While that first type of star — what astronomers call “metal-rich” stars, since to an astronomer, any element on the periodic table that isn’t hydrogen or helium counts as a metal — can come in all different sizes, masses, and colors, the same isn’t true for that second type of star. The “metal-poor” stars in our Universe are overwhelmingly small, low in mass, and red in color.
properties, elements, and planets that they do because of all the stars that died before their creation. This is a relatively young open cluster, as evidenced by the high-mass, bright blue stars that dominate its appearance, but there are hundreds of times as many lower-mass, fainter stars inside.Today, whenever you make a large number of new stars all at once, here’s what happens.
And how easy or hard it is for gas to collapse and form new stars determines what astronomers know as the “,” which tells us what types, masses, colors, temperatures, and lifetimes of the stars that form will be. largest star-forming region known in the local group. The hottest, bluest stars are over 200 times the mass of our Sun, although from our distance of 165,000 light-years away, we predominantly see the brightest, rarest stars; the more common, lower mass ones are not clearly visible here.
Taken into account all the processes in our body, both chemical and physical, we are dynamic systems as well. I´m not the same person as I was a milisecond before. science
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