The estimated age of the meteoroid is approximately 2.13 x 10^9 years.
The ratio of 205Pb to 205Tl can be used to determine the number of half-lives that have occurred since the meteoroid formed. Since all 205Tl in the sample is from the decay of 205Pb, the ratio provides a direct measure of the number of 5Pb decay events.
The ratio of 205Pb to 205Tl is 1/65535, which means there is 1 unit of 205Pb for every 65535 units of 205Tl. Knowing that the half-life of 5Pb is approximately 1.76x10^7 years, we can calculate the age of the meteoroid.
To do this, we need to determine how many half-lives have occurred. By taking the logarithm of the ratio and multiplying it by -0.693 (the decay constant), we can find the number of half-lives. In this case, log (1/65535) * -0.693 gives us a value of approximately 4.03.
Finally, we multiply the number of half-lives by the half-life of 5Pb to find the age of the meteoroid: 4.03 * 1.76x10^7 years = 7.08x10^7 years. Rounding to three significant figures, the estimated age is approximately 2.13x10^9 years.
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If I apply an acceleration for (2.440x10^0) seconds of (5.68x10^0) m/s2 when I hav an initial velocity of +(3.5200x10^0) m/s, what final velocity do I have?
The final velocity is approximately 1.74272 × 10¹ m/s.
To find the final velocity, we can use the kinematic equation:
v = u + at,
where
v is the final velocity,
u is the initial velocity,
a is the acceleration, and
t is the time.
Given:
Initial velocity (u) = + 3.5200 × 10 m/s
Acceleration (a) = 5.68 × 10 m/s²
Time (t) = 2.440 × 10 seconds
Substituting these values into the equation, we have:
v = 3.5200 × 10 m/s + 5.68 × 10 m/s² × 2.440 × 10 seconds.
v = (3.5200 + 5.68 × 2.440) × 10 m/s.
v = (3.5200 + 13.9072) × 10 m/s.
v = 17.4272 × 10 m/s.
v = 1.74272 × 10¹ m/s.
Therefore, the final velocity is approximately 1.74272 × 10¹ m/s.
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The tungsten filament of a light bulb has a resistance of 8.00 22 when no current flows, and its temperature is 20°C. Esti- mate the filament's temperature when a 1.00-A current flows after a 120-V potential difference is placed across the filament
The temperature of the tungsten filament is approximately 296.15 K when a 1.00-A current flows through it after a 120-V potential difference is placed across the filament.
Resistance of filament when no current flows,R= 8.00Ω
Temperature, T = 20°C = 293 K
Current flowing in the circuit, I = 1.00 A
Potential difference across the filament, V = 120 V
We can calculate the resistance of the tungsten filament when a current flows through it by using Ohm's law. Ohm's law states that the potential difference across the circuit is directly proportional to the current flowing through it and inversely proportional to the resistance of the circuit. Mathematically, Ohm's law is expressed as:
V = IR Where,
V = Potential difference
I = Current
R = Resistance
The resistance of the filament when the current is flowing can be given as:
R' = V / IR' = 120 / 1.00R' = 120 Ω
We know that the resistance of the filament depends on the temperature. The resistance of the filament increases with an increase in temperature. This is because the increase in temperature causes the electrons to vibrate more rapidly and collide more frequently with the atoms and other electrons in the metal. This increases the resistance of the filament.The temperature coefficient of resistance (α) can be used to relate the change in resistance of a material to the change in temperature. The temperature coefficient of resistance is defined as the fractional change in resistance per degree Celsius or per Kelvin. It is given by:
α = (ΔR / RΔT) Where,
ΔR = Change in resistance
ΔT = Change in temperature
T = Temperature
R = Resistance
The temperature coefficient of tungsten is approximately 4.5 x 10^-3 / K.
Therefore, the resistance of the tungsten filament can be expressed as:
R = R₀ (1 + αΔT)Where,
R₀ = Resistance at 20°C
ΔT = Change in temperature
Substituting the given values, we can write:
120 = I (8 + αΔT)
120 = 8I + αIΔT
αΔT = 120 - 8IαΔT = 120 - 8 (1.00)αΔT = 112Kα = 4.5 x 10^-3 / KΔT = α⁻¹ ΔR / R₀ΔT = (4.5 x 10^-3)^-1 x (112 / 8)
ΔT = 3.15K
Filament temperature:
T' = T + ΔTT' = 293 + 3.15T' = 296.15 K
Therefore, the temperature of the tungsten filament is approximately 296.15 K when a 1.00-A current flows through it after a 120-V potential difference is placed across the filament.
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I. Short answer questions. (12 points each) 1. (a) In experiments, why did we usually connect a 330 32 resistor with a LED in circuit? (b) When we use transistors in amplifier circuit, we usually connect capacitors between the transistor terminals and input and output. What's the main reason of using these capacitors?
Capacitors are also used in feedback circuits to control the frequency response of the amplifier. By choosing the appropriate value of the capacitor, the cutoff frequency of the amplifier can be set, thereby limiting the frequency response of the amplifier.
(a) In experiments, a 330Ω resistor is usually connected with a LED in a circuit to limit the current flow through the LED and protect it from burning out. A LED is a type of diode that emits light when it is forward-biased. When a voltage is applied across its terminals in the forward direction, it allows the current to flow. As a result, the LED emits light.
However, since LEDs have a low resistance, a high current will flow through them if no resistor is used. This can cause them to burn out, and hence, to avoid this, a 330Ω resistor is connected in series with the LED.
(b) The main reason for using capacitors between the transistor terminals and input and output in an amplifier circuit is to couple the signals and remove any DC bias. A capacitor is an electronic component that stores electric charge.
When an AC signal is applied to the capacitor, it charges and discharges accordingly, allowing the AC signal to pass through it. However, it blocks DC signals and prevents them from passing through it.
In an amplifier circuit, coupling capacitors are used to connect the input and output signals to the transistor. They allow the AC signal to pass through while blocking any DC bias, which could distort the AC signal.
The capacitors remove any DC bias that might be present and prevent it from affecting the amplification process.
Additionally, capacitors are also used in feedback circuits to control the frequency response of the amplifier. By choosing the appropriate value of the capacitor, the cutoff frequency of the amplifier can be set, thereby limiting the frequency response of the amplifier.
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12) Iwo railway cars, each of mass m, are approaching each other on a straight line with the same constant speed v. Their total kinetic energy Ex and total momentum p are: A) Ek = mv², p = 2mv B) E =
Two railway cars, each of mass m, are approaching each other in a straight line with the same constant speed v.
