Topic #4 ENERGY & MATTER OVERVIEW

Similar documents
TOPICS FOR TODAY S CLASS:

Topic #2 (cont.) QUANTIFYING GLOBAL CHANGE (cont.) Time Series Graphs WRAP-UP...

TOPIC # 5 ELECTROMAGNETIC

The Kinetic Theory of Matter. Temperature. Temperature. Temperature. Temperature. Chapter 6 HEAT

Tuesday Sep 9th ANNOUNCEMENTS. Assignment I-1 is due tonight before midnight (11:59 pm)

* Defining Temperature * Temperature is proportional to the kinetic energy of atoms and molecules. * Temperature * Internal energy

Agenda. Chapter 10, Problem 26. All matter is made of atoms. Atomic Structure 4/8/14. What is the structure of matter? Atomic Terminology

Energy, Work, and Power

ENERGY. Unit 12: IPC

Physical Science midterm study guide. Chapter 1 and 2

The (Almost) Modern Atom Model. SUMMARY from previous lecture Energy comes in different forms. ENERGY IS ALWAYS CONSERVED.

4.2 A Scientific View of Energy Kinetic Energy

Matter, Atoms & Molecules

Ready for some more SCIENCE Homer?

The lower the energy of a substance, the interaction between its atoms and molecules.

Kinetic Theory of Matter

Physical Science Chapter 5 Cont2. Temperature & Heat

Grade 7 Science. Unit 1 The Classification of Matter. Competency (Do)

8.5 - Energy. Energy The property of an object or system that enables it to do work. Energy is measured in Joules (J).

Lesson 6 Matter. Introduction: Connecting Your Learning

UNIT 5: WORK and ENERGY RECORD ALL ANSWERS ON ANSWER SHEET.

Unit 6. Unit Vocabulary: Distinguish between the three phases of matter by identifying their different

Qualitative observation descriptive observation has no numerical measurement

Solids, Liquids, and Gases. Chapter 14

Chemistry Terms. atomic number The atomic number of an element is the number of protons in the nucleus of each atom.

Ready for some more SCIENCE Homer? ( Homer gives his brain a pep talk )

A few final review points to emphasize on: Topic #6 Atmospheric Structure & Composition...

Chapter 4. Properties of Matter

To begin, enter your Footprint in Earths with you clicker...

Intro to Galaxies Light and Atoms - I

Chapter: Heat and States

Name Date Class STATES OF MATTER

Figure 1.1. Relation between Celsius and Fahrenheit scales. From Figure 1.1. (1.1)

14-Feb-18 INSIDE STARS. Matter and Energy. Matter and Energy. Matter and Energy. What is matter?

F=ma. Exam 1. Today. Announcements: The average on the first exam was 31/40 Exam extra credit is due by 8:00 am Friday February 20th.

Conceptual Chemistry

SG 4 Elements and Chemical Bonds 5 States of Matter

Chemistry 101 Chapter 10 Energy

Pg , Syllabus

Properties and Structure of Matter

Chapter 6 The States of Matter. Examples of Physical Properties of Three States of Matter

The Sun s Internal Temperature

Thermochemistry. The study of energy changes that occur during chemical reactions and changes in state.

Chapter Introduction Lesson 1 Forms of Energy Lesson 2 Energy Transformations Lesson 3 Thermal Energy on the Move Chapter Wrap-Up

Temperature, Thermal Energy and Heat

Joy of Science Discovering the matters and the laws of the universe

Gases: Properties and Behaviour

Chapter Introduction Lesson 1 Forms of Energy Lesson 2 Energy Transformations Lesson 3 Thermal Energy on the Move Chapter Wrap-Up

Physical Science Final Examination-Review Sheet (14-15) KEY. 1. A process used to answer questions or solve problems is called scientific inquiry.

UNIT 3 DENSITY STRUCTURE S AND ISOTOPES

Module 5: Rise and Fall of the Clockwork Universe. You should be able to demonstrate and show your understanding of:

Unit 1: Analyzing Data 1. Measure the following using the appropriate number of significant digits. Name Hour Date. b. o C

PowerPoint Presentation by: Associated Technical Authors. Publisher The Goodheart-Willcox Company, Inc. Tinley Park, Illinois

First some important preliminary business...

Physical Science Jeopardy!

Energy. on this world and elsewhere. Instructor: Gordon D. Cates Office: Physics 106a, Phone: (434)

CHEM 116 Phase Changes and Phase Diagrams

Conceptual Physics Fundamentals

Recap. There are 3 different temperature scales: Celsius, Kelvin, and Fahrenheit

Observation information obtained through the senses; observation in science often involves measurement

PE = mgh. Potential energy. What is g here? Let s pick up where we left off last time..the topic was gravitational potential energy

may contain one or more neutrons

GLOSSARY OF PHYSICS TERMS. v-u t. a =

WELCOME TO PERIOD 5: THERMAL ENERGY, THE MICROSCOPIC PICTURE. Homework #4 is due today at the beginning of class.

