Imaging low-mass planets within the habitable zone of α Centauri
Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around nearby stars.
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2021
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oai:doaj.org-article:34b7ac7a6b0c49a6be4c1b54f64995932021-12-02T14:10:56ZImaging low-mass planets within the habitable zone of α Centauri10.1038/s41467-021-21176-62041-1723https://doaj.org/article/34b7ac7a6b0c49a6be4c1b54f64995932021-02-01T00:00:00Zhttps://doi.org/10.1038/s41467-021-21176-6https://doaj.org/toc/2041-1723Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around nearby stars.K. WagnerA. BoehleP. PathakM. KasperR. ArsenaultG. JakobU. KäuflS. LeverattoA.-L. MaireE. PantinR. SiebenmorgenG. ZinsO. AbsilN. AgeorgesD. ApaiA. CarlottiÉ. ChoquetC. DelacroixK. DohlenP. DuhouxP. ForsbergE. FuentesecaS. GutrufO. GuyonE. HubyD. KampfM. KarlssonP. KervellaJ.-P. KirchbauerP. KluparJ. KolbD. MawetM. N’DiayeG. Orban de XivryS. P. QuanzA. ReutlingerG. RuaneM. RiquelmeC. SoenkeM. SterzikA. ViganT. de ZeeuwNature PortfolioarticleScienceQENNature Communications, Vol 12, Iss 1, Pp 1-7 (2021) |
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Science Q K. Wagner A. Boehle P. Pathak M. Kasper R. Arsenault G. Jakob U. Käufl S. Leveratto A.-L. Maire E. Pantin R. Siebenmorgen G. Zins O. Absil N. Ageorges D. Apai A. Carlotti É. Choquet C. Delacroix K. Dohlen P. Duhoux P. Forsberg E. Fuenteseca S. Gutruf O. Guyon E. Huby D. Kampf M. Karlsson P. Kervella J.-P. Kirchbauer P. Klupar J. Kolb D. Mawet M. N’Diaye G. Orban de Xivry S. P. Quanz A. Reutlinger G. Ruane M. Riquelme C. Soenke M. Sterzik A. Vigan T. de Zeeuw Imaging low-mass planets within the habitable zone of α Centauri |
description |
Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around nearby stars. |
format |
article |
author |
K. Wagner A. Boehle P. Pathak M. Kasper R. Arsenault G. Jakob U. Käufl S. Leveratto A.-L. Maire E. Pantin R. Siebenmorgen G. Zins O. Absil N. Ageorges D. Apai A. Carlotti É. Choquet C. Delacroix K. Dohlen P. Duhoux P. Forsberg E. Fuenteseca S. Gutruf O. Guyon E. Huby D. Kampf M. Karlsson P. Kervella J.-P. Kirchbauer P. Klupar J. Kolb D. Mawet M. N’Diaye G. Orban de Xivry S. P. Quanz A. Reutlinger G. Ruane M. Riquelme C. Soenke M. Sterzik A. Vigan T. de Zeeuw |
author_facet |
K. Wagner A. Boehle P. Pathak M. Kasper R. Arsenault G. Jakob U. Käufl S. Leveratto A.-L. Maire E. Pantin R. Siebenmorgen G. Zins O. Absil N. Ageorges D. Apai A. Carlotti É. Choquet C. Delacroix K. Dohlen P. Duhoux P. Forsberg E. Fuenteseca S. Gutruf O. Guyon E. Huby D. Kampf M. Karlsson P. Kervella J.-P. Kirchbauer P. Klupar J. Kolb D. Mawet M. N’Diaye G. Orban de Xivry S. P. Quanz A. Reutlinger G. Ruane M. Riquelme C. Soenke M. Sterzik A. Vigan T. de Zeeuw |
author_sort |
K. Wagner |
title |
Imaging low-mass planets within the habitable zone of α Centauri |
title_short |
Imaging low-mass planets within the habitable zone of α Centauri |
title_full |
Imaging low-mass planets within the habitable zone of α Centauri |
title_fullStr |
Imaging low-mass planets within the habitable zone of α Centauri |
title_full_unstemmed |
Imaging low-mass planets within the habitable zone of α Centauri |
title_sort |
imaging low-mass planets within the habitable zone of α centauri |
publisher |
Nature Portfolio |
publishDate |
2021 |
url |
https://doaj.org/article/34b7ac7a6b0c49a6be4c1b54f6499593 |
work_keys_str_mv |
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