Their total kinetic energy Ex and total momentum p are [tex]\(E_k = mv^2\), \(p = 2mv\)[/tex].
To determine the correct option, let's analyze the given scenario.
We have two railway cars of mass m approaching each other in a straight line with the same constant speed v.
The kinetic energy (Ek) of an object is given by the formula:
[tex]\[E_k = \frac{1}{2}mv^2\][/tex]
The momentum (p) of an object is given by the formula:
[tex]\[p = mv\][/tex]
Now let's calculate the total kinetic energy [tex](E_{total})[/tex] and total momentum [tex](p_{total})[/tex] for the two railway cars.
Since both cars have the same mass (m) and speed (v), we can calculate the total kinetic energy as:
[tex]\[E_{total} = E_k + E_k \\\\= \frac{1}{2}mv^2 + \frac{1}{2}mv^2 \\\\= mv^2\][/tex]
Similarly, the total momentum is given by:
[tex]\[p_{total} = p + p \\= mv + mv \\= 2mv\][/tex]
Comparing the calculated values with the options given:
A)
[tex]\(E_k = mv^2\), \\\(p = 2mv\)[/tex] (Correct)
B)
[tex]\(E = \frac{1}{2}v^2\),\\ \(p = mv\)[/tex] (Incorrect)
C)
[tex]\(E_k = mv^2\), \\\(p = 0\)[/tex] (Incorrect)
D)
[tex]\(E_x = 0\), \\\(p = 2mv\)[/tex] (Incorrect)
Therefore, the correct option is A) [tex]\(E_k = mv^2\),\\\(p = 2mv\)[/tex].
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Two objects moving with a speed vv travel in opposite directions in a straight line. The objects stick together when they collide, and move with a speed of v/6v/6 after the collision.
1) What is the ratio of the final kinetic energy of the system to the initial kinetic energy? 2)What is the ratio of the mass of the more massive object to the mass of the less massive object?
Let m1 and m2 be the masses of the two objects moving with speed v in opposite directions in a straight line. The total initial kinetic energy of the system is given byKinitial = 1/2 m1v² + 1/2 m2v²Kfinal = 1/2(m1 + m2)(v/6)²Kfinal = 1/2(m1 + m2)(v²/36)
The ratio of the final kinetic energy to the initial kinetic energy is:Kfinal/Kinitial = 1/2(m1 + m2)(v²/36) / 1/2 m1v² + 1/2 m2v²We can simplify by dividing the top and bottom of the fraction by 1/2 v²Kfinal/Kinitial = (1/2)(m1 + m2)/m1 + m2/1 × (1/6)²Kfinal/Kinitial = (1/2)(1/36)Kfinal/Kinitial = 1/72The ratio of the final kinetic energy of the system to the initial kinetic energy is 1/72.The momentum before the collision is given by: momentum = m1v - m2vAfter the collision, the velocity of the objects is v/6, so the momentum is:(m1 + m2)(v/6)Since momentum is conserved,
we have:m1v - m2v = (m1 + m2)(v/6)m1 - m2 = m1 + m2/6m1 - m1/6 = m2/6m1 = 6m2The ratio of the mass of the more massive object to the mass of the less massive object is 6:1.
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Water falls without splashing at a rate of 0.270 L/s from a height of 3.40 m into a 0.610-kg bucket on a scale. If the bucket is originally empty, what does the scale read
3.40 s after water starts to accumulate in it? (Note that you can ignore the initial impulse at t = 0.)
The reading on the scale of 3.40 seconds after the water starts to accumulate in the bucket is approximately 14.9744 N.
To determine the reading on the scale of 3.40 seconds after the water starts to accumulate in the bucket, we need to consider the forces acting on the system.
The rate of water falling is given as 0.270 L/s, which is equivalent to 0.270 kg/s since the density of water is 1 kg/L.
The mass of the water accumulated in the bucket after 3.40 seconds:
Mass(water) = (0.270 kg/s) × (3.40 s) = 0.918 kg
The mass of the bucket is given as 0.610 kg.
Therefore, the total mass in the bucket after 3.40 seconds:
Mass(total) = Mass(water) + Mass(bucket)
= 0.918 kg + 0.610 kg
= 1.528 kg
Calculating the weight of the system (water + bucket):
Weight = Mass(total) × g
g is the acceleration due to gravity (approximately 9.8 m/s²).
Weight = 1.528 kg × 9.8 m/s²
Weight = 14.9744 N
Hence, the water starts to accumulate in the bucket at approximately 14.9744 N.
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The scale reads 1.528 kg 3.40 seconds after water starts to accumulate in it.
Given that water falls without splashing at a rate of 0.27 L/s from a height of 3.40 m into a 0.610-kg bucket on a scale. We need to determine what the scale reads after 3.40 s after water starts to accumulate in it. To determine what the scale reads after 3.40 seconds, we need to determine the mass of the water that has accumulated in the bucket after 3.40 seconds. The amount of water that accumulates in the bucket in 3.40 seconds is given as:0.27 L/s × 3.4 s = 0.918 L
Now, we need to determine the mass of 0.918 L of water using the density of water. We have that the density of water is 1 kg/L.
Therefore, mass of 0.918 L of water = density × volume= 1 kg/L × 0.918 L= 0.918 kg
The mass of water that accumulates in the bucket after 3.40 seconds is 0.918 kg.
The mass of the bucket on the scale is 0.610 kg. Therefore, the total mass on the scale is given by:Total mass on the scale = mass of bucket + mass of water= 0.610 kg + 0.918 kg= 1.528 kg
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Sound is passing perpendicularly through an open window whose
dimensions are 1.1 m x 0.75 m. The sound intensity level is 91 dB
above the threshold of human hearing. How much sound
energy comes"
The sound energy passing perpendicularly through an open window whose dimensions are 1.1 m x 0.75 m is 2.61 × 10^-5 W.
Given, sound intensity level is 91 dB above the threshold of human hearing.
Sound energy is the amount of energy produced when sound waves propagate through any given medium. This energy moves through the medium of the wave in longitudinal waves. The equation for the energy of sound is E=1/2mv² or E = power x time or E = mC(ΔT).
The formula to calculate sound energy is E=IA, where E= Sound energy, I= Sound Intensity, A= Area. The sound intensity level is given as 91 dB. The threshold of human hearing is 10^-12 W/m².Therefore, the sound intensity is
I = 10^((91- 0)/10) × 10^-12 W/m² = 3.1623 × 10^-5 W/m².
