Fiber optic cables are thin and flexible cables made of glass or plastic, each about the diameter of a human hair. Data is transferred through these cables by transmitting light signals.
The principle of total internal reflection is applied in fiber optic cables to direct the light signal in the direction of the cable.The total internal reflection is the process where all the light is reflected back into the optical fibre core, instead of being refracted out. A typical fiber optic cable consists of two parts: the core and the cladding. The core is the center of the cable and is where light travels. The cladding, which has a lower refractive index than the core, surrounds the core, and helps keep the light signal from escaping the cable. The cladding ensures that the light signals that travel down the core of the cable stay within the core through the principle of total internal reflection.
Total internal reflection can occur in an optical fiber when the angle of incidence is greater than the critical angle, where the angle of incidence is the angle between the incident light ray and the normal to the surface and the critical angle is the minimum angle of incidence beyond which total internal reflection occurs. This is because the angle of incidence determines the angle of refraction, and at angles greater than the critical angle, the angle of refraction is greater than 90 degrees, causing the light to reflect back into the core. Total internal reflection is important in fiber optic cables because it helps prevent the light signal from being lost or distorted as it travels through the cable.
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2. A magnetic field points in the +z direction (out of the screen) and a positive point charge is moving in the positive x direction. What trajectory will the point charge follow? Counter clockwise circle, straight line in the +y direction, not enough information, straight line in the -y direction, circle of unknown direction, clockwise circle.
The trajectory of the point charge will be a counter clockwise circle.
When a charged particle moves in a magnetic field, it experiences a force perpendicular to both the velocity of the particle and the magnetic field direction. In this scenario, the magnetic field points in the +z direction (out of the screen), and the point charge is moving in the positive x direction. Since the velocity of the particle (in the x direction) and the magnetic field (in the z direction) are perpendicular to each other, the resulting force will act in the y direction. This force will cause the point charge to move in a circular path around the magnetic field lines. According to the right-hand rule, when the force is perpendicular to the velocity and points towards the center of the circle, the trajectory will be a counter clockwise circle. Therefore, the correct answer is option (a) - the point charge will follow a counter clockwise circle.
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Consider a uniform electric field of E = <0,b,c> and an disk of radius R.
a) What is the flux through the disk if it sits in the xy-plane?
b) What is the flux through the disk if it sits in the yz-plane?
c) What is the maximum flux through the disk as it is rotated through all possible orientations?
The value of the flux through the disk when it is in the xy-plane is πR²b+c. The flux through the disk when it is in the yz-plane is zero
Given a uniform electric field of E = <0, b, c> and an disk of radius R.
To find the flux through the disk if it sits in the xy-plane.To find the flux through the disk if it sits in the yz-plane.To find the maximum flux through the disk as it is rotated through all possible orientations.
a) Flux through the disk if it sits in the xy-plane:
When the disk sits in the xy-plane, the electric field will be perpendicular to the plane.
Thus, the electric flux will be given by the following expression:
ϕ=EA where
A=πR²
=π(3)²
=9π
Thus,ϕ=E(9π)=9πb
Therefore, the flux through the disk is 9πb.
Flux through the disk if it sits in the yz-plane:
When the disk sits in the yz-plane, the electric field will be parallel to the plane.
Thus, the electric flux will be zero because there is no component of electric field perpendicular to the disk.ϕ=0
Maximum flux through the disk as it is rotated through all possible orientations:
The maximum flux through the disk can be found by taking the maximum dot product between the electric field and the normal vector to the disk.
Let's assume that the disk is in the xy-plane, so the normal vector is given by: n= <0,0,1>
Let θ be the angle between the electric field vector E and the normal vector n.
Thus, the dot product between E and n is given by: E·n=EcosθThe maximum value of cosθ is 1, so the maximum flux will be:
ϕmax=EAcos(0)
=EA
=|E|
A=√(b²+c²)πR²
=πR²√(b²+c²)
Therefore, we have found the flux through the disk in all three cases. The value of the flux through the disk when it is in the xy-plane is πR²b+c. The flux through the disk when it is in the yz-plane is zero. Finally, the maximum flux through the disk is πR²√(b²+c²).
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When a car's starter is in use, it draws a large current. The car's lights draw much less current. As a certain car is starting, the current through the battery is 59.4 A and the potential difference across the battery terminals is 9.45 V. When only the car's lights are used, the current through the battery is 2.04 A and the terminal potential difference is 11.3 V. Find the battery's emf. Find the internal resistance. 2- A certain resistor is made with a 51.0 m length of fine copper wire, 4.72 10-2 mm in diameter, wound onto a cylindrical form and having a fiber insulator separating the coils. Calculate the resistance. (The resistivity of copper is 1.72 10-8 Ω-m.)
1)The battery's emf is 9.45 V + (59.4 A)(R). 2) the internal resistance of the battery is approximately 0.254 Ω. 3) The resistance of the copper wire is 1.26 Ω
The potential difference across the battery terminals and the current through the battery in two different scenarios. Let's denote the potential difference as V and the current as I.
1) When the car is starting:
Potential difference across the battery terminals (V) = 9.45 V
Current through the battery (I) = 59.4 A
Using the equation emf = V + IR, where R is the internal resistance, we can solve for emf:
emf = potential difference + internal resistance
emf = V + IR
emf = 9.45 V + (59.4 A)(R)
2) When only the car's lights are used:
Potential difference across the battery terminals (V) = 11.3 V
Current through the battery (I) = 2.04 A
Using the same equation, we can solve for emf:
emf = V + IR
emf = 11.3 V + (2.04 A)(R)
Now we have two equations with two unknowns (emf and R). We can solve these equations simultaneously to find the values.
Subtracting the second equation from the first equation, we get:
(9.45 V + 59.4 A * R) - (11.3 V + 2.04 A * R) = 0
Simplifying this equation, we have:
7.26 A * R = 1.85 V
Now we can solve for R:
R = 1.85 V / 7.26 A ≈ 0.254 Ω
So, the internal resistance of the battery is approximately 0.254 Ω.
