from the Romans and the Greeks to better understand the world around them.

Size: px
Start display at page:

Download "from the Romans and the Greeks to better understand the world around them."

Transcription

1 During the 14 th and 15 th centuries thinkers and scholars looked to ancient texts from the Romans and the Greeks to better understand the world around them. Astronomers looked back to texts from Aristotle ( B.C.) and Ptolemy (A.D ). This brought about a power struggle between those who followed Geocentric theory, which states that the earth is the center of the Universe and those who followed Heliocentric theory which places the sun at the center. Those that went with church dogma saw the beliefs set fourth by Aristotle in Greece and Ptolemy in Egypt as the way the Universe was arranged with the Earth being the center of all things. Geocentric thinking worked better for the church because the bible was written in such a way as to represent the earth of the center of all things. Those such as Galileo Galilei ( ) and Nicolaus Copernicus ( ) saw these ancient ideas represented in texts such as On The Heavens and Physics by Aristotle and Almagest by Ptolemy as flawed and untrue of the real Universe. Although mostly keeping out of the public eye for fear of execution by the Church, both Galileo and Copernicus spent the majority of their lives disproving the church dogma as well as Hellenistic astronomical thinking. There work both led to a new age in Astronomy and helped to spark the sea of ideas both new and old that were so prominent during this time period. Why choose These Documents? I chose the documents of Galileo and Copernicus mostly because of my pure interest of the topic. I have always been curious about the Universe and often I can be found out gazing at the stars through my telescope. However, that is not the only reason why I chose these documents. It occurred to me that throughout the Renaissance scholars

2 were rediscovering documents from ancient societies and were using them to further advance their culture at the present. When reading these two documents I realized that in this case documents from Ptolemy and Aristotle concerning the Universe were completely wrong and the people of the Renaissance were using them despite the availability of better theories. Aristotle and Ptolemy s views were genius for their time period but were now outdated. Philosophy represented in the document on Copernicus almost completely debunked the philosophies of Aristotle concerning the Universe. After his death it was the science of Galileo that helped to strengthen and prove Copernican theory even more. Unfortunately, because of the great deal of power the Catholic Church had over Europe, both the philosophy and the science were repressed or dejected. Most Universities taught the Aristotelian model of the Universe and had been for centuries. The whole of Europe believed that Aristotle was correct; after all they had been taught his theory for over 4 centuries. In a time of great advancement of society and in logical thought the correct theories about our solar system and the Universe were kept from people. Perhaps during the Renaissance people were so obsessed with the past that they thought scientists and philosophers from then were smarter than the present day scientists and philosophers. Perhaps they just feared change of something that had been a staple in European higher education. Most likely, they probably feared that a new theory would somehow disprove the existence of God that was so key in Aristotle and Ptolemy s works, helping to prove the legitimacy of the bible. In any case Copernicus and Galileo were way ahead of their time when it came to philosophy and science. These documents help to show just how genius they were and how despite the church they published their works so that others could test them and see that they were indeed correct.

3 Documents Similarities and Differences: The documents represented in the Biblobase course pack by Copernicus and Galileo are similar but are also very different. Both documents work together over two centuries to prove the Copernican theory. This was of course done in spite of earlier works by Ptolemy and Aristotle who combine to form Ptolemaic theory. Copernicus s document focuses mainly on the philosophy and ideas of the universe and does not include any of the science. This is both because we wanted to put the science in a more complete later work but also that with the math the church might see the idea as more than a hypothesis and keep Copernicus from continuing his work. Galileo s document contained more science and went a step further to include sketches. Although discovering moons on a distant planet may not seem to have anything to do with a theory that puts the sun at the center of our solar system, in fact this discovery helps to prove that it is unlikely that we have a earth centered universe. If moons of a different planet travel around that planet that means those bodies don t rotate just around the earth and would debunk Aristotle s view of a perfect universe. It is no wonder that because Galileo went this extra step to show the science and diagrams that during his lifetime he was threatened with death unless he recanted his findings. These two documents on the outside appear to be about separate topics but in fact were a compliment of each other to help prove to doubters that the Ptolemaic view of the Universe was outdated and was time to switch to Copernican thinking.

4 Ptolemaic Philosophy: The Ptolemaic system is a view of the heavens based largely on the work of Aristotle and the follow up work on Aristotelian theory by Ptolemy. Aristotle argued that the universe was ordered and the heavens fell into two categories, Earthly region and the Heavens with the earth being the center of the cosmos. The Earthly Region consisted of Earth, fire, water, and air. In his view none of these elements existed in the heavenly region. Outside the Earthly Region there was a 5 th element which he called Aether in which encompassed all else in space. Each of these five elements throughout each region occupied a certain sphere in the universe and each elements natural place in the universe was within these spheres. For example the earth is heaviest and is the center of the universe so it falls into the first sphere, where as water and air are lighter so they surround the first sphere. In the Heavenly sphere the laws of the Earthly Region did not apply. Going by brightness, Aristotle thought that in this sphere from the earth outward the heavenly bodies followed this order: Moon, Mercury, Venus, Sun, Mars, Jupiter, Fixed Stars. After the fixed stars Aristotle assumed that god was running this system and that space was finite and after the fixed stars and god the universe ended. During this time period Aristotle s thinking was genius. However, there were several problems that this basic theory could not explain. For example, Planets such as Mars and Venus appeared in different parts of the sky at different times during the year. This was of course due to the fact that each planet rotates around the sun on a different plane, but this was not known during this time period. Many of the planets would also be seen to be traveling in retrograde orbits which is caused by the earths rotation which is why the sun rises in the East and Sets in the west. Aristotle believed this was because the

