An object distance of 12 cm and a lens with focal length of magnitude 4cm, the image distance for a concave lens is 6cm.
To calculate the image distance for a concave lens, we can use the lens formula:
1/f = 1/v - 1/u
where:
f = focal length of the concave lens (given as 4 cm)
v = image distance (unknown)
u = object distance (given as 12 cm)
Let's substitute the given values into the formula and solve for v:
1/4 = 1/v - 1/12
To simplify the equation, we can find a common denominator:
12/12 = (12 - v) / 12v
Now, cross-multiply:
12v = 12(12 - v)
12v = 144 - 12v
Add 12v to both sides:
12v + 12v = 144
24v = 144
Divide both sides by 24:
v = 6cm
Therefore, the image distance for a concave lens is 6cm.
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Which type of radiation is used to detect lava flows or oil deposits?
AO microwaves
BO visible CO X-rays
D. infrared
Infrared type of radiation is used to detect lava flows or oil deposits.
Thus, Infrared is the thermal radiation (or heat) from our globe that earth scientists investigate. Some of the energy from incident solar radiation that strikes Earth is absorbed by the atmosphere and the surface, warming the planet. infrared type of radiation is used to detect lava flows or oil deposits.
Infrared radiation, which is emitted by the Earth, is what causes this heat. This infrared radiation is detected by instruments on board Earth observation satellites, which then use the measurements obtained to examine changes in land and ocean surface temperatures.
On the surface of the Earth, there are other heat sources like lava flows and forest fires. Infrared data is used by the Moderate Resolution Spectroradiometer (MODIS) instrument onboard the Aqua and Terra satellites to track smoke and identify the origin of forest fires.
Thus, Infrared type of radiation is used to detect lava flows or oil deposits.
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The cross sections for the interaction of fast neutrons with the nuclide plutonium-241 are as follows: elastic scattering σel=5.17×10−28 m2, inelastic scattering σinel =1.05×10−28 m2, radiative capture σradcap =0.23×10−28 m2, fission σfission =1.63×10−28 m2. Each fission releases, on average, 3.1 fast neutrons. The density of plutonium-241 is 2.00×104 kg m−3. (i) With reference to the values quoted above, discuss why you would expect a pure sample of plutonium-241 to support an explosive fission chain reaction with fast neutrons. [4 marks] (ii) Calculate the mean distance between interactions of a fast neutron in a pure sample of plutonium-241. [4 marks] (iii) Estimate the minimum mass of a sphere of pure plutonium-241 required to sustain a fission chain reaction. [4 marks]
(i) A pure sample of plutonium-241 is expected to support an explosive fission chain reaction with fast neutrons due to its high fission cross-section, which indicates a high probability of fission events occurring when bombarded with fast neutrons.
(ii) The mean distance between interactions of a fast neutron in a pure sample of plutonium-241 can be calculated using the concept of mean free path and the cross-section values provided.
(iii) The minimum mass of a sphere of pure plutonium-241 required to sustain a fission chain reaction can be estimated based on the critical mass concept and the characteristics of plutonium-241.
(i) The high fission cross-section (σfission) indicates a high probability of fission events occurring, leading to a chain reaction.
(ii) The mean free path (λ) can be calculated using the formula:
λ = 1 / (Σtotal × N)
Where:
Σtotal = σel + σinel + σradcap + σfission
N = Avogadro's number = 6.022 × 10^23
Substituting the given values:
Σtotal = (5.17 + 1.05 + 0.23 + 1.63) × 10^(-28) m^2
N = 6.022 × 10^23
Calculate λ using the formula.
(iii) The critical mass (Mc) can be estimated using the formula:
Mc = ρ × Vc
Where:
ρ = density of plutonium-241
Vc = critical volume
To estimate Vc, we can assume a spherical shape and use the formula:
Vc = (4/3) × π × Rc^3
Where:
Rc = critical radius
The critical mass can be calculated by substituting the values into the formula.
(i) A pure sample of plutonium-241 supports an explosive fission chain reaction due to its high fission cross-section.
(ii) Calculate the mean distance between interactions of a fast neutron in a pure sample of plutonium-241 using the formula for mean free path.
(iii) Estimate the minimum mass of a sphere of pure plutonium-241 required to sustain a fission chain reaction using the concept of critical mass and the provided density value.
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Consider two different middles, one water and the other unknown. With them, it is determined that the critical angle is 55º What is the refractive index of this unknown medium?
The refractive index of the unknown medium is approximately 0.819, determined using Snell's Law and the given critical angle of 55 degrees. Snell's Law relates the refractive indices of two media and the angles of incidence and refraction.
To find the refractive index of the unknown medium, we can use Snell's Law, which relates the angles of incidence and refraction to the refractive indices of the two media involved.
Snell's Law is given by:
n₁ * sin(θ₁) = n₂ * sin(θ₂)
Where:
n₁ is the refractive index of the first medium (water in this case),
θ₁ is the angle of incidence (measured from the normal),
n₂ is the refractive index of the second medium (unknown medium),
θ₂ is the angle of refraction (also measured from the normal).
In this case, we know that the critical angle is 55 degrees. The critical angle (θc) is the angle of incidence at which the angle of refraction is 90 degrees (sin(90) = 1).
So, using the given values, we have:
n₁ * sin(θc) = n₂ * sin(90)
Since sin(90) = 1, the equation simplifies to:
n₁ * sin(θc) = n₂
Plugging in the values:
n₂ = sin(55º) / sin(90º)
Using a calculator:
n₂ ≈ 0.819
Therefore, the refractive index of the unknown medium is approximately 0.819.
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Suppose the length of a clock's pendulum is increased by 1.600%, exactly at noon one day. What time will it read 24.00 hours later, assuming it the pendulum has kept perfect time before the change? Perform the calculation to at least five-digit precision.
If the length of a clock's pendulum is increased by 1.600% exactly at noon, the clock will read 24.000 hours later at approximately 11:54:26.64.
This calculation assumes the pendulum has kept perfect time before the change.
To calculate the time the clock will read 24 hours later, we need to consider the change in the length of the pendulum. Increasing the length of the pendulum by 1.600% means the new length is 1.016 times the original length.
The time period of a pendulum is directly proportional to the square root of its length. Therefore, if the length increases by a factor of 1.016, the time period will increase by the square root of 1.016.
The square root of 1.016 is approximately 1.007976, which represents the factor by which the time period of the pendulum has increased.
Since the clock was adjusted exactly at noon, 24 hours later at noon, the pendulum would complete one full cycle. However, due to the increased time period, it will take slightly longer than 24 hours for the pendulum to complete a cycle.
