Answer:
Force on each front wheel = 4711 N
Force on each back wheel = 2591 N
Explanation:
Weight of car = 1490 Kg
Distance of COG from front axle= 1.1 m
Distance of COG from back axle = 3.1 - 1.1 = 2 m
Vertical forces are balanced ,
So, R1 + R2 = mg
R1 + R2 = 1490× 9.8
Thus; R1 + R2 = 14602 - - - eq1
Where
R1 is force on front wheel
R2 is force on back wheel
Now, we know that;
Angular momentum about centre of gravity is zero.
Therefore,
R1 × 1.1 = R2 × 2
R1 = (2/1.1)R2
Put this into equation1, to get;
(2/1.1)R2 + R2 = 14602
R2(2.818) = 14602
R2 = 14602/2.818
R2 = 5182 N and R1 = (2/1.1)5182 = 9422 N
Hence, force on each back wheel = R2/2 = 5182/2 = 2591 N
Force on each front wheel = R1/2 = 9422/2 = 4711 N
We can use the following equation to solve this problem:
<h3>Δp=m∣Vi−Vf∣</h3>
(Where p is the momentum change, m is mass, Vi is initial velocity, and
Vf is final velocity)
Substitute the values given to us in the question:
Δp=(0.6)∣(5.7−(−2.7)∣
Δp=4.9 kg.m/s
Final answer: 4.9kg.m/s.
The change in momentum (Δp) is defined as the change in the mass times the velocity of an object. A force is required to change the momentum of an object. This applied force can increase or decrease momentum, or even change the orientation of an object.
Learn more about momentum:
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C.0 because it didn't move<span />
The correct option is D.
According to special relativity, in no frame of reference does light in a vacuum travel at less than the speed of light, the speed of light in a vacuum is the same for any inertial reference frame.This fact remain valid no matter the speed of a light source relative to another observer.
Light is a very complex phenomenon, but in many situations its behavior can be understood with a simple model based on rays and wave fronts. A ray is a thin beam of light that travels in a straight line. A wave front is the line (not necessarily straight) or surface connecting all the light that left a source at the same time. For a source like the Sun, rays radiate out in all directions; the wave fronts are spheres centered on the Sun. If the source is a long way away, the wave fronts can be treated as parallel lines.
Rays and wave fronts can generally be used to represent light when the light is interacting with objects that are much larger than the wavelength of light, which is about 500 nm. In particular, we'll use rays and wave fronts to analyze how light interacts with mirrors and lenses.