PROTO-STARearlieststage of astar- wherenuclearfusion bginsSurfacetemperaturethetemperatureof a starradiothe longestwavelengthin thespectrumAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthSTAR'SCOLORthis isaffected bytemperatureBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeE.R.spectrumenergythat flowsfrom spacein waveslightyearthe distancelight travelsin a yearNEBULAa cloud ofdust andgas inspaceLUMIN-OSITYthebrightnessof a starRedGIANTstar beginsto run out offuel in lowmass starsEdwinHubbleMAINSEQUENCEstars thatare stablein their lifecycleBLACKHOLESstronggravitationalpull thateven lightcan't excapeBigBangbiultra-violetthe wavelengthaftervisible lightthe wavelength oureyes canseevisiblelightthe shortestwavelengthin thespectrumgammaraysNEUTRONSTARtheremainsof a high-mass stara telescopein space thatuses visiblelightHubbleRedSUPERGIANTin high massstars whenstar beginsto run out offuelSUPERNOVAred supergiantexplodesMilkyWayGalaxyourgalaxyEllipticalGalaxygalaxyshaped asan ovala telescopein space thatuses infraredSpitzertelescopeHIGHMASSSTARa star withhighermass thanother starsSpiralGalaxygalaxyshaped ina spiral14.5billionRedShiftBlueShiftinfraredthewavelengthafter radioLOWMASSSTARstars withlowermass thanother starsFUSIONconvertinghydrogento heliumin starsstar left atthe core ofa planetarynebulaWhiteDwarf PLANETa largenaturalobject thatorbits a stara telescopein space thatuses x-rayChandraABSOLUTEMAGNI-TUDEhow brighta starreally isIrregularGalaxygalaxy thathas noparticularshapeH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperaturePROTO-STARearlieststage of astar- wherenuclearfusion bginsSurfacetemperaturethetemperatureof a starradiothe longestwavelengthin thespectrumAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthSTAR'SCOLORthis isaffected bytemperatureBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeE.R.spectrumenergythat flowsfrom spacein waveslightyearthe distancelight travelsin a yearNEBULAa cloud ofdust andgas inspaceLUMIN-OSITYthebrightnessof a starRedGIANTstar beginsto run out offuel in lowmass starsEdwinHubbleMAINSEQUENCEstars thatare stablein their lifecycleBLACKHOLESstronggravitationalpull thateven lightcan't excapeBigBangbiultra-violetthe wavelengthaftervisible lightthe wavelength oureyes canseevisiblelightthe shortestwavelengthin thespectrumgammaraysNEUTRONSTARtheremainsof a high-mass stara telescopein space thatuses visiblelightHubbleRedSUPERGIANTin high massstars whenstar beginsto run out offuelSUPERNOVAred supergiantexplodesMilkyWayGalaxyourgalaxyEllipticalGalaxygalaxyshaped asan ovala telescopein space thatuses infraredSpitzertelescopeHIGHMASSSTARa star withhighermass thanother starsSpiralGalaxygalaxyshaped ina spiral14.5billionRedShiftBlueShiftinfraredthewavelengthafter radioLOWMASSSTARstars withlowermass thanother starsFUSIONconvertinghydrogento heliumin starsstar left atthe core ofa planetarynebulaWhiteDwarf PLANETa largenaturalobject thatorbits a stara telescopein space thatuses x-rayChandraABSOLUTEMAGNI-TUDEhow brighta starreally isIrregularGalaxygalaxy thathas noparticularshapeH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperature

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