The water-ice on the moon, specially at lunar pole Identification of chemical end members of lunar high land rocks Chemical stratigraphy of lunar crust by remote sensing of central upland of large lunar craters, South Pole Aitken Region (SPAR) etc.,
where interior material may be expected To map the height variation of the lunar surface features along the satellite track Observation of X-ray spectrum greater than 10 keV and stereographic coverage of most of the moon’s surface with 5 m resolution, to provide new insights in understanding the moon’s origin and evolution.
