While studying the spectrum of a gas cloud in space, an astronomer magnifies a spectral line that results from a transition from ap state to an s state. She finds that the line at 575.050 nm has actually split into three lines, with adjacent lines 4.70 x 10- nm apart, indicating that the gas is in an external magnetic field. (Ignore effects due to electron spin.) What is the strength of the external magnetic field? B =3.25 T B=2.98 T B=2.79 T B =3.05 T B=2.05 T

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Chapter7: Quantum Mechanics
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While studying the spectrumn of a gas doud in space, an astronomer magnifies a spectral line
that results from a transition from a p state to an s state, She finds that the line at 575.050
nm has actually split into three lines, with adjacent lines 4.70 x 10- nm apart, indicating
that the gas is in an external magnetic field. (Ignore effects due to electron spin.)
What is the strength of the external magnetic field?
O B=3.25 T
OB-2.98 T
O B=2.79 T
O B=3.05 T
OB=2.05 T
Transcribed Image Text:While studying the spectrumn of a gas doud in space, an astronomer magnifies a spectral line that results from a transition from a p state to an s state, She finds that the line at 575.050 nm has actually split into three lines, with adjacent lines 4.70 x 10- nm apart, indicating that the gas is in an external magnetic field. (Ignore effects due to electron spin.) What is the strength of the external magnetic field? O B=3.25 T OB-2.98 T O B=2.79 T O B=3.05 T OB=2.05 T
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