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1<br />

8 m ⎛ 365 d ⎞⎛<br />

⎞⎛<br />

2.62: a) ⎟ ⎞<br />

4<br />

24h 3600s<br />

d = ct = ( 3.0 × 10 )(1y)<br />

⎜<br />

⎟<br />

⎜<br />

⎟<br />

⎜<br />

s ⎝ 1y ⎠⎝<br />

1d ⎠⎝<br />

1h ⎠<br />

15<br />

= 9.5×<br />

10 m<br />

8 m −9<br />

b) d = ct = (3.0×<br />

10 )(10 s) = 0.30 m<br />

s<br />

11<br />

d 1.5×<br />

10 m<br />

c) t = =<br />

= 500 s = 8.<br />

33 min<br />

8<br />

c 3.0×<br />

10 m s<br />

8<br />

d 2(3.84×<br />

10 m)<br />

d) t = =<br />

= 2.6 s<br />

c<br />

8<br />

3.0×<br />

10 m s<br />

9<br />

d 3×<br />

10 mi<br />

e) t = =<br />

= 16,100 s = 4.<br />

5 h<br />

c 186,000 mi s<br />

2.63: a) v = 2π<br />

RE t = 464m s<br />

4<br />

b) v = 2π<br />

r t = 2.99×<br />

10 m s ( r is the radius of the earth's orbit)<br />

c) Let c be the speed of light, then in one second light travels a distance c (1.00s).<br />

The<br />

number of times around the earth to which this corresponds is c ( 1.00s) 2 πR = E<br />

7. 48

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