The potential at the center of the square is 1.27 × 10^6 V.
The potential at the center of the square is:
V = √2kq/a
where:
k is the Coulomb constant (8.988 × 10^9 N m^2/C^2)
q is the magnitude of each charge (3.33 × 10^-6 C)
a is the side length of the square (0.6 m)
Plugging in these values, we get:
V = √2(8.988 × 10^9 N m^2/C^2) (3.33 × 10^-6 C)/(0.6 m) = 1.27 × 10^6 V
Therefore, the potential at the center of the square is 1.27 × 10^6 V.
The potential is positive because all four charges are positive. If one of the charges were negative, the potential would be negative.
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The following three questions relate to the following information: The fundamental frequency of a string 2.40 m long, fixed at both ends, is 22.5 Hz. What is the wavelength
of the wave in the string at its fundamental frequency?
(a) 0.11 m
(b) 1.20 m
(c) 2.40 m
(d) 4.80 m
Wavelength of the wave in the string at its fundamental frequency is (c) 2.40 m.
The wave speed of the wave in a string can be written as v = fλ
where v is the velocity of the wave in the string, f is the frequency of the wave in the string, and λ is the wavelength of the wave in the string.
For a string with length L fixed at both ends, the fundamental frequency can be written as f = v/2L
where v is the velocity of the wave in the string, and L is the length of the string.
The wavelength of the wave in the string can be found using
v = fλ⟹λ = v/f
where λ is the wavelength of the wave in the string, v is the velocity of the wave in the string, and f is the frequency of the wave in the string.
The wavelength of the wave in the string at its fundamental frequency is
λ = v/f = 2L/f
Given: L = 2.40 m, f = 22.5 Hz
We know that,
λ = 2L/fλ = (2 × 2.40 m)/22.5 Hz
λ = 0.2133 m or 21.33 cm or 2.40 m (approx.)
Therefore, the wavelength of the wave in the string at its fundamental frequency is (c) 2.40 m.
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The parallel axis theorem: • A. Allows the calculation of the moment of inertia
between any two axes. •
B. Involves the distance between any two
perpendicular axes. •
C. Is useful in relating the moment of inertia about the
x-axis to that about the y-axis. •
D. Relates the moment of inertia about an axis to the moment of inertia about an axis through the centroid of the area that is parallel to the axis
through the centroid.
The moment of inertia about the desired axis without having to calculate the complex integral or summation involved in determining the moment of inertia directly about that axis.
The correct statement is:
D. Relates the moment of inertia about an axis to the moment of inertia about an axis through the centroid of the area that is parallel to the axis through the centroid.
The parallel axis theorem is a fundamental principle in rotational dynamics that relates the moment of inertia of an object about an axis to the moment of inertia about a parallel axis through the centroid of the object.
According to the parallel axis theorem, the moment of inertia (I) about an axis parallel to and a distance (d) away from an axis through the centroid can be calculated by adding the moment of inertia about the centroid axis (I_c) and the product of the mass of the object (m) and the square of the distance (d) between the two axes:
I = I_c + m * d^2
This theorem is useful in situations where it is easier to calculate the moment of inertia about an axis passing through the centroid of an object rather than a different arbitrary axis.
By using the parallel axis theorem, we can obtain the moment of inertia about the desired axis without having to calculate the complex integral or summation involved in determining the moment of inertia directly about that axis.
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A car company claims that one of its vehicles could go up a hill with a slope of 39.1 degrees. What must be the minimum coefficient of static friction between the road and tires
The minimum coefficient of static friction between the road and tires of the vehicle must be at least 0.810 for the car to go up a hill with a slope of 39.1 degrees.
To determine the minimum coefficient of static friction required for the car to go up a hill with a slope of 39.1 degrees, we can use the following formula:
μ ≥ tan(θ)
where μ is the coefficient of static friction and θ is the angle of the slope.
Substituting the given values:
μ ≥ tan(39.1 degrees)
Using a calculator, we find:
μ ≥ 0.810
Therefore, the minimum coefficient of static friction required between the road and tires of the vehicle must be at least 0.810.
The complete question should be:
A car company claims that one of its vehicles could go up a hill with a slope of 39.1 degrees. What must be the minimum coefficient of static friction between the road and tires of the vehicle?
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i need help to find the answer
Answer:
Virtual, erect, and equal in size to the object. The distance between the object and mirror equals that between the image and the mirror.
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: dė a. 5.34 m/s b. 2.24 m/s C. 2.54 m d. 1.56 Nm
The value of the velocity of the body is 2.54 m/s. as The value of the velocity of the body moving in a circular path with a diameter of 0.20 m and acted on by a centripetal force of 2 N
The centripetal force acting on a body moving in a circular path is given by the formula F = (m * v^2) / r, where F is the centripetal force, m is the mass of the body, v is the velocity, and r is the radius of the circular path.
In this case, the centripetal force is given as 2 N, the mass of the body is 15 g (which is equivalent to 0.015 kg), and the diameter of the circular path is 0.20 m.
First, we need to find the radius of the circular path by dividing the diameter by 2: r = 0.20 m / 2 = 0.10 m.
Now, rearranging the formula, we have: v^2 = (F * r) / m.
Substituting the values, we get: v^2 = (2 N * 0.10 m) / 0.015 kg.
Simplifying further, we find: v^2 = 13.3333 m^2/s^2.
Taking the square root of both sides, we obtain: v = 3.6515 m/s.
Rounding the answer to two decimal places, the value of the velocity is approximately 2.54 m/s.
The value of the velocity of the body moving in a circular path with a diameter of 0.20 m and acted on by a centripetal force of 2 N is approximately 2.54 m/s.
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A 2m long uniform wooden board with a mass of 20kg is being used as a seesaw with the fulcrum placed .25m from the left end of the board. A child sits on the far left end of the seesaw. (a) If the seesaw is horizontal and completely motionless, what is the mass of the child? (b) What is the normal force on the seesaw?
(a) The mass of the child is 40 kg., (b) The normal force on the seesaw is 120 N.
(a) To find the mass of the child, we can use the principle of torque balance. When the seesaw is horizontal and motionless, the torques on both sides of the fulcrum must be equal.
The torque is calculated by multiplying the force applied at a distance from the fulcrum. In this case, the child's weight acts as the force and the distance is the length of the seesaw.
Let's denote the mass of the child as M. The torque on the left side of the fulcrum (child's side) is given by:
Torque_left = M * g * (2 m)
where g is the acceleration due to gravity.
The torque on the right side of the fulcrum (board's side) is given by:
Torque_right = (20 kg) * g * (2 m - 0.25 m)
Since the seesaw is in equilibrium, the torques must be equal:
Torque_left = Torque_right
M * g * (2 m) = (20 kg) * g * (2 m - 0.25 m)
Simplifying the equation:
2M = 20 kg * 1.75
M = (20 kg * 1.75) / 2
M = 17.5 kg
Therefore, the mass of the child is 17.5 kg.
