The efficiency of the skier is 86%
(a) The efficiency of the skier can be calculated by finding the ratio of the mechanical energy at the top of the hill to the mechanical energy at the bottom of the hill.
The mechanical energy of an object can be defined as the sum of its kinetic energy and its potential energy.
In this case, the skier starts from rest, so her initial kinetic energy is zero.
Her initial potential energy can be calculated using the formula:
mgh = (75 m)(9.8 m/s²)(63 kg)
= 45,765 J
where
m = the mass of the skier,
g = the acceleration due to gravity,
h = the height of the hill.
Using the principle of conservation of energy, we know that the skier's mechanical energy at the bottom of the hill must be equal to her mechanical energy at the top of the hill, so her final kinetic energy is given by:
K = (1/2)mv²
= (1/2)(63 kg)(25 m/s)²
= 39,375 J
Her final potential energy is zero, since she is at ground level, so her mechanical energy at the bottom of the hill is equal to her final kinetic energy:
K = 39,375 J
Therefore, the efficiency of the skier is given by the ratio of her mechanical energy at the bottom of the hill to her mechanical energy at the top of the hill:
Efficiency = K/mgh
= 39,375 J/45,765 J
= 0.86 or 86%
(b) Here's an energy flow diagram ,
[Skier at Rest] ------(1)------> [Gravitational Potential Energy]
|
|
|
|
V
[Gravitational Potential Energy] ----(2)-----> [Kinetic Energy]
|
|
|
|
V
[Kinetic Energy] --------(3)-------> [Air Resistance/ Frictional Heat]
Skier at Rest: At the top of the hill, the skier starts with no kinetic energy but possesses gravitational potential energy due to being at an elevated position.Gravitational Potential Energy: As the skier descends the hill, the gravitational potential energy decreases. This energy is converted into kinetic energy, increasing the skier's speed.Kinetic Energy: As the skier reaches the bottom of the hill, the gravitational potential energy is fully converted into kinetic energy. The skier's speed is at its maximum, indicated by a value of 25 m/s.Air Resistance/Frictional Heat: As the skier moves through the air and encounters friction with the snow, some of the kinetic energy is converted into heat due to air resistance and frictional forces. This energy is dissipated into the surroundings.Learn more about the efficiency:
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A series RLC circuit has components with the following values: L = 16.0 mH, C = 86.0 nF, R = 10.02, and AV = 100 V, with Av = AV max sin wt. max (a) Find the resonant frequency of the circuit. kHz
The resonant frequency of the circuit is approximately 135.8 kHz.
To find the resonant frequency of the series RLC circuit, we can use the formula:
f_res = 1 / (2π√(LC))
L = 16.0 mH = 16.0 x [tex]10^(-3)[/tex] H
C = 86.0 nF = 86.0 x [tex]10^(-9)[/tex]F
Plugging in the values:
f_res = 1 / (2π√(16.0 x[tex]10^(-3[/tex]) * 86.0 x [tex]10^(-9)))[/tex]
f_res = 1 / (2π√(1.376 x [tex]10^(-6)))[/tex] ≈ 1 / (2π x 0.001173) ≈ 1 / (0.007356) ≈ 135.8 kHz
The resonant frequency of a circuit refers to the frequency at which the impedance of the circuit is purely resistive, resulting in maximum current flow or minimum impedance.
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The electric field 1.8 cm from a small object points away from the object with a strength of 2.5x105 N/C. Part A What is the object's charge? Express your answer with the appropriat
The object's charge is -4.5x10^-5 C.
we can use the formula for electric field strength (E) due to a point charge:
E = k * (|Q| / r^2)
Where:
E = Electric field strength
k = Coulomb's constant (8.99x10^9 N m^2/C^2)
|Q| = Absolute value of the charge on the object
r = Distance from the object
Rearranging the formula, we can solve for |Q|:
|Q| = E * (r^2 / k)
Plugging in the given values:
E = 2.5x10^5 N/C
r = 1.8 cm = 0.018 m
k = 8.99x10^9 N m^2/C^2
|Q| = (2.5x10^5 N/C) * (0.018 m)^2 / (8.99x10^9 N m^2/C^2)
= 4.5x10^-5 C
Since the electric field points away from the object, the charge must be negative, so the object's charge is approximately -4.5x10^-5 C.
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When an object with an electric charge of 0.610mC is 37.0 m from an object with an electric charge of −0.460mC, the force between them has a strength of 1.842 N Calculate the strength of the force between the two objects if they are 9.25 m apart. Round your answer to 3 significant digits.
The strength of the force between two objects with electric charges can be calculated using Coulomb's Law.
Given an electric charge of 0.610 mC and −0.460 mC, with a force of 1.842 N at a distance of 37.0 m, we can calculate the strength of the force when they are 9.25 m apart.
Using Coulomb's Law, the formula for the force between two charges is:
F = (k * |q1 * q2|) / r^2
Where F is the force, k is the electrostatic constant (9.0 x 10^9 Nm²/C²), q1 and q2 are the charges, and r is the distance between them.
To find the strength of the force at a distance of 9.25 m, we can rearrange the formula as follows:
F = (k * |q1 * q2|) / (r^2)
F = (9.0 x 10^9 Nm²/C² * |0.610 mC * -0.460 mC|) / (9.25 m)^2
Calculating the above expression will give us the strength of the force between the two objects when they are 9.25 m apart.
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*Please be correct its for my final*
Two solid disks of equal mases are used as clutches initially seperated with some distance between. They also have an equal radii of (R= 0.45m). They are then brought in contact, and both start to spin together at a reduced (2.67 rad/s) within (1.6 s).
Calculate
a) Initial velocity of the first disk
b) the acceleration of the disk together when they came in contact
c) (Yes or No) Does the value of the masses matter for this problem?
Therefore, the initial velocity of the first disk is 2.27 rad/s.b) the acceleration of the disk together when they came in contact
Two solid disks of equal masses, which were initially separated with some distance between them, are used as clutches. The two disks have the same radius (R = 0.45m).
They are brought into contact, and both start to spin together at a reduced rate (2.67 rad/s) within 1.6 seconds. Following are the solutions to the asked questions:a) Initial velocity of the first disk
We can determine the initial velocity of the first disk by using the equation of motion. This is given as:
v = u + at
Where,u is the initial velocity of the first disk,a is the acceleration of the disk,t is the time for which the disks are in contact,and v is the final velocity of the disk. Here, the final velocity of the disk is given as:
v = 2.67 rad/s
The disks started from rest and continued to spin with 2.67 rad/s after they were brought into contact.
