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Chapter 7 Our Planetary System What Does the Solar System Look Like? What Can We Learn by Comparing the Planets to One Another?

Chapter 7 Our Planetary System What Does the Solar System Look Like? What Can We Learn by Comparing the Planets to One Another?

Chapter 7 7.1 Studying the Solar System Our • Our goals for learning • What does the solar system look like? • What can we learn by comparing the to one another? • What are the major features of the and planets?

Earth, as viewed by the Voyager

What does the solar system look • Eight major like? planets with nearly circular

is smaller than the major planets and has a more elliptical

What can we learn by comparing the planets to one another? • Planets all orbit in same direction and nearly in same plane

1 Comparative Planetology • Comparing the planets reveals patterns among • We can learn more about a like our them by studying in context with other in the solar system. • Those patterns • Stay focused on processes common to provide insights multiple worlds instead of individual facts that help us specific to a particular world. understand our own

What are the major features of Planets are very tiny the Sun and planets? compared to distances between them.

Sun and planets to scale

Sun

• Over 99.9% of solar system’s • Made of metal and rock; large core • Made mostly of H/He gas () • Desolate, cratered; long, tall, steep cliffs • Converts 4 million tons of mass into each second • Very hot and very cold: 425°C (day), –170°C (night)

2 Earth

Earth and to scale • Nearly identical in size to Earth; surface hidden by • Hellish conditions due to an extreme greenhouse effect: • An oasis of • Even hotter than Mercury: 470°C, day and night • The only surface liquid in the solar system • A surprisingly large moon

Jupiter

• Much farther from Sun than inner planets • Mostly H/He; no solid surface • 300 times more massive than • Looks almost Earth-like, but don’t go without a spacesuit! Earth • Giant volcanoes, a huge canyon, polar caps, more… • Water flowed in the distant past; could there have been • Many , life? rings …

Saturn ’s moons can be as interesting as planets themselves, especially Jupiter’s four

(shown here): Active volcanoes all over • Giant and gaseous like Jupiter • : Possible subsurface • Spectacular rings • : Largest moon in solar system • Many moons, including cloudy : A large, cratered “ ball” • Cassini spacecraft currently studying it

3 Rings are NOT solid; Cassini probe they are made arrived July of countless 2004 small chunks of ice and (Launched in rock, each 1997) orbiting like a tiny moon.

Artist’s conception

Uranus • Smaller than Jupiter/; • Similar to much larger than (except for axis Earth tilt) • Made of H/He gas & • Many moons compounds (including ) (H2O, NH3, CH4) • Extreme axis tilt • Moons & rings

Pluto

• Much smaller than other planets • Icy, -like composition • Its moon is similar in size

4 What have we learned? What have we learned?

• What does the solar system look like? • What are the major features of the Sun and planets? – Planets orbit Sun in the same direction and in – Sun: Over 99.9% of the mass nearly the same plane. – Mercury: A hot rock • What can we learn by comparing the planets to – Venus: Same size as Earth but much hotter one another? – Earth: Only planet with liquid water on surface – Mars: Could have had liquid water in past – Comparative planetology looks for patterns – Jupiter: A gaseous giant among the planets. – Saturn: Gaseous with spectacular rings – Those patterns give us insight into the general – Uranus: A with a highly tilted axis processes that govern planets – Neptune: Similar to Uranus but with normal axis – Studying other worlds in this way tells us – Pluto: An icy “misfit” more like a comet than a planet about our own Earth

What features of the solar system 7.2 Patterns in the Solar System provide clues to how it formed?

• Our goals for learning • What features of the solar system provide clues to how it formed?

Motion of Large Bodies Two Main Planet Types

• All large bodies • Terrestrial in the solar planets are system orbit in rocky, relatively the same small, and close direction and in to the Sun nearly the same • Jovian planets plane are gaseous, • Most also rotate larger, and in that direction farther from Sun

5 Swarms of Smaller Bodies Notable Exceptions

• Many rocky • Several and exceptions to icy the normal populate the patterns need to solar system be explained

Special Topic: How did we learn the scale of the solar system? • Apparent position of Venus on Sun during transit depends on distances in solar system and your position on Earth

Transit of Venus: June 8, 2004

What have we learned? Measuring Distance to Venus • What features of the solar system provide clues • Measure apparent to how it formed? position of Venus – Motions of large bodies: All in same on Sun from two direction and plane locations on Earth – Two main planet types: Terrestrial and jovian • Use trigonometry – Swarms of small bodies: Asteroids and to determine comets Venus’ distance – Notable exceptions: Rotation of Uranus, from the distance Earth’s large moon, etc. between the two locations on Earth

6 7.3 Spacecraft of the Solar How do work? System • Our goals for learning • How do robotic spacecraft work?

Flybys Orbiters

• A flyby mission • Go into orbit around another world flies by a planet • More time to gather data but cannot obtain just once detailed information about world’s surface • Cheaper than other mission but have less time to gather data

Probes or Landers Sample Return Missions

• Land on surface of another world • Gather samples • Spacecraft designed to blast off other world and return to Earth • Land on surface of another world • Apollo missions to Moon are only sample • Explore surface in detail return missions to date

7 What have we learned? Combination Spacecraft • How do robotic spacecraft work? – Flyby: Flies by another world only once. – : Goes into orbit around another world – Probe/Lander: Lands on surface – Sample Return Mission: Returns a sample of another world’s surface to Earth

• Cassini/ mission contains both an orbiter (Cassini) and a lander (Huygens)

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