Peering through Jupiter’s clouds with radio spectral imaging

Author:

de Pater Imke123,Sault R. J.4,Butler Bryan5,DeBoer David1,Wong Michael H.1

Affiliation:

1. Department of Astronomy, 501 Campbell Hall, University of California, Berkeley, CA 94720, USA.

2. Faculty of Aerospace Engineering, Delft University of Technology, 2629 HS Delft, Netherlands.

3. SRON Netherlands Institute for Space Research, 3584 CA Utrecht, Netherlands.

4. School of Physics, University of Melbourne, Victoria 3010, Australia.

5. National Radio Astronomy Observatory, Socorro, NM 87801, USA.

Abstract

A radio view into Jupiter's atmosphere Jupiter's atmosphere is a complex system of belts, layers, storms, and cloud systems. de Pater et al. used Earth-bound radio observations to peer beneath its surface. Previous radio studies have been limited to average properties at each latitude, but the new observations allow a full two-dimensional view. This can be related to features (such as storms) seen in visible or infrared images. The results aid our understanding of gas giant atmospheres and will provide important context for the Juno spacecraft that arrives at Jupiter in July 2016. Science , this issue p. 1198

Funder

NASA Planetary Astronomy (PAST)

NASA Outer Planets Research Program

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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