how are the inner planets similar?

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5.3 The Inner Solar System This imaginative painting shows a possible future human settlement on Mars. Settlers might live in domes to protect themselves from the harsh climate

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This imaginative painting shows a possible future human settlement on Mars. Settlers might live in domes to protect themselves from the harsh climate and to provide an atmosphere for breathing. How are the inner planets similar?. - PowerPoint PPT Presentation

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25.3 The Inner Solar System

This imaginative painting shows a possible future human settlement on Mars. Settlers might live in domes to protect themselves from the harsh climate and to provide an atmosphere for breathing.

25.3 The Inner Solar System

How are the inner planets similar?

The Terrestrial Planets

The four inner planets are all relatively small and dense, and have rocky surfaces. Like Earth, they all have a crust, mantle, and iron core.

25.3 The Inner Solar System

The terrestrial planets are planets similar in structure to Earth: Mercury, Venus, Earth, and Mars

• All of the terrestrial planets have rocky crusts. • Mercury and Mars have surfaces that are

pockmarked by craters. Most craters on Earth and Venus have disappeared because the surface is continually being altered.

The Terrestrial Planets

25.3 The Inner Solar System

The terrestrial planets are much warmer on average than the outer planets.

The inner planets have few (if any) moons and no rings.

The Terrestrial Planets

25.3 The Inner Solar System

The Terrestrial Planets

25.3 The Inner Solar System

What are the characteristics of Mercury?

Mercury

Mercury is the smallest of the terrestrial planets, and the closest planet to the sun.

25.3 The Inner Solar System

Mercury is a dense planet with a very large iron core.

There is no mantle convection within the planet, and little erosion on its surface.

It takes only 88 Earth days for Mercury to complete one revolution. This is the shortest period of revolution of any planet.

Mercury

25.3 The Inner Solar System

Mercury’s surface is heavily cratered from meteoroid collisions. This false-color image was made by combining a series of smaller images taken by the Mariner 10 space probe. Orange areas for which no images are available are blank.

Mercury

25.3 The Inner Solar System

Temperature and Atmosphere

Mercury’s surface temperature ranges between two extremes.

• Day temperatures at the equator reach about 430°C.• At night, the temperature drops as low as –170°C.

The time between sunrise and sunset equals the time it takes for Mercury to revolve around the sun, about 88 days.

Mercury has virtually no atmosphere.

Mercury

25.3 The Inner Solar System

Exploring Mercury

Because Mercury is so close to the sun, it’s hard for astronomers on Earth to see. In 1974–1975, Mariner 10 took many images of Mercury’s surface.

The surface looks like that of Earth’s moon. Mercury’s surface has been largely unchanged for billions of years.

The Messenger space probe will orbit Mercury in 2011.

Mercury

25.3 The Inner Solar System

What are the characteristics of Venus?

Venus

Venus’s thick atmosphere is composed mostly of carbon dioxide, which traps heat and raises the planet’s temperature.

25.3 The Inner Solar System

Venus is called the “evening star” or “morning star” because it is only seen in the west after sunset or in the east before sunrise.

Except for the moon, Venus is the brightest object in Earth’s night sky.

Venus rotates slowly in the direction opposite to which it revolves, and its day is longer than its year.

Venus

25.3 The Inner Solar System

Venus’s Atmosphere

Venus is difficult to study from space because clouds hide its surface.

Venus’s atmosphere is so thick that the pressure at its surface is 90 times that on Earth.

Spacecraft that landed on Venus’s surface in the 1970s found the average surface temperature to be 460°C.

Venus

25.3 The Inner Solar System

Exploring Venus

The high sulfur content of Venus’s atmosphere probably results from numerous volcanoes.

The outpouring of lava from volcanoes has frequently resurfaced the planet, erasing craters as well.

Though Venus probably has active volcanoes, it shows no evidence of plate tectonics.

Venus

25.3 The Inner Solar System

A. Photographs in visible light only show Venus’s clouds.

B. Radar is able to penetrate Venus’s atmosphere. Radar data were used to produce this false-color image of a volcano on Venus.

Venus

25.3 The Inner Solar System

What are the characteristics of Earth?

Earth

Earth’s surface has a suitable atmosphere and temperature range for water to exist as a liquid.

25.3 The Inner Solar System

Earth is unique in several important respects. • The presence of liquid water makes it possible

for Earth to support millions of different species of living things.

• Water also causes erosion, which has shaped Earth’s land surface in many ways.

Earth

25.3 The Inner Solar System

Earth is unique among the planets in having liquid-water oceans at its surface.

Earth

25.3 The Inner Solar System

Unlike most smaller planets and moons, Earth has enough gravity to hold most gas molecules.

This allows Earth to maintain a thick atmosphere.

Earth’s atmosphere is not composed mostly of carbon dioxide, like the atmospheres of Venus and Mars, because some living organisms use carbon dioxide and produce oxygen.

Earth

25.3 The Inner Solar System

The moon, Mercury, and Mars are all so small that over time they have lost much of their internal heat and have become geologically dead.

