2048.77 inches space needed to be allowed for expansion
To calculate the expansion space required for a steel walkway that spans a 170 ft 8.77 inch gap.
we need to consider the walkway's coefficient of thermal expansion and the temperature range it's designed for. Using the given coefficient of and the temperature range of -32.4 C to 39.4 C, we can calculate the expansion space required in inches, which turns out to be 2.39 inches.
The expansion space required for the steel walkway can be calculated using the following formula:
ΔL = L * α * ΔT
Where ΔL is the change in length of the walkway, L is the original length (in this case, the length of the gap the walkway spans), α is the coefficient of thermal expansion, and ΔT is the temperature difference.
[tex]ΔL = 170 ft 8.77 in * (18.4 \times 10^-6 mm/mmC) * (39.4 C - (-32.4 C))[/tex]
Converting the length to inches and the temperature difference to Fahrenheit and Simplifying this expression, we get
ΔL=170ft8.77in∗(18.4×10 − 6mm/mmC)∗(39.4C−(−32.4C))
Therefore, the expansion space required for the steel walkway is 2.39 inches. This means that the gap the walkway spans should be slightly larger than its original length to allow for thermal expansion and prevent buckling or distortion.
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MA2: A-5 uC charge travels from left to right through a magnetic field pointed out of the board. What is the direction and magnitude of the force acting on the charge, if it travels at 200 m/s and the field is 7 x 10-5 T? Sketch the scenario.
Given:
Charge q = +5 µC = 5 × 10⁻⁶ C
Velocity of charge, v = 200 m/s
Magnetic field strength, B = 7 × 10⁻⁵ T
Answer: The direction of the force acting on the charge is upwards and the magnitude of the force is 7 × 10⁻⁷ N.
To determine:
The direction and magnitude of the force acting on the charge.
Sketch the scenario using right-hand rule. The force acting on a moving charged particle in a magnetic field can be determined using the equation;
F = qvBsinθ
Where, q is the charge of the
is the velocity of the particle
B is the magnetic field strength
θ is the angle between the velocity of the particle and the magnetic field strength
In this problem, the magnetic field is pointing out of the board. The direction of the magnetic field is perpendicular to the direction of the velocity of the charge. Therefore, the angle between the velocity of the charge and the magnetic field strength is 90°.
sin90° = 1
Putting the values of q, v, B, and sinθ in the above equation,
F= 5 × 10⁻⁶ × 200 × 7 × 10⁻⁵ × 1
= 7 × 10⁻⁷ N
The direction of the force acting on the charge can be determined using the right-hand rule. The thumb, forefinger, and the middle finger should be placed perpendicular to each other in such a way that the forefinger points in the direction of the magnetic field, the thumb points in the direction of the velocity of the charged particle, and the middle finger will give the direction of the force acting on the charged particle.
As per the right-hand rule, the direction of the force is upwards. Therefore, the direction of the force acting on the charge is upwards and the magnitude of the force is 7 × 10⁻⁷ N.
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How long would it take for 4*10^20 atoms to decay to 1*10^19
atoms if their half life was 14.7 years?
It would take around 17.71 years for 4 × 10²⁰ atoms to decay to 1 × 10¹⁹ atoms if their half-life was 14.7 years.
Radioactive decay is a process in which the unstable atomic nuclei emit alpha, beta, and gamma rays and particles to attain a more stable state. Half-life is the time required for half of the radioactive material to decay.
The given information isNumber of atoms present initially, N₀ = 4 × 10²⁰
Number of atoms present finally, N = 1 × 10¹⁹
Half-life of the element, t₁/₂ = 14.7 years
To find the time required for the decay of atoms, we need to use the decay formula.N = N₀ (1/2)^(t/t₁/₂)
Here, N₀ is the initial number of atoms, and N is the number of atoms after time t.
Since we have to find the time required for the decay of atoms, rearrange the above formula to get t = t₁/₂ × log(N₀/N)
Substitute the given values, N₀ = 4 × 10²⁰N = 1 × 10¹⁹t₁/₂ = 14.7 years
So, t = 14.7 × log(4 × 10²⁰/1 × 10¹⁹)≈ 14.7 × 1.204 = 17.71 years (approx.)
Therefore, it would take around 17.71 years for 4 × 10²⁰ atoms to decay to 1 × 10¹⁹ atoms if their half-life was 14.7 years.
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A 110 kg man lying on a surface of negligible friction shoves a 155 g stone away from him, giving it a speed of 17.0 m/s. What speed does the man acquire as a result?
A 110 kg man lying on a surface of negligible friction shoves a 155 g stone away from him, giving it a speed of 17.0 m/s then the man's speed remains zero.
We have to determine the speed that the man acquires as a result when he shoves the 155 g stone away from him. Since there is no external force acting on the system, the momentum will be conserved. So, before the man shoves the stone, the momentum of the system will be:
m1v1 = (m1 + m2)v,
where v is the velocity of the man and m1 and m2 are the masses of the man and stone respectively. After shoving the stone, the system momentum becomes:(m1)(v1) = (m1 + m2)v where v is the final velocity of the system. Since momentum is conserved:m1v1 = (m1 + m2)v Hence, the speed that the man acquires as a result when he shoves the 155 g stone away from him is given by v = (m1v1) / (m1 + m2)= (110 kg)(0 m/s) / (110 kg + 0.155 kg)= 0 m/s
Therefore, the man's speed remains zero.
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A moving particlo is subject conservative forces only. when its kinetic energy decreases by 103, what happens to its mechanical energy?
When the kinetic energy of a moving particle decreases by 103 units due to the effect of conservative forces, then its mechanical energy will also decrease by 103 units.
