the net radiant heat transfer from the hot disk is approximately 139.66 watts, and the net radiant heat transfer from the cold disk is approximately 69.83 watts. The radiant heat transfer with the room is negligible in this case.
To calculate the net radiant heat transfer between the two parallel disks, we can use the Stefan-Boltzmann law, which states that the rate of radiant heat transfer between two objects is proportional to the fourth power of the temperature difference between them.The formula for radiant heat transfer is: Q = ε * σ * A * (T1^4 - T2^4). Where Q is the net radiant heat transfer, ε is the emissivity of the surface, σ is the Stefan-Boltzmann constant (5.67 x 10^(-8) W/(m^2·K^4)), A is the surface area, T1 is the temperature of the hot disk, and T2 is the temperature of the cold disk.Given the following values:
T1 = 620°C = 893K
T2 = 220°C = 493K
E1 = 0.9 (emissivity of the hot disk)
E2 = 0.45 (emissivity of the cold disk)
Diameter of disks = 80 cm
Distance between disks = 10 cm.
First, we need to calculate the surface areas of the disks: A = π * r^2
For each disk: r = diameter/2 = 80 cm / 2 = 40 cm = 0.4 m
A = π * (0.4 m)^2
Substituting the values into the formula: Q1 = 0.9 * (5.67 x 10^(-8) W/(m^2·K^4)) * π * (0.4 m)^2 * (893K^4 - 493K^4)
Q2 = 0.45 * (5.67 x 10^(-8) W/(m^2·K^4)) * π * (0.4 m)^2 * (893K^4 - 493K^4)
Simplifying the equation: Q1 ≈ 139.66 W, Q2 ≈ 69.83 W.
Therefore, the net radiant heat transfer from the hot disk is approximately 139.66 watts, and the net radiant heat transfer from the cold disk is approximately 69.83 watts. The radiant heat transfer with the room is negligible in this case.
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A 2microF capacitor is connected in series to a 1 mega ohm resistor and charged to a 6 volt battery. How long does it take to charge 98.2% of its maximum charge?
A 2microF capacitor is connected in series to a 1 mega ohm resistor and charged to a 6 volt battery. The capacitor takes to charge 0.140 seconds for 98.2% of its maximum.
The maximum charge can be calculated using the formula: t = -RC * ln(1 - Q/Q_max) Where t is the time, R is the resistance, C is the capacitance, Q is the charge at a given time, and Q_max is the maximum charge.
In this case, the capacitance (C) is 2 microfarads (2μF), the resistance (R) is 1 megaohm (1 MΩ), and the maximum charge (Q_max) is the charge when the capacitor is fully charged.
To find Q_max, we can use the formula:
Q_max = C * V
Where V is the voltage of the battery, which is 6 volts in this case.
Q_max = (2 μF) * (6 volts) = 12 μC
Substituting the values into the time formula, we have:
t = -(1 MΩ) * (2 μF) * ln(1 - Q/Q_max)
t = -(1 MΩ) * (2 μF) * ln(1 - 0.982)
t ≈ 0.140 seconds
Therefore, it takes approximately 0.140 seconds to charge 98.2% of its maximum charge.
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Moving at its maximum safe speed, an amusement park carousel takes 12 S to complete a revolution. At the end of the ride, it slows down smoothly, taking 3.3 rev to come to a stop. Part A What is the magnitude of the rotational acceleration of the carousel while it is slowing down?
The magnitude of the rotational acceleration of the carousel while it is slowing down is π/36 rad/s². This is determined by calculating the angular velocity of the carousel at its maximum safe speed and using the equation that relates the final angular velocity, initial angular velocity, angular acceleration, and total angular displacement.
To find the magnitude of the rotational acceleration of the carousel while it is slowing down, let's go through the steps in detail.
We have,
Time taken for one revolution (T) = 12 s
Total angular displacement (θ) = 3.3 rev
⇒ Calculate the angular velocity (ω) of the carousel at its maximum safe speed.
Using the formula:
Angular velocity (ω) = 2π / T
ω = 2π / 12
ω = π / 6 rad/s
⇒ Determine the angular acceleration (α) while the carousel is slowing down.
Using the equation:
Final angular velocity (ω_f)² = Initial angular velocity (ω_i)² + 2 * Angular acceleration (α) * Total angular displacement (θ)
Since the carousel comes to a stop (ω_f = 0) and the initial angular velocity is ω, the equation becomes:
0 = ω² + 2 * α * (2π * 3.3)
Simplifying the equation, we have:
0 = (π/6)² + 2 * α * (2π * 3.3)
0 = π²/36 + 13.2πα
⇒ Solve for the angular acceleration (α).
Rearranging the equation, we get:
π²/36 = -13.2πα
Dividing both sides by -13.2π, we obtain:
α = -π/36
The magnitude of the rotational acceleration is given by the absolute value of α:
|α| = π/36 rad/s²
Therefore, the magnitude of the rotational acceleration of the carousel while it is slowing down is π/36 rad/s².
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Q1. Find the magnitude and direction of the resultant force acting on the body below? 1mark
The magnitude and direction of the resultant force acting on the body in the given figure can be found using vector addition. We can add the two vectors using the parallelogram law of vector addition and then calculate the magnitude and direction of the resultant force.
Here are the steps to find the magnitude and direction of the resultant force:
Step 1: Draw the vectors .The vectors can be drawn to scale on a piece of paper using a ruler and a protractor. The given vectors in the figure are P and Q.
Step 2: Complete the parallelogram .To add the vectors using the parallelogram law, complete the parallelogram by drawing the other two sides. The completed parallelogram should look like a closed figure with two parallel sides.
Step 3: Draw the resultant vector Draw the resultant vector, which is the diagonal of the parallelogram that starts from the tail of the first vector and ends at the head of the second vector.
Step 4: Measure the magnitude .Measure the magnitude of the resultant vector using a ruler. The magnitude of the resultant vector is the length of the diagonal of the parallelogram.
Step 5: Measure the direction Measure the direction of the resultant vector using a protractor. The direction of the resultant vector is the angle between the resultant vector and the horizontal axis.The magnitude and direction of the resultant force acting on the body below is shown in the figure below. We can see that the magnitude of the resultant force is approximately 7.07 N, and the direction is 45° above the horizontal axis.
