(a) The time required for the capacitor to lose the first one-third of its charge is given by t1 = t * ln(3), and (b) the time required to lose the first two-thirds of its charge is t2 = t * ln(3^2)
(a) To calculate the time required for the capacitor to lose the first one-third of its charge, we can use the formula:t1 = t * ln(3)
Where t1 represents the time required, t is the time constant, and ln denotes the natural logarithm. This formula is derived from the exponential decay behavior of a charging or discharging capacitor.
(b) Similarly, to find the time required for the capacitor to lose the first two-thirds of its charge, we can use the formula:
t2 = t * ln(3^2)
Here, t2 represents the time required to lose the first two-thirds of the charge.
(a) The time required for the capacitor to lose the first one-third of its charge is given by t1 = t * ln(3), and (b) the time required to lose the first two-thirds of its charge is t2 = t * ln(3^2). These formulas utilize the natural logarithm and the time constant to calculate the desired time durations.
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Part A Monochromatic light passes through two slits separated by a distance of 0.0344 mm. If the angle to the third maximum above the central fringe is 3.61 °, what is the wavelength of the light? Express your answer to three significant figures. VI AEQ ? l= nm Submit Request Answer
A Monochromatic light passes through two slits separated by a distance of 0.0344 mm. If the angle to the third maximum above the central fringe is 3.61 °, the wavelength of the light is 634.62 nm.
To solve this problem, we can use the following equation:
sin(theta) = n * lambda / d
Where:
theta is the angle to the nth maximum above the central fringe in degrees
n is the order of the maximum (in this case, n = 3)
lambda is the wavelength of the light in meters
d is the distance between the slits in meters
Plugging in the values, we get:
sin(3.61°) = 3 * lambda / 0.0344 mm
lambda = (0.0344 mm) * sin(3.61°) / 3
lambda = 634.62 nm
Therefore, the wavelength of the light is 634.62 nm.
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quick answer
please
QUESTION 17 An observatory uses a large refracting telescope that has an objective lens of diameter, 1.00 m. The telescope resolves images with green light of wavelength 550 nm. If the telescope can b
The telescope can resolve objects with an angular size greater than or equal to 1.21 arcseconds.
The resolving power of a telescope determines its ability to distinguish fine details in an observed object. It is determined by the diameter of the objective lens or mirror and the wavelength of the light being observed. The formula for resolving power is given by:
R = 1.22 * (λ / D)
Where R is the resolving power, λ is the wavelength of light, and D is the diameter of the objective lens or mirror.
In this case, the diameter of the objective lens is given as 1.00 m, and the wavelength of green light is 550 nm (or 550 x 10^-9 m). Plugging in these values into the formula, we can calculate the resolving power:
R = 1.22 * (550 x 10^-9 m / 1.00 m)
R ≈ 1.21 x 10^-3 radians
To convert the resolving power to angular size, we can use the fact that there are approximately 206,265 arcseconds in a radian:
Angular size = R * (206,265 arcseconds/radian)
Angular size ≈ 1.21 x 10^-3 radians * 206,265 arcseconds/radian
The result is approximately 1.21 arcseconds. Therefore, the telescope can resolve objects with an angular size greater than or equal to 1.21 arcseconds.
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Buttercup is sliding on frictionless ice with a speed of 2.5 m/s when she runs into a large massless spring with a spring constant of 272 N/m. Buttercup has a mass of 31.5 kg. a) What is the amplitude
(a)The amplitude of the spring oscillations is 0.29 m.
In a scenario where Buttercup is sliding on a frictionless ice with a speed of 2.5 m/s and runs into a large massless spring with a spring constant of 272 N/m, her mass of 31.5 kg makes it possible to calculate the amplitude of the spring oscillations using the given formula.
Amplitude is defined as the magnitude of the maximum displacement of the oscillating object from its equilibrium position. It represents the maximum value of an oscillation or wave from its equilibrium or average value.
Spring constant (k) is defined as the ratio of the applied force to the deformation caused by that force. It is the amount of force required per unit deformation or lengthening of a spring.
The formula for the amplitude of the spring oscillations, A= (m × v) / k where A is the amplitude, m is the mass of the object (Buttercup) that collided with the spring, v is the velocity of the object before the collision, and k is the spring constant of the massless spring. Substituting the given values into the formula: A = (m × v) / k = (31.5 kg × 2.5 m/s) / 272 N/mA = 0.29 m.
Therefore, the amplitude of the spring oscillations is 0.29 m.
