A capacitor charging circuit consists of a battery, an uncharged 20 μF capacitor, and a 6.0 kΩ resistor. At t = 0 s the switch is closed; 0.15 s later, the current is 0.46 mA . Part A What is the battery's emf?

Answers

Answer 1

Answer:

Battery voltage will be equal to 9.65 volt

Explanation:

We have given capacitance [tex]C=20\mu F=20\times 10^{-6}F[/tex]

Resistance [tex]R=6kohm=6000ohm[/tex]

Time constant of RC circuit is

[tex]\tau =RC=20\times 10^{-6}\times 6000=0.12sec[/tex]

Time is given t = 0.15 sec

Current i = 0.46 mA

Current in RC circuit is given by

[tex]i=\frac{V}{R}e^{\frac{-t}{\tau }}[/tex]

[tex]0.00046=\frac{V}{6000}e^{\frac{-0.15}{0.12 }}[/tex]

[tex]0.00046=\frac{V}{6000}\times 0.286[/tex]

V = 9.65 volt

So battery emf will be equal to 9.65 volt

Answer 2
Final answer:

To find the emf, use Ohm's Law and the charging formula for a capacitor. With the current, resistance, and capacitor values, calculate the voltage across the resistor. Then, use that to solve for emf with the formula V = emf(1 - e^-t/RC).

Explanation:

To determine the electromotive force (emf) of the battery, we can use the relationship between current, resistance, and emf in the circuit containing a resistor and a capacitor. The relevant formula derived from the natural charging process of a capacitor through a resistor is:

V = emf(1 - e-t/RC) (charging)

Since the question provides the current (I) 0.15 seconds after the circuit is closed, we know that:

I = V/R, where V is the voltage across the resistor at time t, R is the resistance, and I is the current.

Let's solve for emf using the given information:

Identify the given values: R = 6.0 kΩ and C = 20 μF.Adjust units for computations: R = 6000 Ω and C = 20 x 10-6 F.Calculate the voltage (V) across the resistor using Ohm's law: V = I * R = 0.46 mA * 6000 Ω.Convert the current to amperes: I = 0.46 x 10-3 A.Substitute V and I into the equation to find emf: 0.46 x 10-3 A * 6000 Ω = emf(1 - e-0.15/RC).Calculate RC: RC = R * C = 6000 Ω * 20 x 10-6 F = 0.12 s.Substitute RC into the exponent: emf = V/(1 - e-0.15/0.12).After calculations, the emf can be found to be approximately the voltage drop across the resistor divided by the remaining fraction given by the exponential term. This result is the battery's emf.

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Related Questions

A capacitor consists of a set of two parallel plates of area A separated by a distance d . This capacitor is connected to a battery that maintains a constant potential difference V across the plates. If the separation between the plates is doubled, the electrical energy stored in the capacitor will be

Answers

Answer:

if we double the distance the energy stored will be doubled also

Explanation:

The energy stored in a capacitor is given as

Energy stored =1/2(cv²)

Or

= 1/2(Qv)

Where c = capacitance

Q= charge

But the electric field is expressed as

E= v/d

where v= voltage

d= distance

v=Ed

Substituting into any equation above say

Energy stored =1/2(Qv)

Substituting v=Ev

Energy stored =1/2(QEd)

From the equation above it shows that if we double the distance The energy stored will be doubled also

This problem has been solved! See the answer A proton with a speed of 3.5x10^6 m/s is shot into a region between two plates that are separated by distance of 0.23 m. A magnetic field exists between the plates, and it is perpendicular to the velocity of the proton. What must be the magnitude of the magnetic field so the proton just misses colliding with the opposite plate?

Answers

Answer:

The magnitude of the magnetic field 'B' is 0.16 Tesla.

Explanation:

The magnitude of the magnetic field 'B' can be determined by;

             B = [tex]\frac{mV}{qR}[/tex]

where: m is the mass of proton, V is its speed , q is the charge of proton and R is the distance between the plates.

Given that: speed 'V' of the proton = 3.5 × [tex]10^{6} ms^{-2}[/tex], distance 'R' between the plates = 0.23m, the charge 'q' on proton = 1.9 × [tex]10^{-19}[/tex] C and mass of proton = 1.67 × [tex]10^{-27}[/tex]Kg.

Thus,

  B = (1.67 × [tex]10^{-27}[/tex] × 3.5 ×[tex]10^{6}[/tex]) ÷ (1.6 × [tex]10^{-19}[/tex] ×  0.23)

      = [tex]\frac{5.845 * 10^{-21} }{3.68 * 10^{-20} }[/tex]

      = 0.15883

 B = 0.16 Tesla

The magnitude of the magnetic field 'B' is 0.16 Tesla.

To practice Problem-Solving Strategy 27.1: Magnetic Forces. A particle with mass 1.81×10−3 kgkg and a charge of 1.22×10−8 CC has, at a given instant, a velocity v⃗ =(3.00×104m/s)j^v→=(3.00×104m/s)j^. What are the magnitude and direction of the particle’s acceleration produced by a uniform magnetic field B⃗ =(1.63T)i^+(0.980T)j^B→=(1.63T)i^+(0.980T)j^?

Answers

Answer:

The magnitude of the acceleration  is [tex]a = 0.33 m/s^2[/tex]

The direction is [tex]- \r k[/tex] i.e the negative direction of the z-axis

Explanation:

 From  the question we are that

       The mass of the particle [tex]m = 1.8*10^{-3} kg[/tex]

         The charge on the particle is [tex]q = 1.22*10^{-8}C[/tex]

         The velocity is [tex]\= v = (3.0*10^4 m/s ) j[/tex]

        The the magnetic field is  [tex]\= B = (1.63T)\r i + (0.980T) \r j[/tex]

The charge experienced  a force which is mathematically represented as

         

                    [tex]F = q (\= v * \= B)[/tex]

    Substituting value

         [tex]F = 1.22*10^{-8} (( 3*10^4 ) \r j \ \ X \ \ ( 1.63 \r i + 0.980 \r j )T)[/tex]

            [tex]= 1.22 *10^{-8} ((3*10^4 * 1.63)(\r j \ \ X \ \ \r i) + (3*10^4 * 0.980) (\r j \ \ X \ \ \r j))[/tex]

            [tex]= (-5.966*10^4 N) \r k[/tex]

Note :

           [tex]i \ \ X \ \ j = k \\\\j \ \ X \ \ k = i\\\\k \ \ X \ \ i = j\\\\j \ \ X \ \ i = -k \\\\k \ \ X \ \ j = -i\\\\i \ \ X \ \ k = - j\\[/tex]

Now force is also mathematically represented as

        [tex]F = ma[/tex]

Making a the subject

      [tex]a = \frac{F}{m}[/tex]

   Substituting values

     [tex]a =\frac{(-5.966*10^4) \r k}{1.81*10^{-3}}[/tex]

