Thursday, January 14, 2016

Suzaku

 2005-025A


Astro-EII (named Suzaku after launch) was the replacement for Astro E. It had 4 XRT-I telescopes with 0.4m dia, f=4.75m, 175 shells, and one XRT-S with 0.4m dia, 4.50m, 168 shells, plus the HXD hard X-ray detector with 0.6 deg FOV. The telescopes are like those on Astro-E, but precollimator sections were added to reduce background, and the XRS detector was improved.

The XIS CCDs each have a 19 arcminute field of view. The long XRT has the XRS microcalorimeter in a 1.5m long dewar, giving an energy resolution of 6 eV with a 2.9 arcmin field of view in a 6 x 6 pixel array. The dewar is a 4-stage refrigerator with a mechanical cooler, a solid neon shell, a liquid helium stage, and an ADR (adiabatic demagnetizing refrigerator), putting the XRS focal plane at only 1.5 mK.

Although XMM-RGS and Chandra-LETG are more sensitive and higher resolution than XRS at soft energies, the reverse was to be true at 2-10 keV energies where XRS was designed to surpass other missions in sensitivity and resolution. The XRTs have 2 arcminute resolution, so the point source sensitivity would be worse than missions like Chandra.

Soon after launch a design error manifested. After several days observation of the internal calibration source, vented helium built up inside the spacecraft body and a thermal short developed between the cryogenic dewar and the structure, boiling off the cryogen and warming up the focal plane. Once gain there would be no astronomical observations with a spaceborne X-ray calorimeter. As a result of miscommunication between the various mission teams, it had not been realized that a design change in the spacecraft compared to the original Astro-E prevented gas vented from the instrument reaching the outside.

Suzaku nevertheless had a successful career using the XIS and HXD instruments which provided a broader spectral range than other then-operating missions.

ASTRO E-II was a stepped octagonal cylinder, 1700 kg mass, size 4.5m long (launch), 6.5m long (EOB extended), diameter 2.1 x 1.9m with 5.4m solar array span.


ASTRO-E2 
 

DateTimeEventOrbit  

2005 Jul 10  0330  Launch by M-V-6  USC  
  T+1:15 St 2 burn  
  T+3:06 Fairing sep
  T+3:20 St 2 sep 
  T+3:22 St 3 nozzle extend 
  T+3:25 St 3 burn (102s?) 
 0335 T+5:07? St 3 burnout 
  T+5:47 Begin attitude turn  
  T+7:02 End attitude turn 
 0351 T+21:47 Stage 3 sep  295 x 538 x 31.4 
   550 x 550 x 31 
  T+2d Spindown 
  T+4d Solar panel deploy 
  T+5d optical bench extends 
2005 Jul 17   DV1  304 x 537 x 31.4 
2005 Jul 17  2200?  DV2  356 x 536 x 31.4  
2005 Jul 22  0020?  DV3  96.05 565 x 573 x 31.4 
  XRS switchon 
2005 Aug 8   XRS thermal failure 
2006 Nov 9   XIS2 failed 
2015 Jun 1  Power issues, intermittent comm  
2015 Aug 26   end of ops
2015 Sep 2   transmitters off 

Payload:

  • XRS-2 Xray Microcalorimeter, 0.1-10 keV

  • XIS-2 X-ray CCD camera, 0.1-10 keV

  • HXD-2/PIN Hard X-ray Detector, PIN diode detector, 10-50 keV

  • HXD-2/GSO Hard X-ray Detector, Collimator/scintillator, 30-700 keV

  • XRT-2 X-ray telescope for XRS

  • XRT-2 X-ray telescopes (4) for XIS

  • EOB Extensible Optical Bench

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