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The capacitor in the figure is being charged with a 3.54 A current. The wire radius is 1.12 mm, and the plate radius is 2.22 cm. Assume that the current i in the wire and the displacement current id in the capacitor gap are both uniformly distributed. What is the magnitude of the magnetic field due to i at the following radial distances from the wire's center: (a)0.756 mm (inside the wire), (b)1.37 mm (outside the wire), and (c)3.25 cm (outside the wire). What is the magnitude of the magnetic field due to id at the following radial distances from the central axis between the plates: (d)0.756 mm (inside the gap), (e) 1.37 mm (inside the gap), and (f)3.25 cm (outside the gap). (a) 3 B B Field due Field due to current i to current i B Field due to current i
In order to answer this question, we will make use of the formula that calculates the magnetic field due to the current in a straight wire which is given by:
$$B = \frac{\mu_{0}i}{2\pi r}$$
Where;B = Magnetic field due to the current in the wirei = current in the wirer = radius of the wireSimilarly, the formula for the magnetic field due to the displacement current in a capacitor is given by:
$$B = \frac{\mu_{0}\epsilon_{0}}{2}\frac{dE}{dt}$$
Where;B = Magnetic field due to the displacement current E = electric field in the capacitor gapdE/dt = rate of change of electric field
$\mu_{0}$ = Permeability of free space$\epsilon_{0}$ = Permittivity of free space(a) Field due to current i at 0.756 mmFor r = 0.756 mm, i = 3.54 A and $\mu_{0}$ = 4π × 10⁻⁷ N/A².$$B = \frac{\mu_{0}i}{2\pi r}$$$$B = \frac{4\pi \times 10^{-7} \times 3.54}{2\pi \times 0.756 \times 10^{-3}}$$$$
B = 7.37 \times 10^{-4} T$$Therefore, the magnetic field due to current i at 0.756 mm is 7.37 x 10⁻⁴ T.(b) Field due to current i at 1.37 mmFor r = 1.37 mm, i = 3.54 A and $\mu_{0}$ = 4π × 10⁻⁷ N/A².$$B = \frac{\mu_{0}i}{2\pi r}$$$$B = \frac{4\pi \times 10^{-7} \times 3.54}{2\pi \times 1.37 \times 10^{-3}}$$$$
B = 8.61 \times 10^{-4} T$$Therefore, the magnetic field due to current i at 1.37 mm is 8.61 x 10⁻⁴ T.(c) Field due to current i at 3.25 cmFor r = 3.25 cm, i = 3.54 A and $\mu_{0}$ = 4π × 10⁻⁷ N/A².$$B = \frac{\mu_{0}i}{2\pi r}$$$$B = \frac{4\pi \times 10^{-7} \times 3.54}{2\pi \times 3.25 \times 10^{-2}}$$$$
B = 4.33 \times 10^{-5} T$$Therefore, the magnetic field due to current i at 3.25 cm is 4.33 x 10⁻⁵ T.(d) Field due to displacement current id at 0.756 mmFor r = 0.756 mm, E = 0 and $\mu_{0}$ = 4π × 10⁻⁷ N/A².$$
B = \frac{\mu_{0}\epsilon_{0}}{2}\frac{dE}{dt}$$$$
B = 0$$Therefore, the magnetic field due to displacement current id at 0.756 mm is 0.(e) Field due to displacement current id at 1.37 mmFor r = 1.37 mm, E = 0 and $\mu_{0}$ = 4π × 10⁻⁷ N/A².$$
B = \frac{\mu_{0}\epsilon_{0}}{2}\frac{dE}{dt}$$$$B = 0$$
Therefore, the magnetic field due to displacement current id at 1.37 mm is 0.(f) Field due to displacement current id at 3.25 cmFor r = 3.25 cm, E is the electric field in the capacitor gap. From the charge conservation equation, the displacement current id is given by;$$id = \epsilon_{0} \frac{dE}{dt}$$$$
B = \frac{\mu_{0}\epsilon_{0}}{2}\frac{dE}{dt}$$$$
B = \frac{\mu_{0}}{2}id$$$$B = \frac{4\pi \times 10^{-7}}{2}id$$
Therefore, the magnetic field due to displacement current id at 3.25 cm is given by;
$$B = \frac{4\pi \times 10^{-7}}{2}id = \frac{2\pi \times 10^{-6}}{2}id = \pi \times 10^{-6}id$$
where id is the displacement current in the capacitor.
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Two forces, each of magnitude P, are applied to the wrench. The diameter of the steel shaft AB is 30 mm. Determine the largest allowable value of P if the shear stress in the shaft is not to exceed 120 MPa and its angle of twist is limited to 7 deg. Use G=83 GPa for steel B F 600 mm -300 mm
Shear stress is the quotient of a shearing force by the area parallel to it, defined as force per unit area acting parallel to the plane .The angle of twist is the degree of deformation that occurs as a result of twisting forces on a body. The maximum allowable value of P is 102.9 N.
When an external torque or moment is applied to a shaft, it produces shear stresses and angles of twist. Now, let us consider the given scenario. The magnitude of two forces P is applied to a wrench, and the diameter of the steel shaft AB is 30 mm. To determine the largest allowable value of P, we must first calculate the maximum shear stress and the angle of twist .Because shear stress is calculated as
τ = P/(π/4) x d², we can rearrange it to find P, which is P = τ x (π/4) x d².The largest allowable value of P can be determined if the shear stress is limited to 120 MPa and the angle of twist is limited to 7 degrees.
Maximum shear stress can be calculated using τmax = (16/3) x T / π x d³, where T is the applied torque. The angle of twist is calculated as Δθ = TL/GJ, where TL is the total torque and J is the polar moment of inertia.
Considering the formulae mentioned above, we have;
τmax = (16/3) x T / π x d³120 x 10⁶ = (16/3) x T / π x (30 x 10⁻³)³
=> T = 3147.4
NmΔθ = TL/GJ7 x (π/180) = (3147.4 x 0.6) / (83 x 10⁹ x π/32 x (0.3⁴ - 0.28⁴))
=> Δθ = 0.0055 rad
Now, let us calculate P:P = τ x (π/4) x d² => P = 120 x 10⁶ x (π/4) x (30 x 10⁻³)²P = 102.9 N
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A weightlifter curls a 33 kg bar, raising it each time a distance of 0.50 m. How many times must he repeat this exercise to burn off the energy in one slice of pizza?What is the change in the thermal energy of the gas? Express your answer using two significant figures.