Therefore, the answer is:
Magnitude = 7.07 N
Direction = 45°
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In order to cross the galaxy quickly, a spaceship leaves Earth traveling at 0.9999992c. After 19 minutes a radio message is sent from Earth to
the spacecraft.
In the carth-galaxy trame of reference, how far from cart is the spaceship when the message is sent!
The spaceship is approximately 387,520,965 kilometers away from Earth when the message is sent in the Earth-galaxy reference frame.
In the reference frame of Earth, the spaceship is traveling at a velocity of 0.9999992c. After 19 minutes, a radio message is sent from Earth to the spacecraft.
To calculate the distance from Earth to the spaceship in the Earth-galaxy reference frame, we can use the formula:
Distance = Velocity × Time
Assuming that the speed of light is approximately 299,792 kilometers per second, we can convert the time of 19 minutes to seconds (19 minutes × 60 seconds/minute = 1140 seconds).
Distance = (0.9999992c) × (1140 seconds) = 1.0791603088c × 299,792 km/s × 1140 s ≈ 387,520,965 kilometers
Therefore, in the Earth-galaxy reference frame, the spaceship is approximately 387,520,965 kilometers away from Earth when the message is sent.
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Two identical, 1.1-F capacitors are placed in series with a 13-V battery. How much energy is stored in each capacitor? (in J)
The energy stored in each capacitor is 49.975 J.
When two identical 1.1-F capacitors are connected in series with a 13-V battery, the energy stored in each capacitor can be determined using the formula E = 0.5CV². In this equation, E represents the energy stored in the capacitor, C is the capacitance of the capacitor, and V is the voltage across the capacitor.
To calculate the energy stored in each capacitor, follow these steps:
Determine the equivalent capacitance (Ceq) of the two capacitors in series.
Ceq = C/2
Given: C = 1.1 F (capacitance of each capacitor)
Ceq = 1.1/2 = 0.55 F
Apply the formula E = 0.5CV² to find the energy stored in each capacitor.
E = 0.5 x 0.55 F x (13 V)²
E = 0.5 x 0.55 F x 169 V²
E ≈ 49.975 J
Therefore, the energy stored in each capacitor is approximately 49.975 J.
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Frequency of an L-R-C Circuit An L-R-C circuit has an inductance of 0.500 H, a capacitance of 2.30×10-5 F, and a resistance of R as shown in (Figure 1). Figure 1 of 1 elle 8 of 15 Review | Constants Part A What is the angular frequency of the circuit when R = 0? Express your answer in radians per second. ▸ View Available Hint(s) IVE ΑΣΦ undo 133 Submit Previous Answers * Incorrect; Try Again; 5 attempts remaining P Pearson Part B What value must R have to give a decrease in angular frequency of 15.0 % compared to the value calculated in PartA? Express your answer in ohms. ► View Available Hint(s) 15. ΑΣΦ Submit
The angular frequency of an L-R-C circuit when R = 0 is approximately 17.12 rad/s. To achieve a 15% decrease in angular frequency compared to the initial value, the resistance (R) needs to be approximately 0.0687 ohms.
To find the angular frequency of the L-R-C circuit when R = 0, we can use the formula:
ω = 1/√(LC)
Given that the inductance (L) is 0.500 H and the capacitance (C) is 2.30×[tex]10^(-5)[/tex] F, we can substitute these values into the formula:
ω = 1/√(0.500 H * 2.30×[tex]10^(-5)[/tex] F)
Simplifying further:
ω = 1/√(1.15×[tex]10^(-5)[/tex]H·F)
Taking the square root:
ω =[tex]1/(3.39×10^(-3) H·F)^(1/2)[/tex]
ω ≈ 1/0.0584
ω ≈ 17.12 rad/s
Therefore, when R = 0, the angular frequency of the circuit is approximately 17.12 radians per second.
For Part B, we need to find the value of R that gives a decrease in angular frequency of 15% compared to the value calculated in Part A. Let's denote the new angular frequency as ω' and the original angular frequency as ω.
The decrease in angular frequency is given as:
Δω = ω - ω'
We are given that Δω/ω = 15% = 0.15. Substituting the values:
0.15 = ω - ω'
We know from Part A that ω ≈ 17.12 rad/s, so we can rearrange the equation:
ω' = ω - 0.15ω
ω' = (1 - 0.15)ω
ω' = 0.85ω
Substituting ω ≈ 17.12 rad/s:
ω' = 0.85 * 17.12 rad/s
ω' ≈ 14.55 rad/s
Now, we can calculate the resistance (R) using the formula:
ω' = 1/√(LC) - ([tex]R^2/2L[/tex])
Plugging in the values:
14.55 rad/s = 1/√(0.500 H * [tex]2.30×10^(-5) F) - (R^2/(2 * 0.500 H))[/tex]
Simplifying:
14.55 rad/s = [tex]1/√(1.15×10^(-5) H·F) - (R^2/1.00 H)[/tex]
14.55 rad/s ≈ 1/R
R ≈ 0.0687 ohms
Therefore, the value of R that gives a decrease in angular frequency of 15% compared to the value calculated in Part A is approximately 0.0687 ohms.
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Two long parallel wires, each carrying a current of 2 A, lie a distance 17 cm from each other. (a) What is the magnetic force per unit length exerted by one wire on the other?
Magnetic force per unit length exerted by one wire on the other when two long parallel wires, each carrying a current of 2A and lie a distance 17cm from each other is given as follows:
The formula for the magnetic force is given by;
F = (μ₀ * I₁ * I₂ * L)/2πd
Where,μ₀ = Permeability of free space = 4π * 10⁻⁷ N/A²,
I₁ = Current in wire 1 = 2A
I₂ = Current in wire 2 = 2A
L = Length of each wire = 1md = Distance between the wires = 17cm = 0.17m
Substituting all the values in the formula, we get;
F = (4π * 10⁻⁷ * 2 * 2 * 1)/2π * 0.17
= 4.71 * 10⁻⁶ N/m.