        [tex]= (-0.33m/s^2)\r k[/tex]

        [tex]= 0.33m/s^2 * (- \r k)[/tex]

Two strain gauges are mounted so that they sense axial strain on a steel member in uniaxial tension. The 120 Ω gauges form two legs of a Wheatstone bridge, and are mounted on opposite arms (e.g., arms 1 and 4). The gauge factor for each of the strain gauges is 2 and Em for this steel is 29 × 106 psi. For a bridge excitation voltage of 4 V and a bridge output voltage of 120 μV under load (i.e., Ei = 4 V and 0 E =120 μV ):

Answers

Answer:

a. The maximum strain is 60 * 10^-6

b. Resistance change = 0.014395 ohms

Explanation:

The complete question is as follows;

Two strain gauges are mounted so that they sense axial strain on a steel member in uniaxial tension. The 120 V gauges form two legs of a Wheatstone bridge, and are mounted on opposite arms (e.g., arms 1 and 4). The gauge factor for each of the strain gauges is 2 and E m for this steel is 29 × 106 psi. For a bridge excitation voltage of 4 V and a bridge output voltage of 120 μV under load (i.e., Ei = 4 V and 0  E =120 μV ):

(a) Estimate the maximum strain.

(b) What is the resistance change experienced by each gauge?

solution;

Please check attachment for complete solution and step by step explanation

A Van de Graaff generator is one of the original particle accelerators and can be used to accelerate charged particles like protons or electrons. You may have seen it used to make human hair stand on end or produce large sparks. One application of the Van de Graaff generator is to create x-rays by bombarding a hard metal target with the beam. Consider a beam of protons at 2.00 keV and a current of 5.05 mA produced by the generator. (a) What is the speed of the protons (in m/s)? b) How many protons are produced each second?

Answers

Answer:

v = 1.95*10^5 m/s

3.13 x 10^16 proton

Explanation:

Identify the unknown:  

The speed of the protons  

List the Knowns:  

Energy of protons KE = 2 keV = 2*10^3 eV

Current produced by the generator: I= 5.05 mA = 5 x 10^-3 A  

1 eV = 1.6 x 10-19 Joule

Mass of proton: m = 1.67 x 10^-27 kg

Charge of proton: q_p = 1.6 x 10^-19 C  

Set Up the Problem:

Kinetic energy is given by:

KE= 1/2mv^2

v = √2KE/m

Solve the Problem:  

v = √2 x 2*10^3 x 1.6 x 10^-19/ 1.67 x 10^-27

v = 1.95*10^5 m/s

b.  Identify the unknown:  

Number of protons produced each second  

Set Up the Problem:  

Current is given by:

I =ΔQ/Δt

So, the total charge in one second:  

ΔQ =I*Δt = 5 x 10^-3 x 1 = 5 x 10^-3 C  

Number of protons in this charge:

n =   ΔQ/q_p

Solve the Problem:  

n =   5 x 10^-3/1.6 x 10^-19  

  =3.13 x 10^16 proton

Wave motion is characterized by two velocities: the velocity with which the wave moves in the medium (e.g., air or a string) and the velocity of the medium (the air or the string itself). Consider a transverse wave traveling in a string. The mathematical form of the wave is y(x,t)=Asin(kx−ωt). a. Find the speed of propagation vp of this wave.b. Find the y velocity vy(x,t) of a point on the string as a function of x and t.

Answers

Answer with Explanation:

We are given that  the mathematical form of wave

[tex]y(x,t)=Asin(kx-\omega t)[/tex]

a.We have to find the speed of propagation of this wave

In given mathematical form

k=Wave number

[tex]\omega[/tex]=Angular frequency

A=Amplitude

We know that

Speed of propagation of the wave=[tex]v_p=\frac{\omega}{k}[/tex]

b.Differentiate w.r.r t

[tex]v_y(x,t)=-A\omega cos(kx-\omega t)[/tex]

The velocity [tex]v_y(x,t)[/tex] of a point on the string as  a function of x and t is given  by

[tex]v_y(x,t)=-A\omega cos(kx-\omega t)[/tex]

(a) The speed of propagation of the wave is [tex]\frac{\omega}{k}[/tex]

(b) (b) The velocity of a point on the string as a function of x and t is [tex]v_y (x, t) = -A\omega cos(kx - \omega t)[/tex]

The given parameters;

[tex]y(x, t) = Asin(kx - \omega t)[/tex]

where;

t is the time of motiony is the displacement k is the wave number ω is the angular frequency A  is the amplitude of the wave

(a) The speed of propagation of the wave is calculated as follows;

[tex]v_p = \frac{\omega }{k}[/tex]

(b) The velocity of a point on the string as a function of x and t is calculated as follows;

[tex]v = \frac{dy}{dt} \\\\v_y (x, t) = -A\omega cos(kx - \omega t)[/tex]

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Consider the following descriptions of the vertical motion of an object subject only to the acceleration due to gravity. Begin with the acceleration equation ​a(t)equals=v primev′​(t)equals=​g, where gequals=minus−9.8 m divided by s squared9.8 m/s2. a. Find the velocity of the object for all relevant times. b. Find the position of the object for all relevant times. c. Find the time when the object reaches its highest point. What is the​ height? d. Find the time when the object strikes the ground. A softball is popped up vertically​ (from the​ ground) with a velocity of 30 m divided by s30 m/s.

Answers

Answer:

a) [tex]v = v_{o} - \left(9.8\,\frac{m}{s^{2}} \right)\cdot t[/tex], b) [tex]s = s_{o} + v_{o}\cdot t - \left(9.8\,\frac{m}{s^{2}} \right)\cdot t^{2}[/tex], c) [tex]t = \frac{v_{o}}{9.8\,\frac{m}{s^{2}} }[/tex], d) [tex]t = \frac{v_{o}}{2\cdot \left(9.8\,\frac{m}{s^{2}}\right)}+\frac{\sqrt{v_{o}^{2}+4\cdot s_{o}\cdot \left(9.8\,\frac{m}{s^{2}} \right)} }{2\cdot \left(9.8\,\frac{m}{s^{2}} \right)}[/tex]

Explanation:

a) The acceleration of the object is:

[tex]a = - 9.8\,\frac{m}{s^{2}}[/tex]

The velocity function is found by integration:

[tex]v = v_{o} - \left(9.8\,\frac{m}{s^{2}} \right)\cdot t[/tex]

b) The position function is found by integrating the velocity function:

[tex]s = s_{o} + v_{o}\cdot t - \left(9.8\,\frac{m}{s^{2}} \right)\cdot t^{2}[/tex]

c) The time when the object reaches its highest point ocurrs when speed is zero:

[tex]0\,m = v_{o} - \left(9.8\,\frac{m}{s^{2}} \right)\cdot t[/tex]

