A star's internal composition does not change as the star ages, as a result of rising temperatures. The life span of a star is from one to ten-billion years. Larger, more massive stars have a shorter lifespan than smaller ones, due to the pressure on the core causing the larger stars to burn hydrogen more quickly.
Scientists determine the composition of a star by studying its spectrum, which is produced by analyzing the light emitted by the star. By examining the absorption lines in the spectrum, scientists can identify the elements present in the star's atmosphere and infer its overall composition. Additionally, measurements of the star's temperature, luminosity, and mass can also provide valuable information about its composition.
composition and temperature. The spectral lines correspond to different elements present in the star and the wavelengths of these lines are affected by the star's temperature. By analyzing these lines, astronomers can determine the chemical composition and other characteristics of the star.
Yes, a scientist can identify a star's composition by analyzing its continuous spectrum. Different elements emit light at specific wavelengths, creating unique spectral lines that can reveal the presence of specific elements in a star's atmosphere. By analyzing these spectral lines, scientists can determine the composition of a star.
If the spectrum of a star shows the same absorption lines as the sun than you know that the star has the same composition as the sun. This means that the star is made of the same elements as the sun.
It's a star that due to size and composition gives off blueish-white light.
it becomes a volcanic rock that is still very hot but bot as hot as the star was originally
Yes, the ratio of helium atoms to hydrogen atoms does increase as a star ages. Stars undergo nuclear fusion reactions in their core, converting hydrogen into helium over time. This process increases the proportion of helium relative to hydrogen in the star's composition as it ages.
True. As a star ages and uses up its nuclear fuel, the core temperature increases, leading to changes in its internal composition. For example, nuclear fusion reactions in the core can convert hydrogen into helium, and then helium into heavier elements like carbon, oxygen, and eventually iron.
During last ages of life of a star, to find what happens in coming ages of life of star. It determines on its mass explained by chandrashekher that if the mass of given star is 2.42 times the mass of our sun then it explodes in the form of supernova. If the mass of given star is less than the 2.42 times the mass of our sun then it shrinks to become white dwarf.
Scientists determine the composition of a star by studying its spectrum, which is produced by analyzing the light emitted by the star. By examining the absorption lines in the spectrum, scientists can identify the elements present in the star's atmosphere and infer its overall composition. Additionally, measurements of the star's temperature, luminosity, and mass can also provide valuable information about its composition.
Nuclear physics. As a star ages, the fusion of lighter elements into heavier elements changes the composition of the star's core, which in turn affects the dynamics of its interior. Convection patterns change, the core's energy production changes, and so on. This ultimately affects the way a star looks in our telescopes.
the lines in its spectrum
composition and temperature. The spectral lines correspond to different elements present in the star and the wavelengths of these lines are affected by the star's temperature. By analyzing these lines, astronomers can determine the chemical composition and other characteristics of the star.
The chemical composition of the star.
Yes, a scientist can identify a star's composition by analyzing its continuous spectrum. Different elements emit light at specific wavelengths, creating unique spectral lines that can reveal the presence of specific elements in a star's atmosphere. By analyzing these spectral lines, scientists can determine the composition of a star.
composition (and) temperature.
Yes, it is.