Revealing giant planet interiors beneath the cloudy veil.
Where this comes from
- Record sourced from PubMed, PMID 32214104.
- Also identified by DOI 10.1038/s41467-020-15431-5 and PMC identifier 7096516.
- Licence recorded as CC BY.
- The licence permits redistribution, so the abstract is shown in full and the full text is available from the publisher.
Abstract
Observations from the Juno and Cassini missions provide essential constraints on the internal structures and compositions of Jupiter and Saturn, resulting in profound revisions of our understanding of the interior and atmospheres of Gas Giant planets. The next step to understand planetary origins in our Solar System requires a mission to their Ice Giant siblings, Uranus and Neptune.