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Doppler spectroscopy as a path to the detection of Earth-like planets

Title
Doppler spectroscopy as a path to the detection of Earth-like planets
Type
Another Publication in an International Scientific Journal
Year
2014
Authors
Mayor, M
(Author)
Other
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Lovis, C
(Author)
Other
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N.C. Santos
(Author)
FCUP
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Journal
Title: NatureImported from Authenticus Search for Journal Publications
Vol. 513
Pages: 328-335
ISSN: 0028-0836
Publisher: Springer Nature
Other information
Authenticus ID: P-009-T2G
Abstract (EN): Doppler spectroscopy was the first technique used to reveal the existence of extrasolar planetary systems hosted by solar-type stars. Radial-velocity surveys led to the detection of a rich population of super-Earths and Neptune-type planets. The numerous detected systems revealed a remarkable diversity. Combining Doppler measurements with photometric observations of planets transiting their host stars further provides access to the planet bulk density, a first step towards comparative exoplanetology. The development of new high-precision spectrographs and space-based facilities will ultimately lead us to characterize rocky planets in the habitable zone of our close stellar neighbours.
Language: English
Type (Professor's evaluation): Scientific
No. of pages: 8
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