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Sun Composition
73% Hydrogen, 25% helium, 2% other
Sun Structure
Chromosphere, Photosphere and Corona
Chromosphere
The outermost layer of the sun, usually able to be seen during total solar eclipses
Photosphere
sun becomes opaque and marks the area of the sun we can’t see past
Corona
The middle core of the sun, the hottest part
Nuclear Fusion
two nuclei form a bigger nucleus
Proton-Proton Chain
nuclei of hydrogen are built up into nuclei of helium
Radiation
emission of energy as an electromagnetic waves or photons
Convection
movement caused within a gas or liquid by the tendency of hotter and less dense materials
Conduction
heat is transmitted through a substance when there are different temps from a collision.
Accretion Disk
a rotating disk of gas, dust or plasma that slowly loses momentum
Stellar Association
lose unbounding group of young stars
Black Hole
Star - Collapses in on its own weight - compacts so once inside you can’t escape nothing gets out
Chandrasekhar limit
Maximum mass of a stable white dwarf
Clump
clump of stars
Coronal Mass Ejection
Large expulsions of plasma and magnetic fields from the suns corona