Infrared Space Interferometry: Astrophysics & the Study of Earth-Like Planets

Infrared Space Interferometry: Astrophysics & the Study of Earth-Like Planets
Author :
Publisher : Springer Science & Business Media
Total Pages : 333
Release :
ISBN-10 : 9789401154680
ISBN-13 : 9401154686
Rating : 4/5 (686 Downloads)

Book Synopsis Infrared Space Interferometry: Astrophysics & the Study of Earth-Like Planets by : C. Eiroa

Download or read book Infrared Space Interferometry: Astrophysics & the Study of Earth-Like Planets written by C. Eiroa and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 333 pages. Available in PDF, EPUB and Kindle. Book excerpt: The past year has produced some of the most exciting results in the history of astronomy, particularly in the area of planets outside our solar system. Only a half-year before our meeting in Toledo, Spain, the first unambiguous detection of planet-sized masses orbiting main sequence stars were reported. Since that time, evidence for a new exo planet has been reported almost at the rate of about once per month. Some of these objects are likely to turn out to be very low-mass stars, but something like half show characteristics - Jupiter-like mass and near-zero orbital eccentricity - which appear to be unique to planets. Almost at the same time that giant planets were being discovered regularly, the two major space agencies, ESA and NASA, have iden tified searches for and detailed study of Earth-like planets as a major priority for the future. In ESA's "Horizon 2000 Plus" programme, an infrared interferometer has been proposed as a possible future Cor nerstone mission. Similarly, scientists in the US produced the "Road Map for the Exploration of Neighboring Planetary Systems (ExNPS)", which provided NASA with a long-term plan which leads also to an infrared interferometer in space to study hypothetical Earth-like worlds beyond our Solar System. Such an observatory is designed to search for the thermal emission from a family of planets, using interferometric nulling to remove the contaminating light from the central star.


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