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This deck focuses on Gravitational Force, giving you a quick way to review the definitions, rules, and examples that matter most for AP Physics 1.
Study Gravitational Force in AP Physics 1 with focused flashcards that help you recognize the idea, recall the key rule, and apply it in practice-style prompts.
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What does m2 stand for in the gravitational force formula?
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Mass of the second object. Second object's mass in the gravitational force equation.
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This deck focuses on Gravitational Force, giving you a quick way to review the definitions, rules, and examples that matter most for AP Physics 1.
Work through these flashcards in short sessions. Try to answer each prompt before flipping the card, then revisit any cards you miss until the explanation feels automatic.
Answer: Mass of the second object. Second object's mass in the gravitational force equation.
Answer: Causes tidal forces. Moon's gravity creates differential forces causing ocean tides.
Answer: Distance between the centers of masses. Distance measured from center to center, not surface to surface.
Answer: Force triples. Force is directly proportional to each mass individually.
Answer: Every mass attracts every other mass. Newton's law applies universally to all objects with mass.
Answer: Greater mass, stronger attraction. More massive objects exert stronger gravitational pulls.
Answer: Force is quartered. Force varies as 1/r2, so doubling distance reduces force by factor of 4.
Answer: Mass of the second object. Second object's mass in the gravitational force equation.
Answer: 6.674×10−11 N. Substituting m1=m2=1 kg, r=1 m into Newton's formula.
Answer: Force quadruples. Each mass doubles, creating a 2×2=4 factor increase.
Answer: Decreases with altitude. Higher altitude means greater distance from Earth's center.
Answer: F=Gr2m1m2. Newton's universal gravitation formula relating force to masses and distance squared.
Answer: Both objects have mass. Only objects with mass can exert or experience gravitational force.
Answer: Force = mass × field strength. Gravitational field strength equals force per unit mass.
Answer: Both objects have mass. Only objects with mass can exert or experience gravitational force.
Answer: Varies with planetary mass and radius. Different planetary properties create different gravitational field strengths.
Answer: Directly proportional. Larger masses produce stronger gravitational forces.
Answer: Force quadruples. Halving distance means r2 becomes r2/4, so force increases 4 times.
Answer: Inversely proportional to r2. Force decreases rapidly as distance increases due to square relationship.
Answer: Approximately 9.8 N. Weight of 1 kg object equals mass times Earth's surface gravity.
Answer: Force = mass × field strength. Gravitational field strength equals force per unit mass.
Answer: 6.674×10−11 N. Substituting m1=m2=1 kg, r=1 m into Newton's formula.
Answer: Potential energy depends on force and distance. Potential energy is the integral of force over distance.
Answer: Inversely proportional to r2. Force decreases rapidly as distance increases due to square relationship.
Answer: Greater mass, stronger attraction. More massive objects exert stronger gravitational pulls.
Answer: Provides necessary centripetal force. Earth's gravity supplies the centripetal acceleration for orbital motion.
Answer: N m²/kg². Derived from force units divided by mass squared times distance squared.
Answer: Force is quartered. Force varies as 1/r2, so doubling distance reduces force by factor of 4.
Answer: 6.674×10−11 N m2/kg2. Standard value of the universal gravitational constant.
Answer: Centripetal force maintaining orbit. Gravitational attraction provides the inward force needed for circular motion.
Answer: Force doubles. Force is directly proportional to each mass in the equation.
Answer: Centripetal force maintaining orbit. Gravitational attraction provides the inward force needed for circular motion.
Answer: 4.00×10−10 N. Using the gravitational force formula with the specified masses and distance.
Answer: Decreases with altitude. Higher altitude means greater distance from Earth's center.
Answer: Force quadruples. Each mass doubles independently, so total force increases by 2×2=4.
Answer: Force quadruples. Each mass doubles independently, so total force increases by 2×2=4.
Answer: 4.00×10−10 N. Using the gravitational force formula with the specified masses and distance.
Answer: N m²/kg². Derived from force units divided by mass squared times distance squared.
Answer: 6.674×10−11 N m2/kg2. Standard value of the universal gravitational constant.
Answer: Varies with planetary mass and radius. Different planetary properties create different gravitational field strengths.
Answer: Attractive force. Gravity always pulls objects together, never pushes them apart.
Answer: F=Gr2m1m2. Newton's universal gravitation formula relating force to masses and distance squared.
Answer: Force triples. Force is directly proportional to each mass individually.
Answer: Attractive force. Gravity always pulls objects together, never pushes them apart.
Answer: Gravitational constant. Universal constant that makes the gravitational formula dimensionally consistent.
Answer: Potential energy depends on force and distance. Potential energy is the integral of force over distance.
Answer: Force quadruples. Each mass doubles, creating a 2×2=4 factor increase.
Answer: Mass of the first object. First object's mass in the gravitational force equation.
Answer: Directly proportional. Larger masses produce stronger gravitational forces.
Answer: Keeps planets in orbit. Solar gravity provides centripetal force maintaining planetary orbital motion.
Answer: Distance between the centers of masses. Distance measured from center to center, not surface to surface.
Answer: Towards the center of the masses. Gravity always pulls objects toward each other's centers.
Answer: Gravitational constant. Universal constant that makes the gravitational formula dimensionally consistent.
Answer: Approximately 9.8 N. Weight of 1 kg object equals mass times Earth's surface gravity.
Answer: Force quadruples. Halving distance means r2 becomes r2/4, so force increases 4 times.
Answer: Causes tidal forces. Moon's gravity creates differential forces causing ocean tides.
Answer: Force doubles. Force is directly proportional to each mass in the equation.
Answer: Every mass attracts every other mass. Newton's law applies universally to all objects with mass.
Answer: Provides necessary centripetal force. Earth's gravity supplies the centripetal acceleration for orbital motion.
Answer: Mass of the first object. First object's mass in the gravitational force equation.
Answer: Keeps planets in orbit. Solar gravity provides centripetal force maintaining planetary orbital motion.