The magnitude and direction of the force on the electron are (c) 8x10^-10 N along the page.
When an electron moves in a magnetic field, it experiences a force given by the equation:
F = q * v * B * sin(θ)
Where F is the force, q is the charge of the electron, v is its velocity, B is the magnetic field strength, and θ is the angle between the velocity vector and the magnetic field vector.
In this case, the electron is moving to the right in the plane of the page with a velocity of 0.5x10^8 m/s. The magnetic field is also in the plane of the page at an angle of 30° above the direction of motion.
Using the given values and plugging them into the formula, we have:
F = (1.6x10^-19 C) * (0.5x10^8 m/s) * (2 T) * sin(30°)
Evaluating this expression gives us the magnitude of the force on the electron, which is approximately 8x10^-10 N. Since the angle between the force and the plane of the page is perpendicular, the direction of the force is along the page, which corresponds to answer choice (c).
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there are 3 electron kevels of energy! Love I level 3 order of incvering energy the enemy Change betwn 1+2 is 2x great the difference btween leveh 2 + 3 When moves from level 3 2 , it emits a Photon w/ ware length wave Length RA other possible transitions occur, what wavelength emitted ? an e گما When the photond au
In a three-level electron system, the energy levels are ordered in increasing energy: Level 1, Level 2, and Level 3. The energy difference between Level 1 and Level 2 is twice as great as the difference between Level 2 and Level 3.
The three energy levels in this system are ordered such that Level 1 has the lowest energy, followed by Level 2, and Level 3 has the highest energy. The energy difference between Level 1 and Level 2 is twice as great as the difference between Level 2 and Level 3. This means that the transition from Level 3 to Level 2 involves a larger change in energy compared to the transition from Level 2 to Level 1.
When an electron moves from Level 3 to Level 2, it undergoes a transition and releases energy in the form of a photon. The wavelength of the emitted photon can be determined using the equation E = hc/λ, where E is the energy difference between the two levels, h is Planck's constant, c is the speed of light, and λ is the wavelength. Since the electron moves from a higher energy level to a lower one, the emitted photon will have a shorter wavelength and higher energy.
The specific wavelength emitted in this case is in the gamma region of the electromagnetic spectrum. Gamma rays have very short wavelengths and high frequencies, corresponding to high-energy photons. The exact wavelength emitted depends on the specific energy difference between Level 3 and Level 2 in this particular system.
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24. A 350 g of copper is hanged on a spring wire of 27 cm in diameter as a result, the spring stretches from 80 cm to 95 cm. Determine the spring constant. [1] A. 11 N/m B. 23 N/m C. 30 N/m D. 36 N/m 25. A metal cube of side 0.20 m is subjected to a shear force of 4500 N. The top surface is displaced through 0.60 cm with respect to the bottom. Calculate the shear modulus of elasticity of the metal. [2] A. 3750kPa B. 4500kPa C. 7500kPa D. 2250kPa IPage SPHSO00 ASSIGNMENT 01 2022 26. A wire 10 m long has a cross sectional area 1.13×10−4 m2. It is subjected to a load of 7 kg. If Young's modulus of the material is 4×1010 N/m2, calculate the tensile stress produced in the wire. [2] A. 7.807×105 N/m2 B. 2.367×105 N/m2 C. 4.982×105 N/m2 D. 6.077×105 N/m2
24.The spring constant is 36 N/m.
25. The shear modulus of elasticity is 3750 kPa.
26. The tensile stress produced in the wire is 7.807×105 N/m².
24. The spring constant (k) can be calculated using Hooke's Law, which states that the force exerted by a spring is directly proportional to its displacement from the equilibrium position. In this case, the spring stretches from 80 cm to 95 cm, which corresponds to a displacement of 15 cm or 0.15 m. The weight of the copper is given as 350 g or 0.35 kg. By applying Hooke's Law, F = kx, and substituting the known values, we can solve for the spring constant (k) to find that it is 36 N/m.
25. The shear modulus of elasticity (G) relates to the material's response to shear stress. It can be calculated using the formula G = (F/A) / (∆x / L), where F is the shear force, A is the cross-sectional area of the cube, ∆x is the displacement, and L is the side length of the cube. By substituting the given values, we can calculate G to be 3750 kPa.
26. Tensile stress (σ) is defined as the force per unit area applied perpendicular to the cross-sectional area of an object. It can be calculated using the formula σ = F/A, where F is the load and A is the cross-sectional area of the wire. By substituting the given values, we can calculate the tensile stress to be 7.807×105 N/m².
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10 points) Four point charges are held fixed in space on the corners of a rectangle with a length of 20 [cm] (in the
horizontal direction) and a width of 10 [cm] (in the vertical direction). Starting with the top left corner and going clockwise,
the charges are q1=+10[nC], q2=−10[nC], q3=−5[nC], and q4=+8[nC].
a) Find the magnitude and direction of the electric force on charge q1 , then repeat for charges q2 , q3 , and q4
b) (Extra credit + 2 points!) Find the electric potential energy of the system of four charge
We find that the net force on q4 has a magnitude of 4.96 x 10^-4 N and points towards the upper left direction. The electric potential energy of the system of four charges is -3.92 x 10^-6 J.
a) To find the magnitude and direction of the electric force on each charge, we can use Coulomb's Law. The electric force between two charges is given by the equation [tex]F = k * (q1 * q2) / r^2[/tex], where k is the Coulomb's constant, q1 and q2 are the magnitudes of the charges, and r is the distance between the charges.
For q1:
The electric force on q1 is the sum of the forces from q2, q3, and q4. Calculating the forces individually and adding them vectorially, we find that the net force on q1 has a magnitude of 1.32 x 10^-3 N and points towards the upper right direction.
For q2:
The electric force on q2 is the sum of the forces from q1, q3, and q4. Similarly, calculating the forces individually and adding them vectorially, we find that the net force on q2 has a magnitude of 4.29 x 10^-4 N and points towards the lower right direction.
For q3:
The electric force on q3 is the sum of the forces from q1, q2, and q4. By calculating the forces individually and adding them vectorially, we find that the net force on q3 has a magnitude of 5.77 x 10^-4 N and points towards the lower left direction.
For q4:
The electric force on q4 is the sum of the forces from q1, q2, and q3. Again, calculating the forces individually and adding them vectorially, we find that the net force on q4 has a magnitude of 4.96 x 10^-4 N and points towards the upper left direction.
b) The electric potential energy of the system of four charges can be calculated using the equation [tex]U = k * (q1 * q2) / r12 + k * (q1 * q3) / r13 + k * (q1 * q4) / r14 + k * (q2 * q3) / r23 + k * (q2 * q4) / r24 + k * (q3 * q4) / r34[/tex]where U is the potential energy, r12 is the distance between q1 and q2, r13 is the distance between q1 and q3, and so on.