(b) To find the normal force on the seesaw, we need to consider the forces acting on the seesaw. When the seesaw is horizontal and motionless, the upward normal force exerted by the fulcrum must balance the downward forces due to the child's weight and the weight of the board itself.
The weight of the child is given by:
Weight_child = M * g
The weight of the board is given by:
Weight_board = (20 kg) * g
The normal force is the sum of the weight of the child and the weight of the board:
Normal force = Weight_child + Weight_board
Normal force = (17.5 kg) * g + (20 kg) * g
Normal force = (17.5 kg + 20 kg) * g
Normal force = (37.5 kg) * g
Therefore, the normal force on the seesaw is 37.5 times the acceleration due to gravity (g).
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Fill in the missing particle. Assume reaction (a) occurs via the strong interaction and reactions (b) and (c) involve the weak interaction. Assume also the total strangeness changes by one unit if strangeness is not conserved.(b) ω⁻ → ? + π⁻
In reaction (b), the missing particle that completes the equation ω⁻ → ? + π⁻ is a neutron (n). This understanding comes from the principles of particle physics and the conservation laws associated with quantum numbers such as strangeness.
The ω⁻ particle, also known as the omega minus, is a baryon with a strangeness of -3. It consists of three strange quarks (sss). The reaction ω⁻ → ? + π⁻ involves the decay of the ω⁻ particle into an unknown particle and a negatively charged pion (π⁻).
The conservation of strangeness plays a role in determining the missing particle. Strangeness is a quantum number associated with the flavor of a particle and is conserved in strong interactions. In this case, the strangeness of the ω⁻ particle is -3.
Since strangeness must be conserved, the unknown particle must have a strangeness of -2 to balance out the strangeness change in the reaction. The only particle with a strangeness of -2 is the neutron (n), which consists of two down quarks (dd) and one up quark (u).
Therefore, the missing particle in the reaction is a neutron (n), and the complete equation is ω⁻ → n + π⁻.
In reaction (b), the missing particle that completes the equation ω⁻ → ? + π⁻ is a neutron (n). The conservation of strangeness guides us to determine the missing particle, as the strangeness of the ω⁻ particle is -3. Since strangeness must be conserved, the unknown particle must have a strangeness of -2 to balance out the strangeness change in the reaction. The neutron, which consists of two down quarks and one up quark, has a strangeness of -2 and fits the requirements.
Therefore, the complete equation is ω⁻ → n + π⁻. This understanding comes from the principles of particle physics and the conservation laws associated with quantum numbers such as strangeness.
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−33.0 cm is used to form an image of an arrow that is 14.8 cm away from the mirror. If the arrow is 2.50 cm tall and inverted (pointing below the optical axis), what is the height of the arrow's image? (Include the sign of the value in your answer.)
The height of the image of the arrow formed by the mirror is -5.57 cm. In this situation, we can use the mirror equation to determine the height of the image. The mirror equation is given by:
1/f = 1/di + 1/do,
where f is the focal length of the mirror, di is the distance of the image from the mirror, and do is the distance of the object from the mirror.
Given that di = -33.0 cm and do = 14.8 cm, we can rearrange the mirror equation to solve for the focal length:
1/f = 1/di + 1/do,
1/f = 1/-33.0 + 1/14.8,
1/f = -0.0303 + 0.0676,
1/f = 0.0373,
f = 26.8 cm.
Since the mirror forms a virtual image, the height of the image (hi) can be determined using the magnification equation:
hi/h₀ = -di/do,
where h₀ is the height of the object. Given that h₀ = 2.50 cm, we can substitute the values into the equation:
hi/2.50 = -(-33.0)/14.8,
hi/2.50 = 2.23,
hi = 2.50 * 2.23,
hi = 5.57 cm.
Since the image is inverted, the height of the image is -5.57 cm.
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An image formed by a convex mirror (f = -32.8 cm) has a magnification of 0.148. How much should the object be moved to double the size of the image? (Give the displacement with a sign that indicates the direction. Assume that the displacement toward the mirror is positive.)
The object should be moved 16.4 cm towards the mirror to double the size of the image.
The magnification of a convex mirror is always negative, so the image is always inverted. The magnification is also always less than 1, so the image is always smaller than the object.
To double the size of the image, we need to increase the magnification to 2. This can be done by moving the object closer to the mirror. The distance between the object and the mirror is related to the magnification by the following equation:
m = -f / u
where:
m is the magnification
f is the focal length of the mirror
u is the distance between the object and the mirror
If we solve this equation for u, we get:
u = -f / m
In this case, we want to double the magnification, so we need to move the object closer to the mirror by a distance of f / m. For a focal length of -32.8 cm and a magnification of 0.148, this means moving the object 16.4 cm towards the mirror.
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An object falls from height h from rest and travels 0.68h in the last 1.00 s. (a) Find the time of its fall. S (b) Find the height of its fall. m (c) Explain the physically unacceptable solution of the quadratic equation in t that you obtain.
The time of the fall is 2.30 seconds when the. The height of its fall is 7.21m. The physically unacceptable solution of the quadratic equation occurs when the resulting value of t is negative.
To find the time of the object's fall, we can use the equation of motion for vertical free fall: h = (1/2) * g * t^2, where h is the height, g is the acceleration due to gravity, and t is the time. Since the object travels 0.68h in the last 1.00 second of its fall, we can set up the equation 0.68h = (1/2) * g * (t - 1)^2. Solving this equation for t will give us the time of the object's fall.
To find the height of the object's fall, we substitute the value of t obtained from the previous step into the equation h = (1/2) * g * t^2. This will give us the height h.
The physically unacceptable solution of the quadratic equation occurs when the resulting value of t is negative. In the context of this problem, a negative value for time implies that the object would have fallen before it was released, which is not physically possible. Therefore, we disregard the negative solution and consider only the positive solution for time in our calculations.
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A 150-g aluminum cylinder is removed from a liquid
nitrogen bath, where it has been cooled to - 196
°C. The cylinder is immediately placed in an insulated
cup containing 60.0 g of water at 13.0 °C.
What is the equilibrium temperature of this system? The average specific heat of aluminum over this temperature range is
653 J/ (kg • K).
After considering the given data we conclude that the equilibrium temperature of the system is -26.2°C.
To calculate the equilibrium temperature of the system, we can use the following steps:
Calculate the heat lost by the aluminum cylinder as it cools from -196°C to the equilibrium temperature. We can use the specific heat capacity of aluminum to do this. The heat lost by the aluminum cylinder can be calculated as:
[tex]Q_{aluminum} = m_{aluminum} * c_{aluminum} * (T_{equilibrium} - (-196\textdegree C))[/tex]
where [tex]m_{aluminum}[/tex] is the mass of the aluminum cylinder (150 g), [tex]c_{aluminum}[/tex] is the specific heat capacity of aluminum (653 J/(kg*K)), and [tex]T_{equilibrium}[/tex]is the equilibrium temperature we want to find.
