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URANUS

Selective enrichment of volatiles confirmed

Nature Astronomy volume 2, pages 364–365 (2018)Cite this article

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Hydrogen sulfide gas is detected above Uranus’s main cloud deck, confirming the prevalence of H2S ice particles as the main cloud component and a strongly unbalanced nitrogen/sulfur ratio in the planet's deep atmosphere.

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Fig. 1: Microwave spectrum and images of Uranus.

Panel a adapted from ref. 6, Elsevier and panel b courtesy of Mark Hofstadter and Bryan Butler.

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Authors and Affiliations

  1. Department of Astronomy and Department of Earth and Planetary Sciences, University of California, Berkeley, CA, USA

    Imke de Pater

  2. Faculty of Aerospace Engineering, Delft University of Technology, Delft, The Netherlands

    Imke de Pater

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  1. Imke de Pater
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Correspondence to Imke de Pater.

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de Pater, I. Selective enrichment of volatiles confirmed. Nat Astron 2, 364–365 (2018). https://doi.org/10.1038/s41550-018-0457-5

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