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Featured
Planet Formation Through Gravitational Instabilities

"It is now widely accepted that planets form in discs around young stars, with the most widely accepted planet formation scenario being a bottom-up process typically referred to as “core accretion.” The basic process involves a core growing through the accumulation of solids and, if it gets massive enough while there is still gas present in the disc, undergoing a runaway gas accretion phase to form a Jupiter-like gas giant...." – By Ken Rice
Featured
The Orbital Architecture of Exoplanetary Systems

"The great diversity of extrasolar planetary systems has challenged our understanding of how planets form. During the formation process their orbits are modified while the protoplanetary disk is present. After its dispersal orbits may also be modified as a result of mutual gravitational interactions leading to their currently observed configurations in the longer term...." – By John C. B. Papaloizou
What's New to the OREs
In January 2023, 66 new full articles and 10 revised articles across 23 disciplines have been published on the Oxford Research Encyclopedias platform. Explore the recently published articles now.
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On April 20, the Oxford Research Encyclopedia of Global Public Health will be available via subscription and perpetual access. After a successful free period during development, the OREs provide in-depth overviews of the major areas of research and will continue to grow with the field over time. If you're a librarian, explore Subscriber Services to learn how to provide access to the OREs for your institution. If you're not a librarian, you can recommend the OREs to your librarian here.

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