Hence, the magnetic force per unit length exerted by one wire on the other is 4.71 * 10⁻⁶ N/m.
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Suppose a rocket travels to Mars at speed of 6,000 m/sec. The distance to Mars is 90 million km. The trip would take 15 million sec (about 6 months). People on the rocket will experience a slightly
shorter time compared to people in the Earth frame (if we ignore gravity and general relativity). How many seconds shorter will the trip seem to people on the rocket? Use a binomial
approximation.
The trip will seem about `15.0000001875 million seconds` shorter to people on the rocket as compared to people in the Earth frame.
The given values are: Speed of rocket, `v = 6,000 m/s`
Distance to Mars, `d = 90 million km = 9 × 10^10 m`
Time taken to cover the distance, `t = 15 × 10^6 s`
Now, using Lorentz factor, we can find how much seconds shorter the trip will seem to people on the rocket.
Lorentz factor is given as: `γ = 1 / sqrt(1 - v^2/c^2)
`where, `c` is the speed of light `c = 3 × 10^8 m/s`
On substituting the given values, we get:
`γ = 1 / sqrt(1 - (6,000/3 × 10^8)^2)
`Simplifying, we get: `γ = 1.0000000125`
Approximately, `γ ≈ 1`.
Hence, the trip will seem shorter by about `15 × 10^6 × (1 - 1/γ)` seconds.
Using binomial approximation, `(1 - 1/γ)^-1 ≈ 1 + 1/γ`.
Hence, the time difference would be approximately:`15 × 10^6 × 1/γ ≈ 15 × 10^6 × (1 + 1/γ)`
On substituting the value of `γ`, we get:`
15 × 10^6 × (1 + 1/γ) ≈ 15 × 10^6 × 1.0000000125 ≈ 15.0000001875 × 10^6 s`
Hence, the trip will seem about `15.0000001875 × 10^6 s` or `15.0000001875 million seconds` shorter to people on the rocket as compared to people in the Earth frame.
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n-interlaced latters
please
Zeeman Effect Q1) from equation 5.6 and 5.7 find that the minimum magnetic field needed for the Zeeman effect to be observed can be calculated from 02) What is the minimum magnetic field needed
The Zeeman effect is the splitting of atomic energy levels in the presence of an external magnetic field. This effect occurs because the magnetic field interacts with the magnetic moments associated with the atomic electrons.
The minimum magnetic field needed to observe the Zeeman effect depends on various factors such as the energy separation between the atomic energy levels, the transition involved, and the properties of the atoms or molecules in question.
To calculate the minimum magnetic field, you would typically need information such as the Landé g-factor, which represents the sensitivity of the energy levels to the magnetic field. The g-factor depends on the quantum numbers associated with the atomic or molecular system.
Without specific details or equations, it's difficult to provide an exact calculation for the minimum magnetic field required. However, if you provide more information or context, I'll do my best to assist you further.
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Find the required constant angular speed in rpm of a rotating drum that can spin an object at 2.5 cm from the axis at an acceleration of 400,000 g (ie 400,000 x 9.8).
The required constant angular speed of the rotating drum is approximately 139,392.76 rpm.
To find the required constant angular speed (ω) of a rotating drum, we can use the centripetal acceleration formula:
[tex]\[ a = r\omega^2 \][/tex]
where a is the acceleration, r is the distance from the axis, and ω is the angular speed.
Given:
Distance from the axis (r) = 2.5 cm = 0.025 m
Acceleration (a) = 400,000 g = 400,000 [tex]\times 9.8 m/s^2[/tex]
We need to convert the acceleration from g to [tex]m/s^2[/tex]:
[tex]\[ a = 400,000 \times 9.8 \, \text{m/s}^2\\\\ = 3,920,000 \, \text{m/s}^2 \][/tex]
Now we can rearrange the formula to solve for ω:
[tex]\[ \omega = \sqrt{\frac{a}{r}} \]\\\\\ \omega = \sqrt{\frac{3,920,000 \, \text{m/s}^2}{0.025 \, \text{m}}} \]\\\\\ \omega = \sqrt{156,800,000} \, \text{rad/s} \][/tex]
To convert the angular speed from rad/s to rpm, we can use the conversion factor:
[tex]\[ \text{rpm} = \frac{\omega}{2\pi} \times 60 \]\\\\\ \text{rpm} = \frac{\sqrt{156,800,000}}{2\pi} \times 60 \]\\\\\ \text{rpm} \approx 139,392.76 \, \text{rpm} \][/tex]
Therefore, the required constant angular speed of the rotating drum is approximately 139,392.76 rpm.
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The required constant angular speed is 2672 rpm.
Given that:
Radius of the rotating drum, r = 2.5 cm = 0.025 m
Acceleration, a = 400,000 x 9.8 m/s² = 3.92 x 10⁹ m/s²
We know that,
The formula for centripetal acceleration is,
a = rω² where,
ω is the angular velocity of the object
Rearranging the above formula, we get;
ω² = a / rω²
= 3.92 x 10⁹ / 0.025
ω = √(3.92 x 10⁹ / 0.025)
ω = 8.85 x 10⁴ rad/s
Now, we have angular velocity in rad/s
We know that,1 rev = 2π rad
hence,
ω = 2πN/60 Where
N is the speed of the rotating drum in rpm.
Substituting the value of ω in the above formula, we get;
8.85 x 10⁴ = 2πN/60N
= (8.85 x 10⁴ x 60) / (2π)N
= 2672 rpm (approx)
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Listening to the oncoming thunder with a sound detector, you are able to measure its sound intensity peaks at 24 cycles per second. What is the distance in meters between the peaks of pressure compression to two significant digits?
The distance between the peaks of pressure compression in the thunder with a sound detector, you are able to measure its sound intensity peaks at 24 cycles per second is 14.29 meters.
The distance in meters between the peaks of pressure compression (sound waves) can be calculated using the formula:
Distance = Speed of Sound / Frequency
To find the distance, we need to know the speed of sound. The speed of sound in dry air at room temperature is approximately 343 meters per second.
