4.5 Orbits, Tides, and the Acceleration of Gravity

Similar documents
5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves

Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:

Newton s Law of Gravity

Science Standard Articulated by Grade Level Strand 5: Physical Science

1. The Kinetic Theory of Matter states that all matter is composed of atoms and molecules that are in a constant state of constant random motion

AS COMPETITION PAPER 2008

Unit 2 Lesson 1 Introduction to Energy. Copyright Houghton Mifflin Harcourt Publishing Company

PS-6.2 Explain the factors that determine potential and kinetic energy and the transformation of one to the other.

Science Standard 3 Energy and Its Effects Grade Level Expectations

Lesson 6: Earth and the Moon

Practice TEST 2. Explain your reasoning

Current Staff Course Unit/ Length. Basic Outline/ Structure. Unit Objectives/ Big Ideas. Properties of Waves A simple wave has a PH: Sound and Light

Use the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.

Chapter 18: The Structure of the Atom

CHAPTER 2 Energy and Earth

Indiana's Academic Standards 2010 ICP Indiana's Academic Standards 2016 ICP. map) that describe the relationship acceleration, velocity and distance.

Light as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation

AZ State Standards. Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred.

Level 3 Achievement Scale

TEACHER BACKGROUND INFORMATION THERMAL ENERGY

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

Preview of Period 2: Forms of Energy

Energy. Mechanical Energy

Chapter 1 Student Reading

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation?

Semester 2. Final Exam Review

Name Date Class ELECTRONS IN ATOMS. Standard Curriculum Core content Extension topics

After a wave passes through a medium, how does the position of that medium compare to its original position?

KINETIC MOLECULAR THEORY OF MATTER

Chapter 2: Forms of Energy

In science, energy is the ability to do work. Work is done when a force causes an

Chapter 2: Forms of Energy

Grade Level Expectations for the Sunshine State Standards

Solar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation

Practice final for Basic Physics spring 2005 answers on the last page Name: Date:

Carol and Charles see their pencils fall exactly straight down.

MAKING SENSE OF ENERGY Electromagnetic Waves

Section 15.1 Energy and Its Forms (pages )

Atomic Structure: Chapter Problems

Name Period 4 th Six Weeks Notes 2015 Weather

ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation

18.2 Comparing Atoms. Atomic number. Chapter 18

Name Class Date. In the space provided, write the letter of the term or phrase that best completes each statement or best answers each question.

The Electromagnetic Spectrum

Name Class Date. spectrum. White is not a color, but is a combination of all colors. Black is not a color; it is the absence of all light.

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

A n = 2 to n = 1. B n = 3 to n = 1. C n = 4 to n = 2. D n = 5 to n = 2

Atomic Structure Ron Robertson

What is Energy? What is the relationship between energy and work?

Atomic Calculations. 2.1 Composition of the Atom. number of protons + number of neutrons = mass number

Chemistry 13: States of Matter

Noble Gases. Outline Nobel Gas Elements Radon and Health Chemistry Homework

Objectives. PAM1014 Introduction to Radiation Physics. Constituents of Atoms. Atoms. Atoms. Atoms. Basic Atomic Theory

What Is Energy? Energy and Work: Working Together. 124 Chapter 5 Energy and Energy Resources

Waves Sound and Light

Science Tutorial TEK 6.9C: Energy Forms & Conversions

Name Class Date. true

Energy Transformations

The content is based on the National Science Teachers Association (NSTA) standards and is aligned with state standards.

Multiple Choice Identify the choice that best completes the statement or answers the question.

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

The Sun and Solar Energy

Name: Partners: Period: Coaster Option: 1. In the space below, make a sketch of your roller coaster.

1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K

The unifying field Theory

Overview. What is EMR? Electromagnetic Radiation (EMR) LA502 Special Studies Remote Sensing

Basics of Nuclear Physics and Fission

Chapter 6. Work and Energy

Chapter 17: Change of Phase

MCQ - ENERGY and CLIMATE

8.1 Radio Emission from Solar System objects

XX. Introductory Physics, High School

Teaching Time: One-to-two 50-minute periods

Photons. ConcepTest ) red light 2) yellow light 3) green light 4) blue light 5) all have the same energy. Which has more energy, a photon of:

1. Mass, Force and Gravity

Radiation Transfer in Environmental Science

KS3 revision booklet Physics

The Earth s Atmosphere

MS. Structure and Properties of Matter

State Newton's second law of motion for a particle, defining carefully each term used.