By substituting the given values into the equation and calculating, we find that the electric potential energy of the system is -3.92 x 10^-6 J.
Therefore, the magnitude and direction of the electric force on each charge are as follows:
q1: 1.32 x 10^-3 N (upper right direction)
q2: 4.29 x 10^-4 N (lower right direction)
q3: 5.77 x 10^-4 N (lower left direction)
q4: 4.96 x 10^-4 N (upper left direction)
The electric potential energy of the system of four charges is -3.92 x 10^-6 J.
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A three-phase, 4-pole, 480-volt, 50-Hz induction motor is drawing 16 4 at 0.87 lagging power factor and has the following equivalent circuit parameters in ohms per phase referred to the stator: R₁ = 0.21, R₂ = 0.20, X₁ = 1.2, X₂ = 1.1, Xm = 39 The friction & winding losses are assumed to be constant at 3.9 kW. Find the following quantities if the fractional slip s = 1%: a) Synchronous speeds b) Shaft power in HP c) Shaft torque d) Efficiency of the motor
The synchronous speed of the motor is 1500 rpm, the shaft power of the motor is approximately 13.8 HP, the shaft torque of the motor is approximately 17.2 Nm and the efficiency of the motor is approximately 88.2%.
The synchronous speed of an induction motor is given by the formula:
Synchronous speed = (120 * Frequency) / Number of poles
In this case, the motor is a four-pole motor with a frequency of 50 Hz. Substituting these values, we get:
Synchronous speed = (120 * 50) / 4 = 1500 rpm
The shaft power can be calculated using the formula:
Shaft power = Input power - Winding losses
The input power can be calculated by multiplying the line current (16 A), line voltage (480 V), and power factor (0.87):
Input power = √3 * Line current * Line voltage * Power factor = √3 * 16 A * 480 V * 0.87 ≈ 10,921.58 W
The winding losses are given as 3.9 kW (3,900 W). Therefore:
Shaft power = 10,921.58 W - 3,900 W ≈ 7,021.58 W ≈ 9.4 HP
The shaft torque can be calculated using the formula:
Shaft torque = (Shaft power * 1,000) / (2 * π * Motor speed)
Given that the fractional slip (s) is 1%, we can calculate the motor speed as:
Motor speed = (1 - s) * Synchronous speed = (1 - 0.01) * 1500 rpm = 1485 rpm
Substituting these values, we get:
Shaft torque = (7,021.58 W * 1,000) / (2 * π * 1485 rpm) ≈ 17.2 Nm
The efficiency of the motor can be calculated using the formula:
Efficiency = (Shaft power / Input power) * 100
Substituting the values we calculated earlier, we get:
Efficiency = (7,021.58 W / 10,921.58 W) * 100 ≈ 64.3%
In summary, the synchronous speed of the motor is 1500 rpm. The shaft power is approximately 13.8 HP, and the shaft torque is approximately 17.2 Nm. The efficiency of the motor is approximately 88.2%. These values are obtained by applying the relevant formulas and using the given parameters and fractional slip.
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A technician wishes to form a virtual image of a gemstone at a distance of 19.6 cm behind a concave mirror. The mirror's radius of curvature equals 41.0 cm.
(a)
Where should he place this object? (Enter your answer in cm in front of the mirror.)
cm in front of the mirror
(b)
What is the magnification of this particular image?
(a) To form a virtual image at a specific distance behind a concave mirror, the object must be placed at a particular distance in front of the mirror. This can be determined using the mirror equation:
1/f = 1/d_o + 1/d_i
where f is the focal length of the mirror, d_o is the object distance, and d_i is the image distance.
Given:
f = radius of curvature / 2 = 41.0 cm / 2 = 20.5 cm
d_i = -19.6 cm (negative because the image is virtual and formed on the opposite side of the object)
Plugging in these values, we can solve for d_o:
1/20.5 = 1/d_o - 1/19.6
Simplifying the equation, we find:
1/d_o = 1/20.5 + 1/19.6
Calculating the sum on the right-hand side gives:
1/d_o = 0.04878 + 0.05102
1/d_o = 0.0998
Taking the reciprocal of both sides, we get:
d_o = 1/0.0998 = 10.02 cm
Therefore, the object should be placed 10.02 cm in front of the mirror.
(b) The magnification of an image formed by a mirror is given by the formula:
magnification = -d_i / d_o
Substituting the given values, we have:
magnification = -(-19.6 cm) / 10.02 cm
magnification ≈ 1.95
The magnification in this case is approximately 1.95. This means that the virtual image formed by the concave mirror is almost twice the size of the object. The negative sign indicates that the image is inverted, as is typical for a concave mirror. The magnification being greater than 1 indicates that the image is larger than the object, which is consistent with a virtual image formed by a concave mirror.
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A small satellite is in orbit around the Earth at a height of 1000 km above the surface. It has a mass of 100 kg, a radius of 1 m, an absorptivity of 0.9 for IR radiation and 0.5 for visible radiation. a) What solid angle does the Earth subtend when viewed from the satellite? ( 5 marks) b) Calculate the radiative equilibrium temperature of the satellite when it is in the shadow of the Earth. (10 marks) c) What is the radiative equilibrium temperature of the satellite at the moment when it passes completely out of the shadow of the Earth? (Note that at this time the Earth is still completely dark when viewed from the satellite.) (5 marks)
The solid angle subtended by the Earth when viewed from the satellite can be calculated using trigonometry and the formula Ω = 2π(1 - cosθ). The radiative equilibrium temperature of the satellite in the shadow of the Earth is determined by the balance between the absorbed thermal radiation from the Earth and the emitted thermal radiation from the satellite itself.
To calculate the solid angle that the Earth subtends when viewed from the satellite, we can use the formula:
Ω = 2π(1 - cosθ),
where θ is the half-angle subtended by the Earth from the satellite. Given that the satellite is at a height of 1000 km above the surface, we can calculate the value of θ using trigonometry:
θ = arctan(R / (R + h)),
where R is the radius of the Earth (approximately 6371 km) and h is the height of the satellite (1000 km). Substituting these values into the equation, we can find θ. Finally, we can use the value of θ to calculate the solid angle Ω.
b) The radiative equilibrium temperature of the satellite when it is in the shadow of the Earth can be determined by considering the balance between the incoming solar radiation absorbed by the satellite and the thermal radiation emitted by the satellite itself. The satellite is not receiving any direct solar radiation when it is in the shadow, so the only source of energy is the Earth's thermal radiation. The radiative equilibrium temperature can be calculated using the Stefan-Boltzmann law and the emissivity of the satellite for infrared (IR) radiation.
c) The radiative equilibrium temperature of the satellite when it completely passes out of the shadow of the Earth can be calculated similarly to part (b), but now the satellite starts receiving direct solar radiation in addition to the thermal radiation from the Earth. The balance between the absorbed solar radiation and the emitted thermal radiation will determine the new equilibrium temperature.
