6RODU (PLVVLRQ 4/10/00 1

Size: px
Start display at page:

Download "6RODU (PLVVLRQ 4/10/00 1"

Transcription

1 6RODU (PLVVLRQ 95% of the Sun s energy reaches us as sunshine, that is, light and heat Photosynthesis (how plants grow), sunburn, weather are all attributed to this energy The last 5% of the energy determines space weather 4/10/00 1

2 7KH 6XQ At 5 billion years old, our sun is an energy machine The sun's energy released in 1 sec, could power the U.S. for 9 million years 4/10/00 2

3 3DUWV RI WKH 6XQ The sun is a gas ball with various temperatures and densities Core: millions of degrees Surface: thousands of degrees Corona: millions of degrees 4/10/00 3

4 7KH 6XUIDFH :H 6HH Photosphere Surface of the sun You couldn t stand on surface Constantly bubbling 6000 K 4/10/00 4

5 )DLQW 8SSHU $WPRVSKHUH Corona Visible during an eclipse This outer layer extends millions of miles Earth is immersed in this 4/10/00 5

6 %HWZHHQ 6XQ DQG (DUWK Called solarterrestrial environment Solar wind, blows 1 million miles/hr, Shapes Earth s magnetosphere 4/10/00 6

7 (DUWK V 0DJQHWLF )LHOG Earth's magnetic field, without solar wind distortion Magnetic field lines channel charged particles 4/10/00 7

8 6XQ DQG (DUWK DUH $OLNH Active Quiet Summer Winter Each have: Equator Magnetic field, N and S poles Rotation ( day ) Seasons Atmospheric Weather 4/10/00 8

9 6RODU $FWLYLW\ Active Active and Quiet Sun look quite different One Solar Cycle is 11 years long. Quiet 4/10/00 9

10 6XQVSRWV$ Cooler regions 4400 Kelvin Appear in moments or hours, last hours, days, or weeks Disturbed magnetic field, is one cause for solar flares 4/10/00 10

11 6XQVSRWV 7UDYHO Sunspots move across the surface of the sun as the sun rotates They change as they age and may produce repeated flares 4/10/00 11

12 6RODU )ODUH This sunspot, 2 Earths wide, produced a bright flare 4/10/00 12

13 3URPLQHQFH Magnetic fields give structure to ejecta When very disturbed, breaks and plasma goes shooting out into space. 4/10/00 13

14 2SWLFDO 7HOHVFRSHV In white light one can easily see sunspots Light is projected onto a sheet so the eye doesn't look directly through the telescope at the sun. Telescope like one Galileo might have used 4/10/00 14

15 2WKHU 7HOHVFRSHV Radio telescopes and satellite imager tell us other information about the Sun 4/10/00 15

16 (IIHFWV= $XURUD The aurora is directly due to the energy coming from the sun Aurora from space with the shuttle in foreground 4/10/00 16

17 (IIHFWV= 1DYLJDWLRQ Ships at sea require good navigation signals Navigation errors can lead to wasted fuel, groundings, and spilled cargo 4/10/00 17

18 (IIHFWV= 5DGLR Signals can get lost or absorbed, bounce and miss the receivers Communication over the poles at certain frequencies can be completely blacked out 4/10/00 18

19 (IIHFWV= (OHFWULF 3RZHU Huge transformers can be damaged by geomagnetic storms Blackouts can be widespread 4/10/00 19

20 (IIHFWV= 3LSHOLQHV Alaska Pipeline Pipelines can corrode with geomagnetic storms Without mitigation, corrosion can cause severe leaks and damage the environment 4/10/00 20

21 (IIHFWV= 6DWHOOLWHV Satellites can be damaged, lost, returned to Earth early Satellites sit in the space environment and alert us 4/10/00 21

22 (IIHFWV= 5DGLDWLRQ Astronauts in space (EVA, Extra Vehicular Activity) All Space Shuttle missions SST (the Concorde) flying at high altitude, at high latitude 4/10/00 22

23 :RUN LQ 6SDFH Dangers of space travel are many Astronauts working on the Moon 4/10/00 23

24 (IIHFWV= &OLPDWH Is the Sun's variability tied to Earth's climate? Controversial correlation with droughts, ice ages, large-scale weather patterns on Earth 4/10/00 24

