7.2.2 Kepler's Three Laws Flashcards
Kepler’s Three Laws
- Kepler’s first law: The path of an object in a closed orbit around the Sun is an ellipse with the Sun at one focus.
- Kepler’s second law: For an object in a closed orbit around the Sun, the distance between it and the center of the Sun sweeps out a constant area in a given amount of time.
- Kepler’s third law: For an object in a closed orbit around the Sun, the square of its period is proportional to the cube of the semimajor axis of its orbit:
Which of the following statements about Kepler’s first law of planetary motion is not correct?
The orbit of the planets is an ellipse with one focus.
Consider a moon that is 1.15 × 10^6 km from the planet it is orbiting. This moon makes one complete orbit every 27 days. What is the orbital period of a satellite orbiting the planet at a distance of 4.10 × 10^6 km?
181.8 d
Which of the following is the best method to determine that the orbital radius and periods of Jupiter and Saturn are in agreement with Kepler’s laws? Use the subscript j for Jupiter and s for Saturn; r is the radius from the Sun to the planet and T represents the period.
Determine if the value of (rj / rs)3/2 is equal to Tj / Ts.
Kepler’s work resulted in three laws of orbital motion. Which of the following is not true?
Kepler described and explained the motions of the planets known at that time.
Consider Kepler’s second law of planetary motion. Which of the following is not correct?
A planet’s orbital speed is greater when it is farther away from the sun than when it is closer to the sun.
Suppose that a new planet is discovered and its period is determined. The new planet’s distance from the Sun could be found using Kepler’s ________________
third law
Consider Kepler’s third law of planetary motion. Which of the following is not correct?
There is a constant K such that T 2 = K R 3 for all objects orbiting a body.
Planets at a greater distance from the Sun _________________.
have longer periods of revolution
The moon has a period Tm equal to 28 days and an orbital radius rm equal to 3.8*10^5 km. What is the orbital radius of a satellite that travels around the Earth in 1 day?
4.12 × 10^4 km