[tex]t = \frac{v_{o}}{9.8\,\frac{m}{s^{2}} }[/tex]

d) The time when the object hits the ground occurs when [tex]s = 0\,m[/tex]. The roots are found by solving the second-order polynomial:

[tex]t = \frac{-v_{o}\pm \sqrt{v_{o}^{2}+4\cdot s_{o}\cdot \left(9.8\,\frac{m}{s^{2}} \right)} }{2\cdot (-9.8\,\frac{m}{s^{2}} )}[/tex]

[tex]t = \frac{v_{o}}{2\cdot \left(9.8\,\frac{m}{s^{2}}\right)} \mp \frac{\sqrt{v_{o}^{2}+4\cdot s_{o}\cdot \left(9.8\,\frac{m}{s^{2}} \right)} }{2\cdot \left(9.8\,\frac{m}{s^{2}} \right)}[/tex]

Since time is a positive variable and [tex]v_{o} < \sqrt{v_{o}^{2}+4\cdot s_{o}\cdot \left(9.8\,\frac{m}{s^{2}} \right)}[/tex], the only possible solution is:

[tex]t = \frac{v_{o}}{2\cdot \left(9.8\,\frac{m}{s^{2}}\right)}+\frac{\sqrt{v_{o}^{2}+4\cdot s_{o}\cdot \left(9.8\,\frac{m}{s^{2}} \right)} }{2\cdot \left(9.8\,\frac{m}{s^{2}} \right)}[/tex]

Final answer:

The physics of vertical motion under gravity deals with velocity, position, and time. Velocity over time can be calculated by integrating the acceleration function, while position over time is calculated by integrating the velocity function. The height and time at the peak of motion, as well as when the object hits the ground, are determined by setting these equations to zero at appropriate points.

Explanation:

Considering the physics of vertical motion under gravity, the concepts of velocity, position, and time are important. The acceleration needs to be considered for handling such scenarios, which in your case, has been described by the equation ​a(t)=v′(t)=g. The value of g=−9.8 m/s², where 'g' represents the acceleration due to gravity.

a. Velocity over time: Using the equation of acceleration a=v′=g, and because g is a constant, the velocity at any point can be determined by integrating the acceleration function. This gives v(t)=gt+c, where the constant c is the initial velocity. For a softball with an initial vertical velocity of 30 m/s, this becomes v(t)=-9.8*t+30.

b. Position over time: The position equation can be found by integrating the velocity function, that is: s(t)=½gt²+vt+s₀. The s₀ term is the initial height, which is 0 because the softball is popped up from the ground. Therefore, s(t)=-4.9*t²+30*t.

c. Time and height at the highest point: The motion reaches its highest point when the velocity is zero. So, set v(t) equal to zero and solve for t. Substituting this time into the position equation gives the maximum height.

d. Time when the softball strikes the ground: The softball will hit the ground when its position is again zero. Set s(t) equal to zero and solve for t to find this time.

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A radio transmitting station operating at a frequency of 115 MHzMHz has two identical antennas that radiate in phase. Antenna BB is 9.05 mm to the right of antenna AA. Consider point PP between the antennas and along the line connecting them, a horizontal distance xx to the right of antenna A For what values of x will constructive interference occur at point P?

Answers

Final answer:

Constructive interference at point P occurs when the path length difference between the two antennas is an integer multiple of the wavelength. The values of x where this occurs can be found using the equation path length difference = n * wavelength. Solving for n, we find that constructive interference occurs at x = 0.00906 m.

Explanation:

In order to have constructive interference at point P, the path length difference between the two antennas must be an integer multiple of the wavelength. Since the antennas are identical and radiating in phase, the path length difference is simply the distance between the two antennas, which is 9.05 mm.

The wavelength can be calculated using the formula: wavelength = speed of light / frequency. For a frequency of 115 MHz, the wavelength is approximately 2.6 m.

To find the values of x where constructive interference occurs, we can set up an equation: path length difference = n * wavelength, where n is an integer. So, 9.05 mm = n * 2.6 m.

Solving for n, we get:

n = (9.05 mm) / (2.6 m) = 0.00348

Therefore, constructive interference will occur at point P when x = n * wavelength. Substituting n = 0.00348 and wavelength = 2.6 m, we get:

x = (0.00348)(2.6 m) = 0.00906 m

(6 points) A cylinder has a radius of 12 mm and a length of 2.5 m. It is made of steel with a thermal conductivity of LaTeX: 53.4 \frac{\mathrm{W}}{\mathrm{m K}}53.4 W m K. One end of the cylinder is held at a temperature of LaTeX: 361^{\circ}\text{C}361 ∘ C, the other at LaTeX: 105^{\circ}\text{C}105 ∘ C. In steady state how much power will flow through the cylinder in the form of heat?

Answers

Answer:

2.46 W

Explanation:

Thermal conductivity k = 53.4 W/m-K

Radius r = 12 mm = 12x10^-3 m

Lenght = 2.5 m

T1 = 361 °C

T2 = 105 ∘C

Area A = ¶r^2 = 3.142 x (12x10^-3)^2

= 0.00045 m^2

Power P = -AkdT/dx

Where dT = 361 - 105 = 256

dx = lenght of heat travel = 2.5 m

P = -0.00045 X 53.4 X (256/2.5)

= -0.024 X 102.4 = -2.46 W

The negative sign indicates that heat is lost from the metal.

What pushes against gravity in: a main sequence star, a white dwarf, a neutron star, and a black hole? electron degeneracy, neutron degeneracy, nothing, and heat pressure nothing in all cases. Gravity always wins. nothing, heat pressure, electron degeneracy, and neutron degeneracy heat pressure, neutron degeneracy, electron degeneracy, and nothing heat pressure, electron degeneracy, neutron degeneracy, and nothing

Answers

Final answer:

A main sequence star relies on heat pressure to counteract gravity, a white dwarf uses electron degeneracy pressure, a neutron star uses neutron degeneracy pressure, and in a black hole, gravity ultimately triumphs.

Explanation:

In a main sequence star, it is the heat pressure, due to nuclear fusion, which pushes against gravity and maintains the star's stability. A white dwarf is stabilized against gravity by what is known as electron degeneracy pressure, a quantum mechanical effect that arises because no two electrons can be in the same place doing the same thing at the same time (the Pauli exclusion principle).

The neutron star is supported against gravity by neutron degeneracy pressure, the same quantum effect but explained by neutrons instead of electrons. However, if the mass of a star's core is high enough (more than about three times that of the Sun), no known force can stop it from collapsing into a black hole; gravity ultimately overcomes all other forces.

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You are working in a laser laboratory. Your current project involves suspending spherical glass beads in the Earth's gravitational field using a vertically directed laser beam. Today's experiment involves a black bead of radius r and density rho. Assuming that the radius of the laser beam is the same as that of the bead and that the beam is centered on the bead, determine the minimum laser power required to suspend this bead in equilibrium. (Use any variable or symbol stated above along with the following as necessary: g and c.)

