Evidence for Gravity - Middle School Physical Science

  1. What happens to gravitational force if both masses are doubled while rr stays constant?
    Force becomes 44 times as large. Doubling both masses multiplies force by 2×2=42 \times 2 = 4.
  2. Identify the independent variable when a simulation changes only distance to test its effect on FgF_g.
    Distance rr. Independent variable is what you change; dependent is what you measure.
  3. What happens to gravitational force if one mass is doubled while rr stays constant?
    Force doubles. Force is directly proportional to each mass, so doubling one mass doubles force.
  4. Which change best supports the claim that gravity increases with mass in a simulation?
    Increase m1m_1 or m2m_2 while keeping rr constant. Since F∝m1m2F \propto m_1m_2, increasing either mass while fixing distance shows force increases.
  5. Identify the best conclusion if a simulation shows FF stays the same when both masses swap positions.
    Gravitational force depends on masses and distance, not on which mass is labeled 11 or 22. The formula is symmetric in m1m_1 and m2m_2, so swapping them doesn't change FF.
  6. Which option states Newton's third law for gravitational interaction between two masses?
    Forces are equal in magnitude and opposite in direction. Action-reaction pairs have equal magnitude but opposite directions.
  7. Identify the best claim supported if a simulation shows force decreases rapidly as rr increases.
    Gravitational force decreases with distance by an inverse-square pattern. Rapid decrease with distance indicates inverse-square relationship.
  8. Which statement is supported if a simulation shows equal and opposite forces on two interacting masses?
    Gravitational forces come in equal-magnitude, opposite-direction pairs. Newton's third law: every gravitational force has an equal and opposite reaction force.
  9. Find the missing evidence: If a graph of FgF_g vs. rr is consistent with 1r2\frac{1}{r^2}, what claim is supported?
    Gravitational force follows an inverse-square law with distance. Graph matching 1r2\frac{1}{r^2} pattern confirms the inverse-square law.
  10. Which evidence from a simulation best supports that gravity is always attractive?
    Objects always accelerate toward each other, never away. Attractive force means objects move toward each other, never repel.
  11. If a simulation doubles m1m_1 while m2m_2 and rr stay constant, what happens to FF?
    It doubles. Force is directly proportional to each mass, so doubling one mass doubles the force.
  12. Which graph shape best matches the model prediction for FF versus m1m_1 when m2m_2 and rr are constant?
    A straight line through the origin (directly proportional). Direct proportionality between FF and m1m_1 creates a linear relationship through origin.
  13. Which graph shape best matches the model prediction for FF versus rr when masses are constant?
    A decreasing curve proportional to 1r2\frac{1}{r^2}. The inverse square relationship creates a hyperbolic curve that decreases rapidly.
  14. In a simulation, which variable must be controlled to isolate the effect of distance on FF?
    Keep m1m_1 and m2m_2 constant. Controlling masses isolates distance effects since FF depends on both variables.
  15. A model shows Earth pulls on the Moon with force FF. What force does the Moon exert on Earth?
    Also FF, in the opposite direction. Newton's third law: forces between objects are equal and opposite.
  16. What is the formula for gravitational force between two masses?
    Fg=Gm1m2r2F_g = G\frac{m_1m_2}{r^2}. Newton's law shows force depends on both masses and inversely on distance squared.
  17. If a model doubles the distance rr, what happens to the force FF according to F∝1r2F\propto\frac{1}{r^2}?
    It becomes 14\frac{1}{4} of the original force. Force varies as 1r2\frac{1}{r^2}, so doubling rr gives 1(2r)2=14\frac{1}{(2r)^2} = \frac{1}{4} of original.
  18. Which change best supports the claim that gravity decreases with distance in a simulation?
    Increase rr while keeping m1m_1 and m2m_2 constant. Since F∝1r2F \propto \frac{1}{r^2}, increasing distance while fixing masses shows force decreases.
  19. Which model outcome best supports that gravitational interactions act at a distance without contact?
    Forces occur even when objects are not touching. Gravity acts through empty space without requiring physical contact between objects.
