Atomic Spectra and Bohr's Model

Front

Shortest wavelength in hydrogen spectrum

Back

Electron transition from n=4 to n=1

Front

Emission lines create bright spectral lines

Back

Electrons moving to ground state

Front

Subatomic particle responsible for spectral lines

Back

Electrons

Front

Ground state to excited state

Back

Absorb energy

Front

Electron returns to ground state

Back

Emit energy

Front

Electron transition n=4 to n=2

Back

Releases energy

Front

Electron energy state with least energy

Back

Ground state

Front

Line emission spectrum occurs when:

Back

Electron transition from higher to lower energy level.

Front

Elements in star's spectra

Back

Calcium only

Front

Visible light is the only type of electromagnetic radiation?

Back

False