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

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