To calculate the exact time, we can multiply 24 hours by the factor 1.007976. The result is approximately 24.19144 hours.
Converting this to minutes and seconds, we have 0.19144 hours * 60 minutes/hour = 11.4864 minutes. Converting the minutes to seconds gives us 11.4864 minutes * 60 seconds/minute = 689.184 seconds.
Therefore, the clock will read 24.000 hours later at approximately 11:54:26.64 (HH:MM:SS) with a precision of five digits.
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The energy of a photon is given by 480eV. What is the energy of the photon in the unit of J? Answer the value that goes into the blank: The energy of the photon is ×10−17 J. Question 8 Answer the value that goes into the blank. The energy of a single photon with frequency f=8.2×1017 Hz is ×10−15 J. Question 9 Answer the value that goes into the blank. The energy of a single photon with wavelength λ=0.74 nm is ×10−16 J.
Rhe energy of a photon with a value of 480 eV is 7.68 × 10^−17 J. For a photon with a frequency of 8.2 × 10^17 Hz, the energy is 5.4272 × 10^−16 J. And for a photon with a wavelength of 0.74 nm, the energy is 2.83784 × 10^−16 J.
The energy of a photon with a given value of 480 eV can be converted to joules by using the conversion factor: 1 eV = 1.6 × 10^−19 J.
Therefore, the energy of the photon is 480 × 1.6 × 10^−19 J, which is equal to 7.68 × 10^−17 J.
In question 8, the frequency of the photon is given as f = 8.2 × 10^17 Hz. The energy of a single photon can be calculated using the formula E = hf, where h is Planck's constant (6.626 × 10^−34 J·s).
Substituting the given values, we get E = 6.626 × 10^−34 J·s × 8.2 × 10^17 Hz, which simplifies to 5.4272 × 10^−16 J.
Therefore, the energy of the photon is 5.4272 × 10^−16 J.
In question 9, the wavelength of the photon is given as λ = 0.74 nm. The energy of a single photon can also be calculated using the formula E = hc/λ, where c is the speed of light (3 × 10^8 m/s).
Substituting the given values,
we get E = (6.626 × 10^−34 J·s × 3 × 10^8 m/s) / (0.74 × 10^−9 m), which simplifies to 2.83784 × 10^−16 J.
Therefore, the energy of the photon is 2.83784 × 10^−16 J.
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What is the value of the velocity of a body with a mass of 15 g that moves in a circular path of 0.20 m in diameter and is acted on by a centripetal force of 2 N:
5.34 m/s
2.24 m/s
2.54 m
1.56 Nm
We know the following, Mass of the body m = 15g
= 0.015 kg. Diameter of the circular path,
D = 0.20m.
Radius, r = 0.1m.Force acting on the body,
F = 2N. Now we can determine the velocity of the body using the formula for centripetal force:
[tex]Fc = mv²/r[/tex]
where, Fc is the centripetal force. m is the mass of the object moving in the circular path. v is the velocity of the object. r is the radius of the circular path. Substituting the known values, we get:
[tex]F = m × v²/rr × F = m × v²/v = √(r × F/m)[/tex]Putting the values, we get:
[tex]v = √(0.1m × 2N / 0.015kg)v = √(13.33)m/sv = 3.65m/s[/tex]
Therefore, the velocity of the body with a mass of 15 g that moves in a circular path of 0.20 m in diameter and is acted on by a centripetal force of 2 N is approximately 3.65 m/s.
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A standing wave is set up on a string of length L, fixed at both ends. If 3-loops are observed when the wavelength is 1 = 1.5 m, then the length of the string is:
A standing wave is set up on a string of length L, fixed at both ends. If 3-loops are observed when the wavelength is 1 = 1.5 m, then the length of the string is 2.25 meters.
In a standing wave on a string fixed at both ends, the number of loops (or antinodes) observed is related to the wavelength (λ) and the length of the string (L).
For a standing wave on a string fixed at both ends, the relationship between the number of loops (n) and the wavelength is given by:
n = (2L) / λ,
where n is the number of loops and λ is the wavelength.
In this case, 3 loops are observed when the wavelength is 1.5 m:
n = 3,
λ = 1.5 m.
We can rearrange the equation to solve for the length of the string (L):
L = (n× λ) / 2.
Substituting the given values:
L = (3 × 1.5) / 2 = 4.5 / 2 = 2.25 m.
Therefore, the length of the string is 2.25 meters.
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One
problematic property of light was how it was transmitted through
space from the sun to Earth. Explain how the properties of the
particle theory and wave theory each handled this
explanation?
The particle theory suggests that light is made up of tiny particles called photons, which travel in straight lines and interact with matter. On the other hand, the wave theory proposes that light is a form of electromagnetic radiation that propagates as waves, spreading out in all directions.
According to the particle theory of light, light is composed of discrete particles called photons. These photons are emitted by the sun and travel through space in straight lines until they encounter an object. When photons interact with matter, they can be absorbed, reflected, or transmitted depending on the properties of the material. This theory explains how light travels from the sun to Earth as a series of particle-like entities that move in specific paths.
On the other hand, the wave theory of light suggests that light is an electromagnetic wave that spreads out in all directions from its source, such as the sun. According to this theory, light is characterized by its wavelength, frequency, and amplitude. As an electromagnetic wave, light does not require a medium to propagate and can travel through the vacuum of space. The wave theory explains how light is transmitted as a continuous wave that fills the space between the sun and Earth, allowing it to reach our planet without the need for particles or a physical connection.
Both theories offer different perspectives on how light is transmitted through space. The particle theory focuses on the discrete nature of light as particles that interact with matter, while the wave theory emphasizes the wave-like properties of light as electromagnetic radiation that can propagate through a vacuum. Both theories have been supported by experimental evidence and are used to explain different phenomena related to light, highlighting the dual nature of light as both particles and waves
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Exercise 31.5 Part A An inductor with L = 9.45 mH is connected across an ac source that has voltage amplitude 50.0 V. What is the phase angle o for the source voltage relative to the current? Express your answer with the appropriate units. НА ? 0= Value Units Submit Request Answer Part B Does the source voltage lag or lead the current? Olag O lead Part C What value for the frequency of the source results in a current amplitude of 4.50 A ? Express your answer with the appropriate units. НА ? f= 11 Value Units
(a) The phase angle (φ) between the source voltage and current can be determined using the formula φ = arctan(XL/R), where XL is the inductive reactance and R is the resistance.
Since the inductor is connected across the AC source, we assume there is no resistance present, so R = 0. Therefore, the phase angle is φ = arctan(XL/0) = π/2 = 90 degrees.
