FrigidZonesthermal zone inwhich sun's raysstrike the Earth’ssurface at a widerangle and so thetemperatures arealways very low.Meridiansalso known aslines of longitude,they aresemicircles thatrun from onepole to the other.equinoxesoccurs duringspring and autumnwhen day+nightlast same length oftime around theworldParallelsalso called lines oflatitude, are circlesthat runperpendicular tothe axis of theEarth’s rotation.latitudedistance of anyone point onthe Earth fromtheEquator, can beN or S24hours'solar day'-amount of timeit takes forearth tocomplete onerotationtimezones24imaginary zonescorresponding toone hour ofEarth’s rotationthat we use tomeasure timeWinterseason that occursin Earth'shemisphere whenit is turned awayfrom sun during itsrevolutionScaleis the relationshipbetween a distancemeasured on themapand thecorrespondingdistance on Earthitself365 daysand 6hours'solar year' -time it takes forEarth tocomplete onerevolutionaround suncardinalpointsor basicpoints of referencethat we use toknow where weare on the Earthleapyearwhen an extraday is addedto Feb, occursevery fouryearswestto eastthedirectionof Earth'srotationEquatorThe main or 0°line of latitudewhich dividesthe Earth intotwo halves orhemispheresTropicalZonesthe thermal zone inwhich thetemperatures arealways high becausethe sun's rays strikethe Earthperpendicular or nearlyperpendicular to itssurfacegeographicgrida system ofcoordinatesused to locateany point ofEarth's surfaceon a mapchangefrom dayto nightone of theconsequencesof Earth'srotationlongitudedistance from anyone point on theEarth tothe 0° line of latitude,or the prime(Greenwich) meridianSystem ofProjectionName of themethod thatenables theEarth’s sphericalsurface to berepresented on aflat surface.solsticesoccurs duringwinter andsummer whenlength ofday+night isdifferent in eachhemispheredifferentlengths ofday and nightin differentplacesone of theconsequencesof Earth'srevolutionsaround the sunRotationrefers to themovement of earthas if spinning onan imaginary axisthat extends from theNorth to theSouth Poleeastone of thecardinalpointsmovementof sun onthehorizonone of theconsequencesof Earth'srotationFrigidZonesthermal zone inwhich sun's raysstrike the Earth’ssurface at a widerangle and so thetemperatures arealways very low.Meridiansalso known aslines of longitude,they aresemicircles thatrun from onepole to the other.equinoxesoccurs duringspring and autumnwhen day+nightlast same length oftime around theworldParallelsalso called lines oflatitude, are circlesthat runperpendicular tothe axis of theEarth’s rotation.latitudedistance of anyone point onthe Earth fromtheEquator, can beN or S24hours'solar day'-amount of timeit takes forearth tocomplete onerotationtimezones24imaginary zonescorresponding toone hour ofEarth’s rotationthat we use tomeasure timeWinterseason that occursin Earth'shemisphere whenit is turned awayfrom sun during itsrevolutionScaleis the relationshipbetween a distancemeasured on themapand thecorrespondingdistance on Earthitself365 daysand 6hours'solar year' -time it takes forEarth tocomplete onerevolutionaround suncardinalpointsor basicpoints of referencethat we use toknow where weare on the Earthleapyearwhen an extraday is addedto Feb, occursevery fouryearswestto eastthedirectionof Earth'srotationEquatorThe main or 0°line of latitudewhich dividesthe Earth intotwo halves orhemispheresTropicalZonesthe thermal zone inwhich thetemperatures arealways high becausethe sun's rays strikethe Earthperpendicular or nearlyperpendicular to itssurfacegeographicgrida system ofcoordinatesused to locateany point ofEarth's surfaceon a mapchangefrom dayto nightone of theconsequencesof Earth'srotationlongitudedistance from anyone point on theEarth tothe 0° line of latitude,or the prime(Greenwich) meridianSystem ofProjectionName of themethod thatenables theEarth’s sphericalsurface to berepresented on aflat surface.solsticesoccurs duringwinter andsummer whenlength ofday+night isdifferent in eachhemispheredifferentlengths ofday and nightin differentplacesone of theconsequencesof Earth'srevolutionsaround the sunRotationrefers to themovement of earthas if spinning onan imaginary axisthat extends from theNorth to theSouth Poleeastone of thecardinalpointsmovementof sun onthehorizonone of theconsequencesof Earth'srotation

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