PHYSICS. IGCSE Physics. Contact for further information. Dr JL Chapman:
|
|
- Julian Craig
- 7 years ago
- Views:
Transcription
1 PHYSICS Contact for further information Dr JL Chapman: IGCSE Physics Pupils are taught all their lessons by specialist Physics teachers and we currently cover the Edexcel IGCSE specification which includes the following topics:- Forces and Motion Electricity and Electromagnetism Energy Resources and Energy Transfer Solids, Liquids and Gases Radioactivity and Particles Practical work is done extensively throughout the course and assessment is 100% by two terminal written examination papers. IGCSE Physics prepares pupils well for IB Diploma or A Levels. Further details of the specification can be found using the link below.
2 A Level Physics Course description We will be following the AQA Physics specification. This is linear course covering the following topics:- Measurement and their errors Particles and Radiation Waves Mechanics and Materials Electricity Further Mechanics Thermal Physics Fields and their Consequences Nuclear Physics The students are also required to carry out practical work throughout the course including 12 compulsory practical activities. Knowledge of these experiments and the way that experimental data is collected and analysed will be assessed in one of the final written papers. In addition the students study one optional topic. Wellington students usually study for the Astrophysics option but we may be able to offer a second option depending on teacher specialism. Further details of the specification can be found by following the link below. Requirements for A Level Physics Pupils must have attained at least an A* grade in GCSE or IGCSE Physics or the MYP equivalent. GCSE or IGCSE Maths at A* grade is also essential and students will find that studying A level Maths alongside their Physics is advisable. Assessment Structure Assessment is via three written papers at the end of the two year course. Paper 1. This paper assesses measurement and their errors, particles and radiation, waves, mechanics and materials, electricity, and periodic motion. (Short and long questions and multiple choice.) Paper 2. This paper assesses thermal physics, fields and their consequences and nuclear physics. (Short and long answers and multiple choice.) Paper 3. This paper assesses practical skills and data analysis and the additional optional topic. (Short and long answers.) Potential Careers Physics is a well-respected and intellectually challenging subject. Physics graduates go onto a wide variety of careers from banking and finance to industry to teaching. An A Level in Physics will be looked upon favourably by many university admissions tutors across a breadth of courses but is usually a prerequisite for engineering courses, and single or joint honours Physics degrees.
3 IB Physics Course description The course presents the best aspects of traditional physics along with modern concepts in an exciting and flexible way. Pupils will question the way they learn, reflecting on how knowledge and understanding are obtained. Pupils will also be expected to explore ideas, investigate different physical situations by means of simulation, modelling and experimentation and to develop key skills, such as: analysis and presentation of data, communication and empathy with peers and scientific researchers and educators. Standard Level The course covers the following core topics:- Measurement and Uncertainties Mechanics Thermal Physics Waves Electricity and Magnetism Circular Motion and Gravitational Fields Atomic, Nuclear and Particle Physics Energy Production. The students also study an additional optional topic. Options which the teacher could choose include Astrophysics, Engineering Physics, Imaging or Relativity. The students are also required to carry out practical work throughout the course which will be assessed in the final written papers and via an individual internal assessment practical project. They will also have the chance to work with students studying other IB Science courses via the practical Group 4 project. Higher Level The course covers all of the core material studied by Standard Level students (listed above.) In addition, Higher Level students cover the following topics:- Wave Phenomena Fields Electromagnetic Induction Quantum and Nuclear Physics The students also study an additional optional topic. Options which the teacher could choose include Astrophysics, Engineering Physics, Imaging or Relativity. The students are also required to carry out practical work throughout the course which will be assessed in the final written papers and via an individual internal assessment practical project. They will also have the chance to work with students studying other IB Science courses via the practical Group 4 project. Assessment structure for SL and HL 20% of the overall mark is for the individual internal assessment practical project. The remaining 80% of the assessment is via three written/multiple choice papers at the end of the two year course. Requirements
4 Pupils must have attained at least an A* grade in IGCSE or GCSE Physics or the MYP equivalent and have a strong understanding of scientific principles. IGCSE or GCSE Maths at A* is also essential. Perhaps more importantly, successful pupils will be highly motivated, well organised, industrious, open-minded and inquisitive. The course and the individual assessment practical project, in particular, require all of these attributes. Potential careers The successful Physics pupil will find a wide range of careers open up. Skills acquired on the course, along with the discipline and rigour of the core material, will allow pupils to consider a range of future pathways, from university courses in science, business or language to direct employment in city, or country, environments in this country or abroad.
