Structure of the Radiative Zone

The radiative zone extends from the outer edge of the core to the beginning of the convective zone. It is composed of tightly packed gas and plasma, with the density and temperature decreasing as it approaches the convective zone.

Energy Transport

In the radiative zone, energy is transported through the process of radiation. Photons, the particles that make up light, are emitted and absorbed by ions and electrons in the plasma. These photons travel in a random walk, bouncing from one particle to another until they reach the outer edge of the radiative zone.

Characteristics

The radiative zone is characterized by high temperatures, but due to the lack of convection, the temperature gradient is relatively stable. This means that the temperature decreases gradually as you move away from the core towards the convective zone.

Study Guide for the Radiative Zone

What is the location of the radiative zone in a star?
How is energy primarily transported in the radiative zone?
Describe the structure of the radiative zone.
What is the primary mode of energy transport in the radiative zone?
What are the characteristics of the radiative zone?

◂Science Worksheets and Study Guides Sixth Grade. Magnetism

Vocabulary/Answer key

Magnetism

The resources above cover the following skills:

EARTH AND SPACE SCIENCE

Earth’s Systems

Develop and use models of Earth’s interior composition to illustrate the resulting magnetic field (e.g., magnetic poles) and to explain its measureable effects (e.g., protection from cosmic radiation).