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Автор Doyle, Laurance R.
Автор Dunham, Edward T.
Автор Deeg, Hans‐Jörg
Автор Blue, J. Ellen
Автор Jenkins, Jon M.
Дата выпуска 1996
dc.description The detection of terrestrial‐sized extrasolar planets from the ground has been thought to be virtually impossible due to atmospheric scintillation limits. However, we show that this is not the case for specially selected (but nevertheless main sequence) stars, namely small eclipsing binaries. For the smallest of these systems, CM Draconis, several months to a few years of photometric observations with 1‐m‐class telescopes will be sufficient to detect the transits of any short‐period planets of sizes ≥1.5 Earth radii (R<sub>E</sub>), using cross‐correlation analysis with moderately good photometry. Somewhat larger telescopes will be needed to extend this detectability to terrestrial planets in larger eclipsing binary systems. (We arbitrarily define “terrestrial planets” herein as those whose disc areas are closer to that of Earth's than Neptune's i.e., less than about 2.78 R<sub>E</sub>.) As a “spin‐off” of such observations, we will also be able to detect the presence of Jovian‐mass planets without transits using the timing of the eclipse minima. Eclipse minima will drift in time as the binary system is offset by a sufficiently massive planet (i.e., one Jupiter mass) about the binary/giant‐planet barycenter, causing a periodic variation in the light travel time to the observer. We present here an outline of present observations taking place at the University of California Lick Observatory using the Crossley 0.9‐m telescope in collaboration with other observatories (in South Korea, Crete, France, Canary Islands, and New York) to detect or constrain the existence of terrestrial planets around main sequence eclipsing binary star systems, starting with CM Draconis. We demonstrate the applicability of photometric data to the general detection of gas giant planets via eclipse minima timings in many other small‐mass eclipsing binary systems as well.
Формат application.pdf
Копирайт Copyright 1996 by the American Geophysical Union.
Тема Detection of Extrasolar Planets
Тема ELECTROMAGNETICS
Тема Signal processing and adaptive antennas
Тема PLANETARY SCIENCES: FLUID PLANETS
Тема Planetology: Fluid Planets: Origin and evolution
Тема PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS
Тема Planetology: Solar System Objects: Stellar planetary systems
Тема RADIO SCIENCE
Тема Signal processing
Тема SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY
Тема Stellar astronomy
Название Ground‐based detectability of terrestrial and Jovian extrasolar planets: Observations of CM Draconis at Lick Observatory
Тип article
DOI 10.1029/96JE00825
Electronic ISSN 2156-2202
Print ISSN 0148-0227
Журнал Journal of Geophysical Research: Planets
Том 101
Первая страница 14823
Последняя страница 14829
Выпуск E6
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