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Today is Wednesday, June 5 th , 2013

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Today is Wednesday, June 5 th , 2013. Homework: Complete rockets (launch is THIS FRIDAY!!!!) Understand how Newton’s Third Law of Motion makes YOUR particular rocket work! Warm UP: - PowerPoint PPT Presentation
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Today is Wednesday, June 5 th , 2013 Homework: - Complete rockets (launch is THIS FRIDAY!!!!) - Understand how Newton’s Third Law of Motion makes YOUR particular rocket work! Warm UP: With your shoulder partner, discuss what you know about the center of our solar system? Is the sun the only star in the sky? Do you know the names of any other stars in the sky?
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Page 1: Today is Wednesday, June 5 th , 2013

Today is Wednesday, June 5th, 2013

Homework:- Complete rockets (launch is THIS FRIDAY!!!!)- Understand how Newton’s Third Law of Motion

makes YOUR particular rocket work!Warm UP:With your shoulder partner, discuss what you know

about the center of our solar system? Is the sun the only star in the sky? Do you know the names of any other stars in the sky?

Page 2: Today is Wednesday, June 5 th , 2013

Goal for Today

• SWBAT demonstrate an understanding of the characteristic of stars by exploring the sun as an example and looking at examples of other stars.

Page 3: Today is Wednesday, June 5 th , 2013

Only write down the BLUE text…

Date: Wednesday, June 5th, 2013Title: Stars

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StarA gigantic ball of very hot gases (hydrogen

and helium) reacting by the process of nuclear fusion that give off electromagnetic

radiation.

Page 5: Today is Wednesday, June 5 th , 2013

Relative Size of Planets and the Sun

Putting Earth in Perspective

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Rocky (Terrestrial) Planets (and Pluto) in our Solar System

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Terrestrial planets (and Pluto) with gas giants (rings not shown)

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All planets in the Solar System, plus Pluto,and the Sun

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The Sun in relation to large orange giant stars and Sirius (White Dwarf)

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The Sun in relation to Red Supergiant stars Betelgeuse and Antares

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Types of Stars

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Factors that affect the brightness of a star as seen from Earth:

• Size• Distance from Earth• Temperature

– Red is the coolest (but generally the largest in volume)

– Orange and yellow are slightly hotter– White or blue-white stars are the hottest

Page 13: Today is Wednesday, June 5 th , 2013

The SunA medium-heat (a little on the cooler side) Yellow Star at the

center of our Solar System

Page 14: Today is Wednesday, June 5 th , 2013

Layers of the Sun’s AtmospherePhotosphere – 6,000 K

Chromosphere – 10,000 K

Chromosphere/Corona Transition Region – 30,000 to 500,000 K

Prominence – 10,000 K

Corona – 1,500,000 K

Page 15: Today is Wednesday, June 5 th , 2013

Artist’s Depiction

Page 16: Today is Wednesday, June 5 th , 2013

The Sun’s corona can be seen very well during a Solar Eclipse(NEVER LOOK DIRECTLY AT THE SUN, EVEN DURING AN ECLIPSE,

WITHOUT PROPER PROTECTION!!!)

Page 17: Today is Wednesday, June 5 th , 2013

Sun Spots

Darker spots on the photosphere that are cooler than areas around it

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Sun Spots!

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Prominences

Loops and fountains of blazing gases that leap out of the chromosphere

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Solar Flares

Parts of the chromosphere that erupt like a volcano

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Solar Flares interacting with Earth’s magnetic field

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The effects of solar flares interactingwith Earth’s magnetic field (auroras) as seen from Earth’s surface and near-Earth orbit

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Largest flare every recordedNovember 4, 2003

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Closing it up…

• What kind of activity on the surface of the Sun can disrupt Earth’s magnetic field– Solar Flares

• What type of star is our Sun?– Yellow Star

• What are the hottest stars in the sky?– Blue and white stars


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