Saturn

• Least dense planet - Would float on water!

• 2nd largest planet• Atmosphere is

hydrogen and helium• Bulges because of

rapid rotation (10h30m)

• Large, broad rings

Page 8: The Outer Planets p. 575

Saturn’s Rings• Made of countless small

chunks of ice and rock each travelling its own orbit around Saturn.– Why don’t the chunks

combine to form a moon?– Why doesn’t Earth have

rings?

• 170,000 miles wide, <1 mile thick

• Largest moon-Titan is larger than Mercury

• Has 60+ moons

Page 9: The Outer Planets p. 575

Uranus• Discovered by accident

(1781)• Blue-green color from

methane in its atmosphere• 4X diameter of earth• Could hold 1300 Earths• Thick atmosphere of

hydrogen and helium.• -350°F at cloud tops• Twice as far from sun as

Saturn.• Almost featureless; little

weather– Why might Uranus lack

distinctive weather patterns?

Page 10: The Outer Planets p. 575

Uranus’ Axis• Axis tilted 98° from its orbit (rotates top to

bottom)• Orbits Sun every 84y• How would these factors affect its seasons?• At least 27 moons

Page 11: The Outer Planets p. 575

What’s Wrong with Uranus?

• Following its discovery, astronomers calculated its orbit

• Uranus mysteriously speeded up, then slowed down– Why might Uranus

have deviated from its calculated orbit?

Page 12: The Outer Planets p. 575

Neptune• Discovered at its

predicted position (1846)

• At least 13 moons• Blue color from methane• -370°F at cloud tops• Great Dark Spot in

1989, but not 1994– How is this different from

the Great Red Spot?– Why is its weather

different from Uranus? Jupiter?

Page 13: The Outer Planets p. 575

The S.S. Family Portait

Page 14: The Outer Planets p. 575

• http://www.youtube.com/watch?v=HEheh1BH34Q

• www.brainpop.com – jupiter, saturn, uranus, neptune, outer solar system

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