This expulsion of stellar material is referred to as stellar “wind,” and it can travel at millions of kilometres per hour.
This expulsion of stellar material is referred to as stellar "wind", and it can travel at millions of kilometres per hour.
This expulsion of stellar material is referred to as stellar “wind”, and it can travel at millions of kilometres per hour.
Supernova explosions spread the stellar material into the interstellar medium, making it richer in metals.
Supernova explosions spread the stellar material into the interstellar medium, making it rich in metals.
Just 4 percent is the regular matter that we can see: stars, planets, and interstellar and intergalactic gas.
Just 4 per cent is the regular matter that we can see: stars, planets, and interstellar and intergalactic gas.
This ejection of stellar matter was the third largest on record.
Photons can also interact with stellar matter and deposit their energy.
This ejection of stellar matter was the third largest on record.
And what they will see are the highways of seeming blackness between the clumps of star matter.
It also means the galaxy has 3000 times more dark matter than stellar mass.
How did stellar matter from the Big Bang congeal into what we see today?
There is a huge field of science, however, that investigates the formation of stellar matter.
This term comes near to the real fact, since the substance of this form is derived from cosmic matter or star matter, roughly speaking.
Planets are born from the material left over from star birth.
This term comes near to the real fact, since the substance of this form is derived from cosmic matter or star matter, roughly speaking.
All told, the research suggests that an "optimal" close encounter could fuse up to 60 percent of the stellar matter into iron.
We are bits of stellar matter that got cold by accident, bits of a star gone wrong.
For example We are bits of stellar matter that got cold by accident, bits of a star gone wrong.
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