5 IB Astronomy (SL only) Astronomy is only available as a standard level course within the IB (group 4) It is most likely to appeal to two types of pupil Those who are wanting a group 4 subject to complete the IB but for whom the traditional science subjects do not appeal. For these pupils, perhaps Astronomy will offer a fresh and interesting subject. Higher level Physics students in the IB who would like to take two group 4 subjects to play to their strengths. These pupils will find that Astronomy supports their Physics studies and vice versa. The course is split into 4 units. The Stars This topic looks at our star, the Sun, and the processes by which it functions. The topic goes on to examine how we can measure stars and deduce their luminosity, size, mass etc... Finally the topic looks at the life of stars from their birth from a collapsing nebula through its main-sequence lifetime and ultimate demise and possible supernova forming white dwarfs, neutron stars or even black holes. The Planets This topic discusses different theories to explain the formation of the solar system. It continues with a discussion of how life began on Earth and why the conditions of Venus and Mars are so different. We then consider how life has subsequently changed the Earth's atmosphere further. The topic finishes with a consideration of the search for extra-terrestrial life and how we might identify environments where life could exist and how we might detect it. Galaxies The topic starts with an examination of our own galaxy as a basis on which to describe other galaxies, The topic continues to examine how other galaxies are classified and how they differ. this sub-topic concludes with an examination of the evidence for galactic dark matter and what the options for it are. The topic then considers active galaxies, what they are and how they are important to our understanding of the beginnings of the universe. Cosmology The final topic examines the largest scales of all from the large scale structures of the universe and the fundamental shape of space-time. The topic examines the birth, life and ultimate death of the universe and our observations and evidence for these theories.
Science Standard 4 Earth in Space Grade Level Expectations
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
More informationSYLLABUS FORM WESTCHESTER COMMUNITY COLLEGE Valhalla, NY l0595. l. Course #:PHYSC 151 2. NAME OF ORIGINATOR /REVISOR: PAUL ROBINSON
SYLLABUS FORM WESTCHESTER COMMUNITY COLLEGE Valhalla, NY l0595 l. Course #:PHYSC 151 2. NAME OF ORIGINATOR /REVISOR: PAUL ROBINSON NAME OF COURSE: ASTRONOMY 3. CURRENT DATE: OCTOBER 26, 2011. Please indicate
More informationOrigins of the Cosmos Summer 2016. Pre-course assessment
Origins of the Cosmos Summer 2016 Pre-course assessment In order to grant two graduate credits for the workshop, we do require you to spend some hours before arriving at Penn State. We encourage all of
More informationClass 2 Solar System Characteristics Formation Exosolar Planets
Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System
More informationScience Investigations: Investigating Astronomy Teacher s Guide
Teacher s Guide Grade Level: 6 12 Curriculum Focus: Astronomy/Space Duration: 7 segments; 66 minutes Program Description This library of videos contains seven segments on celestial bodies and related science.
