HEAO 1

HEAO 1 (High-Energy Astronomy Observatory 1) was the first in a series of three satellite observatories designed to continue the X-ray and gamma-ray studies initiated by ANS, OAO 3, UK 5, the OSO series, the SAS series, and the gamma-ray burst discoveries of the Vela satellites. 

This mission was specifically designed to map and survey the celestial sphere for X-ray and gamma-ray sources in the energy range of 150 eV to 10 MeV, to establish the size and precise location of X-ray sources to determine the contribution of discrete sources to the X-ray background, and to measure time variations of X-ray sources. 

This observatory consisted of a common spacecraft equipment module (SEM), which carried most of the spacecraft operational equipment, and a unique experiment module (EM), which carried some elements of the electrical distribution system in addition to the four experiments: Large Area X-ray Survey, Cosmic X-ray Background Experiment, Scanning Modulation Collimator, and Hard X-ray and Low Energy Gamma-Ray Experiment. 

Continuous celestial scans were made perpendicular to the satellite-sun vector during the initial phase of the mission. Scan rate was 0.03 rpm. The entire celestial sphere would be scanned in 6 months. When passing over the South Atlantic Anomaly (SAA) of the inner Van Allen Belt, high-voltage supplies were turned off or reduced to prevent damage caused by saturation effects. 

The six-sided HEAO 1 was 5.68 m high and 2.67 2.67 m in diameter, and weighed 2552 kg, which included 1220-kg experiments. Downlink telemetry was at a data rate of 6.5 kb/s for real-time data and 128 kb/s for either of the two tape recorder systems. The mission lifetime was August 12, 1977, to January 9, 1979.

HEAO 1 featured following instruments:

• Large Area Sky Survey experiment (LASS) - covered the energy range 0.25 to 25.0 keV;
• Cosmic X-ray Experiment (CXE) - designed to study the large scale structure of the galaxy and the universe, yielding high quality spatial and spectral data over the energy range 2-60 keV;
• Modulation Collimator (MC) - designed to measure positions of X-ray sources with sufficient precision to identify optical and/or radio counterparts;
• Hard X-Ray / Low Energy Gamma Ray Experiment.
  

Last update: 27.09.2009
Contact: gunter.krebs@skyrocket.de
© Gunter Dirk Krebs