RedShiftH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperatureNEUTRONSTARtheremainsof a high-mass starIrregularGalaxygalaxy thathas noparticularshapePROTO-STARearlieststage of astar- wherenuclearfusion bginsRedSUPERGIANTin high massstars whenstar beginsto run out offuelBigBangbiSurfacetemperaturethetemperatureof a starFUSIONconvertinghydrogento heliumin starsABSOLUTEMAGNI-TUDEhow brighta starreally isEdwinHubblelightyearthe distancelight travelsin a yeara telescopein space thatuses infraredSpitzertelescopeBlueShiftinfraredthewavelengthafter radioRedGIANTstar beginsto run out offuel in lowmass starsMilkyWayGalaxyourgalaxyNEBULAa cloud ofdust andgas inspaceBLACKHOLESstronggravitationalpull thateven lightcan't excapeultra-violetthe wavelengthaftervisible lightradiothe longestwavelengthin thespectrum14.5billionthe wavelength oureyes canseevisiblelightE.R.spectrumenergythat flowsfrom spacein wavesLOWMASSSTARstars withlowermass thanother starsSUPERNOVAred supergiantexplodesa telescopein space thatuses x-rayChandrathe shortestwavelengthin thespectrumgammaraysSTAR'SCOLORthis isaffected bytemperatureBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthSpiralGalaxygalaxyshaped ina spiralstar left atthe core ofa planetarynebulaWhiteDwarf a telescopein space thatuses visiblelightHubbleLUMIN-OSITYthebrightnessof a starHIGHMASSSTARa star withhighermass thanother starsMAINSEQUENCEstars thatare stablein their lifecyclePLANETa largenaturalobject thatorbits a starEllipticalGalaxygalaxyshaped asan ovalRedShiftH-RDIAGRAMa diagram thatcompares stars'brightness, colorand temperatureNEUTRONSTARtheremainsof a high-mass starIrregularGalaxygalaxy thathas noparticularshapePROTO-STARearlieststage of astar- wherenuclearfusion bginsRedSUPERGIANTin high massstars whenstar beginsto run out offuelBigBangbiSurfacetemperaturethetemperatureof a starFUSIONconvertinghydrogento heliumin starsABSOLUTEMAGNI-TUDEhow brighta starreally isEdwinHubblelightyearthe distancelight travelsin a yeara telescopein space thatuses infraredSpitzertelescopeBlueShiftinfraredthewavelengthafter radioRedGIANTstar beginsto run out offuel in lowmass starsMilkyWayGalaxyourgalaxyNEBULAa cloud ofdust andgas inspaceBLACKHOLESstronggravitationalpull thateven lightcan't excapeultra-violetthe wavelengthaftervisible lightradiothe longestwavelengthin thespectrum14.5billionthe wavelength oureyes canseevisiblelightE.R.spectrumenergythat flowsfrom spacein wavesLOWMASSSTARstars withlowermass thanother starsSUPERNOVAred supergiantexplodesa telescopein space thatuses x-rayChandrathe shortestwavelengthin thespectrumgammaraysSTAR'SCOLORthis isaffected bytemperatureBLACKDWARFwhat amedium-massstar becomesat the end ofits lifeAPPARENTMAGNI-TUDEhow bright astar appearshere onEarthSpiralGalaxygalaxyshaped ina spiralstar left atthe core ofa planetarynebulaWhiteDwarf a telescopein space thatuses visiblelightHubbleLUMIN-OSITYthebrightnessof a starHIGHMASSSTARa star withhighermass thanother starsMAINSEQUENCEstars thatare stablein their lifecyclePLANETa largenaturalobject thatorbits a starEllipticalGalaxygalaxyshaped asan oval

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