Line broadening
from class: Intro to Astronomy Definition Line broadening is the phenomenon where spectral lines from astronomical objects are wider than expected. This occurs due to various factors such as thermal motion, rotation, and magnetic fields.
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Predict what's on your test 5 Must Know Facts For Your Next Test Thermal Doppler broadening results from the random motion of particles in a hot gas. Rotational broadening occurs when different parts of a galaxy rotate at different speeds, causing a spread in observed wavelengths. Turbulence within interstellar gas clouds also contributes to line broadening. Zeeman splitting causes line broadening when magnetic fields affect the energy levels of electrons in atoms. Line broadening can provide insights into the physical conditions and dynamics within galaxies. Review Questions What are the main causes of line broadening in astronomical observations? How does rotational motion within a galaxy contribute to line broadening? Explain how Zeeman splitting affects spectral lines. "Line broadening" also found in:
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