https://padlet.com/1skaterchickify/qt15podbm535 en-us 2017-05-10 12:31:15 UTC 2017-05-11 12:40:45 UTC hello@padlet.com 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170991316

]]> 2017-05-10 12:45:22 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170991316 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170991571

]]> 2017-05-10 12:46:31 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170991571 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170992773 The solar core is made up of a really hot and dense gas in a plasma state. The core is where the energy of the Sun is made, where nuclear fusion reactions take place.

]]> 2017-05-10 12:51:15 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170992773 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170993867 In the radiative zone energy from the core is moved outward as electromagnetic radiation.

]]> 2017-05-10 12:55:25 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170993867 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170993971 In this zone turbulent convective motions occur. The overturning motions inside the Sun are responsible for the granulation pattern seen on the Sun's surface.

]]> 2017-05-10 12:55:49 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170993971 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994006 This is known as the surface of the sun, the part we can see directly.  

]]> 2017-05-10 12:55:58 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994006 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994052 This layer is above the Photosphere  and is about 2500 kilometers thick. It appears as a thin reddish ring. 

]]> 2017-05-10 12:56:07 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994052 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994073 The outermost layer, temperature can reach to the tens of thousands of kelvins to a few million. It also cannot be sen with the naked eye except during a solar eclipse.

]]> 2017-05-10 12:56:11 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994073 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994100 Sunspots are dark, planet-sized regions that appear on the surface of the Sun. they are dark because they are colder than the areas around them.

]]> 2017-05-10 12:56:17 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994100 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994152 A solar prominence is a filament when viewed against the solar disk, it is a large bright feature extending outward from the Sun's surface 

]]> 2017-05-10 12:56:28 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994152 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994171 Solar flares are essentially huge explosions on the Sun. Flares occur when intense magnetic fields on the Sun become too tangled. 

]]> 2017-05-10 12:56:31 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994171 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/170994203 The aurora is formed when protons and electrons from the sun travel along the Earth's magnetic field lines. It  comes in a variety of colors 

]]> 2017-05-10 12:56:37 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/170994203 1skaterchickify https://padlet.com/1skaterchickify/qt15podbm535/wish/171000511 http://www.thesuntoday.org/solar-facts/powering-the-sun/
https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html
https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html

]]> 2017-05-10 13:19:43 UTC https://padlet.com/1skaterchickify/qt15podbm535/wish/171000511