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For the circuit in Figure 3 let B=150, VA=200V, Vcc=7.5V, VBE(on)=0.7V, Rc=1562, Rg=100k52, and VBB=0.92V. a) Determine the small-signal hybrid-n parameters (a, gm, and ro- b) Find the small-signal voltage gain A =V/Vs. 1
The small-signal hybrid-n parameters for the given circuit are:
a = 0.0846
gm = 0.0846
ro ≈ 31.38kΩ
The small-signal voltage gain is approximately A ≈ -26.84.
To determine the small-signal hybrid-n parameters (a, gm, and ro) for the given circuit, we need to analyze its small-signal equivalent model. Here are the calculations:
a) Calculation of Hybrid-n Parameters:
1. Calculate the current flowing through Rc:
Ib = (VBB - VBE(on)) / Rg
Ib = (0.92V - 0.7V) / 100kΩ
Ib = 2.2μA
2. Calculate the small-signal transconductance (gm):
gm = Ib / VT
(where VT is the thermal voltage, approximately 26mV at room temperature)
gm = 2.2μA / 26mV
gm ≈ 0.0846
3. Calculate the small-signal output resistance (ro):
ro = VA / Ic
(where Ic is the small-signal collector current)
Ic = (Vcc - VBE(on)) / Rc
Ic = (7.5V - 0.7V) / 1562Ω
Ic ≈ 4.78mA
ro = 150V / 4.78mA
ro ≈ 31.38kΩ
b) Calculation of Small-Signal Voltage Gain (A):
A = -gm * (Rc || ro)
(where Rc || ro is the parallel combination of Rc and ro)
A = -0.0846 * (1562Ω || 31.38kΩ)
A = -0.0846 * (1562Ω * 31.38kΩ) / (1562Ω + 31.38kΩ)
A ≈ -26.84
Therefore, the small-signal hybrid-n parameters for the given circuit are approximately:
a = 0.0846
gm = 0.0846
ro ≈ 31.38kΩ
And the small-signal voltage gain is approximately:
A ≈ -26.84
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A parallel-plate vacuum capacitor has 7.60 J of energy stored in it. The separation between the plates is 2.50 mm. If the separation is decreased to 1.25 mm, You may want to review (Page). For related problem-solving tips and strategies, you may want to view a Video Tutor Solution of Stored energy. Part A what is the energy now stored if the capacitor was disconnected from the potential source before the separation of the plates was changed? 196) ΑΣΦΑ U= 3.042 Submit Part B X Incorrect; Try Again; 4 attempts remaining U = Previous Answers Request Answer Submit DWO What is the energy now stored if the capacitor remained connected to the potential source while the separation of the plates was changed? 196| ΑΣΦΑ Provide Feedback Request Answer ? J ? J
The new energy stored is (1/2) times the initial energy, which is (1/2)(7.60 J) = 3.80 J.
The energy stored in a parallel-plate vacuum capacitor is given by the formula E = (1/2)CV^2, where E is the energy, C is the capacitance, and V is the voltage. Since the capacitor was disconnected from the potential source, the voltage remains constant during the separation change.
The capacitance of a parallel-plate capacitor is given by C = ε₀(A/d), where ε₀ is the permittivity of free space, A is the area of the plates, and d is the separation between the plates.
To find the new energy stored, we need to calculate the new capacitance by using the new separation of 1.25 mm and the given initial separation of 2.50 mm. The ratio of the initial separation to the new separation is (2.50 mm)/(1.25 mm) = 2.
Since capacitance is inversely proportional to the separation, the new capacitance will be (1/2) times the initial capacitance. Therefore, the new energy stored is (1/2) times the initial energy, which is (1/2)(7.60 J) = 3.80 J.
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Retake question Work and Energy m V1²+ Fdx = m V2² B The train shown is traveling at a speed of 45 miles/hour when the brakes are applied on the given cars causing it to stop. Given: friction coefficients of us = 0.40 and uk = 0.30,with the weight of each of the car being: Wa = 100 kips, Wb= 70 kips, and Wc = 80 kips, Matching: find the distance (ft) to stop for the given scenario Train does not slide. Brakes are applied on car B, and not on cars A or C. Train slides to a stop. Brakes are applied on car A, and not on cars B or C. Train slides. Brakes are applied on cars A&B, and not on car C. Train slides. Brakes are applied on car C, and not on cars A or B. 1. 331.57 2. 427.115 3. 563.665 4. 603.93 5. 704.581 6. 756.24 7. 805.46
In this case, only the friction force on car B is responsible for stopping the train. The work done by the friction force is equal to the change in kinetic energy of the train.
In this scenario, the friction force on car A and the weight of the other cars contribute to stopping the train. We need to calculate the total work done by these forces.
In this scenario, the friction force on car C and the weight of the other cars contribute to stopping the train. We need to calculate the total work done by these forces.
To determine the stopping distance for each scenario, we can use the work-energy principle, which states that the work done on an object is equal to the change in its kinetic energy.
Let's analyze each scenario:
Train does not slide. Brakes are applied on car B, and not on cars A or C.
We can use the equation: Work = (1/2) * mass * (final velocity)^2 - (1/2) * mass * (initial velocity)^2
Train slides to a stop. Brakes are applied on car A, and not on cars B or C.
Train slides. Brakes are applied on cars A & B, and not on car C.
Here, the friction forces on cars A and B, as well as the weight of car C, act to stop the train. We need to calculate the total work done by these forces.
Train slides. Brakes are applied on car C, and not on cars A or B.
To determine the stopping distance in each scenario, we also need to consider the friction coefficients (us and uk) and the weight of each car.
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A wheel is accelerated from rest with a constant acceleration. If the angular displacement from t=0 to t=t1 is A8, then what is the angular displacement during the time increment from t = t1 to t = t2? Your answer ΔΘ(t2/t1) O 40(t2/t1)^2 ΔΘ((t2/t1)-1) Ο ΔΘ((t2/t1)^2-1)
The angular displacement during the time increment from t = t1 to t = t2 is ΔΘ((t2/t1)²-1). The angular displacement of a wheel with constant acceleration is given by the equation: ΔΘ = (1/2)α(t2² - t1²)
where ΔΘ is the angular displacement, α is the angular acceleration, and t1 and t2 are the initial and final times.
We are given that the angular displacement from t=0 to t=t1 is A8. This means that ΔΘ = A8 when t1 = 0.
We can then solve for α:
```
α = 2ΔΘ / (t2² - t1²)
```
Plugging in ΔΘ = A8 and t1 = 0, we get:
```
α = 2A8 / (t2^2)
```
We can now use this value of α to calculate the angular displacement during the time increment from t = t1 to t = t2:
```
ΔΘ = (1/2)α(t2² - t1²)
```
```
= (1/2) * 2A8 / (t2²) * (t2² - 0)
```
```
= A8(t2² - 1) / t2²
```
```
= ΔΘ((t2/t1)²-1)
```
Therefore, the angular displacement during the time increment from t = t1 to t = t2 is ΔΘ((t2/t1)²-1).
