Mav Mark 11/3/11 When electricity leaves a power plant is it AC or DC, and is it at high voltage or low voltage?

Slides:



Advertisements
Similar presentations
Ch. 2 The Copernican Revolution (Stonehenge, England)
Advertisements

Lesson 1: Models of the Solar System
Chapter 1: Origins of Modern Astronomy
The Origin of Modern Astronomy
Early Models of the Universe. Pythagoreans (500 B.C.) Believed the stars, planets, sun, and moon were attached to crystalline spheres which rotated around.
Geocentric Model Earth is center of our Solar System
The Solar System 6.E.1.2 Explain why Earth sustains life while other planets do not based on their properties (including types of surface,
Galileo, Tycho, and Kepler and Kepler. Galileo’s Experiments ( ) Galileo tried something new – doing experiments! Dropping balls to measure gravity.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 6.
Models of the Solar System *Early Models of the Solar System *Kepler’s Laws.
Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know.
CHAPTER 2: Gravitation and the Waltz of the Planets.
Intro to Astronomy Through the early history of civilization, people made observations about the night sky, sun, and moon. They tried to explain what they.
From the ancients to the moderns Nicholas Copernicus (1473–1543) Tycho Brahe (1546–1601) Johannes Kepler (1571–1630)
Geocentric vs. Heliocentric
Observing the Solar System Section Early Observations Greek Observations Saw star patterns in the sky travel together (Constellations)
Observing the Solar System
Observing the Solar System: A History
Observing the Solar System. Observers in Ancient Greece noticed that although the stars seemed to move, they stayed in the same position relative to one.
The Solar System Explorers. Ancient Greeks The ancient greeks noticed that the stars would move across the sky, but would stay in the same position relative.
Observing the Solar System Chap 16, Sec 1. Chap 16 Sec 1 Essential Questions 1. What are the geocentric and heliocentric systems? 2. How did Copernicus,
Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know.
History of Astronomy. Our Universe Earth is one of nine planets that orbit the sun The sun is one star in 100 billion stars that make up our galaxy- The.
Goals Explain how accurate observations led to Heliocentric model Explain retrograde motion Describe contributions of Copernicus, Tycho, Galileo, and.
Sun, Moon, Earth, How do they work together to help life survive? Our Solar System.
Questions What was the first idea of how the universe was structured?
Early Astronomers Tycho Brahe Galileo Galilei Johannes Kepler Nicholas Copernicus Edmund Halley Sir Isaac Newton.
Kepler’s Laws of Planetary Motion. Debate on Planet Motions Geocentric or Heliocentric Universe.
What is the difference between geocentric and heliocentric theories?
Early Astronomy Chapter 22, Section 1.
What is the difference between geocentric and heliocentric theories?
Chapter 3.1 – Observing the Solar System
Historical Models of our Solar System Miss Scillieri 6 th Grade.
Unit 1 Physics Detailed Study 3.1 Chapter 10: Astronomy.
Explaining the Universe. Pioneer and Voyager missions Pioneer 10 and 11 Voyager 1 and 2 Portrait of Solar System.
Astronomy- The Original Science
Observing the Solar System
Astronomy Chapter Astronomy People in ancient cultures used the seasonal cycles to determine when they should plant and harvest crops. They built.
 Astronomy- the study of the universe  Year- the time required for the Earth to orbit once around the sun  Month- a division of the year that is based.
Observing the Solar System Mrs. Davis Earth Science.
Models of the Solar System
EARLY ASTRONOMERS. Aristotle (~ BC) Define the five Elements: Water, Aether (the Heavens, and of course, Earth, Wind & Fire Geocentric Model –
Title your notes: Models of the Solar System
History of Astronomy How have ideas about the solar system and our place in it changed over time? How have ideas about the solar system and our place.
Identify the units of a calendar. How do scientists study space?
THE SOLAR SYSTEM Chapter 24A. Unit Objectives Compare models of the solar system To list and describe the objects in our solar system.
History of Astronomy. People have been looking up at the sky trying to figure it out for as long as we have been around. Even earliest man noticed that.
Introduction to Classical Astronomy Mr. Ross Brown Brooklyn School for Law and Technology.
Ptolemaic model In the second century CE, Ptolemy, who lived in the Egyptian town of Alexandria, produced a mathematical representation based on observation.
Astronomy in the Middle Ages to the Modern Era From Copernicus to Galileo to man on the moon.
Historical Models of our Solar System and Kepler’s Laws of Planetary Motion.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
CHAPTER 27 SECTION 2 EARTH AND SPACE AUSTIN HIGH SCHOOL Models of the Solar System.
Outer Space Chapters 25 and Solar System Made up of: Sun (a.k.a. star) Planets Moons (yes plural) Other small objects.
Modelling Celestial Motion. Using Models Designers and engineers use models to help them solve problems without having to construct the real thing. Designers.
History of Astronomy The guys with their eyes on the skies.
Gravity Newton’s Law of Gravitation Gravitational Fields.
The Scientific Revolution. What is a Revolution? A Revolution is a complete change, or an overthrow of a government, a social system, a way of thinking,
Observing the Solar System / Earth in Space Chapters 19 & 20 Sections 1 & 2.
Astronomy- The Original Science
Objective 03/26/12 Identify the units of a calendar. Intro
Observing the solar system!
Week 3 Notes Observing the Solar System
The Solar System 6.E.1.2 Explain why Earth sustains life while other planets do not based on their properties (including types of surface,
Astronomy- The Original Science
Chapter 20 Section 1 Key Concepts: What are the geocentric and heliocentric systems? How did Copernicus, Galileo, and Kepler contribute to our knowledge.
Observing the Solar System
Chapter 6 Lesson 1 Models of the Solar system
Part 1: Historical Models
The Motions of the Planets
Presentation transcript:

Mav Mark 11/3/11 When electricity leaves a power plant is it AC or DC, and is it at high voltage or low voltage?