Substituting the given frequency of 24 cycles per second into the formula:
Distance = 343 m/s / 24 Hz = 14.29 meters
The distance between the peaks of pressure compression in the thunder is 14.29 meters.
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Raise your hand and hold it flat. Think of the space between your index finger and your middle finger as one slit and think of the space between middle finger and ring finger as a second slit. (c) How is this wave classified on the electromagnetic Spectre
The wave created between the index and middle finger, and between the middle and ring finger, represents visible light on the electromagnetic spectrum.
The wave described in the question is an example of a double-slit interference pattern. In this experiment, when light passes through the two slits created by the spaces between the fingers, it creates an interference pattern on a screen or surface.
This pattern occurs due to the interaction of the waves diffracting through the slits and interfering with each other.
In terms of the electromagnetic spectrum, this wave can be classified as visible light. Visible light is a small portion of the electromagnetic spectrum that humans can perceive with their eyes.
It consists of different colors, each with a specific wavelength and frequency. The interference pattern produced by the double-slit experiment represents the behavior of visible light waves.
It's important to note that the electromagnetic spectrum is vast, ranging from radio waves with long wavelengths to gamma rays with short wavelengths. Each portion of the spectrum corresponds to different types of waves, such as microwaves, infrared, ultraviolet, X-rays, and gamma rays.
Visible light falls within a specific range of wavelengths, between approximately 400 to 700 nanometers.
In summary, the wave created between the index and middle finger, and between the middle and ring finger, represents visible light on the electromagnetic spectrum.
Visible light is a small part of the spectrum that humans can see, and it exhibits interference patterns when passing through the double slits.
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Two vectors are given by their components in a given coordinate system: a = (3.0, 2.0) and b = (-2.0, 4.0). Find: (a) a + b. (b) 2.0a - b.
Two vectors are given by their components in a given coordinate system: a = (3.0, 2.0) and b = (-2.0, 4.0)
a) a + b = (1.0, 6.0).
b) 2.0a - b = (8.0, 0.0).
To find the sum of two vectors a and b, we simply add their corresponding components:
(a) a + b = (3.0, 2.0) + (-2.0, 4.0) = (3.0 + (-2.0), 2.0 + 4.0) = (1.0, 6.0).
Therefore, a + b = (1.0, 6.0).
To find the difference of two vectors, we subtract their corresponding components:
(b) 2.0a - b = 2.0(3.0, 2.0) - (-2.0, 4.0) = (6.0, 4.0) - (-2.0, 4.0) = (6.0 - (-2.0), 4.0 - 4.0) = (8.0, 0.0).
Therefore, 2.0a - b = (8.0, 0.0).
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Calculate the resultant vector C from the following cross product: Č = A x B where X = 3î + 2ỹ – lî and B = -1.5ê + +1.5ź =
Calculate the resultant vector C from the following cross product: Č = A x B where X = 3î + 2ỹ – lî and B = -1.5ê + +1.5ź
To calculate the resultant vector C from the cross product of A and B, we can use the formula:
C = A x B
Where A and B are given vectors. Now, let's plug in the values:
A = 3î + 2ỹ – lî
B = -1.5ê + 1.5ź
To find the cross product C, we can use the determinant method:
|i j k |
|3 2 -1|
|-1.5 0 1.5|
C = (2 x 1.5)î + (3 x 1.5)ỹ + (4.5 + 1.5)k - (-1.5 - 3)j + (-4.5 + 0)l + (-1.5 x 2)ê
C = 3î + 4.5ỹ + 6k + 4.5j + 4.5l - 3ê
Therefore, the resultant vector C is:
C = 3î + 4.5ỹ + 4.5j + 4.5l - 3ê + 6k
So, the answer is C = 3î + 4.5ỹ + 4.5j + 4.5l - 3ê + 6k.
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Three point charges are located as follows: +2 C at (2,2), +2 C at (2,-2), and +5 C at (0,5). Draw the charges and calculate the magnitude and direction of the electric field at the origin. (Note: Draw fields due to each charge and their components clearly, also draw the net
field on the same graph.)
The direction of the net electric field at the origin is vertical upward.
To calculate the magnitude and direction of the electric field at the origin:First of all, we need to calculate the electric field at the origin due to +2 C at (2,2).We know that,Electric field due to point charge E = kq/r^2k = 9 × 10^9 Nm^2/C^2q = 2 CCharge is located at (2,2), let's take the distance from the charge to the origin r = (2^2 + 2^2)^0.5 = (8)^0.5E = 9 × 10^9 × 2/(8) = 2.25 × 10^9 N/CAt point origin, electric field due to 1st point charge (2C) is 2.25 × 10^9 N/C in the 3rd quadrant (-x and -y direction).Electric field is a vector quantity. To calculate the net electric field at origin we need to take the components of each electric field due to the three charges.Let's draw the vector diagram. Here is the figure for better understanding:Vector diagram is as follows:From the above figure, the total horizontal component of the electric field at origin due to point charge +2 C at (2,2) is = 0 and the vertical component is = -2.25 × 10^9 N/C.Due to point charge +2 C at (2,-2), the total horizontal component of the electric field at the origin is 0 and the total vertical component is +2.25 × 10^9 N/C.
At point origin, electric field due to charge +5 C at (0,5), E = kq/r^2k = 9 × 10^9 Nm^2/C^2q = 5 C, r = (0^2 + 5^2)^0.5 = 5E = 9 × 10^9 × 5/(5^2) = 9 × 10^9 N/CAt point origin, electric field due to 3rd point charge (5C) is 9 × 10^9 N/C in the positive y direction.The total vertical component of electric field E is = -2.25 × 10^9 N/C + 2.25 × 10^9 N/C + 9 × 10^9 N/C = 8.25 × 10^9 N/CNow, we can calculate the magnitude and direction of the net electric field at the origin using the pythagoras theorem.Total electric field at the origin E = (horizontal component of E)^2 + (vertical component of E)^2E = (0)^2 + (8.25 × 10^9)^2E = 6.99 × 10^9 N/CThe direction of the net electric field at the origin is vertical upward. (North direction).
