Introduction

Chapter 1. Astronomy Imagemap Shockwave Substitutes

Introduction

My Slide Activities
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You must read each slide, and complete any questions on the slide, in sequence.

Shockwave Alternatives for Astronomy Activities

Each slide shows a different activity.

1.1 A Theoretical Model of the Sun

Question 1 of 4

A Theoretical Model of the Sun

Click on the graph that plots distance from the center of the sun against solar density (kg/m3).
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{"title":"Luminosity","description":"","type":"incorrect","color":"#99CCFF","code":"[{\"shape\":\"rect\",\"coords\":\"2,24,286,113\"}]"} {"title":"Mass","description":"","type":"incorrect","color":"#993300","code":"[{\"shape\":\"rect\",\"coords\":\"1,116,285,207\"}]"} {"title":"Temperature","description":"","type":"incorrect","color":"#333300","code":"[{\"shape\":\"rect\",\"coords\":\"2,209,286,300\"}]"} {"title":"Density","description":"","type":"correct","color":"#000080","code":"[{\"shape\":\"rect\",\"coords\":\"2,303,286,383\"}]"}

Click on the graph that plots distance from the center of the sun against solar luminosity (%).
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{"title":"Luminosity","description":"","type":"correct","color":"#99CCFF","code":"[{\"shape\":\"rect\",\"coords\":\"2,24,286,113\"}]"} {"title":"Mass","description":"","type":"incorrect","color":"#993300","code":"[{\"shape\":\"rect\",\"coords\":\"1,116,285,207\"}]"} {"title":"Temperature","description":"","type":"incorrect","color":"#333300","code":"[{\"shape\":\"rect\",\"coords\":\"2,209,286,300\"}]"} {"title":"Density","description":"","type":"incorrect","color":"#000080","code":"[{\"shape\":\"rect\",\"coords\":\"2,303,286,383\"}]"}

Click on the graph that plots distance from the center of the sun against solar mass (%).
Feedback
{"title":"Luminosity","description":"","type":"incorrect","color":"#99CCFF","code":"[{\"shape\":\"rect\",\"coords\":\"2,24,286,113\"}]"} {"title":"Mass","description":"","type":"correct","color":"#993300","code":"[{\"shape\":\"rect\",\"coords\":\"1,116,285,207\"}]"} {"title":"Temperature","description":"","type":"incorrect","color":"#333300","code":"[{\"shape\":\"rect\",\"coords\":\"2,209,286,300\"}]"} {"title":"Density","description":"","type":"incorrect","color":"#000080","code":"[{\"shape\":\"rect\",\"coords\":\"2,303,286,383\"}]"}

Click on the graph that plots distance from the center of the sun against solar temperature (K).
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{"title":"Luminosity","description":"","type":"incorrect","color":"#99CCFF","code":"[{\"shape\":\"rect\",\"coords\":\"2,24,286,113\"}]"} {"title":"Mass","description":"","type":"incorrect","color":"#993300","code":"[{\"shape\":\"rect\",\"coords\":\"1,116,285,207\"}]"} {"title":"Temperature","description":"","type":"correct","color":"#333300","code":"[{\"shape\":\"rect\",\"coords\":\"2,209,286,300\"}]"} {"title":"Density","description":"","type":"incorrect","color":"#000080","code":"[{\"shape\":\"rect\",\"coords\":\"2,303,286,383\"}]"}

1.2 The Sun's Internal Structure

Question 1 of 3

The Sun's Internal Structure

Click on the portion of the figure that shows the sun's convective zone.
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{"title":"convective zone","description":"","type":"correct","color":"#99CCFF","code":"[{\"shape\":\"circle\",\"coords\":\"320,273,16\"},{\"shape\":\"poly\",\"coords\":\"254,193,225,206,172,214,128,208,99,200,97,175,112,142,130,104,149,73,164,60,201,82,226,111,244,136,258,173,257,192,294,204,285,156,261,103,230,67,196,39,164,30,130,65,100,114,88,157,75,223,138,233,186,235,240,227,291,206\"}]"} {"title":"radiative zone","description":"","type":"incorrect","color":"#ff0000","code":"[{\"shape\":\"circle\",\"coords\":\"329,86,16\"},{\"shape\":\"poly\",\"coords\":\"162,62,132,99,105,155,100,198,149,210,184,212,227,206,260,195,249,148,224,110,187,75,164,63,166,131,194,150,202,179,178,189,151,190,137,186,146,152,164,129\"}]"} {"title":"thermonuclear energy core","description":"","type":"incorrect","color":"#99cc00","code":"[{\"shape\":\"circle\",\"coords\":\"288,29,15\"},{\"shape\":\"poly\",\"coords\":\"138,185,148,147,169,124,191,149,201,178,184,186,155,190\"}]"}

Click on the portion of the figure that shows the sun's radiative zone.
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{"title":"convective zone","description":"","type":"incorrect","color":"#99CCFF","code":"[{\"shape\":\"circle\",\"coords\":\"320,273,16\"},{\"shape\":\"poly\",\"coords\":\"254,193,225,206,172,214,128,208,99,200,97,175,112,142,130,104,149,73,164,60,201,82,226,111,244,136,258,173,257,192,294,204,285,156,261,103,230,67,196,39,164,30,130,65,100,114,88,157,75,223,138,233,186,235,240,227,291,206\"}]"} {"title":"radiative zone","description":"","type":"correct","color":"#ff0000","code":"[{\"shape\":\"circle\",\"coords\":\"329,86,16\"},{\"shape\":\"poly\",\"coords\":\"162,62,132,99,105,155,100,198,149,210,184,212,227,206,260,195,249,148,224,110,187,75,164,63,166,131,194,150,202,179,178,189,151,190,137,186,146,152,164,129\"}]"} {"title":"thermonuclear energy core","description":"","type":"incorrect","color":"#99cc00","code":"[{\"shape\":\"circle\",\"coords\":\"288,29,15\"},{\"shape\":\"poly\",\"coords\":\"138,185,148,147,169,124,191,149,201,178,184,186,155,190\"}]"}

Click on the portion of the figure that shows the sun's thermonuclear energy core.
Feedback
{"title":"convective zone","description":"","type":"incorrect","color":"#99CCFF","code":"[{\"shape\":\"circle\",\"coords\":\"320,273,16\"},{\"shape\":\"poly\",\"coords\":\"254,193,225,206,172,214,128,208,99,200,97,175,112,142,130,104,149,73,164,60,201,82,226,111,244,136,258,173,257,192,294,204,285,156,261,103,230,67,196,39,164,30,130,65,100,114,88,157,75,223,138,233,186,235,240,227,291,206\"}]"} {"title":"radiative zone","description":"","type":"incorrect","color":"#ff0000","code":"[{\"shape\":\"circle\",\"coords\":\"329,86,16\"},{\"shape\":\"poly\",\"coords\":\"162,62,132,99,105,155,100,198,149,210,184,212,227,206,260,195,249,148,224,110,187,75,164,63,166,131,194,150,202,179,178,189,151,190,137,186,146,152,164,129\"}]"} {"title":"thermonuclear energy core","description":"","type":"correct","color":"#99cc00","code":"[{\"shape\":\"circle\",\"coords\":\"288,29,15\"},{\"shape\":\"poly\",\"coords\":\"138,185,148,147,169,124,191,149,201,178,184,186,155,190\"}]"}

1.3 Activity Completed!

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