Name Date Per Teacher. Packet #4 The Sun

Similar documents
Our sun is the star in our solar system, which lies within a galaxy (Milky Way) within the universe. A star is a large glowing ball of gas that

The General Properties of the Sun

Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere.

Stars and Galaxies. The Sun and Other Stars

Facts About The Sun. The Sun is a star found at the of the Solar System. It makes up around % of the Solar System s mass.

Sun s Properties. Overview: The Sun. Composition of the Sun. Sun s Properties. The outer layers. Photosphere: Surface. Nearest.

Chapter 23. Light, Astronomical Observations, and the Sun

The Sun as Our Star. Properties of the Sun. Solar Composition. Last class we talked about how the Sun compares to other stars in the sky

Module 4: Astronomy - The Solar System Topic 2 Content: Solar Activity Presentation Notes

Our sole source of light and heat in the solar system. A very common star: a glowing g ball of gas held together by its own gravity and powered

9-1 The Sun s energy is generated by thermonuclear reactions in its core The Sun s luminosity is the amount of energy emitted each second and is

The Sun: Our Star. The Sun is an ordinary star and shines the same way other stars do.

The Sun: Our Star. A glowing ball of gas held together by its own gravity and powered by nuclear fusion

Properties of Stars. Characteristics of Stars

The Quiet Sun The sun is currently being studied by several spacecraft Ulysses, SOHO, STEREO, and ACE.

Learning Objectives. wavelengths of light do we use to see each of them? mass ejections? Which are the most violent?

The Sun sends the Earth:

A Closer Look at the Sun

How the Sun Works. Presented by the

Convection causes granules. Photosphere isn t actually smooth! Granules Up-Close: like boiling water. Corona or of the Sun. Chromosphere: sphere of

Directed Reading. Section: Solar Activity SUNSPOTS. Skills Worksheet. 1. How do the gases that make up the sun s interior and atmosphere behave?

Chapter 24: Studying the Sun. 24.3: The Sun Textbook pages

Astronomy Exam 3 - Sun and Stars

The Sun. Chapter 12. Properties of the Sun. Properties of the Sun. The Structure of the Sun. Properties of the Sun.

Correction to Homework

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 8

Student Instruction Sheet: Unit 4 Lesson 3. Sun

The Sun. How are these quantities measured? Properties of the Sun. Chapter 14

Prentice Hall EARTH SCIENCE

Hydrogen Lines. What can we learn from light? Spectral Classification. Visible Hydrogen Spectrum Lines: Series. Actual Spectrum from SDSS

Lesson 3 THE SOLAR SYSTEM

The Sun. 1a. The Photosphere. A. The Solar Atmosphere. 1b. Limb Darkening. A. Solar Atmosphere. B. Phenomena (Sunspots) C.

Chapter Introduction Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars Lesson 3 Evolution of Stars Lesson 4 Galaxies and the Universe

8.2 The Sun pg Stars emit electromagnetic radiation, which travels at the speed of light.

SOLAR SYSTEM NOTES. Surface of the Sun appears granulated: 10/2/2015 ENERGY TRANSFERS RADIATION FROM THE SUN

The Sun. The Sun is a star: a shining ball of gas powered by nuclear fusion. Mass of Sun = 2 x g = 330,000 M Earth = 1 M Sun

Stars and Galaxies. Content Outline for Teaching

The Sun ASTR /17/2014

The sun, yellow dwarf star at the heart of the solar system NASA.gov, adapted by Newsela staff

10/17/ A Closer Look at the Sun. Chapter 11: Our Star. Why does the Sun shine? Lecture Outline

The Sun Our Extraordinary Ordinary Star

An Overview of the Details

Astronomy 1 Fall Reminder: When/where does your observing session meet? [See from your TA.]

Chapter 8 The Sun Our Star

The Sun. 1a. The Photosphere. A. The Solar Atmosphere. 1b. Limb Darkening. A. Solar Atmosphere. B. Phenomena (Sunspots) C.

Astronomy Chapter 12 Review

The Sun. the main show in the solar system. 99.8% of the mass % of the energy. Homework due next time - will count best 5 of 6

The Sun Our Star. Properties Interior Atmosphere Photosphere Chromosphere Corona Magnetism Sunspots Solar Cycles Active Sun

An Overview of the Details

Our Star: The Sun. Layers that make up the Sun. Understand the Solar cycle. Understand the process by which energy is generated by the Sun.

