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The viking seismic experiment.

D L Anderson, F K Duennebier, G V Latham

    Science (New York, N.Y.)
    |December 11, 1976
    PubMed
    Summary
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    A seismometer on Mars is recording wind noise but has not yet detected any marsquakes. Early data suggests Martian seismic activity remains unknown, requiring further observation over the next two years.

    Area of Science:

    • Planetary Science
    • Seismology
    • Mars Exploration

    Background:

    • The study of seismic activity on Mars is crucial for understanding its internal structure and geological evolution.
    • Previous missions have provided limited seismic data, leaving the planet's seismicity largely uncharacterized.

    Purpose of the Study:

    • To deploy and operate a three-axis short-period seismometer on the Martian surface.
    • To establish a baseline for seismic noise and detect potential marsquakes in the Utopia Planitia region.

    Main Methods:

    • Operation of a three-axis short-period seismometer.
    • Data collection and analysis of seismic signals and environmental factors like wind.
    • Monitoring seismic background noise over an extended period.

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    Main Results:

    • The seismometer is operational in Utopia Planitia, Mars.
    • A strong correlation between background seismic noise and wind gusts has been observed.
    • No seismic events (marsquakes) have been detected in the initial 60 days of operation.

    Conclusions:

    • Current data is insufficient to determine the seismicity of Mars.
    • The instrument's sensitivity to environmental factors like wind is confirmed.
    • Continued data collection for at least two years is necessary to draw meaningful conclusions about Martian seismic activity.