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Unit 2 : The Solar System
Lesson 1 Historical Models of the Solar
System
Ms. Alia Ibrahim
Copyright © Houghton Mifflin Harcourt Publishing Company
Science
What Is the Center of the
Solar System?
Copyright © Houghton Mifflin Harcourt Publishing Company
What is the solar system?
• The solar system is the sun and all of
the bodies that orbit the sun.
• Our current model of the solar system
is the sun-centered, or heliocentric,
model.
• In the heliocentric model, Earth and
the other planets orbit the sun.
Unit 2 Lesson 1 Historical Models of the Solar System
What is the solar system?
• The earliest models of the solar system
assumed that Earth was at the center,
with the sun, moon, and planets circling
it. These are the Geocentric models
• The heliocentric model was not generally
accepted until the work of Copernicus
and Kepler in the late 16th to early 17th
centuries.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Aristotle – Geocentric model
• The Greek philosopher Aristotle was
among the first thinkers to propose
this model.
• His model placed the moon, sun,
planets, and stars on a series of circles
that surrounded Earth.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
• This apparent shift in the position of an
object when viewed from different
locations is known as parallax.
• In fact, the stars are so far away that
parallax cannot be seen with the
unaided eye.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Aristarchus – Heliocentric model
• Aristarchus, a Greek astronomer and
mathematician, is reported to have
proposed a heliocentric model of the
solar system.
• His model, however, was not widely
accepted at the time.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Ptolemy – Geocentric model
• Ptolemy was an astronomer, geographer,
and mathematician who lived in
Alexandria, Egypt.
• He developed a detailed geocentric model
that was used by astronomers for the
next 14 centuries.
• In Ptolemy’s model, the planets moved on
small circles that in turn moved on larger
circles.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
• Ptolemy’s “wheels-on-wheels” system
fit observations better than any model
that had come before.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Copernicus – Heliocentric model
• The Polish astronomer Nicolaus
Copernicus felt that Ptolemy’s model of
the solar system was too complicated.
• He knew about Aristarchus’s ideas when
he developed the first detailed
heliocentric model of the solar system.
• Copernicus adopted Ptolemy’s idea that
planetary paths should be perfect
circles.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
• Like Ptolemy, Copernicus used a
“wheels-on-wheels” model.
• Copernicus’s model is generally seen as
the first step in the development of
modern models of the solar system.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Kepler
• Johannes Kepler was a German
mathematician and astronomer.
• After careful observation and analysis,
he realized that planetary orbits were
not circular but were more like ellipses.
• He formulated three principles, which
are today known as Kepler’s laws.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
• Kepler’s first law states that planetary
orbits are ellipses with the sun at one
focus.
• The second law states that planets
move faster in their orbits when they
are closer to the sun.
• The third law relates the distance of a
planet from the sun to the time the
planet takes to go once around its
orbit.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Galileo
• He significantly improved the newly
invented telescope and used it to view
celestial objects.
• He observed the moons Io, Europa,
Callisto, and Ganymede orbiting Jupiter.
Today, these moons are known as the
Galilean satellites.
• Galileo’s observations showed that Earth
was not the only object that could be
orbited. Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
• This gave support to the heliocentric
model.
• Galileo also observed that Venus went
through phases similar to the phases
of Earth’s moon.
• These phases result from changes in
the direction that sunlight strikes Venus
as Venus orbits the sun.
Copyright © Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 Historical Models of the Solar System
Thank you!

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Historical models of the solar system Lesson 3 PPT.pptx

  • 1. Unit 2 : The Solar System Lesson 1 Historical Models of the Solar System Ms. Alia Ibrahim Copyright © Houghton Mifflin Harcourt Publishing Company Science
  • 2. What Is the Center of the Solar System? Copyright © Houghton Mifflin Harcourt Publishing Company What is the solar system? • The solar system is the sun and all of the bodies that orbit the sun. • Our current model of the solar system is the sun-centered, or heliocentric, model. • In the heliocentric model, Earth and the other planets orbit the sun. Unit 2 Lesson 1 Historical Models of the Solar System
  • 3. What is the solar system? • The earliest models of the solar system assumed that Earth was at the center, with the sun, moon, and planets circling it. These are the Geocentric models • The heliocentric model was not generally accepted until the work of Copernicus and Kepler in the late 16th to early 17th centuries. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 4. Aristotle – Geocentric model • The Greek philosopher Aristotle was among the first thinkers to propose this model. • His model placed the moon, sun, planets, and stars on a series of circles that surrounded Earth. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 5. • This apparent shift in the position of an object when viewed from different locations is known as parallax. • In fact, the stars are so far away that parallax cannot be seen with the unaided eye. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 6. Aristarchus – Heliocentric model • Aristarchus, a Greek astronomer and mathematician, is reported to have proposed a heliocentric model of the solar system. • His model, however, was not widely accepted at the time. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 7. Ptolemy – Geocentric model • Ptolemy was an astronomer, geographer, and mathematician who lived in Alexandria, Egypt. • He developed a detailed geocentric model that was used by astronomers for the next 14 centuries. • In Ptolemy’s model, the planets moved on small circles that in turn moved on larger circles. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 8. • Ptolemy’s “wheels-on-wheels” system fit observations better than any model that had come before. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 9. Copernicus – Heliocentric model • The Polish astronomer Nicolaus Copernicus felt that Ptolemy’s model of the solar system was too complicated. • He knew about Aristarchus’s ideas when he developed the first detailed heliocentric model of the solar system. • Copernicus adopted Ptolemy’s idea that planetary paths should be perfect circles. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 10. • Like Ptolemy, Copernicus used a “wheels-on-wheels” model. • Copernicus’s model is generally seen as the first step in the development of modern models of the solar system. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 11. Kepler • Johannes Kepler was a German mathematician and astronomer. • After careful observation and analysis, he realized that planetary orbits were not circular but were more like ellipses. • He formulated three principles, which are today known as Kepler’s laws. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 12. • Kepler’s first law states that planetary orbits are ellipses with the sun at one focus. • The second law states that planets move faster in their orbits when they are closer to the sun. • The third law relates the distance of a planet from the sun to the time the planet takes to go once around its orbit. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 13. Galileo • He significantly improved the newly invented telescope and used it to view celestial objects. • He observed the moons Io, Europa, Callisto, and Ganymede orbiting Jupiter. Today, these moons are known as the Galilean satellites. • Galileo’s observations showed that Earth was not the only object that could be orbited. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System
  • 14. • This gave support to the heliocentric model. • Galileo also observed that Venus went through phases similar to the phases of Earth’s moon. • These phases result from changes in the direction that sunlight strikes Venus as Venus orbits the sun. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 Historical Models of the Solar System