Speed of car A is given as
![v_a = 70 mph](https://tex.z-dn.net/?f=v_a%20%3D%2070%20mph)
now we need to convert it into SI units
1 miles = 1609 m
1 hour = 3600 s
now we have
![v_a = 70 *\frac{1609}{3600} = 31.3 m/s](https://tex.z-dn.net/?f=v_a%20%3D%2070%20%2A%5Cfrac%7B1609%7D%7B3600%7D%20%3D%2031.3%20m%2Fs)
now its distance from Bambi is given as
![d_a = 350 m](https://tex.z-dn.net/?f=d_a%20%3D%20350%20m)
time taken by it to hit the Bambi
![t = \frac{d}{v}](https://tex.z-dn.net/?f=t%20%3D%20%5Cfrac%7Bd%7D%7Bv%7D)
![t = \frac{350}{31.3}](https://tex.z-dn.net/?f=t%20%3D%20%5Cfrac%7B350%7D%7B31.3%7D)
![t = 11.2 s](https://tex.z-dn.net/?f=t%20%3D%2011.2%20s)
Now other car is moving at speed 50 mph
so its speed in SI unit will be
![v_b = 50* \frac{1609}{3600}](https://tex.z-dn.net/?f=v_b%20%3D%2050%2A%20%5Cfrac%7B1609%7D%7B3600%7D)
![v_b = 22.35 m/s](https://tex.z-dn.net/?f=v_b%20%3D%2022.35%20m%2Fs)
now its distance from Bambi is given as
![d_b = 590 feet](https://tex.z-dn.net/?f=d_b%20%3D%20590%20feet)
as we know that 1 feet = 0.3048 m
![d_b = 590*0.3048 = 179.83 m](https://tex.z-dn.net/?f=d_b%20%3D%20590%2A0.3048%20%3D%20179.83%20m)
now the time to hit the other car is
![t_2 = \frac{179.83}{22.35}](https://tex.z-dn.net/?f=t_2%20%3D%20%5Cfrac%7B179.83%7D%7B22.35%7D)
![t_b = 8.05 s](https://tex.z-dn.net/?f=t_b%20%3D%208.05%20s)
So Car B will hit the Bambi first
(D)
Explanation:
The more massive an object is, the greater is the curvature that they produce on the space-time around it.
The centripetal acceleration a is 4.32
10^-4 m/s^2.
<u>Explanation:</u>
The speed is constant and computing the speed from the distance and time for one full lap.
Given, distance = 400 mm = 0.4 m, Time = 100 s.
Computing the v = 0.4 m / 100 s
v = 4
10^-3 m/s.
radius of the circular end r = 37 mm = 0.037 m.
centripetal acceleration a = v^2 / r
= (4
10^-3)^2 / 0.037
a = 4.32
10^-4 m/s^2.