Conservative forces are defined as forces that are the gradient of a scalar potential function. As a result, these forces have a unique property: they can convert mechanical energy between potential and kinetic energy and vice versa. When a particle is subjected to only conservative forces, it experiences a mechanical force that is conservative. Thus, the total mechanical energy of the particle remains constant as it moves through space.
Considering the law of conservation of energy, we have: Initial mechanical energy of the particle, Ei = Kinetic energy of the particle, Ki Final mechanical energy of the particle, Ef = Potential energy of the particle, Ui
When the kinetic energy of the moving particle decreases by 103 units, the mechanical energy of the particle also decreases by 103 units. Therefore, the new value of mechanical energy is: Ef = Ei - ΔK
Ef = Ki - ΔK
Therefore, the particle's mechanical energy will be reduced by the same amount (103 units) as its kinetic energy. Therefore, when a moving particle is subjected to conservative forces only and its kinetic energy decreases by 103 units, its mechanical energy will also decrease by 103 units.
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A lamp located 3 m directly above a point P on the floor of a
room produces at P an illuminance of 100 lm/m2. (a) What is the
luminous intensity of the lamp? (b) What is the illuminance
produced at an
A lamp located 3 m directly above a point P on the floor of a room produces at P an illuminance of 100 lm/[tex]m^2[/tex], the illuminance at the point 1 m distant from point P is 56.25 lm/[tex]m^2[/tex].
We can utilise the inverse square law for illuminance to address this problem, which states that the illuminance at a point is inversely proportional to the square of the distance from the light source.
(a) To determine the lamp's luminous intensity, we must first compute the total luminous flux emitted by the lamp.
Lumens (lm) are used to measure luminous flux. Given the illuminance at point P, we may apply the formula:
Illuminance = Luminous Flux / Area
Luminous Flux = Illuminance * Area
Area = 4π[tex]r^2[/tex] = 4π[tex](3)^2[/tex] = 36π
Luminous Flux = 100 * 36π = 3600π lm
Luminous Intensity = Luminous Flux / Solid Angle = 3600π lm / 4π sr = 900 lm/sr
Therefore, the luminous intensity of the lamp is 900 lumens per steradian.
b. To find the illuminance at a point 1 m distant from point P:
Illuminance = Illuminance at point P * (Distance at point P / Distance at new point)²
= 100 * [tex](3 / 4)^2[/tex]
= 100 * (9/16)
= 56.25 [tex]lm/m^2[/tex]
Therefore, the illuminance at the point 1 m distant from point P is 56.25 [tex]lm/m^2[/tex]
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Your question seems incomplete, the probable complete question is:
A lamp located 3 m directly above a point P on the floor of a room produces at Pan illuminance of 100 lm/m2. (a) What is the luminous intensity of the lamp? (b) What is the illuminance produced at another point on the floor, 1 m distant from P.
a) I = (100 lm/m2) × (3 m)2I = 900 lm
b) Illuminance produced at a distance of 5 m from the lamp is 36 lm/m2.
(a) The luminous intensity of the lamp is given byI = E × d2 where E is the illuminance, d is the distance from the lamp, and I is the luminous intensity. Hence,I = (100 lm/m2) × (3 m)2I = 900 lm
(b) Suppose we move to a distance of 5 m from the lamp. The illuminance produced at this distance will be
E = I/d2where d = 5 m and I is the luminous intensity of the lamp. Substituting the values, E = (900 lm)/(5 m)2E = 36 lm/m2
Therefore, the illuminance produced at a distance of 5 m from the lamp is 36 lm/m2. This can be obtained by using the formula E = I/d2, where E is the illuminance, d is the distance from the lamp, and I is the luminous intensity. Luminous intensity of the lamp is 900 lm.
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Given the operator a = d^2/dx^2 - 4x^2 and the function f(x) = e^(-x2/2) = evaluate â f(x)
The expression for â f(x) is (-2x^2) e^(-x^2/2).
To evaluate the operator â acting on the function f(x), we need to apply the operator a to the function f(x) and simplify the expression. Let's calculate it step by step:
Start with the function f(x):
f(x) = e^(-x^2/2).
Apply the operator a = d^2/dx^2 - 4x^2 to the function f(x):
â f(x) = (d^2/dx^2 - 4x^2) f(x).
Calculate the second derivative of f(x):
f''(x) = d^2/dx^2 (e^(-x^2/2)).
To find the second derivative, we can differentiate the function twice using the chain rule:
f''(x) = (d/dx)(-x e^(-x^2/2)).
Applying the product rule, we have:
f''(x) = -e^(-x^2/2) + x^2 e^(-x^2/2).
Now, substitute the calculated second derivative into the expression for â f(x):
â f(x) = f''(x) - 4x^2 f(x).
â f(x) = (-e^(-x^2/2) + x^2 e^(-x^2/2)) - 4x^2 e^(-x^2/2).
Simplify the expression:
â f(x) = -e^(-x^2/2) + x^2 e^(-x^2/2) - 4x^2 e^(-x^2/2).
â f(x) = (-1 + x^2 - 4x^2) e^(-x^2/2).
â f(x) = (x^2 - 3x^2) e^(-x^2/2).
â f(x) = (-2x^2) e^(-x^2/2).
Therefore, the expression for â f(x) is (-2x^2) e^(-x^2/2).
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Physics
4. Define refraction, absorption, reflection, index of refraction, optically dense medium, optically less dense medium, monochromatic light.
Refraction refers to the bending or change in direction of a wave as it passes from one medium to another, caused by the difference in the speed of light in the two mediums. This bending occurs due to the change in the wave's velocity and is governed by Snell's law, which relates the angles and indices of refraction of the two mediums.
Absorption is the process by which light or other electromagnetic waves are absorbed by a material. When light interacts with matter, certain wavelengths are absorbed by the material, causing the energy of the light to be converted into other forms such as heat or chemical energy.
