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Observing the Solar System

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The favorable conditions on Earth that allow life to exist Is there life on Mars? Scientists have not yet found evidence for life on Mars. – PowerPoint PPT presentation

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Title: Observing the Solar System


1
Table of Contents
  • Observing the Solar System
  • The Sun
  • The Inner Planets
  • The Outer Planets
  • Comets, Asteroids, and Meteors
  • Is There Life Beyond Earth?

2
Geocentric System
- Observing the Solar System
  • In a geocentric system, Earth is at the center of
    the revolving planets and stars.

3
Heliocentric System
- Observing the Solar System
  • In a heliocentric system, Earth and the other
    planets revolve around the sun.

4
The Sun and Planets
- Observing the Solar System
  • Shown below are the average distances of each
    planet from the sun.

5
Solar System Activity
- Observing the Solar System
  • Click the Active Art button to open a browser
    window and access Active Art about the solar
    system.

6
Planet Speed Versus Distance
- Observing the Solar System
  • Johannes Kepler discovered a relationship between
    the speed of a planet and its distance from the
    sun. Use the graph to discover what Kepler
    learned.

7
Planet Speed Versus Distance
- Observing the Solar System
  • Reading Graphs
  • According to the graph, what is Earths average
    speed?
  • About 30 km/s

8
Planet Speed Versus Distance
- Observing the Solar System
  • Interpreting Data
  • Which is closer to the sun, Mercury or Mars?
    Which moves faster?
  • Mercury Mercury

9
Planet Speed Versus Distance
- Observing the Solar System
  • Drawing Conclusions
  • What is the general relationship between a
    planets speed and its average distance from the
    sun?
  • Planets that are closer to the sun move faster.

10
Planet Speed Versus Distance
- Observing the Solar System
  • Predicting
  • The planet Uranus is about 2,900 million km from
    the sun. Predict whether its speed is greater or
    less than Jupiter's speed. Explain your answer.
  • Uranuss speed is less than that of Jupiter
    because Uranus is farther from the sun than
    Jupiter.

11
Previewing Visuals
- Observing the Solar System
  • Preview Figure 2 and Figure 3. Then write two
    questions you have about Earths history in a
    graphic organizer like the one below. As you
    read, answer your questions.

Models of the Universe
Q. What is a geocentric model?
A. A model that shows Earth at the center of the
revolving planets and stars
Q. What is a heliocentric system?
A. A model that shows Earth and the other planets
revolving around the sun
12
End of SectionObserving the Solar System
13
The Layers of the Sun
- The Sun
  • The sun has an interior and an atmosphere, each
    of which consists of several layers.

14
Outlining
- The Sun
The Sun
  • The Suns Interior
  • The Core
  • The Radiation Zone
  • The Convection Zone
  • The Suns Atmosphere
  • The Photosphere
  • The Chromosphere
  • The Corona
  • Features on the Sun
  • Sunspots
  • Prominences
  • Solar Flares
  • Solar Wind
  • As you read, make an outline about the sun that
    you can use for review. Use the red headings for
    the main topics and the blue headings for the
    subtopics.

15
More on the Sun
- The Sun
  • Click the Planet Diary button for an activity
    about the sun.

16
End of SectionThe Sun
17
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.

18
Earths Layers
- The Inner Planets
  • Earth has three main layersa crust, a mantle,
    and a core.

19
Mercury
- The Inner Planets
  • Mercury is the smallest terrestrial planet and
    the planet closest to the sun.

20
Venus
- The Inner Planets
  • Venuss density and internal structure are
    similar to Earths. But, in other ways, Venus and
    Earth are very different.

21
Venus
- The Inner Planets
  • This figure combines images of Venus taken from
    space with a camera (left) and radar (right). The
    camera image shows Venuss thick atmosphere.
    Radar is able to penetrate Venuss clouds to
    reveal the surface. Both images are false color.

22
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 Marss surface.

23
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.

24
Using Prior Knowledge
- The Inner Planets
  • Look 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.

What You Know
  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.

What You Learned
  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.

25
Links on the Planets
- The Inner Planets
  • Click the SciLinks button for links on the
    planets.

26
End of SectionThe Inner Planets
27
Gas Giants and Pluto
- The Outer Planets
  • The first four outer planetsJupiter, Saturn,
    Uranus, and Neptuneare much larger and more
    massive than Earth, and they do not have solid
    surfaces. Pluto is small and rocky.

