24hours'solar day'-amount of timeit takes forearth tocomplete onerotationEquatorThe main or 0°line of latitudewhich dividesthe Earth intotwo halves orhemispheresSystem ofProjectionName of themethod thatenables theEarth’s sphericalsurface to berepresented on aflat surface.equinoxesoccurs duringspring and autumnwhen day+nightlast same length oftime around theworldRotationrefers to themovement of earthas if spinning onan imaginary axisthat extends from theNorth to theSouth PoleFrigidZonesthermal zone inwhich sun's raysstrike the Earth’ssurface at a widerangle and so thetemperatures arealways very low.solsticesoccurs duringwinter andsummer whenlength ofday+night isdifferent in eachhemisphereScaleis the relationshipbetween a distancemeasured on themapand thecorrespondingdistance on Earthitselfcardinalpointsor basicpoints of referencethat we use toknow where weare on the Earthgeographicgrida system ofcoordinatesused to locateany point ofEarth's surfaceon a mapTropicalZonesthe thermal zone inwhich thetemperatures arealways high becausethe sun's rays strikethe Earthperpendicular or nearlyperpendicular to itssurfacedifferentlengths ofday and nightin differentplacesone of theconsequencesof Earth'srevolutionsaround the sun365 daysand 6hours'solar year' -time it takes forEarth tocomplete onerevolutionaround sunleapyearwhen an extraday is addedto Feb, occursevery fouryearsParallelsalso called lines oflatitude, are circlesthat runperpendicular tothe axis of theEarth’s rotation.changefrom dayto nightone of theconsequencesof Earth'srotationlongitudedistance from anyone point on theEarth tothe 0° line of latitude,or the prime(Greenwich) meridianeastone of thecardinalpointswestto eastthedirectionof Earth'srotationlatitudedistance of anyone point onthe Earth fromtheEquator, can beN or SWinterseason that occursin Earth'shemisphere whenit is turned awayfrom sun during itsrevolutionMeridiansalso known aslines of longitude,they aresemicircles thatrun from onepole to the other.movementof sun onthehorizonone of theconsequencesof Earth'srotationtimezones24imaginary zonescorresponding toone hour ofEarth’s rotationthat we use tomeasure time24hours'solar day'-amount of timeit takes forearth tocomplete onerotationEquatorThe main or 0°line of latitudewhich dividesthe Earth intotwo halves orhemispheresSystem ofProjectionName of themethod thatenables theEarth’s sphericalsurface to berepresented on aflat surface.equinoxesoccurs duringspring and autumnwhen day+nightlast same length oftime around theworldRotationrefers to themovement of earthas if spinning onan imaginary axisthat extends from theNorth to theSouth PoleFrigidZonesthermal zone inwhich sun's raysstrike the Earth’ssurface at a widerangle and so thetemperatures arealways very low.solsticesoccurs duringwinter andsummer whenlength ofday+night isdifferent in eachhemisphereScaleis the relationshipbetween a distancemeasured on themapand thecorrespondingdistance on Earthitselfcardinalpointsor basicpoints of referencethat we use toknow where weare on the Earthgeographicgrida system ofcoordinatesused to locateany point ofEarth's surfaceon a mapTropicalZonesthe thermal zone inwhich thetemperatures arealways high becausethe sun's rays strikethe Earthperpendicular or nearlyperpendicular to itssurfacedifferentlengths ofday and nightin differentplacesone of theconsequencesof Earth'srevolutionsaround the sun365 daysand 6hours'solar year' -time it takes forEarth tocomplete onerevolutionaround sunleapyearwhen an extraday is addedto Feb, occursevery fouryearsParallelsalso called lines oflatitude, are circlesthat runperpendicular tothe axis of theEarth’s rotation.changefrom dayto nightone of theconsequencesof Earth'srotationlongitudedistance from anyone point on theEarth tothe 0° line of latitude,or the prime(Greenwich) meridianeastone of thecardinalpointswestto eastthedirectionof Earth'srotationlatitudedistance of anyone point onthe Earth fromtheEquator, can beN or SWinterseason that occursin Earth'shemisphere whenit is turned awayfrom sun during itsrevolutionMeridiansalso known aslines of longitude,they aresemicircles thatrun from onepole to the other.movementof sun onthehorizonone of theconsequencesof Earth'srotationtimezones24imaginary zonescorresponding toone hour ofEarth’s rotationthat we use tomeasure time

Unit One - 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. 'solar day'- amount of time it takes for earth to complete one rotation
    24 hours
  2. The main or 0° line of latitude which divides the Earth into two halves or hemispheres
    Equator
  3. Name of the method that enables the Earth’s spherical surface to be represented on a flat surface.
    System of Projection
  4. occurs during spring and autumn when day+night last same length of time around the world
    equinoxes
  5. refers to the movement of earth as if spinning on an imaginary axis that extends from the North to the South Pole
    Rotation
  6. thermal zone in which sun's rays strike the Earth’s surface at a wider angle and so the temperatures are always very low.
    Frigid Zones
  7. occurs during winter and summer when length of day+night is different in each hemisphere
    solstices
  8. is the relationship between a distance measured on the map and the corresponding distance on Earth itself
    Scale
  9. or basic points of reference that we use to know where we are on the Earth
    cardinal points
  10. a system of coordinates used to locate any point of Earth's surface on a map
    geographic grid
  11. the thermal zone in which the temperatures are always high because the sun's rays strike the Earth perpendicular or nearly perpendicular to its surface
    Tropical Zones
  12. one of the consequences of Earth's revolutions around the sun
    different lengths of day and night in different places
  13. 'solar year' - time it takes for Earth to complete one revolution around sun
    365 days and 6 hours
  14. when an extra day is added to Feb, occurs every four years
    leap year
  15. also called lines of latitude, are circles that run perpendicular to the axis of the Earth’s rotation.
    Parallels
  16. one of the consequences of Earth's rotation
    change from day to night
  17. distance from any one point on the Earth to the 0° line of latitude, or the prime (Greenwich) meridian
    longitude
  18. one of the cardinal points
    east
  19. the direction of Earth's rotation
    west to east
  20. distance of any one point on the Earth from the Equator, can be N or S
    latitude
  21. season that occurs in Earth's hemisphere when it is turned away from sun during its revolution
    Winter
  22. also known as lines of longitude, they are semicircles that run from one pole to the other.
    Meridians
  23. one of the consequences of Earth's rotation
    movement of sun on the horizon
  24. 24 imaginary zones corresponding to one hour of Earth’s rotation that we use to measure time
    time zones