Learning Outcomes 2. Key Concepts 2. Misconceptions and Teaching Challenges 3. Vocabulary 4. Lesson and Content Overview 5

Similar documents
1 WHAT IS BIG HISTORY? WHY DO WE LOOK AT THINGS FROM FAR AWAY AND CLOSE UP?

Learning Outcomes 2. Key Concepts 2. Misconceptions and Teaching Challenges 3. Vocabulary 4. Lesson and Content Overview 5

CHARLES DARWIN 1 COMPLEXITY & XX THRESHOLDS 820L. 5 billion years ago 1 billion years ago 1million years ago billion.

5 LIFE HOW DO WE DEFINE LIFE AND WHAT DO WE KNOW ABOUT IT?

A Brief Guide to Our Cosmic Context

Explore! Fossils Original Air Date: January 28, 2015 Grade Levels: 3-6 Archived Program URL: Program Materials Page URL: Program Description:

WHAT IS BIG HISTORY? Video Talk / David Christian

Unit 2 Lesson 2: The Study of Pre-History

Todd Nussen - World History

Tell students that Earth is the only planet in our solar system known to have life. Ask:

Earth s Plates, Part 1: What Are They, Where Are They and What Do They Do?

Teacher Edition. Goldilocks. Baby Bear. and the Three Bears. alphakids. Goes for a Walk. Retold by Jenny Feely. Illustrated by Peter Paul Bajer

OUTSIDE THE SOLAR SYSTEM Outside the Solar System

Geology, Part 2: What Is the Mystery Rock?

Teachers Resources: Set One

Hunting for Planets. Overview. Directions. Content Created by. Activitydevelop. How can you use star brightness to find planets?

Subject: Geography Scheme of Work: B1 to B6 Mastery tiles. Term: Autumn/Spring/Summer

Our Solar System Unit of Work

Classroom Activities/Lesson Plan

ORBITAL REFLECTOR DARK SKIES LESSON GRADE: 9-12 LESSON: STANDARDS:

PS 101: Introductory Astronomy Fall 2014

Weather Observations. Weather Observations. 1 of 10. Copyright 2007, Exemplars, Inc. All rights reserved.

Your web browser (Safari 7) is out of date. For more security, comfort and. the best experience on this site: Update your browser Ignore

Inquiry Based Instruction Unit. Virginia Kromhout

SEEING LIKE AN ASTRONOMER grades 4 6

ASTRO 114 Lecture Okay. What we re going to discuss today are what we call radiation laws. We ve

Life on Other Worlds: The Drake Equation Author: Meagan Morscher GK-12 Reach for the Stars Fellow, Northwestern University

1. Engage students in a discussion about conditions that are necessary for life.

Big Bang, Black Holes, No Math

Amount of Substance and Its Unit Mole- Connecting the Invisible Micro World to the Observable Macro World Part 2 (English, mp4)

Overview of Modern Astronomy. Prof. D. L. DePoy

YEAR 5 EARTH AND SPACE PLANNING. History: history of astronomy

8 th Grade Earth and Space Science Megan Seivert, Virginia Standards of Learning Connections: Lesson Summary:

Someone's Been Eating My Porridge

Modeling Eclipses with Size and Distance Scales

Your web browser (Safari 7) is out of date. For more security, comfort and. the best experience on this site: Update your browser Ignore

Teacher s Guide For. Core Astronomy

Resource and Activity Pack. Discussion questions Comprehension exercise Lesson plans Activities

Follow the instructions to determine if your sample is metamorphic, sedimentary or igneous rock.

Master Syllabus Department of Geography GEOG 121: Geography of the Cultural Environment Course Description

History of the universe

Science Literacy: Reading and Writing Diagrams Video Transcript

Lesson Overview Activity video available at edu.zspace.com. Objectives

LESSON 1: WHAT IS ASTRONOMY

Parenting Tip of the Month. April. Lower Elementary Teachers

Earth, Earth s Moon, Mars Balloons Grades: Middle School Grade Prep Time: ~10 Minutes Lesson Time: 60 Mins

TIME: 45 minutes. LESSON: Curious About Clouds GRADE: 1 st SUMMARY:

News English.com Ready-to-use ESL / EFL Lessons

Introduction. THE FORMATION OF THE SOLAR SYSTEM - Theories Old and New Imperial College Press

Astronomy 001 Online SP16 Syllabus (Section 8187)

After completing the Orientation Overview exercises, you now know what this course is going to be about. You know what the course is going to cover.

