Absorption Spectra Simplified Revision Notes for Scottish Highers Physics
Revision notes with simplified explanations to understand Absorption Spectra quickly and effectively.
Learn about Spectra for your Scottish Highers Physics Exam. This Revision Note includes a summary of Spectra for easy recall in your Physics exam
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Absorption Spectra
Absorption Spectra
Introduction
Absorption spectra are patterns of light produced when photons pass through a gas, and certain photons are absorbed by atoms.
These spectra provide valuable information about the energy levels and composition of atoms and molecules.
Absorption Process
When photons of light pass through a gas, some photons have energy that matches the energy gaps between an atom's energy levels.
These specific photons are absorbed by the atoms, leading to the creation of absorption lines in the spectrum.
Absorption Spectra
Absorption spectra are characterised by dark lines or bands on a continuous spectrum.
The dark lines represent the specific wavelengths of light that have been absorbed by the gas.
The positions of these lines are indicative of the energy levels within the gas's atoms.
Relationship with Emission Spectra
The lines in the absorption spectra of an element are in the same positions as the lines in the emission spectra of that element.
This correspondence allows scientists to identify elements based on their unique absorption and emission patterns.
Observing Absorption in the Sun
While sunlight appears as a continuous spectrum, closer inspection using a spectroscope reveals dark, narrow lines known as Fraunhofer lines.
These lines are caused by specific frequencies of sunlight being absorbed by gases in the sun's upper atmosphere.
Absorption Spectra
Significance
Absorption spectra help scientists identify the chemical composition of substances by analysing the specific wavelengths of absorbed light.
These spectra play a crucial role in various fields, including astronomy, chemistry, and environmental science.
Summary
Absorption spectra result from the absorption of specific wavelengths of light by atoms or molecules.
Dark lines or bands on a continuous spectrum represent the absorbed wavelengths.
Absorption and emission spectra of the same element have corresponding lines.
Fraunhofer lines in sunlight are due to the absorption of specific frequencies by gases in the sun's atmosphere.
Absorption spectra aid in identifying the composition of substances and have diverse applications in scientific research.
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