Suzaku (satellite) explained

Suzaku (ASTRO-EII)
Names List:ASTRO-EII
Mission Type:Astronomy
Operator:JAXANASA
Cospar Id:2005-025A
Satcat:28773
Mission Duration:2 years (planned)
10 years 1 month 23 days (achieved)
Spacecraft Type:ASTRO
Spacecraft Bus:ASTRO-E
Manufacturer:Toshiba[1]
Launch Mass: [2]
Dimensions:2 metres x 5 metres
Power:500 watts
Launch Date:10 July 2005, 03:30:00 UTC
Launch Rocket:M-V # 6
Launch Site:Uchinoura Space Center,
Uchinoura, Kagoshima
Deactivated:2 September 2015
Decay Date:No earlier than 2020 [3]
Orbit Reference:Geocentric orbit
Orbit Regime:Low Earth orbit
Orbit Inclination:31°
Orbit Period:96 minutes
Apsis:gee
Instruments:X-ray Spectrometer-2 (XRS-2)
X-ray Imaging Spectrometer (XIS)
Hard X-ray Detector (HXD)
Insignia Size:200px
ASTRO-E
Mission Type:Astronomy
Operator:Institute of Space and Astronautical Science (ISAS) / NASA
Mission Duration:Failed to orbit
Spacecraft Type:ASTRO
Spacecraft Bus:ASTRO-E
Manufacturer:Toshiba
Launch Mass:1600 kg
Dimensions:2 metres x 5 metres
Power:500 watts
Launch Date:10 February 2000, 01:30:00 UTC
Launch Rocket:M-V # 4
Launch Site:Kagoshima Space Center
Decay Date:Failed to orbit
Orbit Reference:Geocentric orbit (planned)
Orbit Regime:Low Earth orbit
Orbit Inclination:31.0°
Orbit Period:96.0 minutes
Apsis:gee
Instruments:X-ray Spectrometer (XRS)
X-ray Imaging Spectrometer (XIS)
Hard X-ray Detector (HXD)
X-ray Telescope (XRT)
Insignia Size:200px

Suzaku (formerly ASTRO-EII) was an X-ray astronomy satellite developed jointly by the Institute of Space and Aeronautical Science at JAXA and NASA's Goddard Space Flight Center to probe high-energy X-ray sources, such as supernova explosions, black holes and galactic clusters. It was launched on 10 July 2005 aboard the M-V launch vehicle on the M-V-6 mission. After its successful launch, the satellite was renamed Suzaku after the mythical Vermilion bird of the South.[4]

Just weeks after launch, on 29 July 2005, the first of a series of cooling system malfunctions occurred. These ultimately caused the entire reservoir of liquid helium to boil off into space by 8 August 2005. This effectively shut down the X-ray Spectrometer-2 (XRS-2), which was the spacecraft's primary instrument. The two other instruments, the X-ray Imaging Spectrometer (XIS) and the Hard X-ray Detector (HXD), were unaffected by the malfunction. As a result, another XRS was integrated into the Hitomi X-ray satellite, launched in 2016, which also was lost weeks after launch. A Hitomi successor, XRISM, launched on 7 September 2023, with an X-ray Spectrometer (Resolve) onboard as the primary instrument.

On 26 August 2015, JAXA announced that communications with Suzaku had been intermittent since 1 June 2015 and that the resumption of scientific operations would take a lot of work to accomplish, given the spacecraft's condition.[5] Mission operators decided to complete the mission imminently, as Suzaku had exceeded its design lifespan by eight years at this point. The mission came to an end on 2 September 2015, when JAXA commanded the radio transmitters on Suzaku to switch themselves off.[3] [6]

Spacecraft instruments

Suzaku carried high spectroscopic resolution, very wide energy band instruments for detecting signals ranging from soft X-rays up to gamma-rays (0.3–600 keV). High-resolution spectroscopy and wide-band are essential factors in physically investigating high-energy astronomical phenomena, such as black holes and supernovas. One such feature, the K-line (x-ray), may be key to more direct imaging of black holes.

Results

Suzaku discovered "fossil" light from a supernova remnant.[8]

ASTRO-E

Suzaku was a replacement for ASTRO-E, which was lost in a launch failure. The M-V launch vehicle on the M-V-4 mission launched on 10 February 2000 at 01:30:00 UTC. It experienced a failure of 1st stage engine nozzle 42 seconds into the launch, causing control system breakdown and underperformance.[9] [10] Later stages could not compensate for underperformance, leaving payload in 250miles x 50miles orbit and subsequent reentry and crashed with its payload into the Indian Ocean.[11] [12]

Further reading

External links

Notes and References

  1. Web site: Encyclopedia Astronautica – Toshiba. https://web.archive.org/web/20101129191524/http://astronautix.com/mfrs/toshiba.htm. dead. 29 November 2010. astronautix.com. 9 September 2015.
  2. The X-Ray Observatory Suzaku. Kazuhisa Mitsuda. Astronomical Society of Japan. 59. SP1. S1–S7. 25 January 2007 . 4 October 2010. astro-ph/0608100. 2007PASJ...59....1T. 10.1093/pasj/59.1.1. 17354373.
  3. Web site: Stephen Clark. Japanese X-ray observatory completes decade-long mission. Spaceflight Now. 4 September 2015. 9 September 2015.
  4. http://www.isas.jaxa.jp/j/snews/2005/0710_suzaku.shtml すざく(朱雀、Suzaku)命名の理由
  5. Web site: X-ray Astronomy Satellite "Suzaku" Completes Scientific Mission. National Research and Development Agency (JAXA). 26 August 2015. 9 September 2015.
  6. Web site: Suzaku Mission Declared Complete. Goddard Space Flight Center. NASA. 28 August 2015. 4 September 2015.
  7. Tadayuki Takahashi. Hard X-ray Detector (HXD) on Board Suzaku. Astronomical Society of Japan. 59. SP1. S23–S33. 25 January 2007. 10.1093/pasj/59.sp1.S23. 4 October 2010 .
  8. http://www.nasa.gov/mission_pages/astro-e2/news/fossil-fireballs.html Suzaku Finds "Fossil" Fireballs from Supernovae 12.30.09
  9. Web site: History | ISAS . 2024-01-02 . History . en.
  10. Web site: 1 How did M-V-4 fly? . 2024-01-02 . www.isas.jaxa.jp.
  11. Web site: Ray . Justin . February 10, 2000 . Spaceflight Now Breaking News Astro-E believed lost following botched launch . 2024-01-02 . spaceflightnow.com.
  12. Web site: Kevin Boyce. ASTRO-E Launch. NASA Goddard Space Flight Center. 2005. 2 March 2010.