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Q: What spectrum are bright lines against dark background?
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What were dark lines in the spectrum named for?

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


Why in an absorption spectrum the back ground is bright and the lines are dark?

Because it is an absorption spectrum. An absorption spectrum begins with a source of pure white light. This hits a prism which spreads it out into a spectrum and the result shows on a screen as a bright band of colours. If you put this into a glass case and seal it to the outside world, nothing changes. Now if blow a gas into the tank, the atoms in the gas absorb different wavelengths (colours) of light. The result you see is a normal spectrum of colours, but with one or more dark lines across it. This is because the atoms in the gas through which the white light is shining are absorbing some or all of various colours in the spectrum. What those colours are is absolutely characteristic and definitive of that particular gas. This is a very powerful technique for identifying elements which are present only in trace amounts. An interesting light on this is that the element Helium was first discovered not on earth, but on the sun by some dark lines in the sun's spectrum which did not belong to any known element.


What is the difference between a continuous spectrum an a line spectrum?

Dispersion, the separation of visible light into a spectrum, may be accomplished by means of a prism or a diffraction grating. Each different wavelength or frequency of visible light corresponds to a different color, so that the spectrum appears as a band of colors ranging from violet at the short-wavelength (high-frequency) end of the spectrum through indigo, blue, green, yellow, and orange, to red at the long-wavelength (low-frequency) end of the spectrum. In addition to visible light, other types of electromagnetic radiation may be spread into a spectrum according to frequency or wavelength. The spectrum formed from white light contains all colors, or frequencies, and is known as a continuous spectrum. Continuous spectra are produced by all incandescent solids and liquids and by gases under high pressure. A gas under low pressure does not produce a continuous spectrum but instead produces a line spectrum, i.e., one composed of individual lines at specific frequencies characteristic of the gas, rather than a continuous band of all frequencies. If the gas is made incandescent by heat or an electric discharge, the resulting spectrum is a bright-line, or emission, spectrum, consisting of a series of bright lines against a dark background. A dark-line, or absorption, spectrum is the reverse of a bright-line spectrum; it is produced when white light containing all frequencies passes through a gas not hot enough to be incandescent. It consists of a series of dark lines superimposed on a continuous spectrum, each line corresponding to a frequency where a bright line would appear if the gas were incandescent. The Fraunhofer lines appearing in the spectrum of the sun are an example of a dark-line spectrum; they are caused by the absorption of certain frequencies of light by the cooler, outer layers of the solar atmosphere. Line spectra of either type are useful in chemical analysis, since they reveal the presence of particular elements. The instrument used for studying line spectra is the spectroscope.


What is s band spectrum?

Band spectrum is the spectrum given by the molecules. It consists of series of closely spaced lines known as bands separated by the dark spaces.


What causes the lines in an atomice spectrum?

wavelengths of absorbed or emitted photons

Related questions

The Orion nebula m 42 is a hot thin cloud of glowing gas so its spectrum is?

A few bright lines against a dark background.


What kind of spectrum do dark lines appear against a bright a bright background of colors ranging from red to blue?

Dark-line spectrum is a "photo-negative" of emission spectrum. It is the gaps that appear in precisely the same location as corresponding bright lines. produced by a cool gas with a hot solid and you


In which case will the woman see a just a spectrum that is almost entirely black except for few bright emission lines?

The spectrum that she will be observing is called an emission spectrum, in which electrons are excited to a higher energy state and then drop back down to the ground state, during which the electrons will emit photons of specific wavelengths, which will be observed as bright lines of color on what appears to be a black background.


What do the bright lines in a bright light spectrum tell us?

to identify elements


Why can the bright-line spectrum of an element be used to identify an element?

The wave lengths of lines of the spectrum are different for each chemical element.


How can you Distinguish absorption spectrum from emission spectrum?

Emission spectra are bright-line spectra, absorption spectra are dark-line spectra. That is: an emission spectrum is a series of bright lines on a dark background. An absorption spectrum is a series of dark lines on a normal spectrum (rainbow) background.


What spectrum is produced by a hot gas under low pressure and appears in a series of bright lines?

Emission Spectrum


What does the term bright line spectrum mean?

There are several kinds of spectra. Bright line spectrum, or emission spectrum, is when light emitted by a gas has an electrical discharge going through it, and it produces a spectrum of just a few isolated parallel lines.


Image of emission or absorption spectrum of manganese?

This would consist of several series of lines corresponding to the energies of electron transitions. They are bright lines for an emission spectrum and dark for absorbtion.


What has the author James Barnes written?

James Barnes has written: 'On the analysis of bright spectrum lines ..' -- subject(s): Accessible book, Spectrum analysis, Interference (Light)


Why is there a line spectrum over a continuous spectrum in a spectroscope?

The lines in a spectroscope tell what element(s) are being observed. The continuous color are background noise or put there for a reference.


Star radiate different colors and lines based on their composition this is know as its?

It sounds like you're describing an emission spectrum. An emission spectrum will contain bright lines at specific colors, each of which is characteristic of a particular chemical element.