Imagine the Universe!

Apollo-Soyuz Test Project

Apollo-Soyuz docking


* Mission Overview

The Apollo-Soyuz mission occurred in July, 1975. In addition to the manned mission objectives of international space cooperation, testing universal docking systems, etc., Apollo-Soyuz carried a number of scientific instruments.

* Instrumentation

The U.S. portion of the mission carried a proportional counter system sensitive to 0.18-0.28 and 0.6-10.0 keV X-rays. The total effective area was 0.1 m2, and there was a 4.5 degree FWHM circular field of view.

* Science

Results from this experiment included the discovery of soft X-ray emission from the supernova remnant MSH 14-63 and of rapid pulsations (0.716 s) from the binary SMC X-1. Due to the (comparatively) short duration of the Apollo-Soyuz mission, little other science of note was done with the proportional counter system. In addition, the detector had a moderately high background level that steadily increased through the duration of the mission until almost no X-ray sources were discernible. The cause of the background problems remains unknown.


[Gallery] (http://heasarc.gsfc.nasa.gov/docs/heasarc/missions/images/apollosoyuz_images.html) [Publications] (http://heasarc.gsfc.nasa.gov/docs/heasarc/missions/biblio/apollosoyuz_biblio.html)
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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