It allowed scientiststo measure G, whichthen made it possibleto calculate Earth'smass using Newton'slaw of universalgravitationIt allowed scientiststo measure G,making it possible tocalculate Earth'smass using Newton'slaw of universalgravitation.Inertial massandgravitationalmass are equalin magnitude.Planetsmove fasterat perihelionand slowerat aphelion.They areequivalentbecause theeffects ofgravitational massand inertial masscancel each otherEarth andplanets movein circlesaround theSun.Orbits Earth ina nearly circularorbit allowingus to treat it asuniform circularmotion.Focithe gravitationalforces of theSun and theMoon arecombined.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.TheKuiper beltor the Oortcloud.The Moonpasses directlybetween theSun and Earth,blocking theSun from view.One is anobjectsresistance tochange and oneis a response togravity.Theyare thesame.the Moon isconstantly fallingtoward Earth butalso movingforward, resultingin its orbit aroundthe Earth.The Sun, Moon,stars, andplanets move inperfect circleswith the Earth atthe center.Masschangesthe spacearound it.It warps the spacearound it to suchan extreme degreethat nothing, noteven light, canescape itsgravitational pull.Mass causes spaceto be curved, andother bodies areacceleratedbecause of the waythey follow thiscurved space.GravitationalForceThe Sun, Moon,stars, andplanets all movein perfect circleswith Earth at thecenter.The timeit takes tocompleteone orbit.The NorthPole is tiltedtoward theSun.Newton'ssecondlaw.Its orbit istilted relativeto the eclipticplane.the Moonmoves 13degrees in itsorbit over a 24-hour period.Sequentialchanges in theappearance ofthe Moon as itorbits Earth.It allowed scientiststo measure G, whichthen made it possibleto calculate Earth'smass using Newton'slaw of universalgravitationIt allowed scientiststo measure G,making it possible tocalculate Earth'smass using Newton'slaw of universalgravitation.Inertial massandgravitationalmass are equalin magnitude.Planetsmove fasterat perihelionand slowerat aphelion.They areequivalentbecause theeffects ofgravitational massand inertial masscancel each otherEarth andplanets movein circlesaround theSun.Orbits Earth ina nearly circularorbit allowingus to treat it asuniform circularmotion.Focithe gravitationalforces of theSun and theMoon arecombined.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.TheKuiper beltor the Oortcloud.The Moonpasses directlybetween theSun and Earth,blocking theSun from view.One is anobjectsresistance tochange and oneis a response togravity.Theyare thesame.the Moon isconstantly fallingtoward Earth butalso movingforward, resultingin its orbit aroundthe Earth.The Sun, Moon,stars, andplanets move inperfect circleswith the Earth atthe center.Masschangesthe spacearound it.It warps the spacearound it to suchan extreme degreethat nothing, noteven light, canescape itsgravitational pull.Mass causes spaceto be curved, andother bodies areacceleratedbecause of the waythey follow thiscurved space.GravitationalForceThe Sun, Moon,stars, andplanets all movein perfect circleswith Earth at thecenter.The timeit takes tocompleteone orbit.The NorthPole is tiltedtoward theSun.Newton'ssecondlaw.Its orbit istilted relativeto the eclipticplane.the Moonmoves 13degrees in itsorbit over a 24-hour period.Sequentialchanges in theappearance ofthe Moon as itorbits Earth.

Chapter 7 - Gravity - Call List

(Print) Use this randomly generated list as your call list when playing the game. There is no need to say the BINGO column name. Place some kind of mark (like an X, a checkmark, a dot, tally mark, etc) on each cell as you announce it, to keep track. You can also cut out each item, place them in a bag and pull words from the bag.


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  1. It allowed scientists to measure G, making it possible to calculate Earth's mass using Newton's law of universal gravitation.
    It allowed scientists to measure G, which then made it possible to calculate Earth's mass using Newton's law of universal gravitation
  2. Inertial mass and gravitational mass are equal in magnitude.
  3. Planets move faster at perihelion and slower at aphelion.
  4. They are equivalent because the effects of gravitational mass and inertial mass cancel each other
  5. Earth and planets move in circles around the Sun.
  6. Orbits Earth in a nearly circular orbit allowing us to treat it as uniform circular motion.
  7. Foci
  8. the gravitational forces of the Sun and the Moon are combined.
  9. The distance term is squared in the equation for Newton's law of universal gravitation.
    The distance term is squared in the equation for Newton's law of universal gravitation.
  10. The Kuiper belt or the Oort cloud.
  11. The Moon passes directly between the Sun and Earth, blocking the Sun from view.
  12. One is an objects resistance to change and one is a response to gravity.
  13. They are the same.
  14. the Moon is constantly falling toward Earth but also moving forward, resulting in its orbit around the Earth.
  15. The Sun, Moon, stars, and planets move in perfect circles with the Earth at the center.
  16. Mass changes the space around it.
  17. It warps the space around it to such an extreme degree that nothing, not even light, can escape its gravitational pull.
  18. Mass causes space to be curved, and other bodies are accelerated because of the way they follow this curved space.
  19. The Sun, Moon, stars, and planets all move in perfect circles with Earth at the center.
    Gravitational Force
  20. The time it takes to complete one orbit.
  21. The North Pole is tilted toward the Sun.
  22. Newton's second law.
  23. Its orbit is tilted relative to the ecliptic plane.
  24. the Moon moves 13 degrees in its orbit over a 24-hour period.
  25. Sequential changes in the appearance of the Moon as it orbits Earth.