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Concepts in astronomyGustav KirchhoffObservational astronomyScattering, absorption and radiative transfer (optics)

Spectroscopy

Adapted from Wikipedia · Discoverer experience

A scientific image showing the spectrum of the Sun, displaying different wavelengths of light for educational purposes.

Spectroscopy is the field of study that measures and interprets electromagnetic spectra as it interacts with matter. In simpler terms, it is the precise study of color as we know it, but expanded from just visible light to all types of energy waves.

A prism separates white light by dispersing it into its component colors, which can then be studied using spectroscopy.

Spectroscopy is a crucial tool in many areas of science, such as astronomy, chemistry, materials science, and physics. It helps scientists discover the composition and structure of matter, from tiny atoms and molecular structures to objects very far away in space over astronomical distances.

Historically, spectroscopy began with studying how gases absorb different colors of visible light when passed through a prism. Today, it is used in many new ways, including biomedical spectroscopy for analyzing tissue and creating medical imaging. Even matter waves and acoustic waves can be studied using spectroscopy, and recently, scientists have linked gravitational waves to special patterns observed by the Laser Interferometer Gravitational-Wave Observatory (LIGO).

Introduction

High resolution spectrum of the Sun, showing the discrete line pattern created by elements in the stellar atmosphere

Spectroscopy is a science that studies how different kinds of matter interact with light. Scientists use special tools like spectrometers and spectrophotometers to measure how light changes when it passes through or bounces off objects. This helps them learn about the structure and properties of materials, from tiny atoms to huge stars.

The idea of spectroscopy started a long time ago when Isaac Newton showed that white light could be split into a rainbow of colors using a prism. Today, spectroscopy looks at all kinds of light, not just the colors we can see. By studying how light is absorbed or emitted by different elements, scientists can identify what those elements are and learn more about their properties. This is very useful in fields like astronomy, where telescopes with spectrographs help us understand stars and planets, and in chemistry, where it helps identify and measure different substances.

Theory

The basic idea of spectroscopy is that light is made of different wavelengths, and each wavelength has a different frequency. Every element has a unique pattern of light it emits or absorbs, which helps scientists study matter at very small scales. This unique pattern, called a spectral signature, is important in many areas of science.

Scientists use tools like absorption spectrophotometers to measure how much light a sample absorbs. They also study how systems, like pendulums or atoms, respond to energy. For example, when light of the right energy hits an atom, it can make an electron jump to a higher energy level. This helps scientists learn about the structure and properties of different materials using various types of spectroscopy.

Classification of methods

Spectroscopy is a broad field with many different ways to study how matter interacts with energy. These methods can be grouped by the type of energy used, how the energy interacts with the material, and what kind of material is being studied.

A huge diffraction grating at the heart of the ultra-precise ESPRESSO spectrograph

Type of radiative energy

Spectroscopy can use different kinds of energy to study materials. The most common is electromagnetic radiation, which includes light of many colors and wavelengths like microwave, terahertz, infrared, near-infrared, ultraviolet-visible, X-ray, and gamma rays. Other types of energy include particles like electrons and neutrons, which act like waves, and pressure waves used in acoustic spectroscopy.

Nature of the interaction

How the energy interacts with the material also helps classify spectroscopy. Absorption spectroscopy measures how much energy a material takes in. Emission spectroscopy looks at energy released by the material. Elastic scattering and reflection study how energy bounces off the material. Other methods include impedance spectroscopy, which measures how a material slows down energy, and inelastic scattering, where energy changes wavelength after hitting the material.

Type of material

Spectroscopy can also be grouped by the type of material studied. Electronic spectroscopy looks at electrons moving between energy levels. Vibronic spectroscopy studies molecules vibrating, and rotational spectroscopy looks at molecules spinning. These methods help scientists identify and learn about the makeup of materials, from single atoms to complex molecules and crystals.

Other types

Spectroscopy has many different types, each used for specific purposes.

Some types, like acoustic resonance spectroscopy, study how materials respond to sound waves. Others, such as Raman spectroscopy, help scientists identify molecules by how they vibrate. There are also techniques like gamma spectroscopy that look at high-energy light from space or radioactive materials, and thermal infrared spectroscopy that measures heat given off by objects to learn about their chemical makeup. Each type of spectroscopy offers unique ways to explore and understand the world around us.

Applications

UVES is a high-resolution spectrograph on the Very Large Telescope.

Spectroscopy is a powerful tool used in many scientific fields like medicine, physics, chemistry, and astronomy. It helps scientists identify different materials and understand how they work by studying how they absorb and emit light.

Some important uses of spectroscopy include studying the sun and faraway galaxies, exploring space, checking food for harmful substances, analyzing blood for toxins, and even determining the speed of distant objects. It is also used in hospitals to analyze breathing gases and in research to study the building blocks of life.

History

Main article: History of spectroscopy

The history of spectroscopy began with Isaac Newton’s experiments with light in the 1660s and 1670s. Newton showed that white sunlight is actually made up of all the colors of the rainbow by passing it through a prism. Later, in 1802, William Hyde Wollaston improved the tools for studying light and noticed dark gaps in the colors. Around the same time, Joseph von Fraunhofer discovered hundreds of these dark lines in the Sun’s light, now called Fraunhofer lines.

These patterns of light and dark lines helped scientists understand the building blocks of matter. The study of these lines played an important role in the development of quantum mechanics, especially in explaining the behavior of hydrogen atoms.

Hobbyist

Spectroscopy has become a popular activity for hobbyists and educators, thanks to the maker movement. Using simple materials like CD or DVD diffraction gratings, smartphones, and 3D-printed parts, people can build their own spectrometers. These DIY tools help users learn about how light interacts with different materials. While they may not be as precise as professional equipment, they offer a great way to explore science and contribute to citizen science projects.

Images

The Crab Nebula is the remnant of a star that exploded long ago, creating beautiful glowing clouds of gas and dust in space.
A scientific diagram showing the structure of nitrous oxide using colored balls and sticks.
A 3D model showing the structure of ethanol, a type of chemical compound.
A 3D model showing the structure of Buckminsterfullerene, a molecule made of carbon atoms.
A stunning view of Earth rising over the Moon, captured by astronauts on the Apollo 8 mission in 1968.
An artist's depiction of HE 1523-0901, one of the oldest known stars in our galaxy, located about 7500 light years from Earth.

This article is a child-friendly adaptation of the Wikipedia article on Spectroscopy, available under CC BY-SA 4.0.

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