what is the magnitude and direction of the electric force on an electron ina uniform electric field of strenght 2360n/c that points due east

Answer: The dissipative component of evolution is in a direction of steepest entropy ascent

Explanation:

According to our definition, every non-equilibrium state of a system or local subsystem for which entropy is well defined must be equipped with a metric in state space with respect to which the irreversible component of its time evolution is in the direction of the steepest entropy ascent permissible under the conservation constraints. We derive (nonlinear) expansions of Onsager reciprocity and fluctuation-dissipation relations to the far-non-equilibrium world inside the rate-controlled constrained-equilibrium approximation to demonstrate the force of the fourth law (also known as the quasi-equilibrium approximation).

(i) The power wasted in heating the wire if the current in part (a) flows in the wire is 53.8 MW.

(ii) The power wasted in heating the wire if the current in part (b) flows in the wire is 17,800 MW.

The value of the power wasted in heating the wire is calculated by applying the following formula.

P = I²R

where;

For the first case when the resistance, R = 9 Ω and current, I = I,

The power wasted is calculated as;

P = I² x 9

P = 9I²

For 22 kV, the current, I = (22,000 V) / 9 Ω

I = 2,444.44 A

P = 9 x (2,444.44)²

P = 5.38 x 10⁷ W

P = 53.8 x 10⁶ W

P = 53.8 MW

For the second case when the resistance, R = 9 Ω and current, I = I,

The power wasted is calculated as;

P = I² x 9

P = 9I²

For 400 kV, the current, I = (400,000 V) / 9 Ω

I = 44,444.44 A

P = 9 x (44,444.44)²

P = 1.78 x 10¹⁰ W

P = 17,800 x 10⁶ W

P = 17,800 MW

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Answer:

La galvanoplastia o electrodeposición es una aplicación práctica de la electroquímica. Se trata de una técnica basada en los principios electroquímicos, en donde se aplica una o varias capas de un metal seleccionado sobre un objeto receptor, por lo general, también metálico.

Explanation:

Espero te sirva de algo ;)

The ball should spin with the speed of 28.8 rpm in order to have an angular momentum of 0.22 kgm2/s .

Given,

mass = 6 kg and diameter = 27 cm

radius = 27/2 = 13.5

angular momentum = L = 0.22kgm^2/sec

we know that,

angular momentum is L= I*w,

where,  I  = moment of inertia          and

            w = angular frequency.

The moment of inertia of a spherical shell is 2/3*M*R^2.

Where , R = radius  and  M= mass

therefore, I = (2/3)(6kg)*(0.135^2).

                  = 0.0729 kg.m^2

solve for speed w,

        L = I x w

       0.22 =  0.0729 x w

therefore, speed = 3.014 m/sec.

        3.014 m/s = 3.014 x 60 / 2π

                         = 28.8 rpm

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The net force that acts on the object is 36.5 N.

We have to note that the first thing that we would have to obtain is the acceleration of the object and we can be able to obtain this by the use of the formula;

v ^2 = u^2 + 2as

v = final velocity

u = initial velocity

a = acceleration

s = distance

(0.75)^2 = (0)^2 + 2 * a * 5.5

a = (0.75)^2 / 2 * 5.5

a = 0.5625/11

a = 0.05 m/s^2

The net force is ma

F = 730 kg * 0.05 m/s^2

F = 36.5 N

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As the object is thrown up with the initial velocity of 20.0 m/s, and there is an air resistance force that would cause an acceleration of 3.00 m/s2, the speed of the object as a return to the ground is 10.8 m/s.

The kinematic equations are a set of equations that describe the motion of an object with constant acceleration.

When we have an initial velocity value, it is written as Vo, while for the final velocity, we simply write V or Vt. As an object moves through the air, air resistance slows the object’s speed.

