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The Solar System There are two broad categories of planets: Earthlike and Jupiter like All of the planets orbit the Sun in the same direction and in almost the same plane Most of the planets have nearly circular orbits

The Solar System There are two broad categories of planets: Earthlike and Jupiter like All of the planets orbit the Sun in the same direction and in almost

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The Solar System

There are two broad categories of planets:Earthlike and Jupiter like

All of the planets orbit the Sun in the same direction and in almost the same plane

Most of the planets have nearly circular orbits

The Solar SystemDensity

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The average density of any substance depends in part on its composition An object sinks in a fluid if its average density is greater than that of the fluid, but rises if its average density is less than that of the fluid The terrestrial (inner) planets are made of rocky materials and have dense iron cores, which gives these planets high average densitiesThe Jovian (outer) planets are composed primarily of light elements such as hydrogen and helium, which gives these planets low average densities

The Solar System

The Inner Planets

- The Inner Planets

The inner planets take up only a small part of the solar system. Note that sizes and distances are not drawn to scale.

The Solar System

Earth is the third planet from the sun and the fifth largest. Earth has only one moon. The earth is 4.5 billion years old.

The Solar System

Earth’s Layers

- The Inner Planets

Earth has three main layers—a crust, a mantle, and a core.

The Solar System

• Mercury is the closest planet to the sun and the eighth largest.

• Mercury has no moons. • Mercury has extreme temperature fluctuations from 430 to -170 degrees celsius (day and night).

The Solar System

Mercury

- The Inner Planets

Mercury is the smallest terrestrial planet and the planet closest to the sun.

The Solar System

• Venus is called Earth’s twin • Venus’s surface is 460

degrees (could melt metal!). • Venus is covered with swirling

clouds (thick atmosphere of CO2 and Sulfuric Acid and always cloudy).

• It is the hottest planet (greenhouse effect).

The Solar System

Venus

- The Inner Planets

Venus’s density and internal structure are similar to Earth’s. But, in other ways, Venus and Earth are very different.

The Solar System

Venus

- The Inner Planets

This figure combines images of Venus taken from space with a camera (left) and radar (right). The camera image shows Venus’s thick atmosphere. Radar is able to penetrate Venus’s clouds to reveal the surface. Both images are false color.

The Solar System

• Mars is the seventh largest planet in the solar system.

• Thin atmosphere is ~95% CO2 (H20 gas or polar ice caps)

• Mars temperature ranges between -140 and 20 degrees C.

• Mars used to be warm with lots of water long ago.

The Solar System

Mars

- The Inner Planets

Mars is called the “red planet.” When you see it in the sky, it has a slightly reddish tinge. This reddish color is due to the breakdown of iron-rich rocks, which creates a rusty dust that covers much of Mars’s surface.

The Solar System

Mars

- The Inner Planets

Mares has ice caps at both poles. Scientists think that a large amount of liquid water flowed on Mars's surface in the distant past.

The Solar System

What You Know

What You Learned

Using Prior KnowledgeLook at the section headings and visuals to see what this section is about. Then write what you know about the inner planets in a graphic organizer like the one below. As you read, write what you learn.

1. Most of Earth is covered with water.2. Mercury is closest to the sun.3. Venus is very hot.4. Mars is called the “red planet.”

1. Earth is unique in our solar system for having liquid water at its surface.2. Mercury has a greater temperature range than any of the other planets.3. A day on Venus is longer than its year.4. The reddish tinge on Mars is caused by the breakdown of iron-rich

rocks.

- The Inner Planets

The Solar System

End of Section:The Inner Planets

The Solar SystemSeven large satellites are almost as big as

the terrestrial planets

Comparable in size to the planet Mercury

The remaining satellites of the solar system are much smaller

The Solar System

Gas Giants and Pluto

- The Outer Planets

The first four outer planets–Jupiter, Saturn, Uranus, and Neptune–are much larger and more massive than Earth, and they do not have solid surfaces. Pluto is small and rocky.

The Solar System

The Solar System

Jupiter’s Red Spot is a 350 year old hurricane!

Nighttime image showing lightning in Jupiter’s

atmosphere

The Solar System

Jupiter’s Structure (no solid surface!)

- The Outer Planets

Jupiter is composed mainly of the elements hydrogen and helium.

The Solar System

Jupiter’s Moons

- The Outer Planets

• The astronomer Galileo discovered Jupiter’s four largest moons. They are named Io, Europa, Ganymede, and Callisto.

• Dozens of additional Jupiter moons have been discovered since Galileo’s time

• Jupiter is the most massive planet by far (1,300 Earths and 2.5 times that of all other planets combined!

The Solar System - The Outer Planets

Saturn

Saturn has the most spectacular rings of any planet.

The Solar System

Saturn

• Saturn is the second largest planet in our solar system• Saturn has an atmosphere of thick clouds and is

composed of hydrogen and helium (similar to Jupiter)• Saturn’s rings are composed of ice and rock chunks

orbiting together in different layers• Saturn has many moons (the largest is Titan)

The Solar System - The Outer Planets

Uranus

Although the gas giant Uranus is about four times the diameter of Earth, it is still much smaller than Jupiter and Saturn.

The Solar System - The Outer Planets

Uranus

Uranus’s axis of rotation is tilted at an angle of about 90 degrees from the vertical.

The Solar System - The Outer Planets

Neptune

Neptune is a cold, blue planet (similar color and size to Uranus). Its atmosphere contains visible clouds.

Discovered by math equation in 1846 (orbital pattern)

*Scientists think Neptune is shrinking in size…and heating up!

The Solar System

Circumference To calculate the circumference of a circle, use this formula:

C = 2πr

In the formula, π ≈ 3.14, and r is the circle’s radius, which is the distance from the center of the circle to its edge. The same formula can be used to calculate the circumference of planets, which are nearly spherical.

Neptune’s radius at its equator is about 24,800 km. Calculate its circumference.

C = 2πr

= 2.00 X 3.14 X 24,800 km

= 156,000 km

- The Outer Planets

The Solar System

Circumference

Practice Problem

Saturn’s radius is 60,250 km. What is its circumference?

2 X 3.14 X 60,250 km = about 378,800 km

- The Outer Planets

The Solar System - The Outer Planets

Pluto

Pluto has a solid surface and is much smaller and denser than the other outer planets.

The Solar System

Pluto

Pluto is a special caseSmaller than any of the terrestrial planets

Intermediate average density of about 1900 kg/m3

Density suggests it is composed of a mixture of ice and rock

The Solar System

Identifying Main IdeasAs you read the section “Gas Giants and Pluto,” write the main idea–the biggest or most important idea–in a graphic organizer like the one below. Then write supporting details that further explain the main idea.

The four gas giants are similar in…

Structure–they do not have a solid surface.

Atmosphere–thick and made up mainly of hydrogen and helium.

Rings–each is surrounded by a set of rings.

Main Idea

Size and mass–each is very large and massive.

Detail Detail Detail Detail

- The Outer Planets

The Solar System

End of Section:The Outer

Planets