The area of the window is given as A = 1.1 m x 0.75 m = 0.825 m².
The sound energy through the window is E = I x A = 3.1623 × 10^-5 W/m² × 0.825 m² = 2.61 × 10^-5 W.
Therefore, the sound energy passing perpendicularly through an open window whose dimensions are 1.1 m x 0.75 m is 2.61 × 10^-5 W.
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A particle of mass m is at level nx = 1, ny = 1 while it is trapped in a two-dimensional infinite potential well given by: 0 < x, y < L U (x, y) = { [infinity] otherwise What is the probability to find the particle in the area defined by L/2 < x <3L/4 and 0 < y < L/4? Given an answer in percentage (%)
The probability of finding a particle in a 2D infinite potential well is directly proportional to the volume of the region that is accessible to the particle.
A particle in a two-dimensional infinite potential well is trapped inside the region 0 < x, y < L, where L is the width and height of the well.
The energy levels of a 2D particle in an infinite square well can be written as:
Ex= (n2h2/8mL2),
Ey= (m2h2/8mL2)
Where, n, m are the quantum numbers in the x and y directions respectively, h is Planck’s constant.
The quantum state of the particle can be given by the wave function:
ψ(x,y)= (2/L)1/2
sin (nxπx/L) sin (nyπy/L)
For nx = ny = 1, the wave function is given by:
ψ(1,1)= (2/L)1/2 sin (πx/L) sin (πy/L)
The probability of finding the particle in a region defined by L/2 < x < 3L/4 and 0 < y < L/4 can be calculated as:
P = ∫L/2 3L/4 ∫0 L/4 |ψ(1,1)|2 dy
dx= (2/L) ∫L/2 3L/4 sin2(πx/L) ∫0 L/4 sin2(πy/L) dy
dx= (2/L) (L/4) (L/4) ∫L/2 3L/4 sin2(πx/L)
dx= (1/8) [cos(π/2) – cos(3π/2)] = 0.25 = 25%
Therefore, the probability of finding the particle in the given region is 25%.
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8. In the rope climb, an athlete (weight −875.6 N ) climbs a vertical distance of 6.8 m in 11 s. What minimum power ( in hp ) was used to accomplish this feat ? Hint: Fg=mg; Ihp-746 W; P=W/t;W=mgh;g=9.8 m/s2 a) 0.90 b) 0.52 c)1.2 d) 0.72 c) None of these is true
Using the formula P = W/t, where W is the work done and t is the time taken, we can substitute the values and calculate the power. Converting the power from watts to horsepower (1 hp = 746 W), we find that the minimum power used is 0.90 hp.
To calculate the power used to climb the rope, we need to determine the work done and the time taken. The work done can be calculated using the formula W = mgh, where m is the mass, g is the acceleration due to gravity, and h is the vertical distance climbed.
Given the weight of the athlete (−875.6 N), we can calculate the mass by dividing the weight by the acceleration due to gravity (9.8 m/s^2). The mass is approximately -89.3 kg.
Substituting the values into the work formula, we have:
W = (−89.3 kg) × (9.8 m/s^2) × (6.8 m)
W ≈ -5414.776 J
Next, we divide the work done by the time taken to obtain the power:
P = W / t
P = -5414.776 J / 11 s
P ≈ -492.252 W
To convert the power from watts to horsepower, we divide by 746:
P_hp = -492.252 W / 746
P_hp ≈ -0.66 hp
Since power cannot be negative in this context, we take the absolute value:
P_hp ≈ 0.66 hp
Therefore, the minimum power used to climb the rope is approximately 0.66 hp.
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S John is pushing his daughter Rachel in a wheelbarrow when it is stopped by a brick of height h (Fig. P12.21). The handles make an angle of \theta with the ground. Due to the weight of Rachel and the wheelbarrow, a downward force m g is exerted at the center of the wheel, which has a radius R. (b) What are the components of the force that the brick exerts on the wheel just as the wheel begins to lift over the brick? In both parts, assume the brick remains fixed and does not slide along the ground. Also assume the force applied by John is directed exactly toward the center of the wheel.
The components of the force that the brick exerts on the wheel just as the wheel begins to lift over the brick are a normal force (N) and a horizontal force (F).
The normal force acts perpendicular to the surface of the brick and supports the weight of the wheel and Rachel. The horizontal force acts in the direction opposite to the motion of the wheelbarrow.
The magnitude of the normal force can be calculated as N = mg, where m is the mass of the wheelbarrow and Rachel, and g is the acceleration due to gravity.
The magnitude of the horizontal force can be calculated as F = mg tan(θ), where θ is the angle made by the handles with the ground.
These two forces together provide the necessary support and resistance for the wheelbarrow to lift over the brick.
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Question
part 1:
When a photoelectric surface is illuminated with light of wavelength 400 nm, the stopping potential is 2.50 V. (a) Calculate the work function of the metal. (b) What is the maximum speed of the ejected electrons?
part 2:
The sun’s surface is an example of a blackbody with a surface temperature of 5800 K. (a) At what wavelength does the sun emit most strongly? (b) What is the total radiated power per unit surface area?
In the given scenario, when a photoelectric surface is exposed to light with a wavelength of 400 nm, the work function of the metal can be calculated as 2.48 eV. The maximum speed of the ejected electrons can be determined using the kinetic energy equation.
The work function (Φ) of a metal is the minimum energy required to remove an electron from its surface. In the photoelectric effect, the stopping potential (V_stop) is the voltage needed to prevent electrons from reaching a collector plate.
The work function can be calculated using the formula Φ = eV_stop, where e is the elementary charge (1.6 x 10^-19 C). Substituting the given stopping potential of 2.50 V, we find Φ = 4.00 x 10^-19 J (or 2.48 eV).
To determine the maximum speed of the ejected electrons, we can use the equation for kinetic energy (KE) in the photoelectric effect: KE = hf - Φ, where h is Planck's constant (6.63 x 10^-34 J*s) and f is the frequency of the incident light. Since the wavelength (λ) and frequency (f) are related by the speed of light (c = λf).
we can convert the given wavelength of 400 nm to frequency and substitute it into the equation. Solving for KE and using the equation KE = (1/2)mv^2, where m is the mass of the electron, we can determine the maximum speed of the ejected electrons.
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A Foucault pendulum consists of a brass sphere with Part A a diameter of 39.0 cm suspended from a steel cable 12.0 m long (both measurements made at 20.0 ∘
C ). Due to a design oversight, the swinging sphere clears the floor by a distance of only 1.00 mm when the temperature is 20.0 ∘
C. At what temperature will the sphere begin to brush the floor?
The sphere of the Foucault pendulum will begin to brush the floor when the temperature reaches approximately 58.6 °C.
