| タイトル | The Kepler Mission and Eclipsing Binaries |
| 著者（英） | Jenkins, Jon; Gautier, Nick; Koch, David; Lissauer, J.; Borucki, William; Brown, Timothy; Dunham, Edward; Cochran, William; Basri, Gibor; Caldwell, Douglas |
| 著者所属（英） | NASA Ames Research Center |
| 発行日 | 2006-01-01 |
| 言語 | eng |
| 内容記述 | The Kepler Mission is a photometric mission with a precision of 14 ppm (at R=12) that is designed to continuously observe a single field of view (FOV) of greater 100 sq deg in the Cygnus-Lyra region for four or more years. The primary goal of the mission is to monitor greater than 100,000 stars for transits of Earth-size and smaller planets in the habitable zone of solar-like stars. In the process, many eclipsing binaries (EB) will also be detected and light curves produced. To enhance and optimize the mission results, the stellar characteristics for all the stars in the FOV with R less than 16 will have been determined prior to launch. As part of the verification process, stars with transit candidates will have radial velocity follow-up observations performed to determine the component masses and thereby separate eclipses caused by stellar companions from transits caused by planets. The result will be a rich database on EBs. The community will have access to the archive for further analysis, such as, for EB modeling of the high-precision light curves. A guest observer program is also planned to allow for photometric observations of objects not on the target list but within the FOV, since only the pixels of interest from those stars monitored will be transmitted to the ground. |
| NASA分類 | Astronomy |
| 権利 | No Copyright |
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