chapter 3 – the solar system lesson 1. in a geocentric system, the planets and stars are thought...

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Observing the Solar System Chapter 3 – The Solar System Lesson 1

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Page 1: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Observing the Solar System

Chapter 3 – The Solar SystemLesson 1

Page 2: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Geocentric vs. Heliocentric Model

Page 3: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Earth at the Center In a geocentric system, the planets

and stars are thought to revolve around a stationary Earth.

Most early Greek astronomers believed the universe to be perfect, with Earth at the center.

The Greeks thought that Earth was inside a rotating dome they called the celestial sphere.

Page 4: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Ptolemy’s Model About A.D. 140, the Greek

astronomer Ptolemy further developed the geocentric model.

Even though the geocentric model was incorrect, it explained the motions observed in the sky fairly accurately.

Page 5: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Sun at the Center In a heliocentric system, Earth and

the other planets revolve around the sun.

The theory was not well received in ancient times because people could not accept the fact that Earth was not the center of the universe.

Page 6: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

The Copernican Revolution Copernicus was able to work out the

arrangements of the known planets and how they move around the sun.

Copernicus’s theory would eventually revolutionize the science of astronomy.

Page 7: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Galileo’s Evidence Galileo used the newly invented

telescope to make discoveries that supported the heliocentric model.

In 1610 he used a telescope to discover four moos revolving around Jupiter. The motions of these moons proved that not everything in the sky revolves around Earth.

Page 8: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Tycho Brahe’s Observations

In the late 1500’s, Tycho Brahe and his assistants made much more accurate observations with the use of a telescope because they were not invented yet.

Page 9: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Kepler’s Calculations Tycho Brahe died in 1601, so one of

his assistants – Kepler took over his observations.

Kepler eventually found that Mar’s orbit was a slightly flattened circle or elipse.

After years of detailed calculations, Kepler found that the orbit of each planet was an ellipse.

Page 10: Chapter 3 – The Solar System Lesson 1.  In a geocentric system, the planets and stars are thought to revolve around a stationary Earth.  Most early

Modern Discoveries Today we know that the solar system

consists of the sun, the planets and their moons and several kinds of smaller objects that revolve around the sun.

Galileo used a telescope to observe the solar system from Earth’s surface. Astronomers today still use telescopes located on Earth, but they have also placed telescopes in space to gain a better view of the universe beyond Earth.