The formula of the kinematic equation used for solving this case is

Vt = V0 + at (the gravity is 10 m/s2)

[tex]Vt = Vo + (-g-a)t\\\0 = 20 + (-10-3)t\\0 = 20-13t\\\13t = 20\\\t = \frac{20}{13}[/tex]

After the time is known, now we can insert the value into the following formula :

[tex]Vt = Vo + (g-a)t\\Vt = 0 + 7.\frac{20}{13} \\Vt = 0 + \frac{140}{13} \\\Vt = 10.8 m/s[/tex]

Thus, the speed of the object returns to the ground after being thrown up with an initial velocity of 20.0 m/s and acceleration of 3.00 m/s2, which is 10.8 m/s.

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The definition of a planet according to the ancient Greeks is an object that orbits the sun.

Massive, circular celestial objects that are neither stars nor their remnants are known as planets. The planetary nebulae hypothesis, that states that an interstellar cloud bursts out of a nebulae to produce a young protostar encircled by a protoplanetary disc, is currently the most promising theory for planet formation. The steady accretion of matter accelerated by gravity, or accretion, is how planets expand within this disc.

Sun's core undergoes nuclear fusion events, transforming it into a nearly perfect ball of hot plasma that is incandescent. The Sun is the most significant source of energy for life on Earth, radiating this energy mostly as light, uv, and infrared rays.

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The distance which a force of 3N will pull a wooden block before transferring 12J of energy is 4m.

This is referred to as an influence that can change the motion of an object and the unit is Newton.

It has a relationship with distance and work which can be seen below:

Work = Force × distance

12J = 3N × d

d = 12/3 = 4m.

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Research demonstrates that group problem-solving produces superior results. If they have a team player behind them, people are more inclined to take calculated risks that result in innovation.

Working as a team promotes the development of the individual, boosts job satisfaction, and lessens stress. Be upbeat and do your best to assist people. Everyone will appreciate your cooperation and willingness to put in a lot of effort, even your boss.

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The evidence that scientists have that Mars used to have a magnetic field is this:

B. The atmosphere of Mars contains evidence of a magnetosphere.

Scientists base whatever conclusions they reach on a subject matter on evidence. To reach their conclusion that mars had a magnetic field that protected it, they used a device known as an orbiter to measure the magnetic strength of mars.

Their discovery showed that the magnetic field on Mars was ten times as strong as the earth's field. This gives evidence of the fact that at a certain time, there was a strong magnetic field on Mars.

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The distance that the support must be from point A . 1.2010 3 N.

At x = 0, where the x axis is parallel to the diving board, we assume the force acting on the left pedestal to be F1. We define the right pedestal's force as F2 and its location as x=d. W is the diver's weight, which is found at x=L. Setting the total of forces (with upward positive) and the sum of torques (around x2) to zero yields the following two equations:

F 1 +F 2 −W=0

F 1 d+W(L−d)=0

(a) The result of the second equation is F 1 = d L d W = (2.5m 3.0m)

(600N) = 800N, which should be rounded to F 1 = 1.210 3 N. Consequently, F 1 = 1.2010 3 N

(b) F 1 is negative, suggesting a downward force.

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It is true that a vector's component can vary depending on the chosen coordinate system, that a vector can be multiplied by a scalar, and that a vector can have a component equal to 0 even if its magnitude is not 0.

The idea that a vector cannot have a different direction in different coordinate systems is untrue. A physical quantity that exists without us is represented by a vector. As a result, the vector itself is independent of the coordinate system we use. However, the vector's coordinates are affected by the coordinate system. Only when two vectors have the same magnitude and direction are they regarded as being equal. The coordinate system has no influence on a vector.

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The magnitude of the net electric field now at a point 15.5 cm due east of the charge is 1721.15 N/C.

The physical field that surrounds electrically charged particles and pulls or attracts all other charged particles in the vicinity is known as an electric field. The physical field for a system of charged particles is another usage of the term.

Conductive materials are affected by electric fields, which change how electric charges are distributed at their surface. As a result, current travels through the body and to the ground. Circulating currents are induced within the human body by low-frequency magnetic fields.

