- Both reactions sacrifice. - This in a nuclear reaction is called the. and is the energy in the reaction

Similar documents
1/13/16. The Big Bang Theory

Matter and Energy. Previous studies have taught us that matter and energy cannot be created nor destroyed We balance equations to obey this law.

History of the Universe Unit Tracking Sheet

GraspIT Questions AQA GCSE Physics Space physics

Q1. Describe, in as much detail as you can, the life history of a star like our Sun

Figure 19.19: HST photo called Hubble Deep Field.

Fission & Fusion Movie

GraspIT Questions AQA GCSE Physics Space physics

25.2 Stellar Evolution. By studying stars of different ages, astronomers have been able to piece together the evolution of a star.

21/11/ /11/2017 Space Physics AQA Physics topic 8

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following:

v = H o d Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d):

Name Date Period. 10. convection zone 11. radiation zone 12. core

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

THE UNIVERSE CHAPTER 20

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe

Chapter 1 Our Place in the Universe

A Short History of the Universe. The universe in a grain of sand Particles and forces The Big Bang Early history of the universe Nucleosynthesis

THE ORIGIN OF THE UNIVERSE AND BLACK HOLES

ET: Astronomy 230 Section 1 MWF Astronomy Building. Outline. The Early Universe? HW1 due today!

BIG BANG SUMMARY NOTES

The slides with white background you need to know. The slides with blue background just have some cool information.

Universe Celestial Object Galaxy Solar System

1. Four different processes are described in List A. The names of these processes are given in List B.

Dr. Birdley Teaches Science!

1 The Life Cycle of a Star

LESSON 1. Solar System

ASTRONOMY. S6E1 a, b, c, d, e, f S6E2 a, b, c,

How do we measure properties of a star? Today. Some Clicker Questions - #1. Some Clicker Questions - #1

What is the solar system?

Welcome Aboard!! CHANGE OF KOMATSU S OFFICE HOURS. Briefing Welcome to the Cosmic Tour: Some Guide Lines. Lecture 1 Our Place in the Universe

14.1 A Closer Look at the Sun

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE

The Big Bang Theory. Rachel Fludd and Matthijs Hoekstra

TA Final Review. Class Announcements. Objectives Today. Compare True and Apparent brightness. Finding Distances with Cepheids

Stars. 1.1 A Modern View of the Universe. What Objects Do We Find in The Universe? 8/12/2010. Our goals for learning:

Chapter 5. Periodic Law.

The History of the Solar System. From cloud to Sun, planets, and smaller bodies

Forces and Nuclear Processes

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.

Cosmic Microwave Background Radiation

1. Cosmology is the study of. a. The sun is the center of the Universe. b. The Earth is the center of the Universe

Name: Space Questions Questions. Class: Date: Time: Marks: Comment s:

Textbook Chapters 24 - Stars Textbook Chapter 25 - Universe. Regents Earth Science with Ms. Connery

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am

AST 100 General Astronomy: Stars & Galaxies

The Big Bang Theory (page 854)

Section 25.1 Exploring the Solar System (pages )

IB Test. Astrophysics HL. Name_solution / a) Describe what is meant by a nebula [1]

Name: P8 SPACE PHYSICS. Class: Question Practice. Date: 140 minutes. Time: 140 marks. Marks: GCSE PHYSICS ONLY. Comments:

Astronomy 104: Second Exam

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe

Stars and Galaxies. Evolution of Stars

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..

TEACHER BACKGROUND INFORMATION

8.8A describe components of the universe, including stars, nebulae, galaxies and use models such as HR diagrams for classification

Dead & Variable Stars

Big Bang Theory How the Universe was Formed

1 A Solar System Is Born

Page 2. Q1. The diagram shows part of the life cycle of a star which is much bigger than the Sun.

The Night Sky. The Universe. The Celestial Sphere. Stars. Chapter 14

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

ASTR Midterm 1 Phil Armitage, Bruce Ferguson

Phys 214. Planets and Life

Name: Space Questions. Class: Date: Time: Marks: Comment s:

Learn Nuclear Science with Marbles

Learn Nuclear Science with Marbles

Lecture 24: Testing Stellar Evolution Readings: 20-6, 21-3, 21-4

þ Tiered questions that probe lower and higher-order thinking þ Differentiated for upper elementary and intermediate students þ Addresses NGSS and

Test Name: 09.LCW.0352.SCIENCE.GR Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: Date: 09/21/2017

Class 15 Formation of the Solar System

Stars & Galaxies. Chapter 27, Section 1. Composition & Temperature. Chapter 27 Modern Earth Science Characteristics of Stars

Light. Transverse electromagnetic wave, or electromagnetic radiation. Includes radio waves, microwaves, infra-red, visible, UV, X-rays, and gamma rays

NSCI 314 LIFE IN THE COSMOS

The Big Bang Theory, General Timeline. The Planck Era. (Big Bang To 10^-35 Seconds) Inflationary Model Added. (10^-35 to 10^-33 Of A Second)

Brock University. Test 1, February, 2017 Number of pages: 9 Course: ASTR 1P02 Number of Students: 480 Date of Examination: February 6, 2017

Spectrographs: instrument to separate white light into the bands of color.

