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what is the difference between line spectrum and continous spectrum?
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what is the difference between line spectrum and continous spectrum? R...
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what is the difference between line spectrum and continous spectrum? R...
Continuous is the one with no single gap such that we can't identify where the new region starts and the old one ends. whereas in line spectrum we can clearly see each region as there is darkness in between
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Read the following text and answer the following questions on the basis of the same:Spectrum Analysis and AstronomyEach element in the periodic table can appear in gaseous form and produce its own spectrum unique to that element. Hydrogen will not look like Helium, which will not look like carbon which will not look like iron... and soon.Astrophysicists can identify what kinds of materials are present in stars from the analysis of star’s spectra. This type of study is called astronomical spectroscopy.The science of spectroscopy is quite sophisticated. From spectrum lines analysis astrophysicists can determine not only the element, but the temperature and density of that element in the star. The spectral line also can tell us about any magnetic field of the star.The width of the line can tell us how fast the material is moving. We can learn about winds in stars from this. The shifting of spectral lines shift back and forth indicates that the star may be orbiting another star.The following table shows a rough guide for the relationship between the temperature of a star and the electromagnetic spectrum.If the spectrum of a star is red or blue shifted, then it can be used to infer its velocity along the line of sight. Edwin Hubble observed that more distant galaxies tended to have more red shifted spectra. This establishes the theory of expansion of the universe.Q. Which nature of spectrum establishes the theory of the expanding universe?

Read the following text and answer the following questions on the basis of the same:Spectrum Analysis and AstronomyEach element in the periodic table can appear in gaseous form and produce its own spectrum unique to that element. Hydrogen will not look like Helium, which will not look like carbon which will not look like iron... and soon.Astrophysicists can identify what kinds of materials are present in stars from the analysis of star’s spectra. This type of study is called astronomical spectroscopy.The science of spectroscopy is quite sophisticated. From spectrum lines analysis astrophysicists can determine not only the element, but the temperature and density of that element in the star. The spectral line also can tell us about any magnetic field of the star.The width of the line can tell us how fast the material is moving. We can learn about winds in stars from this. The shifting of spectral lines shift back and forth indicates that the star may be orbiting another star.The following table shows a rough guide for the relationship between the temperature of a star and the electromagnetic spectrum.If the spectrum of a star is red or blue shifted, then it can be used to infer its velocity along the line of sight. Edwin Hubble observed that more distant galaxies tended to have more red shifted spectra. This establishes the theory of expansion of the universe.Q. What may be the approximate temperature if soft X-rays are found predominantly in the spectrum?

Read the following text and answer the following questions on the basis of the same:Spectrum Analysis and AstronomyEach element in the periodic table can appear in gaseous form and produce its own spectrum unique to that element. Hydrogen will not look like Helium, which will not look like carbon which will not look like iron... and soon.Astrophysicists can identify what kinds of materials are present in stars from the analysis of star’s spectra. This type of study is called astronomical spectroscopy.The science of spectroscopy is quite sophisticated. From spectrum lines analysis astrophysicists can determine not only the element, but the temperature and density of that element in the star. The spectral line also can tell us about any magnetic field of the star.The width of the line can tell us how fast the material is moving. We can learn about winds in stars from this. The shifting of spectral lines shift back and forth indicates that the star may be orbiting another star.The following table shows a rough guide for the relationship between the temperature of a star and the electromagnetic spectrum.If the spectrum of a star is red or blue shifted, then it can be used to infer its velocity along the line of sight. Edwin Hubble observed that more distant galaxies tended to have more red shifted spectra. This establishes the theory of expansion of the universe.Q. What is astronomical spectroscopy?

what is the difference between line spectrum and continous spectrum? Related: Rutherford's Nuclear Model of an Atom?
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