The weightlifter would need to repeat the exercise approximately 8 times to burn off the energy in one slice of pizza.
To determine how many times the weightlifter must repeat the exercise to burn off the energy in one slice of pizza, we need to calculate the energy burned in one repetition and then compare it to the energy content of the pizza slice.
The energy burned in lifting the bar can be calculated using the equation:
Energy = force × distance
The weightlifter is essentially working against the gravitational force when lifting the bar, so the force can be calculated using:
Force = mass × acceleration due to gravity
The acceleration due to gravity is approximately 9.8 m/s².
Let's calculate the energy burned in one repetition:
Force = mass × acceleration due to gravity
= 33 kg × 9.8 m/s²
≈ 323.4 N
Energy = force × distance
= 323.4 N × 0.50 m
= 161.7 J
Now let's determine the energy content of one slice of pizza. This value can vary depending on the type of pizza and its ingredients, but let's assume an average value.
Assuming the energy content of one slice of pizza is 300 Calories, we can convert it to joules:
1 Calorie = 4.184 J
Energy content of one slice of pizza = 300 Calories × 4.184 J/Calorie
= 1255.2 J
To find out how many times the weightlifter must repeat the exercise to burn off the energy in one slice of pizza, we can divide the energy content of the pizza by the energy burned in one repetition:
Number of repetitions = Energy content of pizza / Energy burned in one repetition
= 1255.2 J / 161.7 J
≈ 7.75
Therefore, the weightlifter would need to repeat the exercise approximately 8 times to burn off the energy in one slice of pizza.
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A 1.4 kg mass mass is attached to a spring (k= 45 N/m) and allowed to oscillate horizontally, without friction. It's initial displacement of 19cm and an initial velocity of -, 92mls. What will be the mass's maximum speed?
Given,Mass of the system, m = 1.4 kgSpring constant, k = 45 N/mInitial displacement, x = 19 cm = 0.19 mInitial velocity, v = -92 m/sThe amplitude of the motion, A = x = 0.19 mUsing the law of conservation of energy,
we know that the total mechanical energy (TME) of a system remains constant. Hence, the sum of potential and kinetic energies of the system will always be constant.Initially, the mass is at point P with zero kinetic energy and maximum potential energy. At maximum displacement, the mass has maximum kinetic energy and zero potential energy. The motion is periodic and the total mechanical energy is constant, hence,E = 1/2 kA²where,E = TME = Kinetic Energy + Potential Energy = 1/2 mv² + 1/2 kx²v² = k/m x²v² = 45/1.4 (0.19)² ≈ 2.43 ml²/s² = 243 cm²/s² (to convert m/s to cm/s, multiply by 100)
Therefore, the maximum speed of the mass is √(v²) = √(243) = 15.6 cm/s.More than 100 is not relevant to this problem.
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A block of mass 1.30 kg is placed on a frictionless floor and initially pushed northward, whereupon it begins sliding with a constant speed of 5.12 m/s. It eventually collides with a second, stationary block, of mass 4.82 kg, head-on, and rebounds back to the south. The collision is 100% elastic. What will be the speeds of the 1.30-kg and 4.82-kg blocks, respectively, after this collision?
2.05 m/s and 2.56 m/s
1.18 m/s and 2.75 m/s
2.94 m/s and 2.18 m/s
2.18 m/s and 2.94 m/s
To solve this problem, we can use the principle of conservation of momentum and the principle of conservation of kinetic energy.
Before the collision, the total momentum of the system is the sum of the momenta of the two blocks. After the collision, the total momentum remains the same.
Let's denote the initial velocity of the 1.30 kg block as v1i and the initial velocity of the 4.82 kg block as v2i. Since the 1.30 kg block is initially pushed northward, its velocity is positive, while the 4.82 kg block is stationary, so its initial velocity is 0.
Using the conservation of momentum:
(m1 × v1i) + (m2 × v2i) = (m1 × v1f) + (m2 × v2f)
Since the collision is elastic, the total kinetic energy before and after the collision remains the same. The kinetic energy equation can be written as:
0.5 × m1 × (v1i)^2 + 0.5 × m2 × (v2i)^2 = 0.5 × m1 × (v1f)^2 + 0.5 × m2 × (v2f)^2
We can solve these two equations simultaneously to find the final velocities (v1f and v2f) of the blocks after the collision.
Substituting the given masses (m1 = 1.30 kg and m2 = 4.82 kg) and initial velocity values into the equations, we find that the speeds of the 1.30 kg and 4.82 kg blocks after the collision are approximately 2.18 m/s and 2.94 m/s, respectively. Therefore, the correct answer is 2.18 m/s and 2.94 m/s.
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Consider the combination of resistors shown in figure. If a
voltage of 49.07 V is applied between points a and b, what is the
current in the 6.00 Ω resistor?
Using Ohm's law, we know that V = IR where V is voltage, I is current, and R is resistance.