Reflection is the phenomenon in which light or other waves bounce off the surface of an object and change direction. The angle of incidence, which is the angle between the incident wave and the normal (a line perpendicular to the surface), is equal to the angle of reflection, the angle between the reflected wave and the normal.
Index of Refraction: The index of refraction is a property of a material that quantifies how much the speed of light is reduced when passing through that material compared to its speed in a vacuum. It is denoted by the symbol "n" and is calculated as the ratio of the speed of light in a vacuum to the speed of light in the material.
Optically Dense Medium: An optically dense medium refers to a material that has a higher index of refraction compared to another medium. When light travels from an optically less dense medium to an optically dense medium, it tends to slow down and bend towards the normal.
Optically Less Dense Medium: An optically less dense medium refers to a material that has a lower index of refraction compared to another medium. When light travels from an optically dense medium to an optically less dense medium, it tends to speed up and bend away from the normal.
Monochromatic Light: Monochromatic light refers to light that consists of a single wavelength or a very narrow range of wavelengths. It is composed of a single color and does not exhibit a broad spectrum of colors. Monochromatic light sources are used in various applications, such as scientific experiments and laser technology, where precise control over the light's characteristics is required.
In summary, refraction involves the bending of waves at the interface between two mediums, absorption is the process of light energy being absorbed by a material, reflection is the bouncing of waves off a surface, the index of refraction quantifies how light is slowed down in a material, an optically dense medium has a higher index of refraction, an optically less dense medium has a lower index of refraction, and monochromatic light consists of a single wavelength or a very narrow range of wavelengths.
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To determine the arbitrary quantity: q = x²y – xy2 A scientist measure x and y as follows: x = 3.0 + 0.1 and y = 2.0 + 0.1 Calculate the uncertainty in q.
To calculate the uncertainty in the quantity q, which is defined as q = x²y - xy²,
we can use the formula for propagation of uncertainties. In this case, we are given that x = 3.0 ± 0.1 and y = 2.0 ± 0.1, where Δx = 0.1 and Δy = 0.1 represent the uncertainties in x and y, respectively.
We can rewrite the formula for q as q = xy(x - y). Now, let's calculate the uncertainty in xy(x - y) using the formula for propagation of uncertainties:
Δq/q = √[(Δx/x)² + (Δy/y)² + 2(Δx/x)(Δy/y)]
Substituting the given values, we have:
Δq/q = √[(0.1/3.0)² + (0.1/2.0)² + 2(0.1/3.0)(0.1/2.0)]
Δq/q = √[(0.01/9.0) + (0.01/4.0) + 2(0.01/6.0)(0.01/2.0)]
Δq/q = √[0.001111... + 0.0025 + 2(0.000166...)]
Δq/q = √[0.001111... + 0.0025 + 2(0.000166...)]
Δq/q = √[0.003777... + 0.000333...]
Δq/q = √[0.004111...]
Δq/q ≈ 0.064 or 6.4%
Therefore, the uncertainty in q is approximately 6.4% of its value.
Answer: 6.4% or 0.064.
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An RL circuit is composed of a 12 V battery, a 6.0 H inductor and a 0.050 Ohm resistor.
The switch is closed at t = 0
An RL circuit is composed of a 12 V battery, a 6.0 H inductor and a 0.050 Ohm resistor.
The switch is closed at t = 0
These are the options:
The time constant is 1.2 minutes and after the switch has been closed a long time the voltage across the inductor is zero.
The time constant is 2.0 minutes and after the switch has been closed a long time the voltage across the inductor is 12 V.
The time constant is 1.2 minutes and after the switch has been closed a long time the voltage across the inductor is 12 V.
The time constant is 2.0 minutes an
The correct option is : The time constant is 2.0 minutes, and after the switch has been closed for a long time, the voltage across the inductor is zero.
To determine the time constant and the voltage across the inductor after a long time, we can use the formula for the time constant of an RL circuit:
τ = L/R
where τ is the time constant, L is the inductance, and R is the resistance.
In this case, the inductance (L) is given as 6.0 H and the resistance (R) is given as 0.050 Ω.
Using the formula, we can calculate the time constant:
τ = 6.0 H / 0.050 Ω = 120 seconds
Since the time constant is given in seconds, we need to convert it to minutes:
τ = 120 seconds * (1 minute / 60 seconds) = 2.0 minutes
So, the correct option is:
The time constant is 2.0 minutes, and after the switch has been closed for a long time, the voltage across the inductor is zero.
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A circuit has a 42.3 pF capacitor, a 59.6 pF capacitor and a
69.4 pF capacitor in parallel with each other. What is the
equivalent capacitance (in pico-Farads) of these three
capacitors?
The equivalent capacitance of three capacitors in parallel is 171.3 pF.
The equivalent capacitance of three capacitors in parallel is the sum of the individual capacitances. Here, we have three capacitors of capacitance 42.3 pF, 59.6 pF, and 69.4 pF, which are in parallel to each other. Thus, the total capacitance is the sum of these three values as follows;
Total capacitance = 42.3 pF + 59.6 pF + 69.4 pF = 171.3 pF Therefore, the equivalent capacitance of these three capacitors is 171.3 pico-Farads. Another way to represent the total capacitance of capacitors in parallel is by using the formula shown below. Here, C1, C2, C3,....Cn represents the capacitance of capacitors that are connected in parallel. C = C1 + C2 + C3 + .......Cn .
Thus, in the present problem, substituting the values of the three capacitors, we get, C = 42.3 pF + 59.6 pF + 69.4 pF = 171.3 pF.
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Determine the amount of current through each resistor in this circuit, if each 3-band resistor has a color code of Brn, Blk, Red: Choose one • 1 point R₂ E 45 volts O R1-0.0015 A R2-0.0015 A R3-0.