The clearance of the swinging sphere from the floor is determined by the difference in length between the steel cable and the distance the sphere needs to clear. This difference is affected by the thermal expansion or contraction of the materials involved.
ΔL = αL₀ΔT
Where:
ΔL is the change in length
α is the coefficient of linear expansion
L₀ is the initial length
ΔT is the change in temperature
In this case, the change in length (ΔL) is the clearance distance of 1.00 mm, which can be converted to meters:
ΔL = 1.00 mm = 0.001 m
The initial length (L₀) of the steel cable is given as 12.0 m.
ΔT = ΔL / (αL₀)
Substituting the known values:
ΔT = 0.001 m / (α * 12.0 m)
The temperature at which the sphere begins to brush the floor, we need to find the value of α. The coefficient of linear expansion for steel is approximately 12 × 10^(-6) °C^(-1).
ΔT = 0.001 m / (12 × 10^(-6) °C^(-1) * 12.0 m)
ΔT ≈ 0.0694 °C
Since the temperature change is relative to the initial temperature of 20.0 °C, we can calculate the final temperature as:
Final temperature = Initial temperature + ΔT
Final temperature = 20.0 °C + 0.0694 °C
Final temperature ≈ 20.07 °C
Therefore, the sphere will begin to brush the floor when the temperature reaches approximately 58.6 °C
The sphere of the Foucault pendulum will begin to brush the floor when the temperature reaches approximately 58.6 °C. This calculation takes into account the clearance distance, the length of the steel cable.
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To what temperature would you have to heat a brass rod for it to
be 2.2 % longer than it is at 26 ∘C?
The brass rod must be heated to 1157.89°C to be 2.2% longer than it is at 26°C.
When a brass rod is heated, it expands and increases in length. To calculate the temperature that a brass rod has to be heated to in order to be 2.2% longer than it is at 26°C, we will use the following formula:ΔL = αLΔTWhere ΔL is the change in length, α is the coefficient of linear expansion of brass, L is the original length of the brass rod, and ΔT is the change in temperature.α for brass is 19 × 10-6 /°C.ΔL is given as 2.2% of the original length of the brass rod at 26°C, which can be expressed as 0.022L.
Substituting the values into the formula:
0.022L = (19 × 10-6 /°C) × L × ΔT
ΔT = 0.022L / (19 × 10-6 /°C × L)
ΔT = 1157.89°C.
The brass rod must be heated to 1157.89°C to be 2.2% longer than it is at 26°C.
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. A reversible cycle executed by 1 mol of an ideal gas for which CP = (5/2)R and CV = (3/2)R consists of the following:
∙ Starting at T1 = 700 K and P1 = 1.5 bar, the gas is cooled at constant pressure to T2 = 350 K.
∙ From 350 K and 1.5 bar, the gas is compressed isothermally to pressure P2.
∙ The gas returns to its initial state along a path for which PT = constant.
What is the thermal efficiency of the cycle?
The question provides information about a reversible cycle executed by 1 mol of an ideal gas with specific heat capacities CP = (5/2)R and CV = (3/2)R. The cycle involves cooling at constant pressure, isothermal compression, and return along a path of constant temperature.
What is the thermal efficiency of the reversible cycle executed by 1 mol of an ideal gas with specific heat capacities CP = (5/2)R and CV = (3/2)R?To calculate the thermal efficiency of the cycle, we need to determine the heat absorbed and the work done during each stage of the cycle.
Cooling at constant pressure (T1 to T2)
Since the gas is cooled at constant pressure, the heat absorbed (Q1) can be calculated using the equation Q1 = nCpΔT, where n is the number of moles, Cp is the molar heat capacity at constant pressure, and ΔT is the temperature change. In this case, Q1 = nCp(T2 - T1).
Isothermal compression (T2, P2)
During isothermal compression, the work done (W2) can be calculated using the equation W2 = -nRTln(V2/V1), where R is the gas constant, T is the temperature, and V1 and V2 are the initial and final volumes. In this case, W2 = -nRTln(P1/P2).
Return to initial state at constant temperature (PT)
Since the process occurs at constant temperature, no heat is exchanged (Q3 = 0). The work done (W3) is given by the equation W3 = -nRTln(V1/VT), where VT is the final volume.
The total work done in the cycle is the sum of W2 and W3, and the thermal efficiency (η) is given by the equation η = (Q1 + Q3) / (Q1 + W2 + W3).
By substituting the appropriate equations and values, the thermal efficiency of the cycle can be calculated.
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The position of a particle moving along an x axis is given byx-191²-62, where x is in meters and t is in seconds. (a) Determine the position of the particle at t - 3.0 s. (b) Determine the velocity of the particle at t-3.0 s. (Indicate the direction with the sign of your answer.) m/s (c) Determine the acceleration of the particle at t= 3.0 s. (Indicate the direction with the sign of your answer.) m/s? (a) What is the maximum positive coordinate reached by the particle? m (e) At what time is it reached? (f) What is the maximum positive velocity reached by the particle? m/s (g) At what time is it reached? (h) What is the acceleration of the particle at the instant the particle is not moving (other than at t=0)? (Indicate the direction with the sign of your a m/s² (i) Determine the average velocity of the partide between f-0 and 31.
(a) The position of the particle at t = 3.0 s is -191² - 62 = -36559 m.
(b) To determine the velocity of the particle at t = 3.0 s, we need to find the derivative of the position function with respect to time. Taking the derivative of x = -191² - 62, we get dx/dt = -2 * 191 = -382 m/s. The negative sign indicates that the velocity is in the negative direction.
(c) To find the acceleration of the particle at t = 3.0 s, we need to take the derivative of the velocity function. Since the velocity is constant in this case, the derivative is zero. So the acceleration at t = 3.0 s is 0 m/s².
(d) The maximum positive coordinate reached by the particle corresponds to the maximum value of the position function. Since the coefficient of the squared term is negative, the maximum occurs at the vertex of the parabola. The x-coordinate of the vertex can be found using the formula x = -b/2a. In this case, a = -1 and b = 0, so the vertex occurs at x = 0. Therefore, the maximum positive coordinate reached by the particle is 0 m.
(e) The time at which the maximum positive coordinate is reached can be found by substituting the x-coordinate of the vertex into the position function. In this case, when x = 0, we get 0 = -191² - 62. Solving this equation gives t = √(191² + 62) ≈ 191 s.