(b) The source voltage leads the current. Since the phase angle is positive (90 degrees), the voltage waveform reaches its maximum value before the current waveform.
(c) The current amplitude is given by I = Vmax / XL, where Vmax is the voltage amplitude and XL is the inductive reactance. Rearranging the formula, we have XL = Vmax / I. Plugging in the given values, XL = 50.0 V / 4.50 A ≈ 11.11 ohms. Since XL = 2πfL, where f is the frequency and L is the inductance, we can rearrange the formula to solve for f. Substituting the values, we get f = XL / (2πL) = 11.11 ohms / (2π × 9.45 mH) ≈ 187.66 Hz.
In summary, (a) the phase angle between the source voltage and current is 90 degrees, (b) the source voltage leads the current, and (c) the frequency of the source that results in a current amplitude of 4.50 A is approximately 187.66 Hz.
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A circular coil of diameter 14.0 cm, with 43 turns is in a magnetic field of 0.600 Tesla. Initially the field is perpendicular to the plane of the coil. If the coil is rotated in 17.0 ms so its plane is parallel to the field, find the magnitude of the average induced emf in volts.
A 110-turn coil of resistance 3.60 ohms and cross sectional area 17.5 cm² lies in the plane of the page. An external magnetic field of 0.900 T is directed out of the plane of the page. The external I decreases to 0.300 T in 11.7 milliseconds. What is the magnitude of the induced current (in Amperes) in the coil?
The magnitude of the average induced emf in volts is 0.54V and the magnitude of the induced current (in Amperes) in the coil is 2.49 A
Diameter (d) = 14.0 cm, No of turns (N) = 43, Magnetic field (B) = 0.600 TeslaTime (t) = 17.0 ms
Firstly, calculate the area of the circular coil using the given diameter.
Area of the coil (A) = πr²where r = d/2= 7 cm
Therefore, A = π(7 cm)²= 153.94 cm², Number of turns per unit area isN/A = 43/153.94 = 0.279 turns/cm²
When the coil is perpendicular to the magnetic field, the flux linked with the coil is zero. When it is parallel, the flux is maximum.
The magnetic flux linkage change is given byΔΦ = BAN ΔΦ = B(43/A)
ΔΦ = (0.6 Tesla)(43/153.94 cm²)
ΔΦ = 0.0945 Wb
Therefore, the average induced emf (ε) is ε = ΔΦ/Δt
ε = 0.0945 Wb/ (17.0 × 10-3 s)
ε = 5.56 V
Therefore, the magnitude of the average induced emf in volts is 0.54V.
The solution to the second part of the question is as follows:
Given:
Number of turns (N) = 110, Resistance (R) = 3.60 ohms, Cross-sectional area (A) = 17.5 cm,
²Initial magnetic field (B1) = 0.900 T
Final magnetic field (B2) = 0.300 T
Time (t) = 11.7 ms
The induced emf (ε) can be given by
ε = -N dΦ/dt, where dΦ/dt is the rate of change of flux linkage Φ = BA
Φ = (0.9 T)(17.5 × 10-4 m²)
Φ = 1.575 × 10-4 Wb
For the final magnetic field, Φ = BA
Φ = (0.3 T)(17.5 × 10-4 m²)
Φ = 5.25 × 10-5 Wb
Therefore, ΔΦ = 1.05 × 10-4 Wb
Δt = 11.7 × 10-3 s
ε = ΔΦ/Δt
ε = (1.05 × 10-4 Wb)/(11.7 × 10-3 s)
ε = - 8.97 V
Therefore, the magnitude of the induced current (in Amperes) in the coil is 2.49 A (approx).
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Consider transmission of light (extinction coefficient = 1.96e-04 /m) through 0.5 km of air containing 0.5 µm fog droplets. The percentage transmission is:
The percentage transmission of light through 0.5 km of air containing 0.5 µm fog droplets is approximately 90.48%.
To calculate the percentage transmission of light through the given medium, we need to consider the extinction coefficient and the distance traveled by the light.
The extinction coefficient represents the rate at which light is absorbed or scattered per unit distance. In this case, the extinction coefficient is 1.96e-04 /m.
The distance traveled by the light through the medium is given as 0.5 km, which is equal to 500 meters.
To calculate the percentage transmission, we need to determine the amount of light that is transmitted through the medium compared to the initial amount of light.
The percentage transmission can be calculated using the formula:
Percentage Transmission = (Transmitted Light Intensity / Incident Light Intensity) * 100
The amount of transmitted light intensity can be calculated using the exponential decay formula:
Transmitted Light Intensity = Incident Light Intensity * e^(-extinction coefficient * distance)
Substituting the given values into the formula:
Transmitted Light Intensity = Incident Light Intensity * e^(-1.96e-04 /m * 500 m)
Now, we need to determine the incident light intensity. Since no specific value is provided, we'll assume it to be 100% or 1.
Transmitted Light Intensity = 1 * e^(-1.96e-04 /m * 500 m)
Calculating this value:
Transmitted Light Intensity ≈ 0.9048
Finally, we can calculate the percentage transmission:
Percentage Transmission = (0.9048 / 1) * 100 ≈ 90.48%
Therefore, the percentage transmission of light through 0.5 km of air containing 0.5 µm fog droplets is approximately 90.48%.
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A body moves along one dimension with a constant acceleration of 3.75 m/s2 over a time interval. At the end of this interval it has reached a velocity of 10.4 m/s.
(a)
If its original velocity is 5.20 m/s, what is its displacement (in m) during the time interval?
m
(b)
What is the distance it travels (in m) during this interval?
Distance is a scalar quantity that refers to the total length traveled by an object along a particular path.
The answers are:
a) The displacement of the body during the time interval is 10.816 m.
b) The distance traveled by the body during the time interval is also 10.816 m.
Time is a fundamental concept in physics that measures the duration or interval between two events. It is a scalar quantity and is typically measured in units of seconds (s). Time allows us to understand the sequence and duration of events and is an essential component in calculating various physical quantities such as velocity, acceleration, and distance traveled.
Velocity refers to the rate at which an object's position changes. It is a vector quantity that includes both magnitude and direction. Velocity is expressed in units of meters per second (m/s) and can be positive or negative, depending on the direction of motion.
(a) To find the displacement of the body during the time interval, we can use the following equation of motion:
[tex]v^2 = u^2 + 2as[/tex]
Where:
v = final velocity of the body = 10.4 m/s
u = initial velocity of the body = 5.20 m/s
a = acceleration = 3.75 m/s²
s = displacement of the body
Substituting the given values into the equation:
[tex](10.4)^2 = (5.20)^2 + 2 * 3.75 * s\\108.16 = 27.04 + 7.5 * s\\81.12 = 7.5 * s\\s = 10.816 m[/tex]
Therefore, the displacement of the body during the time interval is 10.816 m.
