Complete the 3 question Bell Ringer independently at your seat You will have 4 Minutes to complete this assignment Please begin immediately Independent.

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What is the fate of our sun and other stars?
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Presentation transcript:

Complete the 3 question Bell Ringer independently at your seat You will have 4 Minutes to complete this assignment Please begin immediately Independent work- No talking

Bell Ringer Question 1: B: Core Question 2: C: Corona Question 3: 1: Core 2: Radiation Zone 3: Convection Zone 4: Photosphere 5: Chromosphere 6: Corona

Sunspots Solar Flares Prominences

Features of the Sun They are all at the surface of the Sun The Photosphere Sunspot:Solar Flare: Prominence:

Sunspots They are found on the Photosphere Due to the difference in temperature Caused by convection currents Usually go in an 11 year activity cycle Appear dark because of the temperature difference A cooler than the rest of the surface

Solar Flare They exit out of the Photosphere Release of radiation from the Sun’s surface Explodes directly outward from the Sun Causes Solar wind A Burst of radiation that is invisible and travels outward from the Sun Happens due to a weak area in the Sun’s magnetic field on the surface that “break” for an instance and allows radiation to come through

Prominence They are found on the Photosphere Loops of gas that exit the Sun and are pulled back into the Sun Huge! The largest record prominence was over 500,000 miles high Prominence= LOOP! Solar Flare= Straight

Features of the Sun Sunspot:Solar Flare: Prominence:

Pictures: Layers of the Sun: Solarcellcentral.com Sunspots: Commons.wikimedia.org Space.com Sciedu.ucar.edu Solar Flare: Bobthealien.co.uk En.wikipedia.org Prominence: Soundofheart.org Spaceweather.sflorg.com