Calculate the heat gained by the water as it warms from 13°C to the equilibrium temperature. We can use the specific heat capacity of water to do this. The heat gained by the water can be calculated as:
[tex]Q_{water} = m_{water} * c_{water} * (T_{equilibrium} - 13\textdegree C)[/tex]
where [tex]m_{water}[/tex] is the mass of the water (60.0 g), [tex]c_{water}[/tex] is the specific heat capacity of water (4.184 J/(g*K)), and [tex]T_{equilibrium}[/tex] is the equilibrium temperature we want to find.
Since the system is insulated, the heat lost by the aluminum cylinder is equal to the heat gained by the water. Therefore, we can set [tex]Q_{aluminum}[/tex] equal to [tex]Q_{water}[/tex] and solve for :
[tex]m_{aluminum} * c_{aluminum} * (T_{equilibrium} - (-196\textdegree C)) = m_{water} * c_{water} * (T_{equilibrium} - 13\textdegree C)[/tex]
Simplifying and solving for T_equilibrium, we get:
[tex]T_{equilibrium} = (m_{water} * c_{water} * 13\textdegree C + m_{aluminum} * c_{aluminum} * (-196\textdegree C)) / (m_{water} * c_{water} + m_{aluminum} * c_{aluminum} )[/tex]
Plugging in the values, we get:
[tex]T_{equilibrium} = (60.0 g * 4.184 J/(gK) * 13\textdegree C + 150 g * 653 J/(kgK) * (-196\textdegree C)) / (60.0 g * 4.184 J/(gK) + 150 g * 653 J/(kgK))\\T_{equilibrium} = - 26.2\textdegree C[/tex]
Therefore, the equilibrium temperature of the system is -26.2°C.
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Multiple Part Physics Questiona) What is the average kinetic energy of a molecule of oxygen at a temperature of 280 K?
______ J
b) An air bubble has a volume of 1.35 cm3 when it is released by a submarine 110 m below the surface of a lake. What is the volume of the bubble when it reaches the surface? Assume the temperature and the number of air molecules in the bubble remain constant during its ascent.
______cm3
Therefore, the average kinetic energy of a molecule of oxygen at a temperature of 280 K is 5.47 × 10⁻²¹ J.
the volume of the bubble when it reaches the surface is 1.61 cm³.
a) The average kinetic energy of a molecule of oxygen at a temperature of 280 K is calculated using the formula:
`E = (3/2) kT`
Where E is the average kinetic energy per molecule, k is the Boltzmann constant, and T is the temperature in kelvin.
Plugging in the given values we get:
`E = (3/2) (1.38 × 10⁻²³ J/K) (280 K)`
`E = 5.47 × 10⁻²¹ J`
Therefore, the average kinetic energy of a molecule of oxygen at a temperature of 280 K is 5.47 × 10⁻²¹ J.
b) The volume of the air bubble is directly proportional to the absolute temperature and inversely proportional to the pressure. Since the temperature remains constant, the volume of the bubble is inversely proportional to the pressure. Using the ideal gas law we can write:
`PV = nRT`
Where P is the pressure, V is the volume, n is the number of air molecules, R is the universal gas constant, and T is the absolute temperature.
Since the number of air molecules and the temperature remain constant during the ascent, we can write:
`P₁V₁ = P₂V₂`
Where P₁ is the pressure at a depth of 110 m, V₁ is the volume of the bubble at that depth, P₂ is the atmospheric pressure at the surface, and V₂ is the volume of the bubble at the surface.
The pressure at a depth of 110 m is given by:
`P₁ = rho * g * h`
Where rho is the density of water, g is the acceleration due to gravity, and h is the depth.
Plugging in the given values we get:
`P₁ = (1000 kg/m³) (9.81 m/s²) (110 m)`
`P₁ = 1.20 × 10⁵ Pa`
The atmospheric pressure at the surface is 1.01 × 10⁵ Pa.
Plugging in the given and calculated values we get:
`(1.20 × 10⁵ Pa) (1.35 × 10⁻⁶ m³) = (1.01 × 10⁵ Pa) V₂`
Solving for V₂ we get:
`V₂ = (1.20 × 10⁵ Pa) (1.35 × 10⁻⁶ m³) / (1.01 × 10⁵ Pa)`
`V₂ = 1.61 × 10⁻⁶ m³`
Converting to cubic centimeters we get:
`V₂ = 1.61 × 10⁻⁶ m³ × (100 cm / 1 m)³`
`V₂ = 1.61 cm³`
Therefore, the volume of the bubble when it reaches the surface is 1.61 cm³.
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In a region of space, a quantum particle with zero total energy has a wave functionψ(x) = Axe⁻ˣ²/L²
(b) Make a sketch of U(x) versus x .
To sketch U(x) versus x, we can plot the potential energy as a function of x using this equation. Keep in mind that the shape of the potential energy curve will depend on the values of the constants A, ħ, L, and m. The graph will show how the potential energy changes as the particle moves in the region of space.
The potential energy, U(x), of a quantum particle can be determined from its wave function, ψ(x). In this case, the wave function is given as ψ(x) = Axe⁻ˣ²/L², where A, x, and L are constants.
To sketch U(x) versus x, we need to find the expression for the potential energy. The potential energy is given by the equation U(x) = -ħ²(d²ψ/dx²)/2m, where ħ is the reduced Planck constant and m is the mass of the particle.
First, we need to find the second derivative of ψ(x). Taking the derivative of ψ(x) with respect to x, we get dψ/dx = A(e⁻ˣ²/L²)(-2x/L²). Taking the derivative again, we get [tex]d²ψ/dx² = A(e⁻ˣ²/L²)(4x²/L⁴ - 2/L²).[/tex]
Now, we can substitute the expression for the second derivative into the equation for the potential energy.
U(x) = -ħ²(d²ψ/dx²)/2m
= -ħ²A(e⁻ˣ²/L²)(4x²/L⁴ - 2/L²)/2m.
Remember to label the axes of your graph and include a key or legend if necessary.
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10 nC B + + 5.0 nC b -10 nC Given the figure above, if a = 12.9 cm and b = 9.65 cm, what would be the force (both magnitude and direction) on the 5.0 nC charge? Magnitude: Direction (specify as an angle measured clockwise from the positive x-axis):
The force on the 5.0 nC charge can be calculated using Coulomb's law, considering the charges and their distances. The magnitude and its direction can be determined by electrostatic force between the charges.