25 6XPPDU\ RI (IIHFWV Space Weather effects on: Satellites * What technology is dependent on satellties? Navigation * What are the risks of lost navigation signals? Manned Space Flights * As an astronaut, would you care about this? Communication * How are communications disrupted? Electric Power * How would you know about this disruption? 4/10/00 25

26 12$$ 6SDFH :HDWKHU 6FDOHV Category Geomagnetic Storms G1-G5 Solar Radiation Storms S1-S5 Radio Blackouts R1-R5 Effects Satellites, Power Grids, other Biological, Satellites, other Navigation, Radio Easy way to communicate conditions and forecasts Like the hurricane or earthquake scales Will be hearing these, seeing them in the news 4/10/00 26

27 12$$ 6FLHQFH (G 3RVWHU Poster shows effects on different systems Also Facts about space weather Questions to answer Websites What would you like to study about Space Weather? 4/10/00 27

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

8.2 The Sun pg Stars emit electromagnetic radiation, which travels at the speed of light. 8.2 The Sun pg. 309 Key Concepts: 1. Careful observation of the night sky can offer clues about the motion of celestial objects. 2. Celestial objects in the Solar System have unique properties. 3. Some

More information

Introduction to Space Weather

Introduction to Space Weather Introduction to Space Weather We may have been taught that there is a friendly, peaceful nonhostile relationship between the Sun and the Earth and that the Sun provides a constant stream of energy and

More information

THE SOLAR WIND & SOLAR VARIABILITY

THE SOLAR WIND & SOLAR VARIABILITY The Sun-Earth System: CONTENTS AN OVERVIEW The Stars Around Us 1 Our Dependence on the Sun 3 The Sun s Inconstancy 3 Intruders from Afar 5 What Gets By 5 Voyages of Discovery in an Age of Exploration 6

More information

The Sun sends the Earth:

The Sun sends the Earth: The Sun sends the Earth: Solar Radiation - peak wavelength.visible light - Travels at the speed of light..takes 8 minutes to reach Earth Solar Wind, Solar flares, and Coronal Mass Ejections of Plasma (ionized

More information

Student Instruction Sheet: Unit 4 Lesson 3. Sun

Student Instruction Sheet: Unit 4 Lesson 3. Sun Student Instruction Sheet: Unit 4 Lesson 3 Suggested time: 1.25 Hours What s important in this lesson: Sun demonstrate an understanding of the structure, and nature of our solar system investigate the

More information

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

Radiation Zone. AST 100 General Astronomy: Stars & Galaxies. 5. What s inside the Sun? From the Center Outwards. Meanderings of outbound photons AST 100 General Astronomy: Stars & Galaxies 5. What s inside the Sun? From the Center Outwards Core: Hydrogen ANNOUNCEMENTS Midterm I on Tue, Sept. 29 it will cover class material up to today (included)

More information

Solar Activity The Solar Wind

Solar Activity The Solar Wind Solar Activity The Solar Wind The solar wind is a flow of particles away from the Sun. They pass Earth at speeds from 400 to 500 km/s. This wind sometimes gusts up to 1000 km/s. Leaves Sun at highest speeds

More information

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

Chapter 24: Studying the Sun. 24.3: The Sun Textbook pages Chapter 24: Studying the Sun 24.3: The Sun Textbook pages 684-690 The sun is one of the 100 billion stars of the Milky Way galaxy. The sun has no characteristics to make it unique to the universe. It is

More information

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

Module 4: Astronomy - The Solar System Topic 2 Content: Solar Activity Presentation Notes The Sun, the largest body in the Solar System, is a giant ball of gas held together by gravity. The Sun is constantly undergoing the nuclear process of fusion and creating a tremendous amount of light

More information

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

10/17/ A Closer Look at the Sun. Chapter 11: Our Star. Why does the Sun shine? Lecture Outline Lecture Outline 11.1 A Closer Look at the Sun Chapter 11: Our Star Our goals for learning: Why does the Sun shine? What is the Sun's structure? Why does the Sun shine? Is it on FIRE? Is it on FIRE? Chemical

More information

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

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 The Sun as Our Star Last class we talked about how the Sun compares to other stars in the sky Today's lecture will concentrate on the different layers of the Sun's interior and its atmosphere We will also

