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Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum

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Is it true that The dark lines of the spectrum were named for Kirchhoff?

Yes, the dark lines in the spectrum were named Kirchhoff lines after the German physicist Gustav Kirchhoff, who, along with Robert Bunsen, contributed to the understanding of spectral lines. They discovered that these lines are specific to each element and can be used to identify chemical composition.


What is a dark line found in a spectrum is called?

A dark line found in a spectrum is called an absorption line. Absorption lines are created when atoms or molecules absorb specific wavelengths of light, resulting in dark lines in the spectrum where that light is missing.


What are some comparisons with a absorption spectrum and a continuous spectrum?

An absorption spectrum shows dark lines at specific wavelengths where light has been absorbed by a substance. A continuous spectrum shows all colors/wavelengths with no gaps, like the rainbow. The main difference is that the absorption spectrum has specific dark lines while the continuous spectrum is smooth and uninterrupted.


What does a dark line in a spectrum mean?

A dark line in a spectrum, also known as an absorption line, represents a specific wavelength of light that has been absorbed by a substance between the source of light and the observer. The presence of dark lines in a spectrum can provide information about the composition and properties of the absorbing material.


What causes the creation of Fraunhofer lines in the Sun's electromagnetic spectrum?

Fraunhofer lines in the Sun's electromagnetic spectrum are caused by the absorption of specific wavelengths of light by elements in the Sun's atmosphere. These elements absorb light at certain frequencies, creating dark lines in the spectrum that help scientists identify the composition of the Sun.

Related Questions

What are dark lines in a stellar spectrum called?

The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.


Continuous spectrum with dark lines where light is absorbed?

dark-line spectrum...


Is it true that The dark lines of the spectrum were named for Kirchhoff?

Yes, the dark lines in the spectrum were named Kirchhoff lines after the German physicist Gustav Kirchhoff, who, along with Robert Bunsen, contributed to the understanding of spectral lines. They discovered that these lines are specific to each element and can be used to identify chemical composition.


What part of the star is responsible for the dark lines in its spectrum?

The dark lines in a star's spectrum are caused by absorption of specific wavelengths of light by the elements in the star's outer atmosphere. This absorption occurs when the elements in the atmosphere absorb photons of specific energies, leading to the creation of dark absorption lines in the spectrum.


What is a dark line found in a spectrum is called?

A dark line found in a spectrum is called an absorption line. Absorption lines are created when atoms or molecules absorb specific wavelengths of light, resulting in dark lines in the spectrum where that light is missing.


Dark lines in an absorption spectrum are called?

Dark lines in an absorption spectrum are called absorption lines. These lines correspond to wavelengths of light that have been absorbed by specific elements or molecules in the sample being analyzed. They appear as dips or gaps in the spectrum where less light is detected.


What does the presence of dark lines in the solar spectrum mean?

The dark lines represents the absorption of energy at that frequency, E=hf.


Why can elements in a star be separated?

Because the spectrum of the star's light can be seen to have dark lines all the way through, and each element has its own set of dark lines in the star's spectrum.


Who discovered the dark line spectrum?

The dark line spectrum was first observed by Joseph von Fraunhofer in 1814 during his study of the Sun's spectrum. These dark lines are now known as Fraunhofer lines and are caused by absorption of specific wavelengths of light by various elements in the Sun's atmosphere.


What does a star's dark-line spectrum reveal?

The dark lines reveal the atoms that are associated with the stars atmosphere. The dark lines are atom energy absorption signatures.


When a star's spectrum shows dark lines against a continuous background what does this indicate?

Dark lines in a star's spectrum indicate absorption lines, which are caused by elements in the star's atmosphere absorbing specific wavelengths of light. These lines provide information about the composition and temperature of the star.


What are some comparisons with a absorption spectrum and a continuous spectrum?

An absorption spectrum shows dark lines at specific wavelengths where light has been absorbed by a substance. A continuous spectrum shows all colors/wavelengths with no gaps, like the rainbow. The main difference is that the absorption spectrum has specific dark lines while the continuous spectrum is smooth and uninterrupted.