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Rubidium-strontium relations in tranquillity base samples.

P M Hurley, W H Pinson

    Science (New York, N.Y.)
    |January 30, 1970
    PubMed
    Summary
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    Igneous rocks show distinct rubidium depletion. Strontium isotope ratios suggest this depletion occurred during early planetary formation, offering insights into terrestrial planet accretion.

    Area of Science:

    • Geochemistry
    • Planetary Science
    • Isotope Geology

    Background:

    • Igneous rocks are crucial for understanding planetary formation.
    • Rubidium (Rb) and Strontium (Sr) isotopes are key tracers in geological processes.

    Purpose of the Study:

    • To investigate the timing and origin of rubidium depletion in terrestrial igneous rocks.
    • To use strontium isotope ratios (87Sr/86Sr) to constrain early solar system processes.

    Main Methods:

    • Preliminary total rock analyses were performed on igneous rock samples.
    • Isotopic analysis of strontium-87 to strontium-86 ratios (87Sr/86Sr) was conducted.

    Main Results:

    • Two distinct groups of igneous rocks exhibited significantly different rubidium depletion levels.

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  • Strontium isotope ratios indicated that rubidium depletion occurred early in planetary history.
  • Conclusions:

    • The observed rubidium depletion in these igneous rocks is linked to the accretion phase of terrestrial planets.
    • This finding provides evidence for early geochemical differentiation processes during planet formation.