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  • The Heat-Flow and Physical Properties Probe (HP3 ) Mars Instrument

    Paper number

    IAC-14,A3,P,28,x26541

    Coauthor

    Mr. Riccardo Nadalini, Active Space Technologies, Germany

    Coauthor

    Dr. Matthew Dalton, Active Space Technologies, Germany

    Coauthor

    Mr. Andrei Cacovean, Active Space Technologies, Germany

    Coauthor

    Prof. Tilman Spohn, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany

    Coauthor

    Ms. Judit Jänchen, DLR (German Aerospace Center), Germany

    Coauthor

    Dr. Anko Börner, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany

    Coauthor

    Dr. Matthias Grott, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany

    Coauthor

    Mr. Olaf Krömer, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany

    Coauthor

    Mr. Christian Krause, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany

    Coauthor

    Dr. Harald Michaelis, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Germany

    Coauthor

    Mr. Emanuel Kopp, DLR (German Aerospace Center), Germany

    Year

    2014

    Abstract
    InSight is a Discovery-class mission to study the geophysical state of the interior of Mars scheduled for launch in 2016. The main goals of the mission are the determination of the size, physical state, and composition of the core, the thickness of the crust, and the thermal state of the martian interior. HP3 is an instrument aboard the InSight lander, designed and built by the German aerospace agency, Deutsches Zentrum für Luft- und Raumfahrt (DLR), to determine the geothermal heat flux by penetrating down into the surface of Mars to at least 3 meters. Heat flow is a major constraint on models of the current state of Mars’ interior and is key to understanding the evolution of terrestrial planets in general. HP3 consists of an electro-mechanical hammering mechanism, the Mole, that penetrates below the martian surface and contains resistive heaters and thermometers, for the active measurement of the thermal conductivity of the soil, as well as tilt sensors to determine its trajectory through the ground. It pulls behind it the Science Tether, with highly calibrated, equally spaced, temperature sensors that monitor the thermal gradient in the soil over the greater part of a Martian year. A Radiometer mounted on the Lander will contribute to the temperature monitoring by providing the temperature of the surface surrounding the lander.
    Abstract document

    IAC-14,A3,P,28,x26541.brief.pdf

    Manuscript document

    IAC-14,A3,P,28,x26541.pdf (🔒 authorized access only).

    To get the manuscript, please contact IAF Secretariat.