While studying the spectrum of a gas cloud in space, an astronomer magnifies a spectral linet hat 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 4.60 * 10^-2 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?
While studying the spectrum of a gas cloud in space, an astronomer magnifies a spectral linet hat 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 4.60 * 10^-2 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?
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![While studying the spectrum of a gas cloud in space, an astronomer
magnifies a spectral linet hat 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 4.60 * 10^-2 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?](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F6fcd7fab-9903-4b0b-a30c-af5d8b8fc75f%2F0bcdcf4d-a8b0-4cdb-bde9-06adbd0ef22d%2Fi16jia4_processed.png&w=3840&q=75)
Transcribed Image Text:While studying the spectrum of a gas cloud in space, an astronomer
magnifies a spectral linet hat 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 4.60 * 10^-2 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?
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