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Also known as HELOS, X-ray Observatory satellite

The European X-ray Observatory Satellite (EXOSAT), originally named HELOS, was an X-ray telescope operational from May 1983 until April 1986 and in that time made 1780 observations in the X-ray band of most classes of astronomical object including active galactic nuclei, stellar coronae, cataclysmic variables, white dwarfs, X-ray binaries, clusters of galaxies, and supernova remnants.

Key facts

Spaceflight.name
EXOSAT
Spaceflight.image
exosat.jpg
Spaceflight.image_caption
EXOSAT
Spaceflight.mission_type
Astronomy
Spaceflight.operator
ESA
Spaceflight.COSPAR_ID
1983-051A
Spaceflight.SATCAT
14095
Spaceflight.mission_duration
3 years
Spaceflight.manufacturer
MBB
Spaceflight.power
165.0 watts
Spaceflight.launch_date
 UTC
Spaceflight.launch_rocket
Delta 3914 D169
Spaceflight.launch_site
Vandenberg SLC-2W
Spaceflight.orbit_epoch
26 May 1983, 11:18:00 UTC
Spaceflight.orbit_reference
Geocentric
Spaceflight.orbit_regime
Low Earth
Spaceflight.orbit_inclination
72.5 degrees
Spaceflight.orbit_eccentricity
0.93428

via Wikipedia infobox

Wikidata facts

Image
Exosat.jpg
Show 2 more facts
UTC date of spacecraft launch
1983-05-26
Commons category
Exosat
Sources (1)

via Wikidata · CC0

~5 min read

Article

5 sections
Contents
  • History of Exosat
  • Satellite operations
  • Observational results
  • References
  • External links

The European X-ray Observatory Satellite (EXOSAT), originally named HELOS, was an X-ray telescope operational from May 1983 until April 1986 and in that time made 1780 observations in the X-ray band of most classes of astronomical object including active galactic nuclei, stellar coronae, cataclysmic variables, white dwarfs, X-ray binaries, clusters of galaxies, and supernova remnants.

This European Space Agency (ESA) satellite for direct-pointing and lunar-occultation observation of X-ray sources beyond the Solar System was launched into a highly eccentric orbit (apogee 200,000 km, perigee 500 km) almost perpendicular to that of the Moon on 26 May 1983. The instrumentation includes two low-energy imaging telescopes (LEIT) with Wolter I X-ray optics (for the 0.04–2 keV energy range), a medium-energy experiment using Ar/CO2 and Xe/CO2 detectors (for 1.5–50 keV), a Xe/He gas scintillation spectrometer (GSPC) (covering 2–80 keV), and a reprogrammable onboard data-processing computer. Exosat was capable of observing an object (in the direct-pointing mode) for up to 80 hours and of locating sources to within at least 10 arcsec with the LEIT and about 2 arcsec with GSPC.

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