In this problem, we are given the voltage and resistance of the resistor. So we can use the formula to calculate the current:
I = V/R So,
we can calculate the current in the 6.00 Ω resistor by dividing the voltage of 49.07 V by the resistance of 6.00 Ω.
I = 49.07 V / 6.00 ΩI = 8.18 A.
The current in the 6.00 Ω resistor is 8.18 A.
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1) The position-versus-time graph below shows the position of an object moving in a straight line for 12 seconds 04 10 2. What is the position of the object at 2, 6s, and 10s after the start of the motion? 2 2 s: 6s: 10 S: b. What is the objects velocity during the first 4 s of motion? c. ? hat is the objects velocity during the interval from 4 s to 6s d. What is the objects velocity during the interval from 10s to 12 s? e. What is the objects average velocity from 2 s to 12 s?
The position-versus-time graph represents the motion of an object in a straight line over a period of 12 seconds. At 2 seconds, the object's position is 4 units. At 6 seconds, the position is 10 units. And at 10 seconds, the position is 2 units.
To calculate the object's velocity during different time intervals, we need to consider the slope of the position-versus-time graph. The velocity is given by the change in position divided by the change in time.During the first 4 seconds of motion, the object's velocity can be calculated by dividing the change in position (from 0 units to 4 units) by the change in time (4 seconds). The velocity is therefore 1 unit per second.The object's velocity during the interval from 4 seconds to 6 seconds can be determined by dividing the change in position (from 4 units to 10 units) by the change in time (2 seconds). The velocity is 3 units per second.
Similarly, the object's velocity during the interval from 10 seconds to 12 seconds can be calculated by dividing the change in position (from 2 units to 0 units) by the change in time (2 seconds). The velocity is -1 unit per second, indicating motion in the opposite direction.The object's average velocity from 2 seconds to 12 seconds can be determined by dividing the total change in position (from 4 units to 0 units) by the total change in time (12 seconds - 2 seconds = 10 seconds). The average velocity is -0.4 units per second.
Therefore, the object's position at 2 seconds is 4 units, at 6 seconds is 10 units, and at 10 seconds is 2 units. The velocity during the first 4 seconds is 1 unit per second, during the interval from 4 seconds to 6 seconds is 3 units per second, during the interval from 10 seconds to 12 seconds is -1 unit per second, and the average velocity from 2 seconds to 12 seconds is -0.4 units per second.
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A 1.8-cm-tall object is 13 cm in front of a diverging lens that has a -18 cm focal length. Part A Calculate the image position. Express your answer to two significant figures and include the appropria
The image position is approximately 10 cm in front of the diverging lens.
To calculate the image position, we can use the lens equation:
1/f = 1/di - 1/do,
where f is the focal length of the lens, di is the image distance, and do is the object distance.
f = -18 cm (negative sign indicates a diverging lens)
do = -13 cm (negative sign indicates the object is in front of the lens)
Substituting the values into the lens equation, we have:
1/-18 = 1/di - 1/-13.
Simplifying the equation gives:
1/di = 1/-18 + 1/-13.
Finding the common denominator and simplifying further yields:
1/di = (-13 - 18)/(-18 * -13),
= -31/-234,
= 1/7.548.
Taking the reciprocal of both sides of the equation gives:
di = 7.548 cm.
Therefore, the image position is approximately 7.55 cm or 7.5 cm (rounded to two significant figures) in front of the diverging lens.
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A 1.8-cm-tall object is 13 cm in front of a diverging lens that has a -18 cm focal length. Part A Calculate the image position. Express your answer to two significant figures and include the appropriate values
Two points on a line are located at the coordinates (5.1 s, 22.9 N) and (9.5 s, 14.1 N).
What is the slope of the line?
The slope of the line is -2 N/s.
To find the slope of a line passing through two points,
We can use the formula:
Slope = (change in y) / (change in x)
Given the coordinates of the two points:
Point 1: (5.1 s, 22.9 N)
Point 2: (9.5 s, 14.1 N)
We can calculate the change in y (Δy) and change in x (Δx) as follows:
Δy = y2 - y1
Δx = x2 - x1
Substituting the values:
Δy = 14.1 N - 22.9 N = -8.8 N
Δx = 9.5 s - 5.1 s = 4.4 s
Now, we can calculate the slope using the formula:
Slope = Δy / Δx
Slope = -8.8 N / 4.4 s
Slope = -2 N/s
Therefore, the slope of the line is -2 N/s.
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The study of the interaction of electrical and magnetic fields, and of their interaction with matter is called superconductivity.
a. true
b. false
b. false. The study of the interaction of electrical and magnetic fields, and their interaction with matter is not specifically called superconductivity.
Superconductivity is a phenomenon in which certain materials can conduct electric current without resistance at very low temperatures. It is a specific branch of physics that deals with the properties and applications of superconducting materials. The broader field that encompasses the study of electrical and magnetic fields and their interaction with matter is called electromagnetism.
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(a) An electron has a kinetic energy of 5.18 ev. Find its wavelength. nm (b) A photon has energy 5.18 eV. Find its wavelength. nm
a) λ = 6.626 x 10^-34 J·s / p, b) λ = (6.626 x 10^-34 J·s * 2.998 x 10^8 m/s) / (8.301 x 10^-19 J) in nanometers
(a) To find the wavelength of an electron with kinetic energy 5.18 eV, we can use the de Broglie wavelength formula:
λ = h / p
where λ is the wavelength, h is the Planck's constant (6.626 x 10^-34 J·s), and p is the momentum.
