Wednesday, March 28, 2012

Akari

 2006-005A


ASTRO-F, the Infrared Imaging Surveyor (IRIS), has a 0.7m telescope cooled to do a 50-200 Mu m far infrared sky survey. It was named Akari ('light') after launch.

The spacecraft mass was 952 kg at launch. Its bus module supports cryostat and star trackers on a truss. The cryostat is 1.5m dia and 2.5m high, while the full satellite is 3.7m long, 1.8m dia, 5.7m span with 2 panels. The telescope has a SiC mirror, a focal plane cooled to 6K with FIR detectors cooled to 1.8K. The telescope beam was 21" at 60 microns.

Orbit 750 x 750 km x 97 deg.

The M-V-8 launch vehicle also carried CUTE-1.7 and a solar sail experiment 15.6m span, the Solar Sail Subpayload (SSP, soraseiru sabupeirodo). There were problems with the Sun sensor that delayed initial operations of Akari, and cover ejection was delayed to Apr 13. The ejectable telescope lid was 2.0m dia 0.4? high.

After initial checkout Akari began a sky scan which lasted 550 days and surveyed 94 percent of the celestial sphere. On 2007 Aug 26 the satellite used up its 170 liters of liquid helium and the 68-cm main telescope began to warm up from its 6-Kelvin operational temperature. In 2008 the Akari infrared observatory began a new phase of its mission. On the ground an international team began production of the source catalogs, which would supersede the 20-year-old IRAS point source catalog and serve as finding lists for new observatories like Herschel. Meanwhile, in space, Akari's shorter wavelength detectors were still operating well thanks to mechanical coolers which keep the focal plane at about 40 Kelvin. The Infrared Camera system developed by a team led by the University of Tokyo takes images in the traditional K, L and M bands as well as the MIR-S and MIR-L bands at 7-11 and 15-25 microns. Akari's other instrument system, the Far IR Surveyor, which was developed by Nagoya University, had four channels returning brightness and spectral information between 50 and 180 microns; it was retired after cryogen depletion.


ASTRO F 
 

DateTimeEventOrbit  

2006 Feb 21  2128:00  Launch by M-V-8  USC 
  T+1:15 St 1 sep, 50 km? 
  T+1:15 St 2 burn 
  T+2:31? St 2 burnout 150 km 
  T+3:06 Fairing sep
  T+3:20 St 2 sep 
  T+3:22 St 3 nozzle extend, spring jettison 
  T+3:25 St 3 burn 225 km?  
 2133 T+5:09 St 3 burnout 305 km  
  T+5:57 180 deg pitch begins 
  T+7:02 Pitch complete 
  Spinup? 
 2136 T+8:39 St 3 sep 
 2145 T+17:20 CUTE-1.7 sep from St 3. 
 2146 T+18:20 Sail deploy from St 3 
  T+1:50:00 Solar panels deployed 
   94.82 301 x 781 x 98.2  
  Orbit raise 
2006 Apr 13  0755  Cover jettison 
2007 Aug 26  0833  LHe depleted 
2011 May 24   Power supply malfunction 
2011 Jun   Science ops ended 
2011 Nov 9    98.8 693 x 706 x 98.3 
2011 Nov 11    97.71 596 x 701 x 98.3 
2011 Nov 24    96.08 441 x 700 x 98.3 
2011 Nov 24   end of ops
2012 Jan 17    96.05 439 x 698 x 98.3 

Payload:

  • 0.67m telescope

  • Cryostat with 170 liters of LHe

  • IRC IR cameras (3): NIR (K,L,M), 10 mu, 20 mu

    • IRC/NIR 10' FOV, 1.5" pixels

    • IRC/MIR-S, 256 x 256 Si:As at 7-11 mu

    • IRC/MIR-L, 256 x 256 SiAs at 15-25 mu, 10' FOV, 2"/pix

  • FIS, Far IR Surveyor, 50-200 mu.

    • 60-micron channel, 30"/pixel, 20x2

    • Wide-S channel, 50-100 mu for FTS

    • Wide-L channel, 100-200 mu with FTS

    • 170-micron channel, 50"/pix, 15x2

Friday, March 23, 2012

ROSAT

 1990-049A


The ROSAT (Rontgensatellit) X-ray observatory, launched in Jun 1990, was similar to NASA's Einstein observatory but with improved spatial and spectral resolution. It carried nested X-ray mirrors which focused radiation onto a PSPC (Position Sensitive Proportional Counter, similar to the Einstein IPC) and an HRI (High Resolution Imager, supplied by the US team that built the similar instrument on Einstein). A separate but coaligned extreme ultraviolet telescope, the Wide Field Camera (WFC), was built by the UK Leicester University group. The mission was operated by MPE in Germany in collaboration with NASA and the UK. The first six months of the mission saw an all sky survey by the PSPC instrument. At the end of the survey, a power failure caused the spacecraft to lose attitude control and accidentally point at the Sun, which severely damaged the PSPC-C instrument then in the focal plane and degraded the WFC. Fortunately a backup PSPC and the HRI were available to support continued operations in the pointed phase, which was opened to astronomers across the world.