4 Layers of the Sun. CORE : center, where fusion occurs

Earth/Space/Physics Kristy Halteman.

The Sun is the nearest star to Earth, and provides the energy that makes life possible.

Energy, Work, and Simple Machines

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

Chapter 14 Lecture. The Cosmic Perspective Seventh Edition. Our Star Pearson Education, Inc.

Solar Dynamics Affecting Skywave Communications

Chapter 14 Lecture. Chapter 14: Our Star Pearson Education, Inc.

Astronomy Ch 16 The Sun. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Name: Date: 2. The temperature of the Sun's photosphere is A) close to 1 million K. B) about 10,000 K. C) 5800 K. D) 4300 K.

The Project. National Schools Observatory

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth)

Chapter 9 The Sun. Nuclear fusion: Combining of light nuclei into heavier ones Example: In the Sun is conversion of H into He

1-4-1A. Sun Structure

10/18/ A Closer Look at the Sun. Chapter 11: Our Star. Why does the Sun shine? Lecture Outline

Lec 7: Classification of Stars, the Sun. What prevents stars from collapsing under the weight of their own gravity? Text

Astronomy 1 Winter 2011

Chapter 3 The Solar System

Outline. Astronomy: The Big Picture. Earth Sun comparison. Nighttime observing is over, but a makeup observing session may be scheduled. Stay tuned.

The Sun. Basic Properties. Radius: Mass: Luminosity: Effective Temperature:

Astronomy 154 Lab 4: The Sun. NASA Image comparing the Earth with the Sun. Image from:

Chapter 14 Our Star Pearson Education, Inc.

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium

THE SUN AND THE SOLAR SYSTEM

The Sun. The Sun Is Just a Normal Star 11/5/2018. Phys1411 Introductory Astronomy. Topics. Star Party

CHAPTER 9: STARS AND GALAXIES

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

Lecture 17 The Sun October 31, 2018

Ocean s Influence on Weather and Climate

Today The Sun. Events

The Structure of the Sun. CESAR s Booklet

Announcements. - Homework #5 due today - Review on Monday 3:30 4:15pm in RH103 - Test #2 next Tuesday, Oct 11

Chapter 10 Our Star. X-ray. visible

Planets Inner vs. outer Composition inner planets are rocky/outer are gas Size inner are smaller/outer are much larger Distance from sun inner are

Radiation Zone. AST 100 General Astronomy: Stars & Galaxies. 5. What s inside the Sun? From the Center Outwards. Meanderings of outbound photons

Guidepost. Chapter 08 The Sun 10/12/2015. General Properties. The Photosphere. Granulation. Energy Transport in the Photosphere.

PTYS/ASTR 206. The Sun 3/1/07

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN

The Sun. SESAME Astronomy Week 4. Thursday, February 10, 2011

B B E D B E D A C A D D C

1. Solar Atmosphere Surface Features and Magnetic Fields

The Sun. Nearest Star Contains most of the mass of the solar system Source of heat and illumination

1.3j describe how astronomers observe the Sun at different wavelengths

Summer 2013 Astronomy - Test 3 Test form A. Name

Earth Science Lesson Plan Quarter 4, Week 7, Day 1

Astronomy 210. Outline. Nuclear Reactions in the Sun. Neutrinos. Solar Observing due April 15 th HW 8 due on Friday.

1 A= one Angstrom = 1 10 cm

CHAPTER 29: STARS BELL RINGER:

The Solar System by Edward P. Ortleb and Richard Cadice

Heat: the transfer of thermal energy from one substance to another. Electrons: the small particles inside an atom that have negative charge.

