AIM: What is Astronomy? Do Now: Answer the following question in your notebook. Where is the sun in our solar system? What percent of our Solar System’s.

Slides:



Advertisements
Similar presentations
Chapter 27.2 Models of the solar system
Advertisements

Motions of the Planets This presentation will introduce these terms: Geocentric, Heliocentric, Retrograde, Rotation, Revolution.
Kepler’s laws.
Early Astronomers & Planetary Motion
Geocentric Model Earth is center of our Solar System
Models of the Solar System *Early Models of the Solar System *Kepler’s Laws.
Models of the Solar System
MODELS OF THE SOLAR SYSTEM. ARISTOTLE Greek philosopher ( BC) He promoted an earth centered called geocentric, model of solar system He said the.
Planets of the Solar System Section 2 Section 2: Models of the Solar System Preview Key Ideas Early Models Kepler’s Laws Newton’s Explanation of Kepler’s.
Introduction to Astronomy. How big, and small, is our universe, and how do scientists measure these vast differences? Scientific Notation—a convenient.
Chapter 19.1 Part 2.
The Solar System Planetary Orbits
Scientific Models & Kepler’s Laws Scientific Models We know that science is done using the Scientific Method, which includes the following steps : Recognize.
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.
Planetary Orbits The ancient Greeks (Aristotle and Plato) thought the only perfect shapes were the circle and line. All things fall in a line toward Earth,
Solar System Overview. Early Ideas  It was assumed that the Sun, planets, and stars orbited a stationary universe  This is known as a “geocentric” model,
Kepler’s Laws of Planetary Motion. Debate on Planet Motions Geocentric or Heliocentric Universe.
Johannas Kepler Johannas Kepler Planetary Orbital Laws Planetary Orbital Laws.
Ch. 22 Origin of Modern Astronomy Sec. 1 Early Astronomy 200.
2.1 History of Astronomy. What is Astronomy?  The branch of science that deals with celestial objects, space, and the physical universe as a whole.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
29 Chapter 29 Our Solar System. Ancient Greeks Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation.
Notebooks: We had a very BASIC notebook check. For our next notebook check you need to have your cover completed, table of contents filled out, titles.
Ch 22 Astronomy. Ancient Greeks 22.1 Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation.
TOPIC #1: Chapter 22 Origin of Modern Astronomy. Section 1: Early Astronomy Astronomy is the science that studies the universe. The “Golden Age” of early.
Learning Log Write about how you think the Earth moves in relation to our Universe and solar system.
 Definition - Earth is at the center of the solar system being orbited by the Sun and other planets  (sketch a picture of a geocentric solar system)
The planets 12/1/14.
Geometry of Earth’s Orbit Kepler’s Laws of Planetary Motion.
KEPLER’S LAWS OF PLANETARY MOTION Objective: I will summarize Kepler’s three laws of planetary motion. 11/10/15.
 Danish astronomer ( )  Built an astronomical observatory on an island  Measured positions of stars and planets over a period of 20 years.
Historical Models of our Solar System and Kepler’s Laws of Planetary Motion.
Formation of the Solar System, Kepler’s Laws Copyright © McGraw-Hill Education Formation of the Solar System.
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.
Our Solar System. Views of our solar system Early explanations of our solar system was thought to be a Geocentric Model -also called Ptolemy model Earth.
Ancient Greeks Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies.
 Compare the models of the universe developed by Ptolemy and Copernicus.  Summarize Kepler’s three laws of planetary motion.  Describe how Newton explained.
Aristotle suggested an Earth-centered, or geocentric, model of the solar system. In this model, the sun, the stars, an the planets revolved around Earth.
PHYS 155 – Introductory Astronomy observing sessions: - observing sessions: Sunday – Thursday, 9pm, weather permitting
Starter 1.What is astronomy? 2.The movement around the sun is ______. 3.The movement around an axis is____. 4.Compare and contrast global warming and greenhouse.
Orbits, Asteroids, and Comets. The Geometry of Orbits Planets revolve in an ellipse around the sun –An ellipse has two fixed points called foci that are.
Our View of the Universe
Earth Basics Something To Model Planets And the Night Sky Johannes
MODELS OF THE SOLAR SYSTEM
Part 1: Planets and SS models Part 2: Kepler’s Laws of Motion
Part 1: Planets and SS models Part 2: Kepler’s Laws of Motion
Science Starter Answer the following in your notebook: 1. When is the Earth closest to the Sun? 2. Does the speed of the Earth’s revolution change? 3.
Origin of Modern Astronomy
22.1 Early Astronomy.
22.1 Early Astronomy.
What is the universe Part 2 Motion in Space
Section 2: Models of the Solar System
Kepler and Planetary Motion
Solar System Overview.
Models of the Solar System
Physics of the Solar System
Section 2: Models of the Solar System
The Laws of Planetary Motion
The sun makes up about 99% of our solar systems mass.
Origin of Modern Astronomy
Observing the Solar System
The sun makes up about 99% of our solar systems mass.
Lesson 2 Models of the Universe
Planetary Motion Intro Video.
Aim: How can we explain the laws that control the planets orbits?
Aim: How do planets move?
Early Ideas.
Eccentricity.
Motion of Objects in Space
Presentation transcript:

AIM: What is Astronomy? Do Now: Answer the following question in your notebook. Where is the sun in our solar system? What percent of our Solar System’s mass is occupied by the Sun? The sun makes up about 99% of our solar systems mass.

I. Astronomy is the science that studies the universe and all objects in it. **Apparent motion= what an object appears to be doing, not what it is actually doing** Why do some objects appear to be moving in space?

II. Two Views: Geocentric: - Earth is motionless at the center of the universe; all planets including the sun revolve around it. Heliocentric: - Sun is the center of the solar system; all planets revolve around it. (Simple explanation) Which one is true? Heliocentric

III. Planetary Motion - Johannes Kepler made observations of objects in the night time sky. In doing this he discovered that: 1. The path of each planet around the sun is an ellipse (oval-shape), with the sun as one focus. - a focus is an object that a planet moves around.

Focus 1 Focus 2 Major Axis Eccentricity = Distance between the foci Length of the major axis - Eccentricity measures the ellipse and describes it’s shape. ESRT Cover

Eccentricity = 1 (a line) Eccentricity = 0.5 Eccentricity = 0 (a circle) FF FF F From the back table take an Ellipse worksheet from the top bin and a ruler Most Eccentric Least Eccentric - Eccentricity can described a planets ellipse as:

2. The closer a planet is to the Sun (foci) the faster it revolves. Faster Slower

Astronomical unit (AU) - it is about 150 million kilometers. - is the average distance between Earth and the sun. Light Year - the distance light travels in one year. IV. Measurement in Space

V. Gravitational Force In which diagram does the star have the greatest gravitation force? The greatest mass and least distance increases as distance between objects decrease. (closer together = stronger force) increases as mass increases. (more mass = more force)

VI. Other Motion: Retrograde Motion is the apparent westward motion of planets as compared to the background stars.

Closure: - Obtain an “Intro to Astronomy” worksheet (back top bin) -Using your ESRT and the notes answer the questions. Focus 1 Focus 2 Major Axis Eccentricity = Distance between the foci Length of the major axis