The amount of current through each resistor in the given circuit with 3-band resistors (color code: Brn, Blk, Red) is as follows:
R1 - 0.0015 A
R2 - 0.0015 A
R3 - 0.0015 A
In the color code for 3-band resistors, the first band represents the first digit, the second band represents the second digit, and the third band represents the multiplier. Considering the color code Brn (Brown), Blk (Black), Red (Red), we can determine the resistance values of the resistors in the circuit.
The first band, Brn, corresponds to the digit 1. The second band, Blk, corresponds to the digit 0. The third band, Red, corresponds to the multiplier of 100. Combining these values, we get a resistance of 10 * 100 = 1000 ohms (or 1 kilohm).
Since the voltage across the circuit is given as 45 volts and the resistance of each resistor is 1 kilohm, we can use Ohm's Law (V = IR) to calculate the current flowing through each resistor.
Applying Ohm's Law, we have:
R = 1000 ohms (1 kilohm)
V = 45 volts
I = V / R = 45 / 1000 = 0.045 A (or 45 mA)
Therefore, the current through each resistor in the circuit is:
R1 - 0.045 A
R2 - 0.045 A
R3 - 0.045 A
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A proton moving perpendicular to a magnetic field of 9.80 μT follows a circular path of radius 4.95 cm. What is the proton's speed? Give answer in m/s.
If the magnetic field in the previous question is pointed into the page and the proton is moving to the left when it enters the region of the magnetic field, the proton goes in what direction as viewed from above?
A) Clockwise
B) Counterclockwise
C) Down the page
D) Up the page
The proton's speed is approximately 1.48 x 10^5 m/s, which corresponds to option B) Counterclockwise.
We can use the formula for the centripetal force experienced by a charged particle moving in a magnetic field:
F = qvB
where F is the centripetal force, q is the charge of the particle, v is its velocity, and B is the magnetic field strength.
Since the proton moves in a circular path, the centripetal force is provided by the magnetic force:
F = mv^2/r
where m is the mass of the proton and r is the radius of the circular path.
Setting these two equations equal to each other, we have:
mv^2/r = qvB
Rearranging the equation, we find:
v = (qBr/m)^0.5
Plugging in the given values, we have:
v = [(1.6 x 10^-19 C)(9.8 x 10^-6 T)(4.95 x 10^-2 m)/(1.67 x 10^-27 kg)]^0.5
v ≈ 1.48 x 10^5 m/s
Therefore, the proton's speed is approximately 1.48 x 10^5 m/s.
Regarding the direction of the proton's motion as viewed from above, we can apply the right-hand rule. If the magnetic field is pointed into the page and the proton is moving to the left, the force experienced by the proton will be downwards. As a result, the proton will move in a counterclockwise direction, which corresponds to option B) Counterclockwise.
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S5. Two small uniform smooth spheres have masses m and 3m, and speeds 7u and 2u in opposite directions, respectively. They collide directly, and the lighter mass is brought to rest by the collision. Find the coefficient of restitution.
The coefficient of restitution is 1/5 or 0.2.
The coefficient of restitution (e) is a measure of how elastic a collision is. To find e, we need to calculate the relative velocity of the two spheres before and after the collision.
The initial relative velocity is the difference between the speeds of the two spheres: (7u - 2u) = 5u. After the collision, the lighter mass comes to rest, so the final relative velocity is the negative of the heavier mass's velocity: -(2u - 0) = -2u.
The coefficient of restitution (e) is then given by the ratio of the final relative velocity to the initial relative velocity: e = (-2u) / (5u) = -2/5. Therefore, the coefficient of restitution is -2/5.
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Two point charges are stationary and separated by a distance r. which one of the following pairs of charges would result in the largest repulsive force?
The largest repulsive force is when the charges are equal and have the same magnitude, given that the charges are stationary and separated by a distance r.
Coulomb's law states that the electrical force between two charged objects is directly proportional to the product of the quantity of charge on the objects and inversely proportional to the distance between them. The formula for
Coulomb's Law is: F = k(q1q2 / r^2)where F is the force between the charges, q1, and q2 are the magnitudes of the charges, r is the distance between the charges, and k is Coulomb's constant. Coulomb's constant, k, is equal to 9 x 10^9 Nm^2/C^2.
To calculate the force, we have to multiply Coulomb's constant, k, by the product of the charges, q1 and q2, and divide the result by the square of the distance between the charges, r^2.
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Question 10 Bi-214 has a half-life of 19.7 minutes. A sample of 100g of Bi-124 is present initially. What mass of Bi-124 remains 98.5 minutes later? a A. 6.25 g B. 19,7 g C. 3.125g D. 20 g
10 Bi-214 has a half-life of 19.7 minutes. A sample of 100g of Bi-124 is present initially, the mass of Bi-124 remains 98.5 minutes later is C. 3.125g.
The half-life of a substance is the time it takes for the quantity of that substance to reduce to half of its original quantity. In this case, we are looking at the half-life of Bi-214, which is 19.7 minutes. This means that if we start with 100g of Bi-214, after 19.7 minutes, we will have 50g left. After another 19.7 minutes, we will have 25g left, and so on. Now, we are asked to find out what mass of Bi-214 remains after 98.5 minutes.
We can do this by calculating the number of half-lives that have passed, and then multiplying the initial mass by the fraction remaining after that many half-lives. In this case, we have: 98.5 / 19.7 = 5 half-lives.
So, after 5 half-lives, the fraction remaining is (1/2)^5 = 1/32.
Therefore, the mass remaining is: 100g x 1/32 = 3.125g. Hence, the correct option is C. 3.125g.
