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ladessa [460]
3 years ago
9

A car starts from a stop at a traffic light and accelerates at a rate of 4.0 m/s 2 . Immediately on reaching a speed of 32 m/s,

the driver sees that the next light ahead is red and instantly applies the brakes (reaction time = 0.00 s). The car decelerates at a constant rate and comes safely to a stop at the next light. The whole episode takes 15.0 s. How far does the car travel?
Physics
1 answer:
Elina [12.6K]3 years ago
5 0

Answer:

140.04 m from the stop.

Explanation:

We can divide the motion in two parts:

First, we have an uniformly accelerated motion, using the following formula we calculate the distance traveled in this part:

v_f^2=v_0^2+2ax_1\\x_1=\frac{v_f^2}{2a}\\x_1=\frac{(32\frac{m}{s})^2}{2(4\frac{m}{s^2})}\\x_1=128m

In the second part, the car decelerates, but we don't know the value of this deceleration. We have to calculate the time spend in the first part, in order to know the time spend on second part:

v_f=v_0+at_1\\t_1=\frac{v_f}{a}=\frac{32\frac{m}{s}}{4\frac{m}{s^2}}\\t_1=8s

Recall that total time is 15 s

t=t_1+t_2\\t_2=t-t_1\\t_2=15s-8s=7s

Now, we calculate the deceleration:

a=\frac{-v_0}{t_2}\\a=\frac{-32\frac{m}{s}}{7s}\\a=-4.57\frac{m}{s^2}

Finally, we find the distance traveled in the second part. In this way, we can know how far does the car travel.

x_2=\frac{-v_0^2}{2a}\\x_2=\frac{-(32\frac{m}{s})^2}{2(-4.57\frac{m}{s^2})}\\x_2=112.04m\\x=x_1+x_2\\x=128m+112.04m\\x=140.04m

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g The international space station has an orbital period of 93 minutes at an altitude (above Earth's surface) of 410 km. A geosyn
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Explanation:

Kepler's third law It is an application of Newton's second law where the forces of the gravitational force, obtaining

            T² = (\frac{4\pi }{G M_s} ) r³             (1)

           

in this case the period of the season is

            T₁ = 93 min (60 s / 1 min) = 5580 s

            r₁ = 410 + 6370 = 6780 km

            r₁ = 6.780 10⁶ m

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if we substitute in equation 1

            T² = K r³

            K = T₁²/r₁³

            K = \frac{ 5580^2}{ (6.780 10^6)^2}

            K = 9.99 10⁻¹⁴ s² / m³

we can replace the satellite values

            r³ = T² / K

            r³ = 86400² / 9.99 10⁻¹⁴

            r = ∛(7.4724 10²²)

            r = 4.21 10⁷ m

this distance is from the center of the earth

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