An object that falls and accelerates solely as a result of gravity is said to be in
1 answer:
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1. 5.5 m/s
We can solve the problem by applying the law of conservation of momentum. The total momentum before the collision must be equal to the total momentum after the collision, so we have:
where
m1 = 0.4 kg is the mass of the ball
u1 = 18 m/s is the initial velocity of the ball
m2 = 0.2 kg is the mass of the bottle
u2 = 0 is the initial velocity of the bottle (which is initially at rest)
v1 = ? is the final velocity of the ball
v2 = 25 m/s is the final velocity of the bottle
Substituting and re-arranging the equation, we can find the final velocity of the ball:
2. 22.2 m/s
We can solve the problem again by using the law of conservation of momentum; the only difference in this case is that the bullet and the block, after the collision, travel together at the same speed v. So we can write:
where
m1 = 0.04 kg is the mass of the bullet
u1 = 300 m/s is the initial velocity of the bullet
m2 = 0.5 kg is the mass of the block
u2 = 0 is the initial velocity of the block (which is initially at rest)
v = ? is the final velocity of the bullet+block, which stick and travel together
Substituting and re-arranging the equation, we can find the final velocity of bullet+block:
3. 6560 N
The impulse exerted on the ball is equal to its change in momentum:
(1)
The impulse can be rewritten as product between force and time of collision:
while the change in momentum of the ball is equal to the product between its mass and the change in velocity:
So, eq.(1) becomes
where:
F = ? is the unknown force
is the duration of the impact
m = 0.16 kg is the mass of the ball
is the final velocity of the ball
is its initial velocity (we must add a negative sign, since it is in opposite direction to the final velocity)
So, by using the equation, we can find the force:
Answer:
635 years old
Explanation:
The light reaching the earth from the sun will travel at a speed called the speed of light, and this has a universal value of 3 × 10⁸ m/s. Bearing this in mind, let us calculate the age of the light reaching the Earth from the sun:
Distance of star from Earth = 6.1 × 10⁸m
Speed of light = 3 × 10⁸ m/s
We have distance and speed, let us calculate the time of travel of the light from the star to the earth.
Distance = speed × time
6.1 × 10⁸ = 3 × 10⁸ × time
In order to do the division above, we will divide the whole numbers normally, then we will apply the law of indices to the power that says:
Xᵃ ÷ Xᵇ = X⁽ᵃ⁻ᵇ⁾
Next, we are told that there are 3.2 × 10⁷ seconds in a year.
∴ The number of years travelled by the light from the star:
please note that:
2.03 × 10¹⁰ = 20300000000
3.2 × 10⁷ = 32000000
The closest answer in the option is 635 years, and we are short of this by some points due probably to approximations in the calculation.