5 sun orbited the earth and refused to believe that the earth could spin that fast and have the spheres stay in tact. This however caused a problem because at different times of the year the planets would appear to travel in different directions across the sky and his theory could not explain these phenomena. Ptolemy recognized these problems and worked to discover ways to maintain Aristotle s geocentric theory while changing it so as to adapt to these problems. He thought that the best way to prove Aristotle correct was through mathematics so in his book Almagest (142 A.D) Ptolemy put fourth three mathematical theories to answer the questions raised Aristotle s philosophy. He called these three constructions The Eccentric, The Epicycle, and The Equant. In all of these equations, most of which are very hard to understand unless you are a mathematician, the earth is slightly placed off center in order to make the mathematics of planetary rotation and retrograde motion work. This meant that the earth wasn t exactly the center of the universe; however the amount of displacement was so minimal that the church let it go because it still put earth as the closest heavenly body to center and thus the most important to god. Plus, such a slight move was alright as long as the mathematics could work out so people would stop questioning the theory. This theory hit the Christian West around 1200 C.E. and was immediately accepted by the church and universities of the day. Copernican Philosophy: Copernicus was not the first philosopher to view the sun as the center of our solar system. The first to set the theory in motion was Aristarchus of Samos who between 310 and 320 B.C.E. he proposed a sun centered universe. In 200 B.C.E. Archimedes relayed his thinking about a heliocentric system in his book Sand Reckoner, recognizing the

6 legitimacy of Aristarchus of Samos. Throughout the middle ages these theories continued to hang around but were never taken seriously, they were just theories and accompanied no mathematic proof. The Ptolemaic theory on the other hand had the equations of Ptolemy to help prove their legitimacy. It was not until Copernicus that these theories were taken seriously and researched further. During the 15 th century there were problems that began to arise that only the Astronomers could fix. For example, the calendar was way off due to miscalculations in the ancient Greek model. Also, Events such as eclipses of the moon and the sun still could not be explained and although they appeared to have a pattern were still being explained as random in the old model. So during the 15 th century interest in Astronomy rose drastically. The Humanist Georg Peurbach ( ) started to read over texts by Aristotle and Ptolemy to fix any mistakes they might encounter. Although he maintained the overall accuracy of Aristotle, there were several ideas brought into question that peaked Copernicus s interest during his college years at the University of Cracow. In 1543, the year of his death, Copernicus published De Revolutionibus Orbium Coelestium which was published in Nuremberg. In this he launched his idea of a heliocentric solar system in what he called a mathematical hypothesis. This theory easily explained the retrograde movements of the planets without the need of an off center earth as in Ptolemy s equations. However, thinkers of the day immediately rejected the fact that the earth was not at the center. The scientists were very impressed by the math and the over all work and some even created a hybrid Copernican and Ptolemaic view that used Copernican math within the geocentric system. This was first done by Erasmus Reinhold in his Prutenic Tables published in The first major

7 scientist to completely accept his theories was Thomas Digges who published his own book in 1576 titled A Perfit Description of the Coelestiall orbes. Unlike Copernicus, Digges equipped his text with diagrams and illustrations to help further show the legitimacy of the work. During the late 1500 s Copernicus was beginning to have some followers but was slow because the physics to prove his theory would not be invented for another century and a half. It took discoveries by Kepler and Galileo with the aid of telescopes to help bring his theory to the forefront of astronomical thought. Galileo Published Sidereus Nuncius in 1610 and Dialogue Concerning the Two Chief World Systems in Throughout these texts Galileo used his telescope to discover the four largest moons of Jupiter which he named after members of the Medici family. He also brought about the idea that perhaps the bible did allow for a heliocentric universe and that it was just being misinterpreted. In all his texts he challenged a great deal the theories set fourth by Aristotle and with each discovery he made, especially the moons which proved there were heavenly bodies that rotated around bodies other than the earth, Galileo slowly ate away at the false science surrounding the universe opening up the way for scientists to discover the physics that would prove Copernicus correct. These documents are very important to not only the history of the sciences but of culture and society as well. These documents along with other documents by Copernicus and Galileo changed scientific theory forever and are considered among the most important astronomic theorists and discoverers of all time. They also helped to change society. The church and the Universities were stuck teaching the wrong ideas for centuries and refused to change their stand despite the obvious conclusions set fourth in

8 these documents. Over time these theories helped to change the way Universities taught and even changed the stance of the church, which was perhaps the most powerful establishment in Europe during the 14 th and 15 th centuries. Although they were not immediately accepted, together their theories and discoveries changed the world..