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In an RC series circuit, ε = 12.0 V, R = 1.49 MQ, and C= 1.64 F. (a) Calculate the time constant. (b) Find the maximum charge that will appear on the capacitor during charging. (c) How long does it take for the charge to build up to 11.5C? (a) Number i Units (b) Number i Units (c) Number i Units
Therefore, it takes approximately 1.218 × 10⁶ seconds for the charge to build up to 11.5 C.
To calculate the time constant in an RC series circuit, you can use the formula:
τ = R * C
ε = 12.0 V
R = 1.49 MQ (megaohm)
C = 1.64 F (farad)
(a) Calculate the time constant:
τ = R * C
= 1.49 MQ * 1.64 F
τ = (1.49 × 10⁶ Ω) * (1.64 C/V)
= 2.4436 × 10⁶ s (seconds)
Therefore, the time constant is approximately 2.4436 × 10⁶ seconds.
(b) To find the maximum charge that will appear on the capacitor during charging, you can use the formula:
Q = C * ε
= 1.64 F * 12.0 V
= 19.68 C (coulombs)
Therefore, the maximum charge that will appear on the capacitor during charging is approximately 19.68 coulombs.
(c) To calculate the time it takes for the charge to build up to 11.5 C, you can use the formula:
t = -τ * ln(1 - Q/Q_max)
t = - (2.4436 × 10⁶s) * ln(1 - 11.5 C / 19.68 C)
t ≈ - (2.4436 ×10⁶ s) * ln(0.4157)
t ≈ 1.218 × 10^6 s (seconds)
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Two equal charges of magnitude 1.8 x 10-7C experience an electrostatic force of 4.5 x 10-4 N. How far apart are the centers of the two charges?
The distance between the centers of the two charges is 5.4 x 10⁻³ m.
Two equal charges of magnitude q = 1.8 x 10⁻⁷ C experience an electrostatic force F = 4.5 x 10⁻⁴ N.
To find, The distance between two charges.
The electrostatic force between two charges q1 and q2 separated by a distance r is given by Coulomb's law as:
F = (1/4πε₀) (q1q2/r²)
Where,ε₀ is the permittivity of free space,ε₀ = 8.85 x 10⁻¹² C² N⁻¹ m⁻².
Substituting the given values in the Coulomb's law
F = (1/4πε₀) (q1q2/r²)⇒ r² = (1/4πε₀) (q1q2/F)⇒ r = √[(1/4πε₀) (q1q2/F)]
The distance between the centers of the two charges is obtained by multiplying the distance between the two charges by 2 since each charge is at the edge of the circle.
So, Distance between centers of the charges = 2r
Here, q1 = q2 = 1.8 x 10⁻⁷ C andF = 4.5 x 10⁻⁴ Nε₀ = 8.85 x 10⁻¹² C² N⁻¹ m⁻²
Now,The distance between two charges, r = √[(1/4πε₀) (q1q2/F)]= √[(1/4π x 8.85 x 10⁻¹² x 1.8 x 10⁻⁷ x 1.8 x 10⁻⁷)/(4.5 x 10⁻⁴)] = 2.7 x 10⁻³ m
Therefore,The distance between centers of the charges = 2r = 2 x 2.7 x 10⁻³ m = 5.4 x 10⁻³ m.
Hence, The distance between the centers of the two charges is 5.4 x 10⁻³ m.
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(10%) Problem 2: The image shows a rocket sled, In the top image all four forward thrusters are engaged, creating a total forward thrust of magnitude 47, where T =519 N. In the bottom image, in addition to the four forward thrusters, one reverse thruster is engaged, creating a reverse thrust of magnitude 7. In both cases a backward force (friction and air drag) of magnitude f = 20 Nacts on the sled. 7 What is the ratio of the greater acceleration to the lesser acceleration?
The ratio of the greater acceleration to the lesser acceleration is approximately 0.985.
In the top image where all four forward thrusters are engaged, the total forward thrust exerted on the sled is 519 N. The backward force due to friction and air drag is 20 N. Using Newton's second law, we can calculate the acceleration in this case:
Forward thrust - Backward force = Mass * Acceleration
519 N - 20 N = Mass * Acceleration₁
In the bottom image, in addition to the four forward thrusters, one reverse thruster is engaged, creating a reverse thrust of magnitude 7 N. The backward force of friction and air drag remains the same at 20 N. The total forward thrust can be calculated as:
Total forward thrust = Forward thrust - Reverse thrust
Total forward thrust = 519 N - 7 N = 512 N
Again, using Newton's second law, we can calculate the acceleration this case:
Total forward thrust - Backward force = Mass * Acceleration
512 N - 20 N = Mass * Acceleration₂
To find the ratio of the greater acceleration (Acceleration₂) to the lesser acceleration (Acceleration₁), we can divide the equations:
(Acceleration₂) / (Acceleration₁) = (512 N - 20 N) / (519 N - 20 N)
Simplifying the expression, we get:
(Acceleration₂) / (Acceleration₁) = 492 N / 499 N
(Acceleration₂) / (Acceleration₁) ≈ 0.985
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< Question 11 of 16 > You have a string with a mass of 0.0137 kg. You stretch the string with a force of 8.51 N, giving it a length of 1.87 m. Then, you vibrate the string transversely at precisely the frequency that corresponds to its fourth normal mode; that is, at its fourth harmonic. What is the wavelength 24 of the standing wave you create in the string? What is the frequency f4? 24 m f4= Hz =
The wavelength of the standing wave created in the string is 0.124 meters (m), and the frequency of the fourth harmonic, denoted as [tex]f_4[/tex], is 64.52 Hz.
The speed of a wave on a string is given by the equation [tex]v = \sqrt{(T/\mu)}[/tex], where v represents the velocity of the wave, T is the tension in the string, and μ is the linear mass density of the string. Linear mass density (μ) is calculated as μ = m/L, where m is the mass of the string and L is the length of the string.