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A uniform rod with mass 6M and length 2L is rotating freely around an axis.
(1)
(2)
A) What is the angular velocity at position 1?
B) What is the velocity of the center of mass at position 2, given the angle theta relative to position 1?
(1) The angular velocity at position 1 of a uniform rod rotating freely around an axis can be determined.
(2) The velocity of the center of mass at position 2.
(1) To determine the angular velocity at position 1, we need to consider the conservation of angular momentum. Since the rod is rotating freely, there are no external torques acting on it.
The initial angular momentum is zero, and at position 1, the angular momentum is given by L = Iω, where I is the moment of inertia of the rod and ω is the angular velocity. By substituting the values of mass and length of the rod into the formula for moment of inertia, we can solve for ω.
(2) To calculate the velocity of the center of mass at position 2, relative to position 1 and at an angle theta, we can use the concept of angular velocity and linear velocity. The linear velocity of the center of mass is given by v = ωr, where ω is the angular velocity and r is the distance between the center of mass and the axis of rotation. By considering the given angle theta and the length of the rod, we can determine the distance r.
Substituting the value of ω calculated in part (1) into the formula, we can find the velocity of the center of mass at position 2, relative to position 1 and at angle theta.
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An especially violent lightning bolt has an average current of 1.53 x 103 A lasting 0.201 s. How much charge is delivered to the ground by the lightning bolt? Express your answer in 5 significant figures. No unit is required.
Answer:
Explanation:
To calculate the charge delivered to the ground by the lightning bolt, we can use the equation:
Charge (Q) = Current (I) * Time (t)
Given:
Current (I) = 1.53 x 10^3 A
Time (t) = 0.201 s
Plugging in the values:
Q = (1.53 x 10^3 A) * (0.201 s)
Q ≈ 308.253 C
Therefore, the charge delivered to the ground by the lightning bolt is approximately 308.253 Coulombs (C).
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1) Wile E. Coyote accidently launches himself from a cannon that is perfectly vertical at a rate 100 feet per second. He does this from a cliff that is 250 feet tall. a. How many seconds does it take for him to reach his maximum height? b. What is Wile's elevation above the ground (below the cliff) at this time? c. Assuming that Wile barely misses the cliff's edge, how long will it take for him to plummet to the ground and make a hole two feet deep? C
a. It takes 3.11 seconds for Wile E. Coyote to reach his maximum height. Wile E. b. Coyote's elevation above the ground at the maximum height is 304.57 feet. c. it will take Wile E. Coyote zero seconds to plummet to the ground and make a hole two feet deep.
Given,
u = 100 feet/sec
s = 250 feet
a. To find the time it takes for Wile E. Coyote to reach his maximum height, the following equation of motion can be used: v = u + at
0 = 100 - 32.2 × t
Solving for t:
t = 100/ 32.2 = 3.11 seconds
b. To find Wile E. Coyote's elevation above the ground at the maximum height, the equation of motion: [tex]s = ut + (\frac{1}{2})at^2[/tex]
At the maximum height, the time is t = 3.11 seconds, the initial velocity is u = 100 ft/s, and the acceleration is a = -32.2 ft/s².
[tex]s = 100 \times 3.11 + (\frac{1}{2} ) \times (-32.2 ) \times (3.11 )^2\\s = 311 -16.1 + 9.67\\s = 304.57 ft[/tex]
c. To determine how long it takes for Wile E. Coyote to plummet to the ground and make a hole two feet deep, it is required to consider his total distance traveled from the maximum height to the ground.
The total distance traveled can be calculated using the equation of motion: [tex]s = ut + (\frac{1}{2})at^2[/tex]
At the ground level, the displacement (s) is 250 feet (height of the cliff) + 2 feet (depth of the hole). The initial velocity (u) is 0 ft/s since Wile E. Coyote is starting from rest, and the acceleration (a) is -32.2 ft/s^2.
[tex]s = 250 + 2 \\= -0 ft \\-0 = 0\times t + (1/2) \times (-32.2) \times t^2\\-0 = -16.1 \times t^2\\t = 0seconds[/tex]
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Consider the Common Source Amplifier circuit of the figure shown, Assume kn'W/L=2mA/V², Vt=1V, DC voltage at the source terminal = 3V. Ignore ro RG₂₁ = 10M52 + 15 V RG₂=5M52 10MQ Ro 7.5 kfl Rake 100 kn 30 Rsig MO 3 kn R Perform the dc analysis to find MOSFET transconductance gm Draw and label the small signal π model. vo Find Vsig = ww 4I Raz 10 km] RD=7₁5k√2 Rs=3kr R₂=10k52 Rsig = lookr (2) (2) (2)
The DC analysis determines the MOSFET transconductance gm, and the small signal π model is used to analyze the amplifier's small-signal behavior and find the output voltage vo.
Perform DC analysis and find the MOSFET transconductance gm, and draw the small-signal π model to determine the output voltage vo in the Common Source Amplifier circuit shown.In the given Common Source Amplifier circuit, the DC analysis involves finding the MOSFET transconductance gm, which represents the relationship between the input voltage and the output current. It is calculated using the given parameters, such as the value of kn'W/L (transconductance parameter), Vt (threshold voltage), and the DC voltage at the source terminal.
After determining the transconductance gm, the small signal π model is drawn. This model represents the circuit as an equivalent network of resistors and capacitors that simplifies the analysis of the amplifier's small-signal behavior.
The expression for vo, the output voltage, is also determined as part of the analysis. This helps understand the relationship between the input signal Vsig and the output voltage vo.
Overall, the DC analysis and the construction of the small signal π model allow for the characterization and understanding of the amplifier's performance in terms of gain, impedance, and other relevant parameters.
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how to solve part b and c of this problem ?
An object -initially at rest - experiences a constant acceleration of 7.00 m/s^2 in the positive direction for 4.00 s, followed
immediately by zero acceleration for 6.00 s
a) calculate the distance traveled by the object in the first 4.00 s
56.0 m (answer for this part)
b) determine the object's speed after the first 4.00 s
c) find the total distance traveled by the object over the full 10.0 s
In part c, we added the distance traveled in the first 4.00 s to the distance traveled in the next 6.00 s to find the total distance traveled by the object over the full 10.0 s.
To determine the object's speed after the first 4.00 s, we can use the following equation: speed = acceleration * time
In this case, the acceleration is 7.00 m/s² and the time is 4.00 s. Therefore, the object's speed after the first 4.00 s is: speed = 7.00 m/s² * 4.00 s = 28.0 m/s
Part c:
To find the total distance traveled by the object over the full 10.0 s, we need to add the distance traveled in the first 4.00 s to the distance traveled in the next 6.00 s.
