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Showing 1–5 of 5 results
Advanced filters: Author: Panayotis Lavvas Clear advanced filters

  • Pluto’s haze could have a major icy component created by the condensation of organic molecules such as C4H2. This is different from Titan whose haze, despite a similar atmospheric composition, is mostly macromolecular aggregates. Triton’s haze, instead, should be dominated by ices, particularly C2H4.

    • P. Lavvas
    • E. Lellouch
    • G. R. Gladstone
    Research
    Nature Astronomy
    Volume: 5, P: 289-297

  • Analysis is presented that indicates that there is strong evidence that SiO or Mg, the major constituents of silicate condensates, must be present in gaseous form in the atmosphere of ultra-hot Jupiter WASP-178b.

    • Joshua D. Lothringer
    • David K. Sing
    • Autumn T. Winch
    Research
    Nature
    Volume: 604, P: 49-52

  • Observations of the gas-giant exoplanet WASP-121b reveal near-infrared emission lines of water, suggesting that the planet has a stratosphere—a layer in the upper atmosphere where temperature increases with altitude.

    • Thomas M. Evans
    • David K. Sing
    • Roxana Lupu
    Research
    Nature
    Volume: 548, P: 58-61