Emission lines and absorption lines

In summary, the question is why emission lines are more commonly observed than absorption lines in the atomic spectra of most elements. It is suggested to consider how emission and absorption spectra are generated in a laboratory setting and the practical aspects of obtaining an absorption spectrum from a gas. The effect of different physical states (solid, liquid, gas) on spectroscopy is also mentioned. Additionally, the differences between laboratory and astronomical spectroscopy are noted.
  • #1
Sweetyme123
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Why more emission lines than absorption lines are usually observed in the atomic spectra of most elements hence explain why this occures?
 
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  • #2
Hi Sweetyme123, is this a homework question?
 
  • #3
Sweetyme123 said:
Why more emission lines than absorption lines are usually observed in the atomic spectra of most elements hence explain why this occures?
Ask yourself (or find out) how an emission spectrum can be generated in a Lab. Find out how absorption spectrum can be observed or measured. Then think in practical terms.
If you want to obtain the (line) absorption spectrum of a gas then how long a light path through a gas is needed before a significant proportion of the light is absorbed at the frequencies of interest. Where do we find large enough volumes of gas to obtain absorption spectra? Its this different for solids and liquids and in what way?
The expression "swings and roundabouts" seems to apply here. Plenty to discuss and to read around about.
PS There are different circumstances in astronomical spectroscopy, which make things different from how they are in a Lab.
 

What are emission lines and absorption lines?

Emission lines and absorption lines are spectral features that appear in the spectrum of light emitted or absorbed by an object. They are caused by the interaction between light and the electrons in the atoms or molecules of the object.

What causes emission lines and absorption lines?

Emission lines are caused by the emission of photons when electrons in an atom or molecule transition from a higher energy state to a lower energy state. Absorption lines are caused by the absorption of photons when electrons in an atom or molecule transition from a lower energy state to a higher energy state.

How are emission lines and absorption lines used in astronomy?

Emission lines and absorption lines are used to study the chemical composition and physical properties of objects in space. By analyzing the specific wavelengths of these lines, scientists can determine the elements present and their relative abundances, as well as other characteristics such as temperature and density.

What is the difference between emission lines and absorption lines?

The main difference between emission lines and absorption lines is the direction of the light. Emission lines appear as bright lines in a dark background, while absorption lines appear as dark lines in a bright background. Additionally, emission lines are produced by the emission of photons, while absorption lines are produced by the absorption of photons.

Can emission lines and absorption lines be used to determine the distance of objects in space?

Emission lines and absorption lines can be used to determine the distance of objects in space through a technique called spectroscopic parallax. By measuring the shift in the wavelengths of these lines, scientists can calculate the distance of the object based on its known spectral characteristics.

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