star left atthe core ofa planetarynebulaWhiteDwarf the shortestwavelengthin thespectrumgammaraysIrregularGalaxygalaxy thathas noparticularshape14.5billionSpiralGalaxygalaxyshaped ina spiralE.R.spectrumenergythat flowsfrom spacein wavesMAINSEQUENCEstars thatare stablein their lifecycleNEUTRONSTARtheremainsof a high-mass starBLACKHOLESstronggravitationalpull thateven lightcan't excapeRedShiftthe wavelength oureyes canseevisiblelightBigBangbiBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperaturePLANETa largenaturalobject thatorbits a starRedGIANTstar beginsto run out offuel in lowmass starsLUMIN-OSITYthebrightnessof a starPROTO-STARearlieststage of astar- wherenuclearfusion bginsEllipticalGalaxygalaxyshaped asan ovalHIGHMASSSTARa star withhighermass thanother starsBlueShifta telescopein space thatuses infraredSpitzertelescopeABSOLUTEMAGNI-TUDEhow brighta starreally isAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthRedSUPERGIANTin high massstars whenstar beginsto run out offuellightyearthe distancelight travelsin a yearSurfacetemperaturethetemperatureof a starultra-violetthe wavelengthaftervisible lightSUPERNOVAred supergiantexplodesSTAR'SCOLORthis isaffected bytemperatureMilkyWayGalaxyourgalaxyFUSIONconvertinghydrogento heliumin starsa telescopein space thatuses x-rayChandraLOWMASSSTARstars withlowermass thanother starsradiothe longestwavelengthin thespectrumEdwinHubbleinfraredthewavelengthafter radioa telescopein space thatuses visiblelightHubbleNEBULAa cloud ofdust andgas inspacestar left atthe core ofa planetarynebulaWhiteDwarf the shortestwavelengthin thespectrumgammaraysIrregularGalaxygalaxy thathas noparticularshape14.5billionSpiralGalaxygalaxyshaped ina spiralE.R.spectrumenergythat flowsfrom spacein wavesMAINSEQUENCEstars thatare stablein their lifecycleNEUTRONSTARtheremainsof a high-mass starBLACKHOLESstronggravitationalpull thateven lightcan't excapeRedShiftthe wavelength oureyes canseevisiblelightBigBangbiBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperaturePLANETa largenaturalobject thatorbits a starRedGIANTstar beginsto run out offuel in lowmass starsLUMIN-OSITYthebrightnessof a starPROTO-STARearlieststage of astar- wherenuclearfusion bginsEllipticalGalaxygalaxyshaped asan ovalHIGHMASSSTARa star withhighermass thanother starsBlueShifta telescopein space thatuses infraredSpitzertelescopeABSOLUTEMAGNI-TUDEhow brighta starreally isAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthRedSUPERGIANTin high massstars whenstar beginsto run out offuellightyearthe distancelight travelsin a yearSurfacetemperaturethetemperatureof a starultra-violetthe wavelengthaftervisible lightSUPERNOVAred supergiantexplodesSTAR'SCOLORthis isaffected bytemperatureMilkyWayGalaxyourgalaxyFUSIONconvertinghydrogento heliumin starsa telescopein space thatuses x-rayChandraLOWMASSSTARstars withlowermass thanother starsradiothe longestwavelengthin thespectrumEdwinHubbleinfraredthewavelengthafter radioa telescopein space thatuses visiblelightHubbleNEBULAa cloud ofdust andgas inspace

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