Transcription:

Packet #4 The Sun Reading Guide: Chapter 29.1 (read text pages 755 760) STRUCTURE OF THE SUN 1e Students know the Sun is a typical star and is powered by nuclear reactions, primarily the fusion of hydrogen to form helium. 1. What elements make up 99% of the suns mass? 2. The sun s spectrum reveals that the sun contains 3a. What is nuclear fusion? 3b. Fusion released huge amounts of. 3c. are the primary fuel for the sun s energy. 4. What is one of the final products of hydrogen fusion? 5. The sun s energy comes from, and the mass that is lost during fusion becomes. 6. What do each of the variables in the formula E=mc 2 represent? E: m: c: 7. The sun changes more that 600 million 8. Does the sun have layers? 9. Core: % of the Sun s diameter Temperature: What is it made of: 10. Radiative Zone: Surrounds the Temperature: to 11. Convective Zone: Surrounds the Temperature: Energy move through this zone 12. Photosphere: means Temperature: spots are shown in Figure 5. Use the caption in Figure 5: The photosphere is referred to 13. When can we see the corona from earth? 13. Chromosphere: sphere Color: What gas gives this layer its color? Temperature: to Describe the Jets of gas: 14. Corona: What is it? What else is it called? Temperature: What does it prevent? What do the ions form that stream out into space? 1

Reading Guide: Chapter 29.2 (read text pages 761 764) SOLAR ACTIVITY 1e Students know the Sun is a typical star and is powered by nuclear reactions, primarily the fusion of hydrogen to form helium. 1a. Does the sun rotate? Because the sun is a ball of gas it not all locations rotate at the same speed. Fill in the rotation rates: 1 b. close to the equator earth days_ 1c. points near the poles earth days_ 2. The movement of gases within the sun s and the movements caused by the sun s produce 3a. What are sunspots? 3b. How much cooler are these spots on the photosphere? 3d. What is the diameter of sunspots: 4a. A sunspot cycle begins when the number of. 4b. How many sunspots are there at the peak of the sunspot cycle? 4c. How long is the sunspot cycle? years 5c. What are solar ejections? 6a. What is a prominence? 6b How long do prominence last? 7a. What are solar flares? 7b. How long do solar flares last? 8. Define Aurora: 9. Where are auroras usually seen? 11a. What is another name for Aurora s? 10. Why are they seen in these locations? 11b. When are they most frequent and why? 11c. Where in the US can you see them, & how often? 2

Reading Guide: Chapter 7.1 & 7.2 (Read text pages 154 164) 1. Earth s crust contains useful. The processes that formed many of these Scientists have identified more than. 2. Define ores: 3. Pick 3 minerals from TABLE 1 on page 157 to fill in the chart: Mineral name Uses i) ii) iii) 4. Define nonrenewable resources: 5. Why are fossil fuels non renewable? 6. Fossil fuels are made from the remains of. The types of fossil fuels are,, and. 7. Define nuclear fission: 8. Define nuclear fusion: Reading Guide: Chapter 7.3 (Read text pages 165 172) 1. Define renewable resources: 2. What is geothermal energy? 3. Where does Iceland get 85% of its energy for heating its homes? 4. What is wind? 5. What is wind a result of? 6. Why can t wind energy be used everywhere? 7. How much longer do scientists predict the worldwide coal reserves will last? 8. Why is mining bad for the environment? 9. Define conservation: 10. Define recycling: 3

What is Fusion? NUCLEAR FUSION Where does fusion happen?, because an amazing amount of is created by the pushing in. Why does high pressure in the core lead to Fusion? High and allows nuclei to interact! Nuclei can together: What type of energy does the sun s fusion create? and! What elements are used in fusion? (the short version) p p p p n p p n + How does the does fusion make energy? 1) The atom is as the that fused to make it. So, some mass is missing 2) The from the H atoms is! Energy from Fusion= E=mc 2 E=, m=, c= 4

Explain below what happens in each step of the nuclear fusion process STEP 1 STEP 2 STEP 3 STEP 4 STEP 5 5

Sun Project I. Make a beautiful picture of the sun with all of the parts listed below: 4. Photosphere 7. Spicules 5.Chromosphere 8. Solar Wind 7. Corona 9. Sun Spots 1. Core 2. Radiation Zone 3. Convection Zone II. For the core, radiation & convection zones: Write in temperature How energy is transferred 1 other important fact III. For the photosphere, chromosphere & corona: Write in temperature Definition 1 other important fact USE: Book pgs. 755 760 Notes: packet pg 6 & 8, 9 10. Solar flare 11. Prominence 12. Granulation GRADING RUBRIC: (so that you know what I ll be looking for ) Picture of the Sun 7 points Section is complete, answers well thought out, pictures drawn, labeled, & colors used. No blanks 5 points Section is mostly complete, most answers complete, pictures mostly drawn & labeled. 3 points Section is only somewhat complete, answers incomplete, pictures drawn, no color, & no labels. 0 points Section incomplete. Lacks sufficient answers, drawings, labels, or color. Core/Inner Zone Atmosphere/ Outer Zone Overall Picture Total /21 6

