The Sun *Our closest star

Slides:



Advertisements
Similar presentations
The Sun.
Advertisements

What is the fate of our sun and other stars?
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.
BY MARCELLA GIUFFRIDA & GRACE HILTON The Sun. Key Terms Nuclear fusion - a nuclear reaction where nuclei of low atomic numbers fuse to form a heavier.
The Sun’s Interior Remember that the sun DOES NOT have a solid surface. The sun is made ENTIRELY of gas However, the sun has an INTERIOR and an ATMOSPHERE.
Stars, Galaxies, and the Universe- Course 3
+ 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.
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 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.
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.
Full name Period II. Chapter 14, section 2: The Sun A. The Sun: is our local star. 1. Spectral Class: G2. 2. Distance to Earth:149,600,000 km *At the speed.
THE SUN.
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 Chapter 28.
The Sun.
The Sun Chapter 3 Lesson 6 Page 122.
Chapter 4; Lesson 4.1 T.O.C: The Sun is our Local Star.
The Sun’s Structure. The Core The temperature inside the sun’s core reaches about 15 million degrees Celsius. The sun produces an enormous amount of energy.
Our Sun  93 million miles (150 million kilometers) from Earth  99.8% of the mass of our solar system.
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 ASSIGNMENT #41  The word "solar" is taken from the Latin word for sun, Sol.  Solar System: a large planetary system that consists of a combination.
Our Sun 93 million miles from Earth 150 million kilometers Earth 99.8% of the mass of our solar system.
The Sun! PH Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Bellwork What two properties effect the force of gravity?
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.
The Sun Chapter 14.2.
+ The Sun.
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.
The Sun. Introduction sun’s gravity is most powerful force in solar system Force so strong because of Sun’s mass 99.8 % of the mass of the solar system.
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 
The Sun The SUN Chapter 29 Chapter 29.
The Sun The Sun is a giant, hot ball of gas held together by gravity. The Sun is a medium-sized compared with other stars in the universe. Main sequence.
The Sun.
Falcon Focus What do you know about the sun?
The Sun Lesson Objective: Students will be able to name the 6 layers of the sun. Success Skills I will divide the sun into inner zones and outer atmospheres.
Earth, Moon, and Sun Astronomy Unit.
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.
THE SUN.
(8th) Chapter 14-2 Cornell Notes
The Sun: Our Very Own Star
THE SUN.
The Sun Section 20.2.
The Sun and Other Stars How do stars shine? How are stars layered?
The sun’s gravity holds all of the planets and comets in orbit
The Sun.
The Sun.
Chapter 20 Section 2: The Sun
What is the fate of our sun and other stars?
The Sun’s Energy The core of the sun acts like a furnace.
Notes The Sun.
The Sun and Stars Lesson 2 pg. 808
The Inner Solar System The four inner planets are all relatively small and dense, and have rocky surfaces. The terrestrial planets are planets similar.
The Sun Our local star.
Studying Space.
The Sun One million Earth’s could fit inside of the sun, approximately.
The Sun (Our Enemy).
The Sun.
The Sun and Eclipses Notes.
The sun is our local star
The sun gives off tremendous amounts of energy
The Inner Solar System The four inner planets are all relatively small and dense, and have rocky surfaces. The terrestrial planets are planets similar.
Sun Lesson 3.
THE SUN.
Here Comes the Sun!! Chapter 14 Section 2 Page 545 Miss Sullivan Rm B2.
Presentation transcript:

The Sun *Our closest star *Accounts for 99.8% of the solar system’s total mass *because of this, it exerts powerful gravitational force throughout the solar system *this force decreases with distance but is strong enough to hold all planets in orbit

Sun’s Interior Ball of glowing gas, (not a solid surface like Earth) ¾ Hydrogen ¼ Helium Small amounts of other elements Has an interior Has an atmosphere

Sun’s Interior Has 3 Zones: Core Radiation zone Convection zone This Photo by Unknown Author is licensed under CC BY-SA

Core Central region of sun Energy comes from nuclear fusion Hydrogen atoms join together to form helium in this process Occurs under conditions of high temperature and pressure (about 15 million degrees Celsius Energy slowly moves out from the core, eventually escaping into space

Radiation Zone Middle layer of sun’s interior Tightly packed gas Energy is transferred in form of electromagnetic radiation Very dense *because of its density, it takes 100,000 years for energy to move through it

Convection Zone Outermost layer of sun’s interior Hot gases rise from bottom of this zone Gases cool as they get to the top of this zone Loops of gas form and move toward the sun’s surface

Sun’s Atmosphere Photosphere Chromosphere Corona

Photosphere Inner layer of atmosphere Seen when you look at an image of the sun Considered to be sun’s surface layer Moon blocks the light of photosphere during solar eclipse

Chromosphere Means “color sphere” This Photo by Unknown Author is licensed under CC BY-SA Chromosphere Means “color sphere” Reddish glow that appears during a solar eclipse is cause by this layer

Corona “white halo” during a solar eclipse Means “crown” in Latin This Photo by Unknown Author is licensed under CC BY-SA-NC “white halo” during a solar eclipse Means “crown” in Latin Corona extends into space for millions of kilometers Thins into streams of electrically charged particles called solar wind

Layers of the Sun This Photo by Unknown Author is licensed under CC BY-SA-NC

Sun’s Features Sunspots Prominences Solar flares

Sunspots Dark spots on sun’s surface Sunspots are larger than Earth (but appear small) Cooler than the gases around them, so it is darker and doesn’t give off as much light Appears to move across sun’s surface Proves sun rotates on its axis just like Earth does This Photo by Unknown Author is licensed under CC BY-SA

Huge, reddish loops of gas Prominences Huge, reddish loops of gas Loops can be seen extending over the edge of the sun This Photo by Unknown Author is licensed under CC BY-SA-NC

Solar Flares Magnetic energy Gas eruptions into space This Photo by Unknown Author is licensed under CC BY-NC-ND