counting backwards to zero

the future's so bright because the sun will eventually kill us 
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sunlifecycle

 

How the sun really works

The main Problems with the current model of the sun are as follows:

* Temperature of the halo-like corona is 300 times that of surface, violating the inverse square law for radiation
* Rotates faster at equator, faster on surface
* Solar wind accelerates (somehow) upon leaving the Sun
* Sunspots reveal cooler interior
* Sunspots travel faster than surrounding surface
* Sunspot penumbra (interior walls) reveal structured filaments and move much faster than slow convection should allow

An eletcrical model would solve many of these problems.

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Life of a Star: 12 billion years in 6 minutes


"don't think about all those things you fear, just be glad to be here"
FC Kahuna - Hayling

The lifecycle of a G-type star, like The Sun.

All original videos are copyrighted to NASA, NASA JPL/Caltech, and ESA. Use is under Creative Commons Share Alike licensing. Please note that I didn't create these videos -- simply compiled them. Enjoy!

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Filed under  //   FC Kahuna Hayling   heliosphere   helium flash   infinite universe   mass loss   molecular cloud accretion   music video   planetary nebula   red giant   space   star   sun lifecycle   universe   video   videos   white dwarf   youtube  

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