More information

The Project. National Schools Observatory

The Project. National Schools Observatory Sunspots The Project This project is devised to give students a good understanding of the structure and magnetic field of the Sun and how this effects solar activity. Students will work with sunspot data

More information

The Magnetic Sun. CESAR s Booklet

The Magnetic Sun. CESAR s Booklet The Magnetic Sun CESAR s Booklet 1 Introduction to planetary magnetospheres and the interplanetary medium Most of the planets in our Solar system are enclosed by huge magnetic structures, named magnetospheres

More information

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

Chapter 14 Lecture. The Cosmic Perspective Seventh Edition. Our Star Pearson Education, Inc. Chapter 14 Lecture The Cosmic Perspective Seventh Edition Our Star 14.1 A Closer Look at the Sun Our goals for learning: Why does the Sun shine? What is the Sun's structure? Why does the Sun shine? Is

More information

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

10/18/ A Closer Look at the Sun. Chapter 11: Our Star. Why does the Sun shine? Lecture Outline 10/18/17 Lecture Outline 11.1 A Closer Look at the Sun Chapter 11: Our Star Our goals for learning: Why does the Sun shine? What is the Sun's structure? Why does the Sun shine? Is it on FIRE? Is it on

More information

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

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 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 generates energy through nuclear fusion in its core. The

More information

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

Learning Objectives. wavelengths of light do we use to see each of them? mass ejections? Which are the most violent? Our Beacon: The Sun Learning Objectives! What are the outer layers of the Sun, in order? What wavelengths of light do we use to see each of them?! Why does limb darkening tell us the inner Sun is hotter?!

More information

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

Chapter 14 Our Star A Closer Look at the Sun. Why was the Sun s energy source a major mystery? Chapter 14 Our Star 14.1 A Closer Look at the Sun Our goals for learning Why was the Sun s energy source a major mystery? Why does the Sun shine? What is the Sun s structure? Why was the Sun s energy source

More information

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

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

More information

This project has received funding from the European Union s Horizon 2020 research and innovation programme under the Marie-Sklodowska-Curie grant

This project has received funding from the European Union s Horizon 2020 research and innovation programme under the Marie-Sklodowska-Curie grant This project has received funding from the European Union s Horizon 2020 research and innovation programme under the Marie-Sklodowska-Curie grant agreement number 721624. Space weather and the variable

More information

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

The Sun. Chapter 12. Properties of the Sun. Properties of the Sun. The Structure of the Sun. Properties of the Sun. Chapter 12 The Sun, Our Star 1 With a radius 100 and a mass of 300,000 that of Earth, the Sun must expend a large amount of energy to withstand its own gravitational desire to collapse To understand this

More information

Chapter 14 Our Star Pearson Education, Inc.

Chapter 14 Our Star Pearson Education, Inc. Chapter 14 Our Star Basic Types of Energy Kinetic (motion) Radiative (light) Potential (stored) Energy can change type, but cannot be created or destroyed. Thermal Energy: the collective kinetic energy

More information

Solar Dynamics Affecting Skywave Communications

Solar Dynamics Affecting Skywave Communications Solar Dynamics Affecting Skywave Communications Ken Larson KJ6RZ October 2010 1 Page Subject 3 1.0 Introduction 3 2.0 Structure of the Sun 3 2.1 Core 3 2.2 Radiation Zone 4 2.3 Convection Zone 4 2.4 Photosphere

More information

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

4 Layers of the Sun. CORE : center, where fusion occurs 4 Layers of the Sun CORE : center, where fusion occurs RADIATION LAYER: energy transfer by radiation (like energy coming from a light bulb or heat lamp which you can feel across the room) CONVECTION LAYER:

More information

CESAR BOOKLET General Understanding of the Sun: Magnetic field, Structure and Sunspot cycle

CESAR BOOKLET General Understanding of the Sun: Magnetic field, Structure and Sunspot cycle CESAR BOOKLET General Understanding of the Sun: Magnetic field, Structure and Sunspot cycle 1 Table of contents Introduction to planetary magnetospheres and the interplanetary medium... 3 A short introduction

More information

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

Chapter 14 Lecture. Chapter 14: Our Star Pearson Education, Inc. Chapter 14 Lecture Chapter 14: Our Star 14.1 A Closer Look at the Sun Our goals for learning: Why does the Sun shine? What is the Sun's structure? Why does the Sun shine? Is it on FIRE? Is it on FIRE?

