''Suzaku'' (formerly ASTRO-EII) was an
X-ray astronomy
X-ray astronomy is an observational branch of astronomy which deals with the study of X-ray observation and detection from astronomical objects. X-radiation is absorbed by the Earth's atmosphere, so instruments to detect X-rays must be taken to ...
satellite developed jointly by the
Institute of Space and Aeronautical Science at
JAXA
The is the Japanese national air and space agency. Through the merger of three previously independent organizations, JAXA was formed on 1 October 2003. JAXA is responsible for research, technology development and launch of satellites into o ...
and
NASA
The National Aeronautics and Space Administration (NASA ) is an independent agencies of the United States government, independent agency of the federal government of the United States, US federal government responsible for the United States ...
's
Goddard Space Flight Center to probe high-energy X-ray sources, such as
supernova explosions,
black hole
A black hole is a massive, compact astronomical object so dense that its gravity prevents anything from escaping, even light. Albert Einstein's theory of general relativity predicts that a sufficiently compact mass will form a black hole. Th ...
s 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.
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 hole
A black hole is a massive, compact astronomical object so dense that its gravity prevents anything from escaping, even light. Albert Einstein's theory of general relativity predicts that a sufficiently compact mass will form a black hole. Th ...
s and
supernova
A supernova (: supernovae or supernovas) is a powerful and luminous explosion of a star. A supernova occurs during the last stellar evolution, evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion ...
s. 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), Gd
2SiO
5(Ce)
** Uses
Bismuth
Bismuth is a chemical element; it has symbol Bi and atomic number 83. It is a post-transition metal and one of the pnictogens, with chemical properties resembling its lighter group 15 siblings arsenic and antimony. Elemental bismuth occurs nat ...
Germanate crystal (BGO), Bi
4Ge
3O
12[
File:ASTRO-EII XRT.JPG, X-ray Telescope (XRT)
File:Suzaku HXD.jpg, Hard X-ray Detector (HXD)
File:Suzaku XIS.jpg, X-ray Imaging Spectrometer (XIS)
File:Suzaku XRS.jpg, X-ray Spectrometer (XRS)
]
Results
Suzaku discovered "fossil" light from a supernova remnant.
ASTRO-E
''Suzaku'' was a replacement for ASTRO-E, which was lost in a launch failure. The M-V launch vehicle
A launch vehicle is typically a rocket-powered vehicle designed to carry a payload (a crewed spacecraft or satellites) from Earth's surface or lower atmosphere to outer space. The most common form is the ballistic missile-shaped multistage ...
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. Later stages could not compensate for underperformance, leaving payload in x orbit and subsequent reentry and crashed with its payload into the Indian Ocean
The Indian Ocean is the third-largest of the world's five oceanic divisions, covering or approximately 20% of the water area of Earth#Surface, Earth's surface. It is bounded by Asia to the north, Africa to the west and Australia (continent), ...
.[ ]
References
Further reading
Special Issue: First Results from Suzaku
Publications of the Astronomical Society of Japan. Vol. 59, No. SP1 30 January 2007. Retrieved 4 October 2010.
External links
(JAXA)
JAXA/ISAS ''Suzaku'' (ASTRO-EII) mission overview
JAXA report presentation of failure analysis of XRS
(in Japanese)
*
NASA/GSFC ''Suzaku'' Learning Center
{{Orbital launches in 2005
X-ray telescopes
Space telescopes
Satellites of Japan
Spacecraft launched in 2005