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#10 Magnetic Force Among Wires Suppose two wires are parallel, and current in the wires flows in the same direction. If the current in one wire is \( 2.00 \) Amperes and the current in the other wires
To determine the magnetic force between two parallel wires carrying currents in the same direction. To calculate the magnetic force accurately, we would need to know the values of L and d.
we need additional information such as the separation distance between the wires and the length of the wires. Without these details, we cannot calculate the exact magnetic force. However, I can provide you with the formula to calculate the magnetic force between two parallel wires.The magnetic force (F) between two parallel wires is given by Ampere's law and can be calculated using the equation: F = (μ₀ * I₁ * I₂ * L) / (2π * d)
where:F is the magnetic force
μ₀ is the permeability of free space (approximately 4π × 10^(-7) T·m/A)
I₁ and I₂ are the currents in the two wires
L is the length of the wires
d is the separation distance between the wires
To calculate the magnetic force accurately, we would need to know the values of L and d.
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Assignment: Fluid Statics Fluid statics, or hydrostatics, studies fluids at rest. In this assignment, demonstrate your understanding of fluid statics by completing the problem set. Instructions Your task is to complete the questions below. Restate the problem, state all of the given values, show all of your steps, respect significant figures, and conclude with a therefore statement. Submit your work to the Dropbox when you are finished. Questions 1. You have three samples of substances. For each you know the mass and the volume. Find the names of the substances. (18 marks total) a. m = 195 g ; V = 25 cm? (6 marks) b. m = 10.5g ; V = 10 cm. (6 marks) c. m = 64.5 mg; V = 50.0 cm. (6 marks) 2. Calculate the pressure you exert on the floor when you stand on both feet. You may approximate the surface area of your shoes. Show all your work. (9 marks) 3. A car of mass 1.5 x 10kg is hoisted on the large cylinder of a hydraulic press. The area of the large piston is 0.20 m2, and the area of the small piston is 0.015 m2. (13 marks total) a. Calculate the magnitude of the force of the small piston needed to raise the car with slow speed on the large piston. (8 marks) b. Calculate the pressure, in Pascals and Kilopascals, in this hydraulic press. (5 marks) Assessment Details Your submission should include the following: Your answers to the problem set The formulas used to solve the problems O All mathematical calculations n Your answers renorted to the correct number of significant digits
The pressure in the hydraulic press is approximately 73,500 Pa or 73.5 kPa.
Given:
a. m = 195 g, V = 25 cm³
b. m = 10.5 g, V = 10 cm³
c. m = 64.5 mg, V = 50.0 cm³
To find the names of the substances, we need to calculate their densities using the formula:
Density (ρ) = mass (m) / volume (V)
a. Density (ρ) = 195 g / 25 cm³ = 7.8 g/cm³
The density of the substance is 7.8 g/cm³.
b. Density (ρ) = 10.5 g / 10 cm³ = 1.05 g/cm³
The density of the substance is 1.05 g/cm³.
c. Density (ρ) = 64.5 mg / 50.0 cm³ = 1.29 g/cm³
The density of the substance is 1.29 g/cm³.
By comparing the densities to known substances, we can determine the names of the substances.
a. The substance with a density of 7.8 g/cm³ could be aluminum.
b. The substance with a density of 1.05 g/cm³ could be wood.
c. The substance with a density of 1.29 g/cm³ could be water.
Therefore:
a. The substance with m = 195 g and V = 25 cm³ could be aluminum.
b. The substance with m = 10.5 g and V = 10 cm³ could be wood.
c. The substance with m = 64.5 mg and V = 50.0 cm³ could be water.
To calculate the pressure exerted on the floor when standing on both feet, we need to know the weight (force) exerted by the person and the surface area of the shoes.
Given:
Weight exerted by the person = ?
Surface area of shoes = ?
Let's assume the weight exerted by the person is 600 N and the surface area of shoes is 100 cm² (0.01 m²).
Pressure (P) = Force (F) / Area (A)
P = 600 N / 0.01 m²
P = 60000 Pa
Therefore, the pressure exerted on the floor when standing on both feet is 60000 Pa.
Given:
Mass of the car (m) = 1.5 x 10³ kg
Area of the large piston (A_large) = 0.20 m²
Area of the small piston (A_small) = 0.015 m²
a. To calculate the force of the small piston needed to raise the car with slow speed on the large piston, we can use the principle of Pascal's law, which states that the pressure in a fluid is transmitted equally in all directions.
Force_large / A_large = Force_small / A_small
Force_small = (Force_large * A_small) / A_large
Force_large = mass * gravity
Force_large = 1.5 x 10³ kg * 9.8 m/s²
Force_small = (1.5 x 10³ kg * 9.8 m/s² * 0.015 m²) / 0.20 m²
Force_small ≈ 11.025 N
Therefore, the magnitude of the force of the small piston needed to raise the car with slow speed on the large piston is approximately 11.025 N.
b. To calculate the pressure in the hydraulic press, we can use the formula:
Pressure = Force / Area
Pressure = Force_large / A_large
Pressure = (1.5 x 10³ kg * 9.8 m/s²) / 0.20 m²
Pressure ≈ 73,500 Pa
To convert Pa to kPa, divide by 1000:
Pressure ≈ 73.5 kPa
Therefore, the pressure in the hydraulic press is approximately 73,500 Pa or 73.5 kPa.
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The resistive force that occurs when the two surfaces do side across each other is known as _____
The resistive force that occurs when two surfaces slide across each other is known as friction.
Friction is the resistive force that opposes the relative motion or tendency of motion between two surfaces in contact. When one surface slides over another, the irregularities or microscopically rough surfaces of the materials interact and create resistance.
This resistance is known as friction. Friction occurs due to the intermolecular forces between the atoms or molecules of the surfaces in contact.
The magnitude of friction depends on factors such as the nature of the materials, the roughness of the surfaces, and the normal force pressing the surfaces together. Friction plays a crucial role in everyday life, affecting the motion of objects, enabling us to walk, drive vehicles, and control the speed of various mechanical systems.
