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Multiwavelength Astronomy

Objects at Different Wavelengths

Type of RadiationWavelength (nm)Temperature (K)Typical Sources
gamma-rays <0.01 >108 no sources; some gamma-rays produced in nuclear reactions
X-rays 0.01-20 106-108 gas in clusters of galaxies; supernova remnants; solar corona
UV 20-400 104-106 supernova remnants; very hot stars
Visible 400-700 103-104 stars
Infrared 103-106 10-103 cool clouds of dust and gas; planets; satellites
Radio >106 <10 no objects this cold; emission produced by electrons moving in magnetic fields

Imagine the Universe is a service of the High Energy Astrophysics Science Archive Research Center (HEASARC), Dr. Nicholas White (Director), within the Laboratory for High Energy Astrophysics at NASA's Goddard Space Flight Center.

The Imagine Team
Project Leader: Dr. Jim Lochner
All material on this site has been created and updated between 1997-2004.

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