Answers

Final answer:

The minimum laser power required to suspend the bead in equilibrium is (3c/8πr³ρg).

Explanation:

In order to suspend the bead in equilibrium, the radiation pressure from the laser beam must be equal to the gravitational force on the bead.

The radiation pressure is given by P = 2I/c, where P is the pressure, I is the laser intensity, and c is the speed of light. The gravitational force is given by F = (4/3)πr³ρg, where F is the force, r is the radius of the bead, ρ is the density, and g is the acceleration due to gravity.

Equating the radiation pressure and gravitational force, we have 2I/c = (4/3)πr³ρg. Rearranging this equation, we get I = (3c/8πr³ρg).

Therefore, the minimum laser power required to suspend the bead in equilibrium is (3c/8πr³ρg).

A bat can detect small objects such as an insect whose size is approximately equal to the wavelength of the sound the bat makes. What is the smallest insect a bat can detect? Assume that bats emit a chirp at a frequency of 47.6 kHz, and that the speed of sound in air is 413 m/s. Answer in units of mm.

Answers

Given that,

Frequency emitted by the bat, f = 47.6 kHz

The speed off sound in air, v = 413 m/s

We need to find the wavelength detected by the bat. The speed of a wave is given by formula as follows :

[tex]v=f\lambda\\\\\lambda=\dfrac{v}{f}\\\\\lambda=\dfrac{413}{47.6\times 10^3}\\\\\lambda=0.00867\ m[/tex]

or

[tex]\lambda=8.67\ mm[/tex]

So, the bat can detect small objects such as an insect whose size is approximately equal to the wavelength of the sound the bat makes i.e. 8.67 mm.

Enter the measured values of the angles of incidence and refraction below. Angle of incidence θi = 76.5 Correct: Your answer is correct. Your value is acceptable.° Angle of refraction θr = 76.5 Incorrect: Your answer is incorrect. Your value is too high.° Calculate the index of refraction using Snell's Law and the measured values of the angles of incidence and refraction. nacrylic = The accepted value of the index of refraction for acrylic is 1.49. What is the percent error between the accepted value and the experimental value of n? Hint Percent error = %

Answers

Answer:

Explanation:

Given that the inputted angle of incidence is accepted

Angle of incidence θi = 76.5°

But angle of refraction is not acceptable

Angle of refraction θr = 76.5°

We are told that the value is too high

Then, θr < 76.5°

We want to calculate index of refraction n?

The acceptable value of refraction index of acrylic is 1.49

So the true value is 1.49

So, let calculate the measure value

Refractive index is given as

n = Sin(i) / Sin(r)

Then,

n = Sin(76.5) / Sin(76.5)

Then, n = 1

Now, percentage error of the refractive index,

Percentage error is

%error= |true value—measure value| / true value × 100

The true value is 1.49

The measure value is 1

Then,

%error = ( |1.49—1| / 1.49 ) × 100

% error = ( 0.49 / 1.49 ) × 100

%error = 0.3289 × 100

%error = 32.89%

Answer:

Explanation:

32.89%

A light beam is directed parallel to the axis of a hollow cylindrical tube. When the tube contains only air, the light takes 8.72 ns to travel the length of the tube, but when the tube is filled with a transparent jelly, the light takes 1.82 ns longer to travel its length. What is the refractive index of this jelly?

Answers

Answer:

Explanation:

velocity of light in a medium of refractive index V = V₀ / μ

V₀  is velocity of light in air and μ is refractive index of light.

time to travel in tube with air =  length of tube / velocity of light

8.72 ns = L / V₀  L is length of tube .

time to travel in tube with jelly =  length of tube / velocity of light

8.72+ 1.82  = L / V  L is length of tube .

10.54 ns = L / V

dividing the equations

10.54 / 8.72 = V₀  / V

10.54 / 8.72 =   μ

1.21 =  μ

refractive index of jelly = 1.21 .

A rod of mass M = 3.5 kg and length L can rotate about a hinge at its left end and is initially at rest. A putty ball of mass m = 45 g, moving with speed v = 5.02 m/s, strikes the rod at angle θ = 42° from the normal at a distance D = 2/3 L, where L = 1.2 m, from the point of rotation and sticks to the rod after the collision.

What is the initial angular momentum of the ball, in kilogram meters squared per second, right before the collision relative to the pivot point of the rod?

Answers

Complete Question

The diagram for this question is shown on the first  uploaded image

Answer:

The initial angular momentum is  [tex]L_i= 0.134 Kg .m^2/s[/tex]

Explanation:

From the question we are told that

        The mass of the rod is [tex]M = 3.5 kg[/tex]

         The mass of the ball is [tex]m =45g = \frac{45}{1000} = 0.045kg[/tex]

          The speed is [tex]v = 5.02 m/s[/tex]

          The angle the ball strikes the rod is [tex]\theta = 42^o[/tex]

           The distance from the center of the rod is [tex]D = \frac{2}{3} L[/tex]

          The length L is  [tex]= 1.2m[/tex]

          The initial angular momentum of the ball is mathematically represented as

                  [tex]L_i = m\ v\ D\ cos \theta[/tex]

Substituting the value

                 [tex]L_i = 45*10^{-3} * 5.02 * \frac{2}{3} * 1.2 * cos (42)[/tex]

                      [tex]= 0.134 Kg .m^2/s[/tex]

     

Following are the calculation of the initial angular momentum of the ball:

Given:

[tex]M = 3.5 \ kg \\\\m = 45\ g = 0.045\ kg\\\\ v = 5.02\ \frac{m}{s}\\\\ \theta = 42^{\circ}\\\\D = \frac{2}{3}\ L\\\\ L = 1.2\ m\\\\[/tex]

To find:

Li=?

Solution:

Using formula:

[tex]Li= m v D \cos \theta=mv\times \frac{2L}{3}\cos \theta\\\\[/tex]

      [tex]=0.045 \times 5.02 \times \frac{2 \times 1.2}{3}\cos 42^{\circ}\\\\=0.2259 \times\frac{2 \times 1.2}{3}\cos 42^{\circ}\\\\=0.18072\times \cos 42^{\circ}\\\\=0.13430113286\\\\=13.43 \times 10^{-2} \ \frac{kg\ m^2}{s}\\\\[/tex]

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A current of 6 A runs through a coffee machine connected to a 120 V circuit. What is the resistance of the coffee machine?

Answers

Answer:

20 ohm

Explanation:

V = I x R

R = V/ I

= 120/6

R = 20 ohm

Considering the Ohm's law, the resistance of the coffee machine is 20 Ω.

Definition of current

The current (I) is a measure of the speed at which the charge passes a given reference point in a specified direction. Its unit of measure is amps (A).