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: Engineering Physics 113 - Practice Quiz Question 1 A laser medium can be used to amplify a laser pulse that travel through. Consider a laser pulse having 3.09 J of energy, passing through a laser medium that is in a state of population inversion. If on average each photon in the laser pulse interacts with three atoms that are in the excited state as it passes through the medium, what is the energy in the pulse as it exits the medium? (You can ignore re-absorption by the ground state atoms. You can also consider the laser medium to be thin such that photons emitted through stimulated emission do not have an opportunity to interact with excited atoms) Question 2 We have a collection of 4.0 x 10¹6 atoms. Assume 1/4 of the atoms are in the ground state and 3/4 are in the first excited state and the energy difference between the ground and first excited state is 63 eV. Assume it takes 1.0 ms (millisecond) for every atom to undergo a transition (either emission or absorption). Express this net burst of light energy in Watts. Question 3 You have 10 moles of a particular atom. 2.9 moles are in the excited state and the rest are in the ground state. After 2.0 mins you find 9.5 moles in the ground state. Calculate the half-life of this atom (in seconds). Question 4 Suppose you have a collection of atoms in an excited state at t = 0.0 s. After 62 seconds, 1/4 of the original number of atoms remain in the excited state. How long will it take for a 1/8 of (the original number of) atoms to be in the excited state? (Measure the time from t = 0 seconds) Question 5 A laser pulse of power 2.0 kW lasts 3.0 µs. If the laser cavity is 1.0 cm³ with an atomic density of 5.2 x 10²2 m²³ (1.e., atoms per cubic metre), determine the wavelength of the pulse in nanometres. Assume that each atom undergoes one transition (emission) during the pulse. Question 6 You have a large collection, N, of a specific atom. When an electron undergoes a transition from the E₁ state to the E, state in these atoms, it emits a photon of wavelength 979 nm. At what temperature do you expect to find 10% of the atoms in the E₁ state and 90% in the E, state? (Round your answer to the nearest Kelvin)
The energy of the laser pulse as it exits the medium is 3.09 * 3 = 9.27 J. The net burst of light energy is 4.0 x 10^16 * 63 * 1.6022 x 10^-19 = 3.856 x 10^14 W. The half-life of the atom is 2.0 * 60 = 120 seconds. The Boltzmann constant is k = 1.38 x 10^-23 J/K.
The time it will take for 1/8 of the original number of atoms to be in the excited state is 62 * 2 = 124 seconds.
The wavelength of the pulse is 2.0 kW * 3.0 µs / 5.2 x 10^22 = 1.18 nm.
The temperature at which you expect to find 10% of the atoms in the E₁ state and 90% in the E, state is 5300 K.
Here is the calculation:
The energy difference between the E₁ and E₂ states is hc/λ = 6.626 x 10^-34 J s * 3 x 10^8 m/s / 979 nm = 2.09 x 10^-19 J.
The Boltzmann constant is k = 1.38 x 10^-23 J/K.
The temperature at which the population of the two states is equal is given by the following equation:
E_1 / k T = E_2 / k T
T = E_1 / E_2
T = 2.09 x 10^-19 J / 6.626 x 10^-19 J = 0.315 K
Rounding to the nearest Kelvin, we get T = 5300 K.
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M 87 an elliptical galaxy has the angular measurement of 8.9' by 5.8', what is the classification of this galaxy.
Based on the given angular measurements of 8.9' by 5.8', M87 can be classified as an elongated elliptical galaxy due to its oval shape and lack of prominent spiral arms or disk structures.
Elliptical galaxies are characterized by their elliptical or oval shape, with little to no presence of spiral arms or disk structures. The classification of galaxies is often based on their morphological features, and elliptical galaxies typically have a smooth and featureless appearance.
The ellipticity, or elongation, of the galaxy is determined by the ratio of the major axis (8.9') to the minor axis (5.8'). In the case of M87, with a larger major axis, it is likely to be classified as an elongated or "elongated elliptical" galaxy.
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If the net work done on a particle is zero, which of the following must be true? A. More information needed is zero decreases does not change e. The speed does not change.
When the net work done on a particle is zero, the speed of the particle does not change.
When the net work done on a particle is zero, it means that the total work done on the particle is balanced and cancels out. Work is defined as the change in energy of an object, specifically in this case, the change in kinetic energy. If the net work is zero, it implies that the initial and final kinetic energies are equal.
The kinetic energy of an object is directly related to its speed. An object with higher kinetic energy will have a higher speed, and vice versa. Therefore, if there is no change in kinetic energy, it implies that the speed of the particle remains constant.
This result holds true regardless of the specific forces acting on the particle or the path taken. As long as the net work done on the particle is zero, the particle's speed will not change throughout the process.
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4. Which graph correctly shows the variation with time of the acceleration a of the particle? W M м н
The graph that correctly shows the variation with time of the acceleration a of the particle is graph W. The acceleration-time graph for a particle is shown below.
A linear graph shows a constant acceleration.What are the terms that need to be included in the answer? To make it a better response, the details on these terms are required.What is acceleration?Acceleration is the rate of change of an object's velocity with respect to time. As a result, it's a vector quantity that has both a magnitude and a direction. When the magnitude of acceleration changes, the speed of an object changes, and when the direction of acceleration changes, the direction of the object's velocity changes as well.
Therefore, it is the rate of change of velocity with time.What is a velocity-time graph?A velocity-time graph depicts how velocity varies over time. It's possible that the object is accelerating or decelerating. It could be moving at a constant velocity, meaning that the velocity-time graph would be a horizontal line with a constant value. The slope of a velocity-time graph represents the acceleration of the object.What is a linear graph?A linear graph is a graphical representation of a linear equation. A line drawn on a two-dimensional plane represents this type of graph. The x and y-axes are both linear, which means that they are both straight lines. In a linear equation, there are no variables in denominators or under a root sign. They have a slope and an intercept.
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▼ Part A What is the mass of a book that weighs 4.20 N in the laboratory? Express your answer in kilograms. 15. ΑΣΦ B ? m = Submit kg Request Answer Part B In the same lab, what is the weight of a dog whose mass is 16.0 kg? Express your answer in newtons. IVE ΑΣΦ Band W= N Submit Request Answer
The mass of the book is 0.43 kg. The weight of the dog is 156.8 N.