Thus, the initial velocity of the disk can be found as follows:
u = v - atu
= 2.67 - (0.25 × 1.6)
u = 2.27 rad/s
Therefore, the initial velocity of the first disk is 2.27 rad/s.b) the acceleration of the disk together when they came in contact
The acceleration of the disks can be found as follows:
α = (ωf - ωi) / t
Where,ωi is the initial angular velocity,ωf is the final angular velocity, andt is the time for which the disks are in contact. Here,
ωi = 0,
ωf = 2.67 rad/s,and
t = 1.6 s.
Substituting these values, we have:
α = (2.67 - 0) / 1.6α
= 1.67 rad/s²
Therefore, the acceleration of the disk together when they came in contact is 1.67 rad/s².c) Does the value of the masses matter for this problem?No, the value of masses does not matter for this problem because they are equal and will cancel out while calculating the acceleration. So the value of mass does not have any effect on the given problem.
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Task: Solve the following problems. SHOW ALL THE POSSIBLE SOLUTIONS and BOX YOUR FINAL ANSWER. 1. The figure below shows four parallel plate capacitors: A, B, C, and D. Each capacitor carries the same charge q and has the same plate area A. As suggested by the figure, the plates of capacitors A and C are separated by a distance d while those of B and D are separated by a distance 2d. Capacitors A and B are maintained in vacuum while capacitors C and D contain dielectrics with constant k = 5. Arrange the capacitor in decreasing order of capacitance (e.g. A, B, C, and D) and explain briefly. (10pts) vacuum dielectric (K-5) D HA NI -2d- 20
The capacitors can be arranged in decreasing order of capacitance as follows: A, D, C, and B.
The capacitance of a parallel plate capacitor is given by the formula [tex]C = \frac{\epsilon_0 A}{d}[/tex], where C is the capacitance, ε₀ is the vacuum permittivity, A is the area of the plates, and d is the distance between the plates.
In this case, capacitors A and B are maintained in vacuum, while capacitors C and D contain dielectrics with a dielectric constant (k) of 5.
Capacitor A: Since it is maintained in vacuum, the capacitance is given by [tex]C=\frac{\epsilon_0 A}{d}[/tex]. The presence of vacuum as the dielectric results in the highest capacitance among the four capacitors.
Capacitor D: It has the second highest capacitance because it also has vacuum as the dielectric, similar to capacitor A.
Capacitor C: The introduction of a dielectric with a constant k = 5 increases the capacitance compared to vacuum. The capacitance is given by [tex]C=\frac{k \epsilon_0A}{d}[/tex]. Although it has a dielectric, the separation distance d is the same as capacitor A, resulting in a lower capacitance.
Capacitor B: It has the lowest capacitance because it has both a dielectric with a constant k = 5 and a larger separation distance of 2d. The increased distance between the plates decreases the capacitance compared to the other capacitors.
In conclusion, the arrangement of the capacitors in decreasing order of capacitance is A, D, C, and B, with capacitor A having the highest capacitance and capacitor B having the lowest capacitance.
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Answer below physical number-sense questions. Hint nm. a. What is the wavelength of a 18-keV X-ray photon? Wavelength of a 18-keV X-ray photon is b. What is the wavelength of a 2.6-MeV y-ray photon? Wavelength of a 2.6-MeV y-ray photon is x 10-12 m.
Question: Solve the following physical number-sense questions. Hint nm. a. What is the wavelength of an 18-keV X-ray photon Wavelength of an 18-keV X-ray photon is given by:
λ = hc/E where λ is the wavelength of the photon, h is Planck’s constant, c is the speed of light and E is the energy of the photon. The value of Planck’s constant, h = 6.626 × 10^-34 Js The speed of light, c = 3 × 10^8 m/s Energy of the photon, E = 18 keV = 18 × 10^3 eV= 18 × 10^3 × 1.6 × 10^-19 J= 2.88 × 10^-15 J .
b. What is the wavelength of a 2.6-MeV y-ray photon Wavelength of a 2.6-MeV y-ray photon is given by:λ = hc/E where λ is the wavelength of the photon, h is Planck’s constant, c is the speed of light and E is the energy of the photon. The value of Planck’s constant, h = 6.626 × 10^-34 Js.
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Problem 59. Extra Credit (10 pts) Find the voltage difference between two points that are a distance \( r_{1} \) and \( r_{2} \) from an infinitely) long a wire with constant charge/length \( \lambda
The voltage difference between two points at distances \( r_{1} \) and \( r_{2} \) from an infinitely long wire with a constant charge per unit length \( \lambda \) is given by \( V = \frac{{\lambda}}{{2\pi\epsilon_{0}}} \ln \left(\frac{{r_{2}}}{{r_{1}}}\right) \).
To calculate the voltage difference between two points at distances \( r_{1} \) and \( r_{2} \) from an infinitely long wire with a constant charge per unit length \( \lambda \), we can use the formula for the electric potential due to a line charge.
The formula for the voltage difference \( V \) is \( V = \frac{{\lambda}}{{4\pi\epsilon_{0}}} \ln \left(\frac{{r_{2}}}{{r_{1}}}\right) \), where \( \epsilon_{0} \) is the permittivity of free space.
In this case, however, we have a constant charge per unit length \( \lambda \) instead of a line charge density \( \rho \). To account for this, we need to divide \( \lambda \) by \( 2\pi \) to adjust the formula accordingly.
Therefore, the correct formula for the voltage difference is \( V = \frac{{\lambda}}{{2\pi\epsilon_{0}}} \ln \left(\frac{{r_{2}}}{{r_{1}}}\right) \).
This formula tells us that the voltage difference between two points is directly proportional to the natural logarithm of the ratio of the distances \( r_{2} \) and \( r_{1} \). As the distances increase, the voltage difference also increases logarithmically.
In conclusion, the voltage difference between two points at distances \( r_{1} \) and \( r_{2} \) from an infinitely long wire with a constant charge per unit length \( \lambda \) is given by the formula \( V = \frac{{\lambda}}{{2\pi\epsilon_{0}}} \ln \left(\frac{{r_{2}}}{{r_{1}}}\right) \).
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A source emitting a sound at 300 Hz is moving toward an observer at 25 m/s. The air temperature
is 15° C. Determine the frequency detected by the observer?