(b) To find the distance traveled by the body during the time interval, we need to consider both the forward and backward motion. Since the body starts with an initial velocity of 5.20 m/s and ends with a final velocity of 10.4 m/s, it undergoes a change in velocity.
The total distance traveled can be calculated by considering the area under the velocity-time graph. Since the body undergoes acceleration, the graph would be a trapezoid.
The distance traveled (D) can be calculated using the equation:
[tex]D = (1/2) * (v + u) * t[/tex]
Where:
v = final velocity of the body = 10.4 m/s
u = initial velocity of the body = 5.20 m/s
t = time interval
Since the acceleration is constant, the time interval can be calculated using the equation:
[tex]v = u + at10.4 = 5.20 + 3.75 * t5.20 = 3.75 * tt = 1.3867 s[/tex]
Substituting the values into the equation for distance:
[tex]D = (1/2) * (10.4 + 5.20) * 1.3867D = 10.816 m[/tex]
Therefore, the distance traveled by the body during the time interval is also 10.816 m.
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2. A ball of mass m is thrown with speed v at an angle of 30° with horizontal. Find angular momentum of the ball with respect to the point of projection when the ball is at maximum height. (6 pts)
Given that, the ball of mass m is thrown with speed v at an angle of 30° with the horizontal.
We are to find the angular momentum of the ball with respect to the point of projection when the ball is at maximum height.
So, we have; Initial velocity u = vcosθ ,Maximum height, h = u²sin²θ/2g
Time is taken to reach maximum height, t = usinθ/g = vcosθsinθ/g.
Now, Angular momentum (L) = mvr Where m is the mass of the ball v is the velocity of the ball r is the perpendicular distance between the point about which angular momentum is to be measured, and the direction of motion of the ball. Here, r = hAt maximum height, the velocity of the ball becomes zero.
So, the angular momentum of the ball with respect to the point of projection when the ball is at maximum height is L = mvr = m × 0 × h = 0.
The angular momentum of the ball is 0.
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An object is located a distance d o
=6.8 cm in front of a concave mirror with a radius of curvature r=17.3c Part (a) Write an expression for the image distance
The expression for the image distance di in terms of the object distance do and the radius of curvature r is di = 1 / (2/r - 1/6.8).
The expression for the image distance in terms of the object distance, radius of curvature, and focal length can be determined using the mirror equation for concave mirrors. The mirror equation states that 1/f = 1/do + 1/di, where f is the focal length, do is the object distance, and di is the image distance.
In this case, we are given the object distance do = 6.8 cm and the radius of curvature r = 17.3 cm. The focal length of a concave mirror is half the radius of curvature, so f = r/2.
Substituting the given values into the mirror equation, we have:
1/(r/2) = 1/6.8 + 1/di
Simplifying, we get:
2/r = 1/6.8 + 1/di
To find the expression for the image distance di, we can rearrange the equation:
1/di = 2/r - 1/6.8
Taking the reciprocal of both sides, we have:
di = 1 / (2/r - 1/6.8)
Therefore, the expression for the image distance di in terms of the object distance do and the radius of curvature r is di = 1 / (2/r - 1/6.8).
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: A microwave source and a parabolic reflector produce a parallel beam of 10,000 megahertz radiation 20 cm in diameter. The radiation in the beam is emitted as pulses 10-9 seconds long, with a total energy of 10-ºjoules per pulse. 20 cm L. (a) During the pulse the waves have an electric field E Em sin(wt – kx){ with constant amplitude Em. Find w and k. (b) Write an expression for the B field of the wave (magnitude and direction) in terms of Em, w and k. (c) What is the numerical value of the average energy per unit volume inside a pulse? (d) All of the beam strikes a detector at right angles to the beam, which absorbs 80% of the radiation and reflects 20% of the radiation. What is the force exerted on the detector during a pulse? (e) Suppose that instead of hitting the detector, the pulse is incident on a single-loop, circular antenna with a radius r that is small compared to the wavelength of the radiation. The antenna picks up a signal from time-varying magnetic flux passing through the loop, which generates an emf via Faraday's law. Find the maximum emf that can be generated in the antenna. (f) How should the antenna be oriented to realize the maximum emf obtained in part (e)?
a) w = 2π(10^10 Hz), k = 2π / (0.03 m).
b) The expression for the magnitude and direction of the magnetic field (B) in terms of Em, w, and k is: B = (Em/c) sin(wt - kx).
c) The average energy per unit volume is: (10^-9 Joules) / (π × 0.01 × 10^-9 m^3).
d) The force exerted on the detector is equal to the change in momentum per pulse divided by the pulse duration (10^-9 s) is (2(hc)/λ) / (10^-9 s).
e) ε = -πr^2 (Em/c)w cos(wt - kx).
(a) The given electric field is E = Em sin(wt - kx), where Em is the constant amplitude. To find the values of w and k, we can compare this expression with the general form of a sinusoidal wave:
E = E0 sin(wt - kx + φ),
where E0 is the amplitude and φ is the phase constant.
Comparing the two expressions, we can equate the corresponding terms:
w = 2πf,
k = 2π/λ,
where f is the frequency and λ is the wavelength of the wave.
In this case, the frequency is 10,000 MHz, which can be converted to 10^10 Hz. The wavelength can be calculated using the formula λ = c/f, where c is the speed of light (approximately 3 × 10^8 m/s):
λ = (3 × 10^8 m/s) / (10^10 Hz)
= 3 × 10^-2 m
= 0.03 m.
Therefore, we have:
w = 2π(10^10 Hz),
k = 2π / (0.03 m).
(b) The magnetic field (B) of an electromagnetic wave is related to the electric field (E) by the equation B = E/c, where c is the speed of light.
Therefore, the expression for the magnitude and direction of the magnetic field (B) in terms of Em, w, and k is:
B = (Em/c) sin(wt - kx).
(c) The average energy per unit volume inside a pulse can be calculated by dividing the total energy of the pulse by its volume.
Given:
Total energy per pulse = 10^-9 Joules,
Diameter of the beam = 20 cm = 0.2 m.
The volume of the pulse can be approximated as a cylinder:
Volume = πr^2h,
where r is the radius of the beam (0.1 m) and h is the duration of the pulse (10^-9 s).
Plugging in the values, we have:
Volume = π(0.1 m)^2(10^-9 s)
= π × 0.01 × 10^-9 m^3.
The average energy per unit volume is:
Average energy per unit volume = Total energy per pulse / Volume
= (10^-9 Joules) / (π × 0.01 × 10^-9 m^3).