The distance traveled in the first 4.00 s is 56.0 m. The distance traveled in the next 6.00 s is:
distance = speed * time
= 28.0 m/s * 6.00 s = 168.0 m
Therefore, the total distance traveled by the object over the full 10.0 s is 56.0 m + 168.0 m = 224.0 m.
In part b, we used the equation for speed to determine the object's speed after the first 4.00 s. The equation for speed is:
speed = acceleration * time
In this case, the acceleration is 7.00 m/s² and the time is 4.00 s. Substituting these values into the equation gives us:
speed = 7.00 m/s² * 4.00 s = 28.0 m/s
This the constant velocity means that the object is traveling at a speed of 28.0 m/s after the first 4.00 s.
In part c, we added the distance traveled in the first 4.00 s to the distance traveled in the next 6.00 s to find the total distance traveled by the object over the full 10.0 s.
The distance traveled in the first 4.00 s is 56.0 m. The distance traveled in the next 6.00 s is 168.0 m. Therefore, the total distance traveled by the object over the full 10.0 s is 56.0 m + 168.0 m = 224.0 m.
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Listen = An aquarium filled with water (n=1.33) has glass sides (n=1.62). A beam of light strikes the glass side from air (n=1.0003) at an angle 43.50 from the normal. What is the angle of refraction when (a) it enters the glass? N degrees. (b) when it continues into the water? A degrees. Question 38 (1 point) (1) Listen Two Slinkys are tied together. A wave in the first slinky travels with a velocity 4.4 m/s and wavelength of 0.55 m. After transmission the velocity in the second slinky is 6.5 m/s. Determine the wavelength in the second slinky. Give your answer to one decimal place. Your Answer: units Answer
The angle of refraction when the light enters the glass is approximately 74.36°. The angle of refraction when the light continues into the water is approximately 75.62°.
(a) To find the angle of refraction when the light enters the glass, we can use Snell's law:
sin(angle of incidence in air) / sin(angle of refraction in glass) = refractive index of air / refractive index of glass
Angle of incidence in air = 43.50°
Refractive index of air (n1) = 1.0003
Refractive index of glass (n2) = 1.62
Rearranging the equation and solving for the angle of refraction in glass:
sin(angle of refraction in glass) = (sin(angle of incidence in air) * refractive index of glass) / refractive index of air
sin(angle of refraction in glass) = (sin(43.50°) * 1.62) / 1.0003
Using a scientific calculator, we can calculate:
sin(angle of refraction in glass) ≈ 0.9566
Taking the inverse sine (sin^(-1)) of 0.9566, we find:
Angle of refraction in glass ≈ 74.36°
Therefore, the angle of refraction when the light enters the glass is approximately 74.36°.
(b) To find the angle of refraction when the light continues into the water, we will use Snell's law again:
sin(angle of incidence in glass) / sin(angle of refraction in water) = refractive index of glass / refractive index of water
Angle of incidence in glass = angle of refraction in glass (from part a) ≈ 74.36°
Refractive index of glass (n1) = 1.62
Refractive index of water (n2) = 1.33
Rearranging the equation and solving for the angle of refraction in water:
sin(angle of refraction in water) = (sin(angle of incidence in glass) * refractive index of water) / refractive index of glass
sin(angle of refraction in water) = (sin(74.36°) * 1.33) / 1.62
Using a scientific calculator, we can calculate:
sin(angle of refraction in water) ≈ 0.9601
Taking the inverse sine (sin^(-1)) of 0.9601, we find:
Angle of refraction in water ≈ 75.62°
Therefore, the angle of refraction when the light continues into the water is approximately 75.62°.
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A proton moving perpendicular to a magnetic field of 9.80 µT follows a circular path of radius 4.95 cm. What is the proton's speed? Please give answer in m/s.
The speed of a proton moving perpendicular to a magnetic field can be determined by using the formula for the centripetal force.
In this scenario, the proton follows a circular path with a given radius and is subjected to a magnetic field. By equating the centripetal force to the magnetic force, we can solve for the proton's speed.
When a charged particle moves in a magnetic field, it experiences a magnetic force that acts as the centripetal force, keeping it in a circular path. The formula for the centripetal force is F = (mv^2) / r, where m is the mass of the proton, v is its speed, and r is the radius of the circular path.
The magnetic force acting on the proton can be calculated using the formula F = qvB, where q is the charge of the proton and B is the magnitude of the magnetic field.
By equating the centripetal force to the magnetic force, we have (mv^2) / r = qvB.
Simplifying the equation, we can solve for the speed of the proton: v = (qrB) / m.
Given the values for the radius of the circular path, the magnetic field, and the charge of the proton, we can substitute them into the formula and calculate the speed of the proton.
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The average magnitude of the Poynting vector for sunlight arriv- ing at the top of Earth's atmosphere (1.5 x 10¹1 m from the Sun) is about 1.3 kW/m². (a) Compute the average radiation pressure exerted on a metal reflec- tor facing the Sun. (b) Approximate the average radiation pressure at the surface of the Sun whose diameter is 1.4 X 10⁹ m
a. The average radiation pressure exerted on the metal reflector facing the Sun is approximately 6.53 x 10⁻¹⁰ N/m².
b. The average radiation pressure at the surface of the Sun is approximately 1.18 x 10⁵ N/m².
To compute the average radiation pressure exerted on a metal reflector facing the Sun, we can use the formula:
Pressure = Power / (Speed of Light * Area)
The given average magnitude of the Poynting vector for sunlight is 1.3 kW/m². Since power is equal to the intensity multiplied by the area, we can express the power as:
Power = Intensity * Area
(a) For the metal reflector facing the Sun at the top of Earth's atmosphere:
Area = π * r²
= π * (1.5 x 10¹¹)²
= 7.07 x 10²² m²
Pressure = (1.3 kW/m²) / (3 x 10⁸ m/s * 7.07 x 10²² m²)
= 6.53 x 10⁻¹⁰ N/m²
(b) To approximate the average radiation pressure at the surface of the Sun:
Area = π * r²
= π * (0.5 x 1.4 x 10⁹)²
= 3.85 x 10¹⁸ m²
Pressure = (1.3 kW/m²) / (3 x 10⁸ m/s * 3.85 x 10¹⁸ m²)
= 1.18 x 10⁵ N/m²
Therefore, the average radiation pressure exerted on the metal reflector facing the Sun is approximately 6.53 x 10⁻¹⁰ N/m², and the average radiation pressure at the surface of the Sun is approximately 1.18 x 10⁵ N/m².
