Порівняння методів
Переглядайте обрані методи поруч; рядки з відмінностями підсвічено.
| Гравітаційне мікролінзування× | Транзитна фотометрія× | |
|---|---|---|
| Галузь | Астрономія | Астрономія |
| Родина | Process / pipeline | Process / pipeline |
| Рік появи≠ | 1986 | 1984 |
| Автор методу≠ | Bohdan Paczynski | William Borucki |
| Тип≠ | Observational detection method | Observational photometric pipeline |
| Основоположне джерело≠ | Paczynski, B. (1986). Gravitational microlensing by the galactic halo. Astrophysical Journal, 304, 1-5. DOI ↗ | Borucki, W. J., & Summers, A. L. (1984). The photometric method of detecting other planetary systems. Astrophysical Journal, 281, 537-553. DOI ↗ |
| Інші назви | Microlensing, Gravitational Lensing Method | Photometric Transit Method, Planetary Transit Detection |
| Пов'язані | 3 | 3 |
| Підсумок≠ | Gravitational microlensing is an observational technique that exploits Einstein's prediction that massive objects bend light. When a star or planet passes in front of a distant star from our perspective, its gravity acts as a lens, magnifying and distorting the background star's light. First proposed by Bohdan Paczynski in 1986, this method has discovered hundreds of exoplanets and provides unique sensitivity to low-mass planets and dark matter. | Transit photometry is an observational technique that detects exoplanets by monitoring the periodic dips in stellar brightness as planets cross in front of their host stars. First systematized by William Borucki in 1984, this method became the most successful exoplanet detection technique, with the Kepler space telescope discovering thousands of confirmed exoplanets using this approach. |
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