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Star brightness and star distance: Difference between revisions

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* how we use black body radiation to calculate the temperature of distant stars
* how we use black body radiation to calculate the temperature of distant stars
|age=Secondary
|age=Secondary
|content=In the 17th century, Christian Huygens discovered how to estimate how far away a star is. He made a series of smaller holes in a screen facing the sun, until he estimated the light was the same intensity as the star Sirius. Huygens' results were surprisingly accurate, but still wrong. This series of slides may inspire you to tell the remarkable story of how we measure stars. The teacher explains his approach in an audio file and provides a web link to an interactive tool used in the presentation. The presentation has been converted to an alternative format.
|content=In the 17th century, Christian Huygens discovered how to estimate how far away a star is. He made a series of smaller holes in a screen facing the sun, until he estimated the light was the same intensity as the star Sirius. Huygens' results were surprisingly accurate, but still wrong. This lesson follows work where students learn how parallax can be used to calculate the distance of stars, though not all. Students often believe that the earlier scientists made foolish assumptions. This series of slides may inspire you to tell the remarkable story of how we measure stars. It may help you help students to
understand the amazing stretches of imagination needed to come up with those early hypotheses.
The teacher explains his slides in an audio file. He also provides a link to an black body radiation tool.  
|format=
|format=
|strategy= See the teacher's note on 'active-note taking'
|strategy=
|additional resources=
|additional resources=
|useful information=
|useful information=
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|other=
|other=
|resources=
|resources=
* Teacher's audio explanation of how the lesson was delivered [[media:CT - Star brightness voiceover.MP3]]
The presentation has been converted to alternative formats:
* Smartboard notebook version [[File:10 - Star Brightness, Size and Distance.notebook]]
* Smartboard notebook version [[File:10 - Star Brightness, Size and Distance.notebook]]
* Powerpoint version:[[File:10 - Star Brightness, Size and Distance.pptx]]
* Powerpoint version:[[File:10 - Star Brightness, Size and Distance.pptx]]
* PDF version [File:Star brightness & distance.pdf]]
* PDF version [File:Star brightness & distance.pdf]]
* Teacher's audio explanation of how the lesson was delivered [[media:CT - Star brightness voiceover.MP3]]
* Link to Blackbody Radiation Applet http://www.mhhe.com/physsci/astronomy/applets/Blackbody/frame.html
* Link to Blackbody Radiation Applet http://www.mhhe.com/physsci/astronomy/applets/Blackbody/frame.html
}}
}}
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