More information

Astronomy 150: Killer Skies. Lecture 18, March 1

Astronomy 150: Killer Skies. Lecture 18, March 1 Assignments: Astronomy 150: Killer Skies HW6 due next Friday at start of class HW5 and Computer Lab 1 due Night Observing continues next week Lecture 18, March 1 Computer Lab 1 due next Friday Guest Lecturer:

More information

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

The sun, yellow dwarf star at the heart of the solar system NASA.gov, adapted by Newsela staff Name: Period: Date: Article of the Week Directions: Read the following article carefully and annotate. You need to include at least 1 annotation per paragraph. Be sure to include all of the following in

More information

Name Date Per Teacher. Packet #4 The Sun

Name Date Per Teacher. Packet #4 The Sun 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

More information

Chapter 8 The Sun Our Star

Chapter 8 The Sun Our Star Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). Chapter 8 The Sun

More information

Teacher Background: The Dancing Lights Program

Teacher Background: The Dancing Lights Program Teacher Background: The Dancing Lights Program The Sun Many people think the Sun is just a fiery yellow ball. The Sun isn t actually burning because fire requires oxygen. Really, the Sun a giant ball of

More information

Correction to Homework

Correction to Homework Today: Chapter 10 Reading Next Week: Homework Due March 12 Midterm Exam: March 19 Correction to Homework #1: Diameter of eye: 2.5 cm #10: See Ch. 11 Office Hours Monday. 11AM -2 PM Help Sessions Available:

More information

1 A= one Angstrom = 1 10 cm

1 A= one Angstrom = 1 10 cm Our Star : The Sun )Chapter 10) The sun is hot fireball of gas. We observe its outer surface called the photosphere: We determine the temperature of the photosphere by measuring its spectrum: The peak

More information

9.5 Troposphere. Describe the characteristics and importance of the troposphere. Explain temperature inversion and its role in the troposphere.

9.5 Troposphere. Describe the characteristics and importance of the troposphere. Explain temperature inversion and its role in the troposphere. 9.5 Troposphere Describe the characteristics and importance of the troposphere. Explain temperature inversion and its role in the troposphere. Why is the troposphere important? All of the wind, rain, and

More information

Solar-terrestrial relation and space weather. Mateja Dumbović Hvar Observatory, University of Zagreb Croatia

Solar-terrestrial relation and space weather. Mateja Dumbović Hvar Observatory, University of Zagreb Croatia Solar-terrestrial relation and space weather Mateja Dumbović Hvar Observatory, University of Zagreb Croatia Planets Comets Solar wind Interplanetary magnetic field Cosmic rays Satellites Astronauts HELIOSPHERE

More information

Is There Really Weather in Space?

Is There Really Weather in Space? SOHO, NASA/ESA Is There Really Weather in Space? Looking at the sky with the naked eye, the Sun seems static, placid, constant. From the ground, the only noticeable variations in the Sun are its location

More information

The Sun ASTR /17/2014

The Sun ASTR /17/2014 The Sun ASTR 101 11/17/2014 1 Radius: 700,000 km (110 R ) Mass: 2.0 10 30 kg (330,000 M ) Density: 1400 kg/m 3 Rotation: Differential, about 25 days at equator, 30 days at poles. Surface temperature: 5800

More information

The Dancing Lights Program

The Dancing Lights Program The Sun Teacher Background: The Dancing Lights Program Margaux Krahe Many people think the Sun is just a fiery yellow ball. The Sun is not actually burning because fire requires oxygen. Really, the Sun

More information

Proton-proton cycle 3 steps PHYS 162 1

Proton-proton cycle 3 steps PHYS 162 1 Proton-proton cycle 3 steps PHYS 162 1 4 Layers of the Sun CORE : center, where fusion occurs RADIATION: energy transfer by radiation CONVECTION: energy transfer by convection PHOTOSPHERE: what we see

More information

ASTR 100. Lecture 15: The Sun

ASTR 100. Lecture 15: The Sun ASTR 100 Lecture 15: The Sun Start reading about: The Sun (Ch. 10), Spectra (Ch. 5), Stars (Ch. 11) Next week: Stars and Spectra Midterm: Tuesday, February 18 th UW planetarium: Tuesday, March 4 th 3:00pm

More information

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

The Sun: Our Star. A glowing ball of gas held together by its own gravity and powered by nuclear fusion Our Star, the Sun The Sun: Our Star A glowing ball of gas held together by its own gravity and powered by nuclear fusion Radius: 700,000 km (435,000 miles) Diameter: 1.392 million km (865,000 miles) Circumference:

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

The Sun. Never look directly at the Sun, especially NOT through an unfiltered telescope!!