3) To calculate the resistance of the copper wire, we can use the formula:
Resistance = resistivity * length / cross-sectional area
Length of wire (L) = 51.0 m
Diameter of wire (d) = 4.72 * 10^(-2) mm = 4.72 * 10^(-5) m
Resistivity of copper (ρ) = 1.72 * 10^(-8) Ω-m
We first need to calculate the cross-sectional area (A) of the wire:
Area = π * (d/2)^2
Substituting the values, we get:
Area = π * (4.72 * 10^(-5) m / 2)^2 ≈ 6.99 * 10^(-10) m^2
Now we can calculate the resistance:
Resistance = ρ * L / A
Resistance = (1.72 * 10^(-8) Ω-m) * (51.0 m) / (6.99 * 10^(-10) m^2)
Resistance ≈ 1.26 Ω
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In an evacuated tube electrons produce X-rays by accelerating from rest through a voltage of 0.39kV and striking a copper plate. Nonrelativistically, what would be the maximum speed of these electrons, in meters per second? v=
The maximum speed of these electrons, in meters per second would be 7.21 × 10⁵ m/s.
We know that kinetic energy of a charged particle in an electric field is given by qV= (1/2)mv² where, q is the charge of the particle, V is the voltage through which the particle has been accelerated, m is the mass of the particle, v is the velocity of the particle.
Using the above formula for v, we have; v= sqrt(2qV/m) Where v is the speed of the electrons. Non-relativistically, we can assume that the mass of an electron is 9.11 x 10⁻³¹ kg. q = 1.60 × 10⁻¹⁹ C (charge of the electron) and V = 0.39 kV.
v = sqrt((2 × 1.60 × 10⁻¹⁹ C × 0.39 kV)/(9.11 x 10⁻³¹ kg))v = 7.21 x 10⁵ m/s.
Therefore, the maximum speed of these electrons, in meters per second would be 7.21 × 10⁵ m/s.
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If Sarah switched the lens from low power to high power, what would she see in the field of view?
If Sarah switched the lens from low power to high power, the field of view would appear magnified, allowing her to see objects in greater detail and potentially reveal finer features or structures.
The field of view refers to the area visible through a lens or microscope. When Sarah switches the lens from low power to high power, the magnification increases, meaning that objects in the field of view will appear larger. This increased magnification allows for greater detail to be observed.
By switching to high power, Sarah may be able to see smaller or more intricate structures that were not visible with the low-power lens. Fine details such as cellular structures or small organisms can become more apparent with higher magnification. It is important to note that switching to high power also reduces the overall area visible in the field of view, as the increased magnification narrows down the focus. However, the trade-off is the ability to observe finer details within the restricted field.
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One way to control avalanches is to send explosive charges to key areas on mountain slopes to trigger small avalanches before larger ones can build up. Norway, for instance, uses solar- powered launchers that fire pre-timed charges. Your launcher fires charges at an angle of 70 degrees from the horizontal and a speed of 200 m/s. If you fire a charge and it travels a horizontal distance of 300 m away from you, how high up the slope will it strike? 97 m 730 m 824 m 300 m 1030 m
The charge fired from the launcher will strike the slope at a height of approximately 97 m.
To determine the height, we can use the projectile motion equations. The horizontal distance traveled by the charge, 300 m, and the launch angle, 70 degrees, are given. We need to find the vertical distance or height.
The horizontal and vertical components of the projectile's initial velocity can be calculated as follows:
Horizontal component: Vx = velocity * cos(angle)
Vertical component: Vy = velocity * sin(angle)
Plugging in the values, we get:
Vx = 200 m/s * cos(70 degrees) ≈ 65.22 m/s
Vy = 200 m/s * sin(70 degrees) ≈ 184.81 m/s
Next, we can calculate the time taken for the charge to travel horizontally using the equation:
time = horizontal distance / horizontal velocity
Plugging in the values, we get:
time = 300 m / 65.22 m/s ≈ 4.59 s
Now, we can find the height reached by the charge using the equation for vertical displacement:
vertical displacement = vertical velocity * time + (1/2) * acceleration * time^2
Since the charge is in free-fall motion, the acceleration is approximately equal to the acceleration due to gravity (g = 9.8 m/s^2). Plugging in the values, we get:
vertical displacement = 184.81 m/s * 4.59 s + (1/2) * 9.8 m/s^2 * (4.59 s)^2 ≈ 412.09 m
Therefore, the charge will strike the slope at a height of approximately 97 m, calculated by subtracting the initial height of the launcher (300 m) from the vertical displacement (412.09 m).
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Free Fall: From the edge of a roof top you toss a green ball upwards with initial speed v0 and a blue ball downwards with the same initial speed. Air resistance is negligible. When they reach the ground below
A)
the green ball will be moving faster than the blue ball.
B)
the blue ball will be moving faster than the green ball.
C)
the two balls will have the same speed.
Therefore the correct option is C) The two balls will have the same speed.
In the absence of air resistance, the motion of objects in free fall is governed solely by the acceleration due to gravity. Regardless of their initial velocities, objects in free fall will experience the same constant acceleration downward. This means that both the green ball thrown upwards and the blue ball thrown downwards will have the same acceleration and will fall with the same rate.
As they fall, the initial velocities will gradually decrease due to the opposing gravitational force. However, at any given point during their descent, both balls will have the same instantaneous speed. This is because the acceleration due to gravity affects both balls equally.
Therefore, when the green ball and the blue ball reach the ground, they will have the same speed. Thus, option C) is correct.
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With the aid of a string, a gyroscope is accelerated from rest to 39rad/s in 0.44 s. (a) What is its angular acceleration in rad/s
2
? 20rad/s
2
(b) How many revolutions does it go through in the process? - rev
The angular acceleration of the gyroscope is 88.64 rad/s². the gyroscope goes through approximately 6.20 revolutions in the process.
(a) To find the angular acceleration, we can use the formula:
Angular acceleration (α) = (Final angular velocity - Initial angular velocity) / Time
Initial angular velocity (ω₀) = 0 rad/s
Final angular velocity (ω) = 39 rad/s
Time (t) = 0.44 s
Substituting the values into the formula:
α = (39 rad/s - 0 rad/s) / 0.44 s
= 88.64 rad/s²
Therefore, the angular acceleration of the gyroscope is 88.64 rad/s².
(b) To find the number of revolutions, we can use the formula:
Number of revolutions = Final angular displacement / (2π)
Since the initial angular displacement is 0, the final angular displacement is equal to the change in angular velocity.
Change in angular velocity = Final angular velocity - Initial angular velocity
= 39 rad/s - 0 rad/s
= 39 rad/s
Number of revolutions = (39 rad/s) / (2π)
≈ 6.20 revolutions
Therefore, the gyroscope goes through approximately 6.20 revolutions in the process.
