Visual Dictionary
Subscribe
The Visual
Virtual Human Body
Language:
English
French
Spanish
Look up an image:
Explore by theme
About the Visual
Books
Games
HOME
>
astronomy
>
celestial bodies
>
Sun
>
structure of the Sun
structure of the Sun
From the center to the periphery are the core, the radiation and convection zones, the photosphere, the chromosphere and the corona.
See structure of the Sun in :
french
|
spanish
flare
Violent projection of extremely hot gas into space, provoking polar auroras on Earth a few days later.
faculae
Luminous region of the photosphere.
spicules
A narrow jet of gas in the form of a plume observed in the solar chromosphere.
photosphere
Visible surface of the Sun, with a temperature of 6,000°C.
corona
The outermost layer of the solar atmosphere, visible in the form of a halo during a total eclipse; corona temperatures can reach 1,000,000°C.
convection zone
Region where hot gas currents circulate between the hot regions of the core and the cool surface.
radiation zone
Region where energy produced in the core cools before migrating in the form of light and heat.
core
The innermost part of the Sun where hydrogen is converted into helium by nuclear fusion; core temperatures reach 15,000,000°C.
prominence
Gas that erupts from the chromosphere and solar corona, contrasting with the darkness of space.
granulation
Network of cells on the photosphere brought about by the convective movement of hot gas from the Sun’s interior.
sunspot
A dark, slightly cooler zone of the photosphere where the magnetic field is more intense.
chromosphere
The lowest level of the solar atmosphere, with a temperature of 10,000°C.