Blackbody Spectrum
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Topics
- Blackbody
- Planck's Law
- Wien's Law
- Electromagnetic Radiation
- Quantum Mechanics
- Astronomy
Description
How does the blackbody spectrum of the sun compare to visible light? Learn about the blackbody spectrum of Sirius A, the sun, a light bulb, and the earth. Adjust the temperature to see the wavelength and intensity of the spectrum change. View the color of the peak of the spectral curve.
Sample Learning Goals
- Describe what happens to the blackbody spectrum as you increase or decrease the temperature. What happens to the shape of the curve and the peak of this curve?
- Describe the blackbody spectrum of a light bulb. Why do light bulbs get hot? Do they seem efficient?
- Imagine that you see 2 hot, glowing objects--one is glowing orange and the other is glowing blue. Which one is hotter?
- Find the relationship between the temperature and the wavelength at the peak of the curve.
Version 2.02
Keywords
Teacher Tips
Overview of sim controls, model simplifications, and insights into student thinking ( PDF ). |
Teacher-Submitted Activities
Title | Authors | Level | Type | Subject | ||
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Visualization and Visual Illusions SIM Homework | Kathy Perkins, Carl Wieman | UG-Intro | HW | Physics | ||
Blackbody Radiation and Wien's Law | Michael Pennisi | HS | Lab | Physics | ||
PhET Sims Aligned to the Chemistry Curriculum | Julia Chamberlain | HS UG-Intro |
Other | Chemistry | ||
Alignment of PhET sims with NGSS | Trish Loeblein | HS | Other | Earth Science Biology Physics Chemistry |
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How do PhET simulations fit in my middle school program? | Sarah Borenstein | MS | Other | Biology Earth Science Physics Chemistry |
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Blackbody Spectrum & Lasers Simulations Homework | Kathy Perkins, Carl Wieman | HS UG-Intro |
HW | Physics | ||
Blackbody Spectrum Simulation Homework | Kathy Perkins, Carl Wieman | UG-Adv UG-Intro |
HW | Physics | ||
Mapping of PhET and IBDP Physics | Jaya Ramchandani | HS | Other | Physics | ||
MS and HS TEK to Sim Alignment | Elyse Zimmer | MS HS |
Other | Physics Chemistry Biology |
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Temperature and Radiation Activity | Dorian McIntire | UG-Intro HS |
HW Lab |
Astronomy Physics Other |
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Temperature and Luminosity of Stars: Wein's Law and the Stephan Boltzmann Law | Rhoda Berenson | UG-Intro | Lab | Astronomy | ||
Blackbody Radiation updated from Michael P. | michael marty | HS | Demo Lab |
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Black Body Radiation: Seeking Patterns in Data Sets | Roberto Marrero | HS | Lab | Chemistry | ||
Solar Astronomy | Mark Kelly | HS | HW Lab |
Astronomy | ||
Blackbody Spectrum | Curt Miller | HS | Lab | Physics | ||
흑체 스펙트럼 SIM 사용지침서 | 이화국(Wha Kuk Lee) | HS MS |
Demo Lab |
Chemistry Earth Science Physics Astronomy |
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Ley de Wien y de Stephan-Boltzmann | José Saldaña | HS UG-Intro |
Lab | Astronomy Physics |
Windows | Macintosh | Linux |
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Microsoft Windows XP/Vista/7/8.1/10 Macromedia Flash 9 or later
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OS X 10.9.5 or later Macromedia Flash 9 or later
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Macromedia Flash 9 or later
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Design Team | Third-party Libraries | Thanks To |
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