gravityforce thatattractsobjects withmasstogetherfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timedensitymeasure ofamount ofspace; massper volumemoleculeatoms thatare linkedtogether bysharingelectronselementa group ofall thesame typesof atomsBigBanga model andtheory thatexplains theorigin of theuniverseelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterconclusionthe section ofthe lab reportwith a summaryof what waslearnedchangeof statewhen mattergoes fromone state toanotherelectrona particlewith anegativechargeelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationmassamount ofmatter inan objecthydrogenmostabundantelement withan atomicnumber of 1binarystartwo starsthat revolvearoundeach otherstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionastronomythe studyof theuniversewhitedwarfa small densestar wherenuclear fusionis no longerhappeningclusterstara group of starsthat share acommon originthat are boundtogether bygravitylightyearthe distancethat lighttravels inone Earthyearlight1 type ofelectromagneticradiation and isvisibleamplitudetheheight ofa waveCMBRcosmicmicrowavebackgroundradiationatomicnumberthe numberof protons intheelement'snucleusresultsthe part ofthe labreport withobservationsand datascientificmodela simplifiedrepresentationof a realsystemlithiumthe third mostcommonelement withan atomicnumber of 3nucleuscenter of anatomcontainingprotons andneutronsweightmeasureshow stronglygravity pullson the matterpresentdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingmatteranythingthat takesup spaceabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthscarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6universewhat containsall matter,energy,space, andtimedarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesdaythe amount oftime it takesEarth torotate onceon its axisparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itwavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemAUthe unit usedto measuredistanceswithin thesolar systemtelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyconstellationa group of starsthat seem togroup togetherin interestingpatternsplasmamost commonstate of visiblematter in theuniversegalaxycollection ofstars, gas,dust, heldby gravityHeliumthe secondmost abundantelement,atomic numberis 2gravityforce thatattractsobjects withmasstogetherfrequencynumber ofwavelengthsthat pass acertain point ina certainamount of timedensitymeasure ofamount ofspace; massper volumemoleculeatoms thatare linkedtogether bysharingelectronselementa group ofall thesame typesof atomsBigBanga model andtheory thatexplains theorigin of theuniverseelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterconclusionthe section ofthe lab reportwith a summaryof what waslearnedchangeof statewhen mattergoes fromone state toanotherelectrona particlewith anegativechargeelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationmassamount ofmatter inan objecthydrogenmostabundantelement withan atomicnumber of 1binarystartwo starsthat revolvearoundeach otherstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionastronomythe studyof theuniversewhitedwarfa small densestar wherenuclear fusionis no longerhappeningclusterstara group of starsthat share acommon originthat are boundtogether bygravitylightyearthe distancethat lighttravels inone Earthyearlight1 type ofelectromagneticradiation and isvisibleamplitudetheheight ofa waveCMBRcosmicmicrowavebackgroundradiationatomicnumberthe numberof protons intheelement'snucleusresultsthe part ofthe labreport withobservationsand datascientificmodela simplifiedrepresentationof a realsystemlithiumthe third mostcommonelement withan atomicnumber of 3nucleuscenter of anatomcontainingprotons andneutronsweightmeasureshow stronglygravity pullson the matterpresentdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingmatteranythingthat takesup spaceabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthscarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6universewhat containsall matter,energy,space, andtimedarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesdaythe amount oftime it takesEarth torotate onceon its axisparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itwavelengththe distancebetween twoadjacent peaksof anelectromagneticwaveblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemAUthe unit usedto measuredistanceswithin thesolar systemtelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studyconstellationa group of starsthat seem togroup togetherin interestingpatternsplasmamost commonstate of visiblematter in theuniversegalaxycollection ofstars, gas,dust, heldby gravityHeliumthe secondmost abundantelement,atomic numberis 2

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