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This deck focuses on Emission And Absorption Spectra, giving you a quick way to review the definitions, rules, and examples that matter most for AP Physics 2.
Study Emission And Absorption Spectra in AP Physics 2 with focused flashcards that help you recognize the idea, recall the key rule, and apply it in practice-style prompts.
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What is an emission spectrum?
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A spectrum of frequencies emitted by an atom or molecule. Shows specific wavelengths of light emitted when electrons drop to lower energy levels.
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This deck focuses on Emission And Absorption Spectra, giving you a quick way to review the definitions, rules, and examples that matter most for AP Physics 2.
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Answer: A spectrum of frequencies emitted by an atom or molecule. Shows specific wavelengths of light emitted when electrons drop to lower energy levels.
Answer: Spectroscope. Optical instrument that disperses light into component wavelengths for observation.
Answer: Intensity of light at different wavelengths. Device separates and measures light intensity across electromagnetic spectrum.
Answer: Excited electrons fall to lower energy levels. Energy release during electron transitions produces characteristic photons.
Answer: Electrons absorb energy and move to higher levels. Energy absorption promotes electrons to higher quantum states.
Answer: Incandescent bulb or blackbody radiator. Thermal sources emit broad, continuous wavelength distribution.
Answer: Emission spectrum of hydrogen. Series of visible lines from electron transitions to n=2 level.
Answer: Emission spectrum. Bright lines indicate emission of specific wavelengths against dark background.
Answer: Incandescent bulb or blackbody radiator. Thermal sources emit broad, continuous wavelength distribution.
Answer: Both emission and absorption spectra. Combined techniques provide comprehensive elemental and quantitative analysis.
Answer: An instrument that records a spectrum photographically. Device that captures and records spectral data permanently for analysis.
Answer: Absorption spectrum. Atmospheric gases absorb specific wavelengths from continuous sunlight.
Answer: The concentration of elements. Line intensity correlates with number of atoms present.
Answer: An instrument that records a spectrum photographically. Device that captures and records spectral data permanently for analysis.
Answer: Continuous spectrum. Hot tungsten filament produces thermal radiation across all visible wavelengths.
Answer: To identify elements present in a sample. Bright emission lines reveal elemental composition through characteristic wavelengths.
Answer: Bright lines indicating emitted wavelengths. Emission spectrum shows bright lines against dark background.
Answer: Emission or absorption of photons. Energy differences between levels determine photon wavelength emitted or absorbed.
Answer: Continuous spectrum. Dense objects emit all wavelengths continuously due to thermal motion.
Answer: A spectrum showing dark lines or bands due to absorption of light. Occurs when electrons absorb specific wavelengths, creating gaps in continuous spectrum.
Answer: Calculates wavelengths of spectral lines of hydrogen. Mathematical formula predicting hydrogen spectral line wavelengths accurately.
Answer: To isolate specific wavelengths of light. Device selects narrow wavelength bands from broader spectrum.
Answer: To isolate specific wavelengths of light. Device selects narrow wavelength bands from broader spectrum.
Answer: Absorption spectrum. Cool gas atoms absorb specific wavelengths from continuous background light.
Answer: Excited electrons fall to lower energy levels. Energy release during electron transitions produces characteristic photons.
Answer: Absorption spectrum. Dark absorption lines reveal elemental composition of stellar atmospheres.
Answer: Electrons absorb energy and move to higher levels. Energy absorption promotes electrons to higher quantum states.
Answer: Infrared emission spectrum of hydrogen. Series of IR lines from electron transitions to n=3 level.
Answer: They identify elements and compounds. Each element produces unique spectral fingerprint for identification.
Answer: Emission spectrum. Low-density gas atoms emit discrete wavelengths when electrons transition downward.
Answer: Continuous spectrum. Prism disperses white light into complete rainbow without gaps.
Answer: Continuous spectrum. Dense objects emit all wavelengths continuously due to thermal motion.
Answer: Absorption spectrum. Dark lines in solar spectrum discovered by Joseph von Fraunhofer.
Answer: Bright lines indicating emitted wavelengths. Emission spectrum shows bright lines against dark background.
Answer: Bright yellow lines. Sodium's characteristic D-lines appear as intense yellow doublet.
Answer: They identify elements and compounds. Each element produces unique spectral fingerprint for identification.
Answer: Bright yellow lines. Sodium's characteristic D-lines appear as intense yellow doublet.
Answer: Emission or absorption of photons. Energy differences between levels determine photon wavelength emitted or absorbed.
Answer: Emission spectrum of hydrogen. Series of visible lines from electron transitions to n=2 level.
Answer: Continuous spectrum. Prism disperses white light into complete rainbow without gaps.
Answer: A spectrum of frequencies emitted by an atom or molecule. Shows specific wavelengths of light emitted when electrons drop to lower energy levels.
Answer: Visible region. Balmer series produces visible light from hydrogen atom transitions.
Answer: Absorption spectrum. Dark lines indicate absorption of specific wavelengths from continuous spectrum.
Answer: Emission shows bright lines; absorption shows dark lines. Emission adds light at specific wavelengths; absorption removes it.
Answer: Absorption of specific wavelengths by a substance. Electrons absorb photons of specific energies, removing those wavelengths from spectrum.
Answer: Ultraviolet emission spectrum of hydrogen. Series of UV lines from electron transitions to n=1 ground state.
Answer: Visible region. Balmer series produces visible light from hydrogen atom transitions.
Answer: Intensity of light at different wavelengths. Device separates and measures light intensity across electromagnetic spectrum.
Answer: Emission spectrum. Bright lines indicate emission of specific wavelengths against dark background.
Answer: Spectroscope. Optical instrument that disperses light into component wavelengths for observation.
Answer: Emission spectrum. Excited gas atoms emit characteristic colors when electrons drop energy levels.
Answer: Infrared emission spectrum of hydrogen. Series of IR lines from electron transitions to n=3 level.
Answer: The concentration of elements. Line intensity correlates with number of atoms present.
Answer: Emission shows bright lines; absorption shows dark lines. Emission adds light at specific wavelengths; absorption removes it.
Answer: To separate light into its component wavelengths. Grating diffracts light into distinct wavelengths for spectral analysis.
Answer: X-ray region. High-energy X-rays probe inner electron shells of atoms.
Answer: Absorption spectrum. Atmospheric gases absorb specific wavelengths from continuous sunlight.
Answer: Emission spectrum. Excited gas atoms emit characteristic colors when electrons drop energy levels.
Answer: Absorption spectrum. Dark absorption lines reveal elemental composition of stellar atmospheres.
Answer: To determine the composition of stars and planets. Spectral lines act as fingerprints identifying specific elements remotely.
Answer: X-ray region. High-energy X-rays probe inner electron shells of atoms.
Answer: Absorption spectrum. Cool gas atoms absorb specific wavelengths from continuous background light.
Answer: Ultraviolet emission spectrum of hydrogen. Series of UV lines from electron transitions to n=1 ground state.