infraredthewavelengthafter radioPROTO-STARearlieststage of astar- wherenuclearfusion bginsBLACKHOLESstronggravitationalpull thateven lightcan't excapeBlueShiftAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthSTAR'SCOLORthis isaffected bytemperaturePLANETa largenaturalobject thatorbits a starlightyearthe distancelight travelsin a yearFUSIONconvertinghydrogento heliumin starsRedShiftthe shortestwavelengthin thespectrumgammaraysE.R.spectrumenergythat flowsfrom spacein wavesBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeABSOLUTEMAGNI-TUDEhow brighta starreally is14.5billionLUMIN-OSITYthebrightnessof a starNEBULAa cloud ofdust andgas inspacea telescopein space thatuses visiblelightHubbleRedSUPERGIANTin high massstars whenstar beginsto run out offuelMAINSEQUENCEstars thatare stablein their lifecyclea telescopein space thatuses infraredSpitzertelescoperadiothe longestwavelengthin thespectrumBigBangbithe wavelength oureyes canseevisiblelightstar left atthe core ofa planetarynebulaWhiteDwarf Surfacetemperaturethetemperatureof a starNEUTRONSTARtheremainsof a high-mass starIrregularGalaxygalaxy thathas noparticularshapeMilkyWayGalaxyourgalaxyEllipticalGalaxygalaxyshaped asan ovalHIGHMASSSTARa star withhighermass thanother starsa telescopein space thatuses x-rayChandraH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperatureSUPERNOVAred supergiantexplodesRedGIANTstar beginsto run out offuel in lowmass starsultra-violetthe wavelengthaftervisible lightLOWMASSSTARstars withlowermass thanother starsSpiralGalaxygalaxyshaped ina spiralEdwinHubbleinfraredthewavelengthafter radioPROTO-STARearlieststage of astar- wherenuclearfusion bginsBLACKHOLESstronggravitationalpull thateven lightcan't excapeBlueShiftAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthSTAR'SCOLORthis isaffected bytemperaturePLANETa largenaturalobject thatorbits a starlightyearthe distancelight travelsin a yearFUSIONconvertinghydrogento heliumin starsRedShiftthe shortestwavelengthin thespectrumgammaraysE.R.spectrumenergythat flowsfrom spacein wavesBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeABSOLUTEMAGNI-TUDEhow brighta starreally is14.5billionLUMIN-OSITYthebrightnessof a starNEBULAa cloud ofdust andgas inspacea telescopein space thatuses visiblelightHubbleRedSUPERGIANTin high massstars whenstar beginsto run out offuelMAINSEQUENCEstars thatare stablein their lifecyclea telescopein space thatuses infraredSpitzertelescoperadiothe longestwavelengthin thespectrumBigBangbithe wavelength oureyes canseevisiblelightstar left atthe core ofa planetarynebulaWhiteDwarf Surfacetemperaturethetemperatureof a starNEUTRONSTARtheremainsof a high-mass starIrregularGalaxygalaxy thathas noparticularshapeMilkyWayGalaxyourgalaxyEllipticalGalaxygalaxyshaped asan ovalHIGHMASSSTARa star withhighermass thanother starsa telescopein space thatuses x-rayChandraH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperatureSUPERNOVAred supergiantexplodesRedGIANTstar beginsto run out offuel in lowmass starsultra-violetthe wavelengthaftervisible lightLOWMASSSTARstars withlowermass thanother starsSpiralGalaxygalaxyshaped ina spiralEdwinHubble

ASTRONOMY - 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 wavelength after radio
    infrared
  2. earliest stage of a star- where nuclear fusion bgins
    PROTO-STAR
  3. strong gravitational pull that even light can't excape
    BLACK HOLES
  4. Blue Shift
  5. how bright a star appears here on Earth
    APPARENT MAGNI- TUDE
  6. this is affected by temperature
    STAR'S COLOR
  7. a large natural object that orbits a star
    PLANET
  8. the distance light travels in a year
    light year
  9. converting hydrogen to helium in stars
    FUSION
  10. Red Shift
  11. gamma rays
    the shortest wavelength in the spectrum
  12. energy that flows from space in waves
    E.R. spectrum
  13. what a medium-mass star becomes at the end of its life
    BLACK DWARF
  14. how bright a star really is
    ABSOLUTE MAGNI- TUDE
  15. 14.5 billion
  16. the brightness of a star
    LUMIN- OSITY
  17. a cloud of dust and gas in space
    NEBULA
  18. Hubble
    a telescope in space that uses visible light
  19. in high mass stars when star begins to run out of fuel
    Red SUPER GIANT
  20. stars that are stable in their life cycle
    MAIN SEQUENCE
  21. Spitzer telescope
    a telescope in space that uses infrared
  22. the longest wavelength in the spectrum
    radio
  23. bi
    Big Bang
  24. visible light
    the wave length our eyes can see
  25. White Dwarf
    star left at the core of a planetary nebula
  26. the temperature of a star
    Surface temperature
  27. the remains of a high-mass star
    NEUTRON STAR
  28. galaxy that has no particular shape
    Irregular Galaxy
  29. our galaxy
    Milky Way Galaxy
  30. galaxy shaped as an oval
    Elliptical Galaxy
  31. a star with higher mass than other stars
    HIGH MASS STAR
  32. Chandra
    a telescope in space that uses x-ray
  33. a diagram that compares stars' brightness, color and temperature
    H-R DIAGRAM
  34. red super giant explodes
    SUPERNOVA
  35. star begins to run out of fuel in low mass stars
    Red GIANT
  36. the wave length after visible light
    ultra-violet
  37. stars with lower mass than other stars
    LOW MASS STAR
  38. galaxy shaped in a spiral
    Spiral Galaxy
  39. Edwin Hubble