The Sun.

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Presentation transcript:

The Sun

Composition of the Sun: 75% Hydrogen 24% Helium 1% Trace Elements

Nuclear Fusion: The process by which nuclei of small atoms combine to form a new more massive nucleus; the process releases a lot of energy

Nuclear Fusion: Fusion powers the sun by combining hydrogen atoms in order to form Helium, the remaining mass is converted to energy, E = mc2 Energy = mass x (speed of light)2

The Sun’s Interior: Three layers: Core, Radiative Zone, Convective zone Fusion occurs in the core Core is ionized gas (plasma)

The Sun’s Atmosphere: Three layers: Photosphere, Chromosphere, and the Corona Photosphere is called the Sun’s “surface” because it is what you see Corona – the outermost layer of the sun’s atmosphere

sunspot the dark area of the photosphere of the sun that is cooler than the surrounding areas and has a strong magnetic field

Sunspot cycle: Observing sunspots showed that the sun rotates (about 27 days) The increase and decrease of sunspots follows an 11 year cycle

Solar Flare: An explosive release of energy (electrically charged particles such as protons and electrons) that comes from the sun, and that is associated with magnetic disturbances on the sun’s surface (sunspots)

Coronal mass ejections: A part of coronal gas that is thrown into space from the sun, causes disturbances with Earth’s radio communications

Auroras: Colored light produced by charged particles from the solar wind and the Earth’s atmosphere that react and excite the oxygen and nitrogen in the Earth’s upper atmosphere