Emission from hydrogen discharge tube

In summary, the conversation discusses the observation of a small number of lines in a lab experiment on emission from atomic hydrogen compared to a large number of lines in the hydrogen spectrum of a star. The possible explanation for this difference is related to temperature, but the exact reason is unknown. The discussion also mentions the role of atomic transitions in determining which lines are observed. Furthermore, the topic of gas-discharge tubes and their light production is briefly mentioned.
  • #1
utkarshakash
Gold Member
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Homework Statement


In a lab experiment on emission from atomic hydrogen in a discharge tube only a small number of lines are observed whereas a large number of lines are present in the hydrogen spectrum of a star. Why?

The Attempt at a Solution



I think it is related to temperatue but I don't know why.
 
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  • #2
The lines come from atomic transitions.
What determines which transitions can happen and which get observed?
 
  • #3
Simon Bridge said:
The lines come from atomic transitions.
What determines which transitions can happen and which get observed?

The photons
 
  • #4
The photons come from the transitions - what determines which transitions can happen and which get observed?
Do you know how a gas-discharge tube makes light? Why it is a particular color?
 
  • #5


It is indeed related to temperature, but there are several factors at play here. In a discharge tube experiment, the hydrogen gas is excited by an electrical current, causing the electrons to jump to higher energy levels and then emit light as they return to their ground state. This results in a limited number of emission lines, as only certain energy transitions are possible in this controlled environment.

In contrast, in the atmosphere of a star, the temperature is much higher and the hydrogen atoms are constantly colliding with each other. This results in a broader range of energy transitions, leading to a larger number of emission lines in the spectrum. Additionally, the presence of other elements and their interactions with hydrogen can also contribute to the complexity of the spectrum.

In summary, the difference in temperature and environmental conditions between a discharge tube and a star's atmosphere can greatly affect the number and complexity of emission lines observed.
 

1. What is a hydrogen discharge tube and how does it work?

A hydrogen discharge tube is a sealed glass tube filled with hydrogen gas at low pressure. When an electric current is passed through the tube, it excites the hydrogen atoms, causing them to emit light at specific wavelengths. This process is known as the emission of light from hydrogen atoms.

2. What causes the different colors of light emitted from a hydrogen discharge tube?

The different colors of light emitted from a hydrogen discharge tube are caused by the different energy levels of the excited hydrogen atoms. As these atoms return to their ground state, they release energy in the form of light at specific wavelengths, which correspond to different colors.

3. How is a hydrogen discharge tube used in scientific research?

Hydrogen discharge tubes are commonly used in scientific research to study the emission spectrum of hydrogen. By analyzing the specific wavelengths of light emitted, scientists can gain insights into the energy levels and structure of hydrogen atoms. This information is crucial for understanding various phenomena in physics and chemistry.

4. Can a hydrogen discharge tube emit other types of radiation besides visible light?

Yes, a hydrogen discharge tube can also emit ultraviolet and infrared radiation, in addition to visible light. The specific wavelengths of these emissions depend on the energy levels of the excited hydrogen atoms.

5. Are there any practical applications of a hydrogen discharge tube?

While hydrogen discharge tubes are mainly used for scientific research, they also have practical applications. For example, they are used in some types of neon signs and in fluorescent lamps to produce light. They are also used in spectroscopy, a technique for analyzing the chemical composition of substances.

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