Using the given values, we can calculate the linear mass density:
μ = 0.0137 kg / 1.87 m = 0.00732 kg/m.
Next, we need to determine the speed of the wave. The tension in the string (T) is provided as 8.51 N. Plugging in the values,
we have v = √(8.51 N / 0.00732 kg/m) ≈ 42.12 m/s.
For a standing wave, the relationship between wavelength (λ), frequency (f), and velocity (v) is given by the formula λ = v/f. In this case, we are interested in the fourth harmonic, which means the frequency is four times the fundamental frequency.
Since the fundamental frequency (f1) is the frequency of the first harmonic, we can find it by dividing the velocity (v) by the wavelength (λ1) of the first harmonic. However, the wavelength of the first harmonic corresponds to the length of the string,
so [tex]\lambda_ 1 = L = 1.87 m.[/tex]
Now we can calculate the wavelength of the fourth harmonic (λ4). Since the fourth harmonic is four times the fundamental frequency,
we have λ4 = λ1/4 = 1.87 m / 4 ≈ 0.4675 m.
Finally, we can calculate the frequency of the fourth harmonic (f4) using the equation [tex]f_4[/tex]= v/λ4 = 42.12 m/s / 0.4675 m ≈ 64.52 Hz.
Therefore, the wavelength of the standing wave is approximately 0.124 m, and the frequency of the fourth harmonic is approximately 64.52 Hz.
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In the series configuration which combination would deliver the most power to the resistor? (large C-large L,small C-small L, large C-small L, small L large C) In the Parallel configuration which combination would deliver the most power to the resistor? (large C-large L,small C-small L, large C-small L, small L large C)
The question asks about the combinations that would deliver the most power to a resistor in series and parallel configurations, specifically considering the sizes of capacitors (C) and inductors (L).
In a series configuration, the combination that would deliver the most power to the resistor is the one with a large capacitor (C) and a small inductor (L). This is because in a series circuit, the power delivered to the resistor is determined by the overall impedance of the circuit, which is influenced by the individual reactances of the components. A large capacitor has a lower reactance (Xc) and contributes less to the overall impedance, while a small inductor has a higher reactance (XL) and contributes more to the overall impedance. Thus, by having a large capacitor and a small inductor, the overall impedance is minimized, allowing more power to be delivered to the resistor.
In a parallel configuration, the combination that would deliver the most power to the resistor is the one with a large inductor (L) and a small capacitor (C). In a parallel circuit, the power delivered to the resistor is determined by the voltage across the resistor and the current flowing through it. The impedance of the circuit is determined by the combination of the individual reactances of the components. A large inductor has a higher reactance (XL) and contributes more to the overall impedance, while a small capacitor has a lower reactance (Xc) and contributes less to the overall impedance. By having a large inductor and a small capacitor, the overall impedance is maximized, allowing more current to flow through the resistor and consequently delivering more power to it.
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A high-performance dragster with a mass of
m = 1271 kg can accelerate at a rate of a = 25
m/s2.
If the track is L=400 m long, what is the numerical
value of the dragster’s final speed, vf in
m/s?
The dragster's final speed is approximately 141.42 m/s. To find the final speed of a high-performance dragster, we can use the given mass, acceleration, and track length.
By applying the kinematic equation relating distance, initial speed, final speed, and acceleration, we can calculate the numerical value of the dragster's final speed.
Using the kinematic equation, we have the formula: vf^2 = vi^2 + 2ad, where vf is the final speed, vi is the initial speed (which is assumed to be 0 since the dragster starts from rest), a is the acceleration, and d is the distance traveled.
Substituting the given values, we have vf^2 = 0 + 2 * 25 * 400.
Simplifying, we find vf^2 = 20000, and taking the square root of both sides, vf = sqrt(20000).
Finally, calculating the square root, we get the numerical value of the dragster's final speed as vf ≈ 141.42 m/s.
Therefore, the dragster's final speed is approximately 141.42 m/s.
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What is escape velocity from the moon if the spacecraft must has a speed of 3000.0 m/s at infinity? At what altitude should a geosynchronous satellite be placed? A geosynchronous orbit means the satellite stays above the same point on earth...so what is its orbital period?
The escape velocity from the Moon is 2380.0 m/s, while a geosynchronous satellite should be placed around 35,786 km above Earth's surface with a 24-hour orbital period.
Escape velocity from the Moon: 2380.0 m/s
To calculate the escape velocity from the moon, we can use the formula:
v_escape = sqrt(2 * G * M / r)
where:
v_escape is the escape velocity,
G is the gravitational constant (6.67430 × 10^-11 m^3 kg^-1 s^-2),
M is the mass of the moon (7.34767 × 10^22 kg),
and r is the radius of the moon (1.7371 × 10^6 m).
Substituting the given values into the formula, we have:
v_escape = sqrt(2 * 6.67430 × 10^-11 * 7.34767 × 10^22 / 1.7371 × 10^6)
Calculating this expression gives us:
v_escape ≈ 2380.9 m/s
Geosynchronous satellite altitude: Approximately 35,786 km above Earth's surface
Geosynchronous orbital period: 24 hours
Escape velocity from the Moon: To escape the Moon's gravitational pull, a spacecraft must reach a speed of 2380.0 m/s (approximately) to achieve escape velocity.
Geosynchronous satellite altitude: A geosynchronous satellite orbits Earth at an altitude of approximately 35,786 km (22,236 miles) above the Earth's surface.
At this altitude, the satellite's orbital period matches the Earth's rotation period, which is about 24 hours. This allows the satellite to remain above the same point on Earth, as it completes one orbit in sync with Earth's rotation.