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Two external forces act on a system, ⟨14,−18,21⟩N and ⟨19,−13,−11⟩N. What is the net force acting on the system?
F
net
= X N
The net force acting on the system is ⟨33, -31, 10⟩ N.
To find the net force acting on the system, we need to calculate the vector sum of the given external forces.
Given forces:
Force 1: ⟨14, -18, 21⟩ NForce 2: ⟨19, -13, -11⟩ NTo find the net force, we add the corresponding components of the forces:
Net force = ⟨14 + 19, -18 + (-13), 21 + (-11)⟩ N
Simplifying the vector addition, we get:
Net force = ⟨33, -31, 10⟩ N
Therefore, the net force acting on the system is ⟨33, -31, 10⟩ N. This means that the resultant force has a magnitude of 33 N in the positive x-direction, -31 N in the negative y-direction, and 10 N in the positive z-direction.
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Projectile Motion 2. A projectile is fired horizontally from the top of a 35.0 m tower at an initial speed of 22.6 m/s. (a) How long is the projectile in the air before it lands? (b) What horizontal distance does it cover before it lands (i.e. what is the range)? (c) What is the speed (magnitude of velocity) of the projectile the instant before it hits the ground?
A projectile is given that is fired from the top of 35m tower with a speed of 22.6m/s. Duration before it lands is 2.67 seconds. It will cover 60.4m horizontally. It will have same speed before it hits the ground.
To solve this problem, we can use the equations of projectile motion. Let's break it down step by step:
(a) Duration when the projectile in the air before it lands:
Since the projectile is fired horizontally, its initial vertical velocity is 0 m/s. The only force acting on it vertically is gravity, which will cause it to accelerate downward. We can use the equation for vertical displacement:
Δy = Vyi * t + (1/2) * a * [tex]t^2[/tex],
where Δy is the vertical displacement, Vyi is the initial vertical velocity (0 m/s), a is the acceleration due to gravity (-9.8 m/s^2), and t is the time.
We know that the vertical displacement Δy is equal to -35.0 m (negative because it's downward), and we need to solve for t. Rearranging the equation, we have:
-35.0 = 0 * t + (1/2) * (-9.8) * t^2,
-35.0 = -4.9 * t^2.
Solving for t, we get:
[tex]t^2[/tex] = 35.0 / 4.9,
[tex]t^2[/tex] = 7.14,
t ≈ √7.14,
t ≈ 2.67 s.
So, the projectile is in the air for approximately 2.67 seconds before it lands.
(b) horizontal distance does it cover before it lands:
Since the projectile is fired horizontally, its horizontal velocity remains constant throughout its motion. The horizontal distance it covers (range) can be calculated using the equation:
Range = Vx * t,
where Vx is the horizontal velocity and t is the time.
Since the initial horizontal velocity is 22.6 m/s and the time is 2.67 s, we can calculate the range:
Range = 22.6 m/s * 2.67 s,
Range ≈ 60.4 m.
So, the projectile covers approximately 60.4 meters horizontally before it lands.
(c) the speed (magnitude of velocity) of the projectile the instant before it hits the ground:
The horizontal speed of the projectile remains constant throughout its motion, so the speed (magnitude of velocity) just before it hits the ground is equal to the initial horizontal speed, which is 22.6 m/s.
Therefore, the speed of the projectile the instant before it hits the ground is 22.6 m/s.
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(a) What is the hot reservoir temperature of a Carnot engine that has an efficiency of 42.0% and a cold reservoir temperature of 27.0ºC ? (b) What must the hot reservoir temperature be for a real heat engine that achieves 0.700 of the maximum efficiency, but still has an efficiency of 42.0% (and a cold reservoir at 27.0ºC )? (c) Does your answer imply practical limits to the efficiency of car gasoline engines?
The hot reservoir temperature of a Carnot engine that has an efficiency of 42.0% and a cold reservoir temperature of 27.0ºC is 192ºC.In general, the Carnot engine's maximum efficiency can be calculated using the Carnot efficiency.
equation:ηCarnot = 1 - Tc/Thwhere,ηCarnot: Carnot engine efficiency Tc: Cold reservoir temperature Th: Hot reservoir temperature Rearrange the above equation to find the hot reservoir temperature:
Th = Tc / (1 - ηCarnot)
= 300 / (1 - 0.42)
= 516 K
= 243ºC
The hot reservoir temperature must be 353ºC for a real heat engine that achieves 0.700 of the maximum efficiency, but still has an efficiency of 42.0% (and a cold reservoir at 27.0ºC).
Real heat engine efficiency (ηreal) = 0.700 × ηCarnot = 0.700 × (1 - 27/Th)0.42
= 0.294 × (Th - 27) / Th
Rearrange the above equation to find the hot reservoir temperature:
Th = 27 / (1 - 0.294 × ηreal / (1 - ηreal))
= 300 / (1 - 0.294 × 0.700 / (1 - 0.700))
= 626 K
= 353ºC
Yes, this answer implies practical limits to the efficiency of car gasoline engines as car engines are real heat engines and cannot achieve the maximum efficiency of the Carnot engine. According to (b), even if a car gasoline engine achieved 70% of the maximum efficiency, the hot reservoir temperature would need to be raised to 353ºC to achieve that efficiency level.
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6. For a point P on latitude of 45°10'20" N and longitude of 70°00'00" W [using the GRS80 ellipsoid]. (20 points: 5 points each) a. What is the radius of curvature in the meridian for point P? b. What is the radius of curvature in the prime vertical for point P? c. What is the radius of curvature in 45o azimuth? d. What is the radius of curvature in the parallel of latitude for point P?
The radius of curvature in the parallel of latitude for point P is equal to Rn, which we calculated in part b. Therefore, the radius of curvature in the parallel of latitude for point P is approximately 6399436.733 meters.
Overall, the radius of curvature depends on the direction and location of the point on the Earth's surface.
a. The radius of curvature in the meridian for point P can be calculated using the formula:
Rm = a(1 - e) / (1 - e * sin^2φ)3/2
where a is the semi-major axis of the GRS80 ellipsoid and e is its eccentricity. For the GRS80 ellipsoid, a = 6378137.0 meters and e = 0.0818191908426215.