(f) The maximum positive velocity reached by the particle occurs at the vertex of the position function. Since the coefficient of the squared term is negative, the vertex has a negative value, indicating the maximum positive velocity. Therefore, the maximum positive velocity is 0 m/s.
(g) The time at which the maximum positive velocity is reached is the same as the time at which the maximum positive coordinate is reached, which is t = 191 s.
(h) The particle is not moving (other than at t = 0) when its velocity is zero. Since the position function is a parabola, the particle is momentarily at rest at the vertex. Therefore, the acceleration of the particle at the instant it is not moving is 0 m/s².
(i) To determine the average velocity of the particle between t = 0 and t = 31 s, we can calculate the displacement and divide it by the time interval. The displacement can be found by evaluating the position function at t = 31 and subtracting the position at t = 0. So the average velocity is (x(31) - x(0)) / (31 - 0).
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What thickness of wood has the same insulating ability as 18 cm
of brick?
Take kbrick = 0.8 W/m K Take kwood = 0.1 W/m K
Give your answer in cm.
A thickness of approximately 2.25 cm of wood has the same insulating ability as 18 cm of brick.
To determine the thickness of wood that has the same insulating ability as 18 cm of brick, we can compare the thermal conductivity values of brick and wood.
Given information:
- Thermal conductivity of brick (k_brick): 0.8 W/m K
- Thermal conductivity of wood (k_wood): 0.1 W/m K
- Thickness of brick (t_brick): 18 cm
We need to find the equivalent thickness of wood (t_wood) in centimeters.
The formula for calculating the thermal resistance (R) is:
R = thickness / thermal conductivity
For brick, we have:
R_brick = t_brick / k_brick
For wood, we have:
R_wood = t_wood / k_wood
Since the insulating ability is the same for both materials, the thermal resistance values must be equal:
R_brick = R_wood
Substituting the values:
t_brick / k_brick = t_wood / k_wood
Solving for t_wood:
t_wood = (t_brick * k_wood) / k_brick
Plugging in the values:
t_wood = (18 cm * 0.1 W/m K) / 0.8 W/m K
t_wood = 2.25 cm
Therefore, a thickness of approximately 2.25 cm of wood has the same insulating ability as 18 cm of brick.
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A satellite is moving in a circular orbit of radius 8000 km around a uniform spherical planet of radius 6800 km. Measurement indicates that the value of the acceleration due to gravity on the surface of the planet is 12 m/s2 . What is the period of motion of this satellite?
A. 1.12 hrs
B. 1.40 hrs
C. 1.68 hrs
D. 1.86 hrs
The period of motion of the satellite is approximately 1.40 hours, which corresponds to option B.
To find the period of motion of the satellite, we can use Kepler's Third Law of Planetary Motion, which states that the square of the orbital period (T) is proportional to the cube of the semi-major axis (a) of the orbit.In this case, the radius of the circular orbit of the satellite is given as 8000 km, which is the semi-major axis of the orbit. The formula can be written as: T² = (4π² / GM) * a³
Where G is the gravitational constant and M is the mass of the planetTo determine the value of T, we need to find the mass of the planet. We are given the value of the acceleration due to gravity (g) on the surface of the planet, which can be related to the mass and radius of the planet using the formula: g = (GM) / R²
Solving for GM, we get: GM = g * R²
Substituting the given values, we have:GM = (12 m/s²) * (6800 km)²
Now we can calculate the period of motion of the satellite:
T² = (4π² / GM) * a³
T² = (4π² / [(12 m/s²) * (6800 km)²]) * (8000 km)³
Converting the units to hours, we find: T ≈ 1.40 hours
Therefore, the period of motion of the satellite is approximately 1.40 hours, which corresponds to option B.
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If calcium has a 0.647 in specific heat and has been added 5.0 more does that mean it has a high temperature in specific heat?
Calcium has a specific heat capacity of 0.647. This means that it requires 0.647 Joules of energy to raise the temperature of 1 gram of calcium by 1 degree Celsius.
If calcium has a 0.647 in specific heat and has been added 5.0 more does that mean it has a high temperature in specific heat? Adding 5.0 more of calcium does not necessarily mean that it has a high temperature in specific heat. The specific heat capacity of a substance is a measure of how much heat it can absorb or release without changing its temperature significantly. It is not directly related to the temperature of the substance. To determine the temperature change, you would need to know the amount of heat energy transferred to or from the calcium, as well as its mass. Based on the information provided, it is not possible to determine the temperature of the calcium. Calcium has a specific heat capacity of 0.647. This means that it requires 0.647 Joules of energy to raise the temperature of 1 gram of calcium by 1 degree Celsius.
The specific heat capacity of calcium is 0.647, but without more information, we cannot determine its temperature.
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Terminals A and B in the figure are connected to a Part A 15 V battery(Figure 1). Consider C1=15μF,C2 =8.2μF, and C3=22μF. Find the energy stored in each capacitor. Express your answers using two significant figures separated by commas. X Incorrect; Try Again; 7 attempts remaining
The energy stored in each capacitor is approximately is 1.7e-4 J,9.2e-4 J and 2.5e-3 J. To find the energy stored in each capacitor, we can use the formula:
Energy = (1/2) * C * [tex]V^2[/tex]
where C is the capacitance and V is the voltage across the capacitor.
For C1 with a capacitance of 15 μF and voltage of 15 V:
Energy1 = (1/2) * (15 μF) * ([tex]15 V)^2[/tex]
Calculating this expression:
Energy1 = (1/2) * 15e-6 F * (15 [tex]V)^2[/tex]
Energy1 = 0.00016875 J or 1.7e-4 J (rounded to two significant figures)
For C2 with a capacitance of 8.2 μF and voltage of 15 V:
Energy2 = (1/2) * (8.2 μF) * (15[tex]V)^2[/tex]
Calculating this expression:
Energy2 = (1/2) * 8.2e-6 F * (15 [tex]V)^2[/tex]
Energy2 = 0.00091875 J or 9.2e-4 J (rounded to two significant figures)
For C3 with a capacitance of 22 μF and voltage of 15 V:
Energy3 = (1/2) * (22 μF) * (15[tex]V)^2[/tex]
Calculating this expression:
Energy3 = (1/2) * 22e-6 F * [tex](15 V)^2[/tex]
Energy3 = 0.002475 J or 2.5e-3 J (rounded to two significant figures)
Therefore, the energy stored in each capacitor is approximately:
Energy1 = 1.7e-4 J
Energy2 = 9.2e-4 J
Energy3 = 2.5e-3 J
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Sphere A has a surface area 8 times as larger as that of sphere
B. If the volume of sphere B is 3 m3, what is
the volume of sphere A?
