The XRISM satellite

The X-Ray Imaging and Spectroscopy Mission (XRISM), previously known as the X-ray Astronomy Recovery Mission (XARM), is an X-ray astronomy satellite collaboration between the Japanese Aerospace Exploration Agency (ISAS/JAXA), NASA and the European Space Agency (ESA). The satellite will be launched on an H-IIA rocket to a low earth orbit with a planned altitude of 550 km and an orbital inclination of 31 degrees. Launch is anticipated early to mid 2023.

There are two primary instruments, Resolve (a Soft X-ray Spectrometer) and Xtend (Soft X-ray Imager). The spectrometer is cryogenically cooled with liquid helium, and the helium supply is anticipated to last for three years, though the mission may be extended thereafter with mechanical cooling. The mission is intended to recover most of the science capability of Hitomi in the 0.3-12 keV energy range, lost during a very early mission mishap.

Mission Characteristics

* Lifetime : Three years from launch (planned); can be extended
* Energy Range : 0.3–12 keV
* Special Features : “hyperspectral“ X-ray microcalorimeter instrument.
* Payload :
XRISM has two X-ray telescopes with a focal lenght of 5.6 m each paired with a detector, Resolve and Xend.
  • Resolve. The unit consists a 6 pixel x 6 pixel X-ray calorimeter spectrometer. Resolve is directly analogous to the SXS instrument on Hitomi, using many of the spare component. There are 35 active pixels and one inactive corner pixel. The calorieter is enclosed in a dewar cooling the detector at 50mK, with a liquid helium tank anticipated to last three year and thereafter the instrument is cooled via mechanic cooling at reduced sensitivity.
    • Energy range : 0.3-12 keV
    • Effective area : 210 cm2 at 6 keV; 160 cm2 at 1 keV
    • Field of view and Angular resolution : 3 x 3 arcmin2 and < 1.3 arcmin
    • Energy Resolution: < 7 eV at 6 keV
    Additional components of the Resolve detector include:
    • A gate valve placed on top of the dewar to protect during initial operation and remove in normal operation.
    • A six filter wheel, mounted at 90 cm from the spectrometer, to use in normal operation modes. The filters are : two empty positions (i.e. no filter), a radioactive 55Fe calibration source, a molybdenum neutral density (or “grey”) filter to attenuate X-ray brightness, and beryllium and polyimide-aluminium filters to exclude X-rays outside specific energy ranges.
    • A Modulation X-ray Source (MXS) mounted below the filter wheel. When turned on, they illuminate the entire detector and are used for calibration. It consists of 4 LEDs operating in pair with targets composed of Cu/Cr and Al/Mg.

  • XTend. The unit consists of 4 CCDs in 2 x 2 configuration. Each CCD is an array of 640 x 640 pixels. It is directly analogous to the SXI on Hitomi.
    • Energy range : 0.4-12 keV
    • Effective area : 360 cm2 at 6 keV
    • Angolar resolution : < 1.3 arcmin
    • Field of View : 38 x 38 arcmin2
    • Energy Resolution: < 200 eV at 6 keV
* Science Highlights:
XRISM has many of the same science goals as Hitomi. These include:

  • Insight on galaxy and cluster evolution
  • Diffuse gas in local environments
  • The physics and dynamics of cosmic plasmas
  • The formation and evolution of compact objects, including ultraluminous sources and magnetic cataclysmic variables
* Archive: HEASARC hosts XRISM data, products, and catalogs.
[XRISM at GSFC] [XRISM at JAXA; English]

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Last modified: Wednesday, 23-Feb-2022 19:10:43 EST