EXOSAT
Sign in to saveAlso 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 sectionsContents
- 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.