Definition of voltage

The driving force (electrical pressure) behind the flow of a current is known as voltage and is measured in volts (V). That is, voltage is a measure of the work required to move a charge from one point to another.

Definition of resistance

Resistance (R) is the difficulty that a circuit opposes to the flow of a current and it is measured in ohms (Ω).

Ohm's law

Ohm's law establishes the relationship between current, voltage, and resistance in an electrical circuit.

This law establishes that the intensity of the current that passes through a circuit is directly proportional to the voltage of the same and inversely proportional to the resistance that it presents:

I= V÷R

Where:

I is the current measured in amps (A).V the voltage measured in volts (V).R the resistance that is measured in ohms (Ω).

Resistance of the coffee machine

In this case, you know that:

The voltage is 120 V.The current through the coffee machine is 6 A.

Replacing in the Ohm's Law:

6 A= 120 V÷R

Solving:

6 A× R= 120 V

R= 120 V÷6 A

R= 20 Ω

Finally, the resistance of the coffee machine is 20 Ω.

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Below is a schematic of a vapor power plant in which water steadily circulates through the four components. The water flows through the boiler and condenser at constant pressure and through the turbine and pump adiabatically. Kinetic and potential energy effects can be ignored. Process data follow: Process 4-1: constant pressure at 8 MPa from saturated liquid to saturated vapor Process 2-3: constant pressure at 8 kPa from x2

Answers

Complete Question:

the first attached file shows the schematic

Answer:

a. irreversible cycle

b. 0.182

c. 0.2646

Explanation:

From the saturated vapour pressure table

When the pressure is 1 MPa

Temperature, T₄₁ = 179.9 °C = 452.9 °k

When Pressure is 20 kPa

Temperature, T₃₂ = 60.06 °C = 333.06 °K

attached images 2, 3, 4 and 5 shows a comprehensive solution to the questions

Final answer:

A vapor power plant uses water as the working substance, which goes through a cycle of becoming vaporized and condensed in order to drive a turbine. The schematic provided includes four components: the boiler, condenser, turbine, and pump. Two specific processes mentioned include 4-1 and 2-3, both of which occur at constant pressures.

Explanation:

A vapor power plant operates by using water as the working substance, which goes through a cycle of becoming vaporized, driving a turbine, and then condensing back into a liquid state. In this specific schematic, the water flows through four components: the boiler, condenser, turbine, and pump. The process data provided includes two specific processes: 4-1 which occurs at a constant pressure of 8 MPa, and 2-3 which also occurs at a constant pressure of 8 kPa.

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Suppose that you are visiting Champaign, IL and on July 10 you wake up early and note the rising azimuth of the Sun. How would the direction of the rising Sun change if you measured

Answers

Answer:

It would raise further south

Explanation:

To those of us who live on earth, the most important astronomical object by far is the sun. It provides light and warmth. Its motions through our sky cause day and night, the passage of the seasons, and earth's varied climates.

On any given day, the sun moves through our sky in the same way as a star. It rises somewhere along the eastern horizon and sets somewhere in the west. If you live at a mid-northern latitude (most of North America, Europe, Asia, and northern Africa), you always see the noon sun somewhere in the southern sky.

The sun's path through the rest of the sky is similarly farther north in June and farther south in December. In summary:

In late March and late September (at the "equinoxes"), the sun's path follows the celestial equator. It then rises directly east and sets directly west. The exact dates of the equinoxes vary from year to year but are always near March 20 and September 22.

After the March equinox, the sun's path gradually drifts northward. By the June solstice (usually June 21), the sun rises considerably north of due east and sets considerably north of due west. For mid-northern observers, the noon sun is still toward the south, but much higher in the sky than at the equinoxes.

After the June solstice, the sun's path gradually drifts southward. By the September equinox, its path is again along the celestial equator. The southward drift then continues until the December solstice (usually December 21), when the sun rises considerably south of due east and sets considerably south of due west.

Answer:

It would rise further south

Explanation:

How do you think air resistance affects measured values of g? If you used a ping pong ball, for example, how would this affect the fall-time? Would you expect the ping pong ball and the steel ball to land at the same time if they were both dropped from a height of ϭ.ϱm? What would happen if you dropped both balls from a height of ϮϬm?

Answers

Answer:

A) Air resistance acts in a direction opposite the the fall of an object reducing it by doing work against the weight of the object due to gravity.

B) using a ping pong ball, the time of fall will be greatly reduced since it has little weight (its mass x acceleration due to gravity) against the air resistance. The net downward force of the weight and the air resistance will be small.

C) No, I wouldn't expect them to fall at the same time. The steel ball will have more weight compared to the ping pong ball and hence it will have a larger net force downwards.

D) If they are both released from a 6 m height, the steel ball will fall to the ground first since it has a larger net force downwards.

Your starship, the Aimless Wanderer, lands on the mysterious planet Mongo. As chief scientist-engineer, you make the following measurements: A 2.50 kg stone thrown upward from the ground at 13.0 m/s returns to the ground in 4.50 s; the circumference of Mongo at the equator is 2.00×10^5km; and there is no appreciable atmosphere on Mongo. The starship commander, Captain Confusion, asks for the following information:

a. What is the mass of Mongo?
b. If the Aimless Wanderer goes into a circular orbit 30,000 km above the surface of Mongo, how many hours will it take the ship to complete one orbit?

Answers

Given Information:  

Initial speed = v₁ = 13 m/s

time = t = 4.50 sec

Circumference of Mongo = C = 2.0×10⁵ km = 2.0×10⁸ m

Altitude = h = 30,000 km = 3×10⁷ m

Required Information:  

a) mass of Mongo = M = ?

b) time in hours = t = ?

Answer:  

a) mass of Mongo = M =  8.778×10²⁵ kg

b) time in hours = t = 11.08 h

Explanation:  

We know from the equations of kinematics,

v₂ = v₁t - ½gt²

0 = 13*4.50 - ½g(4.50)²

58.5 = 10.125g

g = 58.5/10.125

g = 5.78 m/s²

Newton's law of gravitation is given by

M = gC²/4π²G

Where C is the circumference of the planet Mongo, G is the gravitational constant, g is the acceleration of planet of Mongo and M is the mass of planet Mongo.

M = 5.78*(2.0×10⁸)²/(4π²*6.672×10⁻¹¹)

M = 8.778×10²⁵ kg

Therefore, the mass of planet Mongo is 8.778×10²⁵ kg

b) From the Kepler's third law,

T = 2π*(R + h)^3/2/(G*M)^1/2

Where R = C/2π

T = 2π*(C/2π + h)^3/2/(G*M)^1/2

T = 2π*((2.0×10⁸/2π) + 3×10⁷)^3/2/(6.672×10⁻¹¹*8.778×10²⁵)^1/2

T = 39917.5 sec

Convert to hours

T = 39917.5/60*60

T = 11.08 hours

Therefore, it will take 11.08 hours for the ship to complete one orbit.