The Sun. Never look directly at the Sun, especially NOT through an unfiltered telescope!! The Sun Introduction We will meet in class for a brief discussion and review of background material. We will then go outside for approximately 1 hour of telescope observing. The telescopes will already

More information

How the Sun Works. Presented by the

How the Sun Works. Presented by the How the Sun Works Presented by the The Sun warms our planet every day, provides the light by which we see and is absolutely necessary for life on Earth. In this presentation, we will examine the fascinating

More information

Sunspot Cycle Worksheet

Sunspot Cycle Worksheet Sunspot Cycle Worksheet Read the Explore information and answer the Explain questions in your own words. Explore: Global warming and climate change are international concerns and the focus of much controversy.

More information

Solar Flares and CMEs. Solar Physics 1

Solar Flares and CMEs. Solar Physics 1 Solar Flares and CMEs Solar Physics 1 What is a solar flare? What is a CME? A solar flare is a sudden eruption of energetic charged particles from the Sun s corona. A coronal mass ejection (CME) is, by

More information

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

Astronomy 210. Outline. Nuclear Reactions in the Sun. Neutrinos. Solar Observing due April 15 th HW 8 due on Friday. Astronomy 210 Outline This Class (Lecture 30): Solar Neutrinos Next Class: Stars: Physical Properties Solar Observing due April 15 th HW 8 due on Friday. The Sun Our closest star The Outer Layers of the

More information

Space Weather and Satellite System Interaction

Space Weather and Satellite System Interaction Space Engineering International Course, Kyutech, 4 th Quarter Semester 2017 Space Weather and Satellite System Interaction Lecture 2: Space Weather Concept, Reporting and Forecasting Assoc. Prof. Ir. Dr.

More information

SPACE WEATHER: STORMS FROM THE SUN

SPACE WEATHER: STORMS FROM THE SUN GIFT 2013 - Natural Hazards Vienna, Austria, 10 April 2013 SPACE WEATHER: STORMS FROM THE SUN Norma B. Crosby Belgian Institute for Space Aeronomy Ringlaan-3-Avenue Circulaire, B-1180 Brussels, Belgium

More information

Using This Flip Chart

Using This Flip Chart Using This Flip Chart Solar storms can cause fluctuations in the magnetosphere called magnetic storms. These magnetic storms have disabled satellites and burned out transformers shutting down power grids.

More information

Space Weather Awareness in the Arctic. Torsten Neubert Head of Section for Solar System Physics

Space Weather Awareness in the Arctic. Torsten Neubert Head of Section for Solar System Physics Space Weather Awareness in the Arctic Torsten Neubert Head of Section for Solar System Physics Technology in the Arctic There is significant potential Resources Tourism helped by receding ocean ice There

More information

michele piana dipartimento di matematica, universita di genova cnr spin, genova

michele piana dipartimento di matematica, universita di genova cnr spin, genova michele piana dipartimento di matematica, universita di genova cnr spin, genova first question why so many space instruments since we may have telescopes on earth? atmospheric blurring if you want to

More information

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

Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere. Chapter 29 and 30 Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere. Explain how sunspots are related to powerful magnetic fields on the sun.

More information

An Introduction to Space Weather. J. Burkepile High Altitude Observatory / NCAR

An Introduction to Space Weather. J. Burkepile High Altitude Observatory / NCAR An Introduction to Space Weather J. Burkepile High Altitude Observatory / NCAR What is Space Weather? Space Weather refers to conditions in interplanetary space, produced by the Sun, that can disrupt

More information

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

Astronomy Ch 16 The Sun. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch 16 The Sun MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) The light we see from the Sun comes from which layer?