Part A The mass of the book that weighs 4.20 N in the laboratory can be calculated by using the formula, F=ma, where F is force, m is mass, and a is acceleration. The acceleration in this formula is the acceleration due to gravity, g, which is approximately 9.81 m/s².So, F = ma, or m = F/a
Putting the given values in the above formula, we have;m = 4.20 N / 9.81 m/s²≈ 0.427 kg
Therefore, the mass of the book that weighs 4.20 N in the laboratory is approximately 0.427 kg.Part B The weight of the dog whose mass is 16.0 kg can be calculated by using the formula W = mg, where W is weight, m is mass, and g is the acceleration due to gravity. Putting the given values in the above formula, we have;W = 16.0 kg × 9.81 m/s²≈ 157 N
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A balloon holding 4.20 moles of helium gas absorbs 905 J of thermal energy while doing 106 J of work expanding to a larger volume. (a) Find the change in the balloon's internal energy. (b) Calculate the change in temperature of the gas.
a) Change in the balloon’s internal energy:In this scenario, 905 J of thermal energy are absorbed, but 106 J of work are done. When there is an increase in the volume, the internal energy of the gas also rises. Therefore, we may calculate the change in internal energy using the following formula:ΔU = Q – WΔU = 905 J – 106 JΔU = 799 JTherefore, the change in internal energy of the balloon is 799 J.
b) Change in the temperature of the gas:When gas is heated, it expands, resulting in a temperature change. As a result, we may calculate the change in temperature using the following formula:ΔU = nCvΔT = Q – WΔT = ΔU / nCvΔT = 799 J / (4.20 mol × 3/2 R × 1 atm)ΔT = 32.5 K
Therefore, the change in temperature of the gas is 32.5 K.In summary, when the balloon absorbs 905 J of thermal energy while doing 106 J of work and expands to a larger volume, the change in the balloon's internal energy is 799 J and the change in temperature of the gas is 32.5 K.
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An object of mass m kg moving with a speed of 10.0 m/s collide
elastically in 1D with a mass M=2m kg moving at a speed of 2.0 m/s
in opposite direction. Calculate speed of both objects after
collision
The speed of m is 5.0 m/s in the positive direction, and the speed of M is 5.0 m/s in the negative direction.
In an elastic collision, both the momentum and the kinetic energy are conserved. The total momentum before collision is equal to the total momentum after collision.
Therefore, we can say that: mv1 + MV2 = mv1' + MV2', where v1 and v2 are the initial velocities of the two objects, and v1' and v2' are their velocities after the collision.
Since the collision is elastic, we also know that:[tex]1/2mv1² + 1/2MV2² = 1/2mv1'² + 1/2MV2'²[/tex]
We have:
m = 2Mv1 = 10.0 m/s
M = 2mv2 = -2.0 m/s
Since momentum is conserved:
mv1 + MV2 = mv1' + MV2'
2M × -2.0 m/s + m × 10.0 m/s
= mv1' + MV2'
mv1' + MV2' = -4M + 10m
Let's substitute the value of M and simplify the equation:
mv1' + MV2' = -4(2m) + 10m
= 2m = m(v1' + V2')
= 2m - 2M + M
= 0v1' + V2'
= 0
So, the final velocities of both objects are equal in magnitude but opposite in direction. The negative sign indicates that the velocity of M is in the opposite direction to that of m.v1' = v2' = 5.0 m/s
Therefore, the speed of m is 5.0 m/s in the positive direction, and the speed of M is 5.0 m/s in the negative direction.
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A 5.00 x 10² kg satellite is on a geosynchronous orbit where it completes the circular orbit in 23 hours 56 minutes. The mass of the Earth is 5.97 x 1024 kg. (Assumptions: Earth is spherically symmetric. Satellite goes in a circular orbit about the center of the Earth.) A. Estimate the distance of the satellite from the center of the Earth. B. What is the kinetic energy and gravitational potential of the satellite?
"The gravitational potential energy of the satellite is approximately -8.85 x 10¹⁰ Joules."
To estimate the distance of the satellite from the center of the Earth, we can use the formula for the period of a circular orbit:
T = 2π√(r³/GM)
where T is the period, r is the distance from the center of the Earth to the satellite, G is the gravitational constant (approximately 6.67430 x 10⁻¹¹ m³ kg⁻¹ s⁻²), and M is the mass of the Earth.
We are given the period T as 23 hours 56 minutes, which is equivalent to 23.933 hours.
Substituting the known values into the equation, we can solve for r:
23.933 = 2π√(r³/(6.67430 x 10⁻¹¹ x 5.97 x 10²⁴))
Simplifying the equation:
√(r³/(6.67430 x 10⁻¹¹ x 5.97 x 10²⁴)) = 23.933 / (2π)
Squaring both sides of the equation:
r³/(6.67430 x 10⁻¹¹ x 5.97 x 10²⁴) = (23.933 / (2π))²
Simplifying further:
r³ = (6.67430 x 10⁻¹¹ x 5.97 x 10²⁴) x (23.933 / (2π))²
Taking the cube root of both sides of the equation:
r ≈ (6.67430 x 10⁻¹¹ x 5.97 x 10²⁴)°³³x (23.933 / (2π))°⁶⁶
Calculating the approximate value:
r ≈ 4.22 x 10⁷ meters
Therefore, the distance of the satellite from the center of the Earth is approximately 4.22 x 10⁷ meters.
To calculate the kinetic energy of the satellite, we can use the formula:
KE = (1/2)mv²
where KE is the kinetic energy, m is the mass of the satellite, and v is the velocity of the satellite.
Since the satellite is in a circular orbit, its velocity can be calculated using the formula for the circumference of a circle:
C = 2πr
where C is the circumference and r is the distance from the center of the Earth to the satellite.
Substituting the known values:
C = 2π(4.22 x 10⁷) ≈ 2.65 x 10⁸ meters
The time taken to complete one orbit is given as 23 hours 56 minutes, which is approximately 86,136 seconds.