(d) The force exerted on the detector during a pulse can be calculated using the momentum transfer principle. The momentum transferred per pulse is equal to the change in momentum of the photons, which is given by the equation Δp = 2p, where p is the momentum of a photon.
The momentum of a photon is given by p = h/λ, where h is Planck's constant.
Given:
The beam strikes the detector at right angles to the beam.
The radiation is absorbed 80% and reflected 20%.
The force exerted on the detector is equal to the change in momentum per pulse divided by the pulse duration (10^-9 s):
Force = (2p) / (10^-9 s),
= (2(h/λ)) / (10^-9 s),
= (2(hc)/λ) / (10^-9 s).
(e) To find the maximum emf generated in the antenna, we can use Faraday's law of electromagnetic induction, which states that the emf induced in a loop is equal to the rate of change of magnetic flux passing through the loop. The maximum emf can be obtained when the magnetic flux passing through the loop is changing at its maximum rate.
Given:
The pulse is incident on a single-loop, circular antenna with a radius r (small compared to the wavelength).
The maximum emf (ε) can be calculated using the formula:
ε = -(dΦ/dt),
= -(d/dt)(B⋅A),
= -(d/dt)(BAcosθ),
= -(d/dt)(Bπr^2),
= -πr^2 (dB/dt).
Since the pulse is incident on the antenna, the magnetic field (B) is given by B = (Em/c) sin(wt - kx).
Differentiating with respect to time, we get:
dB/dt = (Em/c)(d/dt)sin(wt - kx),
= (Em/c)w cos(wt - kx).
Substituting this into the expression for the maximum emf, we have:
ε = -πr^2 (Em/c)w cos(wt - kx).
(f) To realize the maximum emf obtained in part (e), the antenna should be oriented such that the angle θ between the magnetic field (B) and the normal to the surface of the loop is 0 degrees (i.e., B and the loop's surface are parallel to each other).
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A 300-gram dart is thrown horizontally at a speed of 10m/s against a
1Kg wooden block hanging from a vertical rope. Determine at what vertical height
raise the block with the dart when the latter is nailed to the wood.
The vertical height up to which the wooden block would be raised when the 300g dart is thrown horizontally at a speed of 10m/s against a 1Kg wooden block hanging from a vertical rope is 3.67 m.
Given:
Mass of dart, m1 = 300 g = 0.3 kg
Speed of dart, v1 = 10 m/s
Mass of wooden block, m2 = 1 kg
Height to which wooden block is raised, h = ?
Since the dart is nailed to the wooden block, it would stick to it and the combination of dart and wooden block would move up to a certain height before stopping. Let this height be h. According to the law of conservation of momentum, the total momentum of the dart and the wooden block should remain conserved.
This is possible only when the final velocity of the dart-wooden block system becomes zero. Let this final velocity be vf.
Conservation of momentum
m1v1 = (m1 + m2)vf0.3 × 10 = (0.3 + 1)× vfvf
= 0.3 × 10/1.3 = 2.31 m/s
As per the law of conservation of energy, the energy possessed by the dart just before hitting the wooden block would be converted into potential energy after the dart gets nailed to the wooden block. Let the height to which the combination of the dart and the wooden block would rise be h.
Conservation of energy
m1v12/2 = (m1 + m2)gh
0.3 × (10)2/2 = (0.3 + 1) × 9.8 × hh = 3.67 m
We can start with the conservation of momentum since the combination of dart and wooden block move to a certain height. Therefore, according to the law of conservation of momentum, the total momentum of the dart and the wooden block should remain conserved.
The height to which the combination of the dart and the wooden block would rise can be determined using the law of conservation of energy.
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Two uncharged conducting spheres are separated by a distance d. When charge - Qis moved from sphere A to sphere, the Coulomb force between them has magnitude For HINT (a) is the Coulomb force attractive or repulsive? attractive repulsive (b) an additional charge ou moved from A to , what is the ratio of the new Coulomb force to the original Cowomb force, Chane (If shere is neutralized so it has no net charge, what is the ratio of the new to the original Coulomb forbe, Need Holo
(a) The Coulomb force between two uncharged conducting spheres is always attractive.
(b) When an additional charge is moved from one sphere to another, the ratio of the new Coulomb force to the original Coulomb force depends on the magnitude of the additional charge and the initial separation between the spheres. If the spheres are neutralized, the new-to-original Coulomb force ratio becomes 0.
(a) The Coulomb force between two uncharged conducting spheres is always attractive. This is because when a charge -Q is moved from one sphere to the other, the negatively charged sphere attracts the positive charge induced on the other sphere due to the redistribution of charges. As a result, the spheres experience an attractive Coulomb force.
(b) When an additional charge q is moved from one sphere to another, the new Coulomb force between the spheres can be calculated using the formula:
F' = k * (Q + q)² / d²,
where F' is the new Coulomb force, k is the Coulomb's constant, Q is the initial charge on the sphere, q is the additional charge moved, and d is the separation between the spheres.
The ratio of the new Coulomb force (F') to the original Coulomb force (F) is given by:
F' / F = (Q + q)² / Q².
If the spheres are neutralized, meaning Q = 0, then the ratio becomes:
F' / F = q² / 0² = 0.
In this case, when the spheres are neutralized, the new-to-original Coulomb force ratio becomes 0.
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A diatomic molecule are modeled as a compound composed by two atoms with masses m₁ and m₂ separated by a distance r. Find the distance from the atom with m₁ to the center of mass of the system.
The distance from the atom with mass m₁ to the center of mass of the diatomic molecule is given by r₁ = (m₂ / (m₁ + m₂)) * r.
To determine the distance from the atom with mass m₁ to the center of mass of the diatomic molecule, we need to consider the relative positions and masses of the atoms. The center of mass of a system is the point at which the total mass of the system can be considered to be concentrated. In this case, the center of mass lies along the line connecting the two atoms.
The formula to calculate the center of mass is given by r_cm = (m₁ * r₁ + m₂ * r₂) / (m₁ + m₂), where r₁ and r₂ are the distances of the atoms from the center of mass, and m₁ and m₂ are their respective masses.
Since we are interested in the distance from the atom with mass m₁ to the center of mass, we can rearrange the formula as follows:
r₁ = (m₂ * r) / (m₁ + m₂)
Here, r represents the distance between the two atoms, and by substituting the appropriate masses, we can calculate the distance r₁.
The distance from the atom with mass m₁ to the center of mass of the diatomic molecule is given by the expression r₁ = (m₂ * r) / (m₁ + m₂). This formula demonstrates that the distance depends on the masses of the atoms (m₁ and m₂) and the total distance between them (r).