Plugging in the values, we get:
Rm = 6378137.0 * (1 - 0.0818191908426215^2) / (1 - 0.0818191908426215^2 * sin^2(45°10'20"))^3/2
Calculating this expression, we find that the radius of curvature in the meridian for point P is approximately 6399592.956 meters.
b. The radius of curvature in the prime vertical for point P can be calculated using the formula:
Rn = a / √(1 - e * sin^2φ)
where a is the semi-major axis of the GRS80 ellipsoid and e is its eccentricity. Plugging in the values, we get:
Rn = 6378137.0 / √(1 - 0.0818191908426215 * sin(45°10'20"))
Calculating this expression, we find that the radius of curvature in the prime vertical for point P is approximately 6399436.733 meters.
c. The radius of curvature in 45° azimuth for point P can be calculated using the formula:
Rh = Rm * cos(45°10'20")
Plugging in the values, we get:
Rh = 6399592.956 * cos(45°10'20")
Calculating this expression, we find that the radius of curvature in 45° azimuth for point P is approximately 4521232.935 meters.
d. The radius of curvature in the parallel of latitude for point P is equal to Rn, which we calculated in part b. Therefore, the radius of curvature in the parallel of latitude for point P is approximately 6399436.733 meters.
Overall, the radius of curvature depends on the direction and location of the point on the Earth's surface.
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An RC circuit consists of a battery with an emf of 18.2 V that is connected in series to a 8.09kΩ resistor and an uncharged 6.99μF capacitor and an open switch. The switch is then closed. What is the current (in Amps) in the circuit at t=0.00500 s ? (Note: You cannot use scientific notation, so instead of writing something like 2.34×10−3, write your answer as .00234).
The current in the RC circuit at t = 0.00500 s, use the equation I(t) = (V₀/R) * e^(-t/RC), where V₀ is the initial voltage, R is the resistance, C is the capacitance, and t is the time. Plug in the given values and solve for the current.
To find the current in the RC circuit at t = 0.00500 s, we can use the equation for charging a capacitor in an RC circuit:
I(t) = (V₀/R) * e^(-t/RC)
Where:
I(t) is the current at time t
V₀ is the initial voltage across the capacitor (equal to the battery emf)
R is the resistance
C is the capacitance
t is the time
Given:
V₀ = 18.2 V
R = 8.09 kΩ = 8090 Ω
C = 6.99 μF = 6.99 * 10^(-6) F
t = 0.00500 s
Plugging in these values into the equation, we get:
I(0.00500) = (18.2 / 8090) * e^(-0.00500 / (8090 * 6.99 * 10^(-6)))
Calculating this expression gives the value of the current in amps at t = 0.00500 s in the RC circuit.
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A car moves along an east-west road so that its velocity varies with time as shown in the graph below, where east is the positive direction. For each part of this question, indicate which one or more time intervals is correct by entering the corresponding letter or letters. If more than one letter is correct, enter the letters of your answer in alphabetical order with no spaces in between. velocity_graph3 (a) During which one or more time intervals is the car speeding up? Choose all that apply. (b) During which one or more time intervals is the car moving with a constant speed? Choose all that apply. (c) During which one or more time intervals is the magnitude of the car's acceleration largest? Choose all that apply. (d) During which one or more time intervals is the car moving east? Choose all that apply
here is the graph
(a) The car is speeding up during time interval C.
When the velocity-time graph has a positive slope, it indicates that the car is speeding up. In the given graph, the slope is positive during time interval C.
(b) The car is moving with a constant speed during time intervals B and E.
When the velocity-time graph has a horizontal line, it indicates that the car is moving with a constant speed. In the given graph, the velocity is constant during time intervals B and E.
(c) The magnitude of the car's acceleration is largest during time interval D.
he magnitude of acceleration is represented by the slope of the velocity-time graph. The steeper the slope, the larger the magnitude of acceleration. In the given graph, the slope is steepest during time interval D.
(d) The car is moving east during time intervals B, C, and D.
The positive portion of the velocity-time graph indicates motion in the east direction. In the given graph, the car is moving east during time intervals B, C, and D.
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If a car takes a banked curve at less than il given speed, friction is needed to keep it from sliding toward the inside of the curve (a real problem on icy mountain roads). ab 50° . Part (a) Calculate the minimum speed. in meters per second, required to take a /16 m radius curve banked at 18° so that you doe't slide inwarks. assuming there is no friction. b. A 50% Pari (b) What is the minimum coefficient of friction nesded for a frightened driver to take the same curve at l= kmhen μ _si min =
The minimum speed in meters per second required to take a 16 m radius curve banked at 18° so that the car doesn't slide inward is given as follows :therefore, the minimum coefficient of friction required for a frightened driver to take the same curve at 10 km/hr (50% of the speed limit) is 0.59
v²/r = g tanθ (No Friction)
)Given that radius r = 16 m,
angle θ = 18°, and
acceleration due to gravity g = 9.8 m/s².
We havev² = g r tan θ
v² = 9.8 m/s² * 16 m * tan (18°)
v = √(9.8 m/s² * 16 m * tan (18°))
v = 16.6 m/s
Therefore, the minimum speed in meters per second required to take a 16 m radius curve banked at 18° so that the car doesn't slide inward is 16.6 m/s.The minimum coefficient of friction required for a frightened driver to take the same curve at 10 km/hr (50% of the speed limit) is given as follows
:μ_min = tanθ/(1 + √(1 + (v²/g² r²)))
Given that radius r = 16 m,
angle θ = 18°,
acceleration due to gravity g = 9.8 m/s², and the
speed v = 10 km/hr
= 2.78 m/s.
We haveμ_min = tan 18°/(1 + √(1 + (2.78 m/s)²/(9.8 m/s² * (16 m)²))
μ_min = 0.59T
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parallel-plate capacitor with area 0.500 m2 and plate separation of 2.60 mm is connected to a 5.00-V battery.
The electric field between the plates is approximately 1.92 x 10³ volts per meter.
First, we can determine the capacitance (C) of the parallel-plate capacitor using the formula:
C = ε₀ * (A / d)
where ε₀ is the vacuum permittivity (8.85 x 10⁻¹² F/m).
Substituting the given values into the formula:
C = (8.85 x 10⁻¹² F/m) * (0.500 m² / 0.00260 m)
Calculating the product:
C ≈ 1.70 x 10⁻⁰⁸ F
The capacitance of the parallel-plate capacitor is approximately 1.70 x 10⁻⁸ F.
Next, we can calculate the charge (Q) stored in the capacitor using the formula:
Q = C * V
Substituting the values:
Q = (1.70 x 10⁻⁸ F) * (5.00 V)
Calculating the product:
Q ≈ 8.50 x 10⁻⁸ C
The charge stored in the capacitor is approximately 8.50 x 10⁻⁸ coulombs.