ORGANIC CHEMISTRY. Serkan SAYINER, DVM PhD, Assist. Prof.

PSC 1121 Spring 2017 Final Exam Review

MATTER AND HEAT. Chapter 4 OUTLINE GOALS

Matter & Thermodynamics

CHAPTER 2--LIFE'S CHEMICAL BASIS

Ch(3)Matter & Change. John Dalton

Lecture 3: Light and Temperature

Chapter 5: Thermochemistry. Problems: , , 5.100, 5.106, 5.108, , 5.121, 5.126

Chapter 6: The States of Matter

the energy of motion!

Unit 4: Gas Laws. Matter and Phase Changes

CHEM 116 Phase Changes and Phase Diagrams

Bernoulli s Principle. Application: Lift. Bernoulli s Principle. Main Points 3/13/15. Demo: Blowing on a sheet of paper

Chapter 21: Temperature, Heat and Expansion

The SI unit for Energy is the joule, usually abbreviated J. One joule is equal to one kilogram meter squared per second squared:

Colorado High School Physical Science Standards Foundations of Physical Science, 3rd Edition

Kinds of Energy. Defining Energy is Hard! EXPLAIN: 1. Energy and Radiation. Conservation of Energy. Sco; Denning CSU ESMEI ATS 1

Mr Chiasson Advanced Chemistry 12 / Chemistry 12 1 Unit B: Thermochemical Changes

Atmospheric Basics Atmospheric Composition

CHAPTER 6 - WATER (continued)

Archimedes Principle

CIE Physics IGCSE. Topic 2: Thermal Physics

Page 1 SPH3U. Heat. What is Heat? Thermal Physics. Waterloo Collegiate Institute. Some Definitions. Still More Heat

Properties of Matter

Today. Work, Energy, Power loose ends Temperature Second Law of Thermodynamics

15 Energy and Chemical Change BIGIDEA Write the Big Idea for this chapter.

Name Hour Date. B. Provide an example for the labs that we did to support your explanation.

Chapter 10, Thermal Physics

Key Idea 3: Matter is made up of particles whose properties determine the observable characteristics of matter and its reactivity.

States of matter. Book page , Syllabus /09/2016

3.2 Units of Measurement > Chapter 3 Scientific Measurement. 3.2 Units of Measurement. 3.1 Using and Expressing Measurements

Matter: Properties and Change

Build Your Own Planet Lesson 4: Atmosphere

Gases have important properties that distinguish them from solids and liquids:

Physics 107. Ideas of Modern Physics. Physics for Future Presidents. 1/22/10 Carlsmith, Physics 107

Clicker Question: Momentum. If the earth collided with a meteor that slowed it down in its orbit, what would happen: continued from last time

Transcription:

Topic #4 ENERGY & MATTER OVERVIEW OBJECTIVES: To review basic physical concepts of energy and matter and some key ways in which they interact. CLASS NOTES: pp 21-25

Science shows us that the visible world is neither matter nor spirit; the visible world is the invisible organization of energy. Heinz R. Pagels (b. 1939), U.S. Physicist p 21

LINK TO GLOBAL CHANGE: These concepts provide the foundation for understanding: a) the important energy fluxes (transfers) in the Sun-Earth-Atmosphere system, and b) the important moisture fluxes and phase changes of water (H 2 O) at the Earth-Atmosphere interface.

QUICK ENERGY REVIEW p 21

Energy Terms & Units Energy (def) = the quality of an object that enables it to do work; the ability to do work. Force (def) - A push or pull that, acting alone, causes a change in acceleration of the object on which it acts. p 21

Energy Unit Review Joule (or J) is the physical measurement for work. One joule equals the work needed to lift one kilogram (2.22 pounds) ten centimeters off the ground. It can also be used to measure heat energy. One kilocalorie, an older energy unit, equals 4.1868 kilojoules. Calorie (def) = the amount of heat required to raise 1 gram of room-temperature water 1 degree Celsius in temperature 1 calorie = 4.186 joules 1 calorie per second = 4.186 watts (1 calorie in nutrition context = 1000 calories = 1 kilogram calorie or kilocalorie (Kcal) HOW MUCH ENERGY IN A HURRICANE? http://www.aoml.noaa.gov/hrd/tcfaq/d7.html p 21