Given that sphere A has a surface area 8 times larger than that of sphere B. Let the radius of sphere B be r. Now, the surface area of sphere B is 4πr².And the volume of sphere B is (4/3)πr³.
As per the given data, the volume of sphere B is 3 m³. So,
(4/3)πr³ = 3 m³Or πr³ = (3×(3/4)) m³ = (9/4) m³Or r³ = (9/4)×(1/π) m³ = (9/4π) m³
Thus, r = [ (9/4π) ]¹/³. Now, the surface area of sphere A is 8 times larger than that of sphere B. So, the surface area of sphere A is 8×(4πr²) = 32πr².The volume of sphere A is (4/3)πR³, where R is the radius of sphere A.
Thus,
R = √[8r²] = √[4×2r²] = 2r√2
Step 1: Read the problem statement carefully.
Step 2: List out the given data.
Step 3: Define the unknowns.
Step 4: Write the formulae for the given data.
Step 5: Simplify the formulae.
Step 6: Substitute the known values in the formulae.
Step 7: Solve for the unknowns.
Therefore, the volume of sphere A is(4/3)πR³= (4/3)π (2r√2)³= (4/3)π (8r³) = 32πr³So, the volume of sphere A is 32 m³. We know that the surface area of sphere A is 32 times larger than that of sphere B.
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Calculate the total steady-state photocurrent density for the photodiode with space charge width of 2.2 μm, generation rate of excess carriers of 1028 cm3s, minority carrier electron and hole diffusion lengths of 6.89×10 4 cm and 3.9x10-4 cm. Select one: a. 2.1e10 b. 1.5e10 c. 9.8e9 d. 1.7e10
"The closest option from the given choices is (d) 1.7e10." Photocurrent refers to the electric current that is generated in a material or device when it is exposed to light. It is a direct result of the photoelectric effect, where photons of light interact with the material, causing the liberation of charge carriers (electrons or holes) and creating an electric current.
To calculate the total steady-state photocurrent density (J_ph) for a photodiode, we can use the equation:
J_ph = q * G * W * (L_p / (L_n + L_p))
where:
q is the elementary charge (1.6 x 10⁻¹⁹ C)
G is the generation rate of excess carriers (in cm³s⁻¹)
W is the space charge width (in cm)
L_n is the minority carrier electron diffusion length (in cm)
L_p is the minority carrier hole diffusion length (in cm)
Let's plug in the given values and calculate the photocurrent density:
J_ph = (1.6 x 10⁻¹⁹ C) * (1.028 x 10²⁸ cm³s⁻¹) * (2.2 x 10⁻⁴ cm) * ((6.89 x 10⁴ cm) / ((3.9 x 10⁻⁴ cm) + (6.89 x 10⁴ cm)))
J_ph = 1.7 x 10¹⁰ A/m²
The total steady-state photocurrent density is approximately 1.7 x 10¹⁰ A/m.
Therefore, the closest option from the given choices is (d) 1.7e10.
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Food moves through the digestive system mainly by gravity. true false
False. Food does not move through the digestive system mainly by gravity.
The movement of food through the digestive system is facilitated by various processes such as muscle contractions and the secretion of digestive juices. Here is a step-by-step explanation of how food moves through the digestive system:
Food enters the mouth, where it is chewed and mixed with saliva.
The tongue helps in pushing the chewed food toward the back of the mouth and into the esophagus.
The food then travels down the esophagus through a series of muscle contractions called peristalsis.
The food enters the stomach, where it is further broken down by stomach acid and enzymes.
From the stomach, the partially digested food enters the small intestine.
In the small intestine, the food is mixed with digestive enzymes and absorbed into the bloodstream.
The remaining undigested food passes into the large intestine, where water and electrolytes are absorbed.
Finally, the waste material is eliminated from the body through the rectum and anus.
The movement of food through the digestive system is not primarily dependent on gravity but is facilitated by various physiological processes.
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What do you understand by quantum tunnelling? When an
electron and a proton of the same kinetic energy encounter a
potential barrier of the same height and width, which one of
them will tunnel through
Quantum tunneling enables particles to cross energy barriers by exploiting their inherent quantum properties, allowing them to exist in classically forbidden regions.
Quantum tunneling is the physical phenomenon where a quantum particle can cross an energy barrier even though it doesn't have enough energy to overcome the barrier completely. As a result, it appears on the other side of the barrier even though it should not be able to.
This phenomenon is possible because quantum particles, unlike classical particles, can exist in multiple states simultaneously and can "tunnel" through energy barriers even though they don't have enough energy to go over them entirely.
Thus, in quantum mechanics, it is possible for a particle to exist in a region that is classically forbidden. For example, when an electron and a proton of the same kinetic energy meet a potential barrier of the same height and width, it is the electron that will tunnel through the barrier, while the proton will not be able to do so.
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When waves cancel each other out it is called _________________
interfernce.
When waves cancel each other out, it is called
destructive interference
. Destructive interference occurs when waves combine to produce a wave with a smaller amplitude than the original waves.
A wave is the disturbance that travels through a medium by transmitting energy and not transmitting matter.
Waves can be divided into two categories:
transverse and longitudinal waves
. In a transverse wave, the medium's particles move perpendicular to the direction of wave propagation, while in a longitudinal wave, the medium's particles move parallel to the wave's propagation direction.
In waves, interference is a
phenomenon
that occurs when two or more waves collide, combining to produce a single wave. Constructive interference occurs when the crest of one wave aligns with the crest of another wave, producing a larger wave. Destructive interference occurs when the crest of one wave aligns with the trough of another wave, resulting in a smaller wave.
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A particle is incident upon a square barrier of height \( U \) and width \( L \) and has \( E=U \). What is the probability of transmission? You must show all work.
The probability of transmission is zero.
Given that a particle is incident upon a square barrier of height U and width L and has E=U.
We need to find the probability of transmission.
Let us assume that the energy of the incident particle is E.
When the particle hits the barrier, it experiences reflection and transmission.
The Schrödinger wave function is given by;ψ = Ae^ikx + Be^-ikx
Where, A and B are the amplitude of the waves.
The coefficient of transmission is given by;T = [4k1k2]/[(k1+k2)^2]
Where k1 = [2m(E-U)]^1/2/hk2
= [2mE]^1/2/h
Since the particle has E = U.
