There are a couple of things that cause specific lines to appear in a line spectrum. Two of these things are density and wavelength.
you get line spectra when an excited atom (gained extra energy) releases this energy. The energy is gained by electrons moving from one energy level to one of a higher energy level. The atom is not happy (too much energy) so it gets rid of it. The electrons jump back to their original level releasing the energy gained as light of a fixed frequency, hence a fine line.
Density and wavelengths of absorbed or emitted protons are two things that cause specific lines to appear in a line spectrum.
wavelengths of absorbed or released radioactivity by metals
Wavelengths of absorbed or emitted photons
Wavelengths of absorbed or emitted photons Every line in a line spectrum is caused by a transition, from one quantum state to another quantum state, involving electrons.
when a beam of white light is passed through the vapours or a gas, the element absorbs certain wavelengths, while the rest of wavelengths are passed through it. The spectrum of this radiation is called atomic absorption spectrum.The missing wavelengths appear as dark lines in the spectrum.
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.
An emission spectrum depend on electrons transition in the atom of a chemical element; and elements are different.Absorption spectrum is based on the different absorption pics of different molecules, depending on the frequency of radiation.Spectral methods are largely used in analytical chemistry.
The wave lengths of lines of the spectrum are different for each chemical element.
absorption lines! :)
'Astronomical spectrum' is not a specific term. I suspect you are thinking of the emission spectrum of a star, which can tell us a great deal about the composition of the star. Light and other radiations from the object are spread out into constituent wavelengths and dark lines appear across the spectrum at certain specific wavelengths which are characteristic of elements present.
The color in the flame is the representation of a specific line in the spectrum.
wavelengths of absorbed or emitted photons
because all of the different lines of a star's elements appear together i its spectrum, making the pattern different everytime
The lines indicate which atoms are in the outer layers of stars. The location of the lines is always the same when they form.
Absorption of energy at atom energy levels cause the line spectrum.
Each chemical element has a different spectrum; and each color has a specific wavelength.
Each chemical element has a different spectrum; and each color has a specific wavelength.
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.
Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum
It differs by that white light spectrum is continuous and consists of light of all wavelengths. Emission spectrum is not continuous. It consists of bright lines at specific wavelengths, with complete darkness between them.