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Showing 1–5 of 5 results
Advanced filters: Author: M. R. Zapatero Osorio Clear advanced filters

  • Silane, which is a precursor to the sandy surfaces of rocky planets and dusty clouds on gas giants, is seen directly in another world—a low-metallicity brown dwarf in which oxidation is slow and gas mixing is fast.

    • Jacqueline K. Faherty
    • Aaron M. Meisner
    • Eduardo L. Martin
    Research
    Nature
    Volume: 645, P: 62-66

  • Ultra-hot Jupiters provide a unique window into atmospheric processes and this in-depth study enables integrated global snapshots of the atmosphere and more accurate identification of flow patterns, thus allowing for better comparison to models.

    • Julia V. Seidel
    • Bibiana Prinoth
    • Francesco A. Pepe
    Research
    Nature
    Volume: 639, P: 902-908

  • Absorption lines of iron in the dayside atmosphere of an ultrahot giant exoplanet disappear after travelling across the nightside, showing that the iron has condensed during its travel.

    • David Ehrenreich
    • Christophe Lovis
    • Filippo Zerbi
    Research
    Nature
    Volume: 580, P: 597-601

  • The 20-million-year-old, solar-type star V1298 Tau hosts a multiplanet system. The two outermost planets, gas giants with masses of 0.64 and 1.16 Jupiter masses, respectively, defy current formation models as their mass–radius relationship should be reached much later in the stages of planetary evolution.

    • A. Suárez Mascareño
    • M. Damasso
    • M. Mallonn
    Research
    Nature Astronomy
    Volume: 6, P: 232-240