https://padlet.com/maddie_foushee/M16_A3 Maddie Foushee en-us 2017-08-03 18:12:16 UTC 2017-08-04 20:45:10 UTC hello@padlet.com https://padlet-assets.s3.amazonaws.com/icons/Brightnessdown.png maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180121514 2017-08-04 12:18:31 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180121514 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180121561 https://pbs.twimg.com/profile_images/641353910561566720/VSxsyxs7.jpg
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Module 16 Notes]]> 2017-08-04 12:19:38 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180121561 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180121593 2017-08-04 12:20:21 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180121593 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180122023 Core
Radiative Zone
Convective Zone
Photosphere
Chromosphere
Corona]]> 2017-08-04 12:28:22 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180122023 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180122197 Sunspots are dark spots that appear on the sun's surface. They occur because they are cooler than the surrounding areas]]> 2017-08-04 12:32:08 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180122197 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180147089 Solar Prominences are huge arches of glowing gas that extend outward from the surface of the sun]]> 2017-08-04 19:09:20 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180147089 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180147270 Flares often occur near sunspots, and they're actually explosions on the sun's surface. ]]> 2017-08-04 19:12:31 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180147270 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180147390 Auroras on Earth, like the Northern Lights, are caused by solar flares and Coronal Mass Ejections (CMEs). CMEs are massive bursts of solar wind and magnetic energy that are released into space.]]> 2017-08-04 19:15:02 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180147390 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180147623 The sun's core is, obviously, at the center of the sun. Scientists have found that it has a temperature of around 29 million degrees Fahrenheit, and that it rotates about 4 times faster than the surface.]]> 2017-08-04 19:20:09 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180147623 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180148689 The Radiative Zone is between the Core and the Convective Zone. The tachocline separates the inner and outer parts of the sun.]]> 2017-08-04 19:51:06 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180148689 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180148695 Just outside the Radiative Zone, the Convective Zone carries energy in the same way a pot of boiling water does. The bubbling motions are responsible for the granulation pattern on the surface.]]> 2017-08-04 19:51:13 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180148695 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180148702 The Photosphere is what is considered to be the surface of the sun, and it has temperatures of around 10,000 degrees Fahrenheit, or 5,800 Kelvin]]> 2017-08-04 19:51:18 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180148702 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180148706 This is the layer above the photosphere, and it appears as a reddish glow around the sun. It is nearly transparent.]]> 2017-08-04 19:51:27 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180148706 maddie_foushee https://padlet.com/maddie_foushee/M16_A3/wish/180148708 The Corona, meaning "crown", is the outermost layer of gases surrounding the sun. It's only seen during a solar eclipse; it's not normally visible because of the brightness of the photosphere.]]> 2017-08-04 19:51:30 UTC https://padlet.com/maddie_foushee/M16_A3/wish/180148708