B. Orbit. The planets orbit the sun, the moon orbits earth, etc.
Answer:
The force exerted by the ocean tide is directed to the right (east).
The force exerted by the wind is directed to the northwest (45° N of W).
We should separate the x- and y- components of the wind force, and evaluate each component separately.

We denote the direction to the right as the positive direction, so the x-component of the wind force is in the negative direction.
The resultant force is as follows:
 + [4242.64](\^{y})\\F_R = -2242.64\^{x} + 4242.64\^{y}](https://tex.z-dn.net/?f=F_R%20%3D%20%5B2000%20-%204242.64%5D%28%5C%5E%7Bx%7D%29%20%2B%20%5B4242.64%5D%28%5C%5E%7By%7D%29%5C%5CF_R%20%3D%20-2242.64%5C%5E%7Bx%7D%20%2B%204242.64%5C%5E%7By%7D)
The resultant acceleration can be found by Newton's Second Law:

The magnitude of the resultant acceleration is

3
Explanation:
it will collide then friction will slow it down
Answer:
Therefore, light travelling at 3.0x10^8 meters per second takes 500 seconds (8 minutes, 20 seconds) to reach the Earth, which is 1.5x10^11 meters away from the sun
Explanation:
Answer:
2 revolutions
Explanation:
Assume that when she runs off the edge of the 8.3m high cliff, her vertical speed is 0. So gravitational acceleration g = 9.8m/s2 is the only thing that makes her fall down. So we can use the following equation of motion to calculate the time it takes for her to fall down:

where s = 8.3 m is the distance that she falls, t is the time it takes to fall, which is what we are looking for


Since she rotates with an average angular speed of 1.6rev/s. The number of revolutions she would make within 1.3s is
