He was a Polish astronomer in the XV and XVI century. He was born in 1473 in Torun and he died in 1543 when he was 70 years old.

Similar documents
cosmogony geocentric heliocentric How the Greeks modeled the heavens

Directions: Read each slide

Lecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo

Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion

Chapter 02 The Rise of Astronomy

Earth Science, 13e Tarbuck & Lutgens

Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

Module 3: Astronomy The Universe Topic 6 Content: The Age of Astronomy Presentation Notes

History of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period

Competing Models. The Ptolemaic system (Geocentric) The Copernican system (Heliocentric)

Earth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

Models of the Solar System. The Development of Understanding from Ancient Greece to Isaac Newton

Chapter 2 The Copernican Revolution

2.4 The Birth of Modern Astronomy

The Scientific Method

Chapter 1 The Copernican Revolution

The History of Astronomy. Theories, People, and Discoveries of the Past

Ancient Cosmology: A Flat Earth. Alexandria

Inventors and Scientists: Nicolaus Copernicus

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle

Gravitation and the Waltz of the Planets

Gravitation and the Waltz of the Planets. Chapter Four

The Scientific Revolution

Today. Review. Momentum and Force Consider the rate of change of momentum. What is Momentum?

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky.

First MIDTERM Exam: Mon, Sep. 22, covering chapters tutorials (review later today).

Introduction To Modern Astronomy II

Gravitation and the Motion of the Planets

January 19, notes.notebook. Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

Early Models of the Universe. How we explained those big shiny lights in the sky

Lecture 2 : Early Cosmology

Announcements. Topics To Be Covered in this Lecture

Learning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?

Planets & The Origin of Science

DeAnza College Winter First Midterm Exam MAKE ALL MARKS DARK AND COMPLETE.

The History of Astronomy. Please pick up your assigned transmitter.

PHYS 160 Astronomy Test #1 Name Answer Key Test Version A


History of Astronomy - Part I. Ancient Astronomy. Ancient Greece. Astronomy is a science that has truly taken shape only in the last couple centuries

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios

Ptolemy (125 A.D.) Ptolemy s Model. Ptolemy s Equant. Ptolemy s Model. Copernicus Model. Copernicus ( )

Was Ptolemy Pstupid?

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric

ASTRO 6570 Lecture 1

This Week... Week 3: Chapter 3 The Science of Astronomy. 3.1 The Ancient Roots of Science. How do humans employ scientific thinking?

The History of Astronomy

History of Astronomy. Historical People and Theories

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets) Models of the Universe:

ASTR 2310: Chapter 2

Introduction To Modern Astronomy I

Models of the Solar System, Gravitation and the motion of the Planets A.K.A DEAD WHITE GUYS WEEK! 1/28/14

How Kepler discovered his laws

1. The Moon appears larger when it rises than when it is high in the sky because

In so many and such important. ways, then, do the planets bear witness to the earth's mobility. Nicholas Copernicus

If Earth had no tilt, what else would happen?

Benefit of astronomy to ancient cultures

Astronomy- The Original Science

The Puzzle of Planetary Motion versus

Ch. 22 Origin of Modern Astronomy Pretest

Copernican Revolution. ~1500 to ~1700

What was once so mysterious about planetary motion in our sky? We see apparent retrograde motion when we pass by a planet

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Motions of the Planets ASTR 2110 Sarazin

Scientific Revolution

Origin of Modern Astronomy Chapter 21

Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes

Contents: -Information/Research Packet. - Jumbled Image packet. - Comic book cover page. -Comic book pages. -Example finished comic

Copernican Astronomy. Nicolaus gets the ball rolling

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion

Chapter 2 The Science of Life in the Universe

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified

Monday, October 3, 2011

The History and Philosophy of Astronomy

ASTR 200 Reminder Center section = 'no laptop' zone

Things to do today. Terminal, Astronomy is Fun. Lecture 24 The Science of Astronomy. Scientific Thinking. After this lecture, please pick up:

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.

Ast ch 4-5 practice Test Multiple Choice

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that

You should have finished reading Chapter 3, and started on chapter 4 for next week.

The Birth of Astronomy. Lecture 3 1/24/2018

Lecture 4: Kepler and Galileo. Astronomy 111 Wednesday September 6, 2017

EXAM #2. ANSWERS ASTR , Spring 2008

The following notes roughly correspond to Section 2.4 and Chapter 3 of the text by Bennett. This note focuses on the details of the transition for a

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Goals of the course. What will we cover? How do we do this?

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

THE SUN AND THE SOLAR SYSTEM

Astro 210 Lecture 6 Jan 29, 2018

EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY

1 Astronomy: The Original Science

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that

Copernican Revolution. Motions of the sky. Motions of the sky. Copernican Revolution: questions on reading assignment

The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley. Monday, October 3, 2011

Astronomy 1143 Quiz 1 Review

The Scientific Revolution

Transcription:

Ptolomeo He lived in Rome around 100 AC, where he developed his model of the solar system which had a very important impact on the science because it could explain the motions of heavenly bodies and it helped for the understanding of the structure of the solar system. His model also assumed that the Earth was the center of the entire universe and that each planet was moved on a small sphere or circle, called an epicycle, that was moved on a larger sphere or circle, called a deferent. He also included in his hypothesis that the Earth didn t participate in any movement and that the Universe had a spherical form and a circular trajectory.

He was a Polish astronomer in the XV and XVI century. He was born in 1473 in Torun and he died in 1543 when he was 70 years old.

In 1503 he settled in the Frombork s cathedral to better observe the night sky. After a hard observation of the motion of terrestrial bodies, he concluded that the Earth turned on its axis and the Earth and the others should turn around the sun. And also he discovered that the moon turned around the Earth and this is the difference between the day and the night.

1. The world (universe) is spherical. 2. The Earth is also spherical. 3. The motion of the celestial bodies is regular, circular and perpetual or by circular movements. 4. Circuralr motion was caused by the rotation of the Earth in 24 hours instead of the whole universe. 5. Annual movement of the sun caused by the traslation of the Earth around the sun. 6. Monthly movement of the moon around the Earth. 7. Planetary motion caused by the composition of the movements of the planets. The retrograde motion of the planets is only apparent and not a real movement. 8. The sky is huge compared to the magnitude of the Earth. 9. The order of celestial orbits, after critizicing the Ptolemaic astronomy assigned the planets, it gives the correct order of their distance from the sun.

In his comments he stablished his theory on 6 axioms, and published under the name of On the Revolutions of the Heavenly Spheres. Heliocentric theory was expanded and quickly emerged their theologians detractors. In 1616, the Catholic Church placed the work of Copérnico on its list of banned books. Copérnico s work was the basis for Galileo, Brahe and Kleper to put the foundation of modern astronomy.

WHO WAS HE? He was a German astronomer that developed some theories about how the planets rotate.

HIS THEORIES Kepler developed some laws about the rotation of planets, the Copernico s systems were based on that God couldn t create an imperfect thing. Kepler broke with this dogma when he proposed that orbits of the planets were eliptic.

KEPLER S LAWS FIRST LAW: Planets move in an eliptic trajectory and the Sun is in the focus of the elypse.

SECOND LAW: One line was drawn from the Sun to a planet. It covers equal areas and equal intervals of time(the closer to the Sun, the lower the speed.)

THIRD LAW The square of the orbital period of a planet is proportional to the cube of the semi major axis of its orbit.

Thank you for your attention If you have any question you can ask us. BY VICTOR AND MARIO