![]() ![]() Ultraviolet spectroscopy tells us certain things about the universe, while visible and infrared spectroscopy tells us others. Hubble’s ultraviolet spectroscopy is one of its most powerful contributions to the astronomical community, and this capability will not be replaced or superseded by any mission in the near future. These data reveal important details about the makeup of atmospheres on exoplanets, the compositions of stars and nebulas, the motion of galaxies and more. Spectrographs collect data that tell scientists how much light comes out at each wavelength. Hubble is famous for the images captured by its cameras, but it often also relies on its spectrographs. Astronomers can analyze the pattern of light given off by an object like a star to figure out what elements it is made of. Each element emits a unique pattern of colors, or wavelengths, of visible light. Spectroscopy is as crucial as imaging to understanding the universe.Ībsorption spectra of carbon, oxygen, nitrogen, and iron. ![]() It records this spectrum, which allows scientists to analyze the light and discover properties of the material interacting with it. A spectrograph - sometimes called a spectroscope or spectrometer - breaks the light from a single material into its component colors the way a prism splits white light into a rainbow. It is the key to revealing details that cannot be uncovered through a picture. Spectroscopy is the study of the spectra produced when material interacts with or emits light. What Is Spectroscopy?Īn image tells us what something looks like a spectrum tells us what it is. By examining the intensity of light in each color, scientist can work backward to infer the properties of the material, such as an object’s size, temperature, motion, and composition, that touched the light along the way. This stamp is like a specific fingerprint for each element and molecule. ![]() When material interacts with light, properties of that material are stamped on the light.
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