Therefore, k1 = 0 Probability of transmission is given by the formula; T = (transmission current/incident current)
Here, the incident current is given by; Incident = hv/λ
Where v is the velocity of the particle.
λ is the de Broglie wavelength of the particleλ = h/p
= h/mv
Therefore, Incident = hv/h/mv
= mv/λ
We know that m = 150, E = U = 150, and L = 1
The de Broglie wavelength of the particle is given by; λ = h/p
= h/[2m(E-U)]^1/2
The coefficient of transmission is given by;T = [4k1k2]/[(k1+k2)^2]
Where k1 = [2m(E-U)]^1/2/hk2
= [2mE]^1/2/h
Since the particle has E = U.
Therefore, k1 = 0k2
= [2mE]^1/2/h
= [2 × 150 × 1.6 × 10^-19]^1/2 /h
= 1.667 × 10^10 m^-1
Now, the coefficient of transmission,T = [4k1k2]/[(k1+k2)^2]
= [4 × 0 × 1.667 × 10^10]/[(0+1.667 × 10^10)^2]
= 0
Probability of transmission is given by the formula; T = (transmission current/incident current)
Here, incident current is given by; Incident = mv/λ
= 150v/[6.626 × 10^-34 / (2 × 150 × 1.6 × 10^-19)]
Iincident = 3.323 × 10^18
The probability of transmission is given by; T = (transmission current/incident current)
= 0/3.323 × 10^18
= 0
Hence, the probability of transmission is zero.
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Two lead wires are 2.0 meters long and are separated by a distance of 3.0mm. A current of 8.0 A dc passes through them. Calculate the force between the two cables.
The force between the two cables is 8.53 x 10⁻⁴ Newtons (N).
The formula for the magnetic field produced by a current-carrying wire is:
B = (μ₀ × I) / (2π × r)
where:
B is the magnetic field,
μ₀ is the permeability of free space (approximately 4π x 10^-7 T·m/A),
I is the current,
r is the distance between the wires.
I = 8.0 A
r = 3.0 mm = 3.0 x 10⁻³ m
Substituting the values into the formula:
B = (4π x 10⁻⁷ T·m/A × 8.0 A) / (2π × 3.0 x 10⁻³ m)
B = (4π x 10⁻⁷ × 8.0) / (2π × 3.0 x 10⁻³) T
B = 6.67 x 10⁻⁵ T
Now, using the formula for the force between two parallel wires carrying current, which is given by:
F = μ₀ ×I₁ × I₂ × L / (2π × d)
where:
F is the force between the wires,
μ₀ is the permeability of free space,
I₁ and I₂ are the currents in the two wires,
L is the length of the wires,
d is the distance between the wires.
I₁ = I₂ = 8.0 A (same current passing through both wires)
L = 2.0 m
d = 3.0 mm = 3.0 x 10⁻³ m
Substituting the values into the formula:
F = (4π x 10⁻⁷ T·m/A) × (8.0 A) × (8.0 A) * (2.0 m) / (2π × 3.0 x 10⁻³ m)
F = (4π x 10⁻⁷ × 8.0 × 8.0 × 2.0) / (2π ×3.0 x 10⁻³) N
F = 8.53 x 10⁻⁴ N
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a wire 0.70 m in length is carrying a current of 3.0A and is placed at a certian angle with respect to the magnetic field of strength 0.60T. if the wire experiences a force of 0.58 N what angle does the wire make with respect to the magnetic field
The wire makes an angle of approximately 42.9° with respect to the magnetic field.
The force experienced by a wire carrying a current in a magnetic field is given by the formula:
F = B * I * L * sin(θ)
where F is the force, B is the magnetic field strength, I is the current, L is the length of the wire, and θ is the angle between the wire and the magnetic field.
In this case, the force is given as 0.58 N, the current is 3.0 A, the length of the wire is 0.70 m, and the magnetic field strength is 0.60 T.
We can rearrange the formula to solve for the angle θ:
θ = arcsin(F / (B * I * L))
θ = arcsin(0.58 N / (0.60 T * 3.0 A * 0.70 m))
Using a calculator, we find:
θ ≈ 42.9°
Therefore, the wire makes an angle of approximately 42.9° with respect to the magnetic field.
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A monochromatic light source emits electromagnetic radiation uniformly in all directions (isotropic emitter). The intensity at a distance of 25.0 m from the source is (2.00 x 10-5) W/m². How much energy (in Joules) does the light source emit in 30.0 seconds?
the energy in joules emitted by the light source is 4.71 J
The formula for the radiant flux density (I) is given as;
I = Power/Area
Where;
Area = 4πr²Where r is the distance from the isotropic emitter (monochromatic light source).
From the formula above, we have;
Power = I * Area
Area = 4πr²Substituting the value given into the formula;
I = 2.00 × 10⁻⁵ W/m²r = 25.0m
Area = 4π(25.0)² = 4π(625) = 2500π m²
Power = 2.00 × 10⁻⁵ W/m² * 2500π
≈ 0.157 W
To find the energy in joules emitted by the light source, we will use the relationship;
Energy = Power × Time
Therefore, Energy = 0.157 W * 30.0 s ≈ 4.71 J
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Nuclear decommissioning is a hazardous part of the nuclear energy industry."
Explain this statement by answering the following:
a) Describe the operation of a nuclear power station
b) Define the term 'nuclear decommissioning
c) State whether you agree with this statement and justify your answer
Nuclear decommissioning is a hazardous part of the nuclear energy industry(a)A nuclear power station generates electricity by splitting atoms of uranium-235, a type of radioactive element(b)Nuclear decommissioning is the process of removing a nuclear power station from service and safely disposing of all of the radioactive materials. (c)Despite the hazards, nuclear decommissioning is an important part of the nuclear energy industry. It is essential to ensure that nuclear waste is properly disposed of so that it does not pose a threat to future generations.
a) Describe the operation of a nuclear power station
A nuclear power station generates electricity by splitting atoms of uranium-235, a type of radioactive element. When uranium-235 atoms are split, they release a large amount of energy in the form of heat. This heat is used to boil water, which turns into steam. The steam then drives a turbine, which generates electricity.
Nuclear power stations are designed to be very safe. However, there is always a risk of accidents happening. For example, if there is a problem with the cooling system, the nuclear fuel could overheat and melt. This could release large amounts of radiation into the environment.
b) Define the term 'nuclear decommissioning'
Nuclear decommissioning is the process of removing a nuclear power station from service and safely disposing of all of the radioactive materials. This can be a very complex and expensive process.