Final answer:

To determine the mass of Mongo, we can use the equation of motion for the stone thrown upward and calculate the gravitational acceleration on Mongo. The mass of Mongo can then be found using Newton's law of universal gravitation. To determine the time it takes for the Aimless Wanderer to complete one orbit around Mongo, we can use Kepler's third law of planetary motion.

Explanation:

a. What is the mass of Mongo?

To determine the mass of Mongo, we can use the equation of motion for the stone thrown upward and calculate the gravitational acceleration on Mongo. The equation for the motion of the stone is given by:

h = ut + 0.5gt^2

Where h is the height, u is the initial velocity, g is the acceleration due to gravity, and t is the time. From the given information, we can find that the stone reaches a maximum height and returns to the ground in 4.50 s. Plugging in the values:

0.0 = (13.0 m/s)(4.50 s) + 0.5g(4.50 s)^2

Simplifying, we find:

g = 13.0 m/s / 4.50 s

Then, we can use Newton's law of universal gravitation to find the mass of Mongo:

F = G * (m1 * m2) / r^2

Where F is the gravitational force, G is the gravitational constant, m1 is the mass of the stone, m2 is the mass of Mongo, and r is the radius of Mongo. Since the stone is on the surface of Mongo, the radius is equal to the circumference divided by 2*pi:

r = 2.00×10^5 km / (2 * pi)

Substituting the known values, we can solve for m2:

m2 = (F * r^2) / (G * m1)

Calculating the gravitational force between the stone and Mongo using the known values and substituting them in the formula, the mass of Mongo is determined.

b. If the Aimless Wanderer goes into a circular orbit 30,000 km above the surface of Mongo, how many hours will it take the ship to complete one orbit?

To find the time it takes for the Aimless Wanderer to complete one orbit around Mongo, we need to use Kepler's third law of planetary motion. This law states that the square of the orbital period (T) is proportional to the cube of the orbital radius (r):

T^2 = (4 * pi^2 * r^3) / (G * m)

Where T is the orbital period, r is the orbital radius, G is the gravitational constant, and m is the mass of Mongo. Plugging in the known values, we can solve for T and convert it to hours.

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A charge of +3.0 µC is distributed uniformly along the circumference of a circle with a radius of 20 cm. How much external energy is required to bring a charge of 25µC from infinity to the center of the circle?

Answers

Answer:

3.37x10^6J

Explanation:

The external energy is given as KQ1Q2/r

=(9*10^9)*(3*10^-3)*(25*10^-3)/(0.2)

=3.375 *10^6 J

Final answer:

The external energy required can be calculated using the electric potential energy formula. The external energy required to bring the charge of 25µC from infinity to the center of the circle is 337.5 joules.

Explanation:

The external energy required to bring a charge of 25µC from infinity to the center of the circle can be calculated using the electric potential energy formula, which is given by:

U = k * (q1 * q2) / r

Where U is the electric potential energy, k is the electrostatic constant, q1 and q2 are the charges, and r is the distance between the charges.

In this case, the charge at the center of the circle is 25µC, and the charge distributed uniformly along the circumference is 3.0µC. The radius of the circle is given as 20 cm. Plugging these values into the formula, we have:

U = (9 * 10^9 Nm^2/C^2) * (25 * 10^-6 C) * (3 * 10^-6 C) / (0.20 m) = 337.5 J

Therefore, the external energy required to bring the charge of 25µC from infinity to the center of the circle is 337.5 joules.

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There are two categories of ultraviolet light. Ultraviolet A ( UVA ) has a wavelength ranging from 320 nm to 400 nm . It is not so harmful to the skin and is necessary for the production of vitamin D. UVB, with a wavelength between 280 nm and 320 nm , is much more dangerous, because it causes skin cancer.

Find the frequency ranges of UVA.
Enter your answers separated with commas.

Answers

Answer:

[tex]7.5x10^{14}Hz[/tex], [tex]9.37x10^{14}Hz[/tex].

Explanation:

The ultraviolet light belongs to the electromagnetic spectrum.

The electromagnetic spectrum is the distribution of radiation due to the different frequencies at which it radiates and its different intensities. That radiation is formed by electromagnetic waves, which are transverse waves formed by an electric field and a magnetic field perpendicular to it.

Any radiation from the electromagnetic spectrum has a speed of [tex]3x10^{8}m/s[/tex] in vacuum.

Therefore, in order to know the frequency the following equation can be used:

[tex]c = \nu \cdot \lambda[/tex]  (1)

[tex]\nu = \frac{c}{\lambda}[/tex]  (2)

Where [tex]\nu[/tex] is frequency, c is the speed of light and [tex]\lambda[/tex] is the wavelength.

Notice that it is necessary to express the wavelength in units of meters before it can be used in equation 2.  

[tex]\lambda = 320nm . \frac{1m}{1x10^{9}nm}[/tex] ⇒ [tex]3.2x10^{-7}m[/tex]

[tex]\nu = \frac{3x10^{8}m/s}{3.2x10^{-7}m}[/tex]    

[tex]\nu = 9.37x10^{14}s^{-1}[/tex]    

But [tex]1Hz = s^{-1}[/tex]

[tex]\nu = 9.37x10^{14}Hz[/tex]    

[tex]\lambda = 400nm . \frac{1m}{1x10^{9}nm}[/tex] ⇒ [tex]4x10^{-7}m[/tex]

[tex]\nu = \frac{3x10^{8}m/s}{4x10^{-7}m}[/tex]    

[tex]\nu = 7.5x10^{14}Hz[/tex]    

Hence, the frequency range of UVA is [tex]7.5x10^{14}Hz[/tex]  to [tex]9.37x10^{14}Hz[/tex].

Suppose that the mirror described in Part A is initially at rest a distance R away from the sun. What is the critical value of area density for the mirror at which the radiation pressure exactly cancels out the gravitational attraction from the sun?

Answers

The critical area density for a mirror in space where radiation pressure cancels out gravitational attraction can be computed using the principles of radiation pressure and gravitational force. By equating the momentum transfer from reflected sunlight to the gravitational pull of the Sun, one can find the area density at which these forces balance.

The question posed is about finding the critical area density for a mirror located in space at a distance R from the Sun, where the radiation pressure from sunlight would balance the gravitational attraction exerted by the Sun. The solution to this problem involves using the principle of momentum transfer from sunlight and equating it to the gravitational force to derive the density at which the forces are balanced.

The radiation pressure P exerted by sunlight can be calculated using the formula P = 2I/c, where I is the intensity of sunlight and c is the speed of light. Given that sunlight above Earth's atmosphere has an intensity of 1.30 kW/m², the radiation pressure P would be twice this value divided by the speed of light, due to the reflection phenomenon (momentum is doubled as the direction is reversed).