Observing the Solar System Notes

Earth at the Center Most early Greek astronomers believed that Earth was the center of the universe. They also noticed that a few “stars” in the sky seemed to follow paths separate from the others. The Greeks called them planets from their word for “wanderers.” The Romans would later label these planets Mercury, Venus, Mars, Jupiter, and Saturn after their own gods.

Earth at the Center A model of the universe in which Earth is at the center is called a geocentric system. In a geocentric system, all planets and stars revolve around Earth.

Earth at the Center The Greek astronomer Ptolemy developed a complex geocentric model of the universe around the year 140 CE. Ptolemy’s model seemed to explain motions in the sky. Because the planets occasionally appear to go backwards in the sky, Ptolemy had to come up with some kind of solution for this motion, so he claimed that the planets, in their orbits, would make small circles called epicycles. Ptolemy’s theories fit so well all of the observations of the planets and stars, that his model of the universe would last for nearly 1,500 years, until nearly the end of the Italian Renaissance.

Sun at the Center A system in which the sun is at the center is called a heliocentric system. Earth and other planets revolve around the sun in a heliocentric system. In 1543, a Polish astronomer named Nicolaus Copernicus developed a good heliocentric model of the universe, but still contained a few flaws. Despite the fact that he was mostly correct, his theories would still be rejected for over 50 years.

Sun at the Center In the 1600s, the Italian scientist Galileo Galilei made discovers that supported the heliocentric model. For example, using his telescope, Galileo discovered the four largest moons of Jupiter (known now as the Galilean Moons), proving that not everything orbited Earth. His observations of a full set of phases for Venus also supported a heliocentric view of the universe. Galileo too was ridiculed for his theories. He was even put under house arrest by Pope Urban the VIII for “vehement suspicion of heresy,” where he would eventually die.

Sun at the Center The most accurate measurements of the stars and planets was made by a Danish astronomer named Tycho Brahe. Unfortunately, Brahe was a believer of Ptolemy’s geocentric vision of the universe. At the same time, though, he had to concede that some observations fit a heliocentric view. In a way to keep both versions, he created a new model of the universe. His model came to be known as a geo- heliocentric model, or the Tychonic model.

Sun at the Center Brahe’s greatest contribution, beside his very precise observations, was actually his apprentice, Johannes Kepler. Brahe knew that Kepler was smarter, so he hid some research from Kepler, and presented him with minor tasks, such as figuring out Mars’ orbit, and only gave Kepler part of his research. This would actually allow Kepler to make the greatest discovery of his life.

Sun at the Center After years of study, and Brahe’s eventual death, Kepler had finally reached a very controversial conclusion. The orbit of Mars was not a perfect circle. Kepler discovered that not only Mars, but all of the planets travel in a path in the shape of a flattened circle, or an ellipse.

Sun at the Center Kepler used his own calculations, as well as Brahe’s observations to create his Three Laws of Planetary Motion: 1. The orbit of every planet is an ellipse with the Sun at one of the two foci.orbitplanetellipsefoci 2. A line joining a planet and the Sun sweeps out equal areas during equal intervals of time.lineareas 3. The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.squareorbital periodproportionalcube semi-major axis

Kepler’s Three Laws of Planetary Motion lers_Laws_fullscreen.mov

Modern Discoveries Early astronomers only knew of six planets: Mercury, Venus, Earth, Mars, Jupiter, and Saturn. Uranus was eventually discovered by William Herschel in 1781, but he originally though it to be a comet. "I don't know what to call it. It is as likely to be a regular planet moving in an orbit nearly circular to the sun as a Comet moving in a very eccentric ellipsis. I have not yet seen any coma or tail to it". Due to it’s nearly circular orbit, it was later named a planet, Uranus, after the Greek sky god Ouranos.

Modern Discoveries Neptune was discovered in 1846, but was actually discovered by mathematical prediction rather than by direct observation. Oddities in the orbit of Uranus led to the prediction of a large gravitationally massive object outside of Uranus’ orbit.

Modern Discoveries While Herschel was looking in the sky with his telescope for Uranus, he noticed fuzzy, white patches that he could not identify. Despite the fact that he didn’t know what they were, he noted their positions anyway. In 1923, with the invention of photography, an astronomer named Edwin Hubble studied these “fuzzy patches.” Edwin concluded that they were entire galaxies of stars, each containing their own hundreds of billions of stars. Before Hubble, we really thought that we were the only galaxy out there.

The Scientists _08_The-Scientists-640x360.mov