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

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