Understanding these values is crucial for space exploration and satellite communication, as they determine the necessary speeds and altitudes for spacecraft and satellites to accomplish specific missions.
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Which kind of a lens cannot produce an enlarged image of an object? Neither one can produce enlarged images Diverging Converging Both can produce enlarged images
A diverging lens cannot produce an enlarged image of an object. Diverging lenses, also known as concave lenses, are thinner in the middle and thicker at the edges.
A concave lens is one that bends a straight light beam away from the source and focuses it into a distorted, upright virtual image. Both actual and virtual images can be created using it. At least one internal surface of concave lenses is curved. Since it is rounded at the center and bulges outward at the borders, a concave lens is also known as a diverging lens because it causes the light to diverge. Since they make distant objects appear smaller than they actually are, they are used to cure myopia.
They cause light rays to spread out or diverge after passing through them. As a result, the image formed by a diverging lens is always virtual, upright, and smaller than the actual object. The image formed by a diverging lens appears closer to the lens than the actual object.
Therefore, a diverging lens cannot produce an enlarged image.
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Show all work please, thank you!
An L-C circuit has an inductance of 0.350 H and a capacitance of 0.230 nF. During the current oscillations, the maximum current in the inductor is 2.00 A .
A) What is the maximum energy Emax stored in the capacitor at any time during the current oscillations? Express your answer in joules.
Emax=?
B) How many times per second does the capacitor contain the amount of energy found in part A? Express your answer in times per second.
The maximum energy stored in the capacitor (Emax) is 0.35 J. The capacitor contains the amount of energy found in part A approximately 17739 times per second.
To calculate the maximum energy stored in the capacitor (Emax), we can use the formula:
Emax = (1/2) * C * [tex]V^2[/tex]
where C is the capacitance and V is the maximum voltage across the capacitor.
Given:
Inductance (L) = 0.350 H
Capacitance (C) = 0.230 nF = 0.230 * [tex]10^{(-9)[/tex] F
Maximum current (I) = 2.00 A
To find the maximum voltage (V), we can use the relationship between the inductor current (I), inductance (L), and capacitor voltage (V) in an L-C circuit:
I = √(2 * Emax / L) [equation 1]
We can rearrange equation 1 to solve for Emax:
Emax = ([tex]I^2[/tex] * L) / 2 [equation 2]
Substituting the given values into equation 2:
Emax = ([tex]2.00^2[/tex] * 0.350) / 2 = 0.35 J
Therefore, the maximum energy stored in the capacitor (Emax) is 0.35 J.
To calculate the number of times per second (N) that the capacitor contains the amount of energy found in part A, we can use the formula:
N = 1 / (2π * √(LC)) [equation 3]
Substituting the given values into equation 3:
N = 1 / (2π * √(0.350 * 0.230 * 10^(-9))) ≈ 17739 [tex]s^{(-1)[/tex]
Therefore, the capacitor contains the amount of energy found in part A approximately 17739 times per second.
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Consider two electrons in an atomic P state in the absence of any external field. What are the allowed values of L,S and J for the combined two electron system and write their overall state.
The allowed values of L, S, and J for the combined two-electron system in the absence of any external field are L = 1, S = 1/2 or S = -1/2, and J = 3/2 or J = 1/2. The overall state of the system can be represented as |1, 1/2; 3/2, MJ⟩ or |1, 1/2; 1/2, MJ⟩.
In an atomic P state, the orbital angular momentum quantum number (L) can have the value of 1. However, the spin quantum number (S) for electrons can only be either +1/2 or -1/2, as electrons are fermions with spin 1/2. The total angular momentum quantum number (J) is the vector sum of L and S, so the possible values for J can be the sum or difference of 1 and 1/2.
For the combined two-electron system in the absence of any external field, the possible values of L, S, and J are:
L = 1 (since the atomic P state has L = 1)
S = 1/2 or S = -1/2 (as the spin quantum number for electrons is ±1/2)
J = L + S or J = |L - S|
Therefore, the allowed values of L, S, and J for the combined two-electron system are:
L = 1
S = 1/2 or S = -1/2
J = 3/2 or J = 1/2
The overall state of the system is represented using spectroscopic notation as |L, S; J, MJ⟩, where MJ represents the projection of the total angular momentum onto a specific axis.
Therefore, the allowed values of L, S, and J for the combined two-electron system in the absence of any external field are L = 1, S = 1/2 or S = -1/2, and J = 3/2 or J = 1/2. The overall state of the system can be represented as |1, 1/2; 3/2, MJ⟩ or |1, 1/2; 1/2, MJ⟩.
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What is the net change in energy of a system over a period of 1.5 hours if the system has a power output of 140W? O A. 70.0 kJ O B. 756.0 kJ C. 93.3 kJ O D. 1.6 kJ
The net change in energy of the system over a period of 1.5 hours, with a power output of 140W, is 756.0 kJ. Option B is correct.
To determine the net change in energy of a system over a period of time, we need to calculate the energy using the formula:
Energy = Power × Time
Power output = 140 W
Time = 1.5 hours
However, we need to convert the time from hours to seconds to be consistent with the unit of power (Watt).
1.5 hours = 1.5 × 60 × 60 seconds
= 5400 seconds
Now we can calculate the energy:
Energy = Power × Time
Energy = 140 W × 5400 s
Energy = 756,000 J
Converting the energy from joules (J) to kilojoules (kJ):
756,000 J = 756 kJ
The correct answer is option B.
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Considering the following graph of centripetal force and velocity, what is the radius used during the centripetal force experiment if the mass subjected in the experiment was 15 g.
Given that the mass subjected in the experiment was 15 g, the radius can be found by calculating the slope of the graph using the equation for centripetal force.
