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Lemur [1.5K]
3 years ago
12

An electron remains suspended between the surface of the Earth (assumed neutral) and a fixed positive point charge, at a distanc

e of 8.88 m from the point charge. The acceleration of gravity is 9.8 m/s^2 and the value of Coulomb's constant is 8.98755 x 10^9 Nm^2/C^2. Determine the charge required for this to happen. Mass of electron is 9.10939 x 10^-31 kg.
Physics
1 answer:
DaniilM [7]3 years ago
5 0

To solve this problem we will apply the concept related to the balance of forces. Here the electrostatic force defined by Coulomb's laws must be proportional to the weight of the electron, defined by Newton's second law, so that such balance exists, both can be described as:

F_e = \frac{kq_1q_2}{d^2}

Here,

q_1 = Charge required

q_2 =Charge of electron

d = Distance

k = Coulomb's constant

F_w = mg

Here,

m = mass

g = Gravitational acceleration

In equilibrium the sum  of Force is zero, then,

\sum F = 0

F_e = F_w

\frac{kq_1q_2}{d^2} = mg

\frac{(8.98755*10^9 )(q_1)(1.6*10^{-19})}{8.8^2} = (9.8)(9.10939*10^{-31} )

q_1 = 4.8075*10^{-19}C

Therefore the charge required for this to happen is 4.8075*10^{-19}C

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Answer:

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3 years ago
There are many well-documented cases of people surviving falls from heights greater than 20.0 m. In one such case, a 55.0 kg wom
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1a) -192.7g

1b) 0.0126 s

2) 1309 kg m/s

3) 1.04\cdot 10^5 N

Explanation:

1a)

First of all, we have to find the velocity of the womena just before hitting the ground.

Since the total mechanical energy is conserved during the fall, the initial gravitational potential energy of the woman when she is at the top is entirely converted into kinetic energy.

So we can write:

mgh=\frac{1}{2}mv^2

where

m = 55.0 kg is the mass of the woman

g=9.8 m/s^2 is the acceleration due to gravity

h = 29.0 m is the initial height of the woman

v is her final speed

Solving for v,

v=\sqrt{2gh}=\sqrt{2(9.8)(29.0)}=23.8 m/s

Then, when the woman hits the soil, she is decelerated until a final velocity

v'=0

So we can find the deceleration using the suvat equation:

v'^2-v^2=2as

where

s = 15.0 cm = 0.15 m is the displacement during the deceleration

Solving for a,

a=\frac{v'^2-v^2}{2s}=\frac{0-23.8^2}{2(0.15)}=-1888.3 m/s^2

In terms of g,

a=\frac{-1888.3}{9.8}=-192.7g

1b)

Here we want to find the time it takes for the woman to stop.

Since her motion is a uniformly accelerated motion, we can do it by using the following suvat equation:

v'=v+at

where here we have:

v' = 0 is the final velocity of the woman

v = 23.8 m/s is her initial velocity before the impact

a=-1888.3 m/s^2 is the acceleration of the woman

t is the time of the impact

Solving for t, we find:

t=\frac{v'-v}{a}=\frac{0-23.8}{-1888.3}=0.0126 s

So, the woman took 0.0126 s to stop.

2)

The impulse exerted on an object is equal to the change in momentum experienced by the object.

Therefore, it is given by:

I=\Delta p =m(v'-v)

where

\Delta p is the change in momentum

m is the mass of the object

v is the initial velocity

v' is the final velocity

Here we have:

m = 55.0 kg is the mass of the woman

v = 23.8 m/s is her initial velocity before the impact

v' = 0 is her final velocity

So, the impulse is:

I=(55.0)(0-23.8)=-1309 kg m/s

where the negative sign indicates the direction opposite to the motion; so the magnitude is 1309 kg m/s.

3)

The impulse exerted on an object is related to the force applied on the object by the equation

I=F\Delta t

where

I is the impulse

F is the average force on the object

\Delta t is the time of the collision

Here we have:

I=1309 kg m/s is the magnitude of the impulse

\Delta t = 0.0126 s is the duration of the collision

Solving for F, we find the magnitude of the average force:

F=\frac{I}{\Delta t}=\frac{1309}{0.0126}=1.04\cdot 10^5 N

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The equation provided to us is 6x-2(4x)=12

To solve this, we will multiply 4x with 2 and then subtract the like terms and finally, we evaluate the value of 'x'.

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Answer:

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An orbit can be defined as the curved path through which a astronomical (celestial) object such as planet Earth, in space move around a Moon, Sun, planet or star.

In this scenario, if the scientists want the probe to enter the orbit they should ensure that probe moves in direction X. This ultimately implies that, the probe must move in the same direction as the orbit, in order to enter it.

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