By plugging in the specific values for the masses and the separation distance, one can obtain the distance from the atom with mass m₁ to the center of mass for a given diatomic molecule. It is important to note that the distance will vary depending on the specific system being considered.
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Find the approximate electric field magnitude at a distance d from the center of a line of charge with endpoints (-L/2,0) and (L/2,0) if the linear charge density of the line of charge is given by A= A cos(4 mx/L). Assume that d>L.
The approximate electric field magnitude at a distance d from the center of the line of charge is approximately zero due to cancellation from the oscillating linear charge density.
The resulting integral is complex and involves trigonometric functions. However, based on the given information and the requirement for an approximate value, we can simplify the problem by assuming a constant charge density and use Coulomb's law to calculate the electric field.
The given linear charge density A = A cos(4mx/L) implies that the charge density varies sinusoidally along the line of charge. To calculate the electric field, we need to integrate the contributions from each infinitesimally small charge element along the line. However, this integral involves trigonometric functions, which makes it complex to solve analytically.
To simplify the problem and find an approximate value, we can assume a constant charge density along the line of charge. This approximation allows us to use Coulomb's law, which states that the electric field magnitude at a distance r from a charged line with linear charge density λ is given by E = (λ / (2πε₀r)), where ε₀ is the permittivity of free space.
Since d > L, the distance from the center of the line of charge to the observation point d is greater than the length L. Thus, we can consider the line of charge as an infinite line, and the electric field calculation becomes simpler. However, it is important to note that this assumption introduces an approximation, as the actual charge distribution is not constant along the line. The approximate electric field magnitude at a distance d from the center of the line of charge is approximately zero due to cancellation from the oscillating linear charge density. Using Coulomb's law and assuming a constant charge density, we can calculate the approximate electric field magnitude at a distance d from the center of the line of charge.
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(a) A defibrillator connected to a patient passes 15.0 A of
current through the torso for 0.0700 s. How much charge moves? C
(b) How many electrons pass through the wires connected to the
patient? ele
1.05 Coulombs of charge moves through the torso and approximately 6.54 × 10^18 electrons pass through the wires connected to the patient.
(a) To calculate the amount of charge moved,
We can use the equation:
Charge (Q) = Current (I) * Time (t)
Given:
Current (I) = 15.0 A
Time (t) = 0.0700 s
Substituting the values into the equation:
Q = 15.0 A * 0.0700 s
Q = 1.05 C
Therefore, 1.05 Coulombs of charge moves.
(b) To determine the number of electrons that pass through the wires,
We can use the relationship:
1 Coulomb = 6.242 × 10^18 electrons
Given:
Charge (Q) = 1.05 C
Substituting the value into the equation:
Number of electrons = 1.05 C * 6.242 × 10^18 electrons/Coulomb
Number of electrons ≈ 6.54 × 10^18 electrons
Therefore, approximately 6.54 × 10^18 electrons pass through the wires connected to the patient.
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The plane of a 6 cm by 7 cm rectangular loop of wire is parallel
to a 0.17 T magnetic field, and the loop carries a current of 6.2
A.
A) What toque acts on the loop? T=?
B) What is the Magnetic moment
The torque that acts on the loop is 0.000354 N*m. The magnetic moment of the loop is 0.0002604 A*m².
A) The torque acting on the loop can be calculated using the formula:
Torque (T) = Magnetic field (B) * Current (I) * Area (A) * sin(theta)
Magnetic field (B) = 0.17 T
Current (I) = 6.2 A
Area (A) = length (l) * width (w) = 6 cm * 7 cm = 42 cm² = 0.0042 m²
(Note: Convert the area to square meters for consistency in units)
Theta (θ) = angle between the magnetic field and the plane of the loop = 0° (since the plane is parallel to the magnetic field)
Plugging in the values:
T = 0.17 T * 6.2 A * 0.0042 m² * sin(0°)
T = 0.000354 N*m
Therefore, the torque acting on the loop is 0.000354 N*m.
B) The magnetic moment of a loop is given by the formula:
Magnetic moment (μ) = Current (I) * Area (A) * sin(theta)
Using the given values:
μ = 6.2 A * 0.0042 m² * sin(0°)
μ = 0.0002604 A*m²
Therefore, the magnetic moment of the loop is 0.0002604 A*m².
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12) Iwo railway cars, each of mass m, are approaching each other on a straight line with the same constant speed v. Their total kinetic energy Ex and total momentum p are: A) Ek = mv², p = 2mv B) E =
Two railway cars, each of mass m, are approaching each other in a straight line with the same constant speed v.
Their total kinetic energy Ex and total momentum p are [tex]\(E_k = mv^2\), \(p = 2mv\)[/tex].
To determine the correct option, let's analyze the given scenario.
We have two railway cars of mass m approaching each other in a straight line with the same constant speed v.
The kinetic energy (Ek) of an object is given by the formula:
[tex]\[E_k = \frac{1}{2}mv^2\][/tex]
The momentum (p) of an object is given by the formula:
[tex]\[p = mv\][/tex]
Now let's calculate the total kinetic energy [tex](E_{total})[/tex] and total momentum [tex](p_{total})[/tex] for the two railway cars.
Since both cars have the same mass (m) and speed (v), we can calculate the total kinetic energy as:
[tex]\[E_{total} = E_k + E_k \\\\= \frac{1}{2}mv^2 + \frac{1}{2}mv^2 \\\\= mv^2\][/tex]
Similarly, the total momentum is given by:
[tex]\[p_{total} = p + p \\= mv + mv \\= 2mv\][/tex]
Comparing the calculated values with the options given:
A)
[tex]\(E_k = mv^2\), \\\(p = 2mv\)[/tex] (Correct)
B)
[tex]\(E = \frac{1}{2}v^2\),\\ \(p = mv\)[/tex] (Incorrect)
C)
[tex]\(E_k = mv^2\), \\\(p = 0\)[/tex] (Incorrect)
D)
[tex]\(E_x = 0\), \\\(p = 2mv\)[/tex] (Incorrect)
Therefore, the correct option is A) [tex]\(E_k = mv^2\),\\\(p = 2mv\)[/tex].
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A block with a mass of 47.5 kg is pushed with a horizontal force of 150 N. The block moves at a constant speed across a level, rough floor a distance of 5.50 m. (a) What is the work done (in J) by the 150 N force? ] (b) What is the coefficient of kinetic friction between the block and the floor?
(a) The work done by a force is given by the equation:
Work = Force * Distance * cos(theta)
In this case, the force applied is 150 N and the distance moved is 5.50 m. Since the force is applied horizontally, the angle theta between the force and the displacement is 0 degrees (cos(0) = 1).
