Question

read with a purpose

1. where does the energy travel and in what form?
2. where does this radiation enter and what does the energy do in this region?
3. what happens to the gases as they rise to the top of the convection cell?
4. where is the energy transferred and in what form?

final read: study how energy is transferred between the suns radiative and convection zones (your answers to questions 1 - 5 and figure 3) develop a diagram to model the process.

Explanation:

1. Energy travels from the Sun's core outward. In the radiative zone, it travels as electromagnetic radiation (photons). In the convection zone, it travels as heat - carrying gas motions (convection currents).
2. Radiation enters the radiative zone from the core. In this region, photons are absorbed and re - emitted by atoms, slowly transporting energy outward.
3. As gases rise to the top of the convection cell, they cool down. As they cool, their density increases and they begin to sink back down, creating a convective cycle.
4. Energy is transferred from the radiative zone to the convection zone. In the radiative zone, it is in the form of electromagnetic radiation (photons), and in the convection zone, it is in the form of heat transfer via convection currents. For the final task, a diagram could show the Sun's core, radiative zone with arrows representing photon movement, and the convection zone with circular arrows representing the rising and sinking of gas.

Answer:

1. In the radiative zone as photons, in the convection zone as convection currents.
2. Enters the radiative zone from the core; photons are absorbed and re - emitted to transport energy.
3. Cool down, increase in density and start to sink.
4. From radiative to convection zone; as photons in radiative zone, as convection currents in convection zone. For the diagram: include core, radiative zone with photon arrows, convection zone with convective cycle arrows.