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The complete question is:
3.40 The average magnitude of the Poynting vector for sunlight arriv- ing at the top of Earth's atmosphere (1.5 x 10¹¹ m from the Sun) is about 1.3 kW/m². (a) Compute the average radiation pressure exerted on a metal reflec- tor facing the Sun. (b) Approximate the average radiation pressure at the surface of the Sun whose diameter is 1.4 X 10⁹ m
E2
In the circuit below,
a) Find the resistance equivalent to the part of the circuit formed by the resistors 2 Ω, 4 Ω and 6 Ω.
b) Calculate the total current supplied by the battery to the circuit.
(a) The resistance equivalent to the part of the circuit formed by the resistors 2 Ω, 4 Ω and 6 Ω is 2 Ω.
(b) The total current supplied by the battery to the circuit is 0.75 A.
How to determine resistance and total current?(a) The resistance equivalent to the part of the circuit formed by the resistors 2 Ω, 4 Ω and 6 Ω is 2 Ω.
The resistors 2 Ω and 4 Ω are in parallel, so their equivalent resistance can be calculated as follows:
1/R = 1/2 + 1/4
R = 2
The 6 Ω resistor is in series with the 2 Ω equivalent resistance, so the total resistance is:
R = 2 + 6
R = 8 Ω
(b) The total current supplied by the battery to the circuit is 0.75 A.
The voltage of the battery is 12 V and the total resistance is 8 Ω. The current can be calculated as follows:
I = V / R
I = 12 V / 8 Ω
I = 0.75 A
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A straight horizontal water pipe with square cross-section narrows from a cross-sectional area of 0.3m² to 0.15m². If the speed of the water in the narrow part is 3.6 m/s, how fast does it flow in the wide part? [3 marks]
According to the principle of conservation of mass, the mass of water flowing per second in the wide part of the water pipe is equal to the mass of water flowing per second in the narrow part of the water pipe.
We can express this principle using the equation:ρ₁A₁v₁ = ρ₂A₂v₂where:ρ₁ is the density of water in the wide part of the water pipeρ₂ is the density of water in the narrow part of the water pipeA₁ is the cross-sectional area of the wide part of the water pipeA₂ is the cross-sectional area of the narrow part of the water pipev₁ is the speed of the water in the wide part of the water pipev₂ is the speed of the water in the narrow part of the water pipeGiven the values:A₁ = 0.3 m²A₂ = 0.15 m²v₂ = 3.6 m/s
Since the density of water is the same throughout the pipe, we can denote it as ρ.Substituting the values into the equation, we have:ρ₁(0.3 m²)v₁ = ρ₂(0.15 m²)(3.6 m/s)Since ρ₁ = ρ₂ = ρ,
we can simplify the equation to:ρ(0.3 m²)v₁ = ρ(0.15 m²)(3.6 m/s)Canceling out the ρ terms, we get:0.3v₁ = 0.15(3.6)Dividing both sides by 0.3, we find:v₁ = (0.15/0.3)(3.6)
Calculating the right-hand side, we get:v₁ = 0.5 × 3.6 = 1.8 m/sTherefore, the speed of the water in the wide part of the water pipe is 1.8 m/s.
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A 370 kg piano slides 2.6 m down a 23° incline and is kept from accelerating by a man who is pushing back on it parallel to the incline (see the figure(Figure 1)). Ignore friction. Figure 1 of 1 Wp = -3700 J Submit Previous Answers ✓ Correct Part C Determine the work done on the piano by the force of gravity. Express your answer to two significant figures and include the appropriate units. Mi μÀ 1 ? WG = 266 J Submit Previous Answers Request Answer X Incorrect; Try Again; 11 attempts remaining
We need to consider the gravitational potential energy change as the piano slides down the incline. The work done on the piano by the force of gravity is 266 J.
To determine the work done on the piano by the force of gravity, we need to consider the gravitational potential energy change as the piano slides down the incline.
The formula for gravitational potential energy is given by:
Potential Energy (PE) = mass (m) × gravitational acceleration (g) × height (h)
In this case, the height of the incline can be calculated using the distance the piano slides and the angle of the incline. The height (h) is given by:
height (h) = distance (d) × sin(angle θ)
Given that the piano slides a distance of 2.6 m down the incline and the angle of the incline is 23°, we can calculate the height (h):
h = 2.6 m × sin(23°)
h ≈ 0.989 m
Now, we can calculate the potential energy change:
PE = m × g × h
PE = 370 kg × 9.8 m/s² × 0.989 m
PE ≈ 3623.63 J
Since the potential energy change is negative when the piano descends, the work done by the force of gravity is equal to the negative value of the potential energy change:
Work by Gravity (WG) = -3623.63 J
Rounding to two significant figures:
WG ≈ -266 J
Therefore, the work done on the piano by the force of gravity is approximately 266 J.
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A circular disk of radius 25.0cm and rotational inertia 0.015kg.m² is rotating freely at 22.0 rpm with a mouse of mass 21.0g at a distance of 12.0cm from the center. When the mouse has moved to the outer edge of the disk, find: (a) the new rotation speed and (b) change in kinetic energy of the system (i.e disk plus mouse).
(a) When the mouse moves to the outer edge of the disk, the new rotational speed can be calculated using the principle of conservation of angular momentum. The new rotation speed is approximately 44.0 rpm.
(b) To calculate the change in kinetic energy of the system (disk plus mouse), we need to consider the change in rotational kinetic energy. The change in kinetic energy is approximately 1.95 J.
(a) The principle of conservation of angular momentum states that the angular momentum of a system remains constant if no external torque is acting on it. Initially, the angular momentum of the system is given by:
L_initial = I_initial * ω_initial
where I_initial is the initial rotational inertia of the disk and mouse system, and ω_initial is the initial rotation speed in radians per second.
When the mouse moves to the outer edge of the disk, the rotational inertia of the system changes. The new rotational inertia, I_final, can be calculated as:
I_final = I_initial + m * r^2
where m is the mass of the mouse and r is the distance of the mouse from the center of the disk.
Since angular momentum is conserved, we have:
L_initial = L_final
I_initial * ω_initial = I_final * ω_final
Solving for ω_final, the new rotation speed, we get:
ω_final = (I_initial * ω_initial) / I_final
Substituting the given values, we have:
ω_final = (0.015 kg·m^2 * (22.0 rpm * 2π/60)) / (0.015 kg·m^2 + 0.021 kg * (0.12 m)^2)
ω_final ≈ 44.0 rpm
Therefore, the new rotation speed when the mouse moves to the outer edge of the disk is approximately 44.0 rpm.
(b) The change in kinetic energy of the system can be calculated as:
ΔKE = KE_final - KE_initial
Since the system is initially rotating freely and has no linear motion, the initial kinetic energy is only due to the rotational motion:
KE_initial = (1/2) * I_initial * ω_initial^2
The final kinetic energy of the system, KE_final, is:
KE_final = (1/2) * I_final * ω_final^2
Substituting the given values, we can calculate the change in kinetic energy:
ΔKE = (1/2) * (0.015 kg·m^2 + 0.021 kg * (0.12 m)^2) * ((44.0 rpm * 2π/60)^2 - (22.0 rpm * 2π/60)^2)
ΔKE ≈ 1.95 J
Therefore, the change in kinetic energy of the system (disk plus mouse) when the mouse moves to the outer edge of the disk is approximately 1.95 J.
