Solar System Formation

Similar documents
Chapter 25.1: Models of our Solar System

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

Study Guide: Solar System

Introduction to the Solar System

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)

Chapter 5: Circular Motion, the Planets, and Gravity

From Aristotle to Newton

Lecture 13. Gravity in the Solar System

AE554 Applied Orbital Mechanics. Hafta 1 Egemen Đmre

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

GRAVITATIONAL FIELDS PHYSICS 20 GRAVITATIONAL FORCES. Gravitational Fields (or Acceleration Due to Gravity) Symbol: Definition: Units:

Section 1 Gravity: A Force of Attraction

Chapter 3 The Science of Astronomy

Name Class Period. F = G m 1 m 2 d 2. G =6.67 x Nm 2 /kg 2

A = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great.

Motions of Earth, Moon, and Sun

Earth in the Solar System

Name Class Date. true

Lecture 17 Newton on Gravity

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

How did the Solar System form?

Unit 11: Gravity & the Solar System

Grade 6 Standard 3 Unit Test A Astronomy. 1. The four inner planets are rocky and small. Which description best fits the next four outer planets?

Astronomy 1140 Quiz 1 Review

Computer Animations of Ancient Greek and Arabic Planetary Models

Study Guide due Friday, 1/29

Newton s Law of Gravity

STUDY GUIDE: Earth Sun Moon

1 A Solar System Is Born

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

Exercise: Estimating the Mass of Jupiter Difficulty: Medium

The orbit of Halley s Comet

5- Minute Refresher: Daily Observable Patterns in the Sky

Unit 8 Lesson 2 Gravity and the Solar System

The Solar System. A Collaborative Science Activity for Key Stage 2. Teacher s Notes. Procedure

8.5 Motions of Earth, the Moon, and Planets

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

What causes Tides? If tidal forces were based only on mass, the Sun should have a tidegenerating

Gravity. in the Solar System. Beyond the Book. FOCUS Book

Summary: Four Major Features of our Solar System

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

The Layout of the Solar System

The Moon. Nicola Loaring, SAAO

DIRECT ORBITAL DYNAMICS: USING INDEPENDENT ORBITAL TERMS TO TREAT BODIES AS ORBITING EACH OTHER DIRECTLY WHILE IN MOTION

THE SOLAR SYSTEM - EXERCISES 1

Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System

galaxy solar system supernova (noun) (noun) (noun)

Science Standard 4 Earth in Space Grade Level Expectations

Orbital Dynamics. Orbital Dynamics 1/29/15

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

Gravity? Depends on Where You Are!

The Earth, Sun & Moon. The Universe. The Earth, Sun & Moon. The Universe

RETURN TO THE MOON. Lesson Plan

Class 2 Solar System Characteristics Formation Exosolar Planets

DESCRIPTION ACADEMIC STANDARDS INSTRUCTIONAL GOALS VOCABULARY BEFORE SHOWING. Subject Area: Science

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

Chapter 1: Our Place in the Universe Pearson Education Inc., publishing as Addison-Wesley

Chapter 15.3 Galaxy Evolution

Science Focus 9 Space Exploration Topic Test

Related Standards and Background Information

Page. ASTRONOMICAL OBJECTS (Page 4).

Isaac Newton & the Newtonian Age

The Main Point. Lecture #34: Solar System Origin II. Chemical Condensation ( Lewis ) Model. How did the solar system form? Reading: Chapter 8.

1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram?

The Solar System. I. Introduction. S. Gavin and S. P. Karrer Physics Department, Wayne State University, Detroit, MI,

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

Why don t planets crash into each other?

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

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

GRADE 8 SCIENCE INSTRUCTIONAL TASKS. Gravity

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping

NOTES: GEORGIA HIGH SCHOOL SCIENCE TEST THE SOLAR SYSTEM

Lecture 7 Formation of the Solar System. Nebular Theory. Origin of the Solar System. Origin of the Solar System. The Solar Nebula

Appropriate space vocabulary for Primary School

ELEMENTS OF PHYSICS MOTION, FORCE, AND GRAVITY

Lecture 10 Formation of the Solar System January 6c, 2014

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

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

The Hidden Lives of Galaxies. Jim Lochner, USRA & NASA/GSFC

Phases of the Moon. --demonstrate the ability to apply an in-depth understanding of moon phases to real life situations

A SOLAR SYSTEM COLORING BOOK

Name: Date: Period: Gravity Study Guide

Lab 7: Gravity and Jupiter's Moons

Vocabulary - Understanding Revolution in. our Solar System

Interplanetary Travel. Outline. In This Section You ll Learn to...