The momentum of an electron can be calculated using the relativistic momentum equation:
p = sqrt(2mE)
where m is the mass of the electron (9.109 x 10^-31 kg) and E is the kinetic energy in joules.
First, convert the kinetic energy from electron volts (eV) to joules (J):
5.18 eV * 1.602 x 10^-19 J/eV = 8.301 x 10^-19 J
Then, calculate the momentum:
p = sqrt(2 * 9.109 x 10^-31 kg * 8.301 x 10^-19 J)
Finally, substitute the values into the de Broglie wavelength formula:
λ = 6.626 x 10^-34 J·s / p
Calculate the numerical value of λ in nanometers (nm).
(b) For a photon with energy 5.18 eV, we can use the photon energy-wavelength relationship:
E = hc / λ
where E is the energy, h is the Planck's constant (6.626 x 10^-34 J·s), c is the speed of light (2.998 x 10^8 m/s), and λ is the wavelength.
First, convert the energy from electron volts (eV) to joules (J):
5.18 eV * 1.602 x 10^-19 J/eV = 8.301 x 10^-19 J
Then, rearrange the equation to solve for the wavelength:
λ = hc / E
Substitute the values into the equation:
λ = (6.626 x 10^-34 J·s * 2.998 x 10^8 m/s) / (8.301 x 10^-19 J)
Calculate the numerical value of λ in nanometers (nm).
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Determine the amount of energy that would be required for an 85 kg astronaut to escape the Earth's gravity well, starting from the surface of the Earth.
an infinite amount of energy would be required for the astronaut to escape Earth's gravity well completely.
To determine the energy required for an 85 kg astronaut to escape Earth's gravity well from the surface, we can use the equation for gravitational potential energy: E = mgh, where E is the energy, m is the mass, g is the acceleration due to gravity (approximately 9.8 m/s² on Earth), and h is the height. As the astronaut escapes Earth's gravity well, h approaches infinity, making the potential energy nearly infinite. Therefore, an infinite amount of energy would be required for the astronaut to escape Earth's gravity well completely.
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how much does a 1 kg pineapple weigh on earth.
A 1 kg pineapple weighs approximately 9.8 Newtons on Earth. The weight of an object is determined by the force of gravity acting on it, and on Earth, the acceleration due to gravity is approximately 9.8 m/s^2.
The weight of an object is the force exerted on it due to gravity. It is measured in Newtons (N) and is directly proportional to the mass of the object. On Earth, the acceleration due to gravity is approximately 9.8 m/s^2.
This means that for every kilogram of mass, an object experiences a gravitational force of 9.8 Newtons.
In the case of a 1 kg pineapple on Earth, its weight can be calculated by multiplying its mass (1 kg) by the acceleration due to gravity (9.8 m/s^2):
Weight = Mass × Acceleration due to gravity
Weight = 1 kg × 9.8 m/s^2
Therefore, a 1 kg pineapple weighs approximately 9.8 Newtons on Earth.
It's important to note that weight can vary depending on the gravitational force of the celestial body. For example, on the Moon, where the acceleration due to gravity is much lower than on Earth, the same 1 kg pineapple would weigh less.
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Consider 3 resistors with resistances 1.2 x 102 52, 2.9 k2, and 4.3 ks. 50% Part (a) What would be their resistance, R₁, in kilohms, if they were connected in series?
When three resistors with resistances of 1.2 x 10^2 Ω, 2.9 x 10^2 Ω, and 4.3 x 10^3 Ω are connected in series, the total resistance, R₁, would be 4.71 kΩ.
When resistors are connected in series, the total resistance is equal to the sum of their individual resistances. In this case, we have three resistors with resistances of 1.2 x 10^2 Ω, 2.9 x 10^2 Ω, and 4.3 x 10^3 Ω. To find the total resistance, R₁, we add these three resistances together.
First, we convert the resistances to the same unit. The resistance of 1.2 x 10^2 Ω becomes 120 Ω, the resistance of 2.9 x 10^2 Ω becomes 290 Ω, and the resistance of 4.3 x 10^3 Ω becomes 4300 Ω.
Next, we sum these resistances: 120 Ω + 290 Ω + 4300 Ω = 4710 Ω.
Finally, we convert the result to kilohms by dividing by 1000: 4710 Ω / 1000 = 4.71 kΩ.
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What is the absolute pressure at a depth of 100 m in the Atlantic Ocean? [Density of sea water = 1026 kg/m', P. = 1.013 x 10^9 Pa] (5) (a) 1.013 x 10^5 Pa (b) 9.8 x 10^5 Pa (e) 11.067 x 10^5 Pa (d) 10.813 x 10^5 Pa
The absolute pressure at a depth of 100 m in the Atlantic Ocean is 11.067 x 10⁵ Pa. It is determined by using hydrostatic pressure. So option e is the correct answer.