A uniform electric field of 1350 n/c is already given,

[tex]E_1 = 1350[/tex]

Now, for the point charge, By Coulomb's law,

We get,

[tex]E_2=\frac{Kq}{r^{2} }[/tex]

here, [tex]K = 9*10^{9}[/tex]

According to the question,

[tex]q=2.85*10^{-9} C[/tex]

[tex]r = 0.155 m[/tex]

Putting these values in the formula,

We get,

⇒ [tex]E_2=\frac{(9*10^{9})*(2.85*10^{-9} ) }{(0.155)^{2}}[/tex]

⇒ [tex]E_2= 1067.6 N/C[/tex]

Now,

the net electric field,

⇒ [tex]E = \sqrt{(E_1^{2})+(E_2)^{2} }[/tex]

⇒ [tex]E=\sqrt{(1067.6)^{2} +(1350)^{2} }[/tex]

⇒ [tex]E= 1721.15 N/C[/tex]

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1. The deceleration of the aeroplane in the 35s is -1.6m/s²

2. The force acting on the aeroplane is 4.0× 10⁵N

3. The momentum of the aeroplane when its speed is 6.0m/s is 15 ×10⁶kgm/s

The equation of motion are used in solving problems related to motion. The equations of motion are

1. v = u+ at

2 S = ut + 1/2at²

3. v² = u²+2as

where v is the final velocity

u is the initial velocity

S is the distance

t is time

a is the acceleration

The deceleration of the plane after 35s can be calculated as;

v = u+at

v= 6m/s, u= 62m/s , t = 35s

6 = 62+35a

35a = 6-62

35a =- 56

a = - 56/35

a = -1.6m/s²

the negative sign shows that the plane decelerates.

The force acting on the plane is calculated as;

F = ma

F = 2.5×10⁵× 1.6

F = 4× 10⁵N

The momentum of the plane at 6m/s is ;

p = mv

p = 2.5×10⁵ × 6

p = 1.5× 10⁶ kgm/s

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when a planet, in its orbit, is closer to the sun, it moves faster than average.

In general, the closer a planet is to the Sun, the shorter its orbital period (the time it takes to complete one orbit) will be. As a result, the closer a planet is to the Sun, the faster it will be moving in its orbit.

This is due to the fact that the force of gravity from the Sun on the planet is stronger the closer the planet is to the Sun, which causes the planet to move faster in its orbit.

Additionally, planets that are closer to the Sun will also have a higher surface temperature because they receive more sunlight, and they may have a stronger magnetic field due to the stronger solar wind near the Sun.

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Your question seems incomplete, but I assume the full question was:

"when a planet, in its orbit, is closer to the sun, it:

(group of answer choices)

moves slower than average

spins faster on its axis

reflects less sunlight than average

feels less gravitational pull than average

moves faster than average."

The area of each plate must be 2.6 x 10^-9 m^2 in order to achieve an electric field of 2.0 kV/mm between the plates.

Electric field is a physical quantity that is used to describe the force that an electric charge exerts on other charges in its vicinity. It is a vector field, meaning it has both magnitude and direction. Electric fields are created by electric charges, or by time-varying magnetic fields.

The electric field (E) between the plates of a capacitor is equal to the charge (Q) divided by the area (A) of the plates:
E = Q/A
We can rearrange this equation to solve for A:
A = Q/E
Since the charge on the plates is 5.2 microcoulombs (5.2 x 10^-6 C) and the electric field desired is 2.0 kV/mm (2.0 x 10^3 V/mm), we can plug in these values to find A:
A = 5.2 x 10^-6 C/2.0 x 10^3 V/mm = 2.6 x 10^-9 m^2
Therefore, the area of each plate must be 2.6 x 10^-9 m^2 in order to achieve an electric field of 2.0 kV/mm between the plates.

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In order to calculate time, we need to know one more variable, the gravitational acceleration of earth which is 9.8 m/s^2 and the force exerted on the player's legs, which can be calculated by F=ma.

In order to determine how long the player will remain in the air, we would need to know the player's upward acceleration (which can be affected by factors such as the player's mass and the force exerted on the player's legs as they jump) as well as the player's initial upward velocity. Without this information, it is not possible to calculate how long the player will remain in the air.

