Quick Answer: The Sun Structure Model is a non-working classroom model showing the layers of the Sun, from the core through the radiative and convective zones to the photosphere, chromosphere and corona.
Last updated: October 2026
Key Features
Shows the core, radiative zone, convective zone, photosphere, chromosphere and corona
Helps explain solar energy production, heat transfer and visible sunlight
Supports identification and labelling of each layer
Non-working visual model for supervised classroom use
Technical Specifications
Specification
Value
Model type
Layered solar structure demonstration model
Layers shown
Core, radiative zone, convective zone, photosphere, chromosphere and corona
Learning topics
Solar energy, solar activity and solar layers
About This Product
Teachers identify the core as the energy-producing region, point to the radiative and convective zones as heat-transfer regions, show the photosphere as the visible surface and explain the chromosphere and corona as outer atmospheric layers. Students then label each layer, linking textbook diagrams with a physical model in astronomy, geography and physics lessons. The Sun Structure Model is available for supply within India and for export to Samoa, Fiji, New Zealand, Libya and Armenia.
Frequently Asked Questions
Q1. Which layer is the visible surface of the Sun? The photosphere is shown as the visible surface. The chromosphere and corona above it are presented as outer atmospheric layers.
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