Work (def)- Work (W) is done whenever a force (F) is exerted over a distance (d). Work is equal to the force that is exerted times the distance over which it is exerted: POWER = W work = F done x d divided by the time it takes to do it: P = W / t The POWER of A Hurricane! http://www.nhc.noaa.gov/ p 21

Different Forms of Energy Kinetic (KE or KinE) = energy of motion; the ability of a mass to do work. KE = ½ (mass x velocity 2 ) or KinE = (1/2) ms 2 Potential (PE) = energy a system possess if it is capable of doing work, but is not doing work now Includes: gravitational, elastic, chemical, electrical, l magnetic, nuclear, thermal p 21

Forms of Energy Gravitational PE = energy associated with the position of a mass in a gravitational field, energy stored by virtue of its position GravE = weight x height = wt x ht Compare with: KinE = (1/2) mass x speed 2 p 22

GravE KinE ENERGY IS CONSERVED!

Which figure below depicts an energy flow diagram that t properly illustrates t the energy transformations that occur with a falling book? X Y Z

THERMAL ENERGY Thermal energy (internal energy) = The TOTAL ENERGY (kinetic + potential) of the particles that make up a substance. Atoms and molecules are constantly jiggling in some sort of back-and-forth vibratory motion (i.e., they have kinetic energy, KE) p 22

The Law of Conservation o of Energy: "energy cannot be created or destroyed; it can be transformed from one form to another but the total amount of energy never changes." Efficiency: Although energy may not be destroyed, it can become inefficient i -- i.e., is not easily used or available to do work! Efficiency = work done / energy used p 22

QUICK MATTER REVIEW p 23

Matter: Whatever occupies space & is perceptible p to the senses; made up of atoms; matter can be in form of solids, liquids, or gases p 23

Atom: H -- Fundamental building blocks for all matter -- the smallest representative sample of an element. Element: A chemical substance (material) made from a single type of atom that cannot be broken down any further and still maintain its identity as that element... as in the Periodic Table of the Elements p 23

Molecule: -- Any collection of two or more atoms bound together -- a cluster of atoms bound together MOLECULES are the basic constituent of different kinds of materials. -- the smallest part of any substance that has all the chemical ca properties es of the substance e.g., g, a water molecule = H 2O p 23

STATES OF MATTER Solid: -- a substance that resists changes of shape and volume -- characterized by structure in the particular order and bonding of atoms that make up the material Example = a crystal in which the molecules are locked into a strict geometrical order. p 23

Various Representations of Molecules arranged in a SOLID top down view of water (H 2 O) arranged in solid (ice) form 3-D view of a solid crystal structure top down view of a Neon crystal

Liquid: -- a substance that flows freely in response to unbalanced forces -- molecules more or less move freely past one another as individuals or small groups -- are not confined to fixed positions (as in solids) -- LIQUIDS CAN EXHIBIT PRESSURE (pressure = a force per unit area)... and will take the shape of the container they are in. p 23

Various Representations of Molecules arranged in a LIQUID

Gas: -- a substance that expands (and contracts) easily, rapidly, and indefinitely -- fills all space available to it -- takes the shape of its container -- the distance between molecules is such that no cohesive forces exist -- atoms or molecules are in high speed motion -- many collisions and rebounds occur -- GASES ALSO EXHIBIT PRESSURE p 23

Various Representations of Molecules arranged in a GAS

Heat added = increase in total energy + work done against outside pressure With increasing T (temperature) Volume increases & Density decreases COLD WARM HOT

At higher air temperatures, H 2O molecules collide & rebound more frequently, leading to expansion of the air & the water vapor in the air. At lower air temperatures as air gets more dense, H 2 O molecules are more likely to bond so that a phase change to liquid water or even solid ice can occur.

SUMMARY: SOLID LIQUID GAS

KEY CONCEPT #1: ENERGY & MATTER INTERACT The change in the state of a substance - from a solid to a liquid form, or - from a liquid to a gaseous form, (or vice versa) is called a CHANGE OF STATE or PHASE CHANGE. Thermal energy is involved in phase changes. p 21

PHASE CHANGES in H 2 O ICE WATER (more on this later in the semester)

H 2 O s UNIQUE EXCEPTION at ~ 0º-4 ºC to rule of: heating expansion cooling contraction ice water PHASE CHANGE Volume decreases upon heating (in a short range of temperatures) when the phase change occurs from ice to liquid water (due to collapsing ice crystals)

A Simple Demo : http://www.colorado.edu/physics/2000/bec/temperature.html WHAT DOES THIS HAVE TO DO WITH GLOBAL CHANGE & MY DAILY LIFE?????

