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    Lander Instruments

    Introduction

    The ~100 kg Rosetta Lander will be the first spacecraft ever to make a soft landing on the surface of a comet nucleus. The Lander is provided by a European consortium under the leadership of the German Aerospace Research Institute (DLR). Other members of the consortium are ESA, CNES and institutes from Austria, Finland, France, Hungary, Ireland, Italy and the UK.

    The box-shaped Lander is carried in piggyback fashion on the side of the Orbiter until it arrives at Comet 67P/Churyumov-Gerasimenko. Once the Orbiter is aligned correctly, the ground station commands the Lander to self-eject from the main spacecraft and unfold its three legs, ready for a gentle touch down at the end of the ballistic descent. On landing, the legs damp out most of the kinetic energy to reduce the chance of bouncing, and they can rotate, lift or tilt to return the Lander to an upright position.

    Immediately after touchdown, a harpoon is fired to anchor the Lander to the ground and prevent it escaping from the comet's extremely weak gravity. The minimum mission target for scientific observations is one week, but surface operations may continue for many months.

    Lander Design

    The Lander structure consists of a baseplate, an instrument platform, and a polygonal sandwich construction, all made of carbon fibre. Some of the instruments and subsystems are beneath a hood which is covered with solar cells. An antenna transmits data from the surface to Earth via the Orbiter.

    The Lander Team

    The Lander project managers are:

    • Dr Stephan Ulamec - DLR, Köln Porz-Wahn, Germany
    • Dr Philippe Gaudon - CNES, Toulouse, France
    • Dr Sylvie Espinasse - Italian Space Agency, Matera, Italy

    Lead scientists for the Lander are:

    • Dr Hermann Böhnhardt - Max-Planck-Institut für Aeronomie, Lindau, Germany
    • Dr. Jean-Pierre Bibring - Institut d'Astrophysique Spatiale, Université Paris Sud, Orsay, France

    Rosetta Lander Instruments

    INSTRUMENT

    PURPOSE

    PRINCIPAL INVESTIGATOR

    APXS

    Alpha-p-X-ray spectrometer

    G. Klingelhöfer
    Johannes-Gutenberg Univ.,
    Mainz,
    Germany

    CIVA

    Panoramic and microscopic imaging system

    J-P. Bibring
    Institut d'Astrophysique Spatiale,
    Université Paris Sud, Orsay,
    France

    CONSERT

    Radio sounding, nucleus tomography

    W. Kofman
    Laboratoire de Planetologie,
    Grenoble,
    France

    COSAC

    Evolved gas analyser - elemental and molecular composition

    F. Goesmann
    Max-Planck-Institut für Aeronomie,
    Katlenburg-Lindau,
    Germany

    MODULUS Ptolemy

    Evolved gas analyser - isotopic composition

    I. Wright
    Open University,
    Milton Keynes,
    UK

    MUPUS

    Measurements of surface and subsurface properties

    T. Spohn
    German Aerospace Center (DLR),
    Cologne,
    Germany

    ROLIS

    Imaging

    S. Mottola
    DLR,
    Berlin,
    Germany

    ROMAP

    Magnetometer and plasma monitor

    H-U. Auster
    Technische Universität, Braunschweig,
    Germany
    I. Apathy
    KFKI,
    Budapest,
    Hungary

    SD2

    Drilling and sample retrieval

    A. Ercoli-Finzi
    Politecnico of Milan,
    Italy

    SESAME

    Surface electrical, acoustic and dust impact monitoring

    K. Seidensticker
    German Aerospace Center (DLR),
    Cologne,
    Germany
    I. Apathy
    KFKI,
    Budapest,
    Hungary

    Rosetta Lander Payload

    The Lander experiments will study the composition and structure of Comet 67P/Churyumov-Gerasimenko's nucleus.

    The instruments are designed to:

    • Measure the elemental, molecular, mineralogical, and isotopic composition of the comet's surface and subsurface material
    • Measure characteristics of the nucleus such as near-surface strength, density, texture, porosity, ice phases and thermal properties; texture measurements will include microscopic studies of individual grains

    The Lander also carries a Sampling Drilling and Distribution device (SD2), which will drill more than 20 cm into the surface, collect samples and deposit them in different ovens or deliver them for microscope inspection.

    APXS

    Last Update: 09 Apr 2010

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=31445
    • Related Articles
    • Introduction
    • APXS
    • CIVA
    • CONSERT
    • COSAC
    • MUPUS
    • Ptolemy
    • ROLIS
    • ROMAP
    • SD2
    • SESAME
    • Related Links
    • APXS
    • CIVA
    • CONSERT
    • COSAC
    • MODULUS
    • MUPUS
    • ROLIS
    • ROMAP
    • SD2
    • SESAME
    • Related Publications
    • Robot Technology for the Cometary Landing Mission Rosetta

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