Hinotori (satellite) explained

Hinotori
Names List:Astro-A
Mission Type:Astronomy
Operator:ISAS
Cospar Id:1981-017A
Satcat:12307
Launch Date: UTC[1]
Launch Rocket:Mu-3S
Launch Site:Mu Pad, Kagoshima
Launch Contractor:ISAS
Orbit Reference:Geocentric
Orbit Regime:Low Earth
Orbit Eccentricity:0.00395
Orbit Inclination:31.3 degrees
Orbit Period:96.2 minutes
Orbit Epoch:21 February 1981, 04:30:00 UTC[2]
Apsis:gee

Hinotori, also known as ASTRO-A before launch, was a Japanese X-ray astronomy satellite. It was developed by the Institute of Space and Astronautical Science (ISAS). Its primary mission was to study of solar flares emanating from the Sun during the solar maximum.[3] It was launched successfully on February 21, 1981 using a M-3S rocket as the vehicle from Uchinoura Space Center (known at the time as Kagoshima). After the start of normal operation, it observed a large solar flare and, a month later, succeeded in observing 41 flares of many sizes from the Sun. It reentered the atmosphere on July 11, 1991.[4] The name Hinotori is the Japanese word for Phoenix.

Instruments

Highlights

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Notes and References

  1. JAXA, "Catalogue of ISAS Missions" ; retrieved 2014-12-23.
  2. Web site: NASA - NSSDCA - Spacecraft - Trajectory Details. nssdc.gsfc.nasa.gov. 2018-05-01.
  3. Gunter's Space Page, "Astro A (Hinotori)"; retrieved 2014-12-23.
  4. ISAS, "Solar Observation HINOTORI (ASTRO-A)"; retrieved 2014-12-23.