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OUR SUN
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Solar telescope
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FUSION Need very high temperatures H + H → He + energy Energy= heat
Light EM radiation
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Compositon of the Sun 90% H & 10% He Plasma- gas stripped of electrons
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Sun Layers
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core Where Fusion is taking place 15 million ºC
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Radiative Zone EM radiation is traveling through this zone
2.5 million ºC
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CONVECTIVE ZONE Convection currents
Hot gases rise to surface, cooler gases sink= turbulance
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Photosphere Sun’s surface Bubbling plasma Only 6,000 ºC!
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chromosphere Sun’s atmosphere 20,000 C Source of flares/prominences
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chromosphere
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CORONA “Crown” See only during solar eclipses 2 million C Made of ions
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Journey from the center of the sun
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SUNSPOTS Cool spots on sun Caused by twisting of magnetic field?
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Oct. 17, 2012 Main sequence star
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How long is a sunspot cycle?
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11 year sunspot cycle Cycle number
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Solar prominences (filaments)
Follows magnetic force of sunspots Can last for weeks to a year harmless
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Solar flares Violent eruption Last for minutes Can damage satellites
Can reach Earth- ohoh!
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Coronal Mass Ejections
Produced in corona Large storms Can cause power outages, satellite damage and auroras
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Solar wind Ions are so hot, gravity can’t hold them onto the sun
400 km/sec (1 million mph) Today: speed: km/sec
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AURORAS (Northern lights) caused when Suns’ ions enter Earth’s atm.
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Auroras from space
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Solar activity SpaceWeather.com
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