So the work done by the 150 N force is:
Work = 150 N * 5.50 m * cos(0) = 825 J
Therefore, the work done by the 150 N force is 825 Joules (J).
(b) The work done by the 150 N force is equal to the work done against friction. The work done against friction can be calculated using the equation:
Work = Force of friction * Distance
Since the block moves at a constant speed, the net force acting on it is zero. Therefore, the force of friction must be equal in magnitude and opposite in direction to the applied force of 150 N.
So the force of friction is 150 N.
The coefficient of kinetic friction (μk) can be determined using the equation:
Force of friction = μk * Normal force
The normal force (N) is equal to the weight of the block, which is given by:
Normal force = mass * gravity
where gravity is approximately 9.8 m/s².
Substituting the values:
150 N = μk * (47.5 kg * 9.8 m/s²)
Solving for μk:
μk = 150 N / (47.5 kg * 9.8 m/s²) ≈ 0.322
Therefore, the coefficient of kinetic friction between the block and the floor is approximately 0.322.
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3. AIS MVX, 6.6KV Star connected generator has positive negative and zero sequence reactance of 20%, 20%. and 10. respect vely. The neutral of the generator is grounded through a reactor with 54 reactance based on generator rating. A line to line fault occurs at the terminals of the generator when it is operating at rated voltage. Find the currents in the line and also in the generator reactor 0) when the fault does not involves the ground (1) When the fault is solidly grounded.
When the fault does not involve the ground is 330A,When the fault is solidly grounded 220A.
When a line-to-line fault occurs at the terminals of a star-connected generator, the currents in the line and in the generator reactor will depend on whether the fault involves the ground or not.
When the fault does not involve the ground:
In this case, the fault current will be equal to the generator's rated current. The current in the generator reactor will be equal to the fault current divided by the ratio of the generator's zero-sequence reactance to its positive-sequence reactance.
When the fault is solidly grounded:
In this case, the fault current will be equal to the generator's rated current multiplied by the square of the ratio of the generator's zero-sequence reactance to its positive-sequence reactance.
The current in the generator reactor will be zero.
Here are the specific values for the given example:
Generator's rated voltage: 6.6 kV
Generator's positive-sequence reactance: 20%
Generator's negative-sequence reactance: 20%
Generator's zero-sequence reactance: 10%
Generator's neutral grounded through a reactor with 54 Ω reactance
When the fault does not involve the ground:
Fault current: 6.6 kV / 20% = 330 A
Current in the generator reactor: 330 A / (10% / 20%) = 660 A
When the fault is solidly grounded:
Fault current: 6.6 kV * (20% / 10%)^2 = 220 A
Current in the generator reactor: 0 A
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A student, sitting on a stool rotating at a rate of 34 RPM, holds masses in each hand. When his arms are extended, the total rotational inertia of the system is 8.0 kg.m. He pulls his arms in close to his body, reducing the total rotational inertia to 5.0 kg. m2. If there are no external torques, what is the new rotational velocity of the system?
The new rotational velocity of the system, when the student pulls his arms in, is 5.69 rad/s.
To solve this problem, we can apply the conservation of angular momentum. According to the conservation of angular momentum, the total angular momentum of a system remains constant when no external torques act on it. Mathematically, it can be represented as:
L1 = L2
where
L1 is the initial angular momentum and
L2 is the final angular momentum.
Angular momentum (L) is defined as the product of the moment of inertia (I) and the angular velocity (ω). Therefore, the equation can be written as:
I1 × ω1 = I2 × ω2
where
I1 and I2 are the initial and final moments of inertia, and
ω1 and ω2 are the initial and final angular velocities, respectively.
In this problem, we are given:
Initial rotational inertia (moment of inertia): I1 = 8.0 kg.m²
Final rotational inertia: I2 = 5.0 kg.m²
Initial angular velocity: ω1 = 34 RPM
First, we need to convert the initial angular velocity from RPM (revolutions per minute) to rad/s (radians per second).
Since 1 revolution is equal to 2π radians, we have:
ω1 = (34 RPM) × (2π rad/1 min) × (1 min/60 s)
ω1 = 3.56 rad/s
Now we can rearrange the equation to solve for the final angular velocity (ω2):
I1 × ω1 = I2 × ω2
ω2 = (I1 × ω1) / I2
ω2 = (8.0 kg.m² × 3.56 rad/s) / 5.0 kg.m²
ω2 = 5.69 rad/s
Therefore, the new rotational velocity of the system, when the student pulls his arms in, is 5.69 rad/s.
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2. An electron is xeleased from rest at a distance of 9.00 cm from a proton. If the proton is held in place, how fast will the electron be moving when it is 300 cm from the proton? (me = 9.11 X 103 kg, q= 1.6810-196)
The electron's speed can be determined using conservation of energy principles.
Initially, at a distance of 9.00 cm, the electron possesses zero kinetic energy and potential energy given by -U = kqQ/r.
At a distance of 300 cm, the electron has both kinetic energy (1/2)mv² and potential energy -U = kqQ/r. The total energy of the system, the sum of kinetic and potential energy, remains constant. Thus, applying conservation of energy, we can solve for the electron's speed.
Calculating the values using the given data:
Electron mass (me) = 9.11 x 10³ kg
Electron charge (q) = 1.68 x 10⁻¹⁹ C
Coulomb constant (k) = 9 x 10⁹ Nm²/C²
Proton charge (Q) = q = 1.68 x 10⁻¹⁹ C
Initial distance (r) = 9.00 cm = 0.0900 m
Final distance (r') = 300 cm = 3.00 m
Potential energy (U) = kqQ/r = 2.44 x 10⁻¹⁶ J
Using the equation (1/2)mv² - kqQ/r = -U, we find that v = √(3.08 x 10¹¹ m²/s²) = 5.55 x 10⁵ m/s.
Hence, the electron's speed at any point in its trajectory is 5.55 x 10⁵ m/s.
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A crow wants to fly to a nest 130 km due north of her position, with a wind coming from the east (going west) with a speed of 30 km/hr. If it flies at an airspeed of 260 km/hr, how long will it take it to fly to its nest (in minutes)?
The crow will take approximately 30 minutes to fly to its nest.
When calculating the time it takes for the crow to reach its nest, we need to consider the effect of the wind on its flight. The crow wants to fly due north, but there is a wind coming from the east with a speed of 30 km/hr. This means that the wind will push the crow slightly westward as it flies north.
To determine the actual speed of the crow relative to the ground, we need to subtract the effect of the wind. The crow's airspeed is 260 km/hr, but the wind is blowing in the opposite direction at 30 km/hr. So the crow's ground speed will be 260 km/hr - 30 km/hr = 230 km/hr.
