Lesson 3.3: The Sun

Lesson 3: What is the structure of the sun? What features can you see on the sun?

What Is the Structure of the Sun? No solid surface ¾ of sun’s mass is hydrogen ¼ of sun’s mass is helium Has an interior and an atmosphere Interior is made up of the: Core Radiation zone Convection zone

The Sun’s Interior: The Core Core: central region of the sun An enormous amount of energy is produced here through nuclear fusion Nuclear fusion: when hydrogen atoms join to form helium

The Sun’s Interior: The Radiation Zone Energy produced in the sun’s core moves outward through the radiation zone Radiation zone: a region of very tightly packed gas where energy moves mainly in the form of electromagnetic radiation Is extremely dense; energy can take more than 100,000 years to move through this zone

The Sun’s Interior: The Convection Zone Convection zone: the outermost layer of the sun’s interior Hot gases rise from the bottom of the convection zone and cool as they approach the top Cooler gases sink, forming loops of gas that move energy toward the sun’s surface (convection currents)

The Sun’s Atmosphere Stretches far into space Layers become less dense the farther they are from the radiation zone Mostly composed of hydrogen and helium Includes the: Photosphere Chromosphere Corona

The Sun’s Atmosphere: The Photosphere Photosphere: the inner layer of the sun’s atmosphere Considered to be the surface layer of the sun Sun does not have a solid surface, although the gases of the photosphere are thick enough to be visible When you look at an image of the sun, you see the photosphere

The Sun’s Atmosphere: The Chromosphere Chromosphere: the middle layer of the sun’s atmosphere; means “color sphere” The reddish glow visible around the photosphere at the start and end of a total eclipse

The Sun’s Atmosphere: The Corona Corona: the outer layer that looks like a white halo around the sun; means “crown” Extends into space for millions of kilometers Gradually thins into streams of electrically charged particles called the solar wind

What Features Can You See on the Sun? Using special telescopes to study the sun, scientists have spotted features like: Sunspots Prominences Solar flares

Sunspots Sunspots: dark areas on the sun’s surface; caused by areas of gas on the sun’s surface that are cooler than the gases around them Often look small, but they can be larger than Earth Number of sunspots varies in a regular cycle, with the most sunspots appearing about once every 11 years Sunspots

Prominences Prominences: huge loops of gas; often link different parts of sunspot regions Prominences

Solar Flares Solar flares: eruptions that occur when the loops in sunspot regions suddenly connect, releasing large amounts of magnetic energy The energy heats gas on the sun to millions of degrees Celsius, causing the gas to erupt into solar flares

Solar Wind Made up of electrical particles from the sun Solar flares can increase the solar wind, meaning that more particles reach earth’s upper atmosphere Earth’s atmosphere usually blocks these particles, except near the North and South poles There, they create powerful electric currents that cause gas molecules in the atmosphere to glow, creating the auroras They can also cause magnetic storms