More informationProgramme Specification Mphys (Hons) Physics with Astronomy
Programme Specification Mphys (Hons) Physics with Astronomy 1 Awarding Institution 2 Teaching Institution 3 Programme Accredited by 4 Final Award 5 Programme title 6 UCAS Code 7 QAA Subject Benchmark 8
More informationDegrees in Science (& Physics)
Degrees in Science (& Physics) NUI, Galway College of Science National University of Ireland, Galway Revised January 2008 3 The world has changed...it has become FLAT! Geography no longer matters. Three
More informationThe University of Texas at Austin. Gravity and Orbits
UTeach Outreach The University of Texas at Austin Gravity and Orbits Time of Lesson: 60-75 minutes Content Standards Addressed in Lesson: TEKS6.11B understand that gravity is the force that governs the
More informationUndergraduate Studies Department of Astronomy
WIYN 3.5-meter Telescope at Kitt Peak near Tucson, AZ Undergraduate Studies Department of Astronomy January 2014 Astronomy at Indiana University General Information The Astronomy Department at Indiana
More informationThe Hidden Lives of Galaxies. Jim Lochner, USRA & NASA/GSFC
The Hidden Lives of Galaxies Jim Lochner, USRA & NASA/GSFC What is a Galaxy? Solar System Distance from Earth to Sun = 93,000,000 miles = 8 light-minutes Size of Solar System = 5.5 light-hours What is
More informationEarth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs
Earth Sciences -- Grades 9, 10, 11, and 12 California State Science Content Standards Covered in: Hands-on science labs, demonstrations, & activities. Investigation and Experimentation. Lesson Plans. Presented
More informationCalifornia Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping
California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,
More information1 A Solar System Is Born
CHAPTER 3 1 A Solar System Is Born SECTION Formation of the Solar System BEFORE YOU READ After you read this section, you should be able to answer these questions: What is a nebula? How did our solar system
More informationUNL71 Physics Neil Lister; BSc, Dip, Ed.
UNL71 Physics Your Teacher for Unilearn Physics is Neil Lister; BSc, Dip, Ed. Neil has taught at least 1 physics course at Sunnybank S.H.S. every year from 1971 until he retired from full time teaching
More informationUndergraduate Degree Programs in the Department of Physics and Astronomy
UNIVERSITY OF PITTSBURGH DIETRICH SCHOOL OF ARTS AND SCIENCES DEPARTMENT OF PHYSICS AND ASTRONOMY Undergraduate Degree Programs in the Department of Physics and Astronomy Updated 8/17/2015 This document
More informationIntroduction. IGCSE Physics. The Course. Physics IGCSE
Physics IGCSE IGCSE Physics Welcome to your IGCSE Physics course. This introduction will serve as a guide to what you can expect from the course, and it will show you how to plan your study effectively.
More informationGrade Level Expectations for the Sunshine State Standards
for the Sunshine State Standards FLORIDA DEPARTMENT OF EDUCATION http://www.myfloridaeducation.com/ The seventh grade student: The Nature of Matter uses a variety of measurements to describe the physical
More informationDiscover the Universe AST-1002 Section 0427, Spring 2016
Discover the Universe AST-1002 Section 0427, Spring 2016 Instructor: Dr. Francisco Reyes Office: Room 12 Bryant Space Science Center Telephone: 352-294-1885 Email: freyes@astro.ufl.edu Office hours: Monday
More informationStudy Guide: Solar System
Study Guide: Solar System 1. How many planets are there in the solar system? 2. What is the correct order of all the planets in the solar system? 3. Where can a comet be located in the solar system? 4.
More informationPlease note that only the German version of the Curriculum is legally binding. All other linguistic versions are provided for information only
Please note that only the German version of the Curriculum is legally binding. All other linguistic versions are provided for information only Curriculum for the Erasmus Mundus Joint Master Program in
More informationPHYS 1624 University Physics I. PHYS 2644 University Physics II
PHYS 1624 Physics I An introduction to mechanics, heat, and wave motion. This is a calculus- based course for Scientists and Engineers. 4 hours (3 lecture/3 lab) Prerequisites: Credit for MATH 2413 (Calculus
More informationThe facts we know today will be the same tomorrow but today s theories may tomorrow be obsolete.
