elementa group ofall thesame typesof atomsresultsthe part ofthe labreport withobservationsand dataparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsamplitudetheheight ofa wavedaythe amount oftime it takesEarth torotate onceon its axisgalaxycollection ofstars, gas,dust, heldby gravitylithiumthe third mostcommonelement withan atomicnumber of 3electromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationconstellationa group of starsthat seem togroup togetherin interestingpatternsastronomythe studyof theuniverseuniversewhat containsall matter,energy,space, andtimescientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthselectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationBigBanga model andtheory thatexplains theorigin of theuniverseplasmamost commonstate of visiblematter in theuniverseelectrona particlewith anegativechargeclusterstara group of starsthat share acommon originthat are boundtogether bygravityperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementatomicnumberthe numberof protons intheelement'snucleusscientificmodela simplifiedrepresentationof a realsystemCMBRcosmicmicrowavebackgroundradiationmassamount ofmatter inan objectAUthe unit usedto measuredistanceswithin thesolar systemconclusionthe section ofthe lab reportwith a summaryof what waslearneddopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovinglightyearthe distancethat lighttravels inone Earthyearblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemhydrogenmostabundantelement withan atomicnumber of 1frequencynumber ofwavelengthsthat pass acertain point ina certainamount of timenucleuscenter of anatomcontainingprotons andneutronsstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterchangeof statewhen mattergoes fromone state toanotherHeliumthe secondmost abundantelement,atomic numberis 2whitedwarfa small densestar wherenuclear fusionis no longerhappeningnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itcarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6matteranythingthat takesup spacedensitymeasure ofamount ofspace; massper volumewavelengththe distancebetween twoadjacent peaksof anelectromagneticwavelight1 type ofelectromagneticradiation and isvisibledarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesmoleculeatoms thatare linkedtogether bysharingelectronsweightmeasureshow stronglygravity pullson the matterpresentgravityforce thatattractsobjects withmasstogethertelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studybinarystartwo starsthat revolvearoundeach otherelementa group ofall thesame typesof atomsresultsthe part ofthe labreport withobservationsand dataparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectsamplitudetheheight ofa wavedaythe amount oftime it takesEarth torotate onceon its axisgalaxycollection ofstars, gas,dust, heldby gravitylithiumthe third mostcommonelement withan atomicnumber of 3electromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationconstellationa group of starsthat seem togroup togetherin interestingpatternsastronomythe studyof theuniverseuniversewhat containsall matter,energy,space, andtimescientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionsabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthselectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationBigBanga model andtheory thatexplains theorigin of theuniverseplasmamost commonstate of visiblematter in theuniverseelectrona particlewith anegativechargeclusterstara group of starsthat share acommon originthat are boundtogether bygravityperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementatomicnumberthe numberof protons intheelement'snucleusscientificmodela simplifiedrepresentationof a realsystemCMBRcosmicmicrowavebackgroundradiationmassamount ofmatter inan objectAUthe unit usedto measuredistanceswithin thesolar systemconclusionthe section ofthe lab reportwith a summaryof what waslearneddopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovinglightyearthe distancethat lighttravels inone Earthyearblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemhydrogenmostabundantelement withan atomicnumber of 1frequencynumber ofwavelengthsthat pass acertain point ina certainamount of timenucleuscenter of anatomcontainingprotons andneutronsstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterchangeof statewhen mattergoes fromone state toanotherHeliumthe secondmost abundantelement,atomic numberis 2whitedwarfa small densestar wherenuclear fusionis no longerhappeningnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itcarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6matteranythingthat takesup spacedensitymeasure ofamount ofspace; massper volumewavelengththe distancebetween twoadjacent peaksof anelectromagneticwavelight1 type ofelectromagneticradiation and isvisibledarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesmoleculeatoms thatare linkedtogether bysharingelectronsweightmeasureshow stronglygravity pullson the matterpresentgravityforce thatattractsobjects withmasstogethertelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studybinarystartwo 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 all the same types of atoms
    element
  2. the part of the lab report with observations and data
    results
  3. apparent movement of nearby objects compared to more distant objects
    parallax shift
  4. the height of a wave
    amplitude
  5. the amount of time it takes Earth to rotate once on its axis
    day
  6. collection of stars, gas, dust, held by gravity
    galaxy
  7. the third most common element with an atomic number of 3
    lithium
  8. the electric and magnetic disturbance radiated from a source that travels through space, carrying energy and information
    electromagnetic radiation
  9. a group of stars that seem to group together in interesting patterns
    constellation
  10. the study of the universe
    astronomy
  11. what contains all matter, energy, space, and time
    universe
  12. an approach that uses six steps process relying on logic to ask and snswer questions
    scientific method
  13. spectrum showing dark lines or bands due to specific wavelengths
    absorption spectrum
  14. entire range of wavelengths of electro. magnetic radiation
    electromagnetic spectrum
  15. a model and theory that explains the origin of the universe
    Big Bang
  16. most common state of visible matter in the universe
    plasma
  17. a particle with a negative charge
    electron
  18. a group of stars that share a common origin that are bound together by gravity
    cluster star
  19. a chart with the names and chemical information for every type of atom or element
    periodic table of elements
  20. the number of protons in the element's nucleus
    atomic number
  21. a simplified representation of a real system
    scientific model
  22. cosmic microwave background radiation
    CMBR
  23. amount of matter in an object
    mass
  24. the unit used to measure distances within the solar system
    AU
  25. the section of the lab report with a summary of what was learned
    conclusion
  26. change in wavelength of electromagnetic radiation when the source is moving
    doppler effect
  27. the distance that light travels in one Earth year
    light year
  28. these have a gravitational pull that is so strong that matter, energy, and light are pulled into them
    black holes
  29. most abundant element with an atomic number of 1
    hydrogen
  30. number of wavelengths that pass a certain point in a certain amount of time
    frequency
  31. center of an atom containing protons and neutrons
    nucleus
  32. a massive ball of gas in space that produces its own light and heat through nuclear fusion
    star
  33. model of solor system that puts the sun at the center
    heliocentric model
  34. when matter goes from one state to another
    change of state
  35. the second most abundant element, atomic number is 2
    Helium
  36. a small dense star where nuclear fusion is no longer happening
    white dwarf
  37. when nuclei join together to form a heavier nucleus having more protons and neutrons in it
    nuclear fusion
  38. the sixth element in which all living organisms have and its atomic number is 6
    carbon
  39. anything that takes up space
    matter
  40. measure of amount of space; mass per volume
    density
  41. the distance between two adjacent peaks of an electromagnetic wave
    wavelength
  42. 1 type of electromagnetic radiation and is visible
    light
  43. type of matter that can be observed only indirectly through its gravitational effects on stars and galaxies
    dark matter
  44. atoms that are linked together by sharing electrons
    molecule
  45. measures how strongly gravity pulls on the matter present
    weight
  46. force that attracts objects with mass together
    gravity
  47. a device used to capture and focus large amounts of electromagnetic radiation for study
    telescope
  48. two stars that revolve around each other
    binary star