ROSAT 
 

DateTimeEventOrbit  

1990 Jun 1  2147:59  Launch by Delta 6920  CC LC17A 
  T+0:55 SRM 1-6 burnout 
  T+1:00 SRM 7-9 burn 
  T+1:02 SRM 1-6 sep 
  T+1:56 SRM 7-9 burnout 
 2149:56  T+2:02 Final 3 Castor sep 
 2152:25  T+4:24 Thor cutoff 
 2152:30  T+4:32 Thor sep 
  T+4:38 Delta burn 
 2152  T+4:43 Fairing sep 
 2159:07  T+11:09 SECO-1 299 km 200? x 580? x 53  
 2226:00  T+38:02 Delta circ burn, 12s 
 2226:12 T+38:14 SECO-2 
 2231  T+43:00 Delta sep 577 x 584 x 53.0 
 2226T+1:39:10 SES-3 evasive 
  T+1:39:15 SECO-3 
 2237T+1:50:10 SES-4 depletion 
  T+1:50:31 SECO-4  454 x 557 x 52.51 
1991 Jan 25   Power failure
1991 Feb 10 Pointed phase 
1991 May 13   Y axis gyro failed 
1991 Aug 3   Sky survey completion patch 
1991 Aug 13   Completed sky survey 
1994 Jul   PSPC-B retired 
1998 Apr 28   Star tracker failed 
1998 Sep 20   Pointed at sun, HRI damaged 
1998 Oct 28end of ops 
1998 Dec 6   PSPC observations 
1998 Dec 18   PSPC observations ended
1999 Feb 12   Decommissioned 
2011 Oct 23  0150?  Reentered over Andaman Sea/China? 

Payload:

  • XRT 0.84m aperture Wolter I X-ray Telescope Zerodur/Au, 4 shells, f=2.4m

  • WFC 0.58m aperture XUV Wide Field Camera, Ni-Al/Au mirrors f=0.52m 0.04-0.2 keV (60-300A)

  • PSPC-C Position Sensitive Proportional Counter, 0.1-2.4 keV

  • PSPC-B Position Sensitive Proportional Counter.

  • HRI High Resolution Imager (SAO/Murray)

Sunday, March 18, 2012

Astra 1G

 1997-076A


HS-601HP satellite, launch by ILS Proton. It is colocated with the other Astra 1 satellites. The second HS-601HP, it features GaAs solar cells with 7 kW power. In Mar 1998 it took over digital TV broadcast traffic from Astra 1F.


Astra 1G 
 

DateTimeEventOrbit  

1997 Dec 2  2310  Launch by Proton 382-02/DM3 No. 2L  KB LC81 
 2312 Stage 1 sep T+2:07 
 2315 Stage 2 sep T+5:35 
 2315 Fairing sep T+5:44 
 2315 8S812 burn T+5:40 
 2139 8S812 shutdown T+9:38 
 2319  Stage 3 sep  180? x 200? x 51.6 
 2320  T+10:44 PB (perekhodnikiy blok) sep 
1997 Dec 3  0026? DM burn 1 
  MECO-1  200? x 36000? x 51.5? 
 0530? DM burn 2 
  MECO-2 
1997 Dec 3  0551  T+6:41 Blok-DM sep 
1997 Dec 3    841.70 10316 x 35972 x 12.4 
1997 Dec 5  1400? LAM-1 
1997 Dec 9    1399.32 34118 x 36008 x 0.3 
1997 Dec 11  0700? LAM-2 
1997 Dec 17    1436.13 35755 x 35818 x 0.0 GEO 24.6E+0.01W 
1997 Dec 30    1438.90 35014 x 36668 x 0.0 GEO 19.2E+0.7W 
1998 Feb 24    1436.12 35772 x 35802 x 0.0 GEO 19.2E 
1999 Oct 18    1436.02 35722 x 35848 x 0.0 GEO 19.2E 
2000 Jun 13    1436.06 35755 x 35816 x 0.1 GEO 19.2E 
2006 Oct 28    1436.16 35777 x 35797 x 0.1 GEO 19.2E 
2009 Mar 22    1436.11 35773 x 35800 x 0.0 GEO 19.2E 

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