Download The Inner Planets

The Solar System
4-3 The Inner Planets
Vocabulary
Terrestrial planet-The name often
given to the four inner planets:
Mercury, Venus, Earth, and Mars.
Greenhouse effect- The trapping
Of heat near a planet’s surface by
certain gases in the planet’s
atmosphere.
The Inner Planets – My planet diary p. 146
What’s in a name?
•You can find Lewis and Clark’s guide Sacagawea, artist Frida Kahlo, writer
Helen Keller, and abolitionist Sojourner Truth all on Venus
•Almost every feature on Venus is named for a real, fictional, or mythological
woman.
•The person or people who discover an object or feature in the solar system get
to choose its name
• Guidelines:
•Features on Mercury are named for authors, artists, and musicians.
•Many craters on Mars are named for towns on Earth.
•most of the craters on Earth’s moon are named for astronomers,
physicists, and mathematicians.
Who decides what to name a newly discovered feature in the solar system?
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If you discovered a new planet, how would you decide what to name its
features?
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The Inner Planets – what do the inner planets
have in common p. 147
•The inner planets are small and dense and have rocky surfaces.
•often called the terrestrial planets, from the Latin word terra, which means
“Earth.”
•All have relatively high densities
•Rich in rocky and metallic materials, including iron and silicon
•Each has a solid surface
•All have atmospheres, except Mercury
Figure 1:
Which planet is the largest?
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Which plant has the most moons?
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Which planet is most similar to Earth
In size?
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Assess Your Understanding pg. 147
I Get It! Now I know that the inner planets are
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*The inner planets are Mercury, Venus, Earth, and Mars.
*Close to the Sun and separated from the much larger Outer
Planets by an asteroid belt.
*Sometimes called terrestrial planets and are composed of rock.
* Due to their hard surfaces, these planets have canyons, craters,
mountains, and volcanoes.
* Few or no moons.
* Developed from small grains of dust that collided and formed
together.
The Inner Planets – Mercury p. 148
• Smallest terrestrial planet (not much better than Earth’s
moon) and closet to the sun
•Temperature can range from 430°C to below -170°C
• Interior probably made up mainly of dense metal iron
Surface:
• Flat plains and craters on its surface
• Most craters formed early in the history of the solar system
• Craters have not worn away over time because of lack of
atmosphere and water
Atmosphere:
• Virtually no atmosphere
• Because its mass is so small, its gravity is weak. Particles can
easily escape into space
• Astronomers have detected small amounts of sodium and other
gases around Mercury
Mercury pg. 148
Exploring Mercury:
• Mariner 10 flew by Mercury
3 times in 1974 and 1975
• Mercury MESSENGER has
passed Mercury several times,
and will begin orbiting in 2011
Figure 2:
The photo shows Mercury’s cratered surface.
List 3 things a visitor to Mercury would need to bring.
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How many Mercury days are there in a mercury year? (see figure 1)
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Venus pg. 149
• Venus has a thick atmosphere, an unusual pattern of rotation,
and the hottest surface of any planet.
Venus’s Atmosphere
• Venus’s atmosphere is so thick that it is always cloudy.
• Venus has a smooth cloud cover made mostly of droplets of sulfuric acid.
• Venus’s atmosphere has 90 times the pressure than the Earth’s
Atmosphere. You would be crushed by the weight!
• Venus’s atmosphere is mostly carbon dioxide- so you would not be able
to breathe.
Venus’s Rotation- a day is longer than a year on Venus!!!
• Venus takes 7.5 Earth months to revolve around the sun(a year).
• Venus takes 8 months to rotate once on its axis (a day).
• Venus rotates from east to west, the opposite direction of most other
planets and moons. (This is possibly because Venus was hit by a large object
billions of years ago OR maybe because its thick atmosphere has somehow
changed its rotation).
Figure 3 Venus pg. 149
These figures show images of Venus taken from space with a
camera (left) and radar (right). Radar is able to penetrate Venus’s thick
clouds to reveal the surface. The colors in both images are altered to
show more details.
Infer: Why do scientists need to use radar to study Venus’s surface?
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Blue regions are
flat plains covered
by lava flows.
Venus pg. 150
A Hot Planet
Venus is closer to the sun than Earth, so it receives more solar energy
than Earth does. The thick atmosphere traps the heat so well that,
Venus has the hottest surface of any planet. The average surface
temperature of 460 degrees celsius is hot enough to melt lead. When
heat is trapped by the atmosphere it is called the greenhouse effect.
Exploring Venus
Venera 7 was the first probe to land on the surface of Venus(1970) and
send back data.
Magellan Probe (1990) carried radar instruments and mapped the entire
surface through the thick clouds confirming a rocky surface, more
than 10,000 volcanoes and plains formed by lava flows.
Venus Express from the European Space Agency showed how Venus’s
clouds form and change.
The Greenhouse Effect pg. 150 Figure 4
Gases in the atmosphere trap some heat energy. Some is transmitted into
space. More heat is trapped on Venus than on Earth.
Apply Concepts:
Look at what happens to heat energy on Venus. Then draw arrows to show
what happens on Earth.
Radiation absorbed
by greenhouse gases
Escaping
radiation
Solar
radiation
Solar
radiation
Earth pg. 151
There is only one planet in the solar system where you could live easily.
Earth has liquid water and a suitable temperature range and
atmosphere for living things to survive.
The Water Planet
The Planet Earth is the only planet that has liquid water on its surface(70%).
Earth’s Temperature
Earth’s temperature is not too hot nor too cold for life on Earth. If Earth
was closer (water would evaporate) or farther from the sun (water
would be frozen).
Earth’s Atmosphere
Earth is the only planet with an atmosphere that is rich in oxygen.
Oxygen makes up 20% of the atmosphere. Like Venus, Earth
experiences the Greenhouse Effect. This makes Earth Warmer.
Mars pg. 152
Mars is known as the “red planet”.
Although Mars is too cold for liquid water,
it does have water ice now and had liquid
water in the past.
Mars’s Atmosphere
-is more than 95% carbon dioxide It has few clouds that are very thin.
Temperatures range from -140 to 20 degrees Celsius.
Water and Ice
Scientists think that liquid water flowed on Mars at one time. Now the
atmosphere is so thin that any liquid would turn into a gas. Water is
suspected in the two polar ice caps.
Volcanoes
There are some giant Volcanoes on Mars. The largest is Olympus Mons
which is the largest volcano in the solar system.
Mars
Mars’s Moons
Mars has 2 very small moons.
Phobos- the larger moon is 22 km across
Deimos – the smaller moon is 13 km across.
Both moons are covered in craters.
pg. 153
Exploring Mars
Many space probes have visited Mars. Rovers called Spirit and
Opportunity found traces of salts and minerals that form in the
presence of water.
Curiosity is a rover that is
currently on Mars. Curiosity
collected rock samples for analysis.
http://www.nasa.gov/multimedia/videogallery/index.html?collection_id=
18895&media_id=160133361
Assess Your Understanding pg. 153
1a. Name- Which inner planet has the thickest atmosphere?
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b. Relate Cause and Effect- Why is Venus hotter than Mercury?
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I get it! Now I know that the inner planets differ in _______________
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The Inner Planets
Earth's Structure
Earth has three main layers: the crust, the mantle, and the core.