LESSON 8: IT S ALL IN THE NAME WEATHER VERSUS CLIMATE

CLASSROOM SCIENCE ACTIVITY TO SUPPORT STUDENT ENQUIRY-BASED LEARNING

Module 8: The Cosmos in Motion. UNC-TFA H.S. Astronomy Collaboration, Copyright 2011

Leader Discussion Guide for Cosmos: A SpaceTime Odyssey

Bay Area Scientists in Schools Presentation Plan

Cupcake Geology adapted by Jess Krim from various sources

ESSENTIAL CONCEPTS AND SKILL SETS OF THE IOWA CORE CURRICULUM

Conceptual narrative Science: Earth in space

Early College High School PreAP World Geography Summer Reading Assignment

Chapter Three. Deciphering the Code. Understanding Notation

Geology, Part 1: Can You Categorize Different Types of Rocks?

MIT BLOSSOMS INITIATIVE

Teacher s Guide Listen to Literature

Moon's Orbit ACTIVITY OVERVIEW NGSS CONNECTIONS NGSS CORRELATIONS

Heat Transfer Lesson Plan

What Is It Like Outside?

The Big Bang and The Formation of the Universe. Earth Science- Where It All Began

ED 357/358 - FIELD EXPERIENCE - LD & EI LESSON DESIGN & DELIVERY LESSON PLAN #4

Life of a Star. Lesson development

THEME BASED HOLIDAY HOMEWORK

Part I---Introduction: planets, and habitable planets

What is proof? Lesson 1

1.What are the patterns of movement for the Sun and Moon across the sky? 2.How does Earth compare too other objects orbiting the Sun?

Understanding the Universe S TA R T ING WITH EARTH A ND B E YO ND

Major Languages of the Americas

ASTR : Stars & Galaxies (Spring 2019)... Study Guide for Midterm 1

The Scientific Method

Edible Rocks: How Can a Cookie Be a Model of a Rock?

Science Grade 01 Unit 07 Exemplar Lesson 02: Investigating the Moon, the Stars, and the Sky

Atomic Theory. Introducing the Atomic Theory:

Your web browser (Safari 7) is out of date. For more security, comfort and. the best experience on this site: Update your browser Ignore

Deep-Space Model. Outside the solar system. Purpose. Process Skills. Background. Time 45 minutes Grouping Pairs or small groups

Deep Algebra Projects: Algebra 1 / Algebra 2 Go with the Flow

2 THE SCIENTIFIC REVOLUTION IN ENGLAND AND EUROPE, Lesson Title: The Scientific Revolution in England and Europe,

Dear Teacher, Overview Page 1

Modern Physics notes Paul Fendley Lecture 1

QUANTUM CHEMISTRY BY R.K. PRASAD DOWNLOAD EBOOK : QUANTUM CHEMISTRY BY R.K. PRASAD PDF

Crossing the Event Horizon Presented by Nassim Haramein

Classroom Activities/Lesson Plan. Students will read supported and shared informational materials, including social

How can we use information to solve a societal problem?

Looking for Signs of Life. Overview. Directions. Content Created by. Activitydevelop. How do scientists determine whether a planet has life?

Lesson Plan Summary Magic Tree House #28: High Tide in Hawaii Standing on Solid Ground??

Claircognizance is the physic ability of clear knowing. This is perhaps the least understood of the Psychic Clairs.

Fascinating Fossils Grades 4-8

4 HOW DID THE EARTH FORM?

( )( b + c) = ab + ac, but it can also be ( )( a) = ba + ca. Let s use the distributive property on a couple of

Lesson 32. The Grain of Wheat. John 12:20-26

NAME: DATE: Leaving Certificate GEOGRAPHY: Maps and aerial photographs. Maps and Aerial Photographs

Student Questionnaire (s) Main Survey

Transcription:

UNIT 1 GUIDE Table of Contents Learning Outcomes 2 Key Concepts 2 Misconceptions and Teaching Challenges 3 Vocabulary 4 Lesson and Content Overview 5 BIG HISTORY PROJECT / UNIT 1 GUIDE 1