Chapter 3 The Science of Astronomy

Chapter 3 The Science of Astronomy Chapter 3 The Science of Astronomy Days of the week were named for Sun, Moon, and visible planets. What did ancient civilizations achieve in astronomy? Daily timekeeping Tracking the seasons and calendar

More information

From Aristotle to Newton

From Aristotle to Newton From Aristotle to Newton The history of the Solar System (and the universe to some extent) from ancient Greek times through to the beginnings of modern physics. The Geocentric Model Ancient Greek astronomers

More information

The Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following:

The Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following: Unit 4 The Solar System Chapter 7 ~ The History of the Solar System o Section 1 ~ The Formation of the Solar System o Section 2 ~ Observing the Solar System Chapter 8 ~ The Parts the Solar System o Section

More information

Chapter 25.1: Models of our Solar System

Chapter 25.1: Models of our Solar System Chapter 25.1: Models of our Solar System Objectives: Compare & Contrast geocentric and heliocentric models of the solar sytem. Describe the orbits of planets explain how gravity and inertia keep the planets

More information

WORLD HISTORY: SCIENTIFIC REVOLUTION AND ENLIGHTENMENT. Jeopardy Version Watch out Alex Trebek

WORLD HISTORY: SCIENTIFIC REVOLUTION AND ENLIGHTENMENT. Jeopardy Version Watch out Alex Trebek WORLD HISTORY: SCIENTIFIC REVOLUTION AND ENLIGHTENMENT Jeopardy Version Watch out Alex Trebek Scientists Philosophes Enlightenment Spreads Terms Thnkers 100 100 100 100 100 200 200 200 200 200 300 300

More information

Astronomy 1140 Quiz 1 Review

Astronomy 1140 Quiz 1 Review Astronomy 1140 Quiz 1 Review Prof. Pradhan September 15, 2015 What is Science? 1. Explain the difference between astronomy and astrology. (a) Astrology: nonscience using zodiac sign to predict the future/personality

More information

Computer Animations of Ancient Greek and Arabic Planetary Models

Computer Animations of Ancient Greek and Arabic Planetary Models Computer Animations of Ancient Greek and Arabic Planetary Models Dennis Duke, Florida State University A new set of computer animations is available for those who teach the ancient models of planetary

More information

4. Discuss the information as a class (transparency key)

4. Discuss the information as a class (transparency key) Teacher: Sherry Tipps-Holder Grade: 8 Subject: World History/ Lesson designed for inclusion in unit on Scientific Revolution Essential Question: What were the major contributions/innovations of the who

More information

An Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science

An Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science An Introduction to Astronomy and Cosmology 1) Astronomy - an Observational Science Why study Astronomy 1 A fascinating subject in its own right. The origin and Evolution of the universe The Big Bang formation

More information

Study Guide due Friday, 1/29

Study Guide due Friday, 1/29 NAME: Astronomy Study Guide asteroid chromosphere comet corona ellipse Galilean moons VOCABULARY WORDS TO KNOW geocentric system meteor gravity meteorite greenhouse effect meteoroid heliocentric system

More information

Periods of Western Astronomy. Chapter 1. Prehistoric Astronomy. Prehistoric Astronomy. The Celestial Sphere. Stonehenge. History of Astronomy

Periods of Western Astronomy. Chapter 1. Prehistoric Astronomy. Prehistoric Astronomy. The Celestial Sphere. Stonehenge. History of Astronomy Periods of Western Astronomy Chapter 1 History of Astronomy Western astronomy divides into 4 periods Prehistoric (before 500 B.C.) Cyclical motions of Sun, Moon and stars observed Keeping time and determining

More information

AE554 Applied Orbital Mechanics. Hafta 1 Egemen Đmre

AE554 Applied Orbital Mechanics. Hafta 1 Egemen Đmre AE554 Applied Orbital Mechanics Hafta 1 Egemen Đmre A bit of history the beginning Astronomy: Science of heavens. (Ancient Greeks). Astronomy existed several thousand years BC Perfect universe (like circles

More information

The Solar System. I. Introduction. S. Gavin and S. P. Karrer Physics Department, Wayne State University, Detroit, MI, 48201 sean@physics.wayne.