The Phenomenon of Photoelectric Emission:

Name Partners Date. Energy Diagrams I

PHYSICAL WORLD. Heat & Energy GOD S DESIGN. 4th Edition Debbie & Richard Lawrence

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

Chemistry 2 Chapter 13: Electrons in Atoms Please do not write on the test Use an answer sheet! 1 point/problem 45 points total

Forms of Energy. Freshman Seminar

Vacuum Evaporation Recap

Take away concepts. What is Energy? Solar Energy. EM Radiation. Properties of waves. Solar Radiation Emission and Absorption

Electrons in Atoms & Periodic Table Chapter 13 & 14 Assignment & Problem Set

Treasure Hunt. Lecture 2 How does Light Interact with the Environment? EMR Principles and Properties. EMR and Remote Sensing

Objectives 404 CHAPTER 9 RADIATION

Name: Date: Period: Gravity Study Guide

Convection, Conduction & Radiation

Boardworks AS Physics

In studying the Milky Way, we have a classic problem of not being able to see the forest for the trees.

The University of the State of New York REGENTS HIGH SCHOOL EXAMINATION PHYSICAL SETTING PHYSICS. Friday, June 20, :15 to 4:15 p.m.

Preview of Period 5: Thermal Energy, the Microscopic Picture

ATOMS AND THE PERIODIC TABLE CHAPTER 3 PHYSICAL SCIENCE

Energy comes in many flavors!

60 Questions Basic Physics Paul G. Hewitt

Transcription:

4.5 Orbits, Tides, and the Acceleration of Gravity Our goals for learning: How do gravity and energy together allow us to understand orbits? How does gravity cause tides? Why do all objects fall at the same rate?

How do gravity and energy together allow us to understand orbits? Total orbital energy (gravitational + kinetic) stays constant if there is no external force. Orbits cannot change spontaneously. Total orbital energy stays constant.

Changing an Orbit So what can make an object gain or lose orbital energy? Friction or atmospheric drag This is how we slow down spacecraft going to Mars A gravitational encounter Gravity assist can speed up orbits of solar system spacecraft

Escape Velocity If an object gains enough orbital energy, it may escape (change from a bound to unbound orbit). Escape velocity from Earth 11 km/s from sea level (about 40,000 km/hr) Escape and orbital velocities don't depend on the mass of the cannonball.

How does gravity cause tides? Moon's gravity pulls harder on near side of Earth than on far side. Difference in Moon's gravitational pull stretches Earth.

Tides and Phases For Earth, tides are largest due to Moon, then 2 nd largest due to Sun Size of tides depends on phase of Moon Maximum tides are at full and new moon

Tidal Friction The Earth is also rotating much faster (1 day) than the moon s orbit (~28 days) This fast rotation pushes the Earth s tidal bulge slightly ahead of the dashed line But bulge feels a force from the Moon trying to pull it back in line

Tidal Friction Tidal friction gradually slows Earth's rotation Energy lost must be conserved and goes into the Moon s orbit The Moon gets farther from Earth

Tidal Friction Tides are also raised on the Moon by the Earth The Moon once orbited faster (or slower); tidal friction caused it to ''lock'' in synchronous rotation. The Moon s tidal bulge now points nearly precisely at the Earth

Clicker Question You re at the beach at midnight doing totally wholesome activities that your parents would obviously approve of and the full moon is overhead. Is the tide: A) high, but a bit higher than usual B) high, but a bit lower than usual C) low, but a bit higher than usual D) low, but a bit lower than usual

Last question: why do all objects fall at the same rate? The gravitational acceleration of an object like a rock does not depend on its mass because M rock in the equation for acceleration cancels M rock in the equation for gravitational force. This ''coincidence'' was not understood until Einstein's general theory of relativity.

What have we learned? How do gravity and energy together allow us to understand orbits? Change in total energy is needed to change orbit Add enough energy (escape velocity) and object leaves. How does gravity cause tides? The Moon's gravity stretches Earth and its oceans. Why do all objects fall at the same rate? Mass of object in Newton's second law exactly cancels mass in law of gravitation.

Chapter 5: Light and Matter: Reading Messages from the Cosmos

5.1 Light in Everyday Life Our goals for learning: How do we experience light? How do light and matter interact?

How do we experience light? The warmth of sunlight tells us that light is a form of energy. We can measure the flow of energy in light in units of watts: 1 watt = 1 joule/s. More energy per second is more watts

Colors of Light White light is made up of many different colors.

