qu.1.topic=fill in blanks@ qu.1.1.mode=Blanks@ qu.1.1.editing=useHTML@ qu.1.1.name=Coordinate Systems IV@ qu.1.1.question=
Coordinate systems can help us to determine how star trails will appear and which stars we can see from specific <1>. At any one time, every observer on Earth can see <2> of all the stars (weather conditions pending).
Stars can be classified into three sets by an observer. Circumpolar stars are visible <3> . Rise and set stars are those that change with the season and rise and set every <4> . Never rise stars are stars that are always below <5>.
Examples
The sun appears always inside the ecliptic within a band of width of <13> and the moon and planets appear within a band of roughly<14>.
@ qu.1.1.blank.1=latitudes, altitudes, longitudes, celestial poles@ qu.1.1.blank.2=half, most, one-quarter, one-third@ qu.1.1.blank.3=all of the time, half of the time, never, only above the horizon@ qu.1.1.blank.4=night, 28 days, three months, 12 hours@ qu.1.1.blank.5=the horizon plane, 49 degrees N, the ecliptic, the zenith@ qu.1.1.blank.6=North Pole, equator, North Celestial Pole, zenith@ qu.1.1.blank.7=circumpolar, visible, rise and set, never rise@ qu.1.1.blank.8=rise and set, circumpolar, visible, never rise@ qu.1.1.blank.9=vertical, horizontal, short, parallel@ qu.1.1.blank.10= +57 degrees=> +90 degrees, -57 degrees => -90 degrees, +33 degrees => +90 degrees, -57° => +57 degrees@ qu.1.1.blank.11= 88 degrees,-2 degrees, 2 degrees, -48 degrees@ qu.1.1.blank.12= +88 degrees => +90 degrees, -90 degrees=> -88 degrees, -88 degrees => +88 degrees, -90 degrees => +2 degrees@ qu.1.1.blank.13= 47 degrees, 23.5 degrees,60 degrees, 31 degrees@ qu.1.1.blank.14= 60 degrees, 23.5 degrees, 47 degrees, 31 degrees@ qu.1.1.grader.1=menu@ qu.1.1.grader.2=menu@ qu.1.1.grader.3=menu@ qu.1.1.grader.4=menu@ qu.1.1.grader.5=menu@ qu.1.1.grader.6=menu@ qu.1.1.grader.7=menu@ qu.1.1.grader.8=menu@ qu.1.1.grader.9=menu@ qu.1.1.grader.10=menu@ qu.1.1.grader.11=menu@ qu.1.1.grader.12=menu@ qu.1.1.grader.13=menu@ qu.1.1.grader.14=menu@