Kepler's Law - Burris
Across
- 4. Symmetrical, closed oval shapes (stretched circles) that describe the geometric paths of planetary orbits
- 5. Three foundational rules of planetary motion formulated by Johannes Kepler:Foci
- 7. The curved, regular path that an object follows as it rotates
- 8. The spinning motion of an object around its own internal axis (e.g., Earth takes about 24 hours to complete one full rotation,
- 9. The two fixed internal points inside an ellipse from which the sum of the distances to any point on the ellipse is constant
- 10. The angle at which a planet's rotational axis is inclined relative to its orbital plane
Down
- 1. An imaginary straight line running through the center of a rotating object
- 2. The orbital movement of one object around another (e.g., Earth revolves around the Sun, taking about 365.25 days to complete
- 3. A numerical value (\(0\) to \(1\)) measuring how much an ellipse deviates from a perfect circle
- 6. he distinct periods of the year (spring, summer, autumn, winter) caused primarily by the 23.5-degree tilt of Earth's axis