28
Jupiters Structure
- The Outer Planets
  • Jupiter is composed mainly of the elements
    hydrogen and helium.

29
Jupiters Moons
- The Outer Planets
  • The astronomer Galileo discovered Jupiters four
    largest moons. They are named Io, Europa,
    Ganymede, and Callisto.

30
Saturn
- The Outer Planets
  • Saturn has the most spectacular rings of any
    planet.

31
Uranus
- The Outer Planets
  • Although the gas giant Uranus is about four times
    the diameter of Earth, it is still much smaller
    than Jupiter and Saturn.

32
Uranus
- The Outer Planets
  • Uranuss axis of rotation is tilted at an angle
    of about 90 degrees from the vertical.

33
Neptune
- The Outer Planets
  • Neptune is a cold, blue planet. Its atmosphere
    contains visible clouds.

34
Circumference
- The Outer Planets
  • To calculate the circumference of a circle, use
    this formula
  • C 2pr
  • In the formula, p 3.14, and r is the circles
    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.
  • Neptunes radius at its equator is about 24,800
    km. Calculate its circumference.
  • C 2pr
  • 2.00 X 3.14 X 24,800 km
  • 156,000 km

35
Circumference
- The Outer Planets
  • Practice Problem
  • Saturns radius is 60,250 km. What is its
    circumference?
  • 2 X 3.14 X 60,250 km about 378,800 km

36
Pluto
- The Outer Planets
  • Pluto has a solid surface and is much smaller and
    denser than the other outer planets.

37
Identifying Main Ideas
- The Outer Planets
  • As you read the section Gas Giants and Pluto,
    write the main ideathe biggest or most important
    ideain a graphic organizer like the one below.
    Then write supporting details that further
    explain the main idea.

Main Idea
The four gas giants are similar in
Detail
Detail
Detail
Detail
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.
Size and mass each is very large and massive.
38
More on the Planets
- The Outer Planets
  • Click the PHSchool.com button for an
    activityabout the planets.

39
End of SectionThe Outer Planets
40
Structure of a Comet
- Comets, Asteroids, and Meteors
  • The main parts of a comet are the nucleus, the
    coma, and the tail. Most comets have two tailsa
    bluish gas tail and a white dust tail.

41
Comet Orbits
- Comets, Asteroids, and Meteors
  • Most comets revolve around the sun in very long,
    narrow orbits. Gas and dust tails form as the
    comet approachesthe sun.

42
The Asteroid Belt
- Comets, Asteroids, and Meteors
  • Most asteroids revolve around the sun between the
    orbits of Mars and Jupiter. This region is called
    the asteroid belt.

43
Comparing and Contrasting
- Comets, Asteroids, and Meteors
  • As you read, compare and contrast comets,
    asteroids, and meteoroids by completing a table
    like the one below.

Comets, Asteroids, and Meteoroids
Feature
Comets
Asteroids
Meteoroids
Kuiper belt and Oort cloud
Between the orbits of Mars and Jupiter
Origin
Comets or asteroids
Typically less than 1 km some are more than 300
km in diameter
Excluding the tail, about the size of a mountain
Smaller than comets or asteroids
Size
Ice, dust, small rocky particles
Composition
Rock
Rock or dust
44
Links on Comets, Asteroids, and Meteors
- Comets, Asteroids, and Meteors
  • Click the SciLinks button for links on
    comets,asteroids, and meteors.

45
End of SectionComets, Asteroids, and Meteors
46
Asking Questions
- Is There Life Beyond Earth?
  • Before you read, preview the red headings. In a
    graphic organizer like the one below, ask a
    question for each heading. As you read, write
    answers to your questions.

What are the Goldilocksconditions?
The favorable conditions on Earth that allow life
to exist
Is there life on Mars?
Scientists have not yet found evidence for life
on Mars.
Why do scientists think Europa might have life?
Europa has an ice crust that could have a liquid
water ocean underneath.
47
Links on Extraterrestrial Life
- Is There Life Beyond Earth?
  • Click the SciLinks button for links on
    extraterrestrial life.

48
End of SectionIs There Life Beyond Earth?
49
Graphic Organizer

Feature
Geocentric System
Heliocentric System
Object at center
Earth
Sun
Objects that move around center
Planets and sun
Planets
Proposed by
Early Greek astronomers
Copernicus
Supporters
Ptolemy
Brahe, Kepler, Galileo
50
End of SectionGraphic Organizer
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