Ch. 28.2 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.

Slides:



Advertisements
Similar presentations
BY NICK MITCHELL AND CADE HESS The Suns Atmosphere, Surface Features, Solar Wind, and Effects on the Earth.
Advertisements

Features of the Sun 6 th Grade. The Sun’s Composition.
The Sun 6.E.1.2 Explain why Earth sustains life while other planets do not based on their properties (including types of surface, atmosphere.
The Sun 6.E.1.2 Explain why Earth sustains life while other planets do not based on their properties (including types of surface, atmosphere.
Suns Disturbances Stars Lives Galaxies and Constellations Terms to Know Grab Bag
The Sun – Describe characteristics of the Sun (S6C3PO2 high school)
The Sun Structure of the Sun & Solar Activity. Parts of the Sun Core: enormous pressure & high temperatures cause the fusion of hydrogen into helium.
Structure of the Sun & Solar Activity
CH – Solar Activity CH MARQUES. Terms to know…  Sunspot  Prominence  Granules  solar flare  coronal mass ejection  aurora.
THE SUN NOTES.
+ The Sun. Sun Facts Makes life on our planet possible by giving us great amounts of light and heat Contains about 98% of the mass of the entire Solar.
EARTH & SPACE SCIENCE Chapter 29 The Sun 29.2 Solar Activity.
THE SUN AND STARS And anything I want to put in here.
The Sun Earth Science - Mr. Gallagher. The Sun is the Earth's nearest star. Similar to most typical stars, it is a large ball of hot electrically charged.
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.
Lesson 3.3: The Sun.
The Sun Section 26.1.
Chapter 9 The Sun. 9.4 The Active Sun Sunspots: appear dark because slightly cooler than surroundings:
The Sun Unit 5 PESS 2. Energy from the Sun Electromagnetic energy is a type of energy that can travel through space an example is visible light Light.
 Ch 29: The Sun by: Emily Hartley. Nuclear fusion  The process by which nuclei of small atoms combine to form a new, more massive nucleus; the process.
Inner Workings of the Sun (87). Sun is mostly hydrogen and helium gas (plasma). Core (15,000,000 ° C): –Fuels the sun, where the fusing of Hydrogen 
The Sun – El Sol – Die Sonne ESPS- Palmer High School.
The Sun- Solar Activity. Damage to communications & power systems.
Ch. 26.1: Our Sun!.
The Sun – Our Local Star Only star in our solar system Consists mostly of Hydrogen Gas Hydrogen turns into helium producing energy that is the source of.
THE SUN. The Sun The sun has a diameter of 900,000 miles (>100 Earths could fit across it) >1 million Earths could fit inside it. The sun is composed.
The Sun is our Local Star Pages Energy Flows Through the Sun’s Layers The Sun produces energy from Hydrogen and turns it into Helium The Sun.
Chapter 11. The Sun  average-sized star.  times more mass than Earth  The sun’s mass results in great pressure and heat at the centre of the.
Our Star The Sun. Our Star Our Sun is a star that is at the center of our solar system. The Sun is a hot ball of glowing gasses. Deep inside the core,
+ The Sun.
The Sun Diameter is 110 times Earth’s Mass is 745 times Earth’s
The Sun appears to have been active for 4.6 billion years and has enough fuel to go on for another five billion years or so.
The Sun – El Sol – Die Sonne ESPS- Palmer High School.
Unit 8 Chapter 29 The Sun. We used to think that our sun was a ball of fire in the sky. Looking at our sun unaided will cause blindness. The Sun’s Energy.
Part 6:The Sun Photo from
The Sun Average in size… yes AVERAGE!! Mass is almost times that of Earth and a volume that is times the volume of Earth! Appears to.
THE SUN NOTES. LAYERS of the Interior THE CORE- Nuclear Fusion occurs Diameter- 400,000 km The Radiation Zone- region of compressed gas and energy is.
The Sun. The Sun.  Is located in the outer bands of our Galaxy  Is the center of our Solar System  Is a STAR!!!  Rotation: once in about 25 days 
Chapter 28 The Sun Section 2 Solar Activity Notes 28-2.
The Sun The SUN Chapter 29 Chapter 29.
Chapter 29. Sec 1 Structure of the sun People believed the sun’s energy came from fire They believed the sun burned some type of fuel to produce energy.
Falcon Focus What do you know about the sun?
The Sun.
Performance Indicator 8.E.4B.6
The Sun and Our Earth The Structure of Our Sun The Energy of Our Sun
THE SUN.
California Standards: 1a, e.
Our Sun.
Our Sun Notes.
Chapter 20 Section 2: The Sun
The Sun.
Notes The Sun.
Ch. 26.1: Our Sun!.
Chapter 29-2 Solar Activity.
Galaxies and Constellations
Section 2: Solar Activity
The Sun The interior of the sun has three layers:
Features of the Sun 8.E.4B.6 Analyze and interpret data from the surface features of the Sun (including photosphere, corona, Sunspots, prominences, and.
Studying the Sun Ch. 24.
The Sun’s Layers and Solar Activity
The Sun and Our Earth The Structure of Our Sun The Energy of Our Sun
8.E.4B.6 Notes.
The Sun’s Energy Worksheet Review.
The Sun.
The Sun (Our Enemy).
Brain Pop The Sun
The Sun.
The Sun Fusion: E = mc2 What is Plasma? The 4th state of matter containing charged particles.
THE SUN.
Sun & Solar System Structure of the Sun:.
Presentation transcript:

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 up to 3,000’C cooler than surrounding areas. The cooler areas appear darker than the other parts of the sun.

Sunspots continued. Cool, dark areas of gas within the photosphere that are caused by magnetic fields are called sunspots. Because the sun rotates, the area of sunspots also shift, this change of spots occurs in an 11-year cycle, this is called the sunspot cycle.

Prominences and Solar Flares

Big clouds of glowing gases are called prominences, they form huge arches above the sun’s surface. Solar flares are sudden outward eruption og electrically charged particles. When these charged particles enter the atmosphere of the Earth, they can disturb the magnetic field, this is called a magnetic storm

Auroras

Auroras are magnetic storms on Earth that occur after a peak in the sunspot cycle. Electrically charged particles enter the atmosphere and strike the gas molecules and produce sheets of green, red, blue, or violet colors of light. Depending on the hemisphere where the aurora’s occur they are called either the Southern Lights or the Northern Lights.