Unit 1 What Is Big History? Unit 1 Driving Question: Why do we look at things from far away and close up? Learning Outcomes 1. Define thresholds of increasing complexity, origin stories, and scale. 2. Understand that Big History is a modern, science-based origin story that draws on many different types of knowledge. 3. Understand how you fit into the Big History narrative, using the concept of thresholds to frame your past, present, and future and the history of the Universe. 4. Understand what disciplines are and consider the viewpoints of many different scholars about the same topic. Key Concepts Big History is a course that tells the story of the Universe from the Big Bang to the present, which means you and your students are going to be looking at billions of years of history. Because telling the story of the Universe covers so much time and so many topics, it will probably require a different approach than other courses you ve taught. Scale Seeing yourselves as part of the history of everything can help you and your students understand your place in the Universe. Big History brings together a broad range of historical accounts and many different temporal and spatial scales. In your own life, you can ask yourself, What is my first memory? Or you can ask about your family history or the history of your country. But you can also ask about the history of humanity, of life on Earth, or of the Solar System. In the same way, you can ask about the history of the entire Universe, and you can then try to see how all these stories fit together. Origin Stories Every society has its own history and origin stories. Origin stories focus on the most important questions of our existence; they tell us how all the components of our world were created, and by doing so they demonstrate how each of us is linked to everything else. Big History weaves evidence and insights from many scientific and historical disciplines into accessible origin stories that account for everything within the Universe. Big History tells the origin stories as told by modern science. Ways of Knowing and Understanding The Big History course relies on information from people other than just historians, which is not typical for a history course. Your students will consider what scholars from many disciplines have to say about the past, including scholars in physics, astronomy, chemistry, biology, anthropology, and of course, history. This type of approach, in which you and your students consider the viewpoints of many different scholars about the same topic, is called an BIG HISTORY PROJECT / UNIT 1 GUIDE 2

interdisciplinary approach. Your students will learn that when they use the perspectives of many different disciplines to help them answer complex questions, they ll inevitably get a fascinating and complex answer. Thresholds of Increasing Complexity Obviously, you can t cover everything that s happened in the last 13.8 billion years. In Big History, we use guiding criteria that determine what gets included in the course and what gets left out. These criteria are defined as the eight thresholds of increasing complexity. These are the ideas critical to the story of Big History and they guide decisions about the resources that have been chosen for you to use in teaching the course. You and your students will spend time learning about the ingredients and Goldilocks Conditions necessary to create each of the eight thresholds. Misconceptions and Teaching Challenges Scale Another challenging aspect for students is they may feel that their belief systems are in opposition to both the Big History narrative and the origin stories that they encounter in this unit. It s helpful to point out that there are often many different explanations for the same phenomena, and instead of trying to reconcile different stories, it can be more useful to compare the similarities and differences in the stories. This will open their eyes to other narratives and alternative explanations for history, and set the stage for open-mindedness throughout the course. Reconciling Faith and Science Another challenging aspect for students is they may feel that their belief systems are in opposition to both the Big History narrative and the origin stories that they encounter in this unit. It s helpful to point out that there are often many different explanations for the same phenomena, and instead of trying to reconcile different stories, it can be more useful to compare the similarities and differences in the stories. This will open their eyes to other narratives and alternative explanations for history, and set the stage for open-mindedness throughout the course. Thresholds of Increasing Complexity Unit 1 touches on complexity and thresholds, two critical concepts of the Big History course. Although these topics are important for students to understand, they re less concrete than other topics in the course, which may make them more challenging for some students to understand. Reassure students that they ll return to these ideas in each unit when a new threshold is introduced and over time they ll feel more comfortable with these concepts. Reading, Writing, and Discussion The Big History course is great for addressing English and Language Arts standards because it has a framework for reading, writing, and holding successful class discussions. The course provides leveled readings for all students. There are anywhere from two to four versions of each article so students at different reading levels can all engage with the material. The Big History guides to reading, writing, and discussion will help you and your students navigate and become familiar with the practices that will help them succeed in the course. It may seem like a bit of a grind at first, but if you use these guides and employ the methods they suggest, it will really pay off in the future. A few units into the course, the practices will become second nature for everyone. Instead of having to grapple with how to get through a reading, time will be spent on grappling with Big History s big ideas. BIG HISTORY PROJECT / UNIT 1 GUIDE 3

