Menu
Home Explore People Places Arts History Plants & Animals Science Life & Culture Technology
On this page
Suzaku (satellite)
Decommissioned Japanese X-ray astronomy satellite

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.

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. 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.

Related Image Collections Add Image
Profiles
1 Image
We don't have any YouTube videos related to Suzaku (satellite) yet.
We don't have any PDF documents related to Suzaku (satellite) yet.
We don't have any Books related to Suzaku (satellite) yet.
We don't have any archived web articles related to Suzaku (satellite) yet.

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.

  • X-ray Telescope (XRT)
  • X-ray Spectrometer-2 (XRS-2)
  • X-ray Imaging Spectrometer (XIS)
  • Hard X-ray Detector (HXD)
    • Uses Gadolinium Silicate crystal (GSO), Gd2SiO5(Ce)5
    • Uses Bismuth Germanate crystal (BGO), Bi4Ge3O126

Results

Suzaku discovered "fossil" light from a supernova remnant.7

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.89 Later stages could not compensate for underperformance, leaving payload in 250 miles (400 km) x 50 miles (80 km) orbit and subsequent reentry and crashed with its payload into the Indian Ocean.1011

  • Spaceflight portal

Further reading

References

  1. すざく（朱雀、Suzaku）命名の理由 2005 JAXA http://www.isas.jaxa.jp/j/snews/2005/0710_suzaku.shtml ↩

  2. "X-ray Astronomy Satellite "Suzaku" Completes Scientific Mission". National Research and Development Agency (JAXA). 26 August 2015. Retrieved 9 September 2015. http://global.jaxa.jp/press/2015/08/20150826_suzaku.html ↩

  3. Stephen Clark (4 September 2015). "Japanese X-ray observatory completes decade-long mission". Spaceflight Now. Retrieved 9 September 2015. http://spaceflightnow.com/2015/09/04/japanese-x-ray-observatory-completes-decade-long-mission/ ↩

  4. "Suzaku Mission Declared Complete". Goddard Space Flight Center. NASA. 28 August 2015. Retrieved 4 September 2015. This article incorporates text from this source, which is in the public domain. https://heasarc.gsfc.nasa.gov/docs/suzaku/news/endofmission.html ↩

  5. Tadayuki Takahashi (25 January 2007). "Hard X-ray Detector (HXD) on Board Suzaku". Astronomical Society of Japan. 59 (SP1): S23 – S33. doi:10.1093/pasj/59.sp1.S23. Retrieved 4 October 2010. http://pasj.asj.or.jp/v59/sp1/59s103/59s103-frame.html ↩

  6. Tadayuki Takahashi (25 January 2007). "Hard X-ray Detector (HXD) on Board Suzaku". Astronomical Society of Japan. 59 (SP1): S23 – S33. doi:10.1093/pasj/59.sp1.S23. Retrieved 4 October 2010. http://pasj.asj.or.jp/v59/sp1/59s103/59s103-frame.html ↩

  7. Suzaku Finds "Fossil" Fireballs from Supernovae 12.30.09 This article incorporates text from this source, which is in the public domain. https://www.nasa.gov/mission_pages/astro-e2/news/fossil-fireballs.html ↩

  8. "History ｜ ISAS". History. Retrieved 2 January 2024. https://www.isas.jaxa.jp/en/about/history/ ↩

  9. "1 How did M-V-4 fly?". www.isas.jaxa.jp. Retrieved 2 January 2024. https://www.isas.jaxa.jp/docs/sat/astro-e/how.html ↩

  10. Ray, Justin (10 February 2000). "Spaceflight Now | Breaking News | Astro-E believed lost following botched launch". spaceflightnow.com. Retrieved 2 January 2024. https://spaceflightnow.com/m5/astroe/000210failure.html ↩

  11. Kevin Boyce (2005). "ASTRO-E Launch". NASA Goddard Space Flight Center. Retrieved 2 March 2010. This article incorporates text from this source, which is in the public domain. https://astrophysics.gsfc.nasa.gov/xrays/programs/astroe/ph/grp-launch.html ↩