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

circular motion & gravitation physics 111N

Due Tuesday, January 27th IN CLASS. Grading Summary: Question 11: 12 points. Question 12: 26 points. Question 13: 12 Points.

Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014

Out of This World Classroom Activity

Version A Page The diagram shows two bowling balls, A and B, each having a mass of 7.00 kilograms, placed 2.00 meters apart.

Earth Is Not the Center of the Universe

Astronomy Club of Asheville October 2015 Sky Events

165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars

Discover the planets of our solar system. In 90 minutes through the universe. On a hiking path between Ehrenfriedensdorf and Drebach

The Solar System CHAPTER 19. Chapter Preview. 1 Sun, Earth, and Moon The View from Earth The Moon

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES

Earth, Moon, and Sun Study Guide. (Test Date: )

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

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

Transcription:

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 Force is also known as the strength of gravity or the pull of gravity. It is dependent upon the mass of the two objects and the distance between As mass increases; gravitational force (g force) increases: g-force the two objects. Gravitational Force = G m1 m2 (G = Gravitational Constant = 6.67x 10-11 N m 2 / kg 2 ). r 2 mass 1

Positive slope indicates a direct relationship Sep 29 7:24 PM As distance increases; (g force) decreases: g-force 5 4 3 2 Negative slope indicates an inverse relationship 1 1 2 3 4 5 distance Gravitational Force = G m1 m2 Note: Gravitational Force is reduced by the SQUARE of the distance between the two objects... r 2 Why doesn't gravity simply pull all of the planets into the Sun? For example: if the distance between two objects is doubled, the gravitational force is reduced by 4 times Put in your (or) it is 1/4 th as strong as it was originally. notes... g-force x -4 = 1 g-force = 1 g-force reduced by 4 times original g-force -4 Jul 9 8:13 AM Sep 29 7:21 PM 2

Another consideration concerning solar system formation is INERTIA: The tendency of a body in uniform motion to remain in uniform motion. When the force of gravity and inertia are in, equilibrium the object establishes an ORBIT. Objects orbit around the center of gravity of a system. Formation of our Solar System Stage A: Supernova occurs creating a cloud of intersteller gas and dust In addition to the following notes, these captions are important too. 3

Stage B: Stage C: Gravity causes the cloud to. condense The bulge eventually contracts enough to form a protostar and then a star (our Sun). gravity inertia Eventually, and reach an equilibrium and the planets establish orbits around the Sun. Earth - Centered Belief that everything revolved around a stationary Earth. Belief that everything revolved around a stationary Earth. Established by ancient Greeks as far back as Aristotle s time (350 BC). Ptolemy (TAHL uh mee) (~140 AD) added that each planet had mini orbits of their own as they orbited the Earth. called "epicycles" To reverse direction against background stars Epicycles helped to explain "retrograde" motion of the planets. (other adjustments continued to be made) The epicycle of Venus was placed in line with the Sun to explain the reason that Venus is only visible in the east just before sunrise and in the west just before sunset...never high in the nighttime sky. 4

Heliocentric: Sun-centered Understanding that everything revolved around the Sun. First hypothesized by Copernicus (~1500) Confirmed by Galileo with the use of his telescope (~1600) Heliocentric: Galileo s evidence: 1. Observed 4 moons orbiting the planet Jupiter and not Earth. Venus 2. Observed that the planet had phases that only an orbit around the Sun could produce. Venus's motion according to Ptolemy (epicycle) Sep 1 11:14 AM Galileo's observations best explained by the heliocentric model Phases of Venus as observed by Galileo Supports the reason we can see a "full" phase of Venus. http://www.teachersdomain.org/asset/ess05_vid_galileosys/ Sep 1 11:18 AM Sep 1 11:21 AM 5