The Scale of the Universe Some Introductory Material and Pretty Pictures The facts we know today will be the same tomorrow but today s theories may tomorrow be obsolete. A scientific theory is regarded
More informationThe Expanding Universe
Stars, Galaxies, Guided Reading and Study This section explains how astronomers think the universe and the solar system formed. Use Target Reading Skills As you read about the evidence that supports the
More informationWhere is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014
Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014 Disclaimer We do not know what will be discovered. This is the reason we perform experiments. This is the reason scientific research
More informationPretest Ch 20: Origins of the Universe
Name: _Answer key Pretest: _2_/ 58 Posttest: _58_/ 58 Pretest Ch 20: Origins of the Universe Vocab/Matching: Match the definition on the left with the term on the right by placing the letter of the term
More informationOnline Courses for High School Students 1-888-972-6237
Online Courses for High School Students 1-888-972-6237 PHYSICS Course Description: This course provides a comprehensive survey of all key areas: physical systems, measurement, kinematics, dynamics, momentum,
More information1 SCIENCE AND NATURAL PHILOSOPHY BEFORE THE 17 TH CENTURY
1 SCIENCE AND NATURAL PHILOSOPHY BEFORE THE 17 TH CENTURY FOR TEACHERS Lesson Title: Science and Natural Philosophy Before the Seventeenth Century Area of Learning: chronology, states of affairs Aims.
More informationIndiana's Academic Standards 2010 ICP Indiana's Academic Standards 2016 ICP. map) that describe the relationship acceleration, velocity and distance.
.1.1 Measure the motion of objects to understand.1.1 Develop graphical, the relationships among distance, velocity and mathematical, and pictorial acceleration. Develop deeper understanding through representations
More informationCurriculum Overview IB Physics SL YEAR 1 JUNIOR TERM I (2011)
Curriculum Overview IB Physics SL YEAR 1 JUNIOR TERM I (2011) Resources: Gregg Kerr, Nancy Kerr, (2004) Physics International Baccalaureate, IBID Press, Victoria, Australia. Tim Kirk and Neil Hodgson Physics
More informationMASTER OF SCIENCE IN PHYSICS MASTER OF SCIENCES IN PHYSICS (MS PHYS) (LIST OF COURSES BY SEMESTER, THESIS OPTION)
MASTER OF SCIENCE IN PHYSICS Admission Requirements 1. Possession of a BS degree from a reputable institution or, for non-physics majors, a GPA of 2.5 or better in at least 15 units in the following advanced
More information165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars
Name Date Period 30 GALAXIES AND THE UNIVERSE SECTION 30.1 The Milky Way Galaxy In your textbook, read about discovering the Milky Way. (20 points) For each item in Column A, write the letter of the matching
More information7. In which part of the electromagnetic spectrum are molecules most easily detected? A. visible light B. radio waves C. X rays D.
1. Most interstellar matter is too cold to be observed optically. Its radiation can be detected in which part of the electromagnetic spectrum? A. gamma ray B. ultraviolet C. infrared D. X ray 2. The space
More informationUNIT V. Earth and Space. Earth and the Solar System
UNIT V Earth and Space Chapter 9 Earth and the Solar System EARTH AND OTHER PLANETS A solar system contains planets, moons, and other objects that orbit around a star or the star system. The solar system
More informationGRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter
IT S UNIVERSAL GRAVITY CONCEPTS Gravity is the universal force of attraction between all matter Weight is a measure of the gravitational force pulling objects toward Earth Objects seem weightless when
More informationRadiation and the Universe Higher Exam revision questions and answers
Radiation and the Universe Higher Exam revision questions and answers Madeley High School Q.The names of three different processes are given in List A. Where these processes happen is given in List B.
More informationThe Messier Objects As A Tool in Teaching Astronomy
The Messier Objects As A Tool in Teaching Astronomy Dr. Jesus Rodrigo F. Torres President, Rizal Technological University Individual Member, International Astronomical Union Chairman, Department of Astronomy,
More informationUniversity of the Arts London (UAL) BA (Hons) Animation Communication, Media, Film and Cultural Studies Date of production/revision July 2015
Programme Specification Every taught course of study leading to a UAL award is required to have a Programme Specification. This summarises the course aims, learning outcomes, teaching, learning and assessment
More informationThe content is based on the National Science Teachers Association (NSTA) standards and is aligned with state standards.