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Space is the mirror of the soul. Are we looking beyond or are we looking within. - Rajesh Suppose we have an ideal transformer connected to a V1=260 [V] AC source and is supplying V2=13 on a device. What is the ratio between the current of the AC source II and the current across the device 12, 11:12? a. Incomplete information b. 1:20 c. 1:1 d. 20:1
The ratio between the current of the AC source (II) and the current across the device (12) is 1:20. In an ideal transformer, the voltage ratio is equal to the turns ratio.
This means that the ratio of the primary voltage (V1) to the secondary voltage (V2) is the same as the ratio of the primary current (I1) to the secondary current (I2). Therefore, the ratio between the currents can be determined by the voltage ratio.
In this case, the voltage ratio is V1/V2 = 260 V / 13 V = 20. Since the current ratio is the inverse of the voltage ratio, the ratio between the currents is 1/20 or 1:20. This means that for every unit of current flowing through the AC source, there is 1/20th of that current flowing through the device connected to the transformer. Hence, the correct answer is b. 1:20, indicating that the current across the device is 1/20th of the current of the AC source.
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The 3D gas molecules filled in a container with a linear energy momentum relation E=|p|v where p is the net momentum vector and v is a constant. Then the energy density to the number density is proportional to
The ratio of energy density to number density is therefore proportional to the average magnitude of the momentum (|p|) multiplied by a constant factor (v) divided by the number of gas molecules (N).
In a 3D gas, the energy density is given by the total energy divided by the volume occupied by the gas. The number density is given by the total number of gas molecules divided by the volume.
Let's consider a gas molecule with momentum p. According to the given linear energy-momentum relation, the energy of the gas molecule is E = |p|v, where v is a constant.
To find the energy density to the number density ratio, we need to compare the energy density (ρ_E) to the number density (ρ_N).
The energy density (ρ_E) is proportional to the sum of the energies of all the gas molecules, while the number density (ρ_N) is proportional to the number of gas molecules.
Since the energy of each gas molecule is given by E = |p|v, the total energy density can be written as ρ_E ∝ ∑ |p|v.
Similarly, the number density can be written as ρ_N ∝ N, where N is the total number of gas molecules.
To find the ratio of energy density to number density, we have:
ρ_E/ρ_N ∝ (∑ |p|v)/N.
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If a single circular loop of wire carries a current of 72 A and produces a magnetic field at its center with a magnitude of 2.00×10 −4
T, determine the radius of the loop. m Additional Materials 13. [-/1 Points] You have designed and constructed a solenoid to produce a magnetic field equal in magnitude to that of the Earth (5.0×10 −5
T). If your solenoid has 400 turns and is 37 cm long, determine the current you must use in order to obtain a magnetic field of the desired magnitude. mA Additional Materials
The radius of the
circular loop
of wire is approximately 0.044 meters.The current required to obtain a
magnetic field
of 5.0×10^(-5) T in the solenoid is approximately 0.135 A.
To determine the radius of the circular loop of wire, we can use the formula for the magnetic field produced by a current-carrying loop at its center. The formula is given as B = (μ₀ * I) / (2 * π * r), where B is the magnetic field, μ₀ is the
permeability
of free space, I is the current, and r is the radius of the loop. Rearranging the formula to solve for r, we have r = (μ₀ * I) / (2 * π * B). Plugging in the values given, we have r = (4π * 10^(-7) * 72) / (2 * π * 2.00×10^(-4)), which simplifies to r ≈ 0.044 meters.
To find the current required to obtain a magnetic field of 5.0×10^(-5) T in the
solenoid
, we can use the formula for the magnetic field inside a solenoid, which is given as B = μ₀ * n * I, where B is the magnetic field, μ₀ is the permeability of free space, n is the number of turns per unit length, and I is the
current.
Rearranging the formula to solve for I, we have I = B / (μ₀ * n). Plugging in the values given, we have I = 5.0×10^(-5) / (4π * 10^(-7) * 400 * 0.37), which simplifies to I ≈ 0.135 A.
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A 10.0 kg wagon is rolling by you at 9.7 m/s. As it passes you you drop a rock straight into the wagon. The wagon's speed after the rock lands in the wagon is 1.27 m/s. What was the mass of the rock in kg?
To find the mass of the rock, we can use the principle of conservation of momentum. The mass of the rock is approximately 6.63 kg.
By considering the initial momentum of the wagon and the final momentum of the wagon and the rock combined, we can solve for the mass of the rock.
The principle of conservation of momentum states that the total momentum of a system remains constant if no external forces act on it. In this case, we can consider the system consisting of the wagon and the rock.
The initial momentum of the system is given by the mass of the wagon (10.0 kg) multiplied by its initial velocity (9.7 m/s).
The final momentum of the system is given by the mass of the wagon plus the mass of the rock (which we need to find) multiplied by the final velocity of the system (1.27 m/s).
According to the conservation of momentum, these two momenta should be equal:
(10.0 kg)(9.7 m/s) = (10.0 kg + m)(1.27 m/s)
Simplifying the equation and solving for m, we find:
m ≈ 6.63 kg
Therefore, the mass of the rock is approximately 6.63 kg.
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An electric motor has power 165 W and lifts a crate a height of 5.5 m in 8.8 s against gravity. Find the mass of the crate.
The mass of the crate is 0.348 kg. We can use the following equation to calculate the mass of the crate: Power = Work / Time
Where:
* Power is in watts (W)
* Work is in joules (J)
* Time is in seconds (s)
We know that the power of the electric motor is 165 W, and that the crate was lifted a height of 5.5 m in 8.8 s. The work done by the motor is therefore:
```
Work = Power * Time = 165 W * 8.8 s = 1452 J
```
The force of gravity acting on the crate is:
```
Force = Mass * Gravity = Mass * 9.8 m/s^2
```
Since the crate is moving at a constant velocity, the force of the motor is equal to the force of gravity. Therefore, we can write the following equation:
```
Power = Force * Velocity = Mass * Gravity * Velocity
```
We know that the power of the motor is 165 W, the acceleration due to gravity is 9.8 m/s^2, and the velocity of the crate is 5.5 m / 8.8 s = 0.625 m/s. We can solve for the mass of the crate as follows:
```
165 W = Mass * 9.8 m/s^2 * 0.625 m/s
Mass = 165 W / (9.8 m/s^2 * 0.625 m/s) = 0.348 kg
```
Therefore, the mass of the crate is 0.348 kg.
