Earth Moon Sun Science Review Worksheet Page 2

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13.   D uring   t he   f all,   w hich   6   b right   c onstellations   a re   v isible   f rom   C hicago?   C an   y ou  
identify   t he   b right   s tars   P olaris,   D eneb,   A ltair   a nd   V ega?   W hich   a re   i ncluded   i n   t he  
summer   t riangle?  
 
14.     C an   y ou   d escribe   t he   i mportance   o f   G alileo’s   t wo   p ublications   l isted   b elow?  
 
a.   T he   S tarry   M essenger  
b.   D ialogue   o n   t he   T wo   G reat   W orld   S ystems  
 
15.   C an   y ou   e xplain   P tolemy’s   g eocentric   m odel   o f   t he   U niverse?  
 
16.   C an   y ou   e xplain   w hy   T ycho   B rahe   i s   s till   k nown   t oday   f or   h is   o bservational   d ata  
and   h is   h iring   o f   J ohannes   K epler?  
 
17.   C an   y ou   i dentify   w hich   o f   t he   f ollowing   d escriptions   g o   w ith   w hich   o f   K epler’s   3  
laws   o f   p lanetary   m otion?  
 
a.   T his   l aw   i s   a bout   t he   s peed   o f   p lanet   t raveling   a round   t he   s un.   A s   a   p lanet  
orbits   t he   s un,   t he   l ine   j oining   t he   S un   a nd   t he   p lanet   s weeps   t hrough   e qual  
areas   i n   e qual   t imes.  
b.   T his   l aw   i s   a bout   t he   l ength   o f   t ime   a   p lanet   t akes   t o   o rbit   t he   S un   ( period  
of   r evolution).   I f   y ou   u se   t he   u nit   A U   ( Astronomical   U nit)   t o   m easure   t he  
average   d istance   o f   t he   p lanet   f rom   t he   s un,   K epler’s   e quation   a ppears   i n   i ts  
simplest   f orm:       P 2   =   R 3         w here   P   =   p eriod   o f   r evolution   a nd   R   =   a verage  
distance   o f   p lanet   f rom   s un   ( semimajor   a xis)  
c.   P lanets   o rbit   t he   S un   i n   e llipses  
 

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