carbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6weightmeasureshow stronglygravity pullson the matterpresentscientificmodela simplifiedrepresentationof a realsystemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingchangeof statewhen mattergoes fromone state toanotherlight1 type ofelectromagneticradiation and isvisibleelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieselectrona particlewith anegativechargeelementa group ofall thesame typesof atomsconclusionthe section ofthe lab reportwith a summaryof what waslearnedatomicnumberthe numberof protons intheelement'snucleustelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyplasmamost commonstate of visiblematter in theuniverselithiumthe third mostcommonelement withan atomicnumber of 3Heliumthe secondmost abundantelement,atomic numberis 2stara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionlightyearthe distancethat lighttravels inone Earthyearhydrogenmostabundantelement withan atomicnumber of 1heliocentricmodelmodel ofsolor systemthat puts thesun at thecentergravityforce thatattractsobjects withmasstogetherfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeBigBanga model andtheory thatexplains theorigin of theuniversemassamount ofmatter inan objectuniversewhat containsall matter,energy,space, andtimenucleuscenter of anatomcontainingprotons andneutronsdensitymeasure ofamount ofspace; massper volumewavelengththe distancebetween twoadjacent peaksof anelectromagneticwavebinarystartwo starsthat revolvearoundeach othernuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itwhitedwarfa small densestar wherenuclear fusionis no longerhappeningamplitudetheheight ofa wavescientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsdaythe amount oftime it takesEarth torotate onceon its axisperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementmoleculeatoms thatare linkedtogether bysharingelectronsblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationastronomythe studyof theuniverseAUthe unit usedto measuredistanceswithin thesolar systemconstellationa group of starsthat seem togroup togetherin interestingpatternsgalaxycollection ofstars, gas,dust, heldby gravityclusterstara group of starsthat share acommon originthat are boundtogether bygravityresultsthe part ofthe labreport withobservationsand dataparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsCMBRcosmicmicrowavebackgroundradiationabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsmatteranythingthat takesup spacecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6weightmeasureshow stronglygravity pullson the matterpresentscientificmodela simplifiedrepresentationof a realsystemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingchangeof statewhen mattergoes fromone state toanotherlight1 type ofelectromagneticradiation and isvisibleelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieselectrona particlewith anegativechargeelementa group ofall thesame typesof atomsconclusionthe section ofthe lab reportwith a summaryof what waslearnedatomicnumberthe numberof protons intheelement'snucleustelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyplasmamost commonstate of visiblematter in theuniverselithiumthe third mostcommonelement withan atomicnumber of 3Heliumthe secondmost abundantelement,atomic numberis 2stara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionlightyearthe distancethat lighttravels inone Earthyearhydrogenmostabundantelement withan atomicnumber of 1heliocentricmodelmodel ofsolor systemthat puts thesun at thecentergravityforce thatattractsobjects withmasstogetherfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeBigBanga model andtheory thatexplains theorigin of theuniversemassamount ofmatter inan objectuniversewhat containsall matter,energy,space, andtimenucleuscenter of anatomcontainingprotons andneutronsdensitymeasure ofamount ofspace; massper volumewavelengththe distancebetween twoadjacent peaksof anelectromagneticwavebinarystartwo starsthat revolvearoundeach othernuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itwhitedwarfa small densestar wherenuclear fusionis no longerhappeningamplitudetheheight ofa wavescientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsdaythe amount oftime it takesEarth torotate onceon its axisperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementmoleculeatoms thatare linkedtogether bysharingelectronsblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationastronomythe studyof theuniverseAUthe unit usedto measuredistanceswithin thesolar systemconstellationa group of starsthat seem togroup togetherin interestingpatternsgalaxycollection ofstars, gas,dust, heldby gravityclusterstara group of starsthat share acommon originthat are boundtogether bygravityresultsthe part ofthe labreport withobservationsand dataparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsCMBRcosmicmicrowavebackgroundradiationabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsmatteranythingthat takesup space

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