weightmeasureshow stronglygravity pullson the matterpresentchangeof statewhen mattergoes fromone state toanotherdaythe amount oftime it takesEarth torotate onceon its axisconclusionthe section ofthe lab reportwith a summaryof what waslearnedscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementclusterstara group of starsthat share acommon originthat are boundtogether bygravityabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsscientificmodela simplifiedrepresentationof a realsystemAUthe unit usedto measuredistanceswithin thesolar systemelementa group ofall thesame typesof atomsBigBanga model andtheory thatexplains theorigin of theuniversecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6Heliumthe secondmost abundantelement,atomic numberis 2plasmamost commonstate of visiblematter in theuniversematteranythingthat takesup spacetelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studystara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionlight1 type ofelectromagneticradiation and isvisibleconstellationa group of starsthat seem togroup togetherin interestingpatternsnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itgravityforce thatattractsobjects withmasstogetherastronomythe studyof theuniverseelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationhydrogenmostabundantelement withan atomicnumber of 1moleculeatoms thatare linkedtogether bysharingelectronsheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovinglithiumthe third mostcommonelement withan atomicnumber of 3wavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveelectrona particlewith anegativechargebinarystartwo starsthat revolvearoundeach otherwhitedwarfa small densestar wherenuclear fusionis no longerhappeningamplitudetheheight ofa waveelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsresultsthe part ofthe labreport withobservationsand datauniversewhat containsall matter,energy,space, andtimeblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeCMBRcosmicmicrowavebackgroundradiationgalaxycollection ofstars, gas,dust, heldby gravityatomicnumberthe numberof protons intheelement'snucleusdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieslightyearthe distancethat lighttravels inone Earthyearmassamount ofmatter inan objectdensitymeasure ofamount ofspace; massper volumenucleuscenter of anatomcontainingprotons andneutronsweightmeasureshow stronglygravity pullson the matterpresentchangeof statewhen mattergoes fromone state toanotherdaythe amount oftime it takesEarth torotate onceon its axisconclusionthe section ofthe lab reportwith a summaryof what waslearnedscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementclusterstara group of starsthat share acommon originthat are boundtogether bygravityabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsscientificmodela simplifiedrepresentationof a realsystemAUthe unit usedto measuredistanceswithin thesolar systemelementa group ofall thesame typesof atomsBigBanga model andtheory thatexplains theorigin of theuniversecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6Heliumthe secondmost abundantelement,atomic numberis 2plasmamost commonstate of visiblematter in theuniversematteranythingthat takesup spacetelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studystara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionlight1 type ofelectromagneticradiation and isvisibleconstellationa group of starsthat seem togroup togetherin interestingpatternsnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itgravityforce thatattractsobjects withmasstogetherastronomythe studyof theuniverseelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationhydrogenmostabundantelement withan atomicnumber of 1moleculeatoms thatare linkedtogether bysharingelectronsheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovinglithiumthe third mostcommonelement withan atomicnumber of 3wavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveelectrona particlewith anegativechargebinarystartwo starsthat revolvearoundeach otherwhitedwarfa small densestar wherenuclear fusionis no longerhappeningamplitudetheheight ofa waveelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsresultsthe part ofthe labreport withobservationsand datauniversewhat containsall matter,energy,space, andtimeblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeCMBRcosmicmicrowavebackgroundradiationgalaxycollection ofstars, gas,dust, heldby gravityatomicnumberthe numberof protons intheelement'snucleusdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieslightyearthe distancethat lighttravels inone Earthyearmassamount ofmatter inan objectdensitymeasure ofamount ofspace; massper volumenucleuscenter of anatomcontainingprotons andneutrons

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