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  • NEO Sample Return Mission

    Paper number

    IAC-07-A3.5.05

    Author

    Dr. Maria Antonietta Barucci, Observatoire de Paris, France

    Coauthor

    Prof. Marcello Fulchignoni, Observatoire de Paris, France

    Coauthor

    Dr. Stephan Ulamec, German Aerospace Center (DLR), Germany

    Year

    2007

    Abstract
    The NEOs are representative of the population of asteroids and dead comets  thought to be the remnants of the ancient planetesimals that accreted to form the planets.  The chemical investigation of NEOs having primitive characteristics is thus essential in the understanding the planet formation and evolution. They carry records of the solar system's birth/early phases and the geological evolution of small bodies in the interplanetary regions. Moreover, collisions of NEOs with Earth represent a serious hazard to life. For all these reasons the exploration and characterization of these objects are particularly interesting and urgent. 
    
    NEOs are interesting and highly accessible targets for scientific research and robotic exploration. 
    A new Sample Return mission is under study within a large European community and possible collaboration with the Japanese Space Agency JAXA in reply to the ESA Cosmic Vision AO. This type of mission appears clearly to have the potential to revolutionize our understanding of primitive materials. 
    
    
    The principal scientific objectives are to investigate on 1) the properties of the building blocks of the terrestrial planets; 2) the major events (e.g. agglomeration, heating, ..…) which  ruled  the history of planetesimals;   3)  the primitive asteroids which could contain presolar material unknown in meteoritic samples; 4) the organics in primitive materials; 5) the initial conditions and evolution history of the solar nebula; and 6) how they can shed light on the origin of molecules necessary for life.
    
    
    A mission with sample return to an appropriately chosen NEO  will help in understanding the chemical and biological aspect of the formation and the evolution of our and other planetary systems.  Moreover robotic missions to NEOs will be pathfinders for sample returns from high gravity bodies and later on for human missions that might use asteroid resources to facilitate human exploration and the development of space.
    
    Abstract document

    IAC-07-A3.5.05.pdf