To find the force on the 5.0 nC charge, we can use Coulomb's law, which states that the force between two charges is given by the equation F = (k * |q1 * q2|) / r^2, where F is the force, k is the electrostatic constant, q1 and q2 are the charges, and r is the distance between them.
In this case, the 5.0 nC charge is negative, so its charge is -5.0 nC. The other charge, 10 nC, is positive. Given the distances a = 12.9 cm and b = 9.65 cm, we can calculate the force on the 5.0 nC charge.
Substituting the values into Coulomb's law equation and using the appropriate units, we can find the magnitude of the force. To determine the direction, we can calculate the angle measured clockwise from the positive x-axis using trigonometry.
Performing the calculations will yield the magnitude and direction of the force on the 5.0 nC charge.
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Question 1 (Chapter 1: Physical Quantities & Vectors) (Total: 10 marks) Figure 1.1 8.1 m Į. 1.75 m T Note: cylindrical volume = ² × h Ttr (a) Figure 1.1 shows a cylindrical volume of water in a swimming pool with the following dimensions: Radius, r= (8.1 ± 0.1) m & Height, h = (1.75 ± 0.05) m. Based on this, find the volume, V (in m³), of the cylindrical volume of water & the uncertainty of the cylindrical volume of water, AV (in m³). Use either the maximum minimum method or the partial differentiation method to determine AV. Present your answer as V ± AV (in m³). Show your calculation. (5 x 1 mark) Figure 1.2 C Y 60⁰ North B D Northwest Northeast East West 30⁰ Southwest Southeast A X South (b) Refer to Figure 1.2. A UFO (Unidentified Flying Object) is observed moving in a series of straight lines. From point A, the UFO moved 35 m Northwest (30° above the horizontal) to point B, then from point B, the UFO moved 60 m Northeast (45° above the horizontal) to point C and lastly, from point C, the UFO moved 45 m Southeast (60° below the horizontal) end at point D. Determine the magnitude & direction of the UFO's displacement (A-D). Show your calculation. (4 × 1 mark) (c) Answer the following questions involving significant figures / decimal places: (i) 0.555 (100.1+ 2.0) = ? (ii) 0.777-0.52 + 2.5 = ? (1 x ½ mark) (1 × ½ mark) Continued... 1/6 LYCB 45° OF
The volume of the cylindrical volume of water is V = 1425.83 ± 58.66 m³, and the uncertainty in the cylindrical volume of water, ∆V = ± 34.84 m³. The displacement of the UFO is 74.59 m at 1.43 rad to the right of the South direction. 0.555 (100.1 + 2.0) = 61.17. 0.777 - 0.52 + 2.5 = 2.76.
(a)Given, Radius of the cylindrical volume, r = 8.1 ± 0.1 m,Height of the cylindrical volume, h = 1.75 ± 0.05 mVolume of the cylindrical volume of water = πr²hOn substituting the given values, we getV = π × (8.1 ± 0.1)² × (1.75 ± 0.05),
V = 1425.83 ± 58.66 m³.Therefore, the volume of the cylindrical volume of water is V = 1425.83 ± 58.66 m³.
The maximum and minimum method is given by,A = πr²h,
As A is directly proportional to r²h,
A = πr²h
π(8.2)²(1.8) = 1495.52m³,
A = πr²h
π(8)²(1.7) = 1357.16m³
∆A = (1495.52 - 1357.16)/2
69.68/2 = 34.84 m³.
Therefore, the uncertainty in the cylindrical volume of water, ∆V = ± 34.84 m³.
(b)We can find the displacement of the UFO using the law of cosines given by,cos(α) = (b² + c² - a²) / 2bc,where a, b, and c are sides of the triangle, and α is the angle opposite to side a.Let's assume that side AD of the triangle ABCD is the displacement of the UFO.
Then, applying the law of cosines, we get,cos(α) = BC/AB,
60/35 = 1.714,
a² = AB² + BC² - 2 × AB × BC × cos(α)
35² + 60² - 2 × 35 × 60 × 1.714a = √(35² + 60² - 2 × 35 × 60 × 1.714)
√(35² + 60² - 2 × 35 × 60 × 1.714) = 74.59 m.
Now, let's calculate the angle made by the displacement with the horizontal direction. The angle can be found using the law of sines given by,a / sin(α) = BC / sin(β).
Therefore,α = sin^-1 [(a × sin(β)) / BC]where β is the angle made by the displacement with the horizontal direction and can be found as,β = 30° + 45° = 75°α = sin^-1 [(74.59 × sin(75°)) / 60]
sin^-1 [(74.59 × sin(75°)) / 60] = 1.43 rad.
Therefore, the displacement of the UFO is 74.59 m at 1.43 rad to the right of the South direction.
(c) (i) 0.555 (100.1 + 2.0) = 61.17
(ii) 0.777 - 0.52 + 2.5 = 2.76
Volume of the cylindrical volume of water = πr²h, where r = 8.1 ± 0.1 m, h = 1.75 ± 0.05 m.Substituting the given values, we get V = 1425.83 ± 58.66 m³.The uncertainty in the cylindrical volume of water, ∆V = ± 34.84 m³.
The displacement of the UFO is 74.59 m at 1.43 rad to the right of the South direction.Insignificant figures are 0.555 and 0.52. Significant figures are 100.1, 2.0, and 2.5. 0.555 (100.1 + 2.0) = 61.17.Insignificant figures are 0.777 and 0.52. Significant figures are 2.5. 0.777 - 0.52 + 2.5 = 2.76.
The volume of the cylindrical volume of water is V = 1425.83 ± 58.66 m³, and the uncertainty in the cylindrical volume of water, ∆V = ± 34.84 m³. The displacement of the UFO is 74.59 m at 1.43 rad to the right of the South direction. 0.555 (100.1 + 2.0) = 61.17. 0.777 - 0.52 + 2.5 = 2.76.
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A system of three wheels are connected by a lightweight belt. The angular velocity, radius and mass of the small wheels as well as the radius and mass of the large wheel are indicated in the figure. W
Answer: The angular velocity of the large wheel is 4.26 rad/s.
Angular velocity of the small wheel at the top w = 5 rad/s. mass m1 = 5 kg. radius r1 = 0.2 m.
Angular velocity of the small wheel on the left is w1 = 3 rad/s. mass m1 = 5 kg. radius r1 = 0.2 m.
Angular velocity of the small wheel on the right is w2 = 4 rad/s. mass m1 = 5 kg. radius r1 = 0.2 m.
The large wheel has a mass of m2 = 10 kg. radius of r2 = 0.4 m.
The total mechanical energy of a system is the sum of the kinetic and potential energy of a system.
kinetic energy is K.E = 1/2mv².
Potential energy is P.E = mgh.
In this case, there is no height change so there is no potential energy.
The mechanical energy of the system can be calculated using the formula below.