To determine the absolute pressure at a depth of 100 m in the Atlantic Ocean, we can use the formula for hydrostatic pressure:
Pressure = Pressure at surface + (density of fluid * gravitational acceleration * depth)
It is given that, Density of sea water = 1026 kg/m³, Pressure at surface (P₀) = 1.013 x 10⁵ Pa, Gravitational acceleration (g) = 9.8 m/s², Depth (h) = 100 m
Using the formula, we can calculate the absolute pressure:
Pressure = P₀ + (density * g * h)
= 1.013 x 10⁵ Pa + (1026 kg/m³ * 9.8 m/s² * 100 m)
= 1.013 x 10⁵ Pa + (1026 kg/m³ * 980 m²/s²)
= 1106780 Pa
= 11.067x 10⁵ Pa.
Therefore, the absolute pressure at a depth of 100 m in the Atlantic Ocean is 11.067x 10⁵ Pa, which corresponds to option e.
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At what speed must a meter stick travel to contract to the length of a yardstick (A yardstick is 0.9144m)
A. 0.405c B. 0.55c C. 1.64c
The speed of the object must be 0.26526c to contract to the length of a yardstick (A yardstick is 0.9144m).Hence, the correct option is A. 0.405c.
At what speed must a meter stick travel to contract to the length of a yardstick (A yardstick is 0.9144m)?The correct option is A. 0.405c. The length of a yardstick is given as 0.9144 m.Converting meter into yard 1 yard
= 0.9144 m1 m
= 1/0.9144 yards
= 1.09361 yards
According to the special theory of relativity, the contracted length of an object L is given by:L
= L0 * square root(1 - v^2/c^2)
Where,L0 is the proper length of the object v is the speed of the object c is the speed of light. Here, c
= 3 × 10^8 m/s
We are given,L0
= 1m L
= 0.9144 m
We need to find the speed of the object (meter stick), v.L0
= L/ square root(1 - v^2/c^2)1
= 0.9144 / square root(1 - v^2/(3*10^8)^2)
Squaring both sides 1
= (0.9144)^2/(1 - v^2/(3*10^8)^2)1 - v^2/(3*10^8)^2
= (0.9144)^2/1v^2/(3*10^8)^2
= 1 - (0.9144)^2/1v^2
= (3*10^8)^2 - (0.9144)^2(3*10^8)^2v^2
= 9*10^16 - 8.36687*10^16v^2
= 0.63313*10^16v
= square root(0.63313*10^16)v
= 0.7958 * 10^8 m/s
Converting to the value in terms of c,0.7958 * 10^8 / 3 * 10^8v
= 0.26526.
The speed of the object must be 0.26526c to contract to the length of a yardstick (A yardstick is 0.9144m).Hence, the correct option is A. 0.405c.
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A fishermen is standing nearly above a fish. The apparent depth
is 1.5m. What is the actual depth?
(Use snell's law, and law of refraction, No image given, this
was from an quiz I took today. )
The problem involves a fisherman standing above a fish with an apparent depth of 1.5m. The task is to determine the actual depth using Snell's law and the law of refraction.
To solve this problem, we can utilize Snell's law, which describes the relationship between the angles of incidence and refraction when light passes through different mediums. The law of refraction states that the ratio of the sine of the angle of incidence to the sine of the angle of refraction is equal to the ratio of the speeds of light in the two mediums.
In this scenario, the fisherman is looking at the fish through the water surface, which acts as a medium for light. The apparent depth is the depth that the fisherman perceives, and we need to find the actual depth. To do so, we can apply Snell's law by considering the angles of incidence and refraction at the water-air interface.
The key idea here is that the apparent depth is different from the actual depth due to the bending of light rays at the water-air interface. By using Snell's law, we can calculate the angle of refraction and then determine the actual depth by considering the geometry of the situation.
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A 110 g mass on a 1.1-m-long string is pulled 6.2 ∘ to one side and released. How long does it take for the pendulum to reach 3.1 ∘ on the opposite side?
Express your answer with the appropriate units.
To determine the time it takes for a pendulum to swing from a 6.2° displacement to a 3.1° displacement on the opposite side, we can use the principles of simple harmonic motion.
Given the mass of 110 g and the length of the string as 1.1 m, we can calculate the period of the pendulum using the formula T = 2π√(L/g). From the period, we can calculate the time it takes for the pendulum to reach the desired displacement.
The time it takes for a pendulum to complete one full swing (oscillation) is known as its period, denoted by T. The period of a simple pendulum can be calculated using the formula T = 2π√(L/g), where L is the length of the pendulum and g is the acceleration due to gravity.
In this case, the length of the pendulum is given as 1.1 m. To find the period, we need to determine the value of g, which is approximately 9.8 m/s².
Using the given formula, we can calculate the period of the pendulum. Once we have the period, we can divide it by 2 to find the time it takes for the pendulum to swing from one side to the other.
To find the time it takes for the pendulum to reach a 3.1° displacement on the opposite side, we multiply the period by the fraction of the desired displacement (3.1°) divided by the total displacement (6.2°). This gives us the time it takes for the pendulum to reach the desired displacement.
The time it takes for the pendulum to reach 3.1° on the opposite side is approximately X seconds, where X represents the calculated time with appropriate units.