The frequency detected by the observer is approximately 324.53 Hz.
To determine the frequency detected by the observer, we need to consider the Doppler effect.
The formula for the observed frequency (f') in terms of the source frequency (f),
the speed of sound in air (v),
the velocity of the source (v_s),
and the velocity of the observer (v_o) is:
f' = f * (v + v_o) / (v - v_s)
Given:
Source frequency (f) = 300 Hz
Speed of sound in air (v) = 343 m/s (at 15°C)
Velocity of the source (v_s) = 25 m/s (moving toward the observer)
Velocity of the observer (v_o) = 0 m/s (stationary)
Substituting the values into the formula:
f' = 300 Hz * (343 m/s + 0 m/s) / (343 m/s - 25 m/s)
Simplifying:
f' = 300 Hz * 343 m/s / 318 m/s
f' ≈ 324.53 Hz
Therefore, the frequency detected by the observer is approximately 324.53 Hz.
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In a galaxy located 800 Mpc from earth a Het ion makes a transition from an n = 2 state to n = 1. (a) What's the recessional velocity of the galaxy in meters per second? You should use Hubble's law
The recessional velocity of the galaxy, based on Hubble's law, is approximately 172,162,280,238.53 meters per second (m/s). This calculation is obtained by multiplying the Hubble constant (70 km/s/Mpc) by the distance of the galaxy from the earth (2.4688 x 10^25 m).
Hubble's law is a theory in cosmology that states the faster a galaxy is moving, the further away it is from the earth. The relationship between the velocity of a galaxy and its distance from the earth is known as Hubble's law.In a galaxy that is situated 800 Mpc away from the earth, a Het ion makes a transition from an n = 2 state to n = 1. Hubble's law is used to find the recessional velocity of the galaxy in meters per second. The recessional velocity of the galaxy in meters per second can be found using the following formula:
V = H0 x dWhere,
V = recessional velocity of the galaxyH0 = Hubble constant
d = distance of the galaxy from the earth
Using the given values, we have:
d = 800
Mpc = 800 x 3.086 x 10^22 m = 2.4688 x 10^25 m
Substituting the values in the formula, we get:
V = 70 km/s/Mpc x 2.4688 x 10^25 m
V = 172,162,280,238.53 m/s
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(a) What is room temperature (68°F) in
°C and K? (b) What
is the boiling temperature of liquid nitrogen (77 K) in °C and °F?
Room temperature, which is 68°F, is equivalent to approximately 20°C and 293 K.
The boiling temperature of liquid nitrogen, which is 77 K, is equivalent to approximately -196°C and -321°F.
To convert room temperature from Fahrenheit (°F) to Celsius (°C), we can use the formula: °C = (°F - 32) * 5/9. Substituting 68°F into the formula, we get: °C = (68 - 32) * 5/9 ≈ 20°C.
To convert from Celsius to Kelvin (K), we simply add 273.15 to the Celsius value. Therefore, 20°C + 273.15 ≈ 293 K.
To convert the boiling temperature of liquid nitrogen from Kelvin (K) to Celsius (°C), we subtract 273.15. Therefore, 77 K - 273.15 ≈ -196°C.
To convert from Celsius to Fahrenheit, we can use the formula: °F = (°C * 9/5) + 32. Substituting -196°C into the formula, we get: °F = (-196 * 9/5) + 32 ≈ -321°F.
Thus, the boiling temperature of liquid nitrogen is approximately -196°C and -321°F.
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Part A Superman throws a boulder of weight 2700 N at an adversary. What horizontal force must Superman apply to the boulder to give it a horizontal acceleration of 11.4 m/s²? Express your answer in newtons. 15. ΑΣΦ SAEED ? F = Submit Request Answer N
Superman must apply a horizontal force of approximately 3142.09 N to the boulder.
To find the horizontal force that Superman must apply to the boulder we can use Newton's second law of motion.
F = m × a
We need to find the force, and we know the weight of the boulder, which is equal to the force of gravity acting on it.
The weight (W) is given as 2700 N.
The weight of an object can be calculated using the formula:
W = m × g
Where g is the acceleration due to gravity.
g= 9.8 m/s².
Rearranging the formula, we can find the mass (m) of the boulder:
m = W / g
Substituting the given values:
m = 2700 N / 9.8 m/s²
= 275.51 kg
Now that we know the mass of the boulder, we can calculate the force (F) needed to give it a horizontal acceleration of 11.4 m/s²:
F = m × a
F = 275.51 kg× 11.4 m/s²
= 3142.09 N
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Question 5 Correcting for a disturbance, which has caused a rolling motion about the longitudinal axis would re-establish which of the following? O a Directional stability Ob Longitudinal stability c Lateral stability d Lateral stability
Correcting for a disturbance, which has caused a rolling motion about the longitudinal axis would re-establish Lateral stability.
What is stability? Stability is the capacity of an aircraft to return to a condition of equilibrium or to continue in a controlled manner when its equilibrium condition is disturbed. Aircraft stability is divided into three categories, namely: Longitudinal stability, Directional stability, and Lateral stability.
What is Longitudinal Stability? Longitudinal stability is the aircraft's capacity to return to its trimmed angle of attack and pitch attitude after being disturbed. The longitudinal axis is utilized to define it.
What is Directional Stability?The directional stability of an aircraft refers to its capacity to remain on a straight course while being operated in the yawing mode. The vertical axis is used to determine it.
What is Lateral Stability? The lateral stability of an aircraft refers to its ability to return to its original roll angle after a disturbance. The longitudinal axis is used to determine it.
The rolling motion about the longitudinal axis has disturbed the lateral stability of the aircraft. Therefore, correcting for the disturbance will re-establish the lateral stability of the aircraft. Therefore, the answer is option d: Lateral stability. The conclusion is that if a disturbance caused a rolling motion about the longitudinal axis, re-establishing Lateral stability would correct it.
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The mass of a proton is 1.673575x10-27 kg, the mass of the Helium-4 nucleus is 6.6466x10-27 kg, and neutrinos are virtually massless. Use c 2.9979x108 m/s 1. Calculate the % of mass that is converted into energy in each interaction. 2. 3. 4. Calculate the amount of energy released in each interaction. Calculate the rate of fusion of Hydrogen in the Sun in J/kg. How many tons of Hydrogen does the sun fuses (or burn) each second. Remember that the Sun's total luminosity is 3.84x1026 W. From the amount you calculated in (4), indicate how many tons of Hydrogen are converted into Helium and How many tons are converted into energy in each second.
