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| Manewr Asysty Grawitacyjnej× | Analiza krzywych blasku× | |
|---|---|---|
| Dziedzina | Fizyka stosowana | Fizyka stosowana |
| Rodzina | Process / pipeline | Process / pipeline |
| Rok powstania≠ | 1961 | 1880 |
| Twórca≠ | Michael Minovitch | Edward Pickering |
| Typ≠ | Orbital maneuver technique | Signal processing and astronomical observation technique |
| Źródło pierwotne≠ | Minovitch, M. A. (1961). The determination and characteristics of ballistic interplanetary trajectories under the influence of multiple planetary gravitational fields. Technical Report 32-464, Jet Propulsion Laboratory. link ↗ | Ricker, G. R., et al. (2015). TESS: Transiting Exoplanet Survey Satellite. Journal of Astronomical Telescopes, Instruments, and Systems, 1(1), 014003. DOI ↗ |
| Inne nazwy≠ | swing-by, gravitational slingshot | photometric analysis, transit photometry, eclipsing binary analysis |
| Pokrewne≠ | 4 | 3 |
| Podsumowanie≠ | A gravity assist (or swing-by) maneuver uses the gravitational field of a planet or other celestial body to alter a spacecraft's trajectory and velocity without expending fuel. Discovered by Michael Minovitch at JPL in 1961, this technique is crucial for reaching distant planets economically. It works by exploiting the relative motion between the spacecraft, the assisting body, and the Sun. | Light curve analysis is the study of the brightness variation of a celestial object over time, used to detect and characterize exoplanets, eclipsing binaries, and variable stars. When a planet transits in front of its host star, the star's brightness dips slightly. By analyzing these photometric signatures, astronomers can determine planetary radii, orbital periods, and atmospheric properties. This method has discovered thousands of exoplanets and revealed the structure of stellar systems. |
| ScholarGateZbiór danych ↗ |
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