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Alpha Particle X-Ray Spectrometer (APXS) On-board Chandrayaan-2 Rover -- Pragyan

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arxiv 1910.09232 v1 pith:MAWJ43YZ submitted 2019-10-21 astro-ph.IM astro-ph.EPphysics.ins-det

classification astro-ph.IMastro-ph.EPphysics.ins-det
keywords apxsx-rayalphadetectorenergyparticlex-rayschandrayaan-2
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Alpha Particle X-ray Spectrometer (APXS) is one of the two scientific experiments on Chandrayaan-2 rover named as Pragyan. The primary scientific objective of APXS is to determine the elemental composition of the lunar surface in the surrounding regions of the landing site. This will be achieved by employing the technique of X-ray fluorescence spectroscopy using in-situ excitation source Cm-244 emitting both X-rays and alpha particles. These radiations excite characteristic X-rays of the elements by the processes of particle induced X-ray emission (PIXE) and X-ray fluorescence (XRF). The characteristic X-rays are detected by the state-of-the-art X-ray detector known as Silicon Drift Detector (SDD), which provides high energy resolution as well as high efficiency in the energy range of 1 to 25 keV. This enables APXS to detect all major rock forming elements such as, Na, Mg, Al, Si, Ca, Ti and Fe. The Flight Model (FM) of the APXS payload has been completed and tested for various instrument parameters. The APXS provides energy resolution of 135 eV at 5.9 keV for the detector operating temperature of about -35 deg C. The design details and the performance measurement of APXS are presented in this paper.

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  1. Cross-Calibration of Chandrayaan-2 XSM with INSPIRESat-1 DAXSS and GOES-16 XRS

    astro-ph.SR 2026-08 conditional novelty 6.0 of 10

    Chandrayaan-2 XSM's beryllium window is effectively 25 μm thick, not 8 μm; the corrected calibration brings its spectra and fluxes into ~10-25% agreement with DAXSS and GOES-16.

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