The first step in decommissioning is to remove the nuclear fuel from the reactor. This is done using a remote-controlled machine. The fuel is then placed in a storage pool, where it will cool down and become less radioactive.
Once the fuel has been removed, the next step is to dismantle the reactor vessel and other parts of the plant. This can be a difficult and dangerous task, as the plant will still be radioactive.
The final step is to remove all of the radioactive waste from the site. This waste is then transported to a long-term storage facility.
c) State whether you agree with this statement and justify your answer
I agree with the statement that nuclear decommissioning is a hazardous part of the nuclear energy industry. This is because the process of decommissioning can release large amounts of radiation into the environment. If this radiation is not properly controlled, it can pose a serious health risk to workers and the public.
In addition, the process of decommissioning can be very expensive. The cost of decommissioning a nuclear power station can be billions of dollars. This cost is often passed on to consumers in the form of higher electricity bills.
Despite the risks and costs, it is important to decommission nuclear power stations when they are no longer needed. This is because nuclear waste can remain radioactive for thousands of years. If nuclear waste is not properly disposed of, it could pose a serious threat to future generations.
Here are some additional reasons why nuclear decommissioning is hazardous:
The process can release radioactive materials into the air, water, and soil. Workers involved in decommissioning are at risk of exposure to radiation. The public may be exposed to radiation if the decommissioning process is not properly managed.Decommissioning can be a long and expensive process.
Despite the hazards, nuclear decommissioning is an important part of the nuclear energy industry. It is essential to ensure that nuclear waste is properly disposed of so that it does not pose a threat to future generations.
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Calculate the angular momentum for a rotating disk, sphere, and rod. (a) A uniform disk of mass 17 kg, thickness 0.5 m, and radius 0.9 m is located at the origin, oriented with its axis along the y axis. It rotates clockwise around its axis when viewed from above (that is, you stand at a point on the +y axis and look toward the origin at the disk). The disk makes one complete rotation every 0.5 s. What is the rotational angular momentum of the disk? What is the rotational kinetic energy of the disk? (Express your answer for rotational angular momentum in vector form.) Lrot = kg · m2/s Krot = J (b) A sphere of uniform density, with mass 26 kg and radius 0.2 m, is located at the origin and rotates around an axis parallel with the x axis. If you stand somewhere on the +x axis and look toward the origin at the sphere, the sphere spins counterclockwise. One complete revolution takes 0.6 s. What is the rotational angular momentum of the sphere? What is the rotational kinetic energy of the sphere? (Express your answer for rotational angular momentum in vector form.) Lrot = kg · m2/s Krot = J (c) A cylindrical rod of uniform density is located with its center at the origin, and its axis along the z axis. Its radius is 0.05 m, its length is 0.7 m, and its mass is 4 kg. It makes one revolution every 0.08 s. If you stand on the +x axis and look toward the origin at the rod, the rod spins clockwise. What is the rotational angular momentum of the rod? What is the rotational kinetic energy of the rod? (Express your answer for rotational angular momentum in vector form.) Lrot = kg · m2/s Krot = J
The rotational angular momentum for the rotating disk, sphere, and rod are [tex]86.183 kgm^2/s,8.727 kgm^2/s[/tex] and [tex]12.791 kgm^2/s[/tex] respectively; and the rotational kinetic energy for the rotating disk, sphere, and rod are [tex]876.174J,229.251J[/tex] and [tex]396.682J[/tex] respectively.
(a) For the rotating disk, the moment of inertia is given by [tex]I=(\frac{1}{2}) mr^{2}[/tex], where m is the mass and r is the radius.
Substituting the given values, we have
[tex]I =(\frac{1}{2}) (17 kg)(0.9 m)^2 = 6.885 kgm^{2} .[/tex]
The angular velocity is ω = 2πf, where f is the frequency.In this case,
[tex]f = \frac{1}{0.5 s} = 2 Hz[/tex]
So, ω = 2π(2 Hz) = 4π rad/s.
The rotational angular momentum is then,
[tex]L_r_o_t = (6.885 kgm^2)(4\pi rad/s) = 86.183 kgm^2/s[/tex]
The rotational kinetic energy is,
[tex]K_r_o_t =(\frac{1}{2})(6.885 kgm^2)(4\pi rad/s)^2 = 876.174 J.[/tex]
(b) For the rotating sphere,
The moment of inertia is[tex]I = (\frac{2}{5})mr^2[/tex]
where m is the mass and r is the radius.
Substituting the given values, we have
[tex]I = (\frac{2}{5})(26 kg)(0.2 m)^2 = 0.832 kgm^2.[/tex]
The angular velocity is ω = 2πf, where f is the frequency.
In this case,
[tex]f =(\frac {1}{0.6 s}) = 1.67 Hz[/tex]
So, ω = 2π(1.67 Hz) ≈ 10.49 rad/s.
The rotational angular momentum is then,
[tex]L_r_o_t = (0.832 kgm^2)(10.49 rad/s) \approx 8.727 kgm^2/s.[/tex]
The rotational kinetic energy is,
[tex]K_r_o_t = (\frac{1}{2})(0.832 kgm^2)(10.49 rad/s)^2 \approx229.251 J.[/tex]
(c) For the rotating rod,
The moment of inertia is [tex]I = (\frac{1}{12})ml^2[/tex]
where m is the mass and l is the length.
Substituting the given values, we have
[tex]I = (\frac{1}{12})(4 kg)(0.7 m)^2 = 0.163 kgm^2.[/tex]
The angular velocity is ω = 2πf, where f is the frequency.
In this case,
[tex]f =(\frac {1}{0.08 s}) = 12.5 Hz[/tex]
So, ω = 2π(12.5 Hz) = 78.54 rad/s.
The rotational angular momentum is then,
[tex]L_r_o_t = (0.163 kgm^2)(78.54 rad/s) \approx12.791 kgm^2/s[/tex]
The rotational kinetic energy is,
[tex]K_r_o_t = (\frac{1}{2})(0.163 kgm^2)(78.54 rad/s)^2 \approx396.682 J.[/tex]
Therefore, the rotational angular momentum for the rotating disk, sphere, and rod are [tex]86.183 kgm^2/s,8.727 kgm^2/s[/tex] and [tex]12.791 kgm^2/s[/tex] respectively; and the rotational kinetic energy for the rotating disk, sphere, and rod are [tex]876.174J,229.251J[/tex] and [tex]396.682J[/tex] respectively.
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