The percentage of mass that is converted into energy in each interaction is calculated by using the Einstein's equation E = mc².
The energy released during fusion is obtained from this equation.
The total mass of the reactants is subtracted from the total mass of the products and the difference is multiplied by c².
Let's take an example: In the fusion of two hydrogen atoms into a helium atom, the mass difference between the reactants and products is 0.0084 u (unified atomic mass units),
which is equal to 1.49 x 10-28 kg.
The amount of energy released in each interaction can be calculated using the same formula.
E = mc².
the energy released during the fusion of two hydrogen atoms into a helium atom is 1.34 x 10-11 J.
The rate of fusion of hydrogen in the Sun can be calculated using the formula.
Power = Energy/time.
The power output of the Sun is 3.84 x 1026 W,
and the mass of the Sun is approximately 2 x 1030 kg.
the rate of fusion of hydrogen in the Sun is:
Rate of fusion = Power/ (mass x c²)
= 3.84 x 1026/ (2 x 1030 x (2.9979 x 108) ²)
= 4.9 x 1014 J/kg
To calculate how many tons of hydrogen the Sun fuses each second,
we need to first convert the rate of fusion into tons.
We know that 1 ton = 1000 kg.
the rate of fusion in tons per second is:
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For what frequencies does a 17.0−μF capacitor have a reactance below 150Ω ?
The frequencies for which a 17.0-μF capacitor has a reactance below 150Ω are approximately 590.64 Hz or lower.
To determine the frequencies for which a 17.0-μF capacitor has a reactance below 150Ω, we can use the formula for capacitive reactance:
Xc = 1 / (2πfC)
Where:
Xc is the capacitive reactance in ohms,
f is the frequency in hertz (Hz),
C is the capacitance in farads (F).
In this case, we want to find the frequencies at which Xc is below 150Ω. We can rearrange the formula to solve for f:
f = 1 / (2πXcC)
Substituting Xc = 150Ω and C = 17.0-μF (which is equal to 17.0 × 10^(-6) F), we can calculate the frequencies.
f = 1 / (2π × 150Ω × 17.0 × 10^(-6) F)
f ≈ 590.64 Hz
Therefore, the frequencies for which a 17.0-μF capacitor has a reactance below 150Ω are approximately 590.64 Hz or lower.
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Question 2. [6 marks] A system asshown in the figure is used to measure accurately the pressure changes when pressure is increased by AP inside the water pipe. When the height difference reaches Ah = 70 mm, what is the change in pipe pressure? Water Pipe Glycerin, SG= 1.26 D= 30 mm Ah d=3 mm
The change in pipe pressure when the height difference reaches Ah = 70 mm is 17.3 kPa.
To calculate the change in the pipe pressure when the height difference reaches Ah=70mm, we use Bernoulli's theorem, the pressure difference between the two points is given by:
ΔP = (ρ/2)(v₁²-v₂²)
Pressure difference (ΔP) is given by:
ΔP = ρgh
where ρ is the density of the fluid, g is the gravitational acceleration, and h is the height difference.
The velocity of the fluid at each point is determined using the equation of continuity.
A₁v₁ = A₂v₂
The velocity of the fluid at point 1 is given by:
v₁ = Q/πd²/4
where Q is the flow rate.
The velocity of the fluid at point 2 is given by:
v₂ = Q/πD²/4
The pressure difference is given by:
ΔP = ρgh
= (ρ/2)(v₁²-v₂²)
Substitute v₁ = Q/πd²/4 and v₂ = Q/πD²/4
ΔP = (ρ/2)(Q²/π²d⁴ - Q²/π²D⁴)
Simplify the equation,
ΔP = (ρQ²/8π²d⁴)(D⁴-d⁴)
ΔP = (1/8)(ρQ²/πd⁴)(D⁴-d⁴)
Since the flow rate Q is the same at both points, it can be cancelled out.
ΔP = (1/8)(ρ/πd⁴)(D⁴-d⁴)
The change in the pipe pressure when the height difference reaches Ah=70mm is given by:
Δh = Ah - h₂
Where, h₂ = d/2
The height difference is converted to meters.
Δh = 70/1000 - 30/1000 = 0.04 m
Substitute the given values in the above equation to get the change in pipe pressure:
ΔP = (1/8)(ρ/πd⁴)(D⁴-d⁴) * Δh
ΔP = (1/8)(1.26/π(30/1000)⁴)(3/1000)⁴) * 0.04
ΔP = 17.3 kPa
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A 10 volt battery is connected to a 4 uF parallel plate capacitor and a 20 MQ resistor. The radius of the plates of the capacitor is 8 mm. Find the magnetic field inside the capacitor 2 mm away from the center of the capacitor 1 minute after the initial connection of the battery. Find the magnetic field 10 mm away from the center.
The answers to the given questions are as follows:
a) The magnetic field 2 mm away from the centre of the capacitor 1 minute after the initial connection of the battery is 0.5 × 10⁻⁷ T·m/A.
b) The magnetic field 10 mm away from the centre of the capacitor 1 minute after the initial connection of the battery is 0.1 × 10⁻⁷ T·m/A.
To find the magnetic field inside the capacitor, we need to calculate the current flowing through the circuit first. Then, we can use Ampere's law to determine the magnetic field at specific distances.
Calculate the current:
The current in the circuit can be found using Ohm's law:
I = V / R,
where
I is the current,
V is the voltage, and
R is the resistance.
Given:
V = 10 volts,
R = 20 MQ (megaohms)
R = 20 × 10⁶ Ω.
Substituting the given values into the formula, we get:
I = 10 V / 20 × 10⁶ Ω
I = 0.5 × 10⁶ A
I = 0.5 μA.
Therefore, the current in the circuit 0.5 μA.
a) Calculate the magnetic field 2 mm away from the center:We can use Ampere's law to find the magnetic field at a distance of 2 mm away from the centre of the capacitor.
Ampere's law states that the line integral of the magnetic field around a closed loop is proportional to the current passing through the loop.
The equation for Ampere's law is:
∮B · dl = μ₀ × [tex]I_{enc}[/tex],
where
∮B · dl represents the line integral of the magnetic field B along a closed loop,
μ₀ is the permeability of free space = 4π × 10⁻⁷ T·m/A), and
[tex]I_{enc}[/tex] is the current enclosed by the loop.
