What is Kepler's 2nd Law?
Kepler's 2nd Law

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Science
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9th - 12th Grade
•
Hard
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1.
FLASHCARD QUESTION
Front
Back
Kepler's 2nd Law states that a line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time, meaning a planet moves faster when it is closer to the Sun.
2.
FLASHCARD QUESTION
Front
What does eccentricity measure in an ellipse?
Back
Eccentricity measures the deviation of an ellipse from being circular. It ranges from 0 (circle) to 1 (parabola). Higher eccentricity means a more elongated shape.
3.
FLASHCARD QUESTION
Front
How does increasing the distance between an ellipse’s foci affect its shape?
Back
Increasing the distance between an ellipse’s foci increases its eccentricity, making the ellipse more elongated.
4.
FLASHCARD QUESTION
Front
What is the formula for calculating eccentricity (e) of an ellipse?
Back
The formula for eccentricity (e) is e = c/a, where c is the distance from the center to a focus, and a is the distance from the center to a vertex.
5.
FLASHCARD QUESTION
Front
What is the significance of the area swept out by a planet in Kepler's 2nd Law?
Back
The area swept out by a planet in Kepler's 2nd Law is significant because it indicates that a planet's speed varies depending on its distance from the Sun.
6.
FLASHCARD QUESTION
Front
What happens to a planet's speed as it approaches the Sun?
Back
As a planet approaches the Sun, it speeds up due to the gravitational pull, allowing it to sweep out larger areas in shorter times.
7.
FLASHCARD QUESTION
Front
What is the relationship between the time taken to orbit the Sun and the distance from the Sun according to Kepler's 3rd Law?
Back
According to Kepler's 3rd Law, the square of the orbital period (p^2) of a planet is directly proportional to the cube of the semi-major axis (a^3) of its orbit.
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