hydrogenmostabundantelement withan atomicnumber of 1daythe amount oftime it takesEarth torotate onceon its axisatomicnumberthe numberof protons intheelement'snucleusscientificmodela simplifiedrepresentationof a realsystemmatteranythingthat takesup spaceclusterstara group of starsthat share acommon originthat are boundtogether bygravitywhitedwarfa small densestar wherenuclear fusionis no longerhappeningwavelengththe distancebetween twoadjacent peaksof anelectromagneticwavecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6CMBRcosmicmicrowavebackgroundradiationelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationmassamount ofmatter inan objectblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itAUthe unit usedto measuredistanceswithin thesolar systemscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionslithiumthe third mostcommonelement withan atomicnumber of 3nucleuscenter of anatomcontainingprotons andneutronsgalaxycollection ofstars, gas,dust, heldby gravitylightyearthe distancethat lighttravels inone EarthyearBigBanga model andtheory thatexplains theorigin of theuniversechangeof statewhen mattergoes fromone state toanotherplasmamost commonstate of visiblematter in theuniverseperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesconstellationa group of starsthat seem togroup togetherin interestingpatternsconclusionthe section ofthe lab reportwith a summaryof what waslearnedmoleculeatoms thatare linkedtogether bysharingelectronsbinarystartwo starsthat revolvearoundeach otherweightmeasureshow stronglygravity pullson the matterpresentelementa group ofall thesame typesof atomsresultsthe part ofthe labreport withobservationsand dataelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationgravityforce thatattractsobjects withmasstogethertelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studylight1 type ofelectromagneticradiation and isvisibledensitymeasure ofamount ofspace; massper volumeabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthselectrona particlewith anegativechargeheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionastronomythe studyof theuniverseuniversewhat containsall matter,energy,space, andtimeamplitudetheheight ofa waveHeliumthe secondmost abundantelement,atomic numberis 2frequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjectshydrogenmostabundantelement withan atomicnumber of 1daythe amount oftime it takesEarth torotate onceon its axisatomicnumberthe numberof protons intheelement'snucleusscientificmodela simplifiedrepresentationof a realsystemmatteranythingthat takesup spaceclusterstara group of starsthat share acommon originthat are boundtogether bygravitywhitedwarfa small densestar wherenuclear fusionis no longerhappeningwavelengththe distancebetween twoadjacent peaksof anelectromagneticwavecarbonthe sixthelement inwhich all livingorganisms haveand its atomicnumber is 6CMBRcosmicmicrowavebackgroundradiationelectromagneticspectrumentire range ofwavelengths ofelectro.magneticradiationmassamount ofmatter inan objectblackholesthese have agravitational pullthat is so strongthat matter,energy, and lightare pulled intothemdopplereffectchange inwavelength ofelectromagneticradiation whenthe source ismovingnuclearfusionwhen nuclei jointogether to form aheavier nucleushaving moreprotons andneutrons in itAUthe unit usedto measuredistanceswithin thesolar systemscientificmethodan approach thatuses six stepsprocess relyingon logic to askand snswerquestionslithiumthe third mostcommonelement withan atomicnumber of 3nucleuscenter of anatomcontainingprotons andneutronsgalaxycollection ofstars, gas,dust, heldby gravitylightyearthe distancethat lighttravels inone EarthyearBigBanga model andtheory thatexplains theorigin of theuniversechangeof statewhen mattergoes fromone state toanotherplasmamost commonstate of visiblematter in theuniverseperiodictable ofelementsa chart with thenames andchemicalinformation forevery type ofatom or elementdarkmattertype of matter thatcan be observedonly indirectlythrough itsgravitationaleffects on starsand galaxiesconstellationa group of starsthat seem togroup togetherin interestingpatternsconclusionthe section ofthe lab reportwith a summaryof what waslearnedmoleculeatoms thatare linkedtogether bysharingelectronsbinarystartwo starsthat revolvearoundeach otherweightmeasureshow stronglygravity pullson the matterpresentelementa group ofall thesame typesof atomsresultsthe part ofthe labreport withobservationsand dataelectromagneticradiationthe electric andmagnetic disturbanceradiated from asource that travelsthrough space,carrying energy andinformationgravityforce thatattractsobjects withmasstogethertelescopea device used tocapture and focuslarge amounts ofelectromagneticradiation for studylight1 type ofelectromagneticradiation and isvisibledensitymeasure ofamount ofspace; massper volumeabsorptionspectrumspectrumshowing darklines or bandsdue to specificwavelengthselectrona particlewith anegativechargeheliocentricmodelmodel ofsolor systemthat puts thesun at thecenterstara massive ball ofgas in spacethat produces itsown light andheat throughnuclear fusionastronomythe studyof theuniverseuniversewhat containsall matter,energy,space, andtimeamplitudetheheight ofa waveHeliumthe secondmost abundantelement,atomic numberis 2frequencynumber ofwavelengthsthat pass acertain point ina certainamount of timeparallaxshiftapparentmovement ofnearby objectscompared tomore distantobjects

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