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Showing 1–6 of 6 results
Advanced filters: Author: Maxwell L. Rudolph Clear advanced filters

  • Several moons in the outer Solar System have oceans encased beneath an ice shell. If the ice shell thins, ocean pressure decreases. Modelling shows that on Mimas, Enceladus, and Miranda, the ocean can boil. On larger bodies, instead, compressional forces form tectonic features.

    • Maxwell L. Rudolph
    • Michael Manga
    • Matthew Walker
    Research
    Nature Astronomy
    Volume: 10, P: 76-83

  • Cryptic degassing, whereby mantle-derived CO2 fluxes continue after surface eruptions slow, can explain prolonged warming that followed some large igneous province events, according to geodynamic and climate modelling.

    • Benjamin A. Black
    • Leif Karlstrom
    • Andrew Merdith
    ResearchOpen Access
    Nature Geoscience
    Volume: 17, P: 1162-1168

  • Enceladus’s tiger stripes at the south pole formed in cascade and spaced equally after the first fracture—probably Baghdad Sulcus—was created by the release of accumulated tensile stress, caused in turn by secular cooling.

    • Douglas J. Hemingway
    • Maxwell L. Rudolph
    • Michael Manga
    Research
    Nature Astronomy
    Volume: 4, P: 234-239

  • The size of the caldera formed when the surface collapses after a large volcanic eruption is thought to reflect the size of the evacuated magma chamber. Numerical modelling shows that magma stored in different parts of the chamber can be mobile or locked, so caldera size may only correspond to the volume of evacuated mobile magma.

    • Leif Karlstrom
    • Maxwell L. Rudolph
    • Michael Manga
    Research
    Nature Geoscience
    Volume: 5, P: 402-405