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Detection and Characterization Methods of Exoplanets

Title
Detection and Characterization Methods of Exoplanets
Type
Chapter or Part of a Book
Year
2020
Authors
N.C. Santos
(Author)
FCUP
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Barros, SC
(Author)
FCUP
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Demangeon, OD
(Author)
Other
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Faria, JP
(Author)
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Other information
Authenticus ID: P-00T-D1Z
Abstract (EN): <p>Is the Solar System unique, or are planets ubiquitous in the universe? The answer to this long-standing question implies the understanding of planet formation, but perhaps more relevant, the observational assessment of the existence of other worlds and their frequency in the galaxy.</p> <p>The detection of planets orbiting other suns has always been a challenging task. Fortunately, technological progress together with significant development in data reduction and analysis processes allowed astronomers to finally succeed. The methods used so far are mostly based on indirect approaches, able to detect the influence of the planets on the stellar motion (dynamical methods) or the planet¿s shadow as it crosses the stellar disk (transit method). For a growing number of favorable cases, direct imaging has also been successful. The combination of different methods also allowed probing planet interiors, composition, temperature, atmospheres, and orbital architecture. Overall, one can confidently state that planets are common around solar-type stars, low mass planets being the most frequent among them.</p> <p>Despite all the progress, the discovery and characterization of temperate Earth-like worlds, similar to the Earth in both mass and composition and thus potential islands of life in the universe, is still a challenging task. Their low amplitude signals are difficult to detect and are often submerged by the <italic>noise</italic> produced by different instrumentation sources and astrophysical processes. However, the dawn of a new generation of ground and space-based instruments and missions is promising a new era in this domain.</p>
Language: English
Type (Professor's evaluation): Scientific
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