Understanding the Website A common issue for Big History teachers is that their students didn t learn how to use the website early on in the course, and this affected their experience throughout the school year. It may seem silly and not terribly academic, but it s worth your and your students time to complete the Big History Website Scavenger Hunt activity. This will save you a lot of headaches down the road. Vocabulary astrophysics The study of the properties and interactions of planets, stars, galaxies, and other astronomical objects. Big Bang A theory, first articulated in the 1920s, proposing that the Universe started out extremely hot and dense and gradually cooled off as it expanded. Big History A unified account of the entire history of the Universe that uses evidence and ideas from many disciplines to create a broad context for understanding humanity; a modern scientific origin story. complexity A quality of an object or system that has diverse components precisely arranged in connection with one another (so that new properties emerge which did not exist in the components alone). cosmology The study of the Universe on its largest scales, including its origin. emergent properties Properties of a complex system that are not present within its parts but that emerge only when those parts are combined. entropy (the law of) The natural tendency of all things to move from order to disorder. (Note: Although often called the law of entropy, it is more accurate to refer to it as the second law of thermodynamics.) Goldilocks Conditions Specific set of conditions necessary to enable greater complexity. The reference is to the fairy tale Goldilocks and the Three Bears, in which Goldilocks looks for the porridge, chair, and bed that are just right. history The study of past events. ingredients Components that are put together to form something new and more complex. interdisciplinary approach An approach to a subject that uses the viewpoints of many different kinds of scholars about the same topic. For instance, Big History relies on information from cosmologists, astrophysicists, geologists, chemists, paleontologists, biologists, anthropologists, and historians, as well as experts in other disciplines, to learn about the past. origin story A narrative about the beginning of the Universe and humanity. religion A set of beliefs and practices that concern humanity s relationship with the spiritual, the supernatural, and reality. scale Degrees of magnification, or perspective, used to measure time, space, and size. science An approach to discovering knowledge about the natural world that relies on testing ideas through observation or experiment. scientific notation A method of expressing very large and very small numbers to avoid using the many zeros that would be required otherwise. BIG HISTORY PROJECT / UNIT 1 GUIDE 4

thresholds of increasing complexity Moments in the history of the Universe when specific ingredients under the right Goldilocks Conditions come together to create something new and more complex. Universe All the matter and energy in existence, as well as the space that contains it. Lesson and Content Overview Lesson name Lesson description Content Activity 1.0 Welcome to Big History Big History starts with the big picture. Examining Big History big ideas from the beginning helps set the stage for the rest of the course. Watch: What Is Big History? Watch: The Big Bang Crash Course Watch: A Big History of Everything H2 Activity: Visions of the Future Activity: Big History Website Scavenger Hunt 1.1 Scale Big History is so big that we need to use a variety of scales to understand different topics in the course. Looking at things temporal and spatial scales helps us do this. Activity: Powers of 10 Activity: DQ Notebook Vocab Activity: Memorization Activity: Big History on a Football Field 1.2 Origin Stories People have always told origin stories stories about how the Universe and humans came to be. Big History is a modern, scientific origin story. Watch: Big Questions H2 Read: Cosmology and Faith Opening: BANG! The Universe Verse Book 1 Activity: Origin Stories Introduction Activity: Origin Stories from a Variety of Cultures Closing: DQ Notebook 1.3 What Are Disciplines? Big History enlists scholars from many disciplines including physics, astronomy, chemistry, biology, anthropology, and history to help answer complex questions. Watch: Are We Alone? H2 Watch: Ways of Knowing Introduction to Cosmology Watch: Ways of Knowing Introduction to Astrophysics Opening: Who Knows What? Vocab Activity: Comprehension Activity: Easter Island Mystery Closing: Exit Ticket What Do You Know, What Do You Ask? 1.4 My Big History Students place themselves in the Big History narrative by exploring the scale of their own lives, and the core concepts of Goldilocks Conditions and thresholds of increasing complexity are introduced. Watch: A Big History of Everything H2 Read: Complexity and Thresholds Opening: My Timeline Activity: Threshold Concentration Activity: History of Me Closing: Investigation 1 Investigation: Why do we look at things from far away and close up? The first investigation in the course is focused on scale and why it is important to look at things from different spatial and temporal perspectives. David Christian and Fernand Braudel on historical scales Different geographic and time scales Worksheets BIG HISTORY PROJECT / UNIT 1 GUIDE 5

Lesson name Lesson description Content Activity Additional content Additional content items, including image galleries, can be used to augment lessons or customize your own unit. Introduction to Thresholds of Increasing Complexity (video) The Big History (video) A Student of Big History (video) Learning tips Random facts Related galleries, images, websites, and videos Web links Assessments Unit 1 includes lesson and glossary quizzes. Lesson Quizzes Glossary Challenge Actions The Unit Log is required for every unit. Unit 1 includes a survey, which students and teachers are encouraged to take. Unit Log Survey BIG HISTORY PROJECT / UNIT 1 GUIDE 6

BIG HISTORY PROJECT / UNIT 1 GUIDE 7