CORDIS Project
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This project investigates white dwarfs that host remnants of planetary systems, utilizing data from various astronomical surveys. It aims to analyze the composition of planetesimals and identify planets in close orbits, enhancing our understanding of planetary formation and evolution.
In the 25 years since the discovery of 51 Peg b, we went from not knowing if the Solar system is a fluke of Nature to realising that it is totally normal for stars to have planets.
The common fate of practically all planet hosts is that they will eventually evolve into white dwarfs, the Earth-sized embers that are the evolutionary end-points of most stars.
Many of the known planets will survive the post main-sequence evolution of their host stars - in the solar system, this includes Mars, and al…
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