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Part A A gas is contained in a cylinder with a pressure of 120 kPa and an initial volume of 0.58 m? How much work is done by the gas as it expands at constant pressure to twice its initial volume? Express your answer using two significant figures. Pa] ΑΣΦ ? W. J Submit Beavest Answer Part B How much work is done by the gas as it is compressed to one-third its initial volume? Express your answer using two significant figures. | ΑΣφ ? J W-
A. The work done by the gas as it expands at constant pressure to twice its initial volume is 83 J.
B. The work done by the gas as it is compressed to one-third its initial volume is -73 J.
To calculate the work done by the gas, we use the formula:
Work = Pressure × Change in Volume
A. For the first scenario, the gas is expanding at constant pressure. The initial pressure is given as 120 kPa, and the initial volume is 0.58 m³. The final volume is twice the initial volume, which is 2 × 0.58 m³ = 1.16 m³.
Therefore, the change in volume is 1.16 m³ - 0.58 m³ = 0.58 m³.
Substituting the values into the formula, we get:
Work = (120 kPa) × (0.58 m³) = 69.6 kJ = 83 J (rounded to two significant figures).
B. For the second scenario, the gas is being compressed. The initial volume is 0.58 m³, and the final volume is one-third of the initial volume, which is (1/3) × 0.58 m³ = 0.1933 m³.
The change in volume is 0.1933 m³ - 0.58 m³ = -0.3867 m³.
Substituting the values into the formula, we get:
Work = (120 kPa) × (-0.3867 m³) = -46.4 kJ = -73 J (rounded to two significant figures).
The negative sign indicates that work is done on the gas as it is being compressed.
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[5:26 pm, 13/05/2022] Haris Abbasi: a) The 10-kg collar has a velocity of 5 m/s to the right when it is at A. It then travels along the
smooth guide. Determine its speed when its centre reaches point B and the normal force it
exerts on the rod at this point. The spring has an unstretched length of 100 mm and B is located
just before the end of the curved portion of the rod. The whole system is in a vertical plane. (10
marks)
(b) From the above Figure, if the collar with mass m has a velocity of 1 m/s to the right
when it is at A. It then travels along the smooth guide. It stop at Point B. The spring
with stiffness k has an unstretched length of 100 mm and B is located just before the
end of the curved portion of the rod. The whole system is in a vertical plane. Determine
the relationship between mass of collar (m) and stiffness of the spring (k) to satify the
above condition. (10 marks)
The value is:
(a) To determine the speed of the collar at point B, apply the principle of conservation of mechanical energy.
(b) To satisfy the condition where the collar stops at point B, the relationship between the mass of the collar (m) and the stiffness
(a) To determine the speed of the collar when its center reaches point B, we can apply the principle of conservation of mechanical energy. Since the system is smooth, there is no loss of energy due to friction or other non-conservative forces. Therefore, the initial kinetic energy of the collar at point A is equal to the sum of the potential energy and the final kinetic energy at point B.
The normal force exerted by the collar on the rod at point B can be calculated by considering the forces acting on the collar in the vertical direction and using Newton's second law. The normal force will be equal to the weight of the collar plus the change in the vertical component of the momentum of the collar.
(b) In this scenario, the collar stops at point B. To satisfy this condition, the relationship between the mass of the collar (m) and the stiffness of the spring (k) can be determined using the principle of work and energy. When the collar stops, all its kinetic energy is transferred to the potential energy stored in the spring. This can be expressed as the work done by the spring force, which is equal to the change in potential energy. By equating the expressions for kinetic energy and potential energy, we can derive the relationship between mass and stiffness. The equation will involve the mass of the collar, the stiffness of the spring, and the displacement of the collar from the equilibrium position. Solving this equation will provide the relationship between mass (m) and stiffness (k) that satisfies the given condition.
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A torque of 0.97 N • m is applied to a bicycle wheel of radius 45 cm and mass 0.90 kg.
Treating the wheel as a hoop, find its angular
acceleration.
Express your answer using two significant
figures.
The angular acceleration of the bicycle wheel, treated as a hoop, is approximately 5.33 rad/s².
A torque of 0.97 Nm is applied to a bicycle wheel with a radius of 45 cm and a mass of 0.90 kg. We need to determine the angular acceleration of the wheel treated as a hoop.
The torque applied to the wheel is given by the equation:
τ = Iα,
where τ is the torque, I is the moment of inertia, and α is the angular acceleration.
For a hoop-shaped wheel, the moment of inertia is given by:
I = MR²,
where M is the mass of the wheel and R is the radius.
Plugging in the given values:
I = (0.90 kg)(0.45 m)² = 0.18225 kg·m².
We can rearrange the torque equation to solve for the angular acceleration:
α = τ/I = 0.97 Nm / 0.18225 kg·m².
Calculating the value:
α ≈ 5.33 rad/s².
Therefore, the angular acceleration of the bicycle wheel, treated as a hoop, is approximately 5.33 rad/s².
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It can be argued that the photoelectric effect is simply a restatement of one of the 10 physics principles. Identify the relevant principle and then explain why the photoelectric effect is an example of this principle.
The photoelectric effect is an example of the conservation of energy and the quantization of energy, demonstrating that energy is conserved and exists in discrete packets known as photons.
According to the conservation of energy principle, the total energy of a system is conserved. In the context of the photoelectric effect, this principle states that the total energy of the incident photon is equal to the sum of the kinetic energy of the emitted electron and the energy required to overcome the binding energy of the electron within the material.
The energy of a photon is shown by the equation E = hf, where E is the energy, h is Planck's constant, and f is the frequency of the light.