FEDERAL STANDARD: Fuel at gas pump should be dispensed into a vehicle s tank at a temperature of 60 ºF The U.S. government defined volume of a gallon of gas: If temperature is not 60 º F, the cost of a gallon should be adjusted to reflect the volume of fuel at 60 º F. http://articles.latimes.com/2008/may/23/business/fi-hotfuel23 At 60 degrees, a gallon is 231 cubic inches. But when fuel is warmer than 60 degrees, the liquid expands, yielding less energy per gallon.

Rules of physics cost us money!! Basic physics! Depending on the temperature, the difference can amount to a few cents per gallon........ But it adds up to big money coming straight out of consumers' pockets.

Now let s focus on the atoms themselves and their internal structure... p 23

ATOMIC STRUCTURE: Electron Nucleus Proton Neutron p 22

ELECTRON: Tiny negatively charged particles that circle in orbits around a positively charged nucleus of an atom. The electron is an atomic particle with a negative charge and very low mass. NUCLEUS: The small, massive central part of an atom; it is made up of elementary particles that are even smaller p 22

PROTON: Positively charged nuclear particle. The atomic number of an atom is the number of protons, or units of positive charge, in the nucleus. If the atom is neutral -- the atomic number is also equivalent to the number of electrons. NEUTRON: Electrically neutral nuclear particle, approximately equal in mass to a proton. (Both protons and neutrons have much greater relative mass than electrons. ) The mass number of an atom is the total number of protons and neutrons in the nucleus of the atom. p 23

Schematic dot diagram of an oxygen atom Fill in blanks on p 24 A = ELECTRON B = NUCLEUS # electrons = 8 # protons = 8 # neutrons = 8 atomic # = 8 p 24

Review the details about shells and energy levels on p25 (on your own later if necessary) shells or energy levels

THE PLANETARY MODEL OF THE ATOM p 24

The BOHR MODEL OF THE ATOM: According to Neils Bohr's model of the atom, electrons circling the nucleus cannot maintain their orbits at just any distance from the center of the atom (the early model). p 25 (1 st bullet)

There are only certain "allowed orbits" - in which hihan electron can exist it for long periods of time without giving off radiation. - As long as the electron remains at one of these distances, its energy is fixed. VS. p 25

Schematic Diagrams representing ELECTRON ENERGY STATES (Shells) for Hydrogen H in the Bohr model : GROUND State Excited State 1 Excited State 2 p 25

-- The empty spaces represent areas with little likelihood of finding an electron -- Dark areas represent places (or energy levels) where electrons are allowed to be... but how do they get from one level to another??? p 25

The quantum model of the atom states that: electrons can exist only in discrete allowed places within shells (or energy levels) and not in between. p 24

The electrons move -- NOT according to Newtonian laws of motion -- but according to quantum mechanics. MORE on how this happens and what it has to do with GLOBAL CLIMATE CHANGE next week!! p 25

A little rusty on atoms, elements, shells, and the Periodic Table? See pp 109-113 113 in Class Notes This is an ungraded on your own review activity answers will be posted this weekend. You may need to know this for a future test... So do the review if you need it! Class Notes Appendix p 109-113

GROUP ACTIVITY G-1 GROUP ECOLOGICAL FOOTPRINT

ASSIGNMENT G-1 GROUP ECOLOGICAL FOOTPRINTS GET GROUP FOLDER (color coded) EVERYONE SIGN YOUR NAME inside the GROUP FOLDER First in alphabet in your group is TODAY s GROUP LEADER. Your job is to keep the discussion going and get assignment done! GO AROUND THE CIRCLE AND INTRODUCE YOURSELF: where from, major (if known) Ecological Footprint! WORK ON G-1 TOGETHER GROUP LEADER appoints a RECORDER, who is responsible for getting all the info on the form, although each student will write in something! REPORT BACK TO CLASS ON GROUP S TOTAL FOOTPRINT. NOTE: Leave your I-1 s in the folder and submit G-1 by leaving it in your group folder. NEVER TAKE YOUR GROUP FOLDERS OUT OF THE CLASSROOM!

Here s the Group Seating Here s the Group Seating Arrangment

RE-CAP of ANNOUNCEMENTS RQ-1 was cutoff at 30 minutes before class TODAY. Missed the cutoff deadline? See FAQ #22 Be sure you have submitted the Practice RQ on the Syllabus & FAQ with a perfect score of 7/7 by midnight tonight to earn one point on Assignment I-1 OFFICE HOURS are now in operation for Dr H and the GTA s See the hours on the TEACHING TEAM link. RQ-2 is due next Thursday (Sep 10) 30 minutes before class begins. (For those still without textbooks, if necessary, I will post the required chapter in a password-protected protected PDF next week) Have a Great Weekend... GO CATS!