QUESTION IMAGE
Question
practice 5
describe the flow of energy from the core
of the sun to its surface. type your
answer in the box.
photosphere
convection
zone
radiation
zone
core
sunspots
Brief Explanations
- Core: Energy is first generated in the Sun's core via nuclear fusion, where hydrogen fuses into helium, releasing high-energy photons (gamma rays and X-rays).
- Radiation Zone: Energy travels outward through this dense zone via radiative transfer. Photons repeatedly absorb and re-emit energy, slowly moving toward the convection zone; this process can take hundreds of thousands of years.
- Convection Zone: In this outer layer, energy moves via convection. Hot, energy-rich plasma rises to the surface, cools, and sinks back down to absorb more energy, creating circular convection currents.
- Photosphere: The rising plasma releases its energy as visible light and other radiation from this layer, which is the Sun's visible surface that we observe.
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- Energy is produced in the Sun's core through nuclear fusion of hydrogen into helium, generating high-energy photons.
- These photons move outward through the radiation zone via radiative transfer, bouncing between particles over thousands of years.
- In the convection zone, energy is carried upward by hot, rising plasma currents; the plasma cools near the surface and sinks back down to repeat the cycle.
- Finally, energy is released as visible light and other radiation from the photosphere, the Sun's visible surface.