All About the Extreme Ultraviolet Explorer

The Extreme Ultraviolet Explorer (EUVE) is a NASA-funded astronomy mission operating in the relatively unexplored extreme ultraviolet (70-760 Å) band. The science payload, which has been designed and built at the Space Sciences Laboratory at the University of California, Berkeley, under the direction of Dr. Roger F. Malina, consists of three grazing incidence scanning telescopes and an extreme ultraviolet (EUV) spectrometer/deep survey instrument. The science payload is attached to a Multi-Mission Modular spacecraft.

The EUVE mission, which launched on June 7, 1992 on a Delta II rocket from Cape Canaveral, is the culmination of nearly thirty years of effort at the University of California at Berkeley to create the field of EUV Astronomy. EUVE opens up this last unexplored spectral window in astrophysics.

The first six months of the mission were dedicated to mapping the EUV sky with the scanning telescopes. The mission is now in the Guest Observer phase.

Science Goals

EUVE Mission Phases


For additional information on the technical aspects of the EUVE Mission (scanner design, bandpass of telescopes, astronomical objects detected to date, etc), please review the following resources:

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