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- Author:
-
David Stern, Ph.D.
- Subject:
- Science and Technology
- Institution Name:
- NASA
- Collection:
-
NASA
- Grade Level:
- Secondary
- Abstract:
As part of this lesson plan, students will learn about how energy is produced and dissipated by stars, including our own Sun. In addition, materials presented here explain the formation, evolution,and eventual "death" of stars in supernova explosions, and some fundamentals of nuclear physics. Definitions of terms and questions for the class are included.
- Course Type:
- Learning Module
- Languages:
- English
- Material Type:
- Lesson Plans
- Media Format:
- Graphics/Photos, Text/HTML
- Conditions of Use:
-
Public Domain
NASA still images; audio files; video; and computer files used in the rendition of 3-dimensional models, such as texture maps and polygon data in any format, generally are not copyrighted. You may use NASA imagery, video, audio, and data files used for the rendition of 3-dimensional models for educational or informational purposes, including photo collections, textbooks, public exhibits, computer graphical simulations, and Internet Web pages. This general permission extends to personal Web pages.
No restrictions on your remixing, redistributing, or making derivative works.
Give credit to the author, as required.
Your remixing, redistributing, or making derivatives works comes with some
restrictions, including how it is shared.
Your redistributing comes with some restrictions. Do not remix or make
derivative works.
Copyrighted materials, available under Fair Use and the TEACH Act for US-based
educators, or other custom arrangements. Go to the resource provider to see
their individual restrictions.
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