Connecting Planetary Composition with Formation: a New Paradigm Emerges

TL;DR

This paper reviews recent observational and theoretical advances in exoplanet and protoplanetary disk studies, proposing a new paradigm where MHD disk winds drive planet formation and migration, linking disk physics to exoplanet properties.

Contribution

It introduces a novel paradigm emphasizing MHD disk winds over turbulence in disk evolution and planet formation, supported by recent observations and simulations.

Findings

MHD disk winds dominate disk evolution processes.

Disk chemistry and structure influence exoplanet atmospheres.

Observations support the new dynamic planet formation paradigm.

Abstract

Extensive ground and space based surveys have now characterized the properties of thousands of exoplanets; their radii, masses, orbits around their host stars, and the beginnings of accurate measurements of the chemical compositions of their atmospheres and cores. How are these properties linked to their formation in physically and chemically evolving protoplanetary disks wherein they accrete pebbles, planetesimals, and gas as they undergo migration? To address this challenge, our review assembles a large and varied body of exoplanet observations as well as recent Atacama Large Millimeter Array (ALMA) and James Webb Space Telescope (JWST) observations of disk structure, chemistry, kinematics, and winds. The latest advances in theory and MHD simulations that bear on these issues are also reviewed and compared with the observations. Taken together, this review argues that a new dynamic paradigm for planet formation is emerging wherein MHD disk winds and not disk turbulence play a central role in disk evolution and planet formation including: angular momentum transport, gap and ring formation. disk astrochemistry, and planet formation and migration. These processes leave their mark on the resulting atmospheric composition, radii, and orbital characteristics of exoplanet populations, offering the possibility of future observational tests.