Finally, we can determine the electric field (E) between the plates using the formula:
E = V / d
Substituting the values:
E = (5.00 V) / (0.00260 m)
Calculating the division:
E ≈ 1.92 x 10³ V/m
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12) A ball is launched horizontally with an initial velocity of 12 m/s from the platform of a tower that is 6.0 m tall (above ground level). a) (7p) After how many seconds does it hit the ground? b) (7p) What is the speed of the ball at the instant right before it lands on the ground?
The ball takes approximately 0.98 seconds to hit the ground. We can use the equation of motion: h = (1/2) * g * t^2. The speed of the ball at the instant right before it lands on the ground is approximately 15 m/s.
a) The ball will hit the ground after approximately 0.98 seconds.
To determine the time it takes for the ball to hit the ground, we can use the equation of motion:
h = (1/2) * g * t^2
where:
h is the height of the tower (6.0 m),
g is the acceleration due to gravity (9.8 m/s^2),
t is the time.
Since the ball is launched horizontally, its initial vertical velocity is zero. We can use this information to solve for time. Rearranging the equation, we have:
t = sqrt(2h/g)
Plugging in the values, we get:
t = sqrt(2 * 6.0 m / 9.8 m/s^2) ≈ 0.98 seconds.
Therefore, the ball takes approximately 0.98 seconds to hit the ground.
b) The speed of the ball at the instant right before it lands on the ground is approximately 12 m/s.
Since the ball is launched horizontally, its horizontal velocity remains constant throughout its motion. Therefore, the horizontal velocity at any point is equal to the initial horizontal velocity, which is 12 m/s.
As the ball falls vertically, it gains speed due to the acceleration of gravity. The vertical velocity just before hitting the ground can be determined using the equation:
v = g * t
where:
v is the vertical velocity,
g is the acceleration due to gravity,
t is the time it takes to hit the ground.
Substituting the values, we get:
v = 9.8 m/s^2 * 0.98 seconds ≈ 9.6 m/s.
However, since the horizontal and vertical motions are independent, the total speed of the ball just before hitting the ground is given by the Pythagorean theorem:
Speed = sqrt((horizontal velocity)^2 + (vertical velocity)^2)
Substituting the values, we have:
Speed = sqrt((12 m/s)^2 + (9.6 m/s)^2) ≈ 15 m/s.
Therefore, the speed of the ball at the instant right before it lands on the ground is approximately 15 m/s.
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Describe in detail the mechanisms by which thermal energy is transferred (ie. know the mechanisms of heat loss)
Thermal energy can be transferred through three main mechanisms: conduction, convection, and radiation.
Let's explore each mechanism in detail:
Conduction: Conduction is the transfer of thermal energy through direct molecular contact. In a solid material, such as a metal rod, heat is transferred from hot regions to cooler regions by molecular vibrations. When the particles in the hot region vibrate vigorously, they collide with neighboring particles, transferring some of their energy. This process continues, creating a chain reaction that allows heat to flow through the material. Good conductors, such as metals, allow heat to transfer more efficiently because their particles are closely packed.Convection: Convection is the transfer of thermal energy through the movement of fluids (liquids or gases). It occurs due to differences in density caused by temperature variations. When a fluid is heated, it expands and becomes less dense. The warmer, less dense fluid rises, while the cooler, denser fluid sinks. This sets up a circulation pattern known as convection currents, which facilitate the transfer of heat. Convection is responsible for heat transfer in liquids and gases, such as the boiling of water or the circulation of warm air in a room.Radiation: Radiation is the transfer of thermal energy through electromagnetic waves. Unlike conduction and convection, radiation does not require a medium for transfer. All objects emit thermal radiation in the form of electromagnetic waves, primarily in the infrared range. Hotter objects emit more radiation, and the energy is transferred from the hotter object to cooler surroundings. This transfer can occur in a vacuum, making radiation the only mechanism for heat transfer in space. Examples of radiation include the heat we receive from the Sun or the warmth we feel standing near a fire.It's important to note that heat transfer often occurs through a combination of these mechanisms. For example, when you hold a hot cup of coffee, heat is conducted from the cup to your hand, while convection occurs within the coffee as it circulates due to the temperature difference. At the same time, the cup radiates thermal energy, which can be felt as warmth. Understanding these mechanisms helps us comprehend how heat is transferred in various situations and allows for effective thermal mana.
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A converging lens has a focal length of 18.6 cm. Construct accurate ray diagrams for object distances of (i) 3.72 cm and (ii) 93.0 cm.
(d) What is the magnification of the image?
Image (i)
Image (ii)
The magnification of the image formed for an object distance of 93.0 cm is approximately -0.1667.
To determine the magnification of the image formed by a converging lens, we can use the lens formula:
1/f = 1/v - 1/u
where:
f is the focal length of the lens,
v is the image distance (distance of the image from the lens),
u is the object distance (distance of the object from the lens).
Using the magnification formula:
magnification (m) = -v/u
where the negative sign indicates that the image formed is inverted.
Let's calculate the magnification for each scenario:
(i) Object distance (u) = 3.72 cm
Using the lens formula:
1/18.6 cm = 1/v - 1/3.72 cm
To solve for v, we can rearrange the equation:
1/v = 1/18.6 cm + 1/3.72 cm
1/v = (1 + 5)/18.6 cm
1/v = 6/18.6 cm
v = 18.6 cm / 6
v = 3.1 cm
Using the magnification formula:
magnification (m) = -v/u
magnification (m) = -3.1 cm / 3.72 cm
magnification (m) ≈ -0.83
Therefore, the magnification of the image formed for an object distance of 3.72 cm is approximately -0.83.
(ii) Object distance (u) = 93.0 cm
Using the lens formula:
1/18.6 cm = 1/v - 1/93.0 cm
To solve for v, we can rearrange the equation:
1/v = 1/18.6 cm + 1/93.0 cm
1/v = (5 + 1)/93.0 cm
1/v = 6/93.0 cm
v = 93.0 cm / 6
v = 15.5 cm
Using the magnification formula:
magnification (m) = -v/u
magnification (m) = -15.5 cm / 93.0 cm
magnification (m) ≈ -0.1667
Therefore, the magnification of the image formed for an object distance of 93.0 cm is approximately -0.1667.
