Universal Gravitation Constant

Flashcard
•
Science
•
10th Grade
•
Hard
+2
Standards-aligned
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15 questions
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1.
FLASHCARD QUESTION
Front
What is the Universal Gravitation Constant?
Back
The Universal Gravitation Constant (G) is a fundamental physical constant that quantifies the strength of the gravitational force between two masses. Its value is approximately 6.674 × 10^-11 N(m/kg)^2.
Tags
NGSS.HS-PS2-4
2.
FLASHCARD QUESTION
Front
Why is the sun the anchor point of our solar system?
Back
The sun is the anchor point of our solar system because of its huge mass, which creates a strong gravitational pull that keeps the planets in orbit.
Tags
NGSS.MS-ESS1-2
NGSS.MS-PS2-4
3.
FLASHCARD QUESTION
Front
What does Newton's law of universal gravitation state?
Back
Newton's law of universal gravitation states that every point mass attracts every other point mass in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
Tags
NGSS.MS-ESS1-2
NGSS.MS-PS2-4
4.
FLASHCARD QUESTION
Front
What are the two main factors affecting the force of gravity between two objects?
Back
The two main factors affecting the force of gravity between two objects are their masses and the distance between them.
Tags
NGSS.MS-ESS1-2
NGSS.MS-PS2-4
5.
FLASHCARD QUESTION
Front
How does distance affect gravitational force?
Back
The gravitational force decreases as the distance between two objects increases. Specifically, it is inversely proportional to the square of the distance.
Tags
NGSS.HS-PS2-4
6.
FLASHCARD QUESTION
Front
What is the relationship between mass and gravitational force?
Back
The gravitational force is directly proportional to the masses of the objects involved; as the mass of either object increases, the gravitational force between them also increases.
Tags
NGSS.MS-PS2-2
NGSS.MS-PS2-4
7.
FLASHCARD QUESTION
Front
What is the formula for calculating gravitational force?
Back
The formula for calculating gravitational force (F) is F = G * (m1 * m2) / r^2, where G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between their centers.
Tags
NGSS.HS-PS2-4
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