Throughout history, the Sun has been central to cultures all over the world. In Saskatchewan, the Nakawe understand that the Sun sees all, even through.

Slides:



Advertisements
Similar presentations
Features of the Sun 6 th Grade. The Sun’s Composition.
Advertisements

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.
 How Many Stars are in our Solar System???? a.Hundreds b.Millions c.Billions Explain why you chose the answer you picked.
The Sun – Describe characteristics of the Sun (S6C3PO2 high school)
The Sun. Of medium size by star standards, it is composed mainly of hydrogen (73 percent by mass) and helium (25 percent by mass)
Stars, Galaxies, and the Universe- Course 3
The sun and our solar system Grade 9 Science Space Part 2.
+ 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.
Youtube: Secrets of a Dynamic Sun The Sun – Our Star
The Sun. Sun Considered a medium STAR 93,000,000 miles away from Earth 1.39 million kilometers in diameter (one million Earths can fit inside the sun.
Our Sun A medium sized star. Our Sun Our sun is a typical medium sized star. A star is a hot ball of plasma that shines because nuclear fusion is taking.
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.
Notes The Sun. Stars an object that produces it own energy, including heat and light.
Grade 9 Academic Science.  the center of our solar system – heliocentric model.  the Sun has many different layers – each performing different activities.
Lesson 3.3: The Sun.
The Sun Section 26.1.
Chapter 20, Section 2 The Sun Anne Marie Scrudato’s notes borrowed by Rusty Sturken.
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.
The Sun.
The Sun Chapter 3 Lesson 6 Page 122.
The Sun 1 of 200 billion stars in the Milky Way. Our primary source of energy.
Our Sun  93 million miles (150 million kilometers) from Earth  99.8% of the mass of our solar system.
Ch. 26.1: Our Sun!.
SUN
Pennsylvania is misspelled on the Liberty Bell. The sun is a main sequence star. It is about 93 million miles away. And is about 5 Billion yrs old and.
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.
Our Sun 93 million miles from Earth 150 million kilometers Earth 99.8% of the mass of our solar system.
THE SUN Energy from the sun, in the form of sunlight supports all life via photosynthesis, and drives the Earth’s climate and weather.
The Sun! PH Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
The Sun – Our Star Our sun is considered an “average” star and is one of the 100 BILLION stars that make up the Milky Way galaxy. But by no MEANS does.
The Sun Distance from Earth: 150 million km OR 93 million miles Size: 1.4 million km in diameter Age: 4.5 billion years old, halfway through its 10 billion.
+ The Sun.
The Sun: A Medium-sized StarSunThe Sun: A Medium-sized StarSun.
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.
Lesson 2.  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.
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.
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.
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.
Our Star the Sun. The Sun – Our Star Our sun is considered an “average” star and is one of the 200 BILLION stars that make up the Milky Way galaxy. But.
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.
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.
Starter 1.The word refract means “______________”. 2.Name two types of optical telescopes. 3.List the advantages of using radio telescopes instead of optical.
The Sun.
The Sun Average in size… yes AVERAGE!!
Falcon Focus What do you know about the sun?
THE SUN.
The Sun Sun Facts Our sun accounts for 99.8% of ALL the mass in our solar system Average size star ( ~ 1.3 million Earths could fit inside.
Performance Indicator 8.E.4B.6
The Sun Our Star.
THE SUN.
The Sun.
Fusion vs Fission Fission Fusion Division of an atom’s nucleus
Our Sun Notes.
The Sun.
Chapter 20 Section 2: The Sun
Bell Ringer The outer layer of the Sun’s atmosphere is actually hotter than the interior of the Sun. Explain why you believe this is so.
The Sun’s Energy The core of the sun acts like a furnace.
Notes The Sun.
Ch. 26.1: Our Sun!.
24.3 – The Sun.
The Sun.
The sun gives off tremendous amounts of energy
THE SUN.
Sun & Solar System Structure of the Sun:.
The Sun.
THE SUN.
Presentation transcript:

Throughout history, the Sun has been central to cultures all over the world. In Saskatchewan, the Nakawe understand that the Sun sees all, even through clouds and storms. Because of this and the light the Sun gives-both spiritual and physical-it inspires us to achieve excellence in all we do. -Pearson Saskatchewan Science 9

The Sun supports almost all life on Earth. It provides the energy needed by all plants and animals on Earth

Because the Sun is the closest star to the Earth, it is also the brightest object in the sky.