More information

A Closer Look at the Sun

A Closer Look at the Sun Our Star A Closer Look at the Sun Our goals for learning Why was the Sun s energy source a major mystery? Why does the Sun shine? What is the Sun s structure? Why was the Sun s energy source a major mystery?

More information

Space Weather. Dr Thomas J Bogdan Director, Space Weather Prediction Center Boulder, CO

Space Weather. Dr Thomas J Bogdan Director, Space Weather Prediction Center Boulder, CO Space Weather Dr Thomas J Bogdan Director, Space Weather Prediction Center Boulder, CO 2011 DIB CIP Meeting 25 August 2011 Space Weather Prediction Center Our Mission: To provide space weather products

More information

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

Guidepost. Chapter 08 The Sun 10/12/2015. General Properties. The Photosphere. Granulation. Energy Transport in the Photosphere. Guidepost The Sun is the source of light an warmth in our solar system, so it is a natural object to human curiosity. It is also the star most easily visible from Earth, and therefore the most studied.

More information

19 The Sun Introduction. Name: Date:

19 The Sun Introduction. Name: Date: Name: Date: 19 The Sun 19.1 Introduction The Sun is a very important object for all life on Earth. The nuclear reactions that occur in its core produce the energy required by plants and animals for survival.

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Name Team Period. Station #1 (drawing)

Name Team Period. Station #1 (drawing) Unit 5 Notes ATMOSPHERE Name Team Period Station #1 (drawing) When done drawing, read and answer the following questions. Troposphere - layer closest to Earth s surface. Extends from surface to altitudes

More information

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

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Homework Ch 7, 8, 9 Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Our most detailed knowledge of Uranus and Neptune comes from 1) A) the

More information

Lesson 3 THE SOLAR SYSTEM

Lesson 3 THE SOLAR SYSTEM Lesson 3 THE SOLAR SYSTEM THE NATURE OF THE SUN At the center of our solar system is the Sun which is a typical medium sized star. Composed mainly of Hydrogen (73% by mass), 23% helium and the rest is

More information

Investigations in Earth and Space Science Semester Review: Unit 1 and Unit 2

Investigations in Earth and Space Science Semester Review: Unit 1 and Unit 2 IESS Unit 1: Solar Energy & Fluid Circulation Review Directions: Write the answer to each question in the box to the right of the question. Fold your paper along the line and use this as a review sheet!

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? 10.1 Atmospheric Basics Our goals for learning:! What is an atmosphere?! How does the greenhouse effect warm

More information

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

The Sun Our Star. Properties Interior Atmosphere Photosphere Chromosphere Corona Magnetism Sunspots Solar Cycles Active Sun The Sun Our Star Properties Interior Atmosphere Photosphere Chromosphere Corona Magnetism Sunspots Solar Cycles Active Sun General Properties Not a large star, but larger than most Spectral type G2 It

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? Planetary Atmospheres Pressure Composition Greenhouse effect Atmospheric structure Color of the sky 1 Atmospheres

More information

Chapter 8 Geospace 1

Chapter 8 Geospace 1 Chapter 8 Geospace 1 Previously Sources of the Earth's magnetic field. 2 Content Basic concepts The Sun and solar wind Near-Earth space About other planets 3 Basic concepts 4 Plasma The molecules of an

More information

Astronomy Chapter 12 Review

Astronomy Chapter 12 Review Astronomy Chapter 12 Review Approximately how massive is the Sun as compared to the Earth? A. 100 times B. 300 times C. 3000 times D. 300,000 times E. One million times Approximately how massive is the

More information

Physical Science Context Lecture 2 The Earth and Sun's Magnetic Fields

Physical Science Context Lecture 2 The Earth and Sun's Magnetic Fields Physical Science Context Lecture 2 The Earth and Sun's Magnetic Fields The earth is a huge magnetic and close to its surface it can be approximated as a bar magnet (a magnetic dipole) that is positioned

More information

INCREASED LEVEL OF UV AND X-RAY RADIATION

INCREASED LEVEL OF UV AND X-RAY RADIATION INCREASED LEVEL OF UV AND X-RAY RADIATION By Senem ÜNAL Page 1 WHAT IS UV AND X-RAY? The sun radiates energy in a wide range of wavelengths, most of which are invisible to human eyes. The shorter the wavelength,

More information

Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of the normal stars.

Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of the normal stars. Chapter 23 Our Solar System Our Solar System Historical Astronomy Wandering Stars Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of

More information

Website Lecture 3 The Physical Environment Part 1

Website   Lecture 3 The Physical Environment Part 1 Website http://websites.rcc.edu/halama Lecture 3 The Physical Environment Part 1 1 Lectures 3 & 4 1. Biogeochemical Cycling 2. Solar Radiation 3. The Atmosphere 4. The Global Ocean 5. Weather and Climate

More information

Earth s Magnetic Field

Earth s Magnetic Field Magnetosphere Earth s Magnetic Field The Earth acts much like a bar magnet: its magnetic field deflects compasses on the Earth s surface to point northwards. Magnetic field lines North Pole S N South Pole

More information

The Structure of the Sun. CESAR s Booklet

The Structure of the Sun. CESAR s Booklet How stars work In order to have a stable star, the energy it emits must be the same as it can produce. There must be an equilibrium. The main source of energy of a star it is nuclear fusion, especially

More information

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

Earth Science Lesson Plan Quarter 4, Week 7, Day 1 Earth Science Lesson Plan Quarter 4, Week 7, Day 1 Outcomes for Today Standard Focus: Earth Sciences 1.e Students know the Sun is typical star and is powered by nuclear reactions, primarily the fusion

More information

Killer Skies. Homework 5 due Monday Night Observing continuing Last time: White Dwarf Today: Active Sun. Music: Invisible Sun Police

Killer Skies. Homework 5 due Monday Night Observing continuing Last time: White Dwarf Today: Active Sun. Music: Invisible Sun Police Killer Skies Homework 5 due Monday Night Observing continuing Last time: White Dwarf Today: Active Sun Music: Invisible Sun Police 1 Night Observing Night Observing probably last week if you do it, need

More information

Effective August 2007 All indicators in Standard / 14

Effective August 2007 All indicators in Standard / 14 8-4.1 Summarize the characteristics and movements of objects in the solar system (including planets, moons, asteroids, comets, and meteors). Taxonomy level: 2.4-B Understand Conceptual Knowledge Previous/Future

More information

Chapter 23. Our Solar System

Chapter 23. Our Solar System Chapter 23 Our Solar System Our Solar System 1 Historical Astronomy Wandering Stars Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths

More information

Geomagnetic Disturbances (GMDs) History and Prediction

Geomagnetic Disturbances (GMDs) History and Prediction Geomagnetic Disturbances (GMDs) History and Prediction J. Patrick Donohoe, Ph.D., P.E. Dept. of Electrical and Computer Engineering Mississippi State University Box 9571 Miss. State, MS 39762 donohoe@ece.msstate.edu

More information

Chapter 10 Our Star. X-ray. visible

Chapter 10 Our Star. X-ray. visible Chapter 10 Our Star X-ray visible Radius: 6.9 10 8 m (109 times Earth) Mass: 2 10 30 kg (300,000 Earths) Luminosity: 3.8 10 26 watts (more than our entire world uses in 1 year!) Why does the Sun shine?

More information

1-4-1A. Sun Structure

1-4-1A. Sun Structure Sun Structure A cross section of the Sun reveals its various layers. The Core is the hottest part of the internal sun and is the location of nuclear fusion. The heat and energy produced in the core is

More information

Sun Earth Connection Missions

Sun Earth Connection Missions Sun Earth Connection Missions ACE Advanced Composition Explorer The Earth is constantly bombarded with a stream of accelerated particles arriving not only from the Sun, but also from interstellar and galactic

More information

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

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 The Sun Visible Image of the Sun 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 by nuclear fusion at its

More information

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

Chapter 9 The Sun. Nuclear fusion: Combining of light nuclei into heavier ones Example: In the Sun is conversion of H into He Our sole source of light and heat in the solar system A common star: a glowing ball of plasma held together by its own gravity and powered by nuclear fusion at its center. Nuclear fusion: Combining of

More information

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

Sun s Properties. Overview: The Sun. Composition of the Sun. Sun s Properties. The outer layers. Photosphere: Surface. Nearest. Overview: The Sun Properties of the Sun Sun s outer layers Photosphere Chromosphere Corona Solar Activity Sunspots & the sunspot cycle Flares, prominences, CMEs, aurora Sun s Interior The Sun as an energy

More information

Stars and Galaxies. Content Outline for Teaching

Stars and Galaxies. Content Outline for Teaching Section 1 Stars A. Patterns of stars - constellations 1. Ancient cultures used mythology or everyday items to name constellations 2. Modern astronomy studies 88 constellations 3. Some constellations are

More information

Weather What is weather? Weather. is the study of our atmosphere. Atmosphere literally means vapor (atmos) of a sphere.