The Solar System. I. Introduction. S. Gavin and S. P. Karrer Physics Department, Wayne State University, Detroit, MI, 48201 sean@physics.wayne. The Solar System S. Gavin and S. P. Karrer Physics Department, Wayne State University, Detroit, MI, 48201 sean@physics.wayne.edu I. Introduction As children we all learned that the Earth is one of many

More information

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015 Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015 Why are celestial motions and forces important? They explain the world around

More information

Introduction to the Solar System

Introduction to the Solar System Introduction to the Solar System Lesson Objectives Describe some early ideas about our solar system. Name the planets, and describe their motion around the Sun. Explain how the solar system formed. Introduction

More information

Solar System Formation

Solar System Formation Solar System Formation Background Information System: Many pieces that make up a whole Solar System: Anything that orbits the Sun Just like in the formation of of stars.. Gravity plays a major role. Gravitational

More information

1 SCIENCE AND NATURAL PHILOSOPHY BEFORE THE 17 TH CENTURY

1 SCIENCE AND NATURAL PHILOSOPHY BEFORE THE 17 TH CENTURY 1 SCIENCE AND NATURAL PHILOSOPHY BEFORE THE 17 TH CENTURY FOR TEACHERS Lesson Title: Science and Natural Philosophy Before the Seventeenth Century Area of Learning: chronology, states of affairs Aims.

More information

Scale of the Solar System. Sizes and Distances: How Big is Big? Sizes and Distances: How Big is Big? (Cont.)

Scale of the Solar System. Sizes and Distances: How Big is Big? Sizes and Distances: How Big is Big? (Cont.) Scale of the Solar System Scale of the Universe How big is Earth compared to our solar system? How far away are the stars? How big is the Milky Way Galaxy? How big is the Universe? How do our lifetimes

More information

Science and Religion

Science and Religion 1 Science and Religion Scripture: Colossians 1:15-20 By Pastor John H. Noordhof Williamsburg Christian Reformed Church October 21, 2012 Morning Service People of God: Today we will deal with the troubling

More information

http://eprints.gla.ac.uk/58982/ Deposited on: 15 th February 2012

http://eprints.gla.ac.uk/58982/ Deposited on: 15 th February 2012 McNeill, F. (2012) Counterblast: a Copernican correction for community sentences? The Howard Journal of Criminal Justice, 51 (1). pp. 94-99. ISSN 0265-5527 http://eprints.gla.ac.uk/58982/ Deposited on:

More information

ELEMENTS OF PHYSICS MOTION, FORCE, AND GRAVITY

ELEMENTS OF PHYSICS MOTION, FORCE, AND GRAVITY 1 Pre-Test Directions: This will help you discover what you know about the subject of motion before you begin this lesson. Answer the following true or false. 1. Aristotle believed that all objects fell

More information

astronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

astronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were increased,

More information

Galileo Galilei. Introduction

Galileo Galilei. Introduction Galileo Galilei Introduction Galileo Galilei (1564 1642) was one of the most significant figures of the Scientific Revolution. Galileo was involved in nearly all fields of natural philosophy, including

More information

Unit 11: Gravity & the Solar System

Unit 11: Gravity & the Solar System Unit 11: Gravity & the Solar System Inquiry Physics www.inquiryphysics.org Historical development Kepler s Laws Newton s Universal Gravitation Next 11: Gravity & the Solar System Historical development

More information

The Arts and Architecture

The Arts and Architecture Lesson 4 The Legacy of Greece MAIN IDEAS Culture Greek art and architecture introduced new styles and concepts that set standards for generations of artists around the world. Culture The Greek love of

More information

Lab 6: Kepler's Laws. Introduction. Section 1: First Law

Lab 6: Kepler's Laws. Introduction. Section 1: First Law Lab 6: Kepler's Laws Purpose: to learn that orbit shapes are ellipses, gravity and orbital velocity are related, and force of gravity and orbital period are related. Materials: 2 thumbtacks, 1 pencil,

More information

Isaac Newton & the Newtonian Age

Isaac Newton & the Newtonian Age Newton By William Blake ~1800 Ch 5 pg. 91-95 ++ Lecture 3 Isaac Newton & the Newtonian Age If I have ever made any valuable discoveries, it has been owing more to patient attention, than to any other talent.

More information

The sun and planets. On this picture, the sizes of the sun and 8 planets are to scale. Their positions relative to each other are not to scale.

The sun and planets. On this picture, the sizes of the sun and 8 planets are to scale. Their positions relative to each other are not to scale. The solar system The solar system consists of our sun and its eight planets. The word solar means to do with the sun. The solar system formed 4½ billion years ago, when the universe was about two-thirds

More information

CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS

CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS INTRODUCTION CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS This is a scientific presentation to provide you with knowledge you can use to understand the sky above in relation to the earth. Before

More information

Newton s derivation of Kepler s laws (outline)

Newton s derivation of Kepler s laws (outline) Newton s derivation of Kepler s laws (outline) 1. Brief history. The first known proposal for a heliocentric solar system is due to Aristarchus of Samos (ancient Greece, c. 270 BC). Following a long period

More information

Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?

Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? Solar System 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? A) Earth B) Sun C) Moon D) Polaris 2. Which object orbits Earth in both the Earth-centered

More information

Physics Section 3.2 Free Fall

Physics Section 3.2 Free Fall Physics Section 3.2 Free Fall Aristotle Aristotle taught that the substances making up the Earth were different from the substance making up the heavens. He also taught that dynamics (the branch of physics

More information

EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1

EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 Instructor: L. M. Khandro EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 1. An arc second is a measure of a. time interval between oscillations of a standard clock b. time

More information

Inductive Reasoning Page 1 of 7. Inductive Reasoning

Inductive Reasoning Page 1 of 7. Inductive Reasoning Inductive Reasoning Page 1 of 7 Inductive Reasoning We learned that valid deductive thinking begins with at least one universal premise and leads to a conclusion that is believed to be contained in the

More information

The following questions refer to Chapter 19, (PAGES 259 278 IN YOUR MANUAL, 7 th ed.)

The following questions refer to Chapter 19, (PAGES 259 278 IN YOUR MANUAL, 7 th ed.) GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Locating the Planets (Chapter 19) and the Moon and Sun (Chapter 21) For this assignment you will require: a calculator, colored pencils, a metric

More information

Lecture 13. Gravity in the Solar System

Lecture 13. Gravity in the Solar System Lecture 13 Gravity in the Solar System Guiding Questions 1. How was the heliocentric model established? What are monumental steps in the history of the heliocentric model? 2. How do Kepler s three laws

More information

Exercise: Estimating the Mass of Jupiter Difficulty: Medium

Exercise: Estimating the Mass of Jupiter Difficulty: Medium Exercise: Estimating the Mass of Jupiter Difficulty: Medium OBJECTIVE The July / August observing notes for 010 state that Jupiter rises at dusk. The great planet is now starting its grand showing for

More information

1.1 A Modern View of the Universe" Our goals for learning: What is our place in the universe?"

1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe? Chapter 1 Our Place in the Universe 1.1 A Modern View of the Universe What is our place in the universe? What is our place in the universe? How did we come to be? How can we know what the universe was

More information

Please be sure to save a copy of this activity to your computer!

Please be sure to save a copy of this activity to your computer! Thank you for your purchase Please be sure to save a copy of this activity to your computer! This activity is copyrighted by AIMS Education Foundation. All rights reserved. No part of this work may be

More information

Are Those Sunspots Really on the Sun?

Are Those Sunspots Really on the Sun? Are Those Sunspots Really on the Sun? Summary of Activity: Students will acquire solar images (or draw sunspots), and record coordinates of sunspots. They will calculate and plot their apparent movement

More information

Activity 3: Observing the Moon

Activity 3: Observing the Moon Activity 3: Observing the Moon Print Name: Signature: 1.) KEY. 2.). 3.). 4.). Activity: Since the dawn of time, our closest neighbor the moon has fascinated humans. In this activity we will explore the

More information

CELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault

CELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault CELESTIAL MOTIONS Stars appear to move counterclockwise on the surface of a huge sphere the Starry Vault, in their daily motions about Earth Polaris remains stationary. In Charlottesville we see Polaris

More information

Science Benchmark: 06 : 01 Standard 01: THE MYSTICAL MOON axis of rotation,

Science Benchmark: 06 : 01 Standard 01: THE MYSTICAL MOON axis of rotation, Science Benchmark: 06 : 01 The appearance of the lighted portion of the moon changes in a predictable cycle as a result of the relative positions of Earth, the moon, and the sun. Standard 01: Students

More information

Night Sky III Planetary Motion Lunar Phases

Night Sky III Planetary Motion Lunar Phases Night Sky III Planetary Motion Lunar Phases Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day Everything has a natural explanation. The moon is not a god, but

More information

Explain the Big Bang Theory and give two pieces of evidence which support it.

Explain the Big Bang Theory and give two pieces of evidence which support it. Name: Key OBJECTIVES Correctly define: asteroid, celestial object, comet, constellation, Doppler effect, eccentricity, eclipse, ellipse, focus, Foucault Pendulum, galaxy, geocentric model, heliocentric

More information

Newton s Law of Gravity

Newton s Law of Gravity Gravitational Potential Energy On Earth, depends on: object s mass (m) strength of gravity (g) distance object could potentially fall Gravitational Potential Energy In space, an object or gas cloud has

More information

5 DARWIN, EVOLUTION & FAITH 850L

5 DARWIN, EVOLUTION & FAITH 850L 5 DARWIN, EVOLUTION & FAITH 850L DARWIN, EVOLUTION & FAITH By John F. Haught, adapted by Newsela Nothing in modern science is more challenging to religious believers than the theory of evolution. For more

More information

Study Guide: Solar System

Study Guide: Solar System Study Guide: Solar System 1. How many planets are there in the solar system? 2. What is the correct order of all the planets in the solar system? 3. Where can a comet be located in the solar system? 4.