Literacy Advantage Physical Science Physical Science Literacy Advantage offers a tightly focused curriculum designed to address fundamental concepts such as the nature and structure of matter, the characteristics
More informationPreview of Period 2: Forms of Energy
Preview of Period 2: Forms of Energy 2.1 Forms of Energy How are forms of energy defined? 2.2 Energy Conversions What happens when energy is converted from one form into another form? 2.3 Efficiency of
More informationFinal. Mark Scheme. Additional Science / Physics (Specification 4408 / 4403) PH2FP. Unit: Physics 2
Version.0 General Certificate of Secondary Education January 203 Additional Science / Physics (Specification 4408 / 4403) Unit: Physics 2 Final Mark Scheme Mark schemes are prepared by the Principal Examiner
More informationUnderstanding the UK education system
Understanding the UK education system The education system in the UK is currently undergoing perhaps more change than at any time since the 1944 Butler Education Act. There are now a huge range of schools
More informationFriday 20 January 2012 Morning
THIS IS A NEW SPECIFICATION H Friday 20 January 2012 Morning GCSE TWENTY FIRST CENTURY SCIENCE PHYSICS A A181/02 Modules P1 P2 P3 (Higher Tier) *A131500112* Candidates answer on the Question Paper. A calculator
More informationAstronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:
Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007 Name: Directions: Listed below are twenty (20) multiple-choice questions based on the material covered by the lectures this past week. Choose
More informationCosmic Journey: Teacher Packet
Cosmic Journey: Teacher Packet Compiled by: Morehead State University Star Theatre with help from Bethany DeMoss Table of Contents Table of Contents 1 Corresponding Standards 2 Vocabulary 4 Sizing up the
More informationBig bang, red shift and doppler effect
Big bang, red shift and doppler effect 73 minutes 73 marks Page of 26 Q. (a) Scientists have observed that the wavelengths of the light from galaxies moving away from the Earth are longer than expected.
More informationTHE SOLAR SYSTEM Syllabus
THE SOLAR SYSTEM Syllabus Course Title The Solar System: Earth and Space Science Course Description This course provides an overview of what we know about the Solar System: how it began and evolved, its
More informationOne Stop Shop For Teachers
Physical Science Curriculum The Georgia Performance Standards are designed to provide students with the knowledge and skills for proficiency in science. The Project 2061 s Benchmarks for Science Literacy
More informationAZ State Standards. Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred.
Forms of Energy AZ State Standards Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred. PO 1. Describe the following ways in which
More informationWhat Does a Physics Degree Actually Mean?
DEPARTMENT OF PHYSICS AND ASTRONOMY Brandon University Faculty of Science Department of Physics & Astronomy Phone (204) 727-9680 Fax (204) 728-7346 www.brandonu.ca/physics This document is meant as a planning
More informationUnit 2 Lesson 1 Introduction to Energy. Copyright Houghton Mifflin Harcourt Publishing Company
Get Energized! What are two types of energy? Energy is the ability to cause change. Energy takes many different forms and causes many different effects. There are two general types of energy: kinetic energy
More informationAppendix A: Science Practices for AP Physics 1 and 2
Appendix A: Science Practices for AP Physics 1 and 2 Science Practice 1: The student can use representations and models to communicate scientific phenomena and solve scientific problems. The real world
More informationNeutron Stars. How were neutron stars discovered? The first neutron star was discovered by 24-year-old graduate student Jocelyn Bell in 1967.