On the other hand, the gravitational force acting on an object is given by the formula F = GMm/R², where G is the gravitational constant, M is the mass of the Sun, m is the mass of the object (or spacecraft with the mirror), and R is the distance from the Sun. The mass m can be represented in terms of the area density ρA, where ρ is the area density and A is the area of the mirror.

Setting the radiation pressure equal to the gravitational force and solving for ρ will yield the critical value of area density at which the two forces cancel out.

The critical value of area density for the mirror at which the radiation pressure exactly cancels out the gravitational attraction from the sun is:

[tex]\[ \sigma = \frac{P_{sun}}{4\pi G M_{sun} R^2 c} \][/tex]

To find the critical value of area density (σ) for the mirror at which the radiation pressure exactly cancels out the gravitational attraction from the sun, we need to set the radiation pressure equal to the gravitational force per unit area.

Let's denote the radiation pressure as [tex]\( P_{rad} \)[/tex] and the gravitational force per unit area as [tex]\( P_{grav} \)[/tex]

The radiation pressure [tex]\( P_{rad} \)[/tex] can be calculated using the formula:

[tex]\[ P_{rad} = \frac{I}{c} \][/tex]

where [tex]\( I \)[/tex] is the intensity of the sunlight at the mirror's position and [tex]\( c \)[/tex] is the speed of light.

The intensity [tex]\( I \)[/tex] at a distance [tex]\( R \)[/tex] from the sun can be found using the inverse square law:

[tex]\[ I = \frac{P_{sun}}{4\pi R^2} \][/tex]

where [tex]\( P_{sun} \)[/tex] is the total power output of the sun.

The gravitational force per unit area [tex]\( P_{grav} \)[/tex] is given by:

[tex]\[ P_{grav} = \frac{F_{grav}}{A} = \frac{G M_{sun} m_{mirror} / R^2}{A} \][/tex]

where [tex]\( G \)[/tex] is the gravitational constant, [tex]\( M_{sun} \)[/tex] is the mass of the sun, [tex]\( m_{mirror} \)[/tex] is the mass of the mirror, and [tex]\( A \)[/tex] is the area of the mirror.

Since [tex]\( m_{mirror} = \sigma A \), where \( \sigma \)[/tex] is the area density of the mirror, we can write:

[tex]\[ P_{grav} = \frac{G M_{sun} \sigma A / R^2}{A} = \frac{G M_{sun} \sigma}{R^2} \][/tex]

Now, we set [tex]\( P_{rad} = P_{grav} \)[/tex] to find the critical value of [tex]\( \sigma \)[/tex]:

[tex]\[ \frac{I}{c} = \frac{G M_{sun} \sigma}{R^2} \][/tex]

Substituting [tex]\( I \)[/tex] from the intensity equation, we get:

[tex]\[ \frac{P_{sun}}{4\pi R^2 c} = \frac{G M_{sun} \sigma}{R^2} \][/tex]

Solving for [tex]\( \sigma \)[/tex], we find:

[tex]\[ \sigma = \frac{P_{sun}}{4\pi R^2 c} \cdot \frac{1}{G M_{sun}} \][/tex]

[tex]\[ \sigma = \frac{P_{sun}}{4\pi G M_{sun} R^2 c} \][/tex]

Complete question:- Suppose that the mirror described in Part

A quantity of gas with an initial volume of 5 cubic feet and a pressure of 1700 pounds per square foot expands to a volume of 9 cubic feet. Find the work done by the gas for the given volume and pressure. Round your answer to two decimal places. Assume the temperature of the gas in this process remain constant.

Answers

Answer:

Work done by the gas for the given volume and pressure [tex]= 4996.18[/tex] pounds foot

Explanation:

Given

Pressure applied [tex]= 1700[/tex] pounds per square foot

Initial Volume [tex]= 5[/tex] cubic feet

Final Volume [tex]= 9[/tex] cubic feet

As we know pressure is inversely proportional to V

[tex]P = \frac{k}{V}[/tex]

where k is the proportionality constant

V is the volume and

P is the pressure

Work done

[tex]\int\limits^{V_2}_{V_1} {P} \, dV[/tex]

 [tex]\int\limits^{V_2}_{V_1} {\frac{k}{V} } \, dV\\= \int\limits^{V_2}_{V_1} {\frac{1700 * 5}{V} } \, dV\\= 8500* \int\limits^{V_2}_{V_1} {\frac{1}{V} } \, dV[/tex]

Integrating the above equation, we get-

[tex]8500 ln \frac{V_2}{V_1} \\8500 * 2.303 * \frac{9}{5} \\= 4996.18[/tex]

Work done by the gas for the given volume and pressure [tex]= 4996.18[/tex] pounds foot

A beam of light traveling through a liquid (of index of refraction n1 = 1.47) is incident on a surface at an angle of θ1 = 49° with respect to the normal to the surface. It passes into the second medium and refracts at an angle of θ2 = 69.5° with respect to the normal.

Required:
a. Write an expression for the index of refraction of the second material.
b. Numerically, what is this index?
c. Numerically, what is the light's velocity in medium 1, in meters per second?
d. Numerically, what is the light's velocity in medium 2, in meters per second?

Answers

Answer:

a) n2=(n1sin1)(sin2)

b) 1.18

c) 201081632.7m/s

d) 254237288.1m/s

Explanation:

a) We can calculate the index of refraction of the second material by using the Snell's law:

[tex]n_1sin\theta_1=n_2sin\theta_2[/tex]

[tex]n_2=\frac{n_1sin\theta_1}{sin\theta_2}[/tex]

b) By replacing in the equation of a) we obtain:

[tex]n_2=\frac{(1,47)sin49\°}{sin69.5\°}=1.18[/tex]

c) light velocity in the medium is given by:

[tex]v=\frac{c}{n_1}=\frac{3*10^{8}m/s}{1.47}=204081632.7\frac{m}{s}[/tex]

d)

[tex]v=\frac{c}{n_2}=\frac{3*10^{8}m/s}{1.18}=254237288.1\frac{m}{s}[/tex]

hope this helps!!

The index of refraction for the second material can be found using Snell's Law, which is given by:  n₁sin(θ₁) = n₂sin(θ₂). The refractive index of the second material is approximately 1.19, The light's velocity in medium 1 is 2.04 x 10⁸ m/s. The light's velocity in medium 2 is 2.52 x 10⁸ m/s.

Using the provided angles and refractive index, we calculate the index of the second material to be approximately 1.19, with the corresponding light velocities as 2.04 x 10⁸ m/s in medium 1 and 2.52 x 10⁸ m/s in medium 2.

This question involves the concept of light refraction and the application of Snell's Law. Let's go through each part step-by-step.

