The Sun Chapter 17.

Slides:



Advertisements
Similar presentations
What is the fate of our sun and other stars?
Advertisements

Sun Mr. Skirbst Physical Science Topic 26. The Sun.
Complete the 3 question Bell Ringer independently at your seat You will have 4 Minutes to complete this assignment Please begin immediately Independent.
Chapter 8 The Sun – Our Star.
Understanding Sunspots. What is a Sunspot? The Sun’s Visible Surface The Lower Atmosphere.
Agenda: Here comes the sun April 10 1.Learning Target: I can make a presentation of one aspect of solar study to teach other astronomers about the sun.
The Sun – Our Star Chapter 7:. General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years)
General Properties Absolute visual magnitude M V = 4.83 Central temperature = 15 million 0 K X = 0.73, Y = 0.25, Z = 0.02 Initial abundances: Age: ~ 4.52.
Instructor Notes These images correspond to the layers of the Sun discussed in the Features of the Sun – 3D Sun lesson. Layers – Photosphere:
CH – Solar Activity CH MARQUES. Terms to know…  Sunspot  Prominence  Granules  solar flare  coronal mass ejection  aurora.
1 Grades 3 - 5: Introduction. 2 Better Observation Of The Sun And Earth Importance of Space Technology.
Chapter 7 The Sun. Solar Prominence – photo by SOHO spacecraft from the Astronomy Picture of the Day site link.
The Sun- Our Star. The Sun- Our Star Star Parts: core radiation zone convection zone photosphere chromosphere corona solar wind.
1 The Sun in STEREO K. Murawski Department of Astrophysics, UMCS.
How The Sun Works Brady Gurley. The Sun: What it’s made of -~70% Hydrogen -~28% Helium -~1.5% Carbon, Nitrogen, & Oxygen -~0.5% Other Elements (Neon,
The Active Sun. Sunspots Umbra Penumbra Granulation.
The Sun a medium sized star 93,000,000 miles away 109 times diameter of Earth 1 million Earths could fit in the Sun Made of gas: 82% hydrogen, 17% helium,
The Sun. 99% of the matter of the solar system is in the Sun. The Sun is an Average Star (main sequence star) The sun is not a Binary Star. (most stars.
Our Sun. Why do we care about the Sun... - Light, heat, life - Space weather solar wind (1,000,000 mph) flares (UV, x-ray radiation) disturb Earth's magnetic.
Space Weather Alice Hirsh International Studies and Economics College of Arts and Sciences.
Solar Physics & upper-Atmosphere Research Group University of Sheffield Linear and non-linear waves and oscillations L1: Examples for waves Robert von.
The Sun.
The SUN!.
SLIDE SHOW 3 B changes due to transport + diffusion III -- * * magnetic Reynold number INDUCTION EQUATION B moves with plasma / diffuses through it.
The Sun. Components of the Sun Core Radiative zone Convective zone Atmosphere –Photosphere –Chromosphere –Corona Solar wind (mass loss)
The Sun- Solar Activity. Damage to communications & power systems.
Observing the Solar System It is now thought that the Sun is the center of the solar system – called the heliocentric model - Copernicus It was once thought.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 1 Announcements: Homework #6 due Tuesday Last problem requires.
SUN, EARTH AND SPACE. THE SUN CLOSE UP: INSIDE AND OUT.
SOLAR FLARES AND ERUPTIONS Lyndsay Fletcher University of Glasgow.
Chapter 9 Our Star, the Sun. What do you think? What is the surface of the Sun like? Does the Sun rotate? What makes the Sun shine?
CHAPTER 24.3 THE SUN. Learning Targets 1.Describe the layers of the Sun 2.Describe the surface features of the Sun.
The Sun Diameter is 110 times Earth’s Mass is 745 times Earth’s
Chapters 12 and 13 The Sun & Measuring the Properties of Stars.
Sun Notes. Characteristics CLOSEST star to earth CLOSEST star to earth The bright star in the center is Proxima Centauri.
Sun, Moon, Earth, How do they work together to help life survive? our sun.
Outer Layers of the Sun Photosphere –Limb darkening –Sun spots Chromosphere Corona Prominences, flares, coronal mass ejections Reading
Our Star, the Sun. The Sun is the Largest Object in the Solar System The Sun contains more than 99.85% of the total mass of the solar system If you.
Ch Solar Activity. Sunspots Gases inside the sun move up and down due to convection and the sun’s magnetic fields. Regions of the photosphere are.
Sun phenomena. sunspots By tracking them, we realized the sun rotates Click here.
The Sun. Solar Structure Core Radiative zone Convective zone Atmosphere –Photosphere –Chromosphere –Corona Solar wind (mass loss)
Our amazing sun. sunspots By tracking them, we realized the sun rotates Click here.
OUR SUN.
(8th) Chapter 14-2 Cornell Notes
Sun: General Properties
THE SUN.
The Sun.
Magnetic Field.
The Sun: Portrait of a G2V star
Our Sun Notes.
Chapter 20 Section 2: The Sun
What is the fate of our sun and other stars?
The Sun and the Moon.
Overview of the Sun Jie Zhang Art Poland
Sun’s Layers Create a Circle Map on page: 130
Star Light Star Bright Desktop Constellations
Solar Activity Chapter 8 Section 3.
What is the sun? What is the structure of the sun?
8.E.4B.6 Notes.
Solar and Heliospheric Physics
Chapter 9 The Sun.
Sunspots Sunspots are the most well known feature on the photosphere. They are a region of the solar surface that is dark and relatively cool; and has.
Bell Ringer Complete the 3 question Bell Ringer independently at your seat You will have 4 Minutes to complete this assignment Please begin immediately.
Grades 3 - 5: Introduction
Kick Start Complete the 3 question Kick Start independently at your seat You will have 4 Minutes to complete this assignment Please begin immediately Independent.
Note topic for chapter 17 what is the source of the sun’s energy
The Sun Fusion: E = mc2 What is Plasma? The 4th state of matter containing charged particles.
Grades 3 - 5: Introduction
Chapter 26 The Sun The Sun Is a star Is a main sequence star
8-11 The Sun Astronomy November 18, 2008 Sanders.
Presentation transcript:

The Sun Chapter 17

Fig. 17.1

Fig. 17.2

Fig. 17.4

Fig. 17.5

Fig. 17.6

Fig. 17.7

Fig. 17.8

Fig. 17.9

Fig. 17.10

Fig. 17.11

Fig. 17.12

Fig. 17.13

Fig. 17.14

Fig. 17.15

Fig. 17.16

Fig. 17.17

Fig. 17.18

Fig. 17.19 Magnetic field and sun spots

Fig. 17.20 Chromosphere

Spicules on the Chromosphere Fig. 17.21 Spicules on the Chromosphere

Fig. 17.22

Fig. 17.23

Fig. 17.24

Fig. 17.25 Coronal holes

Fig. 17.26

Fig. 17.27 Coronal loops

Fig. 17.29 Solar Prominence

Fig. 17.30

Fig. 17.31 Solar Flare

Fig. 17.32

Fig. 17.33 Sunspot Cycle

Fig. 17.34 Solar Activity

Fig. 17.35 The butterfly diagram

Fig. 17.36

Fig. 17.37