Earth is large enough that it has not had a chance to cool down much, so Earth has moving tectonic plates that continually change its surface.

Earth

25.3 The Inner Solar System

What are the characteristics Mars?

Mars

Mars shows evidence of once having a great deal of liquid surface water.

25.3 The Inner Solar System

Mars is the most Earthlike of all of the planets. • The weathering of iron-rich rocks on its surface

gives the planet a reddish color. • Though the surface of Mars is very old, as

shown by the presence of many impact craters, it once had many volcanic eruptions.

Mars

25.3 The Inner Solar System

Mars’s Atmosphere

Mars has a very thin atmosphere, which allows astronomers to see its surface with a telescope.

• The thin Martian atmosphere and its distance from the sun make the surface very cold. Temperatures vary from –140°C to 20°C.

• Mars’s atmosphere is more than 95% carbon dioxide, similar to the atmosphere of Venus, but much thinner.

Mars

25.3 The Inner Solar System

Water on Mars

There is no liquid water on Mars’s surface now, but there likely was some in the past. Some geologists think Mars’s northern lowlands were once covered by an ocean.

Some water vapor has escaped into space. Some water is stored in ice caps at the poles, and some is frozen underground just below the surface.

Mars

25.3 The Inner Solar System

Because Mars had liquid water on its surface in the past, many scientists wonder if life once existed there.

Robotic probes have carried out experiments on the Martian surface to look for signs of life.

None of these probes found clear evidence for the existence of life on Mars.

Mars

25.3 The Inner Solar System

A. Mars has ice caps at both poles.

Mars

25.3 The Inner Solar System

B. Olympus Mons is the largest volcano in the solar system.

Mars

25.3 The Inner Solar System

C. These Martian valleys are thought to have been formed at least in part by large flows of liquid water in the distant past.

Mars

25.3 The Inner Solar System

Martian Seasons

Like Earth, Mars has distinct seasons. Mars’s seasons are caused by the tilt of its axis.

Over the course of a Martian year, Mars’s ice caps grow and shrink.

The change in seasons also causes large dust storms that occasionally rage across the surface.

Mars

25.3 The Inner Solar System

This photo of a dark boulder on Martian sand was taken by the Mars Exploration Rover Spirit in 2006. Spirit found rocks and minerals that formed in, or were altered by, water.

Mars

25.3 The Inner Solar System

What are asteroids and how were they formed?

Asteroids

Scientists now hypothesize that asteroids are remnants of the early solar system that never came together to form a planet.

25.3 The Inner Solar System

Beyond Mars is a region of the solar system where small, rocky bodies called asteroids can be found orbiting the sun.

This region is referred to as the asteroid belt.

Although most asteroids are found in the asteroid belt, others orbit near Jupiter or range through the inner solar system.

Asteroids

25.3 The Inner Solar System

Astronomers have discovered more than 10,000 asteroids, and many more are thought to exist.

Most asteroids are less than 1 kilometer in diameter; only three are larger than 500 kilometers across.

Asteroids

25.3 The Inner Solar System

The largest asteroids have enough gravity to have pulled themselves into nearly spherical or oval shapes while forming.

Smaller asteroids, however, can have very irregular forms.

Scientists think that some asteroids are like floating rubble heaps, held together by weak gravity.

Asteroids

25.3 The Inner Solar System

A. The asteroid Ida was photographed by the Galileo probe on its way to Jupiter.

B. In 2001, the NEAR Shoemaker space probe landed on the asteroid Eros.

Asteroids

25.3 The Inner Solar System

In the past, scientists thought that asteroids were the remnants of a shattered planet. Scientists now hypothesize that asteroids are remnants of the early solar system that never came together to form a planet.

This hypothesis is supported by the lack of mass in the asteroid belt. All the asteroids together would form a planetary body only about 1500 kilometers in diameter.

Asteroids

25.3 The Inner Solar System

Assessment Questions

1. Which object in the solar system has conditions on its surface most like the conditions on planet Earth? a. Mercury

b. Venus

c. the moon

d. Mars

25.3 The Inner Solar System

Assessment Questions

1. Which object in the solar system has conditions on its surface most like the conditions on planet Earth? a. Mercury

b. Venus

c. the moon

d. Mars

ANS: D

25.3 The Inner Solar System

Assessment Questions

2. Why do most scientists no longer accept the hypothesis that asteroids are remnants of a shattered planet?a. Their total mass is much less than the mass of a planet.b. They are not as spherical as are all the planets.c. Unlike planets, asteroids are made primarily of ice.d. There is no known cause for a planet to shatter.

25.3 The Inner Solar System

Assessment Questions

2. Why do most scientists no longer accept the hypothesis that asteroids are remnants of a shattered planet?a. Their total mass is much less than the mass of a planet.b. They are not as spherical as are all the planets.c. Unlike planets, asteroids are made primarily of ice.d. There is no known cause for a planet to shatter.

ANS: A