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| Astrosejsmologia× | Analiza krzywej rotacji× | |
|---|---|---|
| Dziedzina | Astronomia | Astronomia |
| Rodzina | Process / pipeline | Process / pipeline |
| Rok powstania | 1970 | 1970 |
| Twórca≠ | Roger Ulrich | Vera Rubin |
| Typ≠ | Observational technique | Observational kinematic method |
| Źródło pierwotne≠ | Ulrich, R. K. (1970). The five-minute oscillations on the solar surface. Astrophysical Journal, 162, 993-999. DOI ↗ | Vera C. Rubin & W. Kent Ford Jr. (1970). Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. Astrophysical Journal, 159, 379-403. DOI ↗ |
| Inne nazwy | Stellar Oscillations, Stellar Seismology, Helioseismology | Galactic Rotation Curves, Rotation Curve Method, Velocity Curve Analysis |
| Pokrewne | 3 | 3 |
| Podsumowanie≠ | Asteroseismology is the study of stellar oscillations—tiny brightness and radial velocity variations caused by sound waves resonating inside stars. Proposed by Roger Ulrich in 1970 and established as a major field by the Kepler and TESS space telescopes, asteroseismology provides unprecedented precision in determining stellar masses, ages, and internal structure. | Galaxy rotation curve analysis is the technique of measuring how orbital velocities change with distance from the center of a galaxy. Pioneered by Vera Rubin and W. Kent Ford Jr. in 1970, rotation curves revealed one of astronomy's great mysteries: galaxies rotate too fast to be held together by their visible stars alone, providing direct evidence for dark matter. |
| ScholarGateZbiór danych ↗ |
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