https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6 Made with a wish on a star en-us 2018-08-06 15:52:35 UTC 2018-08-06 16:52:02 UTC hello@padlet.com https://padlet-assets.s3.amazonaws.com/icons/Brightnessdown.png s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093157

https://cdn.images.express.co.uk/img/dynamic/151/590x/worldwide-617284.jpg]]> 2018-08-06 16:02:11 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093157 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093169

https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/images/678410main_layerzoo_full.jpg]]> 2018-08-06 16:02:20 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093169 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093180 This is the innermost layer of the sun and what the sun draws its energy from. Inside, temperatures are extremely hot and everything is packed together. This allows for nuclear reactions to happen in and on the sun. 

http://www.passmyexams.co.uk/GCSE/physics/images/sun-02.jpg]]> 2018-08-06 16:02:26 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093180 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093704 This is the layer between the core and the convective zone. Here, energy made by nuclear fusion moves outward in the form of electromagnetic radiation. This zone occupies about 70% of the space of the sun. This zone is smaller and also is has a cooler temperature in comparison to the sun. 

http://www.passmyexams.co.uk/GCSE/physics/images/sun-03.jpg]]> 2018-08-06 16:07:18 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272093704 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094074 This layer is just below the Earth's surface and is considered the interior of the sun. The sun's temperature is very unstable because it is moving so quickly and unstable. This allows energy to diffuse outwards from the sun by convective fluid. When the fluid rises it cools and expands. 

http://www.passmyexams.co.uk/GCSE/physics/images/sun-04.jpg]]> 2018-08-06 16:11:27 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094074 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094350 This layer is the most visible to us on Earth. It is a very thin layer that is 1/7,000 of the total of Earth's radius. On this layer, the temperature also drops, and it would be very hard to see on this layer.

https://www.astronomynotes.com/starsun/sunsurf.jpg]]> 2018-08-06 16:14:37 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094350 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094619 This layer is 2,000 - 3,000 km thick and can only be seen during a good total solar eclipse. It also glows a slight red color.

https://www.astronomynotes.com/starsun/chromosphere.jpg]]> 2018-08-06 16:17:10 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094619 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094745 This layer is the outer atmosphere of the sun. Here, temperature reaches millions of degrees. The pressure and density of this layer is much lower than that of Earth's atmosphere. You can only see this during a total solar eclipse or with a corona graph. 

https://www.astronomynotes.com/nakedeye/TSE73.jpeg]]> 2018-08-06 16:18:34 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094745 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094979 Theses are created when the sun's magnetic field gets twisted all around the inside of the sun. The magnetic field rises up and then pokes through, creating these spots.

https://www.astronomynotes.com/starsun/granulationsm.gif]]> 2018-08-06 16:21:16 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272094979 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272095103 These are the arcs of gas/plasma that erupt from the photophere. Some can last from a few hours to months. Even today scientists aren't completely sure how these form.

https://www.astronomynotes.com/starsun/prominencesm.jpg]]> 2018-08-06 16:22:47 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272095103 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272095403 These are energy charged particles that flow out of the sun and towards the Earth by solar winds. This energy reacts with Earth's magnetic field by changing the energy and creating a huge hole.

https://apod.nasa.gov/apod/image/1804/DragonAurora_Bastoni_960.jpg]]> 2018-08-06 16:26:08 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272095403 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272095689 http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Core.html
http://csep10.phys.utk.edu/astr162/lect/sun/interior.html
http://solarscience.msfc.nasa.gov/interior.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/photosphere.html
http://solarscience.msfc.nasa.gov/surface.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/chromosphere.html
http://csep10.phys.utk.edu/astr162/lect/sun/corona.html
https://www.eso.org/public/outreach/eduoff/vt-2004/mt-2003/mt-2003-sun-corona-normal.jpg
https://upload.wikimedia.org/wikipedia/commons/d/d4/Sun_poster.svg
http://coolcosmos.ipac.caltech.edu/ask/11-Why-does-the-Sun-have-spots-
http://www.enchantedlearning.com/subjects/astronomy/sun/prominences.shtml
http://www.nasa.gov/mission_pages/sunearth/news/News022411-monsterprom.html#.VmoKlfmrTIV
http://hesperia.gsfc.nasa.gov/sftheory/flare.htm
http://pwg.gsfc.nasa.gov/polar/EPO/auroral_poster/aurora_all.pdf
https://www.astronomynotes.com/starsun/s2.htm]]> 2018-08-06 16:28:47 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272095689 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272096191 https://www.astronomynotes.com/starsun/s2.htm
http://hesperia.gsfc.nasa.gov/sftheory/flare.htm
http://coolcosmos.ipac.caltech.edu/ask/11-Why-does-the-Sun-have-spots-
http://www.enchantedlearning.com/subjects/astronomy/sun/prominences.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/chromosphere.html
http://csep10.phys.utk.edu/astr162/lect/sun/corona.html
http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Core.html
http://media.web.britannica.com/eb-media/04/92904-034-7C3D6409.jpg
http://csep10.phys.utk.edu/astr162/lect/sun/interior.html
http://solarscience.msfc.nasa.gov/interior.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/photosphere.html
http://solarscience.msfc.nasa.gov/surface.shtml]]> 2018-08-06 16:34:02 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272096191 s_w_a_w_2_6_0 https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272097417 These happen suddenly and rapidly. They are made when magnetic energy is released and can release intense variation in bright light.

https://cdn.cnn.com/cnnnext/dam/assets/170914181101-earth-ducks-a-cosmic-bullet-opinion-lincoln-exlarge-169.jpg]]> 2018-08-06 16:47:14 UTC https://padlet.com/s_w_a_w_2_6_0/unxk8225mfw6/wish/272097417