Sun Structure The sun is made up of layers. There are 6 main layers. 3 Inner Layers (inner zones) and 3 Outer Layers (atmosphere) Inner Zones 1 1 2 2 3 3 Atmosphere Book: p758 764 Layer Name Temperature Energy transfer Fact Inner Zones Layer Name other name Fact 1 Fact 2 Atmosphere There are many features and phenomena that can be observed either on the surface of the sun or in the Earth s atmosphere. Define the following words. Book p758 764 Word Definition Sun Spots Granules Prominences Solar Winds Solar Flares Spicules Aurora Narrow jets of rising gas along the chromosphere. They look like hair like structures on the outer edge of the chromosphere. Magnetic field Nuclear Fusion 7

SUN DIAGRAM REVIEW Part I. Name each of the numbered features from the sun picture. 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. Part II: Match the features shown on the diagram with the statements below. A. Where does hydrogen fusion take place? B. Dark areas of the sun that are cooler than the surrounding areas and are caused by the sun's magnetic field. C. Lowest layer of the sun's atmosphere that gives off light. D. Charged particles (ions) that continually escape from the corona and move through space. E. Huge, arching columns of glowing gas. F. Gases near a sunspot that suddenly brighten, shooting gases outward at high speed. G. The sunlight we see from earth that is used for photosynthesis. H. The "surface" of the sun. I. Energy moves in the form of electromagnetic waves. J. Energy is transferred through the movement of gases. K. Color sphere. Gases glow red. L. Outermost layer of the sun's atmosphere. M. Not normally seen from Earth, except during an eclipse. N. May cause magnetic storms on Earth or sudden disturbances that interfere with radio communications on Earth. O. Created the auroras on Earth. 8

The Sun Diameter km 1 million could fit inside the sun The sun rotates on its axis once every. ( at poles at equator) Hydrogen & Helium + traces of other elements The Sun is made of 6 main layers Inner layers ( ) & Outer layers ( ) Structure or the Sun Inner Zones (inner layers): Radiative Zone Atmosphere ( ): Photosphere Corona The Core The core is so & under so much that can take place. Fusion of can also take place because of the. Fusion is what makes the Sun s energy =! The Radiative Zone the core Energy travels in The Convective Zone Energy moves through convection of gas and liquid. Convective cells The & become less dense, they carry the energy to the surface. At the surface the atoms, become & back down. The Photosphere =, This is the of the Sun Energy is given off in the form of that we see on earth. a grainy appearance from the / gases in convection zone. The Chromosphere = sphere of layer glows with reddish light has energetic magnetic activity: Flares, (those loopy things), The Corona Can only be seen during a! of the Sun of degrees but very diffuse (spread out) Extends into space Hot and energetic, gives off lots of! 9

Solar Activity Types: & Coronal Mass Ejections C.M.E What Causes Solar Activity? What makes the magnetic Field? 1) 2) The of in the convection zone. Sunspots on the Photosphere Sunspots: Regions where the pokes through the. Sunspots are than surrounding stuff, so they look! Granules: Where the convection zone underneath. Sunspot Facts They occur in an cycle. They are usually in ( ) charge. Hot gasses eject out of them ( & ). Size up to 100,000 km ( ) Location between the equator & poles of the sun.! Solar Flares 1) An near a sun spot. 2) Sends particles into space & causes on earth Auroras Only seen in because the charged particles are pulled in by the earth s! Flares Facts. They can last. Can have during the peak sunspot cycle. thousands of km Coronal Mass Ejections C.M.E. The corona ejects a massive amount of material into space, causing, this is a CME. Like a solar flare,! Prominence a loopy structure that usually! Last weeks to a year Prominence Formation Gases follow the curved lines of the from one to another. 10