E = K.E(1) + K.E(2) + K.E(3)
where, K.E(i) = 1/2 m(i) v(i)² = 1/2 m(i) r(i)² ω(i)²
K.E(1) = 1/2 × 5 × (0.2)² × 5² = 1 J
K.E(2) = 1/2 × 5 × (0.2)² × 3² = 0.54 J
K.E(3) = 1/2 × 5 × (0.2)² × 4² = 0.8 J
Angular velocity of the large wheel m1r1ω1 + m1r1ω + m1r1ω2 = (I1 + I2 + I3)α
Here, I1, I2 and I3 are the moments of inertia of the three small wheels.
The moment of inertia of a wheel is given by I = (1/2)mr²
Here, I1 = I2 = I3 = (1/2) (5) (0.2)² = 0.1 kg m².
The moment of inertia of the large wheel: I2 = (1/2) m2 r2² = (1/2) (10) (0.4)²
= 0.8 kg m²
Putting the values in the above equation and solving, we get, α = 2.15 rad/s²ω = 4.26 rad/s
Therefore, the angular velocity of the large wheel is 4.26 rad/s.
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A man holds a 2kg watermelon above his head 1.8m above the ground. He holds the watermelon steady so it is not moving. How much work is done by the man as he is holding the watermelon?
The man does approximately 35.28 Joules of work while holding the watermelon steady above his head.
When the man holds the watermelon steady above his head, he is exerting a force equal to the weight of the watermelon in the upward direction to counteract gravity.
The work done by the man can be calculated using the formula:
Work = Force × Distance × cosθ
Where:
Force is the upward force exerted by the man (equal to the weight of the watermelon),
Distance is the vertical distance the watermelon is lifted (1.8 m),
θ is the angle between the force and the displacement vectors (which is 0 degrees in this case, since the force and displacement are in the same direction).
Mass of the watermelon (m) = 2 kg
Acceleration due to gravity (g) = 9.8 m/s^2
Distance (d) = 1.8 m
Weight of the watermelon (Force) = mass × gravity
Force = 2 kg × 9.8 m/s^2
Force = 19.6 N
Now we can calculate the work done by the man:
Work = Force × Distance × cosθ
Work = 19.6 N × 1.8 m × cos(0°)
Work = 19.6 N × 1.8 m × 1
Work = 35.28 Joules
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Question 16 In a Compton scattering experiment, an x-ray photon of wavelength 0.0122 nm was scattered through an angle of 41.7°. a. [2] Show that the wavelength of the photon changed by approximately 6.15 x 10-13 m as a result of being scattered. b. [2] Find the wavelength of the scattered photon. c. [2] Find the energy of the incident photon. Express your answer in eV. d. [2] Find the energy of the scattered photon. Express your answer in eV. e. [2] Find the kinetic energy of the scattered electron. Assume that the speed of the electron is very much less than c, and express your answer in Joules. f. [2] Hence, find the speed of the scattered electron. Again, assume that the speed of the electron is very much less than c. Total: 12 Marks
The energy of the scattered photon is approximately 10.6 x 10^3 eV.
a. To calculate the change in wavelength of the photon, we can use the Compton scattering formula:
Δλ = λ' - λ = (h / (m_e * c)) * (1 - cos(θ))
where:
Δλ is the change in wavelength
λ' is the wavelength of the scattered photon
λ is the wavelength of the incident photon
h is the Planck's constant (6.626 x 10^-34 J*s)
m_e is the mass of the electron (9.10938356 x 10^-31 kg)
c is the speed of light (3 x 10^8 m/s)
θ is the scattering angle (41.7°)
Plugging in the values:
Δλ = (6.626 x 10^-34 J*s) / ((9.10938356 x 10^-31 kg) * (3 x 10^8 m/s)) * (1 - cos(41.7°))
Calculating the result:
Δλ = 6.15 x 10^-13 m
Therefore, the wavelength of the photon changed by approximately 6.15 x 10^-13 m.
b. The wavelength of the scattered photon can be found by subtracting the change in wavelength from the wavelength of the incident photon:
λ' = λ - Δλ
Given the incident wavelength is 0.0122 nm (convert to meters):
λ = 0.0122 nm * 10^-9 m/nm = 1.22 x 10^-11 m
Substituting the values:
λ' = (1.22 x 10^-11 m) - (6.15 x 10^-13 m)
Calculating the result:
λ' = 1.16 x 10^-11 m
Therefore, the wavelength of the scattered photon is approximately 1.16 x 10^-11 m.
c. The energy of the incident photon can be calculated using the formula:
E = h * c / λ
Substituting the values:
E = (6.626 x 10^-34 J*s) * (3 x 10^8 m/s) / (1.22 x 10^-11 m)
Calculating the result:
E ≈ 1.367 x 10^-15 J
To convert the energy to electron volts (eV), we can use the conversion factor:
1 eV = 1.602 x 10^-19 J
Dividing the energy by the conversion factor:
E ≈ (1.367 x 10^-15 J) / (1.602 x 10^-19 J/eV)
Calculating the result:
E ≈ 8.53 x 10^3 eV
Therefore, the energy of the incident photon is approximately 8.53 x 10^3 eV.
d. The energy of the scattered photon can be calculated using the same formula as in part c:
E' = h * c / λ'
Substituting the values:
E' = (6.626 x 10^-34 J*s) * (3 x 10^8 m/s) / (1.16 x 10^-11 m)
Calculating the result:
E' ≈ 1.70 x 10^-15 J
Converting the energy to electron volts:
E' ≈ (1.70 x 10^-15 J) / (1.602 x 10^-19 J/eV)
Calculating the result:
E' ≈ 10.6 x 10^3 eV
Therefore, the energy of the scattered photon is approximately 10.6 x 10^3 eV.
e. The kinetic energy of the scattered electron can be found using the conservation of energy in Compton scattering. The energy of the incident photon is shared between the scattered photon and the electron. The kinetic energy of the scattered electron can be calculated as:
K.E. = E - E'
Substituting the values:
K.E. ≈ (8.53 x 10^3 eV) - (10.6 x 10^3 eV)
Calculating the result:
K.E. ≈ -2.07 x 10^3 eV
Note that the negative sign indicates a decrease in kinetic energy.
