| タイトル | Direct imaging of extra-solar planets with stationary occultations viewed by a space telescope |
| 著者（英） | Elliot, J. L. |
| 著者所属（英） | Cornell Univ. |
| 発行日 | 1978-07-01 |
| 言語 | eng |
| 内容記述 | The use of a telescope in space to detect planets outside the solar system by means of imaging at optical wavelengths is discussed. If the 'black' limb of the moon is utilized as an occulting edge, a hypothetical Jupiter-Sun system could be detected at a distance as great as 10 pc, and a signal-to-noise ratio of 9 could be achieved in less than 20 min with a 2.4 m telescope in space. An orbit for the telescope is proposed; this orbit could achieve a stationary lunar occultation of any star for a period of nearly two hours. |
| NASA分類 | ASTRONOMY |
| レポートNO | 78A48974 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/431259 |
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