elementa group ofall thesame typesof atomsbinarystartwo starsthat revolvearoundeach otherstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusiondopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesweightmeasureshow stronglygravity pullson the matterpresentabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsamplitudetheheight ofa waveelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationmassamount ofmatter inan objectBigBanga model andtheory thatexplains theorigin of theuniverseconstellationa group of starsthat seem togroup togetherin interestingpatternsatomicnumberthe numberof protons intheelement'snucleusnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemlithiumthe third mostcommonelement withan atomicnumber of 3Heliumthe secondmost abundantelement,atomic numberis 2CMBRcosmicmicrowavebackgroundradiationmoleculeatoms thatare linkedtogether bysharingelectronselectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationAUthe unit usedto measuredistanceswithin thesolar systemcarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6heliocentricmodelmodel ofsolor systemthat puts thesun at thecenterclusterstara group of starsthat share acommon originthat are boundtogether bygravitydensitymeasure ofamount ofspace; massper volumechangeof statewhen mattergoes fromone state toanotherastronomythe studyof theuniversenucleuscenter of anatomcontainingprotons andneutronsdaythe amount oftime it takesEarth torotate onceon its axisfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementlight1 type ofelectromagneticradiation and isvisiblematteranythingthat takesup spacewavelengththe distancebetween twoadjacent peaksof anelectromagneticwavelightyearthe distancethat lighttravels inone Earthyeargalaxycollection ofstars, gas,dust, heldby gravityplasmamost commonstate of visiblematter in theuniverseresultsthe part ofthe labreport withobservationsand dataconclusionthe section ofthe lab reportwith a summaryof what waslearnedgravityforce thatattractsobjects withmasstogetherwhitedwarfa small densestar wherenuclear fusionis no longerhappeningscientificmodela simplifiedrepresentationof a realsystemuniversewhat containsall matter,energy,space, andtimescientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionselectrona particlewith anegativechargehydrogenmostabundantelement withan atomicnumber of 1parallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectstelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyelementa group ofall thesame typesof atomsbinarystartwo starsthat revolvearoundeach otherstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusiondopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesweightmeasureshow stronglygravity pullson the matterpresentabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsamplitudetheheight ofa waveelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationmassamount ofmatter inan objectBigBanga model andtheory thatexplains theorigin of theuniverseconstellationa group of starsthat seem togroup togetherin interestingpatternsatomicnumberthe numberof protons intheelement'snucleusnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemlithiumthe third mostcommonelement withan atomicnumber of 3Heliumthe secondmost abundantelement,atomic numberis 2CMBRcosmicmicrowavebackgroundradiationmoleculeatoms thatare linkedtogether bysharingelectronselectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationAUthe unit usedto measuredistanceswithin thesolar systemcarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6heliocentricmodelmodel ofsolor systemthat puts thesun at thecenterclusterstara group of starsthat share acommon originthat are boundtogether bygravitydensitymeasure ofamount ofspace; massper volumechangeof statewhen mattergoes fromone state toanotherastronomythe studyof theuniversenucleuscenter of anatomcontainingprotons andneutronsdaythe amount oftime it takesEarth torotate onceon its axisfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementlight1 type ofelectromagneticradiation and isvisiblematteranythingthat takesup spacewavelengththe distancebetween twoadjacent peaksof anelectromagneticwavelightyearthe distancethat lighttravels inone Earthyeargalaxycollection ofstars, gas,dust, heldby gravityplasmamost commonstate of visiblematter in theuniverseresultsthe part ofthe labreport withobservationsand dataconclusionthe section ofthe lab reportwith a summaryof what waslearnedgravityforce thatattractsobjects withmasstogetherwhitedwarfa small densestar wherenuclear fusionis no longerhappeningscientificmodela simplifiedrepresentationof a realsystemuniversewhat containsall matter,energy,space, andtimescientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionselectrona particlewith anegativechargehydrogenmostabundantelement withan atomicnumber of 1parallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectstelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for study

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