It sends out so much light energy that you can not see the other stars until the sun has set.

Like all stars the sun produces energy through a process called nuclear fusion. Nuclear Fusion: a process during which substances fuse to form new substances, releasing huge amounts of heat, light and other forms of energy.

Every second the sun makes more energy than humans have used throughout our entire history. Scientists have calculated that the sun has been producing energy for about 5 billion years. Scientists estimate that it will continue producing energy for about another 5 billion years.

Space Probe – Ulysses was launched in 1990 to study the poles of the sun

SOHO – has 12 special instruments for observing the sun

Corona: the hot outer part of the Sun, where the gases reach temperatures of about 1 million degrees Celsius. Chromosphere: the inner atmosphere of the sun

Photosphere: called the surface of the Sun, although it is made up of churning gases, not a solid surface at all.

Core: where nuclear fusion produces the Sun’s energy. Temperatures here reach 15 million degrees Celsius and the pressure is enormous

Sunspot: a region on the Sun’s surface that is cooler than the surrounding areas. Although still very bright, by contrast it looks darker than the surrounding areas. Sunspots indicate regions where the magnetic field is extremely strong, slowing down convection. This prevents the plasma from mixing, allowing the region to cool.

Solar Prominence: is a large, low energy, curved, bright stream of particles. The electrically charged plasma in the prominence is shaped by the Sun’s magnetic field lines. This makes part of the magnetic field visible. The curved shape often forms a complete loop and may last for several hours or several weeks.

Solar flare: is a high energy massive explosion at the surface of the Sun. This sudden release of magnetic energy often flings hot plasma out into space. It travels outward from the chromosphere through the corona. Solar flares travel extremely quickly and last only a few minutes

The tremendous amount of energy at the surface of the Sun produces a thin but steady stream of subatomic particles, or plasma. This constant flow of particles streaming out of the Sun’s surface in all directions is called the solar wind.

The solar wind is responsible for creating displays of green, yellow, and red light in the skies near Earth’s northern and southern regions.

In the northern hemisphere, these light displays are called the aurora borealis (the Northern Lights) and in the southern hemisphere, they are called the aurora australis (the Southern lights). Auroras form as particles from the solar wind and are trapped by Earth’s magnetic field and are swept toward the North and South Poles. The strength of the solar wind affects the shape and size of the aurora in these zones. Changes in the solar wind make the aurora appear to be “dancing” in the night sky.

Many First Nations and Metis peoples understand that the Northern Lights are the spirits of family dancing in the night sky. The round dance is connected to the aurora. Many believe that when the round dance occurs, the Northern Lights are all around. Some Dene believe the Northern Lights provide them with the caribou and so were important for their survival. Some Indigenous cultures of Saskatchewan also consider the Northern Lights to be very potent spirits or spirit dancers, who, if disrespected, may come down from the sky. First Nations and Metis peoples treat the night sky with respect and speak about it with great reverence and humility. Some Elders express a concern that many young First Nations and Metis peoples have lost their connection to the sacred night sky. They worry all the light pollution in towns and cities erodes our relationship with the land and our concept of night. - Pearson Saskatchewan Science 9, p. 324

Episode 1: Secrets of the Sun It is a fireball in the sky, a bubbling, boiling, kinetic sphere of white hot plasma, exploding and erupting. Its size is almost unimaginable--one million Earths would fit within its boundaries. In this violence is born almost all the energy that makes existence on Earth possible, yet, its full mysteries are only now beginning to be understood. From Sun spots to solar eclipses, solar flares to solar storms, the birth of the sun to its potential death, discover the science and history behind this celestial object that makes life on Earth exist