the gravitationalforces of theSun and theMoon arecombined.Planetsmove fasterat perihelionand slowerat aphelion.FociIt warps the spacearound it to suchan extreme degreethat nothing, noteven light, canescape itsgravitational pull.Earth andplanets movein circlesaround theSun.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.The Moonpasses directlybetween theSun and Earth,blocking theSun from view.The NorthPole is tiltedtoward theSun.The timeit takes tocompleteone orbit.Inertial massandgravitationalmass are equalin magnitude.the Moon isconstantly fallingtoward Earth butalso movingforward, resultingin its orbit aroundthe Earth.the Moonmoves 13degrees in itsorbit over a 24-hour period.One is anobjectsresistance tochange and oneis a response togravity.Its orbit istilted relativeto the eclipticplane.Theyare thesame.Masschangesthe spacearound it.They areequivalentbecause theeffects ofgravitational massand inertial masscancel each otherOrbits Earth ina nearly circularorbit allowingus to treat it asuniform circularmotion.The Sun, Moon,stars, andplanets move inperfect circleswith the Earth atthe center.Newton'ssecondlaw.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.GravitationalForceThe Sun, Moon,stars, andplanets all movein perfect circleswith Earth at thecenter.TheKuiper beltor the Oortcloud.Mass causes spaceto be curved, andother bodies areacceleratedbecause of the waythey follow thiscurved space.Sequentialchanges in theappearance ofthe Moon as itorbits Earth.the gravitationalforces of theSun and theMoon arecombined.Planetsmove fasterat perihelionand slowerat aphelion.FociIt warps the spacearound it to suchan extreme degreethat nothing, noteven light, canescape itsgravitational pull.Earth andplanets movein circlesaround theSun.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.The Moonpasses directlybetween theSun and Earth,blocking theSun from view.The NorthPole is tiltedtoward theSun.The timeit takes tocompleteone orbit.Inertial massandgravitationalmass are equalin magnitude.the Moon isconstantly fallingtoward Earth butalso movingforward, resultingin its orbit aroundthe Earth.the Moonmoves 13degrees in itsorbit over a 24-hour period.One is anobjectsresistance tochange and oneis a response togravity.Its orbit istilted relativeto the eclipticplane.Theyare thesame.Masschangesthe spacearound it.They areequivalentbecause theeffects ofgravitational massand inertial masscancel each otherOrbits Earth ina nearly circularorbit allowingus to treat it asuniform circularmotion.The Sun, Moon,stars, andplanets move inperfect circleswith the Earth atthe center.Newton'ssecondlaw.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.The distanceterm is squaredin the equationfor Newton'slaw of universalgravitation.GravitationalForceThe Sun, Moon,stars, andplanets all movein perfect circleswith Earth at thecenter.TheKuiper beltor the Oortcloud.Mass causes spaceto be curved, andother bodies areacceleratedbecause of the waythey follow thiscurved space.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. the gravitational forces of the Sun and the Moon are combined.
  2. Planets move faster at perihelion and slower at aphelion.
  3. Foci
  4. It warps the space around it to such an extreme degree that nothing, not even light, can escape its gravitational pull.
  5. Earth and planets move in circles around the Sun.
  6. 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
  7. The Moon passes directly between the Sun and Earth, blocking the Sun from view.
  8. The North Pole is tilted toward the Sun.
  9. The time it takes to complete one orbit.
  10. Inertial mass and gravitational mass are equal in magnitude.
  11. the Moon is constantly falling toward Earth but also moving forward, resulting in its orbit around the Earth.
  12. the Moon moves 13 degrees in its orbit over a 24-hour period.
  13. One is an objects resistance to change and one is a response to gravity.
  14. Its orbit is tilted relative to the ecliptic plane.
  15. They are the same.
  16. Mass changes the space around it.
  17. They are equivalent because the effects of gravitational mass and inertial mass cancel each other
  18. Orbits Earth in a nearly circular orbit allowing us to treat it as uniform circular motion.
  19. The Sun, Moon, stars, and planets move in perfect circles with the Earth at the center.
  20. Newton's second law.
  21. 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.
  22. The Sun, Moon, stars, and planets all move in perfect circles with Earth at the center.
    Gravitational Force
  23. The Kuiper belt or the Oort cloud.
  24. Mass causes space to be curved, and other bodies are accelerated because of the way they follow this curved space.
  25. Sequential changes in the appearance of the Moon as it orbits Earth.