
Kepler's Laws and Gravity Concepts
Flashcard
•
Physics
•
9th - 12th Grade
•
Practice Problem
•
Hard
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1.
FLASHCARD QUESTION
Front
What are Kepler's Laws of Planetary Motion?
Back
Kepler's Laws describe the motion of planets around the Sun: 1) The Law of Orbits: Planets move in elliptical orbits with the Sun at one focus. 2) The Law of Areas: A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time. 3) The Law of Periods: The square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit.
2.
FLASHCARD QUESTION
Front
What is eccentricity in the context of orbits?
Back
Eccentricity is a measure of how much an orbit deviates from being circular. It ranges from 0 (perfectly circular) to 1 (parabolic). Higher eccentricity indicates a more elongated orbit.
3.
FLASHCARD QUESTION
Front
What does Kepler's 3rd Law state?
Back
Kepler's 3rd Law states that the square of the orbital period (p) of a planet is directly proportional to the cube of the semi-major axis (a) of its orbit: p² = a³.
4.
FLASHCARD QUESTION
Front
What is the semi-major axis of an orbit?
Back
The semi-major axis is half of the longest diameter of an ellipse. It represents the average distance from a planet to the Sun in an elliptical orbit.
5.
FLASHCARD QUESTION
Front
How does distance from the Sun affect a planet's orbital period?
Back
According to Kepler's 3rd Law, as the distance from the Sun increases, the orbital period increases. This means planets further from the Sun take longer to complete one orbit.
6.
FLASHCARD QUESTION
Front
What is the relationship between a planet's distance from the Sun and its orbital speed?
Back
A planet closer to the Sun moves faster in its orbit than a planet that is farther away. This is due to the stronger gravitational pull from the Sun.
7.
FLASHCARD QUESTION
Front
What is gravitational force?
Back
Gravitational force is the attractive force between two masses. It is proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
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