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Stars - Coggle Diagram
Stars
Stellar Temperature
Blue = Hot
Red = Cool
Thermal Radiation
Hotter = Brighter
MKGFABO
The Sun
Nuclear Fusion
Gravitational Equilibrium
Small nuclei stick together to grow
Nuclear Fission
Nucleus Splits
Sun's Structure
Photosphere
Convection Zone
Chromosphere
Radiation Zone
Corona
Core
Solar Wind
Solar Neutrinos
Luminosity
Apparent Magnitude
Absolute Magnitude
Hertzsprung-Russell Diagram
Giants and Supergiants
White Dwarf
Main Sequence
Types of Binary Star Systems
Eclipsing Binary
Spectroscopic Binary
Doppler Shift
Visual Binary
How Do Stars Form?
Begins with a turbulent cloud
Random motions cause some parts to be denser than others
The large cloud fragments
What Can Slow the Contraction of a Star-Forming Cloud?
Trapping of Thermal NRG
Growth of a Protostar
Collapse of a Spinning Cloud