CMBRcosmicmicrowavebackgroundradiationlight1 type ofelectromagneticradiation and isvisibledensitymeasure ofamount ofspace; massper volumelightyearthe distancethat lighttravels inone Earthyearnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itdaythe amount oftime it takesEarth torotate onceon its axisatomicnumberthe numberof protons intheelement'snucleusplasmamost commonstate of visiblematter in theuniverseblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingBigBanga model andtheory thatexplains theorigin of theuniverseelementa group ofall thesame typesof atomsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementelectrona particlewith anegativechargebinarystartwo starsthat revolvearoundeach otheruniversewhat containsall matter,energy,space, andtimeelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationconclusionthe section ofthe lab reportwith a summaryof what waslearnedtelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studygravityforce thatattractsobjects withmasstogethergalaxycollection ofstars, gas,dust, heldby gravitynucleuscenter of anatomcontainingprotons andneutronswavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveamplitudetheheight ofa wavedarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieshydrogenmostabundantelement withan atomicnumber of 1lithiumthe third mostcommonelement withan atomicnumber of 3weightmeasureshow stronglygravity pullson the matterpresentchangeof statewhen mattergoes fromone state toanotherfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timestara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionastronomythe studyof theuniverseheliocentricmodelmodel ofsolor systemthat puts thesun at thecentercarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6absorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsresultsthe part ofthe labreport withobservationsand dataAUthe unit usedto measuredistanceswithin thesolar systemclusterstara group of starsthat share acommon originthat are boundtogether bygravitymassamount ofmatter inan objectwhitedwarfa small densestar wherenuclear fusionis no longerhappeningmoleculeatoms thatare linkedtogether bysharingelectronsmatteranythingthat takesup spaceHeliumthe secondmost abundantelement,atomic numberis 2electromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationscientificmodela simplifiedrepresentationof a realsystemscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsconstellationa group of starsthat seem togroup togetherin interestingpatternsCMBRcosmicmicrowavebackgroundradiationlight1 type ofelectromagneticradiation and isvisibledensitymeasure ofamount ofspace; massper volumelightyearthe distancethat lighttravels inone Earthyearnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itdaythe amount oftime it takesEarth torotate onceon its axisatomicnumberthe numberof protons intheelement'snucleusplasmamost commonstate of visiblematter in theuniverseblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingBigBanga model andtheory thatexplains theorigin of theuniverseelementa group ofall thesame typesof atomsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementelectrona particlewith anegativechargebinarystartwo starsthat revolvearoundeach otheruniversewhat containsall matter,energy,space, andtimeelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationconclusionthe section ofthe lab reportwith a summaryof what waslearnedtelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studygravityforce thatattractsobjects withmasstogethergalaxycollection ofstars, gas,dust, heldby gravitynucleuscenter of anatomcontainingprotons andneutronswavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveamplitudetheheight ofa wavedarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieshydrogenmostabundantelement withan atomicnumber of 1lithiumthe third mostcommonelement withan atomicnumber of 3weightmeasureshow stronglygravity pullson the matterpresentchangeof statewhen mattergoes fromone state toanotherfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timestara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionastronomythe studyof theuniverseheliocentricmodelmodel ofsolor systemthat puts thesun at thecentercarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6absorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsresultsthe part ofthe labreport withobservationsand dataAUthe unit usedto measuredistanceswithin thesolar systemclusterstara group of starsthat share acommon originthat are boundtogether bygravitymassamount ofmatter inan objectwhitedwarfa small densestar wherenuclear fusionis no longerhappeningmoleculeatoms thatare linkedtogether bysharingelectronsmatteranythingthat takesup spaceHeliumthe secondmost abundantelement,atomic numberis 2electromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationscientificmodela simplifiedrepresentationof a realsystemscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsconstellationa group of starsthat seem togroup togetherin interestingpatterns

Astonomy - 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. cosmic microwave background radiation
    CMBR
  2. 1 type of electromagnetic radiation and is visible
    light
  3. measure of amount of space; mass per volume
    density
  4. the distance that light travels in one Earth year
    light year
  5. when nuclei join together to form a heavier nucleus having more protons and neutrons in it
    nuclear fusion
  6. the amount of time it takes Earth to rotate once on its axis
    day
  7. the number of protons in the element's nucleus
    atomic number
  8. most common state of visible matter in the universe
    plasma
  9. these have a gravitational pull that is so strong that matter, energy, and light are pulled into them
    black holes
  10. change in wavelength of electromagnetic radiation when the source is moving
    doppler effect
  11. a model and theory that explains the origin of the universe
    Big Bang
  12. a group of all the same types of atoms
    element
  13. a chart with the names and chemical information for every type of atom or element
    periodic table of elements
  14. a particle with a negative charge
    electron
  15. two stars that revolve around each other
    binary star
  16. what contains all matter, energy, space, and time
    universe
  17. the electric and magnetic disturbance radiated from a source that travels through space, carrying energy and information
    electromagnetic radiation
  18. the section of the lab report with a summary of what was learned
    conclusion
  19. a device used to capture and focus large amounts of electromagnetic radiation for study
    telescope
  20. force that attracts objects with mass together
    gravity
  21. collection of stars, gas, dust, held by gravity
    galaxy
  22. center of an atom containing protons and neutrons
    nucleus
  23. the distance between two adjacent peaks of an electromagnetic wave
    wavelength
  24. the height of a wave
    amplitude
  25. type of matter that can be observed only indirectly through its gravitational effects on stars and galaxies
    dark matter
  26. most abundant element with an atomic number of 1
    hydrogen
  27. the third most common element with an atomic number of 3
    lithium
  28. measures how strongly gravity pulls on the matter present
    weight
  29. when matter goes from one state to another
    change of state
  30. number of wavelengths that pass a certain point in a certain amount of time
    frequency
  31. a massive ball of gas in space that produces its own light and heat through nuclear fusion
    star
  32. the study of the universe
    astronomy
  33. model of solor system that puts the sun at the center
    heliocentric model
  34. the sixth element in which all living organisms have and its atomic number is 6
    carbon
  35. spectrum showing dark lines or bands due to specific wavelengths
    absorption spectrum
  36. apparent movement of nearby objects compared to more distant objects
    parallax shift
  37. the part of the lab report with observations and data
    results
  38. the unit used to measure distances within the solar system
    AU
  39. a group of stars that share a common origin that are bound together by gravity
    cluster star
  40. amount of matter in an object
    mass
  41. a small dense star where nuclear fusion is no longer happening
    white dwarf
  42. atoms that are linked together by sharing electrons
    molecule
  43. anything that takes up space
    matter
  44. the second most abundant element, atomic number is 2
    Helium
  45. entire range of wavelengths of electro. magnetic radiation
    electromagnetic spectrum
  46. a simplified representation of a real system
    scientific model
  47. an approach that uses six steps process relying on logic to ask and snswer questions
    scientific method
  48. a group of stars that seem to group together in interesting patterns
    constellation