Why Does Hydrogen Emit a Line Spectrum Instead of a Continuous Spectrum?

In summary, The line spectrum of hydrogen gas is explained by Bohr's model of the atom, which states that electrons can only occupy specific energy levels. When these electrons transition between levels, they emit photons of light at specific wavelengths, resulting in a line spectrum. A continuous spectrum is created by the unique energy levels of different elements, and an electron must absorb a specific amount of energy to move between levels. The electron is constantly jumping between levels, but only emits light when it moves from a higher level to a lower level.
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Homework Statement



My Chemistry book says: "Before reading further about the details of Bohr's model, speculate as to how they explain the fact that hydrogen gas emits a line spectrum rather than a continuous spectrum."

Homework Equations



The Rydberg Equation, though I suppose this is more of a conceptual confusion.

The Attempt at a Solution



If I am correct... this is because there are only so many orbits that that electron can assume (its relaxing from these exited orbits that emit the light? Thats where the engery goes when in depart the atom...). But this begs the question: how come anything, then, emits a continuous spectrum? Also, does a hydrogen atom have to absorb a certain amount of quanta for the electron to move up to any given orbit? Or is it CONSTANTLY jumping back down and it... well, I'd appreciate any help...

Thanks!
 
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  • #2


Hello,

Thank you for your question! The line spectrum of hydrogen gas can be explained by Bohr's model of the atom, which states that electrons can only occupy specific energy levels or orbits around the nucleus. When an electron in a higher energy level "jumps" down to a lower energy level, it emits a photon of light with a specific energy corresponding to the energy difference between the two levels. This explains why hydrogen gas emits specific wavelengths of light, or a line spectrum, rather than a continuous spectrum.

To address your question about continuous spectra, this can be explained by the fact that not all atoms have the same energy levels or orbits for their electrons. Each element has a unique set of energy levels, and when the electrons in these levels transition, they emit light at different wavelengths, resulting in a continuous spectrum.

As for your question about the absorption of quanta, yes, an electron must absorb a specific amount of energy (in the form of a photon) to move from one energy level to another. This energy corresponds to the energy difference between the two levels. And yes, the electron is constantly jumping between energy levels, but it is only when it jumps from a higher level to a lower level that it emits light.

I hope this helps clarify your confusion. Let me know if you have any other questions!



Chemist
 

1. What are spectral lines of hydrogen?

Spectral lines of hydrogen refer to the specific wavelengths of light emitted or absorbed by hydrogen atoms when they undergo a change in energy levels. These lines are unique to hydrogen and can be used to identify and study the element.

2. How are spectral lines of hydrogen formed?

Spectral lines of hydrogen are formed when the electrons in a hydrogen atom move from one energy level to another. This change in energy causes the emission or absorption of a specific wavelength of light, resulting in the characteristic spectral lines.

3. What is the significance of spectral lines of hydrogen?

Spectral lines of hydrogen have significant importance in the fields of astronomy, physics, and chemistry. They allow scientists to identify and study the composition of stars, galaxies, and other celestial bodies. They also provide insight into the structure of atoms and the behavior of electrons.

4. How many spectral lines does hydrogen have?

Hydrogen has an infinite number of spectral lines, but only a few are visible to the human eye. The most well-known spectral lines of hydrogen are the Balmer series, which consists of four visible lines in the red, blue-green, blue-violet, and violet regions of the electromagnetic spectrum.

5. Can spectral lines of hydrogen be used to determine the temperature of a star?

Yes, spectral lines of hydrogen can be used to determine the temperature of a star. The intensity and shape of the spectral lines can provide information about the energy levels and temperature of the atoms in the star's atmosphere. This allows scientists to classify stars based on their temperature, such as classifying them as hot, cool, or intermediate.

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