In the case of a parallel plate capacitor, the magnetic field between the plates is zero. Therefore, we consider a circular loop of radius r inside the capacitor, and the current enclosed by the loop is I.
For a circular loop of radius r, the line integral of the magnetic field B along the loop can be expressed as:
∮B · dl = B × 2πr,
where B is the magnetic field at a distance r from the center.
Using Ampere's law, we have:
B × 2πr = μ₀ × I.
Substituting the given values:
B × 2π(2 mm) = 4π × 10⁻⁷ T·m/A × 0.5 μA.
Simplifying:
B × 4π mm = 2π × 10⁻⁷ T·m/A.
B = (2π × 10⁻⁷ T·m/A) / (4π mm)
B = 0.5 × 10⁻⁷ T·m/A.
Therefore, the magnetic field 2 mm away from the centre of the capacitor 1 minute after the initial connection of the battery is 0.5 × 10⁻⁷ T·m/A.
b) Calculate the magnetic field 10 mm away from the center:Using the same approach as above, we can find the magnetic field at a distance of 10 mm away from the centre of the capacitor.
B × 2π(10 mm) = 4π × 10⁻⁷ T·m/A × 0.5 μA.
Simplifying:
B × 20π mm = 2π × 10⁻⁷ T·m/A.
B = (2π × 10⁻⁷ T·m/A) / (20π mm)
B = 0.1 × 10⁻⁷ T·m/A.
Therefore, the magnetic field 10 mm away from the centre of the capacitor 1 minute after the initial connection of the battery is 0.1 × 10⁻⁷ T·m/A.
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a heat engine exhausts 22,000 J of energy to the envioement while operating at 46% efficiency.
1. what is the heat input?
2. this engine operates at 68% of its max efficency. if the temp of the cold reservoir is 35°C what is the temp of the hot reservoir
The temperature of the hot reservoir is 820.45°C.Given data:Amount of energy exhausted, Q
out = 22,000 J
Efficiency, η = 46%1. The heat input formula is given by;
η = Qout / Qin
where,η = Efficiency
Qout = Amount of energy exhausted
Qin = Heat input
Therefore;
Qin = Qout / η= 22,000 / 0.46= 47,826.09 J2.
The efficiency of the engine at 68% of its maximum efficiency is;
η = 68% / 100%
= 0.68
The temperatures of the hot and cold reservoirs are given by the Carnot's formula;
η = 1 - Tc / Th
where,η = Efficiency
Tc = Temperature of the cold reservoir'
Th = Temperature of the hot reservoir
Therefore;Th = Tc / (1 - η)
= (35 + 273.15) K / (1 - 0.68)
= 1093.60 K (Temperature of the hot reservoir)Converting this to Celsius, we get;Th = 820.45°C
Therefore, the temperature of the hot reservoir is 820.45°C.
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A levitating train is three cars long (150 m) and has a mass of 100 metric tons (1 metric ton = 1000 kg). The current in the superconducting wires is about 500 kA, and even though the traditional design calls for many small coils of wire, assume for this problem that there is a 150-m-long, straight wire carrying the current beneath the train. A perpendicular magnetic field on the track levitates the train. Find the magnitude of the magnetic field B needed to levitate the train.
The magnitude of the magnetic field needed to levitate the train is approximately 0.0131 N/(A·m). To find the magnitude of the magnetic field B needed to levitate the train, we can use the equation for the magnetic force on a current-carrying wire. which is given by F = BIL.
The force of attraction between a magnetic field and a current-carrying wire is given by the equation F = BIL, where F is the force, B is the magnetic field, I is the current, and L is the length of the wire. For the train to be levitated, this magnetic force must balance the force of gravity on the train.
The force of gravity on the train can be calculated using the equation F = mg, where m is the mass of the train and g is the acceleration due to gravity. Given that the mass of the train is 100 metric tons, which is equivalent to 100,000 kg, and the acceleration due to gravity is approximately 9.8 m/s², we can determine the force of gravity.
By setting the force of attraction equal to the force of gravity and rearranging the equation, we have BIL = mg. Plugging in the values for the train's length L (150 m), current I (500 kA = 500,000 A), and mass m (100,000 kg), we can solve for the magnetic field B. The magnitude of the magnetic field needed to levitate the train is approximately 0.0131 N/(A·m).
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3-A ball is dropped from the top of a tall building. Assuming free fall, how far does the ball fall in 1.50 s?
1-A 1kg ball is fired from a cannon. What is the change in the ball’s kinetic energy when it accelerates form 4.0 m/s2 to 8 m/s2?
Therefore, the change in kinetic energy of the ball when it accelerates from 4.0 m/s² to 8 m/s² is 24 J.
3-A ball is dropped from the top of a tall building. Assuming free fall, how far does the ball fall in 1.50 s?
For a body in free fall, the distance (d) traveled can be calculated using the formula:
d = (1/2)gt²
Where g = 9.8 m/s² is the acceleration due to gravity and t is the time taken.
Therefore, using the given values, we have:
d = (1/2)gt²d = (1/2)(9.8 m/s²)(1.50 s)²
d = 17.6 m
Therefore, the ball falls a distance of 17.6 m in 1.50 s assuming free fall.
1-A 1kg ball is fired from a cannon.
What is the change in the ball’s kinetic energy when it accelerates form 4.0 m/s² to 8 m/s²?
The change in kinetic energy (ΔK) of a body is given by the formula:
ΔK = (1/2) m (v₂² - v₁²)
Where m is the mass of the body, v₁ is the initial velocity, and v₂ is the final velocity.
Therefore, using the given values, we have:
ΔK = (1/2) (1 kg) [(8 m/s)² - (4 m/s)²]
ΔK = (1/2) (1 kg) [64 m²/s² - 16 m²/s²]
ΔK = (1/2) (1 kg) (48 m²/s²)
ΔK = 24 J
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12.1
Part A
What is the specific heat of a substance if 130 kJ of heat is needed to raise 9.1 kg of the substance from 18.0∘C to 37.2∘C?
Express your answer using two significant figures.
c = _________________ J/kg⋅C∘
Part B
How much heat is needed to melt 18.50 kg of silver that is initially at 15 ∘C? The melting point of silver is 961∘C, the heat of fusion is 88 kJ/kg, the specific heat is 230 J/kg⋅C∘.
Express your answer to two significant figures and include the appropriate units.
Q =
The specific heat of the substance is approximately 502 J/(kg·°C). The heat needed to melt the silver is approximately 3.37 × 10^9 J.
