inhomogeneous interiors

Miguel and her team will develop new computational tools, in which they incorporate new knowledge that they gained from the Juno and Cassini missions. One of the main changes is that the interiors are actually inhomogeneous. That alters the way energy is transported, leading to higher temperatures, a different density and other interactions with the atmosphere. Miguel: ‘This will lead us into a new era in the study of giant planet interiors, one that will revolutionize the way of interpreting observations in exoplanets and learning about their origins.’

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two other grants

On top of this ERC Consolidator grant, Miguel received two other grants in the past few weeks. An NWO/NSO grant adds one extra PhD student to the effort of understanding the interior of gas giants, as part of the call for “Use of space infrastructure for Earth Observation and Planetary Research”. This PhD student will develop physical models to interpret data from the Cassini and Juno mission about this topic. An NWO M-grant was awarded to Miguel and her Leiden colleague Matthew Kenworthy to study the formation pathways for exoplanets far from their parent stars. This grant entails one PhD student and one postdoc.

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