To convert the kinetic energy to joules, we can use the conversion factor:
1 eV = 1.602 x 10^-19 J
Multiplying the kinetic energy by the conversion factor:
K.E. ≈ (-2.07 x 10^3 eV) * (1.602 x 10^-19 J/eV)
Calculating the result:
K.E. ≈ -3.32 x 10^-16 J
Therefore, the kinetic energy of the scattered electron is approximately -3.32 x 10^-16 J.
f. The speed of the scattered electron can be found using the relativistic energy-momentum relationship:
E = sqrt((m_e * c^2)^2 + (p * c)^2)
where:
E is the energy of the scattered electron
m_e is the mass of the electron (9.10938356 x 10^-31 kg)
c is the speed of light (3 x 10^8 m/s)
p is the momentum of the scattered electron
Since the speed of the electron is much less than the speed of light, we can assume its relativistic mass is its rest mass, and the equation simplifies to: E ≈ m_e * c^2
Rearranging the equation to solve for c: c ≈ E / (m_e * c^2)
Substituting the values: c ≈ (-3.32 x 10^-16 J) / ((9.10938356 x 10^-31 kg) * (3 x 10^8 m/s)^2)
Calculating the result: c ≈ -3.86 x 10^5 m/s
Therefore, the speed of the scattered electron is approximately -3.86 x 10^5 m/s.
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what kind are ray diagram is this. pls identify it
Letter A is the plane surface
Letter B is the incident ray
Letter C is the reflected ray.
What are the terms of the ray diagram?The terms of the ray diagram is illustrated as follows;
(i) This arrow indicates the incident ray, which is known as the incoming ray.
(ii) This arrow indicates the normal, a perpendicular line to the plane of incidence.
(iii) This arrow indicates the reflected ray; the out going arrow.
(iv) This the angle of incident or incident angle.
(v) This is the reflected angle or angle of reflection.
Thus, based on the given letters, we can match them as follows;
Letter A is the plane surface (surface containing the incident, reflected rays)
Letter B is the incident ray
Letter C is the reflected ray.
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The figure below shows a horizontal pipe with a varying cross section. A liquid with a density of 1.65 g/cm3 flows from left to right in the pipe, from larger to smaller cross section. The left side's cross-sectional area is 10.0 cm2, and while in this side, the speed of the liquid is 2.73 m/s, and the pressure is 1.20 ✕ 105 Pa. The right side's cross sectional-area is 3.00 cm2. The flow within a horizontal tube is depicted by five lines. The tube extends from left to right, with the left end wider than the right end. The five lines start at the left end, go horizontally to the right, curve slightly toward the center of the tube such that all five lines come closer together, and again go horizontally to the right to exit at the right end. Arrows on the lines point to the right to represent the direction of flow. (a) What is the speed (in m/s) of the liquid in the right side (the smaller section)? (Enter your answer to at least three significant figures.) m/s (b) What is the pressure (in Pa) of the liquid in the right side (the smaller section)? Pa
a) The speed of the liquid on the right side (the smaller section) is 9.54 m/s.
b) The pressure of the liquid on the right side (the smaller section) is 3.49 x [tex]10^5[/tex] Pa.
The mass of liquid flowing through a horizontal pipe is constant. As a result, the mass of fluid entering section A per unit time is the same as the mass of fluid exiting section B per unit time. Conservation of mass may be used to write this.ρ1A1v1 = ρ2A2v2The pressure difference between A and B, as well as the height difference between the two locations, results in a change in pressure from A to B. As a result, we have the Bernoulli's principle:
P1 + ρgh1 + 1/2 ρ[tex]v1^2[/tex]
= P2 + ρgh2 + 1/2 ρ[tex]v2^2[/tex]
Substitute the given values:
P1 + 1.20 ✕ 105 Pa + 1/2 pv [tex]1^2[/tex]
= P2 + 1/2 ρ[tex]v2^2[/tex]ρ1v1A1
= ρ2v2A2
We can rewrite the equation in terms of v2 and simplify:
P2 = P1 + 1/2 ρ([tex]v1^2[/tex] - [tex]v2^2[/tex])P2 - P1
= 1/2 ρ([tex]v1^2[/tex] - [tex]v2^2[/tex])
Substitute the given values:
P2 - 1.20 ✕ 105 Pa
= 1/2 [tex](1.65 g/cm3)(2.73 m/s)^2[/tex] - [tex](9.54 m/s)^2[/tex])
= 3.49 x [tex]10^5[/tex] Pa
The velocity of the fluid in the right side (the smaller section) can be found using the above formula.
P2 - P1 = 1/2 ρ([tex]v1^2[/tex] - [tex]v2^2[/tex])
Substitute the given values:
3.49 x [tex]10^5[/tex] Pa - 1.20 ✕ 105 Pa
= 1/2 [tex](1.65 g/cm3)(2.73 m/s)^2[/tex] - [tex]v2^2[/tex])
= 9.54 m/s
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A circuit has a resistor, an inductor and a battery in series. The battery is a 10 Volt battery, the resistance of the coll is negligible, the resistor has R = 500 m, and the coil inductance is 20 kilo- Henrys. The circuit has a throw switch to complete the circuit and a shorting switch that cuts off the battery to allow for both current flow and interruption a. If the throw switch completes the circuit and is left closed for a very long time (hours?) what will be the asymptotic current in the circuit? b. If the throw switch is, instead switched on for ten seconds, and then the shorting switch cuts out the battery, what will the current be through the resistor and coil ten seconds after the short? (i.e. 20 seconds after the first operation.) C. What will be the voltage across the resistor at time b.?
a. After the throw switch is closed for a very long time, the circuit will reach a steady-state condition. In this case, the inductor behaves like a short circuit and the asymptotic current will be determined by the resistance alone. Therefore, the asymptotic current in the circuit can be calculated using Ohm's Law: I = V/R, where V is the battery voltage and R is the resistance.
b. When the throw switch is closed for ten seconds and then the shorting switch cuts out the battery, the inductor builds up energy in its magnetic field. After the battery is disconnected, the inductor will try to maintain the current flow, causing the current to gradually decrease. The current through the resistor and coil ten seconds after the short can be calculated using the equation for the discharge of an inductor: I(t) = I(0) * e^(-t/τ), where I(t) is the current at time t, I(0) is the initial current, t is the time elapsed, and τ is the time constant of the circuit.
a. When the circuit is closed for a long time, the inductor behaves like a short circuit as it offers negligible resistance to steady-state currents. Therefore, the current in the circuit will be determined by the resistance alone. Applying Ohm's Law, the asymptotic current can be calculated as I = V/R, where V is the battery voltage (10V) and R is the resistance (500Ω). Thus, the asymptotic current will be I = 10V / 500Ω = 0.02A or 20mA.
b. When the throw switch is closed for ten seconds and then the shorting switch cuts out the battery, the inductor builds up energy in its magnetic field. After the battery is disconnected, the inductor will try to maintain the current flow, causing the current to gradually decrease. The time constant (τ) of the circuit is given by the equation τ = L/R, where L is the inductance (20 kH) and R is the resistance (500Ω). Calculating τ, we get τ = (20,000 H) / (500Ω) = 40s. Using the equation for the discharge of an inductor, I(t) = I(0) * e^(-t/τ), we can calculate the current at 20 seconds as I(20s) = I(0) * e^(-20s/40s) = I(0) * e^(-0.5) ≈ I(0) * 0.6065.
c. The voltage across the resistor can be calculated using Ohm's Law, which states that V = I * R, where V is the voltage, I is the current, and R is the resistance. In this case, we already know the current through the resistor at 20 seconds (approximately I(0) * 0.6065) and the resistance is 500Ω. Therefore, the voltage across the resistor can be calculated as V = (I(0) * 0.6065) * 500Ω.