To find the time it takes for the crow to cover a distance of 130 km at a speed of 230 km/hr, we divide the distance by the speed: 130 km / 230 km/hr = 0.565 hours.
To convert this time to minutes, we multiply by 60: 0.565 hours * 60 minutes/hour = 33.9 minutes.
Therefore, it will take the crow approximately 30 minutes to fly to its nest.
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A pulsar la rotating neutron star) has a mass of 1.43 solar masses and rotates with a period of 2.7575 1 solar mass is the mass of our Sun or 1.988 x 100 kg (A) What is the angular speed of the pulsar? rad/s (B) We will model the neutron star as a uniform sphere with an effective radius of 11000 m (11 km). With this model what would its rotational Inertia be? 'pulsar What is the rotational (kinetic) energy of the pulsar? KErot (D) The pulsar loses energy and slows down very slowly. Every second the pulsar's frequency changes by only A/ - 2.6970 x 10-15 Hz or A 1.6946 x 10-12 rad/s. This slowing of the rotation is due mostly to energy lost by electromagnetic radiation from the rotating magnetic moment of the pulsar, How much rotational Idnetic energy is lost in one second? This is such a small relative change that we would have problems calculating the change in kinetic energy using AKE-RE, KE (naccurate due to numerical computation errors) This curacy because we are directing the numbers that many candy for example two values apree to 14 mificant dit, you would need to calculate their values to 17 s/icontatto esteticane digits eft in their difference However, it can be shown that the change in rotational kinetic energy can be calculated without hupe round-off errors by using AKE- This approximate formula is valid when der is very small compared to , Chery lost in 1 second CAKE) For a young pular this energy fuels the glowing gates in the nebula until they have moved far from the pulsar. Due Sur NAM
The angular speed is 2.277 rad/s, the rotational inertia is [tex]1.37\times10^{38} kgm^2[/tex], the rotational energy is [tex]3.55\times10^{38} J[/tex] and the change in rotational energy is [tex]-5.286\times10^{26}J[/tex].
(a) To find the angular speed of the pulsar, we use the formula:
[tex]angular speed =\frac {2\pi}{period}[/tex].
Substituting the given period of 2.7575 seconds,
[tex]angular speed=\frac{2\pi}{2.7575}=2.277 rad/s.[/tex]
Therefore, the angular speed is approximately 2.277 rad/s.
(b) The rotational inertia of a uniform sphere is given by the formula:
Rotational Inertia =[tex](\frac{2}{5}) mass\times radius^2[/tex].
Substituting the mass of the pulsar (1.43 solar masses or 2.846 × 10^30 kg) and the effective radius (11 km or 11,000 m),we get
Rotational Inertia =[tex](\frac{2}{5} )\times 2.846\times10^{30}\times (11,000)^2=1.37\times10^{38}.[/tex]
Therefore, the rotational inertia to be approximately [tex]1.37\times 10^{38} kgm^2[/tex].
(c) The rotational (kinetic) energy of the pulsar is given by the formula:
Rotational Energy = [tex](\frac{1}{2}) rotational inertia \times angular speed^2[/tex].
Substituting the calculated values for rotational inertia and angular speed,
Rotational Energy = [tex](\frac{1}{2})\times 1.37\times10^{38} \times (2.277)^2=3.55\times 10^{38} J[/tex]
Therefore, the rotational energy is approximately [tex]3.55 \times 10^{38} J[/tex].
(d) The change in rotational kinetic energy can be calculated using the formula:
Change in rotational energy = -angular speed x change in angular speed x rotational inertia.
Substituting the given change in angular speed (-1.6946 × 10^(-12) rad/s) and the calculated rotational inertia, we find the change in rotational energy
Change in rotational energy = [tex]2.277\times(-1.6946\times10^{-12})\times (1.37\times10^{38})=-5.286\times10^{26}J[/tex]
Therefore, the change in rotational energy is approximately [tex]-5.286 \times 10^{26} J[/tex].
In conclusion, the angular speed is 2.277 rad/s, the rotational inertia is [tex]1.37\times10^{38} kgm^2[/tex], the rotational energy is [tex]3.55\times10^{38} J[/tex] and the change in rotational energy is [tex]-5.286\times10^{26}J[/tex].
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A swimming pool measures a length of 6.0 m, width 4.3 m , and depth 3.3 m. Compute the force exerted by the water against the bottom. Do not include the force due to air pressure. Express your answe
The force due to air pressure, is approximately 836,532 Newtons.
To compute the force exerted by the water against the bottom of the swimming pool, we need to consider the concept of pressure and the area of the pool's bottom.
The pressure exerted by a fluid at a certain depth is given by the formula P = ρgh, where P is the pressure, ρ is the density of the fluid, g is the acceleration due to gravity, and h is the depth.
In this case, the fluid is water, which has a density of approximately 1000 kg/m³, and the acceleration due to gravity is 9.8 m/s².
The depth of the pool is given as 3.3 m. Substituting these values into the formula, we can calculate the pressure at the bottom of the pool:
P = (1000 kg/m³)(9.8 m/s²)(3.3 m) = 32,340 Pa
To determine the force exerted by the water against the bottom, we need to multiply this pressure by the area of the pool's bottom. The area is calculated by multiplying the length and width of the pool:
Area = 6.0 m × 4.3 m = 25.8 m²
Now, we can calculate the force using the formula Force = Pressure × Area:
Force = (32,340 Pa)(25.8 m²) = 836,532 N
Therefore, the force exerted by the water against the bottom of the swimming pool, without considering the force due to air pressure, is approximately 836,532 Newtons.
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Create your own kinematics word problem involving uniform
acceleration. Solve your word problem.
A car accelerates uniformly from rest at a rate of 2 m/s² for a distance of 100 meters. How long does it take for the car to reach this distance?
Using the kinematic equation s = ut + (1/2)at², where s is the distance, u is the initial velocity (0 m/s since the car starts from rest), a is the acceleration (2 m/s²), and t is the time, we can solve for t.
Given that the car starts from rest (u = 0 m/s) and accelerates uniformly at a rate of 2 m/s², we can use the kinematic equation s = ut + (1/2)at² to solve for the time taken (t) to cover a distance of 100 meters (s = 100 m).
Substituting the given values into the equation, we have 100 = 0 + (1/2)(2)t². Simplifying the equation, we get 100 = t². Taking the square root of both sides, we find t = ±10.
Since time cannot be negative in this context, the car takes 10 seconds to reach a distance of 100 meters when accelerating uniformly at a rate of 2 m/s².
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