More information

The University of Texas at Austin. Gravity and Orbits

The University of Texas at Austin. Gravity and Orbits UTeach Outreach The University of Texas at Austin Gravity and Orbits Time of Lesson: 60-75 minutes Content Standards Addressed in Lesson: TEKS6.11B understand that gravity is the force that governs the

More information

XXX Background information

XXX Background information XXX Background information The solar system Our solar system is made up of the Sun, the planets, the dwarf planets, moons, asteroids and comets. The Sun is the star around which everything orbits. There

More information

Celestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun)

Celestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun) Lecture 3: Motions of the and Moon ecliptic (path of ) ecliptic (path of ) The 23.5 degree tilt of Earth s spin axis relative to its orbital axis around the causes the seasons Celestial Sphere Celestial

More information

1 Branches of Earth Science

1 Branches of Earth Science CHAPTER 1 1 Branches of Earth Science SECTION The World of Earth Science BEFORE YOU READ After you read this section, you should be able to answer these questions: What are the four major branches of Earth

More information

Newton s Law of Universal Gravitation

Newton s Law of Universal Gravitation Newton s Law of Universal Gravitation The greatest moments in science are when two phenomena that were considered completely separate suddenly are seen as just two different versions of the same thing.

More information

Class 2 Solar System Characteristics Formation Exosolar Planets

Class 2 Solar System Characteristics Formation Exosolar Planets Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System

More information

Religion and Science

Religion and Science Religion and Science Glossary Cosmology the study of the origins of the universe How did the world come into existence? Theory one Aristotle Taught that the universe has always existed and would always

More information

Motions of Earth, Moon, and Sun

Motions of Earth, Moon, and Sun Motions of Earth, Moon, and Sun Apparent Motions of Celestial Objects An apparent motion is a motion that an object appears to make. Apparent motions can be real or illusions. When you see a person spinning

More information

Unit 8 Lesson 2 Gravity and the Solar System

Unit 8 Lesson 2 Gravity and the Solar System Unit 8 Lesson 2 Gravity and the Solar System Gravity What is gravity? Gravity is a force of attraction between objects that is due to their masses and the distances between them. Every object in the universe

More information

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton Halliday, Resnick & Walker Chapter 13 Gravitation Physics 1A PHYS1121 Professor Michael Burton II_A2: Planetary Orbits in the Solar System + Galaxy Interactions (You Tube) 21 seconds 13-1 Newton's Law

More information

Exploration of the Solar System

Exploration of the Solar System Exploration of the Solar System I. Phases of the Moon all about perspective. In this section you will use WWT to explore how the moon appears to change phases from our vantage point on Earth over the course

More information

The Holy Office v Galileo Galilei: BASIC INFO

The Holy Office v Galileo Galilei: BASIC INFO The Holy Office v Galileo Galilei: BASIC INFO STIPULATED FACTS (BACKGROUND) Born in 1564 in Italy, Galileo Galilei became a brilliant scientist and lecturer. He made several inventions, including the telescope.

More information

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF FIRST GRADE UNIVERSE WEEK 1. PRE: Describing the Universe. LAB: Comparing and contrasting bodies that reflect light. POST: Exploring

More information

Chapter 5: Circular Motion, the Planets, and Gravity

Chapter 5: Circular Motion, the Planets, and Gravity Chapter 5: Circular Motion, the Planets, and Gravity 1. Earth s gravity attracts a person with a force of 120 lbs. The force with which the Earth is attracted towards the person is A. Zero. B. Small but

More information

Today FIRST HOMEWORK DUE NEXT TIME. Seasons/Precession Recap. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy

Today FIRST HOMEWORK DUE NEXT TIME. Seasons/Precession Recap. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy Today FIRST HOMEWORK DUE NEXT TIME Seasons/Precession Recap Phases of the Moon Eclipses Lunar, Solar Ancient Astronomy How do we mark the progression of the seasons? We define four special points: summer

More information

Understanding the Cosmos: Changing Models of the Solar System and the Universe

Understanding the Cosmos: Changing Models of the Solar System and the Universe teacher s guide primary source set Understanding the Cosmos: Changing Models of the Solar System and the Universe For millennia, humans have gazed at the sky and tried to make sense of what they saw there.

More information

THE SOLAR SYSTEM - EXERCISES 1

THE SOLAR SYSTEM - EXERCISES 1 THE SOLAR SYSTEM - EXERCISES 1 THE SUN AND THE SOLAR SYSTEM Name the planets in their order from the sun. 1 2 3 4 5 6 7 8 The asteroid belt is between and Which planet has the most moons? About how many?

More information

Background Biology and Biochemistry Notes A

Background Biology and Biochemistry Notes A Background Biology and Biochemistry Notes A Vocabulary dependent variable evidence experiment hypothesis independent variable model observation prediction science scientific investigation scientific law

More information

5- Minute Refresher: Daily Observable Patterns in the Sky

5- Minute Refresher: Daily Observable Patterns in the Sky 5- Minute Refresher: Daily Observable Patterns in the Sky Key Ideas Daily Observable Patterns in the Sky include the occurrence of day and night, the appearance of the moon, the location of shadows and

More information

Today. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME

Today. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME Today Solstices & Equinoxes Precession Phases of the Moon Eclipses Lunar, Solar Ancient Astronomy FIRST HOMEWORK DUE NEXT TIME The Reason for Seasons Hypothesis check: How would seasons in the northern

More information

The Celestial Sphere. Questions for Today. The Celestial Sphere 1/18/10

The Celestial Sphere. Questions for Today. The Celestial Sphere 1/18/10 Lecture 3: Constellations and the Distances to the Stars Astro 2010 Prof. Tom Megeath Questions for Today How do the stars move in the sky? What causes the phases of the moon? What causes the seasons?

