clusterstara group of starsthat share acommon originthat are boundtogether bygravitycarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6lightyearthe distancethat lighttravels inone Earthyeargalaxycollection ofstars, gas,dust, heldby gravityCMBRcosmicmicrowavebackgroundradiationuniversewhat containsall matter,energy,space, andtimeblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsconstellationa group of starsthat seem togroup togetherin interestingpatternsresultsthe part ofthe labreport withobservationsand datahydrogenmostabundantelement withan atomicnumber of 1parallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementheliocentricmodelmodel ofsolor systemthat puts thesun at thecentermoleculeatoms thatare linkedtogether bysharingelectronsnucleuscenter of anatomcontainingprotons andneutronswhitedwarfa small densestar wherenuclear fusionis no longerhappeningweightmeasureshow stronglygravity pullson the matterpresentconclusionthe section ofthe lab reportwith a summaryof what waslearnedabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthselectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationelectrona particlewith anegativechargeAUthe unit usedto measuredistanceswithin thesolar systemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingatomicnumberthe numberof protons intheelement'snucleusdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesdensitymeasure ofamount ofspace; massper volumeelementa group ofall thesame typesof atomsHeliumthe secondmost abundantelement,atomic numberis 2matteranythingthat takesup spacestara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusiondaythe amount oftime it takesEarth torotate onceon its axisfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timegravityforce thatattractsobjects withmasstogetherlithiumthe third mostcommonelement withan atomicnumber of 3electromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationamplitudetheheight ofa waveastronomythe studyof theuniversenuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in ittelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyplasmamost commonstate of visiblematter in theuniversechangeof statewhen mattergoes fromone state toanotherBigBanga model andtheory thatexplains theorigin of theuniversescientificmodela simplifiedrepresentationof a realsystemmassamount ofmatter inan objectwavelengththe distancebetween twoadjacent peaksof anelectromagneticwavelight1 type ofelectromagneticradiation and isvisiblebinarystartwo starsthat revolvearoundeach otherclusterstara group of starsthat share acommon originthat are boundtogether bygravitycarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6lightyearthe distancethat lighttravels inone Earthyeargalaxycollection ofstars, gas,dust, heldby gravityCMBRcosmicmicrowavebackgroundradiationuniversewhat containsall matter,energy,space, andtimeblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsconstellationa group of starsthat seem togroup togetherin interestingpatternsresultsthe part ofthe labreport withobservationsand datahydrogenmostabundantelement withan atomicnumber of 1parallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementheliocentricmodelmodel ofsolor systemthat puts thesun at thecentermoleculeatoms thatare linkedtogether bysharingelectronsnucleuscenter of anatomcontainingprotons andneutronswhitedwarfa small densestar wherenuclear fusionis no longerhappeningweightmeasureshow stronglygravity pullson the matterpresentconclusionthe section ofthe lab reportwith a summaryof what waslearnedabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthselectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationelectrona particlewith anegativechargeAUthe unit usedto measuredistanceswithin thesolar systemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingatomicnumberthe numberof protons intheelement'snucleusdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesdensitymeasure ofamount ofspace; massper volumeelementa group ofall thesame typesof atomsHeliumthe secondmost abundantelement,atomic numberis 2matteranythingthat takesup spacestara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusiondaythe amount oftime it takesEarth torotate onceon its axisfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timegravityforce thatattractsobjects withmasstogetherlithiumthe third mostcommonelement withan atomicnumber of 3electromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationamplitudetheheight ofa waveastronomythe studyof theuniversenuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in ittelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyplasmamost commonstate of visiblematter in theuniversechangeof statewhen mattergoes fromone state toanotherBigBanga model andtheory thatexplains theorigin of theuniversescientificmodela simplifiedrepresentationof a realsystemmassamount ofmatter inan objectwavelengththe distancebetween twoadjacent peaksof anelectromagneticwavelight1 type ofelectromagneticradiation and isvisiblebinarystartwo starsthat revolvearoundeach other

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