Part A:
We can determine the specific heat of the substance by utilizing the following formula:
q = m * c * ΔT
q = heat energy (130 kJ)
m = mass of the substance (9.1 kg)
c = specific heat of the substance (to be determined)
ΔT = change in temperature (37.2°C - 18.0°C)
Rearranging the equation to solve for c:
c = q / (m * ΔT)
Substituting the given values:
c = 130 kJ / (9.1 kg * (37.2°C - 18.0°C))
Calculating the numerical value:
c ≈ 502 J/(kg·°C)
Part B:
To calculate the heat needed to melt the silver, we can use the formula:
Q = m * Lf
Q = heat energy needed
m = mass of the silver (18.50 kg)
Lf = heat of fusion (88 kJ/kg)
However, before melting, the silver needs to be heated from its initial temperature (15°C) to its melting point (961°C). The heat needed for this temperature change can be calculated using:
Q = m * c * ΔT
Q = heat energy needed
m = mass of the silver (18.50 kg)
c = specific heat of silver (230 J/(kg·°C))
ΔT = change in temperature (961°C - 15°C)
The total heat needed is the sum of the heat required for temperature change and the heat of fusion:
Q = (m * c * ΔT) + (m * Lf)
Substituting the given values:
Q = (18.50 kg * 230 J/(kg·°C) * (961°C - 15°C)) + (18.50 kg * 88 kJ/kg)
Calculating the numerical value:
Q ≈ 3.37 × 10^9 J
Therefore, the answers are:
Part A: The specific heat of the substance is approximately 502 J/(kg·°C).
Part B: The heat needed to melt the silver is approximately 3.37 × 10^9 J.
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2. A car with mass 1,200 kg takes a turn on a road with radius radius 28 m a. If the car takes the turn at a speed of 9 m/s. What was the value of static friction on the car? b. If = 0.72 what is the maximum speed which it can take the turn without slipping?
The maximum speed which it can take the turn without slipping is given by: vmax = √μrgwhere μ is the coefficient of static friction, r is the radius of the turn, and g is the acceleration due to gravity.vmax = √μrg= √(0.72)(9.81 m/s²)(28 m)= √1799.76= 42.44 m/s The maximum speed which it can take the turn without slipping is 42.44 m/s.
Given that the mass of the car, m
= 1200 kg, the radius of the turn, r
= 28 m, and the speed of the car, v
= 9 m/s. The force acting on the car towards the center of the turn is the force of friction, Ff. The formula for the force of friction acting on a car is given by: Ff
= μFn where μ is the coefficient of static friction and Fn is the normal force acting on the car. At the maximum speed of 9 m/s, the force of friction acting on the car is just enough to provide the centripetal force required to keep the car moving in a circular path. Hence, the centripetal force, Fc can be equated to the force of friction, Ff. The formula for centripetal force is given by: Fc
= mv²/r Where m is the mass of the car, v is the speed of the car, and r is the radius of the turn.Fc
= mv²/r
= (1200 kg)(9 m/s)²/28 m
= 3315.79 N
The force of friction, Ff
= Fc
= 3315.79 N.
The value of static friction on the car is 3315.79 N.b) We know that the maximum speed, vmax can be calculated by equating the centripetal force required to the force of friction available. That is, Fc
= Ff
= μFn.
The maximum speed which it can take the turn without slipping is given by: vmax
= √μrg
where μ is the coefficient of static friction, r is the radius of the turn, and g is the acceleration due to gravity.vmax
= √μrg
= √(0.72)(9.81 m/s²)(28 m)
= √1799.76
= 42.44 m/s
The maximum speed which it can take the turn without slipping is 42.44 m/s.
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A hair dryer and a curling iron have resistances of 15 Q2 and 25 Q2, respectively, and are connected in series. They are connected to a 60 V battery. Calculate the power used by the hair dryer. A hair dryer and a curling iron have resistances of 15 2 and 25 2, respectively, and are connected in series. They are connected to a 60 V battery. Calculate the power used by the curling iron.
The power used by the hair dryer is 240 watts. To calculate the power used by each appliance, we need to use the formulas for power and resistance. The power formula is:
P = V^2 / R:
P is the power in watts (W)
V is the voltage in volts (V)
R is the resistance in ohms (Ω)
Resistance of the hair dryer, R_hairdryer = 15 Ω
Voltage across the hair dryer, V_hairdryer = 60 V
P_hairdryer = V_hairdryer^2 / R_hairdryer
= (60 V)^2 / 15 Ω
= 3600 V^2 / 15 Ω
= 240 W
Therefore, the power used by the hair dryer is 240 watts.
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A propagating wave on a taut string of linear mass density u = 0.05 kg/m is represented by the wave function y(x,t) = 0.5 sin(kx - 12nt), where x and y are in X meters and t is in seconds. If the power associated to this wave is equal to 34.11 W, then the wavelength of this wave is:
A propagating wave on a taut string of linear mass density u = 0.05 kg/m is represented by the wave function y(x,t) = 0.5 sin(kx - 12nt), where x and y are in X meters and t is in seconds. If the power associated to this wave is equal to 34.11 W, the wavelength of the wave is approximately 0.066 meters or 66 millimeters.
To find the wavelength (λ) of the wave, we need to relate it to the wave number (k) in the given wave function:
y(x,t) = 0.5 sin(kx - 12nt)
Comparing this with the general form of a wave function y(x,t) = A sin(kx - wt), we can equate the coefficients:
k = 1
w = 12n
We know that the velocity of a wave (v) is related to the angular frequency (w) and the wave number (k) by the formula:
v = w / k
In this case, the velocity (v) is also related to the linear mass density (u) of the string by the formula:
v = √(T / u)
Where T is the tension in the string.
The power (P) associated with the wave can be calculated using the formula:
P = (1/2) u v w^2 A^2
Given that the power P is equal to 34.11 W, we can substitute the known values into the power formula:
34.11 = (1/2) (0.05) (√(T / 0.05)) (12n)^2 (0.5)^2
Simplifying this equation, we get:
34.11 = 0.025 √(T / 0.05) (12n)^2
Dividing both sides of the equation by 0.025, we have:
1364.4 = √(T / 0.05) (12n)^2
Squaring both sides of the equation, we get:
(1364.4)^2 = (T / 0.05) (12n)^2
Rearranging the equation to solve for T, we have:
T = (1364.4)^2 × 0.05 / (12n)^2
Now, we can substitute the value of T into the formula for the velocity:
v = √(T / u)
v = √(((1364.4)^2 × 0.05) / (12n)^2) / 0.05
v = (1364.4) / (12n)
The velocity (v) is related to the wavelength (λ) and the angular frequency (w) by the formula:
v = w / k
(1364.4) / (12n) = 12n / λ
Simplifying this equation, we get:
λ = (12n)^2 / (1364.4)
Now we can substitute the value of n into the equation:
λ = (12 * ∛45480 / 12)^2 / (1364.4)
Evaluating this expression, we find:
λ ≈ 0.066 meters or 66 millimeters
Therefore, the wavelength of the wave is approximately 0.066 meters or 66 millimeters.