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Captain Proton confronts the flatulent yet eerily floral Doctor Yango in his throne room. Doctor
Yango is clutching his Rod of Command as Captain Proton pushes him over the edge of the
Throne Room balcony, right out into that 17 T magnetic field surrounding the Palace of Evil.
Doctor Yango activates his emergency escape rocket and flies off at 89.7 m/s. Assuming that the
Rod is conductive, 0.33 m long, and held perpendicular to the field, determine the voltage
generated in the Rod as Doctor Yango flies off.
The voltage generated in the Rod as Doctor Yango flies off is approximately 514 volts.
As we know, the voltage induced in a conductor moving through a magnetic field is given by this formula;
v = Bl
voltage induced = magnetic field × length of conductor × velocity
Now, substituting the values given in the question;
v = (17 T) (0.33 m) (89.7 m/s) = 514 T⋅m/s ≈ 514 V
Therefore, the voltage generated in the Rod as Doctor Yango flies off is approximately 514 volts.
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Pelicans tuck their wings and free-fall straight down Part A when diving for fish. Suppose a pelican starts its dive from a height of 20.0 m and cannot change its If it takes a fish 0.20 s to perform evasive action, at what minimum height must it path once committed. spot the pelican to escape? Assume the fish is at the surface of the water. Express your answer using two significant figures.
the minimum height at which it must spot the pelican to escape is approximately 2.02 s * 0.20 s = 0.404 m, which can be rounded to 0.40 mTo determine the minimum height at which the fish must spot the pelican to escape, we can use the equations of motion. The time it takes for the pelican to reach the surface of the water can be calculated using the equation:
h = (1/2) * g * t^2,
where h is the initial height of 20.0 m, g is the acceleration due to gravity (approximately 9.8 m/s^2), and t is the time taken by the pelican to reach the surface.
Rearranging the equation to solve for t, we have:
t = sqrt(2h / g).
Substituting the given values into the equation, we get:
t = sqrt(2 * 20.0 m / 9.8 m/s^2) ≈ 2.02 s.
Since the fish has only 0.20 s to perform evasive action, the minimum height at which it must spot the pelican to escape is approximately 2.02 s * 0.20 s = 0.404 m, which can be rounded to 0.40 m (two significant figures).
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A uniform magnetic field points directly into this page. A group of protons are moving toward the top of the page. What can you say about the magnetic force acting on the protons? A. toward the right B. toward the left C. toward the top of the page D. toward the bottom of the page E. directly into the page F. directly out of the page
According to the rule, the magnetic force will be directed toward the left. The correct answer is B. toward the left.
The direction of the magnetic force acting on a charged particle moving in a magnetic field can be determined using the right-hand rule for magnetic forces.
According to the rule, if the right-hand thumb points in the direction of the particle's velocity, and the fingers point in the direction of the magnetic field, then the palm will face in the direction of the magnetic force.
In this case, the protons are moving toward the top of the page, which means their velocity is directed toward the top. The uniform magnetic field points directly into the page. Applying the right-hand rule, we point our right thumb toward the top of the page to represent the velocity of the protons.
Then, we extend our right fingers into the page to represent the direction of the magnetic field. According to the right-hand rule, the magnetic force acting on the protons will be directed toward the left, which corresponds to answer option B. toward the left.
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A transverse sinusoidal wave on a wire is moving in the direction is speed is 10.0 ms, and its period is 100 m. Att - a colored mark on the wrotx- has a vertical position of 2.00 mod sowo with a speed of 120 (6) What is the amplitude of the wave (m) (6) What is the phase constant in rad? rad What is the maximum transversed of the waren (wite the wave function for the wao. (Use the form one that and one om and sons. Do not wcase units in your answer. x- m
The amplitude of the wave is 2.00 m. The phase constant is 0 rad. The maximum transverse displacement of the wire can be determined using the wave function: y(x, t) = A * sin(kx - ωt), where A is the amplitude, k is the wave number, x is the position, ω is the angular frequency, and t is the time.
The given vertical position of the colored mark on the wire is 2.00 m. In a sinusoidal wave, the amplitude represents the maximum displacement from the equilibrium position. Therefore, the amplitude of the wave is 2.00 m.
The phase constant represents the initial phase of the wave. In this case, the phase constant is given as 0 rad, indicating that the wave starts at the equilibrium position.
To determine the maximum transverse displacement of the wire, we need the wave function. However, the wave function is not provided in the question. It would be helpful to have additional information such as the wave number (k) or the angular frequency (ω) to calculate the maximum transverse displacement.
Based on the given information, we can determine the amplitude of the wave, which is 2.00 m. The phase constant is given as 0 rad, indicating that the wave starts at the equilibrium position. However, without the wave function or additional parameters, we cannot calculate the maximum transverse displacement of the wire.
In this problem, we are given information about a transverse sinusoidal wave on a wire. We are provided with the speed of the wave, the period, and the vertical position of a colored mark on the wire. From this information, we can determine the amplitude and the phase constant of the wave.
The amplitude of the wave represents the maximum displacement from the equilibrium position. In this case, the amplitude is given as 2.00 m, indicating that the maximum displacement of the wire is 2.00 m from its equilibrium position.
The phase constant represents the initial phase of the wave. It indicates where the wave starts in its oscillatory motion. In this case, the phase constant is given as 0 rad, meaning that the wave starts at the equilibrium position.
To determine the maximum transverse displacement of the wire, we need the wave function. Unfortunately, the wave function is not provided in the question. The wave function describes the spatial and temporal behavior of the wave and allows us to calculate the maximum transverse displacement at any given position and time.
Without the wave function or additional parameters such as the wave number (k) or the angular frequency (ω), we cannot calculate the maximum transverse displacement of the wire or provide the complete wave function.
It is important to note that units should be included in the final answer, but they were not specified in the question.
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A circular loop of wire (radius = 6.0 cm, resistance = 40 mΩ ) is placed in a uniform magnetic field making an angle of 30∘ with the plane of the loop. The magnitude of the field changes with time according to B = 30 sin (20t) mT, where t is measured in s. Determine the magnitude of the emf induced in the loop at t = π/20 s.
The magnitude of the induced emf in the loop at t = π/20 s is zero.
To determine the magnitude of the induced emf in the loop, we can use Faraday's law of electromagnetic induction, which states that the induced emf in a loop is equal to the rate of change of magnetic flux through the loop.
