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Chapter 5 Our Solar System Survey of Astronomy a s t r o 1 0 1 0 - l e e . c o m [email protected]
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Chapter 5

Feb 22, 2016

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Chapter 5. Survey of Astronomy. a stro1010-lee.com. Our Solar System. [email protected]. Chapter 5. Our Solar System. Survey of Astronomy. Astro1010-lee.com. [email protected]. Chapter 5. Our Solar System. An Inventory of the Solar System. - PowerPoint PPT Presentation
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Page 1: Chapter 5

Chapter 5

Our Solar System

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Page 2: Chapter 5

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Chapter 5Our Solar System

Page 3: Chapter 5

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Chapter 5Our Solar System

An Inventory of the Solar SystemEarly astronomers knew: Sun, Moon, Stars, Mercury, Venus, Mars, Jupiter, Saturn, comets, and meteors

Now we know: Solar system has one star, eight planets (added Uranus, and Neptune), 135+ moons, asteroids, comets, and meteoroids.

Pluto was added as a Planet then reduced to a Dwarf Planet

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Chapter 5Our Solar System

Page 5: Chapter 5

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Chapter 5Our Solar System

Planetary PropertiesOrbital period can be observed

Distance from Sun known by Kepler’s laws

Radius known from angular size

Masses from Kepler’s 3rd Law as modified by Newton’

Rotation period from observations

Density can be calculated knowing radius and mass

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Chapter 5Our Solar System

Comparison of the Terrestrial Family of Planets to the Jovian Family of Planets

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Chapter 5Our Solar System

Differences between the terrestrial planets

Atmospheres and surface conditions are very dissimilar

Only Earth has oxygen in atmosphere and liquid water on surface

Earth and Mars rotate at about the same rate; Venus and Mercury are much slower, and Venus rotates in the opposite direction

Earth and Mars have moons; Mercury and Venus don’t

Earth, Mars and Mercury have magnetic fields; Venus does not.

Page 8: Chapter 5

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Chapter 5Our Solar System

Interplanetary Debris

Asteroids and meteoroids are rocky; asteroids are bigger

Asteroid Eros is 34 km long:

Comets are icy, with some rocky parts.

Comet Hale–Bopp

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Chapter 17A

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Cloud of gas and dust contracts due to gravity. Conservation of Angular Momentum means it spins faster and faster as it contracts

Page 10: Chapter 5

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Chapter 5Our Solar System

Condensation theory:

Interstellar dust grains help cool the

cloud, and act as condensation nuclei

to produce flakes

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Chapter 5Our Solar System

Local temperature in the condensing cloud determines where various materials condense

Page 12: Chapter 5

Early Spacecraft Exploration of the Solar System

Soviet Venera probes landed on Venus from 1970–1978

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Page 13: Chapter 5

Early Spacecraft Exploration

Pioneer and Voyager flew through the outer solar system. This is Voyager

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Chapter 5Our Solar System

End Chapter 5