constellationa group of starsthat seem togroup togetherin interestingpatternsdensitymeasure ofamount ofspace; massper volumeperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementplasmamost commonstate of visiblematter in theuniverseuniversewhat containsall matter,energy,space, andtimeweightmeasureshow stronglygravity pullson the matterpresentgravityforce thatattractsobjects withmasstogetherelectrona particlewith anegativechargeparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionmassamount ofmatter inan objectscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsHeliumthe secondmost abundantelement,atomic numberis 2scientificmodela simplifiedrepresentationof a realsystemlight1 type ofelectromagneticradiation and isvisiblecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6lithiumthe third mostcommonelement withan atomicnumber of 3conclusionthe section ofthe lab reportwith a summaryof what waslearneddopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingdaythe amount oftime it takesEarth torotate onceon its axisBigBanga model andtheory thatexplains theorigin of theuniversedarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieshydrogenmostabundantelement withan atomicnumber of 1resultsthe part ofthe labreport withobservationsand datanucleuscenter of anatomcontainingprotons andneutronslightyearthe distancethat lighttravels inone Earthyeartelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyamplitudetheheight ofa waveelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterelementa group ofall thesame typesof atomsnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itwavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveatomicnumberthe numberof protons intheelement'snucleusbinarystartwo starsthat revolvearoundeach otherabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsclusterstara group of starsthat share acommon originthat are boundtogether bygravityelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationmatteranythingthat takesup spacewhitedwarfa small densestar wherenuclear fusionis no longerhappeningchangeof statewhen mattergoes fromone state toanothermoleculeatoms thatare linkedtogether bysharingelectronsgalaxycollection ofstars, gas,dust, heldby gravityfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeAUthe unit usedto measuredistanceswithin thesolar systemblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemastronomythe studyof theuniverseCMBRcosmicmicrowavebackgroundradiationconstellationa group of starsthat seem togroup togetherin interestingpatternsdensitymeasure ofamount ofspace; massper volumeperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementplasmamost commonstate of visiblematter in theuniverseuniversewhat containsall matter,energy,space, andtimeweightmeasureshow stronglygravity pullson the matterpresentgravityforce thatattractsobjects withmasstogetherelectrona particlewith anegativechargeparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionmassamount ofmatter inan objectscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsHeliumthe secondmost abundantelement,atomic numberis 2scientificmodela simplifiedrepresentationof a realsystemlight1 type ofelectromagneticradiation and isvisiblecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6lithiumthe third mostcommonelement withan atomicnumber of 3conclusionthe section ofthe lab reportwith a summaryof what waslearneddopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingdaythe amount oftime it takesEarth torotate onceon its axisBigBanga model andtheory thatexplains theorigin of theuniversedarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxieshydrogenmostabundantelement withan atomicnumber of 1resultsthe part ofthe labreport withobservationsand datanucleuscenter of anatomcontainingprotons andneutronslightyearthe distancethat lighttravels inone Earthyeartelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyamplitudetheheight ofa waveelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterelementa group ofall thesame typesof atomsnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itwavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveatomicnumberthe numberof protons intheelement'snucleusbinarystartwo starsthat revolvearoundeach otherabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthsclusterstara group of starsthat share acommon originthat are boundtogether bygravityelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationmatteranythingthat takesup spacewhitedwarfa small densestar wherenuclear fusionis no longerhappeningchangeof statewhen mattergoes fromone state toanothermoleculeatoms thatare linkedtogether bysharingelectronsgalaxycollection ofstars, gas,dust, heldby gravityfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeAUthe unit usedto measuredistanceswithin thesolar systemblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemastronomythe studyof theuniverseCMBRcosmicmicrowavebackgroundradiation

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