CORDIS Project
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This project focuses on studying debris discs around nearby stars, which consist of asteroids, comets, and dust. By analyzing these discs, the project aims to gain insights into the planetary systems of these stars and improve the understanding of planet formation processes.
This proposal concerns the debris discs of nearby stars; ie, discs of asteroids, comets and dust.
Such dust can be imaged, providing clues to the underlying planetary system.
Debris images have already predicted planets later confirmed in direct imaging.
Most debris lies in cold outer (~100AU) regions of planetary systems, but a growing number of stars have hot dust in regions where terrestrial planets are expected (few AU).
This proposal aims learn about the planetary systems of nearby stars th…
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