1. Star: A object made of gas found in outer space that radiates.

Abundance of Elements. Relative abundance of elements in the Solar System

Lunar Eclipse. Solar Eclipse

The Big Bang. Mr. Mike Partridge Earth & Space Science J.H. Reagan High School, Houston, TX

BROCK UNIVERSITY. Test 2, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

D. most intense and of longest duration C. D.

Chapter 24. Stars, Galaxies & the Universe. Distance units

CONTENT EXPECTATIONS

Edwin Hubble Discovered galaxies other than the milky way. Galaxy:

Chapter 12: The Life Cycle of Stars (contʼd) How are stars born, and how do they die? 4/9/09 Habbal Astro Lecture 25 1

Chapter 14 Our Star A Closer Look at the Sun. Why was the Sun s energy source a major mystery?

Outline 8: History of the Universe and Solar System

LIFE CYCLE OF A STAR

Brock University. Test 1, January, 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 500 Date of Examination: January 29, 2015

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars

2. Very generally, describe how the Milky Way Galaxy formed. (Words or labeled picture)

Star. Planet. Chapter 1 Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe?

9/5/16. Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM. Astronomy 1001 First Assignments: Chapter 1: A Modern View of the Universe

The Universe. But first, let s talk about light! 2012 Pearson Education, Inc.

Potter Name: Date: Hour: Earth Science Unit 2: Astronomy

25/11/ Cosmological Red Shift:

How to Build a Habitable Planet Summary. Chapter 1 The Setting

Transcription:

Unit 2: Origins I. Time Begins a. The b. The universe begins as the size of a single atom c. The universe began as a i. All matter and space were created from a single point of pure energy in an instant II. 3 Minutes after Big Bang a. The universe has grown from the size of an atom to larger than the size a grapefruit b. c. energy froze into matte r according to Albert Einstein s equation. d. This basically says that like snowflakes freezing, energy forms matter into clumps that today we call protons, neutrons and electrons. e. These parts later form into atoms III. Several Hundred Thousand Years after Big Bang a. ATOMS form (specifically Hydrogen and its isotopes with a small amount of Heliu m.) b. The early Universe was about 75% Hydrogen and 25% Helium. c. It is still almost the same today. IV. 200-400 Million Years After Big Bang a. 1 st stars and Galaxies form V. 4.6 Billion Years Ago a.. VI. Evidence for Big Bang 1. 2. 3. 4. 5.

VII. Fission and Fusion Fission - Example: Fusion Example: VIII. Where does Energy come from? - Both reactions sacrifice - This in a nuclear reaction is called the and is the energy in the reaction Similarities and Differences between Nuclear Fission and Fusion Unique to Nuclear Fission Common to Both Unique to Nuclear Fusion - nucleus into particles - - Used to produce - Produces radioactive - Both generate the same way ( Convert ) - two small to form a one - Used by - Produces essentially

Student sheet Name Title: Heavy Elements Introduction: On Earth, we have 92 naturally occurring elements. The atoms of each element are unique. Every gold atom has 79 protons in its nucleus. Every carbon atom has 6 protons. The number of protons gives each element its distinctive properties. Stars are the birthplace of all the different types of elements we find on Earth. Through the process of nuclear fusion (the nucleus of two atoms getting smashed together) atoms change and become heavier during every star cycle they go through. In this activity you will play a game to model the formation of heavy elements in the star cycle. Materials: per group: one game board, 4 set of element cards (per group of 4), game pieces (small items you have) one paper dice Directions: 1. Line your game pieces up on the nebula, the gas cloud where it all begins. Deal out 10 hydrogens to each player to start. 2. Roll to see who goes first. 3. Follow the directions on the game board. When you fuse atoms, turn in the fusing atoms for the new product. For example: H + H = He, you will turn in two hydrogen cards and get one helium. 4. You will have a set amount of time to play. Your teacher will tell you how much. 5. The winner has the largest atom at the end of the time. If you cross the start you collect another 10 hydrogens. Analysis: 1. What creates the energy given off by stars? 2. Why do they expand and contract in size? 3. Why don t more heavy elements form in smaller stars like brown and white dwarves? 4. What does the presence of atoms as large as Mercury (80 protons) or Lead (82 protons) suggest about the star cycle? Conclusion:

Mission 11 ALT Logbook Mission to Mars Spectroscopy Can You detect signs of past water? Elemental Fingerprints Worksheet 2 Name: Date: Mystery Spectra Identify the elements in spectra A, B, and C by comparing the bright lines present with the bright lines in the spectra for known elements. Helium Hydrogen Sodium Lithium Spectra A Elements: Spectra B Elements: Spectra C Elements: If spectrum A, B, and C were samples of spectroscopy data collected by the Mars Global Surveyor, what could you say about the chemical composition of the surface of Mars? 2 L:H?T?E? SETI Institute

Red shift/blue shift Practice Blue Red Nearby Star Andromeda Galaxy Bernard s Galaxy Bear Galaxy Venus SR - 5 1. Which galaxy or planet is moving at the same speed as the nearby star? 2. What galaxies or planets are moving toward the nearby star? 3. What galaxies or planets are moving away from the nearby star? 4. Is the Andromeda galaxy red or blue shifted? 5. According to Hubble s law, which galaxy or planet is moving fastest away from the nearby star? 6. Which galaxy or planet is moving the slowest away from the nearby star?