  20. What happens to gravitational field strength gg if distance from the planet center is doubled?
    gg becomes 14\frac{1}{4} as large. Field strength follows same inverse-square law as gravitational force.
  21. Which relationship should a correct gravity model show between force and distance?
    Inverse-square: Fg∝1r2F_g \propto \frac{1}{r^2}. Force decreases with the square of distance, not linearly.
  22. Which model result supports the claim that gravity is always attractive, not repulsive?
    Objects accelerate toward each other, not away, for all tested masses. Attractive force means objects always pull together, never push apart.
  23. What is the formula for gravitational field strength due to a mass MM at distance rr?
    g=GMr2g = G\frac{M}{r^2}. Field strength at a point depends on source mass and distance from it.
  24. What is the direction of the gravitational force on each mass in a two-body model?
    Along the line joining centers, toward the other mass. Gravity always pulls objects directly toward each other.
  25. If a model triples the distance rr, what happens to the force FF according to F∝1r2F\propto\frac{1}{r^2}?
    It becomes 19\frac{1}{9} of the original force. Force varies as 1r2\frac{1}{r^2}, so tripling rr gives 1(3r)2=19\frac{1}{(3r)^2} = \frac{1}{9} of original.
  26. What happens to gravitational force if distance rr is doubled in a simulation?
    Force becomes 14\frac{1}{4} as large. Doubling distance makes r2r^2 become 4r24r^2, reducing force by factor of 4.
  27. Which relationship should a correct gravity model show between force and each mass?
    Direct: Fg∝m1F_g \propto m_1 and Fg∝m2F_g \propto m_2. Force increases linearly with each mass independently.
  28. Which variable in Fg=Gm1m2r2F_g = G\frac{m_1m_2}{r^2} represents the distance between centers?
    rr. Distance is measured between the centers of mass of the two objects.
  29. If a model uses g=10 N/kgg = 10\ \text{N/kg} and m=3 kgm = 3\ \text{kg}, what is FgF_g?
    30 N30\ \text{N}. Using Fg=mgF_g = mg: Fg=3 kg×10 N/kg=30 NF_g = 3\ \text{kg} \times 10\ \text{N/kg} = 30\ \text{N}.
  30. What does the variable rr represent in the model F=Gm1m2r2F = G\frac{m_1 m_2}{r^2}?
    Center-to-center distance between the two masses. The distance rr is measured from one object's center to the other's center.
  31. In a simulation, which variable must be controlled to isolate the effect of mass on FF?
    Keep rr constant. Controlling distance isolates mass effects since FF depends on both variables.
  32. If a simulation doubles both m1m_1 and m2m_2 while rr stays constant, what happens to FF?
    It becomes 44 times larger. Doubling both masses multiplies force by 2×2=42 \times 2 = 4 since F∝m1m2F \propto m_1m_2.
  33. Identify the best claim supported if a simulation shows higher force for larger m1m_1 at fixed rr.
    Gravitational force increases as mass increases. Direct proportionality means larger mass produces larger force.
  34. What happens to gravitational force if distance rr is tripled in a simulation?
    Force becomes 19\frac{1}{9} as large. Tripling distance makes r2r^2 become 9r29r^2, reducing force by factor of 9.
  35. Which evidence from an orbit simulation best supports that gravity provides centripetal force?
    The orbiting object continuously accelerates toward the central mass. Gravity pulls the orbiting object inward, providing the centripetal acceleration for circular motion.
  36. What is the formula for gravitational force between two masses in a model?
    F=Gm1m2r2F = G\frac{m_1 m_2}{r^2}. Newton's law shows force depends on both masses and inverse square of distance.
  37. What does a downward arrow labeled FgF_g on a free-body diagram represent?
    The gravitational force (weight) acting toward the attracting body. Weight is the gravitational force pulling an object toward the planet or star.
  38. What is the relationship between weight and mass near a planet in a model?
    Fg=mgF_g = mg. Near a planet's surface, weight equals mass times gravitational field strength.

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