Neutron Stars How were neutron stars discovered? The first neutron star was discovered by 24-year-old graduate student Jocelyn Bell in 1967. Using a radio telescope she noticed regular pulses of radio
More information8.1 Radio Emission from Solar System objects
8.1 Radio Emission from Solar System objects 8.1.1 Moon and Terrestrial planets At visible wavelengths all the emission seen from these objects is due to light reflected from the sun. However at radio
More informationTaught Postgraduate programmes in the School of Physics and Astronomy
Astrophysics (MSc) Theoretical Physics (MSc) Physics: Advanced Materials (MSc) Physics: Energy and the Environment (MSc) Physics: Global Security (MSc) Physics: Life Sciences (MSc) Physics: Nuclear Technology
More informationChapter 1 Student Reading
Chapter 1 Student Reading Chemistry is the study of matter You could say that chemistry is the science that studies all the stuff in the entire world. A more scientific term for stuff is matter. So chemistry
More informationData Provided: A formula sheet and table of physical constants is attached to this paper. DARK MATTER AND THE UNIVERSE
Data Provided: A formula sheet and table of physical constants is attached to this paper. DEPARTMENT OF PHYSICS AND ASTRONOMY Autumn Semester (2014-2015) DARK MATTER AND THE UNIVERSE 2 HOURS Answer question
More informationPhysical Therapy 602-523-4092
320 Physics and Astronomy PHI 351 Philosophy in Literature (3). Philosophical issues as expressed in the novel, drama, and poetry. Fall or Spring. PHI 352 Philosophy of Religion (3). Problems concerning
More informationCarol and Charles see their pencils fall exactly straight down.
Section 24-1 1. Carol is in a railroad car on a train moving west along a straight stretch of track at a constant speed of 120 km/h, and Charles is in a railroad car on a train at rest on a siding along
More informationThe Solar System. Source http://starchild.gsfc.nasa.gov/docs/starchild/solar_system_level1/solar_system.html
The Solar System What is the solar system? It is our Sun and everything that travels around it. Our solar system is elliptical in shape. That means it is shaped like an egg. Earth s orbit is nearly circular.
More informationSummary: Four Major Features of our Solar System
Summary: Four Major Features of our Solar System How did the solar system form? According to the nebular theory, our solar system formed from the gravitational collapse of a giant cloud of interstellar
More informationPHYSICAL WORLD. Heat & Energy GOD S DESIGN. 4th Edition Debbie & Richard Lawrence
PHYSICAL WORLD Heat & Energy GOD S DESIGN 4th Edition Debbie & Richard Lawrence God s Design for the Physical World is a complete physical science curriculum for grades 3 8. The books in this series are
More informationDepartment of Science Education and Mathematics Education
Department of Science Education and Mathematics Education http://www.utdallas.edu/dept/sci_ed/ Faculty Professors: Thomas R. Butts (interim head), Frederick L. Fifer, Jr., Russell Hulse Associate Professors:
More informationAstro 102 Test 5 Review Spring 2016. See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14
Astro 102 Test 5 Review Spring 2016 See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14 Sec 14.5 Expanding Universe Know: Doppler shift, redshift, Hubble s Law, cosmic distance ladder, standard candles,
More informationBeginning of the Universe Classwork 6 th Grade PSI Science
Beginning of the Universe Classwork Name: 6 th Grade PSI Science 1 4 2 5 6 3 7 Down: 1. Edwin discovered that galaxies are spreading apart. 2. This theory explains how the Universe was flattened. 3. All
More informationASTRONOMY and ASTROPHYSICS
UNDERGRADUATE CURRICULUM B. S. PROGRAM ASTRONOMY and ASTROPHYSICS MICHIGAN STATE UNIVERSITY February 2013 Prof. Daniel Stump Undergraduate Program Director Department of Physics and Astronomy Michigan
More informationMAKING SENSE OF ENERGY Electromagnetic Waves