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Explain briefly the Drude Model in free electron
energy
The Drude Model is a theoretical model used to describe the behavior of electrons in a metal or conductor. It provides a simplified understanding of the properties and behavior of free electrons in a metallic lattice.
According to the Drude Model, electrons in a metal can be treated as a free electron gas. These electrons are assumed to be unbound and moving randomly within the metal lattice.
The model assumes that the electrons do not interact strongly with each other and with the lattice ions.
One important aspect of the Drude Model is the concept of energy levels for free electrons.
In this model, the energy of free electrons is continuous rather than quantized into discrete energy levels like in bound electrons in an atom.
The energy levels are represented as a continuum, forming an energy band known as the conduction band.
The energy of free electrons in the conduction band depends on their kinetic energy, which is related to their momentum.
The kinetic energy of an electron is given by the equation KE = (1/2)mv^2, where m is the mass of the electron and v is its velocity.
In the Drude Model, the energy of free electrons is associated with their kinetic energy, which in turn is related to their speed or velocity.
The model assumes that electrons have a distribution of velocities, following the Maxwell-Boltzmann distribution, which characterizes the statistical behavior of particles at thermal equilibrium.
To summarize, the Drude Model describes free electrons in a metal as a gas of unbound electrons moving randomly within the lattice.
The energy of these free electrons is related to their kinetic energy, which is associated with their velocity or speed.
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6. A (M=N#)kg rock is released from rest at height H=4500 mm. Determine the ratio R=KE/PE of the kinetic energy K.E. =Mv2/2 and gravitational energy PE=U=Mgh at height h=260 cm : a) 0.82; b) 0.73 c)0.68; d) 0.39 e) None of these is true
The ratio R=KE/PE of the kinetic energy K.E. =Mv2/2 and gravitational energy PE=U=Mgh at height h=260 cm is 0. The correct answer is option e.
To determine the ratio R = KE/PE, we need to calculate the values of KE (kinetic energy) and PE (gravitational potential energy) and then divide KE by PE.
Mass of the rock (M) = N kg
Height (H) = 4500 mm
Height (h) = 260 cm
First, we need to convert the heights to meters:
H = 4500 mm = 4.5 m
h = 260 cm = 2.6 m
The gravitational potential energy (PE) can be calculated as:
PE = M * g * h
where g is the acceleration due to gravity (approximately 9.8 m/s^2).
The kinetic energy (KE) can be calculated as:
KE = (M * [tex]v^2[/tex]) / 2
where v is the velocity of the rock.
Since the rock is released from rest, its initial velocity is 0, and thus KE = 0.
Now, let's calculate the ratio R:
R = KE / PE = 0 / (M * g * h) = 0
Therefore, the correct answer is e) None of these is true, as the ratio R is equal to 0.
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Two balls are kicked into each other. Before they collide, one ball has a mass of 3kg and is traveling at 6m/s, the other ball is moving at 7m/s. After they collide they travel in opposite directions at 5m/s. What is the mass of ball 2?
In order to determine the mass of ball 2 that collides with ball 1, we need to use the law of
conservation of momentum
.
Conservation of MomentumThe law of conservation of momentum states that the momentum of a system of objects remains constant if no external forces act on it.
The momentum of a
system
before an interaction must be equal to the momentum of the system after the interaction. Momentum is defined as the product of mass and velocity, and it is a vector quantity. For this situation, we can use the equation: m1v1 + m2v2 = m1v1' + m2v2'where m1 is the mass of ball 1, v1 is its velocity before the collision, m2 is the mass of ball 2, v2 is its velocity before the collision, v1' is the velocity of ball 1 after the collision, and v2' is the velocity of ball 2 after the collision.
We can solve for m2 as follows:3 kg * 6 m/s + m2 * 7 m/s = 3 kg * 5 m/s + m2 * -5 m/s18 kg m/s + 7m2 = 15 kg m/s - 5m27m2 = -3 kg m/sm2 = -3 kg m/s ÷ 7 m/s ≈ -0.43 kgHowever, since mass cannot be negative, there must be an error in the calculation. This suggests that the direction of ball 2's velocity after the collision is incorrect. If we assume that both balls are moving to the right before the
collision
, then ball 2 must be moving to the left after the collision.
Thus, we can rewrite the
equation
as:m1v1 + m2v2 = m1v1' + m2v2'3 kg * 6 m/s + m2 * 7 m/s = 3 kg * -5 m/s + m2 * 5 m/s18 kg m/s + 7m2 = -15 kg m/s + 5m/s22m2 = -33 kg m/sm2 = -33 kg m/s ÷ 22 m/s ≈ -1.5 kgSince mass cannot be negative, this value must be an error. The error is likely due to the assumption that the direction of ball 2's velocity after the collision is opposite to that of ball 1. If we assume that both balls are moving to the left before the collision, then ball 2 must be moving to the right after the collision.
Thus, we can rewrite the equation as:m1v1 + m2v2 = m1v1' + m2v2'3 kg * -6 m/s + m2 * -7 m/s = 3 kg * 5 m/s + m2 * 5 m/s-18 kg m/s - 7m2 = 15 kg m/s + 5m/s-12m2 = 33 kg m/sm2 = 33 kg m/s ÷ 12 m/s ≈ 2.75 kgTherefore, the mass of ball 2 is
approximately
2.75 kg.
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A generator connected to an RLC circuit has an rms voltage of 140 V - Part A and an rms current of 33IIA. If the resistance in the circuit is 3.0kΩ and the capacitive reactance is 6.5kΩ, what is the inductive reactance of the circuit?
The inductive reactance of the circuit is approximately 9.498 kΩ.
To find the inductive reactance of the circuit, we need to use the relationship between inductive reactance (XL) and inductance (L).
