Spectral lines are specific wavelengths of light that are emitted or absorbed by atoms or molecules. They serve as a unique "fingerprint" for each element, allowing scientists to identify the composition of celestial objects and analyze their properties.
Imagine you have a set of colored markers, each with its own unique color. Just like how each marker has a distinct color, each element has its own set of spectral lines that can be used to identify it.
Emission Spectrum: The pattern of spectral lines produced when an atom or molecule emits light.
Absorption Spectrum: The pattern of dark lines observed when an atom or molecule absorbs specific wavelengths of light.
Balmer Series: A series of spectral lines in the visible region of the electromagnetic spectrum that corresponds to transitions in hydrogen atoms.
Study guides for the entire semester
200k practice questions
Glossary of 50k key terms - memorize important vocab
© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.