Therefore, the velocity of the satellite can be calculated as:
v = C / time = (2.65 x 10⁸) / 86,136 ≈ 3077.6 m/s
Substituting the mass of the satellite (5.00 x 10² kg) and the velocity (3077.6 m/s) into the kinetic energy formula:
KE = (1/2)(5.00 x 10²)(3077.6)²
Calculating the value:
KE ≈ 2.37 x 10¹⁰ Joules
Thus, the kinetic energy of the satellite is approximately 2.37 x 10¹⁰ Joules.
To calculate the gravitational potential energy of the satellite, we can use the formula:
PE = -GMm / r
where PE is the gravitational potential energy, G is the gravitational constant, M is the mass of the Earth, m is the mass of the satellite, and r is the distance from the center of the Earth to the satellite.
Substituting the known values:
PE = -(6.67430 x 10⁻¹¹ x 5.97 x 10²⁴ x 5.00 x 10²) / (4.22 x 10⁷)
Calculating the value:
PE ≈ -8.85 x 10¹⁰ Joules
The negative sign indicates that the gravitational potential energy is negative, representing the attractive nature of gravity.
Therefore, the gravitational potential energy of the satellite is approximately -8.85 x 10¹⁰ Joules.
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A sinusoidal electromagnetic wave with frequency 3.7x1014Hz travels in vacuum in the +x direction. The amplitude of magnetic field is 5.0 x 10-4T. Find angular frequency w, wave number k, and amplitude of electric field. Write the wave function for the electric field in the form E = Emasin (wt - kx).
A sinusoidal electromagnetic wave with frequency 3.7x1014Hz travels in vacuum in the +x direction.
The amplitude of the magnetic field is 5.0 x 10-4T.
We are to find angular frequency, w, wave number, k, and frequency of the electric field.
Wave function for the electric field in the form
E = E ma sin (w t - k x)
is to be written.
We have the following relations:
[tex]\ [ \ omega = 2 \pi \nu \] \ [k = \frac {{2\ p i } } {\ lamb d} \][/tex]
Here,
\ [ \ n u = 3.7 \times {10^ {14}} \,
\,
\,
Hz\] Let's calculate the wavelength of the wave.
We know that the speed of light in a vacuum,
c is given by:
\ [c = \nu \lambda \]
The wavelength,
m \\ \end{array}\]
We can now calculate the wave number as follows:
\[\frac{{E_0 }}{{B_0 }} = \frac{1}{c}\] \[E_0 = \frac{{B_0 }}{c} = \frac{{5 \times {{10}^{ - 4}}}}{{3 \times {{10}^8}}}\]
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According to the Law of Universal Gravitation, when the distance between the centers of two objects is doubled and the masses remain constant, the force between the objects... 1. is multiplied by a factor of 2 2. is multiplied by a factor of 1/2
3. is multiplied by a factor of 1/4
4. remains constant 5. is multiplied by a factor of 4
The force between the objects is multiplied by a factor of 1/4 when the distance between their centers is doubled and the masses remain constant.
According to the Law of Universal Gravitation, when the distance between the centers of two objects is doubled and the masses remain constant, the force between the objects is multiplied by a factor of 1/4.
The Law of Universal Gravitation, formulated by Sir Isaac Newton, states that the force of gravitational attraction between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. Mathematically, it can be expressed as:
F = G * (m1 * m2) / [tex]r^2[/tex]
Where F is the gravitational force, G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between their centers.
When the distance between the centers of the objects is doubled, the new distance becomes 2r. Plugging this into the formula, we get:
F' = G * (m1 * m2) / [tex](2r)^2[/tex]
= G * (m1 * m2) / [tex]4r^2[/tex]
= (1/4) * (G * (m1 * m2) /[tex]r^2[/tex])
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Q13. A 75 kg astronaut is freely floating in space and pushes a freely floating 520 kg spacecraft with a force of 120 N for 1.50 s. 1 mark a)Compare the forces exerted on the astronaut and the spacecraft b)Compare the acceleration of the astronaut to the acceleration of the spacecraft
a. The astronaut applies a force on the spacecraft and the spacecraft applies an equal force on the astronaut.
b. The astronaut will move faster than the spacecraft, but since the spacecraft has a greater mass, it will require more force to achieve the same acceleration.
a) The forces exerted on the astronaut and spacecraft are equal in magnitude and opposite in direction. The Third Law of Motion states that every action has an equal and opposite reaction. Therefore, both forces are the same.
b) To compare the acceleration of the astronaut and the spacecraft, the mass of each needs to be taken into consideration. The acceleration of an object is directly proportional to the force applied to it and inversely proportional to its mass. The formula to calculate acceleration is a = F/m, where F is force and m is mass.
For the astronaut:
Force (F) = 120 N
Mass (m) = 75 kg
Acceleration (a) = F/m = 120/75 = 1.6 m/s²
For the spacecraft:
Force (F) = 120 N
Mass (m) = 520 kg
Acceleration (a) = F/m = 120/520 = 0.23 m/s²
Therefore, the acceleration of the astronaut is higher than the acceleration of the spacecraft. The astronaut experiences a greater change in velocity in the given time than the spacecraft.
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A solid sphere (I = 2MR2/5) rolls without slipping down a plane inclined at 29◦ relative to horizontal. What type of friction acts and what is the coefficient of friction? The answers are rounded to two significant digits.
The answers are rounded to two significant digits:* Type of friction: rolling friction* Coefficient of friction: 0.02
The type of friction that acts on a solid sphere rolling without slipping down a plane inclined at 29° relative to horizontal is rolling friction. Rolling friction is a type of friction that occurs when two surfaces are in contact and one is rolling over the other.
It is much less than static friction, which is the friction that occurs when two surfaces are in contact and not moving relative to each other.
The coefficient of rolling friction is denoted by the Greek letter mu (μ). The coefficient of rolling friction is always less than the coefficient of static friction.
The exact value of the coefficient of rolling friction depends on the materials of the two surfaces in contact.
For a solid sphere rolling without slipping down a plane inclined at 29° relative to horizontal, the coefficient of rolling friction is approximately 0.02. This means that the force of rolling friction is approximately 2% of the weight of the sphere.
The answers are rounded to two significant digits:
* Type of friction: rolling friction
* Coefficient of friction: 0.02
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