Our solar system sun born story 💥💥💥💥
Out solar
History of our sun!
system sun story very mistress because our sun our solar system big star so our sun divided by 3 layer first of all surface layer that's layer temperature 5 thousand 500c and 2 layer temperature 30,000c and 3 layer temperature 79 lakhs 87 thousand 596c we thinking about it where was angry inside the sun ,
sun inside billons atom inside around the sun this sun light to reaching by our earth thinking about it that's objects how was born so that's neutrino particles many estragole that came sun inside out the neutrino particles 720 p/ km h speed inside out our sun
because sun layer like radiation zone other particles destroyed neutrino particles that's particles with him destroyed a born new particles that's inside out the sun surface very speed now sun surface neutrino particles that's not simple
because sun surface spot very dangers to put rubbers band they rubber bands temperature very high and neutrino particles
that's destroyed it so neutrino particles many billons years after sun surface out that's cycles every billons years ago
History of our sun!
In a wide expanse of space, gravity drew dust and gas together to create the young solar system. The sun formed first from the vast material, with the planets close behind. But how did a sea of swirling particles become the brightest star in our sky?
"The sun is terrifying and gorgeous, and it's also the best physics laboratory in our solar system," Sabrina Savage, project scientist for NASA's Hinode at NASA's Marshall Space Flight Center in Huntsville, Alabama, said in a statement.
Although it may look empty, space is filled with gas and dust. Most of the material was hydrogen and helium, but some of it was made up of leftover remnants from the violent deaths of stars. About 4.5 billion years ago, waves of energy traveling through space pressed clouds of such particles closer together, and gravity caused them to collapse in on themselves and then start to spin. The spin caused the cloud to flatten into a disk like a pancake. In the center, the material clumped together to form a protostar that would eventually become the sun.
"There is a rotationally supported disk around this protostar," astronomer John Tobin told Space.com about a similar early sun, adding it's a "key element" in building planets. "It lets the material hang out long enough for the planet formation process."
The young protostar was a ball of hydrogen and helium not yet powered by fusion. Over tens of millions of years, the temperature and pressure of the material inside increased, jumpstarting the fusion of hydrogen that drives the sun today.
system sun story very mistress because our sun our solar system big star so our sun divided by 3 layer first of all surface layer that's layer temperature 5 thousand 500c and 2 layer temperature 30,000c and 3 layer temperature 79 lakhs 87 thousand 596c we thinking about it where was angry inside the sun ,
sun inside billons atom inside around the sun this sun light to reaching by our earth thinking about it that's objects how was born so that's neutrino particles many estragole that came sun inside out the neutrino particles 720 p/ km h speed inside out our sun
because sun layer like radiation zone other particles destroyed neutrino particles that's particles with him destroyed a born new particles that's inside out the sun surface very speed now sun surface neutrino particles that's not simple
because sun surface spot very dangers to put rubbers band they rubber bands temperature very high and neutrino particles
that's destroyed it so neutrino particles many billons years after sun surface out that's cycles every billons years ago
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