Olber'sParadoxIf the universeis infinite, whyisn't the nightsky infinitelybright?This is a speed-time graph foran object falling(with airresistance)lengthcontractionMovingobjectsappearshorterEmissionSpectrumThisspectrum iscreated by acool gassineWhat trig functiondo we use to findthe verticalcomponent of theinitial velocity of aprojectile?ElasticKinetic energyis conservedin an__________collision.takingrepeatedmeasurementsrandomuncertaintiescan bereduced by_______DiffractionGratingThis is what isoften used tomake aspectrum fromlight from adistant object.-9.8The verticalaccelerationof aprojectile.HotterBlue objectsare ______than redobjectsThe 1-2PunchFree BodyDiagram.Newton'ssecond law.A displacement-time graph witha constant,positiveaccelerationRedshiftthe ________ of agalaxy is thechange inwavelengthdivided by theemittedwavelengththespeedof lightThe is constantfor allobservers in allreferenceframes.darkmatterevidence supportingthe existence of____________comes fromestimations of themass of galaxiesusing their rotationcurvesDisplacement-time graph witha constant,negativeaccelerationDopplerdiagram for anobject travellingAT the speed ofsoundcosineWhat trig functiondo we use to findthe horizontalcomponent of theinitial velocity of aprojectile?terminalvelocityWhen the forceson a skydiver arefinally balanced,they have reached_______.parabolicThe shape ofthe trajectoryof aprojectileDisplacement-time graph fora bouncingballcontinuousspectrumThisspectrum iscreated by ahot, denseobjectcooler_____objectsemit LESSradiation perunit surfacearea per unittimedarkenergyevidence supportingthe existence of____________comesfrom the acceleratingrate of expansion ofthe Universesuvatequationsalsoknown asequationsof motiontimedilationthe “slowing down” ofa clock asdetermined by anobserver who is inrelative motion withrespect to that clock.noexternalforcesMomentumis onlyconserved ifthere are______.displacementThe areaunder avelocity-timegraph =0Thehorizontalaccelerationof aprojectileDopplerEffectthe change inwave frequencyduring the relativemotion between awave source andits observerheadto tailHow doweconnectvectors?Velocity-Time graphfor abouncingballAlwaysEnergy isconserved_______Hubble'sLawAllows us toestimate theage of theuniverseImpulseThe areaunder aforce-timegraphchangeinvelocityThe areaunder anacceleration-time graph =Doppler effectdiagram foran objectmoving to theRIGHTOlber'sParadoxIf the universeis infinite, whyisn't the nightsky infinitelybright?This is a speed-time graph foran object falling(with airresistance)lengthcontractionMovingobjectsappearshorterEmissionSpectrumThisspectrum iscreated by acool gassineWhat trig functiondo we use to findthe verticalcomponent of theinitial velocity of aprojectile?ElasticKinetic energyis conservedin an__________collision.takingrepeatedmeasurementsrandomuncertaintiescan bereduced by_______DiffractionGratingThis is what isoften used tomake aspectrum fromlight from adistant object.-9.8The verticalaccelerationof aprojectile.HotterBlue objectsare ______than redobjectsThe 1-2PunchFree BodyDiagram.Newton'ssecond law.A displacement-time graph witha constant,positiveaccelerationRedshiftthe ________ of agalaxy is thechange inwavelengthdivided by theemittedwavelengththespeedof lightThe is constantfor allobservers in allreferenceframes.darkmatterevidence supportingthe existence of____________comes fromestimations of themass of galaxiesusing their rotationcurvesDisplacement-time graph witha constant,negativeaccelerationDopplerdiagram for anobject travellingAT the speed ofsoundcosineWhat trig functiondo we use to findthe horizontalcomponent of theinitial velocity of aprojectile?terminalvelocityWhen the forceson a skydiver arefinally balanced,they have reached_______.parabolicThe shape ofthe trajectoryof aprojectileDisplacement-time graph fora bouncingballcontinuousspectrumThisspectrum iscreated by ahot, denseobjectcooler_____objectsemit LESSradiation perunit surfacearea per unittimedarkenergyevidence supportingthe existence of____________comesfrom the acceleratingrate of expansion ofthe Universesuvatequationsalsoknown asequationsof motiontimedilationthe “slowing down” ofa clock asdetermined by anobserver who is inrelative motion withrespect to that clock.noexternalforcesMomentumis onlyconserved ifthere are______.displacementThe areaunder avelocity-timegraph =0Thehorizontalaccelerationof aprojectileDopplerEffectthe change inwave frequencyduring the relativemotion between awave source andits observerheadto tailHow doweconnectvectors?Velocity-Time graphfor abouncingballAlwaysEnergy isconserved_______Hubble'sLawAllows us toestimate theage of theuniverseImpulseThe areaunder aforce-timegraphchangeinvelocityThe areaunder anacceleration-time graph =Doppler effectdiagram foran objectmoving to theRIGHT

Higher ODU Bingo - 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. If the universe is infinite, why isn't the night sky infinitely bright?
    Olber's Paradox
  2. This is a speed-time graph for an object falling (with air resistance)
  3. Moving objects appear shorter
    length contraction
  4. This spectrum is created by a cool gas
    Emission Spectrum
  5. What trig function do we use to find the vertical component of the initial velocity of a projectile?
    sine
  6. Kinetic energy is conserved in an __________ collision.
    Elastic
  7. random uncertainties can be reduced by _______
    taking repeated measurements
  8. This is what is often used to make a spectrum from light from a distant object.
    Diffraction Grating
  9. The vertical acceleration of a projectile.
    -9.8
  10. Blue objects are ______ than red objects
    Hotter
  11. Free Body Diagram. Newton's second law.
    The 1-2 Punch
  12. A displacement-time graph with a constant, positive acceleration
  13. the ________ of a galaxy is the change in wavelength divided by the emitted wavelength
    Redshift
  14. The is constant for all observers in all reference frames.
    the speed of light
  15. evidence supporting the existence of ____________ comes from estimations of the mass of galaxies using their rotation curves
    dark matter
  16. Displacement-time graph with a constant, negative acceleration
  17. Doppler diagram for an object travelling AT the speed of sound
  18. What trig function do we use to find the horizontal component of the initial velocity of a projectile?
    cosine
  19. When the forces on a skydiver are finally balanced, they have reached _______.
    terminal velocity
  20. The shape of the trajectory of a projectile
    parabolic
  21. Displacement-time graph for a bouncing ball
  22. This spectrum is created by a hot, dense object
    continuous spectrum
  23. _____objects emit LESS radiation per unit surface area per unit time
    cooler
  24. evidence supporting the existence of ____________comes from the accelerating rate of expansion of the Universe
    dark energy
  25. also known as equations of motion
    suvat equations
  26. the “slowing down” of a clock as determined by an observer who is in relative motion with respect to that clock.
    time dilation
  27. Momentum is only conserved if there are ______.
    no external forces
  28. The area under a velocity-time graph =
    displacement
  29. The horizontal acceleration of a projectile
    0
  30. the change in wave frequency during the relative motion between a wave source and its observer
    Doppler Effect
  31. How do we connect vectors?
    head to tail
  32. Velocity-Time graph for a bouncing ball
  33. Energy is conserved _______
    Always
  34. Allows us to estimate the age of the universe
    Hubble's Law
  35. The area under a force-time graph
    Impulse
  36. The area under an acceleration-time graph =
    change in velocity
  37. Doppler effect diagram for an object moving to the RIGHT