365 daysand 6hours'solar year' -time it takes forEarth tocomplete onerevolutionaround sunFrigidZonesthermal zone inwhich sun's raysstrike the Earth’ssurface at a widerangle and so thetemperatures arealways very low.latitudedistance of anyone point onthe Earth fromtheEquator, can beN or STropicalZonesthe thermal zone inwhich thetemperatures arealways high becausethe sun's rays strikethe Earthperpendicular or nearlyperpendicular to itssurfaceeastone of thecardinalpointsScaleis the relationshipbetween a distancemeasured on themapand thecorrespondingdistance on Earthitselfmovementof sun onthehorizonone of theconsequencesof Earth'srotationcardinalpointsor basicpoints of referencethat we use toknow where weare on the Earthsolsticesoccurs duringwinter andsummer whenlength ofday+night isdifferent in eachhemispheretimezones24imaginary zonescorresponding toone hour ofEarth’s rotationthat we use tomeasure time24hours'solar day'-amount of timeit takes forearth tocomplete onerotationRotationrefers to themovement of earthas if spinning onan imaginary axisthat extends from theNorth to theSouth PoleWinterseason that occursin Earth'shemisphere whenit is turned awayfrom sun during itsrevolutionEquatorThe main or 0°line of latitudewhich dividesthe Earth intotwo halves orhemispheresleapyearwhen an extraday is addedto Feb, occursevery fouryearsequinoxesoccurs duringspring and autumnwhen day+nightlast same length oftime around theworldMeridiansalso known aslines of longitude,they aresemicircles thatrun from onepole to the other.System ofProjectionName of themethod thatenables theEarth’s sphericalsurface to berepresented on aflat surface.Parallelsalso called lines oflatitude, are circlesthat runperpendicular tothe axis of theEarth’s rotation.differentlengths ofday and nightin differentplacesone of theconsequencesof Earth'srevolutionsaround the sunchangefrom dayto nightone of theconsequencesof Earth'srotationgeographicgrida system ofcoordinatesused to locateany point ofEarth's surfaceon a maplongitudedistance from anyone point on theEarth tothe 0° line of latitude,or the prime(Greenwich) meridianwestto eastthedirectionof Earth'srotation365 daysand 6hours'solar year' -time it takes forEarth tocomplete onerevolutionaround sunFrigidZonesthermal zone inwhich sun's raysstrike the Earth’ssurface at a widerangle and so thetemperatures arealways very low.latitudedistance of anyone point onthe Earth fromtheEquator, can beN or STropicalZonesthe thermal zone inwhich thetemperatures arealways high becausethe sun's rays strikethe Earthperpendicular or nearlyperpendicular to itssurfaceeastone of thecardinalpointsScaleis the relationshipbetween a distancemeasured on themapand thecorrespondingdistance on Earthitselfmovementof sun onthehorizonone of theconsequencesof Earth'srotationcardinalpointsor basicpoints of referencethat we use toknow where weare on the Earthsolsticesoccurs duringwinter andsummer whenlength ofday+night isdifferent in eachhemispheretimezones24imaginary zonescorresponding toone hour ofEarth’s rotationthat we use tomeasure time24hours'solar day'-amount of timeit takes forearth tocomplete onerotationRotationrefers to themovement of earthas if spinning onan imaginary axisthat extends from theNorth to theSouth PoleWinterseason that occursin Earth'shemisphere whenit is turned awayfrom sun during itsrevolutionEquatorThe main or 0°line of latitudewhich dividesthe Earth intotwo halves orhemispheresleapyearwhen an extraday is addedto Feb, occursevery fouryearsequinoxesoccurs duringspring and autumnwhen day+nightlast same length oftime around theworldMeridiansalso known aslines of longitude,they aresemicircles thatrun from onepole to the other.System ofProjectionName of themethod thatenables theEarth’s sphericalsurface to berepresented on aflat surface.Parallelsalso called lines oflatitude, are circlesthat runperpendicular tothe axis of theEarth’s rotation.differentlengths ofday and nightin differentplacesone of theconsequencesof Earth'srevolutionsaround the sunchangefrom dayto nightone of theconsequencesof Earth'srotationgeographicgrida system ofcoordinatesused to locateany point ofEarth's surfaceon a maplongitudedistance from anyone point on theEarth tothe 0° line of latitude,or the prime(Greenwich) meridianwestto eastthedirectionof 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. 'solar year' - time it takes for Earth to complete one revolution around sun
    365 days and 6 hours
  2. 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
  3. distance of any one point on the Earth from the Equator, can be N or S
    latitude
  4. 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
  5. one of the cardinal points
    east
  6. is the relationship between a distance measured on the map and the corresponding distance on Earth itself
    Scale
  7. one of the consequences of Earth's rotation
    movement of sun on the horizon
  8. or basic points of reference that we use to know where we are on the Earth
    cardinal points
  9. occurs during winter and summer when length of day+night is different in each hemisphere
    solstices
  10. 24 imaginary zones corresponding to one hour of Earth’s rotation that we use to measure time
    time zones
  11. 'solar day'- amount of time it takes for earth to complete one rotation
    24 hours
  12. refers to the movement of earth as if spinning on an imaginary axis that extends from the North to the South Pole
    Rotation
  13. season that occurs in Earth's hemisphere when it is turned away from sun during its revolution
    Winter
  14. The main or 0° line of latitude which divides the Earth into two halves or hemispheres
    Equator
  15. when an extra day is added to Feb, occurs every four years
    leap year
  16. occurs during spring and autumn when day+night last same length of time around the world
    equinoxes
  17. also known as lines of longitude, they are semicircles that run from one pole to the other.
    Meridians
  18. Name of the method that enables the Earth’s spherical surface to be represented on a flat surface.
    System of Projection
  19. also called lines of latitude, are circles that run perpendicular to the axis of the Earth’s rotation.
    Parallels
  20. one of the consequences of Earth's revolutions around the sun
    different lengths of day and night in different places
  21. one of the consequences of Earth's rotation
    change from day to night
  22. a system of coordinates used to locate any point of Earth's surface on a map
    geographic grid
  23. distance from any one point on the Earth to the 0° line of latitude, or the prime (Greenwich) meridian
    longitude
  24. the direction of Earth's rotation
    west to east