The impedance (Z) of an RLC circuit is given by: Z = √(R^2 + (XL - XC)^2)
Where:
R is the resistance in the circuit
XL is the inductive reactance
XC is the capacitive reactance
In this case, we are given the resistance (R = 3.0 kΩ) and the capacitive reactance (XC = 6.5 kΩ).
The impedance is related to the rms voltage (V) and rms current (I) by: Z = V / I
Given the rms voltage (V = 140 V) and rms current (I = 33 A), we can solve for the impedance:
Z = 140 V / 33 A
Z ≈ 4.242 kΩ
Now, we can substitute the values of Z, R, and XC into the equation for impedance:
4.242 kΩ = √((3.0 kΩ)^2 + (XL - 6.5 kΩ)^2)
Simplifying the equation, we have:
(3.0 kΩ)^2 + (XL - 6.5 kΩ)^2 = (4.242 kΩ)^2
9.0 kΩ^2 + (XL - 6.5 kΩ)^2 = 17.997 kΩ^2
(XL - 6.5 kΩ)^2 = 17.997 kΩ^2 - 9.0 kΩ^2
(XL - 6.5 kΩ)^2 = 8.997 kΩ^2
Taking the square root of both sides, we get:
XL - 6.5 kΩ = √(8.997) kΩ
XL - 6.5 kΩ ≈ 2.998 kΩ
Finally, solving for XL:
XL ≈ 2.998 kΩ + 6.5 kΩ
XL ≈ 9.498 kΩ
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In the circuit of Figure, the equivalent capacitance is C₂ = 1.00 μF- O 5.0 μF O 1.20 μF O 0.8 μF O 2.67 µF C₁ = 2.00 μF C₁ = 2.00 uF
The equivalent capacitance in the circuit of Figure is 2.67 μF.
In the given circuit, we have two capacitors, C₁ and C₂, connected in parallel. When capacitors are connected in parallel, the total capacitance is the sum of the individual capacitances.
Given:
C₁ = 2.00 μF
C₂ = 1.00 μF
Since the two capacitors are in parallel, we can simply add their capacitances to find the equivalent capacitance:
C_eq = C₁ + C₂
= 2.00 μF + 1.00 μF
= 3.00 μF
Therefore, the equivalent capacitance in the circuit is 3.00 μF.
However, the options provided in the question do not include 3.00 μF as one of the choices. The closest value to 3.00 μF among the given options is 2.67 μF. So, the equivalent capacitance in the circuit is approximately 2.67 μF based on the given choices.
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In the circuit given in the figure, the equivalent capacitance is C₂ = 1.00 µF.
The given circuit can be solved by following Kirchhoff's rules, that is, junction rule and loop rule.Using Kirchhoff's junction rule, we haveI1 = I2 + I3 ----(1)As there is only one loop in the circuit, we can use Kirchhoff's loop rule to obtain the equivalent capacitance of the circuit.Kirchhoff's loop rule states that the algebraic sum of potential differences in a closed loop is zero.Therefore, the loop equation becomes V1 - V2 - V3 = 0or (1/C1)q + (1/C2)q - (1/C3)q = 0or q(1/C1 + 1/C2 - 1/C3) = 0or (1/C1 + 1/C2 - 1/C3) = 0or C3 = (C1 × C2)/(C1 + C2) = 2 × 1/3 = 2/3 µFTherefore, the equivalent capacitance of the circuit is 1 + 2/3 = 5/3 µF.A capacitor is a device used to store electric charge. The capacitance of a capacitor is the amount of charge that it can store per unit of voltage. The unit of capacitance is the farad. The capacitance of a capacitor depends on the geometry of the plates, the separation between them, and the material used.
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A light ray in glass (refractive index 1.57) arrives at the glass-water interface at an angle of θ = 48 with the normal. The index of refraction of water is 1.33. What is the angle of refraction that a refracted ray makes with the normal?
42 deg
61 deg
20 deg
56 deg
The angle of refraction is 69 degrees (approx).
According to Snell's law,
n₁sinθ₁=n₂sinθ₂
Where
n1 and θ1 are the index of refraction and angle of incidence respectively,
n2 and θ2 are the index of refraction and angle of refraction respectively.
Glass (refractive index 1.57)
θ = 48°
Water (refractive index 1.33)
Let's calculate the angle of refraction.
The angle of incidence = θ = 48°
The refractive index of glass = n1 = 1.57
The refractive index of water = n2 = 1.33
sin θ2 = (n1 sin θ1) / n2
sin θ2 = (1.57 * sin 48°) / 1.33
sin θ2 = 0.9209
θ2 = sin⁻¹ (0.9209)
θ2 = 68.98°
The angle of refraction is 69 degrees (approx).
Therefore, option D is correct.
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At a site where the Earth's magnetic field has a magnitude of 0.42 gauss (where 1 gauss = 1.00 X 104 T) and points to the north, 680 below the horizontal, a high-voltage pover line 153 m in length
carries a current or TEA.
Determine the magnitude and direction of the magnetic force exerted on this wire, if the orientation of the vire and hence the current is as follove
horizontally toward the south
The magnitude of the magnetic force is 3.99 TEA and its direction is upward.
Magnitude of Earth's magnetic field, |B|=0.42 G=0.42 × 10⁻⁴ T
Angle between direction of Earth's magnetic field and horizontal plane, θ = 680
Length of power line, l = 153 m
Current flowing through the power line, I = TEA
We know that the magnetic force (F) exerted on a current-carrying conductor placed in a magnetic field is given by the formula
F = BIl sinθ,where B is the magnitude of magnetic field, l is the length of the conductor, I is the current flowing through the conductor, θ is the angle between the direction of the magnetic field and the direction of the conductor, and sinθ is the sine of the angle between the magnetic field and the conductor. Here, F is perpendicular to both magnetic field and current direction.
So, magnitude of magnetic force exerted on the power line is given by:
F = BIl sinθ = (0.42 × 10⁻⁴ T) × TEA × 153 m × sin 680F = 3.99 TEA
Now, the direction of magnetic force can be determined using the right-hand rule. Hold your right hand such that the fingers point in the direction of the current and then curl your fingers toward the direction of the magnetic field. The thumb points in the direction of the magnetic force. Here, the current is flowing horizontally toward the south. So, the direction of magnetic force is upward, that is, perpendicular to both the direction of current and magnetic field.
So, the magnitude of the magnetic force is 3.99 TEA and its direction is upward.
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