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A power cycle operating between two reservoirs receives energy by heat transfer from a hot reservoir, Qh = 1764 kJ at Th=1544 K and rejects energy by heat transfer Qc= 441 kJ to a cold reservoir at Tc = 386 K. Determine whether the cycle operates reversibly irreversibly, or does not verify the second law of thermodynamics. O a. reversibly Ob. irreversibly Oc does not verify the second law of thermodynamics
(Oc) The cycle does not verify the second law of thermodynamics.
It is known that according to the second law of thermodynamics, no engine can have a higher efficiency than that of a reversible engine operating between the same two reservoirs. The efficiency of a reversible engine is given by:
ηr = 1 – Tc/Th
Where ηr is the efficiency of a reversible engine, Tc is the absolute temperature of the cold reservoir, and Th is the absolute temperature of the hot reservoir.
Energy received by heat transfer from the hot reservoir, Qh = 1764 kJ at Th = 1544 K.
Energy rejected by heat transfer to a cold reservoir, Qc = 441 kJ at Tc = 386 K.
The efficiency of the cycle, η = W/Qh.
We know that W = Qh – Qc.
Therefore, η = (Qh – Qc)/Qh.
η = (1764 - 441)/1764
η = 0.750
Therefore, the cycle is not operating reversibly, and neither is it verifying the second law of thermodynamics.
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Two very large parallel sheets are 5.00 cm apart. Sheet A carries a uniform surface charge density of −6.80μC/m
2
, and sheet B, which is to the right of A, carries a uniform charge density of −12.1μC/m
2
. Assume that the sheets are large enough to be treated as infinite. Part C Find the magnitude of the net electric field these sheets produce at a point 4.00 cm to the left of sheet A.
The magnitude of the net electric field is 2.31 × 10⁶ N/C.
Distance between two parallel sheets = 5.00 cm
Surface charge density of sheet A = -6.80 μC/m²
Surface charge density of sheet B = -12.1 μC/m²
The distance of the point from sheet A = 4.00 cm
The magnitude of the net electric field these sheets produce at a point 4.00 cm to the left of sheet A.
To find out the magnitude of the net electric field, we need to first find the electric field intensity produced by sheet A and B separately. After that, we can add them vectorially to get the net electric field intensity.
Electric field due to sheet A:
By applying the electric field formula, we get:
Electric field due to sheet A = σ / (2ε₀)
Where,
σ is the surface charge density of the sheet, and
ε₀ is the permittivity of free space.
Substituting the given values of surface charge density, we get:
Electric field due to sheet A = (-6.80 × 10⁻⁶) / (2 × 8.85 × 10⁻¹²)
= 4.53 × 10⁶ N/C
The electric field due to sheet A is towards the right.
Electric field due to sheet B:
The direction of the electric field due to sheet B is towards the left.
Substituting the given values of surface charge density, we get:
Electric field due to sheet B = (-12.1 × 10⁻⁶) / (2 × 8.85 × 10⁻¹²)
= 6.84 × 10⁶ N/C
The electric field due to sheet B is towards the left.
Magnitude of the net electric field:
Both the electric fields due to sheet A and B are not in the same direction. So, the net electric field would be the difference between the electric field due to sheet B and the electric field due to sheet A.
At a point which is 4.00 cm to the left of sheet A, the net electric field can be calculated as:
E_net = E_B - E_A
Where, E_A and E_B are the electric fields due to sheet A and sheet B, respectively.
Substituting the known values, we get:
E_net = 6.84 × 10⁶ - 4.53 × 10⁶
= 2.31 × 10⁶ N/C
Therefore, the magnitude of the net electric field is 2.31 × 10⁶ N/C.
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A rock is thrown vertically upward from ground level at time t=0. At t=2.5 s it passes the top of a tall tower, and 1.0 s later it reaches its maximum height. What is the height of the tower?
Answer:
The height of the tower is approximately 85.75 meters.
Explanation:
To determine the height of the tower, we need to consider the motion of the rock at different time intervals.
Given:
The time when the rock passes the top of the tower (t₁) = 2.5 s
Time when the rock reaches its maximum height (t₂) = 2.5 s + 1.0 s = 3.5 s
At time t₁ = 2.5 s, the rock has reached the top of the tower, which means its vertical displacement at that point is equal to the height of the tower.
To find the height of the tower, we need to calculate the vertical displacement of the rock at t₁ = 2.5 s.
Using the equation for vertical displacement in free-fall motion:
Δy = v₀t + (1/2)at²
Since the rock is thrown vertically upward, its initial velocity (v₀) is positive, and acceleration (a) due to gravity is negative (-9.8 m/s²).
At t = 2.5 s:
Δy = v₀t + (1/2)at²
Δy = v₀(2.5) + (1/2)(-9.8)(2.5)²
Δy = 2.5v₀ - 12.25
We know that at t = 2.5 s, the vertical displacement is equal to the height of the tower, so:
Tower height = Δy = 2.5v₀ - 12.25
Now, to find v₀, the initial velocity of the rock, we can use the information provided that 1.0 seconds after passing the top of the tower, the rock reaches its maximum height.
At t = 3.5 s, the rock reaches its maximum height, so its final velocity (v) is 0 m/s.
Using the equation for final velocity in free-fall motion:
v = v₀ + at
0 = v₀ + (-9.8)(3.5)
v₀ = 34.3 m/s
Now, substitute the value of v₀ into the equation for the tower height:
Tower height = 2.5v₀ - 12.25
Tower height = 2.5(34.3) - 12.25
Tower height ≈ 85.75 m
Therefore, the height of the tower is approximately 85.75 meters.
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An object's velocity is given as a function of position by the equation v=−2x, where x is in m and v is in m/s. At t=0,x=5 m. (a) What is x at t=0.2 s ? (b) What is its velocity at that time? (c) How far will the object travel after a long time?
(a) x at t=0.2 s is 4.6 m.
(b) Velocity at that time is -9.2 m/s.
(c) The object will travel an infinite distance in the negative direction.
(a) At t=0.2 s, the position x is given by the relation below: x = x0 + v0t + (1/2)at²
where x0 is the initial position, v0 is the initial velocity, a is the acceleration, and t is the time taken.
Substituting the given values in the formula above, we obtain:
x = 5 + (-2 × 0.2) + (1/2) × 0 × (0.2)²
Simplifying gives:
x = 4.6 m
Therefore, x is 4.6 m at t = 0.2 s.
