It depends exactly what you mean. You probably mean the Red Dwarf stars. I only know of one element that they make and that's Helium.
Only the most massive stars play a crucial role in enriching the galaxy with heavy elements because they undergo rapid nuclear fusion and have shorter lifespans, leading to explosive events like supernovae. During these explosions, they synthesize and disperse heavy elements, such as iron and gold, into the interstellar medium. In contrast, lower-mass stars do produce heavy elements, but their contributions are less significant and occur over much longer timescales. Thus, the violent death of massive stars is key to the rapid recycling of heavy elements in the galaxy.
Generally, yes. For stars on the main sequence, meaning that they fuse hydrogen at their cores, mass, size, color, brightness, and temperature are all closely related. More massive stars are larger, brighter and hotter than less massive ones. The least massive stars are red. As you go to more massive stars color changes to orange, then yellow, then white, and finally to blue for the most massive stars.
The stars in the constellation Scorpius exhibit a range of colors, including blue, white, and red. Blue stars are hotter and more massive, while red stars are cooler and less massive. The colors of the stars in Scorpius can vary based on their temperature and composition.
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).
Red stars are cooler and less massive than blue stars. They emit light in the red and infrared parts of the spectrum, indicating lower surface temperatures. Blue stars, on the other hand, are hotter and more massive, emitting light in the blue and ultraviolet parts of the spectrum.
1st generation stars, also known as Population III stars, formed shortly after the Big Bang and consisted mainly of hydrogen and helium. They are believed to have been massive and short-lived. 2nd generation stars, or Population II stars, formed from the remnants of 1st generation stars and contain heavier elements produced in their cores. They are typically older and less massive than 1st generation stars.
Yes, both black holes and neutron stars are remnants of the death of massive stars. Neutron stars form when the core of a massive star collapses but does not produce a black hole. Black holes are formed when the core of a massive star collapses beyond the neutron star stage.
Iron is not formed in the Sun through nuclear fusion. Iron is the element with the highest nuclear binding energy per nucleon, making it less energetically favorable for fusion reactions to produce iron in the Sun. Iron is typically formed in the later stages of a massive star's life during a supernova explosion.
Younger stars often are made up mainly of hydrogen, perhaps with some helium. Less massive stars will only fues hydrogen into helium, so eventually they will end up having a lot of helium. More massive stars however will eventually start fusing helium to metals, i.e., heavier elements. In any case, the "metallicity" (percentage of elements heavier than helium) and the percentages of different elements should vary somewhat between different stars.Younger stars often are made up mainly of hydrogen, perhaps with some helium. Less massive stars will only fues hydrogen into helium, so eventually they will end up having a lot of helium. More massive stars however will eventually start fusing helium to metals, i.e., heavier elements. In any case, the "metallicity" (percentage of elements heavier than helium) and the percentages of different elements should vary somewhat between different stars.Younger stars often are made up mainly of hydrogen, perhaps with some helium. Less massive stars will only fues hydrogen into helium, so eventually they will end up having a lot of helium. More massive stars however will eventually start fusing helium to metals, i.e., heavier elements. In any case, the "metallicity" (percentage of elements heavier than helium) and the percentages of different elements should vary somewhat between different stars.Younger stars often are made up mainly of hydrogen, perhaps with some helium. Less massive stars will only fues hydrogen into helium, so eventually they will end up having a lot of helium. More massive stars however will eventually start fusing helium to metals, i.e., heavier elements. In any case, the "metallicity" (percentage of elements heavier than helium) and the percentages of different elements should vary somewhat between different stars.
Only the most massive stars play a crucial role in enriching the galaxy with heavy elements because they undergo rapid nuclear fusion and have shorter lifespans, leading to explosive events like supernovae. During these explosions, they synthesize and disperse heavy elements, such as iron and gold, into the interstellar medium. In contrast, lower-mass stars do produce heavy elements, but their contributions are less significant and occur over much longer timescales. Thus, the violent death of massive stars is key to the rapid recycling of heavy elements in the galaxy.
No, stars less massive than the Sun do not have enough mass to undergo a supernova explosion. Instead, they may end their lives as a white dwarf or, if they are even less massive, a planetary nebula. Supernovae are events associated with more massive stars.
Nuclear fusion.
Less massive stars age more slowly than more massive stars primarily because they burn their nuclear fuel at a much slower rate. While massive stars have more fuel, they also have higher core temperatures and pressures, leading to rapid fusion processes that exhaust their fuel quickly. In contrast, less massive stars, like red dwarfs, fuse hydrogen slowly and can maintain stable fusion for billions of years, resulting in a longer lifespan overall. Thus, their slower consumption of fuel contributes to their extended lifetimes compared to their more massive counterparts.
Yes they can
Neutron stars smaller than white dwarfs are thought to be remnants of massive stars that have undergone supernova explosions. When these stars exhaust their nuclear fuel, they collapse under their own gravity, resulting in a neutron star if the core's mass is sufficient. In contrast, white dwarfs are formed from less massive stars that shed their outer layers, leaving behind a dense core. Therefore, neutron stars represent the end stage of more massive stellar evolution compared to white dwarfs.
Generally, yes. For stars on the main sequence, meaning that they fuse hydrogen at their cores, mass, size, color, brightness, and temperature are all closely related. More massive stars are larger, brighter and hotter than less massive ones. The least massive stars are red. As you go to more massive stars color changes to orange, then yellow, then white, and finally to blue for the most massive stars.
The most massive stars; they will use up their fuel much faster than less-massive stars. or even low mass star which is less then half the mass of our sun may able to last more then a trillion years that is longer then the universe age