The index of refraction for the second material can be found using Snell's Law, which is given by:

n₁sin(θ₁) = n₂sin(θ₂)

where:

n₁ = 1.47 (refractive index of the first medium)θ₁ = 49° (angle of incidence)θ₂ = 69.5° (angle of refraction)

Rearranging for n₂ gives:

n₂ = (n₁sin(θ₁))/sin(θ₂)

Using the values:

n₂ = (1.47 * sin(49°)) / sin(69.5°)

Let's calculate it step by step:

sin(49°) ≈ 0.7547sin(69.5°) ≈ 0.9336n₂ ≈ (1.47 * 0.7547) / 0.9336n₂ ≈ 1.1886

So, the refractive index of the second material is approximately 1.19.

The velocity of light in a medium is given by:

v = c/n

where c is the speed of light in vacuum (approximately 3.00 x 10⁸ m/s), and n is the refractive index of the medium. For medium 1:

v₁ = 3.00 x 10⁸ m/s / 1.47v₁ ≈ 2.04 x 10⁸ m/s

Similarly, for medium 2:

v₂ = 3.00 x 10⁸ m/s / 1.19v₂ ≈ 2.52 x 10⁸ m/s

The plates of a parallel-plate capacitor are maintained with a constant voltage by a battery as they are pushed together, without touching. How is the amount of charge on the plates affected during this process? Question 3 options: The amount of charge on the plates becomes zero. The amount of charge remains constant. The amount of charge on the plates increases during this process. The amount of charge on the plates decreases during this process.

Answers

Answer:

The amount of charge on the plates increases during this process

Explanation:

In order to maintain a constant voltage across the plates, pushing the plates closer will increase the charge on the plate

An initially stationary electron is accelerated by a uniform 640 N/C Electric Field. a) Calculate the kinetic energy of the electron after it has traveled 15 cm in a direction parallel to this field. b) Calculate the speed of the electron after it has traveled 15 cm in a direction parallel to this field.

Answers

Answer:

(a) 1.298 * 10^(-4) J

(b) 5.82 * 10^6 m/s

Explanation:

Parameters given:

Electric field, E = 640 N/C

Distance traveled by electron, r = 15 cm = 0.15 m

Mass of electron, m = 9.11 * 10^(-31) kg

Electric charge of electron, q = 1.602 * 10^(-19) C

(a) The kinetic energy of the electron in terms of Electric field is given as:

K = (q² * E² * r²) / 2m

Therefore, Kinetic energy, K, is:

K = [(1.602 * 10^(-19))² * 640² * 0.15²] / [2 * 9.11 * 10^(-31)]

K = {23651.981 * 10^(-38)} / [18.22 * 10^(-31)]

K = 1298.13 * 10^(-7) J = 1.298 * 10^(-4) J

(b) To find the final velocity of the electron, we have to first find the acceleration of the electron. This can be gotten by using the equations of force.

Force is generally given as:

F = ma

Electric force is given as:

F = qE

Therefore, equating both, we have:

ma = qE

a = (qE) / m

a = (1.602 * 10^(-19) * 640) / (9.11 * 10^(-31))

a = 112.54 * 10^(12) m/s² = 1.13 * 10^(14) m/s²

Using one of the equations of motion, we have that:

v² = u² + 2as

Since the electron started from rest, u = 0 m/s

Therefore:

v² = 2 * 1.13 * 10^(14) * 0.15

v² = 3.39 * 10^(13)

v = 5.82 * 10^6 m/s

The velocity of the electron after moving a distance of 15 cm is 5.82 * 10^6 m/s.

(a) The kinetic energy of the electron is 1.53×10⁻¹⁷ J

(b) The final speed of the electron is 5.8×10⁶ m/s

Kinetic energy and final speed:

The electron is under motion due to the electrostatic force F produced by the electric field E = 640 N/C.

The equation of motion of the electron can be written as:

F = qE

ma = qE

where q = 1.6×10⁻¹⁹ C is the charge on the electron

m = 9.1×10⁻³¹ kg is the mass of the electron

and a is the acceleration.

So,

a = qE/m

a =  1.6×10⁻¹⁹×640 /  9.1×10⁻³¹

a = 1.12×10¹⁴ m/s²

The initial speed of the electron is zero, so u = 0

From the third equation of motion:

v² = u² + 2as

where v is the final speed,

and s is the distance traveled  = 15cm = 0.15m

v² = 0 + 2× 1.12×10¹⁴×0.15

v = 5.8×10⁶ m/s

So the Kinetic energy of the electron is:

KE = ¹/₂mv²

KE = 0.5×9.1×10⁻³¹×(5.8×10⁶)²

KE = 1.53×10⁻¹⁷ J

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a correlation coefficient represents what two things

Answers

Answer:

A correlation coefficient represents the following:

1- The direction of the relationship

2- The strength of the relationship

Final answer:

A correlation coefficient represents the relationship between two variables. It quantifies the strength and direction of the relationship.

Explanation:

A correlation coefficient represents the relationship between two variables. It quantifies the strength and direction of the relationship. The correlation coefficient ranges from -1 to 1, where a value close to -1 indicates a strong negative correlation, a value close to 1 indicates a strong positive correlation, and a value close to 0 indicates no or weak correlation.

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Which of the following correctly describes the result of a voltage difference?
A. Charges more randomly
B. Charges not to move
C. Charges flow from low voltage areas to high voltage areas.
D. Charges flow from high voltage areas to low voltage areas.

Answers

Answer:

D from high to low areas

The answer is d charges flow from high voltage areas to low voltage areas

Two very large parallel metal plates, separated by 0.20 m, are connected across a 12-V source of potential. An electron is released from rest at a location 0.10 m from the negative plate. When the electron arrives at a distance 0.050 m from the positive plate, how much kinetic energy (J) has the electron gained

Answers

Answer:

[tex]{\rm K} = 2.4\times 10^{-19}~J[/tex]

Explanation:

The electric field inside a parallel plate capacitor is

[tex]E = \frac{Q}{2\epsilon_0 A}[/tex]

where A is the area of one of the plates, and Q is the charge on the capacitor.

The electric force on the electron is

[tex]F = qE = \frac{qQ}{2\epsilon_0 A}[/tex]

where q is the charge of the electron.

By definition the capacitance of the capacitor is given by

[tex]C = \epsilon_0\frac{A}{d} = \frac{Q}{V}\\\frac{Q}{\epsilon_0 A} = \frac{V}{d} = \frac{12}{0.20} = 60[/tex]

Plugging this identity into the force equation above gives

[tex]F = \frac{qQ}{2\epsilon_0 A} = \frac{q}{2}(\frac{Q}{\epsilon_0 A}) = \frac{q}{2}60 = 30q[/tex]

The work done by this force is equal to change in kinetic energy.

W = Fx = (30q)(0.05) = 1.5q = K

The charge of the electron is [tex]1.6 \times 10^{-19}[/tex]

Therefore, the kinetic energy is [tex]2.4\times 10^{-19}[/tex]

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