A solar prominence (also known as a filament when viewed against the solar disk) is a large, bright feature extending outward from the Sun's surface
In the core is where fusion of hydrogen occurs in the sun
Sunspots are cooler than the plasma around them
Atoms are combined into heavier elements through the process called Nuclear Fusion
According to Keplers first law planets orbit in a Ellipse
A planets revolution is the slowest when furthest from the sun
Hydrogen and Helium make up most of the suns mass
Hydrogen and Helium make up most of the suns mass
In the core is where fusion of hydrogen occurs in the sun
Atoms are combined into heavier elements through the process called Nuclear Fusion
The "p" in Keplers third law stands or Orbital Period
The "p" in Keplers third law stands or Orbital Period
In the convection zone plasma rises as it heats up then falls
In the convection zone plasma rises as it heats up then falls
Sunspots are cooler than the plasma around them
According to Keplers first law planets orbit in a Ellipse
A planets revolution is the slowest when furthest from the sun
A solar prominence (also known as a filament when viewed against the solar disk) is a large, bright feature extending outward from the Sun's surface
The "r" in Keplers third law stand for Radius
The "r" in Keplers third law stand for Radius