More information

Climate Discovery Teacher s Guide

Climate Discovery Teacher s Guide Climate Discovery eacher s Guide Sunspots and Climate Unit:Little Ice Age Lesson: 7 Materials & Preparation ime: Preparation: 10 min eaching: 60 min Materials for the eacher: Overhead projector ransparencies

More information

1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.

1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d. Chapter 1 1-1. How long does it take the Earth to orbit the Sun? a.) one sidereal day b.) one month c.) one year X d.) one hour 1-2. What is the name given to the path of the Sun as seen from Earth? a.)

More information

KINDERGARTEN 1 WEEK LESSON PLANS AND ACTIVITIES

KINDERGARTEN 1 WEEK LESSON PLANS AND ACTIVITIES KINDERGARTEN 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF KINDERGARTEN UNIVERSE WEEK 1. PRE: Discovering misconceptions of the Universe. LAB: Comparing size and distances in space. POST:

More information

Related Standards and Background Information

Related Standards and Background Information Related Standards and Background Information Earth Patterns, Cycles and Changes This strand focuses on student understanding of patterns in nature, natural cycles, and changes that occur both quickly and

More information

The Scientific Method

The Scientific Method Chapter 2 The Scientific Method In the history of philosophical ideation, scientific discoveries, and engineering inventions, it has almost never happened that a single person (or a single group of people)

More information

Aristotelian Physics. Aristotle's physics agrees with most people's common sense, but modern scientists discard it. So what went wrong?

Aristotelian Physics. Aristotle's physics agrees with most people's common sense, but modern scientists discard it. So what went wrong? Aristotelian Physics Aristotle's physics agrees with most people's common sense, but modern scientists discard it. So what went wrong? Here's what Aristotle said: Aristotelian Physics Aristotle s classification

More information

Planets and Dwarf Planets by Shauna Hutton

Planets and Dwarf Planets by Shauna Hutton Name: Wow! Technology has improved so well in the last several years that we keep finding more and more objects in our solar system! Because of this, scientists have had to come up with new categories

More information

Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti

Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking

More information

Newton s Law of Universal Gravitation

Newton s Law of Universal Gravitation 12.1 Newton s Law of Universal Gravitation SECTION Explain Kepler s laws. Describe Newton s law of universal gravitation. Apply Newton s law of universal gravitation quantitatively. KEY TERMS OUTCOMES

More information

The Earth, Sun, and Moon

The Earth, Sun, and Moon reflect The Sun and Moon are Earth s constant companions. We bask in the Sun s heat and light. It provides Earth s energy, and life could not exist without it. We rely on the Moon to light dark nights.

More information

SSWH3 THE STUDENT WILL EXAMINE THE POLITICAL, PHILOSOPHICAL, AND CULTURAL INTERACTION OF CLASSICAL MEDITERRANEAN SOCIETIES FROM 700 BCE TO 400 CE.

SSWH3 THE STUDENT WILL EXAMINE THE POLITICAL, PHILOSOPHICAL, AND CULTURAL INTERACTION OF CLASSICAL MEDITERRANEAN SOCIETIES FROM 700 BCE TO 400 CE. SSWH3 THE STUDENT WILL EXAMINE THE POLITICAL, PHILOSOPHICAL, AND CULTURAL INTERACTION OF CLASSICAL MEDITERRANEAN SOCIETIES FROM 700 BCE TO 400 CE. A. COMPARE THE ORIGINS AND STRUCTURE OF THE GREEK POLIS,

More information

Solar Matters II Teacher Page

Solar Matters II Teacher Page Solar Matters II Teacher Page Sun Misconceptions Student Objective understands why some common phrases about the Sun are incorrect can describe how the Earth s rotation affects how we perceive the Sun

More information

The Solar System. Olivia Paquette

The Solar System. Olivia Paquette The Solar System Olivia Paquette Table of Contents The Sun 1 Mercury 2,3 Venus 4,5 Earth 6,7 Mars 8,9 Jupiter 10,11 Saturn 12 Uranus 13 Neptune Pluto 14 15 Glossary. 16 The Sun Although it may seem like

More information

Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:

Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name: Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007 Name: Directions: Listed below are twenty (20) multiple-choice questions based on the material covered by the lectures this past week. Choose

More information

Plato. RAPHAEL: School of Athens. Center section

Plato. RAPHAEL: School of Athens. Center section Plato RAPHAEL: School of Athens. Center section Profile: Plato (c.427-347 B.C.E.) was born to an aristocratic family in Athens. As a young man Plato had political ambitions, but he became disillusioned

