10.2 The Solar Interior Flashcards
(9 cards)
Solar layers in order of location (highest to lowest)
-Photosphere
-Convective zone
-Radiative zone
-Core
Solar layers in order of temperature (hottest to coldest)
-Core
-Radiative zone
-Convective Zone
-Photosphere
Solar core
Hot enough for nuclear fusion to occur: producing energy
Radiative zone
Energy travels as constantly absorbed and re-emitted photons of radiation to the convective zone
Convective zone
Transfers energy to the photosphere through convection currents of plasma
Photosphere
Radiates the energy into space as light
Proton-proton-cycle
The cycle by which the sun’s core fuses protons into helium nuclei
Proton-proton-cycle visualisation
1/1H + 1/1H -> 2/1H + positron + neutrino
2/1H + 1/1H -> 3/2He
3/2He + 3/2He -> 4/2 He + 1/1H + 1/1H
How is energy produced in the proton-proton-cycle
At each stage, when mass is lost it is converted into energy