In physics, an object's vertical motion can be described by the equation:

y = vi*t + (1/2)at^2

where y is the vertical displacement (or height) of the object, vi is the initial upward velocity, t is the time in the air, and a is the upward acceleration.

If we know the initial upward velocity (vi) and the acceleration (a), we can use this equation to solve for the time in the air (t). The acceleration of the object is determined by various factors such as the force applied on the object and the mass of the object.

In this case, we know the initial upward velocity of the basketball player is 3.53 m/s, but we don't have the acceleration value, which means we cannot solve for time. In order to calculate time, we need to know one more variable, the gravitational acceleration of earth which is 9.8 m/s^2 and the force exerted on the player's legs, which can be calculated by F=ma.

Therefore, without additional information, it is not possible to calculate the time the player will remain in the air.

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The electrons transferred during the process of rubbing a balloon on your head are -1.88×10¹¹.

The electrons, which are negatively charged particles, whirl about the nucleus' periphery. Because of how swiftly they rotate, it might be challenging for scientists to keep an eye on them. The tiny atoms in an atom are drawn to the positive ions of the protons; you can fit 2000 of them in a proton.

Charge on the balloon q = 30 nc

Charge on the electron = -1.6 × 10⁻¹⁹ C

The number of electrons is determined by adding the charge of one particle's entire value.

Suppose there are n electrons,

Number of electrons = (30× 10⁻⁹)/-1.6 × 10⁻¹⁹ = -(3× 10⁻⁸)/(1.6 × 10⁻¹⁹) = -1.88×10¹¹  

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The mass of cell wall is m = 6.082 x 10⁻¹⁶ kg = 6.082 x 10⁻¹⁰ mg , assuming the cell to be spherical and the wall to be a very thin spherical shell

Semi-permeable membrane - A membrane through which only smaller molecules like water can pass but not the bigger molecules like solutes is known as semi-permeable membranes (SPM)

--First, we find the the surface area of the cell wall. Since, the cell is spherical in shape. Therefore, surface area of cell wall will be:

                                             A = 4πr²

where,

A = Surface Area = ?

r = Radius of Cell = Diameter/2

                         = 2.2 μm/2

                         = 1.1 μm

                       = 1.1 x 10⁻⁶ m

Therefore,

                           A = 4π(1.1 x 10⁻⁶ m)²

                          A = 15.2 x 10⁻¹² m²

Now, we find the volume of the cell wall. For that purpose, we use formula:

V = Volume of the Cell Wall = ?

t = Thickness of Wall = 40 nm

= 4 x 10⁻⁸ m

Therefore,

                              V = (15.2 x 10⁻¹² m²)(4 x 10⁻⁸ m)

                                   V = 60.82 x 10⁻²⁰ m³

Now, to find mass of cell wall, we use formula:

                                 ρ = m/V

                                       m = ρV

where,

ρ = density of water = 1000 kg/m³

m = Mass of Wall = ?

Therefore,

                        m = (1000 kg/m³)(60.82 x 10⁻²⁰ m³)

                          m = 6.082 x 10⁻¹⁶ kg

                            = 6.082 x 10⁻¹⁰ mg

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The least speed is required to cover the rest of the trip to arrive in time for the interview is [tex]114.05km/hr[/tex]

Distance and displacement are two quantities that seem to mean the same but are distinctly different with different meanings and definitions. Distance is the measure of “how much ground an object has covered during its motion” while displacement refers to the measure of “how far out of place is an object.”

Here distance formula is,

Δ[tex]d=d_{1} +d_{2}[/tex]

Here we need to find the time left and the distance covered:

T[tex]1[/tex] [tex]=\frac{100}{100}=1hr=60 min[/tex]

T[tex]2[/tex] [tex]=\frac{43}{41} =1.04hr=62.92 min[/tex]

Total time was [tex]3.25hr[/tex][tex]=195min[/tex]

So, Time left is: [tex]1.21hr =72.08min[/tex]

Total distance left to cover is:

D[tex]=280-100-43=137[/tex][tex]km[/tex]

Now minimum speed required is:

[tex]s=\frac{distance}{time} =\frac{137}{1.21} =114.05km/hr[/tex]

Therefore, the least speed is required to cover the rest of the trip to arrive in time for the interview is [tex]114.05 km/hr[/tex].