More information

Soul-Winning Commitment Day. Sunday School/ Small Group Lessons. Soul-Winning. Commitment Day

Soul-Winning Commitment Day. Sunday School/ Small Group Lessons. Soul-Winning. Commitment Day Sunday School/ Small Group Lessons Soul-Winning Commitment Day Purpose of Lesson: This guide is for the purpose of preparing older children through adult Sunday school members to understand the importance

More information

Activity 10 - Universal Time

Activity 10 - Universal Time Activity 10 - Universal Time Teacher s Guide Scientists use the Universal Time reference to talk about data that is taken around the globe. Universal Time is the time kept in the time zone centered on

More information

GRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter

GRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter IT S UNIVERSAL GRAVITY CONCEPTS Gravity is the universal force of attraction between all matter Weight is a measure of the gravitational force pulling objects toward Earth Objects seem weightless when

More information

Best of the Solar System

Best of the Solar System Best of the Solar System Topic Area: Solar system, planets and moons Purpose: Introduce students to planetary research and familiarize them with the planets and their features. Key Questions: What are

More information

A Study Guide for The Structure of Scientific Revolutions by Thomas Kuhn

A Study Guide for The Structure of Scientific Revolutions by Thomas Kuhn A Study Guide for The Structure of Scientific Revolutions by Thomas Kuhn In 1962, Thomas Kuhn wrote one of the most influential books of the last half of the twentieth century. He was inspired to write

More information

2 ISAAC NEWTON BIOGRAPHY 780L

2 ISAAC NEWTON BIOGRAPHY 780L 2 ISAAC NEWTON BIOGRAPHY 780L ISAAC NEWTON PHYSICS, GRAVITY & LAWS OF MOTION Born January 4, 1643 Lincolnshire, England Died March 31, 1727 London, England By Cynthia Stokes Brown, adapted by Newsela Sir

More information

Note S1: Eclipses & Predictions

Note S1: Eclipses & Predictions The Moon's Orbit The first part of this note gives reference information and definitions about eclipses [14], much of which would have been familiar to ancient Greek astronomers, though not necessarily

More information

Planets beyond the solar system

Planets beyond the solar system Planets beyond the solar system Review of our solar system Why search How to search Eclipses Motion of parent star Doppler Effect Extrasolar planet discoveries A star is 5 parsecs away, what is its parallax?

More information

Objectives After completing this section, you should be able to:

Objectives After completing this section, you should be able to: Chapter 5 Section 1 Lesson Angle Measure Objectives After completing this section, you should be able to: Use the most common conventions to position and measure angles on the plane. Demonstrate an understanding

More information

Adult cognition of large-scale geometric facts

Adult cognition of large-scale geometric facts Roberto Casati, David Mark, Ira Noveck Adult cognition of large-scale geometric facts Draft 4, April 1999 Project description Objectives 1. Adult cognition of large-scale geometric facts The primary objective

More information

Solar System. Trading Cards. Solar System Trading Cards, Jr. Edition. Learn more about the solar system on these Web sites:

Solar System. Trading Cards. Solar System Trading Cards, Jr. Edition. Learn more about the solar system on these Web sites: Solar System Trading Cards, Jr. Edition To use these cards: Print out onto card stock or heavy paper. Cut out and fold in half along dotted line; glue or tape each card together. FOLD National Aeronautics

More information

A long time ago, people looked

A long time ago, people looked Supercool Space Tools! By Linda Hermans-Killam A long time ago, people looked into the dark night sky and wondered about the stars, meteors, comets and planets they saw. The only tools they had to study

More information

The orbit of Halley s Comet

The orbit of Halley s Comet The orbit of Halley s Comet Given this information Orbital period = 76 yrs Aphelion distance = 35.3 AU Observed comet in 1682 and predicted return 1758 Questions: How close does HC approach the Sun? What

More information

Name Class Date. true

Name Class Date. true Exercises 131 The Falling Apple (page 233) 1 Describe the legend of Newton s discovery that gravity extends throughout the universe According to legend, Newton saw an apple fall from a tree and realized

More information

Astronomy Club of Asheville October 2015 Sky Events

Astronomy Club of Asheville October 2015 Sky Events October 2015 Sky Events The Planets this Month - page 2 Planet Highlights - page 10 Moon Phases - page 13 Orionid Meteor Shower Peaks Oct. 22 nd - page 14 Observe the Zodiacal Light - page 15 2 Bright

More information

Science Lesson Plan: Our Solar System: I Wonder? (I 1- D- R)

Science Lesson Plan: Our Solar System: I Wonder? (I 1- D- R) 1 P age Science Lesson Plan: Our Solar System: I Wonder? (I 1- D- R) Learning Outcomes (corresponding to science standards for grades K-2) 1. Generate curiosity to study and explore our surroundings. 2.

More information