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Consider two stars with temperatures of 10,000 and 25,000 Kelvin. 3. Calculate the ratio of atoms in the n=2 to n=1 energy levels for hydrogen atoms in the atmosphere of the star with A spectral type. Note: the statistical weights of the energy levels for hydrogen are equal to gn=2n²-

Consider two stars with temperatures of 10,000 and 25,000 Kelvin. 3. Calculate the ratio of atoms in the n=2 to n=1 energy levels for hydrogen atoms in the atmosphere of the star with A spectral type. Note: the statistical weights of the energy levels for hydrogen are equal to gn=2n²-

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Consider two stars with temperatures of 10,000 and 25,000 Kelvin. 3. Calculate the ratio of atoms in the n=2 to n=1 energy levels for hydrogen atoms in the atmosphere of the star with A spectral type. Note: the statistical weights of the energy levels for hydrogen are equal to gn=2n²
Transcribed Image Text:Consider two stars with temperatures of 10,000 and 25,000 Kelvin. 3. Calculate the ratio of atoms in the n=2 to n=1 energy levels for hydrogen atoms in the atmosphere of the star with A spectral type. Note: the statistical weights of the energy levels for hydrogen are equal to gn=2n²
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