The magnetic flux (Φ) through the loop can be calculated using the formula:
Φ = B × A × cosθ
where: B is the magnetic field strength,
A is the area of the loop,
and θ is the angle between the magnetic field and the plane of the loop.
Given: Radius of the loop (r) = 6.0 cm = 0.06 m
Resistance of the loop (R) = 40 mΩ = 0.04 Ω
Magnetic field strength (B) = 30 sin(20t) mT
Angle between the field and the loop (θ) = 30°
At t = π/20 s, we can substitute this value into the equation to calculate the induced emf.
First, let's calculate the area of the loop:
A = πr²
A = π(0.06 m)²
A ≈ 0.0113 m²
Now, let's calculate the magnetic flux at t = π/20 s:
Φ = (30 sin(20 × π/20)) mT × 0.0113 m² × cos(30°)
Φ ≈ 0.0113 × 30 × sin(π) × cos(30°)
Φ ≈ 0.0113 × 30 × 0 × cos(30°)
Φ ≈ 0
Since the magnetic flux is zero, the induced emf in the loop at t = π/20 s is also zero.
Therefore, the magnitude of the induced emf in the loop at t = π/20 s is zero.
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What is the angular momentum LA if rA = 4, −6, 0 m and p = 11,
15, 0 kg · m/s? (Express your answer in vector form.)
The angular momentum LA if rA = 4, −6, 0 m and p = 11,15, 0 kg · m/s is LA= (-90i+44j+15k) kg.m^2/s.
The formula for the angular momentum is L = r x p where r and p are the position and momentum of the particle respectively.
We can write the given values as follows:
rA = 4i - 6j + 0k (in m)
p = 11i + 15j + 0k (in kg.m/s)
We can substitute the values of rA and p in the formula for L and cross-multiply using the determinant method.
Therefore, L = r x p = i j k 4 -6 0 11 15 0 = (-90i + 44j + 15k) kg.m^2/s where i, j, and k are unit vectors along the x, y, and z axes respectively.
Thus, the angular momentum LA is (-90i+44j+15k) kg.m^2/s in vector form.
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If you draw a few electric field lines and equipotential surfaces outside a negatively charged hollow conducting sphere, what will be the shape of the equipotential surfaces? ! circle
semicircle Sphere hemisphere
The shape of the equipotential surfaces outside a negatively charged hollow conducting sphere will be spherical.
When considering a negatively charged hollow conducting sphere, the excess negative charge will distribute itself uniformly on the outer surface of the sphere. Due to this uniform charge distribution, the electric field inside the hollow region of the sphere is zero.
For points outside the sphere, the electric field lines will originate from the negative charge on the surface of the sphere and will extend radially outward. Since the electric field lines are perpendicular to the equipotential surfaces, the equipotential surfaces will be perpendicular to the electric field lines.
In a spherically symmetric system, the equipotential surfaces are concentric spheres centered at the origin. Therefore, the equipotential surfaces outside the negatively charged hollow conducting sphere will be spherical in shape.
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A disk of mass 2 Kg and radius 60 cm is at rest and is allowed to spin freely about its center. A force of 50 N acts tangent to the edge of the wheel during 12 seconds. a- If the disk was initially at rest, what is its angular angular velocity after the action of the applied force ? b- Use the Work - Energy Theorem to calculate the angular displacement.
Given the following information: Mass of disk (m) = 2 Kg.
The radius of the disk (r) = 60 cm
Force applied (F) = 50 N
Time (t) = 12 seconds
Initial angular velocity (ωi) = 0
Find out the final angular velocity (ωf) and angular displacement (θ) of the disk.
a) The torque produced by the force is given as: T = F × r
where, T = torque, F = force, and r = radius of the disk
T = 50 N × 60 cm = 3000 Ncm
The angular acceleration (α) produced by the torque is given as:
α = T / I where, I = moment of inertia of the disk.
I = (1/2) × m × r² = (1/2) × 2 kg × (60 cm)² = 0.36 kgm²α = 3000 Ncm / 0.36 kgm² = 8333.33 rad/s².
The final angular velocity (ωf) of the disk is given as:
ωf = ωi + α × t
because the disk was initially at rest,
ωi = 0ωf = 0 + 8333.33 rad/s² × 12 sωf = 100000 rad/s.
Thus, the angular velocity of the disk is 100000 rad/s.
b)The work done (W) by the force is given as W = F × d
where d = distance traveled by the point of application of the force along the circumference of the disk
d = 2πr = 2 × 3.14 × 60 cm = 376.8 cm = 3.768 mW = 50 N × 3.768 m = 188.4 J.
The kinetic energy (Kf) of the disk after 12 seconds is given as:
Kf = (1/2) × I × ωf²Kf = (1/2) × 0.36 kgm² × (100000 rad/s)²Kf = 1.8 × 10¹² J
By the Work-Energy Theorem, we have:Kf - Ki = W
where, Ki = initial kinetic energy of the disk
Ki = (1/2) × I × ωi² = 0
Rearrange the above equation to find out the angular displacement (θ) of the disk.
θ = (Kf - Ki) / Wθ = Kf / Wθ = 1.8 × 10¹² J / 188.4 Jθ = 9.54 × 10⁹ rad.
Thus, the angular displacement of the disk is 9.54 × 10⁹ rad.
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Answer the following - show your work! (5 marks): Maximum bending moment: A simply supported rectangular beam that is 3000 mm long supports a point load (P) of 5000 N at midspan (center). Assume that the dimensions of the beams are as follows: b= 127 mm and h = 254 mm, d=254mm. What is the maximum bending moment developed in the beam? What is the overall stress? f = Mmax (h/2)/bd3/12 Mmax = PL/4
The maximum bending moment developed in the beam is 3750000 N-mm. The overall stress is 4.84 MPa.
The maximum bending moment developed in a beam is equal to the force applied to the beam multiplied by the distance from the point of application of the force to the nearest support.
In this case, the force is 5000 N and the distance from the point of application of the force to the nearest support is 1500 mm. Therefore, the maximum bending moment is:
Mmax = PL/4 = 5000 N * 1500 mm / 4 = 3750000 N-mm
The overall stress is equal to the maximum bending moment divided by the moment of inertia of the beam cross-section. The moment of inertia of the beam cross-section is calculated using the following formula:
I = b * h^3 / 12
where:
b is the width of the beam in mm
h is the height of the beam in mm
In this case, the width of the beam is 127 mm and the height of the beam is 254 mm. Therefore, the moment of inertia is:
I = 127 mm * 254 mm^3 / 12 = 4562517 mm^4
Plugging in the known values, we get the following overall stress:
f = Mmax (h/2) / I = 3750000 N-mm * (254 mm / 2) / 4562517 mm^4 = 4.84 MPa
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