(b) To get the velocity at t = 0.2 s, we differentiate the equation for x with respect to time:
dx/dt = -2x(t)dx/dt = v(t)
This gives the expression for the velocity as a function of time: v(t) = dx/dt = -2x(t)
Substituting x = 4.6 into the equation for velocity,v = -2(4.6)v = -9.2 m/s
Therefore, the velocity at t = 0.2 s is -9.2 m/s.
(c) To determine how far the object will travel after a long time, we need to find the limit of x as time t approaches infinity. When t becomes very large, position x will approach zero. Therefore, the object will travel an infinite distance in the negative direction.
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The trajectory of a projectile is a parabola. Use two position equations and prove that a projectile moves on a parabolic path.
The equation is quadratic, we can conclude that the trajectory of a projectile is a parabola.
To demonstrate that a projectile moves on a parabolic path, we can utilize two position equations: one for horizontal motion and another for vertical motion. Let's consider a projectile launched with an initial velocity of V₀ at an angle θ with respect to the horizontal.
For horizontal motion, we know that the only force acting on the projectile is gravity, which does not influence horizontal velocity. Therefore, the horizontal velocity remains constant throughout the motion, denoted as Vx = V₀ * cos(θ). The horizontal position of the projectile, x, can be expressed as x = V₀ * cos(θ) * t, where t represents time.
For vertical motion, the only force acting on the projectile is gravity, causing it to accelerate downwards. The vertical position of the projectile, y, can be described as y = V₀ * sin(θ) * t - (1/2) * g * t², where g represents the acceleration due to gravity.
By substituting the value of t from the horizontal position equation into the vertical position equation, we get y = (x * tan(θ)) - (g * x²) / (2 * V₀² * cos²(θ)). This equation represents the path of the projectile, and we observe that it is a quadratic equation in the form of y = ax² + bx + c, where a = -g / (2 * V₀² * cos²(θ)), b = tan(θ), and c = 0.
Since the equation is quadratic, we can conclude that the trajectory of a projectile is a parabola.
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A ball rolls off a platform that is 10 meters above the ground. The ball's horizontal velocity as it leaves the platform is 5 m/3. NOTE: This is a multi-part question. Once an answer is submitted, you will be unable to return to this part. Using the approximate value of g=10 m/s 2
. how much time does it take for the ball to hit the ground? The time taken by the ball to hit the ground is
The time taken by the ball to hit the ground is only one second.
To calculate the time it takes for the ball to hit the ground, we can consider the vertical motion of the ball. Given:
Initial vertical position (y0) = 10 meters
Acceleration due to gravity (g) = 10 m/s^2
We can use the equation for vertical motion:
y = y0 + v0y * t + (1/2) * g * t^2
Since the ball starts from rest vertically (v0y = 0), the equation simplifies to: y = y0 + (1/2) * g * t^2
Substituting the given values:
0 = 10 meters + (1/2) * 10 m/s^2 * t^2
Rearranging the equation:
5 meters = 5 m/s^2 * t^2
Dividing both sides by 5 m/s^2:
t^2 = 1
Taking the square root: t = 1 second
Therefore, it takes approximately 1 second for the ball to hit the ground.
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A mule is haressed to a sled having a mass of 201 kg, indoding sugplies. The mule muat exert a force exceeding 1220 N at an anglo of 36.3. (above the horizontal) in order ta get the sled moving. Trot the sled as a point particle. (4) Caiculate the normat ferce (in N ) sn the sied ahen the magnitude of the applied force is 1220 N. (Enter the magnituse.) N (b) Find wa ebetficient of static triction between the ved and the ground bencath ic. (c) Rind the static frictiso force (in N) when the mule is exerting a force of 6.10×10
2
N on the sled at the same angie. (Enter the mugnitude.)
The static friction force when the mule exerts a force of 6.10 × 10² N on the sled at the same angle is 339.16 N. Given:Mass of sled, m = 201 kg
Force exerted, F = 1220 N
Angle, θ = 36.3°
Part A:Calculate the normal force on the sled when the applied force is 1220 N.The normal force, FN can be found out as shown below;FN = mg - Fsinθ
Where, g = 9.8 m/s²
Substituting the given values, we get;FN = (201 × 9.8) - 1220sin(36.3)FN
= 1709.33 N
Thus, the normal force on the sled when the applied force is 1220 N is 1709.33 N.
Part B:Find the coefficient of static friction between the sled and the ground beneath it.The force of static friction can be found using the formula below;Ff = μs × FN
Where, Ff is the force of static frictionμs is the coefficient of static frictionFN is the normal force
Substituting the values obtained from Part A, we get;Ff = μs × 1709.33
At maximum, the force of static friction is given by;
Ff = Fcosθ
Hence, at maximum;Fcosθ = μs × FN
Thus,μs = Fcosθ / FNSubstituting the given values, we get;
μs = (1220cos36.3) / 1709.33μs
= 0.556
Thus, the coefficient of static friction between the sled and the ground beneath it is 0.556.
Part C:Find the static friction force when the mule exerts a force of 6.10 × 10² N on the sled at the same angle.The force of static friction is given by;Ff = μs × FN
Substituting the given values, we get;Ff = 0.556 × (6.10 × 10²)Ff
= 339.16 N
Thus, the static friction force when the mule exerts a force of 6.10 × 10² N on the sled at the same angle is 339.16 N.
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Four identical point charges (+1.15 nC) are placed at the corners of a rectangle, which measures 8.00 m by 5.00 m. If the electric potential is taken to be zero at infinity, what is the potential at the geometric center of this rectangle?
The electric potential at the geometric center of a rectangle, where four identical point charges (+1.15 nC) are placed at the corners, is approximately -9.48 V.
Four identical point charges (+1.15 nC) are placed at the corners of a rectangle, which measures 8.00 m by 5.00 m. If the electric potential is taken to be zero at infinity, the potential at the geometric center of this rectangle can be calculated as follows:
Potential due to point charges at the corners of rectangle is given by:
V = kQ/rl (in volts)
where Q is the magnitude of charge, r is the distance from the point charge, l is the distance from the point charge due to which the potential is being calculated, and k is Coulomb's constant = 9 × 10^9 Nm^2/C^2.
