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The Sun
Vocabulary of The Sun
Term | Definition |
---|---|
Nuclear Fusion | The process by witch nuclei of small atoms combine to form a new, more massive nucleus; the process releases energy. |
Sunspots | A dark area of the photoshere of the sun that is cooler than the surrounding areas and that has a strong magnetic field. |
Solar Flares | An explosive release of energy that comes from the sun and that is associated with magnetic disturbance on the suns surface. |
Prominence | A loop of relatively cool, incandescent gas that extends above the photophere and above the suns's edge as seen from Earth. |
Corona | The rarefied gaseous envelope of the sun and other stars. The sun's corona is normally visible only during a total solar eclipse when it is seen as an irregularly shaped pearly glow surrounding the darkened disk of the moon. |
Chromosphere | a reddish gaseous layer immediately above the photosphere of the sun or another star. Together with the corona, it constitutes the star's outer atmosphere. |
Photosphere | The luminous envelope of a star from which its light and heat radiate. |
Convection Zone | Of a star is the range of radii in which energy is transported primarily by convection. In the radiation zone, energy is transported by radiation. |
Radiative Zone | A layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion, rather than by convection. |
Core | The central part of earth below the mantle |
Radiation | The transfer of energy as electromacnetic waves |
Convection | The movement of matter due to differences in densities that are cause by temperature variations; can result in the transfer of energy as heat. |