The same as on Earth - but in different proportions. Most stars are made up almost entirely of hydrogen and helium; the so-called "metals" (heavier elements) are present in much smaller quantities.
The Hertzsprung-Russell diagram helps scientists study the properties and evolution of globular clusters by showing the relationship between a star's brightness and temperature. This diagram allows researchers to classify stars in globular clusters based on their stage of evolution and helps them understand how these clusters change over time.
Shortly after the big bang, the first stars were formed - Population III stars. These comprised of nothing more than hydrogen and helium and maybe a little lithium for good measure. When these stars died, they would have exploded as massive supernova and spread the first 26 elements into the Universe. These 26 elements would have mixed with hydrogen and helium to make the next set of stars - population II stars. Most of these stars, when they died, would have exploded as supernova, enriching the Universe with the rest of the elements. These elements, along with even more hydrogen and helium, combined to make our Sun. Our Sun is a metal rich star or population I star. Just in case your wondering what the next set of stars will be called, I have no idea - Population 0 maybe?
Its very own fuel: made up of hydrogen, carbon, and a few other elements. Stars were given 4 basic elements hydrogen carbon something something look it up. They used these to make new elements: all the elements on the periodic table. You are made up of elements created by stars long ago.
Stars less massive than the Sun primarily fuse hydrogen into helium in their cores. This process releases energy and creates elements up to helium. These stars do not have enough mass to create heavier elements through nuclear fusion processes.
Of which elements? - Stars usually consist mainly of hydrogen, less helium, and small amounts of the so-called "metals" (which, in astronomy, means any heavier elements).Of which elements? - Stars usually consist mainly of hydrogen, less helium, and small amounts of the so-called "metals" (which, in astronomy, means any heavier elements).Of which elements? - Stars usually consist mainly of hydrogen, less helium, and small amounts of the so-called "metals" (which, in astronomy, means any heavier elements).Of which elements? - Stars usually consist mainly of hydrogen, less helium, and small amounts of the so-called "metals" (which, in astronomy, means any heavier elements).
Globular clusters can contain anywhere from hundreds of thousands to millions of stars. The exact number varies depending on the cluster.
Globular clusters are dense groups of stars with close interactions that make it difficult for planets to form and remain stable. The strong gravitational forces and frequent stellar encounters can disrupt planetary systems, leading to their absence in globular clusters. Additionally, the metal-poor nature of globular cluster stars may hinder planet formation, as metals are important building blocks for planets.
Many stars together can make up a galaxy. Depending on the arrangement of the stars, they could either make up an elliptical, spiral, barred spiral, lenticular, or irregular galaxy. Stars can also be together by gravity in clusters. Stars that are clustered together in a spherical group are called globular clusters. Many stars are binary stars, meaning that 2 stars circle around either each other, or around a central point of gravity. These are the most basic star groupings in which there are "many" stars.
The Hertzsprung-Russell diagram helps scientists study the properties and evolution of globular clusters by showing the relationship between a star's brightness and temperature. This diagram allows researchers to classify stars in globular clusters based on their stage of evolution and helps them understand how these clusters change over time.
First stars made the smallest elements, from hydrogen up and progressively larger stars made progressively larger elements
Stars are composed mostly of hydrogen and helium.
Shortly after the big bang, the first stars were formed - Population III stars. These comprised of nothing more than hydrogen and helium and maybe a little lithium for good measure. When these stars died, they would have exploded as massive supernova and spread the first 26 elements into the Universe. These 26 elements would have mixed with hydrogen and helium to make the next set of stars - population II stars. Most of these stars, when they died, would have exploded as supernova, enriching the Universe with the rest of the elements. These elements, along with even more hydrogen and helium, combined to make our Sun. Our Sun is a metal rich star or population I star. Just in case your wondering what the next set of stars will be called, I have no idea - Population 0 maybe?
The first is hydrogen, and the second is helium, they make up 97% if the mass if the stars.
The elements on the periodic table were created by stars through nuclear fusion. We use the term stellar nucleosynthesis to describe what stars are doing through fusion. Stars fuse hydrogen into helium, and then start making heavier elements by a different fusion process. But stars can only make elements up through iron. They can't make the heavier elements. Enter the supernova. A supernova is that "big blast" that occurs at the end of the life of some stars. In a supernova, the trans-iron elements are formed. That is, all the elements heavier than iron are formed in a supernova. Because the elements heavier than iron are formed in a supernova, we can say that there is a relationship between the supernova and the periodic table of elements.
Actually the typical distances between stars vary a lot. Inside a globular cluster, you can have a million stars or so, which are much closer together than in our region.If you ask "Why are they distant from one another in our region of the galaxy", I would say that that can POSSIBLY be answered by the anthropic principle: if stars are much closer together, the conditions MIGHT be catastrophic, and make it difficult for life to survive.
That would probably be a globular cluster. (A galaxy usually has more stars than that - from several million to several billion stars.)
The scientific basis behind the idea that humans are made out of stars is that the elements that make up our bodies, such as carbon, oxygen, and nitrogen, were created in the cores of stars through nuclear fusion. When these stars exploded in supernova events, these elements were scattered into space and eventually formed new stars, planets, and life forms, including humans. This connection between the elements in our bodies and the processes that occur in stars is what leads to the poetic notion that we are made of stardust.