Let's assume that the charges are located at the corners A, B, C, and D as shown in the figure below:
Potential at point P, due to charge at corner A is:
V_A = kQ/r_AO
Potential at point P, due to charge at corner B is:
V_B = kQ/r_BO
Potential at point P, due to charge at corner C is:
V_C = kQ/r_CO
Potential at point P, due to charge at corner D is:
V_D = kQ/r_DO
Rectangle dimensions = 8 m × 5 m
Let's find the distance of the point P from each corner as follows:
r_AO = r_CO = 5/2 = 2.5 m
r_BO = r_DO = √((5/2)^2 + (8/2)^2) = 4.7 m
Charge on each point = 1.15 nC = 1.15 × 10^-9 C
The electric potential at the center of the rectangle can be obtained as the sum of all four point charges:
V_total = V_A + V_B + V_C + V_D
We know that the potential is taken to be zero at infinity. Hence the potential due to each charge is the work done in bringing the charge from infinity to the specified position. It can be represented as follows:
V = W/Q, where W is the work done in bringing the charge from infinity to the point in question and Q is the magnitude of the charge.
The potential due to each point charge can therefore be represented as:
V_A = W_A/Q = 0 - kQ/r_AO = - kQ/r_AO
V_B = W_B/Q = 0 - kQ/r_BO = - kQ/r_BO
V_C = W_C/Q = 0 - kQ/r_CO = - kQ/r_CO
V_D = W_D/Q = 0 - kQ/r_DO = - kQ/r_DO
We can now substitute the values in the above equation as follows:
V_total = kQ/r_AO + kQ/r_BO + kQ/r_CO + kQ/r_DO
= - kQ[(1/r_AO) + (1/r_BO) + (1/r_CO) + (1/r_DO)]
Therefore, the electric potential at the center of the rectangle is:
V_total = -9.48 V (approx.)
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A standard 1 kllogram weight is a cylinder 51.0 mm in height and 50.5 mm in diameter. What is the density of the material? kg/m
3
The density of the material can be calculated using the formula: density = mass/volume. By knowing the dimensions of the cylinder, we can determine its volume and then divide the mass of 1 kilogram by that volume to obtain the density.
To find the density of the material in [tex]kg/m^3[/tex], we first need to determine the volume of the cylinder. The formula for the volume of a cylinder is [tex]V = \pi r^2h[/tex], where r is the radius and h is the height. In this case, the diameter is given as 50.5 mm, which means the radius is half of that, or 25.25 mm (0.02525 m). The height is given as 51.0 mm (0.051 m). Substituting these values into the volume formula, we get [tex]V = \pi (0.02525)^2(0.051)[/tex]. Calculating this yields the volume of the cylinder as approximately 0.000101 [tex]m^3[/tex].
Next, we divide the mass of 1 kilogram by the volume we calculated to obtain the density. The formula for density is density = mass/volume. Thus, density = 1 kg / 0.000101 [tex]m^3[/tex], which gives us a density of approximately 9,901 [tex]kg/m^3[/tex] for the material of the cylinder.
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A river flows due south with a speed of 2.10 m/s. A man steers a motorboat across the river; his velocity relative to the water is 4.40 m/s. The river is 900 m wide. For related problem-solving tips and strategies, you may want to view a Video Tutor Solution of Compensating for a crosswind. In which direction should the motorboat head in order to reach a point on the opposite bank directly east from the starting point? (The boat's speed relative to the water remains 4.40 m/s.) Express your answer in degrees. X Incorrect; Try Again; 7 attempts remaining Part B What is the velocity of the boat relative to the earth? Express your answer in meters per second. How much time is required to cross the river? Express your answer in seconds.
The motorboat should head approximately 26.3° to the north of east in order to reach a point directly east from the starting point. The velocity of the boat relative to the earth is approximately 5.8 m/s. The time required to cross the river is approximately 214 seconds.
Let the direction of the motorboat be θ. Thus, its components are 4.40 cos θ to the east and 4.40 sin θ to the north. The component of the river's velocity is 2.10 to the south. Therefore, the velocity of the boat relative to the earth is (4.40 cos θ) i + (4.40 sin θ + 2.10) j.
If the boat is to reach a point on the opposite bank directly east from the starting point, then it must travel in a direction perpendicular to the river. Thus, 4.40 cos θ = 2.10t, where t is the time taken to cross the river. Solving the above equation for θ, we get:
θ = arctan(2.10 / 4.40) = 26.3° (to the north of east)
Therefore, the boat should head 26.3° to the north of east. The velocity of the boat relative to the earth is given as:
(4.40 cos θ) i + (4.40 sin θ + 2.10) j = 4.40 cos 26.3° i + (4.40 sin 26.3° + 2.10) j = 4.0 i + 4.4 j.
The magnitude of velocity of the boat relative to the earth is:
|V| = √(4.0² + 4.4²) ≈ 5.8 m/s.
Thus, the velocity of the boat relative to the earth is approximately 5.8 m/s.
The time required to cross the river is given by:
t = 900 / 4.40 cos 26.3° ≈ 214 seconds.
Therefore, the time required to cross the river is approximately 214 seconds.
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The electron mass is 9×10
−31
kg. What is the momentum of an electron traveling at a velocity of (0,0,−2.8×10
6
) m/s?
rho
= lg⋅m/s What is the magnitude of the momentum of the electron? p= kg⋅m/s
The momentum of an electron traveling at a velocity of (0,0,-2.8x10^6) m/s is - 2.52 × 10^-24 kg.m/s.
Magnitude of the momentum of the electron is given byρ = |p| = √(px^2 + py^2 + pz^2)ρ = |p| = √[(0)^2 + (0)^2 + (-2.52 x 10^-24)^2]ρ = |p| = 2.52 x 10^-24 kg.m/s.
The momentum of an electron traveling at a velocity of (0,0,-2.8x10^6) m/s,
given the electron mass to be 9x10^-31 kg,
and the momentum (p) of the electron is calculated using the relation:
p=mv, where m is the mass of the electron and v is the velocity of the electron.
p = momentum of the electron = kg.m/s
m = mass of the electron = 9 x 10^-31 kg
v = velocity of the electron = (0, 0, -2.8 x 10^6) m/s
The momentum of an electron traveling at a velocity of (0,0,-2.8x10^6) m/s is - 2.52 × 10^-24 kg.m/s.
Magnitude of the momentum of the electron is given byρ = |p| = √(px^2 + py^2 + pz^2)ρ = |p| = √[(0)^2 + (0)^2 + (-2.52 x 10^-24)^2]ρ = |p| = 2.52 x 10^-24 kg.m/s.
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