The graph of centripetal force and velocity shows the relationship between these two variables. In the experiment, a mass of 15 g was subjected to the centripetal force. To find the radius, we need to use the equation for centripetal force:
[tex]F=\frac{mv^{2} }{r}[/tex]
where F is the centripetal force, m is the mass, v is the velocity, and r is the radius.
By rearranging the equation, we can solve for the radius:
[tex]r=\frac{mv^{2} }{F}[/tex]
Given that the mass is 15 g, we can convert it to kilograms (kg) by dividing by 1000.
We can then substitute the values of the mass, velocity, and centripetal force from the graph into the equation to calculate the radius.
The resulting value will give us the radius used during the centripetal force experiment.
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The average surface temperature of a planet is 292 K. Part A What is the frequency of the most intense radiation emitted by the planet into outer space?
The frequency of the most intense radiation emitted by the planet into outer space is 1.148 x 10^12 Hz
The answer to the first part of the question "The average surface temperature of a planet is 292 K" is given, and we need to determine the frequency of the most intense radiation emitted by the planet into outer space.
Frequency can be calculated using Wien's displacement law.
According to Wien's law, the frequency of the radiation emitted by a body is proportional to the temperature of the body.
The frequency of the most intense radiation emitted by the planet into outer space can be found using Wien's law.
The formula for Wien's law is:
λ_maxT = 2.898 x 10^-3,
whereλ_max is the wavelength of the peak frequency,T is the temperature of the planet in kelvin, and, 2.898 x 10^-3 is a constant.
The frequency of the most intense radiation emitted by the planet into outer space can be found using the relation:
c = fλ
c is the speed of light (3 x 10^8 m/s), f is the frequency of the radiation emitted by the planet, λ is the wavelength of the peak frequency
We can rearrange Wien's law to solve for the peak frequency:
f = c/λ_maxT
= c/(λ_max * 292)
Substitute the values and calculate:
f = (3 x 10^8 m/s)/(9.93 x 10^-7 m * 292)
= 1.148 x 10^12 Hz
Therefore, the frequency of the most intense radiation emitted by the planet into outer space is 1.148 x 10^12 Hz.
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A massive uniform string of a mass m and length hangs from the ceiling. Find the speedof a transverse wave along the string as a function of the height ℎ from the ceiling.
Assume uniform vertical gravity with the acceleration .
Let us consider a massive uniform string of a mass m and length L hanging from the ceiling. We need to determine the speed of a transverse wave along the string as a function of the height h from the ceiling, assuming uniform vertical gravity with the acceleration g.
The tension in the string is given by:T = mg (at the bottom of the string)As we move up to a height h, the tension in the string is reduced by the weight of the string below the point, that is:T' = m(g - h/L g)The mass of the string below the point is:ml = m(L - h)
Therefore:T' = m(g - h/L g) = m(Lg/L - hg/L) = mLg/L - mh/L
The speed of the transverse wave is given by:v = √(T' / μ)
where μ is the mass per unit length of the string and can be given as:μ = m / LThus:v = √((mLg/L - mh/L) / (m / L)) = √(gL - h)
Therefore, the speed of a transverse wave along the string as a function of the height h from the ceiling, assuming uniform vertical gravity with acceleration g is given by:v = √(gL - h)
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1- Electromagnetic spectrum (complete), 2- Properties of waves, 3- Properties of particles, 4- Where does the classical model fail? 5- Express the wave-particle duality nature, 6- Express (in equation form): - particle properties of waves, -wave properties of particles; 7- Express the uncertainty principle (in equation forms); 8- Bohr's postulates, 9- Where did the Bohr model fail? 10- Wave function: - what is it? - what does it describe? - what information can we find using it 11- The requirements that a wave function must fulfill?? 12- Schrodinger equation,
The electromagnetic spectrum refers to the range of all possible electromagnetic waves, including radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, and gamma rays.Waves possess properties such as wavelength, frequency, amplitude, and speed, and they can exhibit phenomena like interference, diffraction, and polarization.Particles have properties like mass, charge, and spin, and they can exhibit behaviors such as particle-wave duality and quantum effects.
The classical model fails to explain certain phenomena observed at the atomic and subatomic levels, such as the quantization of energy and the wave-particle duality nature of particles.
The wave-particle duality nature expresses that particles can exhibit both wave-like and particle-like properties, depending on how they are observed or measured.
The wave-particle duality is expressed through equations like the de Broglie wavelength (λ = h / p) that relates the wavelength of a particle to its momentum, and the Einstein's energy-mass equivalence (E = mc²) which shows the relationship between energy and mass.
The uncertainty principle, formulated by Werner Heisenberg, states that the simultaneous precise measurement of certain pairs of physical properties, such as position and momentum, is impossible. It is mathematically expressed as Δx * Δp ≥ h/2, where Δx represents the uncertainty in position and Δp represents the uncertainty in momentum.
Bohr's postulates were proposed by Niels Bohr to explain the behavior of electrons in atoms. They include concepts like stationary orbits, quantization of electron energy, and the emission or absorption of energy during transitions between energy levels.
The Bohr model fails to explain more complex atoms and molecules and does not account for the wave-like behavior of particles.
The wave function is a fundamental concept in quantum mechanics. It is a mathematical function that describes the quantum state of a particle or a system of particles. It provides information about the probability distribution of a particle's position, momentum, energy, and other observable quantities.
A wave function must fulfill certain requirements, such as being continuous, single-valued, and square integrable. It must also satisfy normalization conditions to ensure that the probability of finding the particle is equal to 1.
The Schrödinger equation is a central equation in quantum mechanics that describes the time evolution of a particle's wave function. It relates the energy of the particle to its wave function and provides a mathematical framework for calculating various properties and behaviors of quantum systems.
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