INSTRUMENTS USED IN CHANDRAYAAN 1 MISSION

The scientific payload has a total mass of 90 kg and contains six Indian instruments and six foreign instruments.

• The Terrain Mapping Camera (TMC) has 5 m resolution and a 40 km swath in the panchromatic band and will be used to produce a high-resolution map of the Moon.

• The Hyper Spectral Imager (HySI) will perform mineralogical mapping in the 400-900 nm band with a spectral resolution of 15 nm and a spatial resolution of 80 m.

• The Lunar Laser Ranging Instrument (LLRI) will determine the surface topography.

• An X-ray fluorescence spectrometer C1XS covering 1- 10 keV with a ground resolution of 25 km and a Solar X-ray Monitor (XSM) to detect solar flux in the 1–10 keV range. C1XS will be used to map the abundance of Mg, Al, Si, Ca, Ti, and Fe at the surface,nd the XSM will monitor the solar flux. This payload is a collaboration between Rutherford Appleton laboratory, U.K, ESA and ISRO.

• A High Energy X-ray/gamma ray spectrometer (HEX) for 30- 200 keV measurements with ground resolution of 40 km, the HEX will measure U, Th, ²¹⁰Pb, ²²²Rn degassing, and other radioactive elements
• Moon Impact probe(MIP) developed by ISRO is in turn a small satellite that will be carried by Chandrayaan-1 and will be ejected once it reaches 100 km orbit around moon, to impact on the moon. MIP carries three more instruments namely, a high resolution mass spectrometer, an S-Band altimeter and a video camera.

• Among foreign payloads, The Sub-keV Atom Reflecting Analyzer (SARA) from ESA will map composition using low energy neutral atoms sputtered from the surface

• The Moon Mineralogy Mapper (M3) from Brown University and JPL (funded by NASA) is an imaging spectrometer designed to map the surface mineral composition.

• A near infrared spectrometer (SIR-2) from ESA, built at the Max PlancNK Institute for Solar System Research, Polish Academy of Science and University of Bergen, will also map the mineral composition using an infrared grating spectrometer. The instrument will be similar to that of the Smart-1 SIR.

• S-band miniSAR from the APL at the Johns Hopkins University (funded by NASA) is the active SAR system to map lunar polar ice. The instrument will transmit right polarized radiation with a frequency of 2.5 GHz and will monitor the scattered left and right polarized radiation. The Fresnel reflectivity and the cicular polarization ratio (CPR) are the key parameters deduced from this measurments. Ice shows the Coherent Backscatter Opposition Effect which results in an enhancement of refelections and CPR. With the data the water content of the moon polar region can estimated.^[5]

• Radiation Dose Monitor (RADOM-7) from Bulgaria is to map the radiation environment around the moon.