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Complete question: you are to drive to an interview in another town, at a distance of 280km on a expressway. The interview is at 11:15 a.m. you plan to drive at 100km/h, but then construction work forces you to slow to 41.0km/h for 43.0km what would be the least speed needed for the rest of the trip to arrive in time for the interview?

The term "distance" refers to how far you move. The rate is a measurement of your trip speed. Time is measured by how far you travel.

Time must be measured in hours if the rate in the problem is given in miles per hour (mph). To find the number of hours before calculating the problem, divide the time, if it is given in minutes, by sixty.

Algebra word problems frequently take the form of distance word problems. They involve a situation in which you must determine the speed, distance, or duration of one or more objects' travels.

Because one of the most well-known distance problems involves determining the precise moment when two trains traveling in opposite directions cross paths, these are frequently referred to as "train problems."

Therefore, The term "distance" refers to how far you move. The rate is a measurement of your trip speed. Time is measured by how far you travel.

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Two objects attract each other with a gravitational force of magnitude 1.00 × 1 0 − 8 1.00 \times 10 ^ { - 8 } 1.00×10−8 N when separated by 20.0 cm.

What is meant by magnitude?

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Answer:

they have the same atoms

Celestial navigation is the best method of naming or locating stars, if we have to give someone the location of a star.

With the help of "sights" or time angular measurements taken typically between a celestial body (e.g. the Sun, a planet, the moon or a star) and the visible horizon, Celestial navigation locate a star or any celestial body. However it can also take advantage of measurements between celestial bodies without taking the Earth horizon as reference, such as when the Moon is used in the practice, then it is called "lunars" or lunar distance method, which is used for determining precise time when time is unknown.

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The pressure of the fluid inside the heart chamber gets increased when the heart chamber contracts.

A typical heart has 4 chambers, two upper and two lower chambers. The upper two chambers, the right and left, receive incoming blood. The lower two chambers, the more muscular right and left, pump the blood out of the heart. The heart valves, which maintain blood flowing in the right direction, are gates at the chamber openings. We know when a closed chamber which is filled with a fluid is compressed, the fluid inside the chamber tries to come out of the chamber. Which increases the blood pressure in case of a heart chamber.

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The greatest distance away from the initial position that an object can be if it struck by the airplane is 12.5 ft, if the initial speed of the airplane is 10 ft/s.

Initial speed of the paper airplane, u = 10 ft/s

Final speed of the paper airplane, v = 0

deceleration of the airplane, a = -4 ft/s²

By the first equation of motion, v = u -at

Time of flight, t = (v-u)/a

t = (0 - 10)/-4 = 2.5 sec

Maximum distance travelled by the airplane, = S

S = ut + 0.5at²

S = 10 × 2.5 - 0.5 × 4 × 2.5²

S = 12.5 ft

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The velocity of an object experiencing an acceleration of 24m/s while traveling in a circle of radius 6.0m is 12m/s.

The required details for velocity in given paragraph

a = v²/r

Given a = 24m/s²; radius = 6m

24 = v²/6

Cross multiplying will give;

v² = 24×6

v² = 144

v =√144

v = 12m/s

The velocity of the object is 12m/s

How does the acceleration and radius of the circle relate to the object's velocity?

The acceleration of an object traveling in a circle is known as centripetal acceleration and is caused by the force of the object's velocity acting towards the center of the circle. The acceleration is directly proportional to the radius of the circle and the square of the velocity of the object. The equation for centripetal acceleration is a = v^2 / r, where a is the acceleration, v is the velocity, and r is the radius. So the bigger the radius of the circle, the lesser the object's velocity needs to be in order to maintain the same acceleration and vice versa.

The object's velocity and the radius of the circle are inversely proportional to each other.

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