The sun makes up about 99% of our solar systems mass.

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.
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.
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.
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.
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.
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.
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.
The planets 12/1/14.
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.
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.
Eccentricity.
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
Warmup Why is “space” called “space”? How did our solar system form?
Earth Basics Something To Model Planets And the Night Sky Johannes
Orbital Geometry.
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.
History of our Knowledge of the Solar System
L. O: swbat calculate the elliptical orbits of planets
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
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?
The Solar System Ch.11.
Eccentricity.
Aim: How do we compute Eccentricity?
Aim: How do planets move?
The (brief) History of Astronomy
Early Ideas.
Kepler’s Laws EARTH SCIENCE
Eccentricity.
Motion of Objects in Space
Presentation transcript:

The sun makes up about 99% of our solar systems mass. 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.

Why do some objects appear to be moving in space? 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?

Which one is true? II. Two Views: Heliocentric 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.

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

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

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

IV. Measurement in Space 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.

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

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

Obtain your review book from the back of the room. Closure: Obtain your review book from the back of the room. Review Book p. 451-452 #1-4 1) 2) 3) 4) p. 455-456 #1-13 1) 2) 3) 4) 5) 6) 7) 8) 9) 10) 11) 12) 13) 1 4 4 2 3 1 3 2 3 1 4 2 4 2 2 2 3

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