SUNSPOT ACTIVITY- The photographs below show sunspots as they appeared on three different dates. Like the poles of a magnet, sunspots seem to occur in pairs. It is sometimes difficult to decide weather or not two sunspots are part of a pair. A. Look at the pictures below & answer the questions. A. May 01 B. May 05 C. May 10 1. How many pairs of sunspots are in each photograph? A. B. C. 2. What kind of evidence did you use in deciding that two sunspots were part of a pair? 3. What causes sunspots? 4. What feature occurs between sunspots? 5. What happens when the pair of sunspots meet (join)? Table of Sunspot Activity in the 1700 s Year Number of observed Sunspots Year Number of observed Sunspots 1728 135 1766 20 1732 7 1770 130 1739 125 1775 5 1743 6 1778 165 1750 90 1784 18 1756 15 1788 140 1761 80 1797 6 1. In the table above underline in red all the years that include at least 80 sunspots. 2. Which years did you underline in red? These are the years of sunspot maximum. 3. Which years are NOT underlined? These are years of sunspot minimum. 4. How many years are between 1728 & 1739? 1739 & 1750? 1750 & 1761? 1761 & 1770? 1770 & 1778? 1778 & 1788? 5. Do sunspot maximums always occur every 11 years? If not, is there a general pattern? 6. How many years are between 1732 & 1743? 1743 & 1756? 1756 & 1766? 1766 & 1775? 1775 & 1784? 1784 & 1797? 7. Scientists think the sunspot minimums are also on an 11-year cycle. Do your data support this theory? 8. If the last sunspot maximum was in 1990, when will the next two maximums most likely occur? 11

Energy Where does energy come from? The Sun is the source of:,,,,, The sun s energy made the plants/animals grow that became coal, natural gas, oil & gasoline Energy Resources 2 categories: 1. Once used these resources CANNOT be used again (coal, oil, gas) 2. These resources can be used over and over again (wind, water or solar) Non Renewable Resources: COAL What is it? How much left in the world? About 200 years Advantages? Plenty left; Mining is getting more efficient Disadvantages? : CO 2 emissions ( ), SO 2 (acid rain) Heavy & bulky to transport Non Renewable Resources: OIL What is it? Formed underground from decaying animal and plant material How much left in the world? About years! Advantages?, Efficient in producing energy, Disadvantages?, Pollution: air and danger of water pollution through spills Non Renewable Resources: NATURAL GAS What is it? Formed underground from decaying animal and plant material How much left in the world? About 60 years Advantages? Clean, least polluting of all non renewables; Easy to transport Disadvantages? Some air pollution; Danger of explosions Non Renewable Resources: NUCLEAR What is it? How much left in the world? Not known Advantages? Not much waste and few CO 2 emissions released, as well as, few other greenhouse gases Disadvantages? High cost to build and close down power stations;. Problem with getting rid of waste safely Renewable Resources: WIND What is it? It the movement of air from high to low pressure How much left? Advantages? Disadvantages? Winds change all the time, Renewable Resources: SOLAR What is it? How much left? Endless Advantages? No pollution, can be used in remote areas Disadvantages? Can be expensive, needs sunlight, limited production on cloudy days and at night time Renewable Resources: BIO ENERGY What is it? Biomass and Biogas fermented animal or plant waste, vegetation from sustainable sources How much left? Advantages? Disadvantages? Can be expensive to set up 12

Renewable Resources: Hydro Electric DAMS What is it? How much left? Endless Advantages? No CO2 emissions, can control flooding and provide a good water supply to an area Disadvantages?. Large areas maybe flooded. Visual and water pollution. Renewable Resources: GEOTHERMAL What is it? How much left? A lot Advantages? Disadvantages? Expensive and more cost effective in volcanically active areas or along plate boundaries. Renewable Resources: WAVES & TIDAL What is it? How much left? Endless Advantages? Disadvantages? Expensive to set up, along coast lines How do we use these sources to make energy for.electric light, Mobile phone, ipods/mp3, TV,Hot Water We generate electricity: 1. Use an energy resource source (coal, wind, solar) to heat water. 2.. 3. The steam then turns a turbine. 4. 5. The generator then produces electricity. 6.. The Sun Video Bill Nye, the science guy 1. How hot is the sun? 2. How many Earths could you fit inside the Sun? 3. How many Earths would fit across the diameter of the sun? 4. What is the temperature of the sun s core? 5. Almost all the energy we use comes from the. 6. List several things that directly or indirectly get their energy from the sun: 7. How hot is a solar flare? 8. Compare the power of the sun to the power of a typical family house. 9. How many Watts of energy hits the Earth from the sun?. 10. How many Watts of energy is the Sun producing? 11. When are we due for another sun spot cycle? 12. What are sun spots?. 13