Detection of exoplanets: exploiting each property of light
Up to now and probably for still a long time, the only support of information used to detect exoplanets has been the analysis of light, either visible or infrared. In the vast majority of cases it is the light from a star and not the light from the planet itself which is used, because the huge contr...
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Académie des sciences
2023-08-01
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Series: | Comptes Rendus. Physique |
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Online Access: | https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.135/ |
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author | Rouan, Daniel Lagrange, Anne-Marie |
author_facet | Rouan, Daniel Lagrange, Anne-Marie |
author_sort | Rouan, Daniel |
collection | DOAJ |
description | Up to now and probably for still a long time, the only support of information used to detect exoplanets has been the analysis of light, either visible or infrared. In the vast majority of cases it is the light from a star and not the light from the planet itself which is used, because the huge contrast in brightness between the star and a planet orbiting it as well as the extremely short angular distance between them makes direct imaging a real challenge. It is then a subtle effect detected on the starlight that in general indicates the planet’s presence and provides information on some of its characteristics: mass, radius, distance to the star, temperature, etc. As an introduction to the different contributions appearing in this volume, this article proposes a kind of brief review of the various methods imagined by astronomers to exploit one of the properties of the light to succeed in detecting and characterizing exoplanets. We’ll show that even direct detection became a reality and contributes to the more than 5000 exoplanets detected today. |
format | Article |
id | doaj-art-c71585ded3f04cf5bae661ffbaea0d41 |
institution | Kabale University |
issn | 1878-1535 |
language | English |
publishDate | 2023-08-01 |
publisher | Académie des sciences |
record_format | Article |
series | Comptes Rendus. Physique |
spelling | doaj-art-c71585ded3f04cf5bae661ffbaea0d412025-02-07T13:52:55ZengAcadémie des sciencesComptes Rendus. Physique1878-15352023-08-0124S2112510.5802/crphys.13510.5802/crphys.135Detection of exoplanets: exploiting each property of lightRouan, Daniel0Lagrange, Anne-Marie1LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris-Cité, 5 place Jules Janssen, 92195 Meudon, FranceLESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris-Cité, 5 place Jules Janssen, 92195 Meudon, FranceUp to now and probably for still a long time, the only support of information used to detect exoplanets has been the analysis of light, either visible or infrared. In the vast majority of cases it is the light from a star and not the light from the planet itself which is used, because the huge contrast in brightness between the star and a planet orbiting it as well as the extremely short angular distance between them makes direct imaging a real challenge. It is then a subtle effect detected on the starlight that in general indicates the planet’s presence and provides information on some of its characteristics: mass, radius, distance to the star, temperature, etc. As an introduction to the different contributions appearing in this volume, this article proposes a kind of brief review of the various methods imagined by astronomers to exploit one of the properties of the light to succeed in detecting and characterizing exoplanets. We’ll show that even direct detection became a reality and contributes to the more than 5000 exoplanets detected today.https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.135/TransitDirect imagingVelocimetryCoronagraphyInterferometryAstrometryGravitational lensing |
spellingShingle | Rouan, Daniel Lagrange, Anne-Marie Detection of exoplanets: exploiting each property of light Comptes Rendus. Physique Transit Direct imaging Velocimetry Coronagraphy Interferometry Astrometry Gravitational lensing |
title | Detection of exoplanets: exploiting each property of light |
title_full | Detection of exoplanets: exploiting each property of light |
title_fullStr | Detection of exoplanets: exploiting each property of light |
title_full_unstemmed | Detection of exoplanets: exploiting each property of light |
title_short | Detection of exoplanets: exploiting each property of light |
title_sort | detection of exoplanets exploiting each property of light |
topic | Transit Direct imaging Velocimetry Coronagraphy Interferometry Astrometry Gravitational lensing |
url | https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.135/ |
work_keys_str_mv | AT rouandaniel detectionofexoplanetsexploitingeachpropertyoflight AT lagrangeannemarie detectionofexoplanetsexploitingeachpropertyoflight |