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

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