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69. We define the “effective gravity” in his environment as
g
eff
= 220/60 = 3.67 m/s
2
.
Thus, using equations from Chapter 2 (and selecting downwards as the positive
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Unformatted text preview: direction), we find the “falltime” to be 2 2 1 2(2.1 m) 1.1 s. 2 3.67 m/s eff y v t g t t Δ = + ¡ = =...
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This note was uploaded on 05/17/2011 for the course PHY 2049 taught by Professor Any during the Spring '08 term at University of Florida.
 Spring '08
 Any
 Physics, Gravity

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