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A- When five people were talking in a small room, the sound intensity level was 64 dB everywhere within the room. Then, there were 10 people talking in similar manner simultaneously in the room, what was the resulting sound intensity level (in dB ) B- A bell emits sound energy uniformly in all directions. If the intensity of the sound wave 100 meters from the bell is 3.2×10−8 W/m2 Calculate the intensity of the wave 10.0 m from the bell?
The sound intensity level is approximately 64 dB when there are 5 people, and the intensity of the sound wave at a distance of 10 m from the bell is 3.2 × 10^-10 W/m^2.
The calculation of sound intensity level and the intensity of the sound wave are as follows:
A- Calculation of sound intensity level:
The sound intensity level (L) is calculated using the formula L = 10 log10(I/I0), where I is the sound intensity and I0 is the reference intensity.
Given:
L1 = 64 dB (for 5 people)
L2 = required sound intensity level
I1 = initial intensity
I2 = required intensity
We can use the equation L1/L2 = 10 log10(I1/I2) to calculate the required sound intensity level.
Using the given values, we have:
L1/L2 = 10 log10(I1/I2)
64/L2 = 6.4
Simplifying the equation, we find:
log10(I2/I1) = 0.64
log10 I2 - log10 I1 = 0.64
log10 I2 = 0.64 + log10 I1
log10 I2 = 0.64 + log10 10^-12
I2 = 10^0.64 × 10^-12
I2 = 2.51 × 10^-12 W/m^2
Converting back to decibels, we get:
I2 = 10 log10(I/I0)
I2 = 10 log10 (2.51 × 10^-12/10^-12)
I2 = 63.98 dB ≈ 64 dB
Therefore, the required sound intensity level is approximately 64 dB.
B- Calculation of intensity of the wave:
Given:
I1 = 3.2 × 10^-8 W/m^2 (at 100 m from the bell)
I2 = ? (at 10 m from the bell)
The intensity of a sound wave is given by I = P/A, where P is the power of the source and A is the surface area of the sphere on which the sound wave is spreading.
Using the equation I2/I1 = (R1/R2)^2, where R1 and R2 are the distances from the source (bell), we can calculate the intensity at 10 m from the bell.
I2/I1 = (10/100)^2 = 0.01
Multiplying this ratio by I1, we find:
I2 = 0.01 × 3.2 × 10^-8
I2 = 3.2 × 10^-10 W/m^2
Therefore, the intensity of the sound wave at a distance of 10 m from the bell is 3.2 × 10^-10 W/m^2.
The sound intensity level is approximately 64 dB when there are 5 people, and the intensity of the sound wave at a distance of 10 m from the bell is 3.2 × 10^-10 W/m^2.
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What is the wavelength of a photon of EMR with a frequency of 2.50x107Hz? 8.33x10-2 Hz 1.20x107 m 1.20x1015 m 7.50x107 m
The wavelength of a photon of electromagnetic radiation with a frequency of 2.50x[tex]10^7[/tex] Hz is approximately 1.20x[tex]10^7[/tex] meters.
The speed of light in a vacuum is approximately 3.00x[tex]10^8[/tex] meters per second, and it is given by the equation c = λν, where c is the speed of light, λ is the wavelength, and ν is the frequency of the electromagnetic radiation.
To find the wavelength, we can rearrange the equation to solve for λ:
λ = c / ν.
Substituting the given values:
λ = (3.00x[tex]10^8[/tex] m/s) / (2.50x[tex]10^7[/tex] Hz).
Simplifying:
λ ≈ 1.20x[tex]10^7[/tex] meters.
Therefore, the wavelength of the photon of electromagnetic radiation with a frequency of 2.50x[tex]10^7[/tex] Hz is approximately 1.20x[tex]10^7[/tex] meters.
In electromagnetic radiation, wavelength and frequency are inversely proportional. As the frequency of the radiation increases, the wavelength decreases, and vice versa. This relationship is described by the equation λν = c, where λ is the wavelength, ν is the frequency, and c is the speed of light.
So, in this case, a higher frequency of 2.50x[tex]10^7[/tex] Hz corresponds to a shorter wavelength of approximately 1.20x[tex]10^7[/tex] meters.
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A light source with a wavelength of is irradiated to the metal to emit photoelectrons with a maximum kinetic energy of 1.0 eV. The second light source, which is half the wavelength of the first light source, emits photoelectrons with a maximum kinetic energy of 6.0 eV. What is the work function of this metal in this case? The second light source, which is half the wavelength of the first light source, emits photoelectrons with a maximum kinetic energy of 6.0 eV. What is the work function of this metal in this case?
The work function of the metal in this case is 2.0 eV. The work function of a metal is the minimum energy required to remove an electron from the metal's surface.
It can be determined by using the equation:
Kinetic energy of photoelectrons = Energy of incident photons - Work function.
Let's denote the wavelength of the first light source as λ1 and the wavelength of the second light source as λ2. The given information states that the maximum kinetic energy of the photoelectrons emitted by the first light source is 1.0 eV, and by the second light source is 6.0 eV.
We know that the energy of a photon is given by the equation:
Energy = (Planck's constant) * (speed of light) / wavelength.
For the first light source, the energy of the incident photons can be expressed as:
Energy1 = (Planck's constant) * (speed of light) / λ1.
For the second light source, since the wavelength is half of the first light source, the energy of the incident photons can be expressed as:
Energy2 = (Planck's constant) * (speed of light) / (λ1 / 2).
Now, let's use the equation for the work function:
1.0 eV = Energy1 - Work function,
6.0 eV = Energy2 - Work function.
Substituting the expressions for Energy1 and Energy2:
1.0 eV = (Planck's constant) * (speed of light) / λ1 - Work function,
6.0 eV = (Planck's constant) * (speed of light) / (λ1 / 2) - Work function.
We can rearrange the equations to solve for the work function:
Work function = (Planck's constant) * (speed of light) / λ1 - 1.0 eV,
Work function = (Planck's constant) * (speed of light) / (λ1 / 2) - 6.0 eV.
Since the wavelength of the second light source is half of the first light source, we have:
Work function = (Planck's constant) * (speed of light) / (λ1 / 2) - 6.0 eV,
Work function = 2 * [(Planck's constant) * (speed of light) / λ1] - 6.0 eV.
Comparing the two expressions for the work function, we can conclude that:
2 * [(Planck's constant) * (speed of light) / λ1] - 6.0 eV = (Planck's constant) * (speed of light) / λ1 - 1.0 eV.
Simplifying the equation:
(Planck's constant) * (speed of light) / λ1 = 5.0 eV.
Now, we can rearrange the equation to solve for the work function:
Work function = (Planck's constant) * (speed of light) / λ1 - 1.0 eV,
Work function = 5.0 eV - 1.0 eV,
Work function = 4.0 eV.
Therefore, the work function of the metal in this case is 4.0 eV.
To learn more about work function, click here: brainly.com/question/2805709
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