Adapted from State of Delaware TOE Unit MAKING SENSE OF ENERGY Electromagnetic Waves GOALS: In this Part of the unit you will Learn about electromagnetic waves, how they are grouped, and how each group
More informationThe Physics Graduate Program
The Physics Graduate Program p. 1/3 The Physics Graduate Program Jacobus Verbaarschot, Graduate Program Director jacobus.verbaarschot@stonybrook.edu Stony Brook, August 2015 The Physics Graduate Program
More informationWorld of Particles Big Bang Thomas Gajdosik. Big Bang (model)
Big Bang (model) What can be seen / measured? basically only light (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)
More informationScope and Sequence Interactive Science grades 6-8
Science and Technology Chapter 1. What Is Science? 1. Science and the Natural World 2.Thinking Like a Scientist 3. Scientific Inquiry Scope and Sequence Interactive Science grades 6-8 Chapter 2. Science,
More informationIntroduction to the Solar System
Introduction to the Solar System Lesson Objectives Describe some early ideas about our solar system. Name the planets, and describe their motion around the Sun. Explain how the solar system formed. Introduction
More informationLecture 7 Formation of the Solar System. Nebular Theory. Origin of the Solar System. Origin of the Solar System. The Solar Nebula
Origin of the Solar System Lecture 7 Formation of the Solar System Reading: Chapter 9 Quiz#2 Today: Lecture 60 minutes, then quiz 20 minutes. Homework#1 will be returned on Thursday. Our theory must explain
More informationAn Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science
An Introduction to Astronomy and Cosmology 1) Astronomy - an Observational Science Why study Astronomy 1 A fascinating subject in its own right. The origin and Evolution of the universe The Big Bang formation
More informationChemical Building Blocks: Chapter 3: Elements and Periodic Table
Name: Class: Date: Chemical Building Blocks: Chapter 3: Elements and Periodic Table Study Guide Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.
More informationA Universe of Galaxies
A Universe of Galaxies Today s Lecture: Other Galaxies (Chapter 16, pages 366-397) Types of Galaxies Habitats of Galaxies Dark Matter Other Galaxies Originally called spiral nebulae because of their shape.
More informationTeaching Time: One-to-two 50-minute periods
Lesson Summary Students create a planet using a computer game and change features of the planet to increase or decrease the planet s temperature. Students will explore some of the same principles scientists
More informationIntroduction and Origin of the Earth
Page 1 of 5 EENS 1110 Tulane University Physical Geology Prof. Stephen A. Nelson Introduction and Origin of the Earth This page last updated on 30-Jul-2015 Geology, What is it? Geology is the study of
More informationProfessional Master of Science in Physics
Professional Master of Science in Physics UW Physics Department Information Session UW Professional MS in Physics Program Boeing Information Session - Agenda Welcome & Introductions The MS-Physics (PMSP)
More informationRelated Standards and Background Information
Related Standards and Background Information Earth Patterns, Cycles and Changes This strand focuses on student understanding of patterns in nature, natural cycles, and changes that occur both quickly and
More informationCHEMISTRY (CHEM & CLAB)
Interim Head of the Department: Associate Professor McCarthy Professors: Corkern, Holmes, Munchausen, Shaw Associate Professor: Doughty, Elbers, Parkinson, Robertson Assistant Professors: Allain, Belter,
More informationgalaxy solar system supernova (noun) (noun) (noun)
WORDS IN CONTEXT DAY 1 (Page 1 of 4) galaxy A galaxy is a collection of stars, gas, and dust. We live in the Milky Way galaxy. One galaxy may contain billions of stars. solar system A solar system revolves
More informationThis Performance Standards include four major components. They are
Eighth Grade Science Curriculum Approved July 12, 2004 The Georgia Performance Standards are designed to provide students with the knowledge and skills for proficiency in science at the eighth grade level.
