SETI public: ESA Deep Space Vessel Pulsar Navigation Study

From: LARRY KLAES (ljk4_at_msn.com)
Date: Tue Jun 28 2005 - 19:31:47 PDT

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    http://www.esa.int/gsp/ACT/mission_analysis/pulsar.htm

    Pulsar Navigation Study

    Millisecond pulsars offer the most reliable timing standard known to us.
    Hence it appears logical to investigate if navigation in deepspace can
    benefit from using this timing information. The possibility of using pulsar
    signals for the positioning of spacecraft was reviewed in the Ariadna study
    Feasibility study for a spacecraft navigation system relying on pulsar
    timing information conducted by the Universitat Politècnica de Catalunya and
    Universitat de Barcelona.

    Earth-based navigation of deepspace satellites has several drawbacks: The
    navigational accuracy is high only along the line-of-sight (this is still
    true even if ?VLBI is taken into consideration). During Solar conjunctions
    no precision navigation is possible. A remedy could come from two possible
    approaches. The first one would be a positioning system based on a network
    of deepspace satellites. This solution would be extremely costly. The second
    possibility would be autonomous navigation. In order to enable
    high-precision autonomous navigation the spacecraft position needs to be
    tied to a precisely known natural reference frame. The best currently known
    reference frame is set up by the positions of remote millisecond pulsars.

    While exhibiting an extremely high timing stability the pulsar signals are
    very weak compared to a conventional radio-tracking signal. Hence the
    question arises if pulsar signals can effectively be employed for navigation
    when the constraints that a deepspace mission poses to the mass and power
    consumption of the navigation hardware are taken into account. The study
    treated convincingly the characterisation of suitable astrophysical sources
    and derived from this the minimal hardware requirements for a positioning
    system. This was done for both, radio and x-ray signals. The results are
    however not clear cut: A positioning accuracy of 1,000 km is attainable with
    a moderate antenna size (10 m2) and a signal integration time of the order
    of an hour. However simultaneous observation of several pulsars with
    separate antennas seems desirable for a reduced integration time or an
    enhanced accuracy. However, this seems to require prohibitively heavy
    hardware.

    The study report can be downloaded here:

    J. Sala, A. Urruela, X. Villares, R. Estalella and J. Paredes: Feasibility
    study for a spacecraft navigation system relying on pulsar timing
    information.

    Page last updated by Andreas Rathke 6-Oct-2004


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