Weather What is weather? Weather. is the study of our atmosphere. Atmosphere literally means vapor (atmos) of a sphere. Weather What is weather? Weather is the study of our atmosphere. Atmosphere literally means vapor (atmos) of a sphere. Our atmosphere is made up of 4 basic layers: The outermost layer is the thermosphere

More information

Space Weather and Amateur Radio: Science, Forecasting and Effects. The Aerospace Corporation Dayton Hamvention Antenna Forum 19 May 2017

Space Weather and Amateur Radio: Science, Forecasting and Effects. The Aerospace Corporation Dayton Hamvention Antenna Forum 19 May 2017 Space Weather and Amateur Radio: Science, Forecasting and Effects The Aerospace Corporation Dayton Hamvention Antenna Forum 19 May 2017 What is Space Weather? Essentially Space Weather is: A planet s interaction

More information

The Moon s relationship with Earth The formation of the Moon The surface of the Moon Phases of the Moon Travelling to the Moon

The Moon s relationship with Earth The formation of the Moon The surface of the Moon Phases of the Moon Travelling to the Moon The Moon The Moon s relationship with Earth The Moon orbits the Earth every 27.3 days. The tides on Earth are caused mostly by the gravitational pull of the Moon and the Sun. The Moon's gravitational pull

More information

Chapter 23. Light, Astronomical Observations, and the Sun

Chapter 23. Light, Astronomical Observations, and the Sun Chapter 23 Light, Astronomical Observations, and the Sun The study of light Electromagnetic radiation Visible light is only one small part of an array of energy Electromagnetic radiation includes Gamma

More information

Weather forecasting & Optical Phenomena

Weather forecasting & Optical Phenomena Weather forecasting & Optical Phenomena Weather forecasting Weather forecasting Weather forecasting National Weather Service (NWS) is a branch of the National Oceanic and Atmospheric Administration (NOAA).

More information

NOAA Space Weather Prediction Center. A Profile of Space Weather

NOAA Space Weather Prediction Center. A Profile of Space Weather NOAA Space Weather Prediction Center A Profile of Space Weather Space Weather Prediction Center 24-hour Forecast Center, Boulder, CO U. S. Department of Commerce National Oceanic and Atmospheric Administration

More information

About the Van Allen Probes Mission

About the Van Allen Probes Mission Van Allen Probes Exploring th About the Van Allen Probes Mission To help us understand how Earth responds to changes in the sun s energy and how that response affects life and society, NASA launched the

More information

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

The Sun is the nearest star to Earth, and provides the energy that makes life possible. 1 Chapter 8: The Sun The Sun is the nearest star to Earth, and provides the energy that makes life possible. PRIMARY SOURCE OF INFORMATION about the nature of the Universe NEVER look at the Sun directly!!

More information

The Sun: A Star of Our Own ASTR 2110 Sarazin

The Sun: A Star of Our Own ASTR 2110 Sarazin The Sun: A Star of Our Own ASTR 2110 Sarazin Sarazin Travel Wednesday, September 19 afternoon Friday, September 21 Will miss class Friday, September 21 TA Molly Finn will be guest lecturer Cancel Office

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc. Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

MAGNETISM QUIZ MAGNETISM

MAGNETISM QUIZ MAGNETISM MAGNETISM QUIZ MAGNETISM 1. What force steers particles in a supercollider? A. Centrifugal B. Electric C. Magnetic D. Gravity 2. What can we learn from the paths of charged particles after a supercollider

More information

CHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration

CHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration CHAPTER 11 We continue to Learn a lot about the Solar System by using Space Exploration Section 11.1 The Sun page 390 -Average sized star -Millions of km away -300,000 more massive then Earth, 99% of all

More information