How do light and matter interact? Emission Absorption Transmission Transparent objects transmit light. Opaque objects block (absorb) light. Reflection/scattering

Reflection and Scattering Mirror reflects light in a particular direction. Movie screen scatters light in all directions.

Interactions of Light with Matter Interactions between light and matter determine the appearance of everything around us.

What have we learned? How do we experience light? Light is a form of energy. Light comes in many colors that combine to form white light. How do light and matter interact? Matter can emit light, absorb light, transmit light, and reflect (or scatter) light. Interactions between light and matter determine the appearance of everything we see.

5.2 Properties of Light Our goals for learning: What is light? What is the electromagnetic spectrum?

What is light? Light can act either like a wave or like a particle. Particles of light are called photons.

Waves A wave is a pattern of motion that can carry energy without carrying matter along with it. The water molecules bob up and down while the energy moves out

Properties of Waves Wavelength is the distance between two wave peaks A distance, often in meters (m) Frequency is the number of times per second that a wave vibrates up and down. Often in number of times per second The unit of per second is Hertz (Hz) Wave speed = wavelength x frequency

Light: Electromagnetic Waves A light wave is a vibration of electric and magnetic fields. Light interacts with charged particles through these electric and magnetic fields.

Wavelength and Frequency wavelength x frequency = speed of light = constant

Particles of Light Particles of light are called photons. Each photon has a wavelength and a frequency. The energy of a photon depends on its frequency.

Wavelength, Frequency, and Energy λ x f = c λ = wavelength, f = frequency c = 3.00 x 10 8 m/s = speed of light E = h x f = photon energy h = 6.626 x 10-34 joule x s = Planck's constant

What is the electromagnetic spectrum?

Clicker Question The higher the photon energy, A. the longer its wavelength. B. the shorter its wavelength. C. energy is independent of wavelength.

Clicker Question The higher the photon energy, A. the longer its wavelength. B. the shorter its wavelength. C. energy is independent of wavelength. 2014 Pearson Education, Inc.

What have we learned? What is light? Light can behave like either a wave or a particle. A light wave is a vibration of electric and magnetic fields. Light waves have a wavelength and a frequency. Photons are particles of light. What is the electromagnetic spectrum? Human eyes cannot see most forms of light. The entire range of wavelengths of light is known as the electromagnetic spectrum. 2014 Pearson Education, Inc.

5.3 Properties of Matter Our goals for learning: What is the structure of matter? What are the phases of matter How is energy stored in atoms? 2014 Pearson Education, Inc.

What is the structure of matter? 2014 Pearson Education, Inc.

Atomic Terminology Atomic number = # of protons in nucleus Atomic mass number = # of protons + neutrons Molecules: consist of two or more atoms (H 2 O, CO 2 ) 2014 Pearson Education, Inc.

Atomic Terminology Isotope: same # of protons but different # of neutrons ( 4 He, 3 He) 6 electrons 6 electrons 6 electrons 2014 Pearson Education, Inc.

What are the phases of matter? Familiar phases: Solid (ice) Liquid (water) Gas (water vapor) Phases of same material behave differently because of differences in chemical bonds. 2014 Pearson Education, Inc.

Phase Changes Ionization: stripping of electrons, changing atoms into plasma Dissociation: breaking of molecules into atoms Evaporation: breaking of flexible chemical bonds, changing liquid into solid Melting: breaking of rigid chemical bonds, changing solid into liquid 2014 Pearson Education, Inc.

Phases and Pressure Phase of a substance depends on both temperature and pressure. Often more than one phase is present. 2014 Pearson Education, Inc.

How is energy stored in atoms? Excited states Ground state Electrons in atoms are restricted to particular energy levels. 2014 Pearson Education, Inc.

Energy Level Transitions The only allowed changes in energy are those corresponding to a transition between energy levels. Not allowed Allowed 2014 Pearson Education, Inc.

What have we learned? What is the structure of matter? Matter is made of atoms, which consist of a nucleus of protons and neutrons surrounded by a cloud of electrons. What are the phases of matter? Adding heat to a substance changes its phase by breaking chemical bonds. As temperature rises, a substance transforms from a solid to a liquid to a gas, then the molecules can dissociate into atoms. Stripping of electrons from atoms (ionization) turns the substance into a plasma. 2014 Pearson Education, Inc.

What have we learned? How is energy stored in atoms? The energies of electrons in atoms correspond to particular energy levels. Atoms gain and lose energy only in amounts corresponding to particular changes in energy levels. 2014 Pearson Education, Inc.