More informationThe Universe. The Solar system, Stars and Galaxies
The Universe The Universe is everything. All us, the room, the U.S. the earth, the solar system, all the other stars in the Milky way galaxy, all the other galaxies... everything. How big and how old is
More informationSolar Energy Production
Solar Energy Production We re now ready to address the very important question: What makes the Sun shine? Why is this such an important topic in astronomy? As humans, we see in the visible part of the
More informationThursday 23 May 2013 Morning
THIS IS A NEW SPECIFICATION H Thursday 23 May 2013 Morning GCSE TWENTY FIRST CENTURY SCIENCE PHYSICS A A181/02 Modules P1 P2 P3 (Higher Tier) *A137270613* Candidates answer on the Question Paper. A calculator
More informationThe Physics Degree. Graduate Skills Base and the Core of Physics
The Physics Degree Graduate Skills Base and the Core of Physics Version date: September 2011 THE PHYSICS DEGREE This document details the skills and achievements that graduates of accredited degree programmes
More informationWELCOME to Aurorae In the Solar System. J.E. Klemaszewski
WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets
More informationProbes of Star Formation in the Early Universe
Gamma Ray Bursts Probes of Star Formation in the Early Universe Edward P.J.van den Heuvel Universiteit van Amsterdam &KITP-UCSB KITP, March 17, 2007 Age of the Universe: 13.7 billion years Age of our Milky
More informationUnit 8 Lesson 2 Gravity and the Solar System
Unit 8 Lesson 2 Gravity and the Solar System Gravity What is gravity? Gravity is a force of attraction between objects that is due to their masses and the distances between them. Every object in the universe
More informationDepartment of Mathematics
Department of Mathematics 220 Yost Hall http://www.case.edu/artsci/math Daniela Calvetti, Department Chair daniela.calvetti@case.edu The Department of Mathematics at Case Western Reserve University is
More informationEinstein s theory of relativity
Department of Mathematics, Institute of Origins, December 5, 2008 Overview UCL Institute of Origins Origins UCL has established the Institute of Origins to promote world leading research in topics related
More informationStellar Evolution: a Journey through the H-R Diagram
Stellar Evolution: a Journey through the H-R Diagram Mike Montgomery 21 Apr, 2001 0-0 The Herztsprung-Russell Diagram (HRD) was independently invented by Herztsprung (1911) and Russell (1913) They plotted
More informationGrade 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?
Grade 6 Standard 3 Unit Test A Astronomy Multiple Choice 1. The four inner planets are rocky and small. Which description best fits the next four outer planets? A. They are also rocky and small. B. They
More information9 th Grade Physical Science Springfield Local Schools Common Course Syllabi. Course Description
9 th Grade Physical Science Springfield Local Schools Common Course Syllabi Course Description The purpose of the Physical Science course is to satisfy the Ohio Core science graduation requirement. The
More informationInterpretation of Data (IOD) Score Range
These Standards describe what students who score in specific score ranges on the Science Test of ACT Explore, ACT Plan, and the ACT college readiness assessment are likely to know and be able to do. 13
More informationElements of Physics Motion, Force, and Gravity Teacher s Guide
Teacher s Guide Grade Level: 9 12 Curriculum Focus: Physical Science Lesson Duration: Three class periods Program Description Examine Isaac Newton's laws of motion, the four fundamental forces of the universe,
More informationFaculty of Science. Science Foundation at Reading
Faculty of Science Science Foundation Science Foundation Challenging and invaluable! Now I m well into Part 1 of my degree, I ve really come to see the value of completing the Foundation Year in Science.
More informationExplain the Big Bang Theory and give two pieces of evidence which support it.
Name: Key OBJECTIVES Correctly define: asteroid, celestial object, comet, constellation, Doppler effect, eccentricity, eclipse, ellipse, focus, Foucault Pendulum, galaxy, geocentric model, heliocentric
More informationREALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe
REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe The End of Physics Albert A. Michelson, at the dedication of Ryerson Physics Lab, U. of Chicago, 1894 The Miracle Year - 1905 Relativity Quantum
More informationMS. Structure and Properties of Matter
MIDDLE SCHOOL PHYSICAL SCIENCE Alignment with National Science Standards Use the chart below to find Science A-Z units that best support the Next Generation Science Standards* for Middle School Physical
More informationSection: Solar system / Earth and Moon
Project description for the national event for participation in the European Science on Stage festival from 25 28 April 2013 in Słubice Frankfurt (Oder) Project title: Main contact Astronomy in primary
More information