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A bimodal distribution of haze in Pluto’s atmosphere

Author

Listed:
  • Siteng Fan

    (California Institute of Technology
    LMD/IPSL, Sorbonne Université, PSL Research University, École Normale Supérieure, École Polytechnique, CNRS)

  • Peter Gao

    (Carnegie Institution for Science)

  • Xi Zhang

    (University of California Santa Cruz)

  • Danica J. Adams

    (California Institute of Technology)

  • Nicholas W. Kutsop

    (Cornell University)

  • Carver J. Bierson

    (University of California Santa Cruz
    Arizona State University)

  • Chao Liu

    (California Institute of Technology
    Nanjing University of Information Science & Technology)

  • Jiani Yang

    (California Institute of Technology)

  • Leslie A. Young

    (Southwest Research Institute)

  • Andrew F. Cheng

    (Johns Hopkins University Applied Physics Laboratory)

  • Yuk L. Yung

    (California Institute of Technology
    California Institute of Technology)

Abstract

Pluto, Titan, and Triton make up a unique class of solar system bodies, with icy surfaces and chemically reducing atmospheres rich in organic photochemistry and haze formation. Hazes play important roles in these atmospheres, with physical and chemical processes highly dependent on particle sizes, but the haze size distribution in reducing atmospheres is currently poorly understood. Here we report observational evidence that Pluto’s haze particles are bimodally distributed, which successfully reproduces the full phase scattering observations from New Horizons. Combined with previous simulations of Titan’s haze, this result suggests that haze particles in reducing atmospheres undergo rapid shape change near pressure levels ~0.5 Pa and favors a photochemical rather than a dynamical origin for the formation of Titan’s detached haze. It also demonstrates that both oxidizing and reducing atmospheres can produce multi-modal hazes, and encourages reanalysis of observations of hazes on Titan and Triton.

Suggested Citation

  • Siteng Fan & Peter Gao & Xi Zhang & Danica J. Adams & Nicholas W. Kutsop & Carver J. Bierson & Chao Liu & Jiani Yang & Leslie A. Young & Andrew F. Cheng & Yuk L. Yung, 2022. "A bimodal distribution of haze in Pluto’s atmosphere," Nature Communications, Nature, vol. 13(1), pages 1-11, December.
  • Handle: RePEc:nat:natcom:v:13:y:2022:i:1:d:10.1038_s41467-021-27811-6
    DOI: 10.1038/s41467-021-27811-6
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    References listed on IDEAS

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    1. David K. Sing & Jonathan J. Fortney & Nikolay Nikolov & Hannah R. Wakeford & Tiffany Kataria & Thomas M. Evans & Suzanne Aigrain & Gilda E. Ballester & Adam S. Burrows & Drake Deming & Jean-Michel Dés, 2016. "A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion," Nature, Nature, vol. 529(7584), pages 59-62, January.
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