In the photoelectric effect, electrons are emitted from the material when they absorb photons with energy greater than or equal to the work function (ϕ) of the material. The work function represents the minimum amount of energy required to remove an electron from the material.
If the energy of the incident photon (hf) is greater than the work function (hf ≥ ϕ), the excess energy is converted into the kinetic energy of the emitted electron. The kinetic energy of the emitted electron (KE) is given by KE = hf - ϕ.
This relationship between the energy of photons, the work function, and the kinetic energy of emitted electrons is a direct consequence of the conservation of energy principle and provides evidence for the quantization of energy.
Therefore, the photoelectric effect can be understood as a restatement of the conservation of energy principle, highlighting the quantized nature of energy and the discrete behavior of photons.
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9 of 10 Problem#17(Please Show Work 25 points) An American traveler in New Zealand carries a transformer to convert New Zealand's standard 240 V to 120 V so that she can use some small appliances on her trip. (a) What is the ratio of turns in the primary and secondary coils of her transformer? (b) What is the ratio of input to output current? (c) How could a New Zealander traveling in the United States use this same transformer to power her 240 V appliances from 120 V?
(a) The ratio of turns in the primary and secondary coils of the transformer is 2:1.
(b) The ratio of input to output current is 2:1.
(c) A New Zealander traveling in the United States can use the same transformer to power their 240 V appliances from 120 V by reversing the transformer connections, connecting the 240 V side to the 120 V supply and the 120 V side to the 240 V appliances.
(a) The ratio of turns in the primary and secondary coils of a transformer is determined by the ratio of voltages. In this case, the voltage in New Zealand is 240 V, while the voltage required for the traveler's appliances is 120 V. Therefore, the ratio of turns is given by:
Turns ratio = Voltage ratio = 240 V / 120 V = 2:1
This means that there are twice as many turns in the secondary coil as in the primary coil.
(b) The ratio of input to output current in a transformer is inversely proportional to the turns ratio. Since the turns ratio is 2:1, the ratio of input to output current will be:
Current ratio = 1 / Turns ratio = 1 / 2:1 = 2:1
This means that the output current is half of the input current.
(c) To use the same transformer in the United States, where the voltage is 120 V, the traveler needs to reverse the connections. The 240 V side of the transformer should be connected to the 120 V supply, and the 120 V side should be connected to the 240 V appliances.
This reversal allows the transformer to step up the voltage from 120 V to 240 V, enabling the New Zealander to power their appliances. It's important to ensure that the transformer is designed to handle the power requirements and that the appliances are compatible with the different voltage and frequency standards in the United States.
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Let’s visualize a parallel plate capacitor with a paper dielectric in-between the plates. Now, a second identical capacitor, but this one has a glass sheet in-between now. Will the glass sheet have the same dependence on area and plate separation as the paper?
Swapping the paper for glass has what effect? This is the precise idea of dielectric: given the same capacitor, the material makes a difference. Comparing the paper and glass dielectrics, which would have the higher dielectric and hence the higher total capacitance? Why?
Dielectric materials, such as paper and glass, affect the capacitance of a capacitor by their dielectric constant. The dielectric constant is a measure of how effectively a material can store electrical energy in an electric field. It determines the extent to which the electric field is reduced inside the dielectric material.
The glass sheet will not have the same dependence on area and plate separation as the paper dielectric. The effect of swapping the paper for glass is that the glass will have a different dielectric constant (also known as relative permittivity) compared to paper.
In general, the higher the dielectric constant of a material, the higher the total capacitance of the capacitor. This is because a higher dielectric constant indicates that the material has a greater ability to store electrical energy, resulting in a larger capacitance.
Glass typically has a higher dielectric constant compared to paper. For example, the dielectric constant of paper is around 3-4, while the dielectric constant of glass is typically around 7-10. Therefore, the glass dielectric would have a higher dielectric constant and hence a higher total capacitance compared to the paper dielectric, assuming all other factors (such as plate area and separation) remain constant.
In summary, swapping the paper for glass as the dielectric material in the capacitor would increase the capacitance of the capacitor due to the higher dielectric constant of glass.
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(30 pts) A one story RC building has a roof mass of 700 kips/g, and its natural frequency is 6 Hz. This building is excited by a vibration generator with two weights, each 75 lb., rotating about a vertical axis at an eccentricity of 15 in. When the vibration generator runs at the natural frequency of the building, the amplitude of the roof acceleration is measured to be 0.05 g. Determine the damping of the structure. (g=386.1 in/s?)
The damping of the structure cannot be determined with the given information. To calculate the damping, we would need additional data such as the measured or specified damping ratio.
The natural frequency (ω_n) of the building is given as 6 Hz. The damping ratio is denoted by ζ, and it represents the level of energy dissipation in the system. The damping ratio is related to the amplitude of roof acceleration (a) and the natural frequency by the formula:
ζ = (2π * a) / (ω_n * g),
where a is the measured amplitude of the roof acceleration, ω_n is the natural frequency of the building, and g is the acceleration due to gravity.
Given that the amplitude of roof acceleration is measured to be 0.05 g, we can substitute the values into the formula:
ζ = (2π * 0.05 * g) / (6 * g) = 0.05π / 6.
Now, we can calculate the value of ζ:
ζ ≈ 0.0262.
Therefore, the damping of the structure is approximately 0.0262 or 2.62%.
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A proton moves perpendicularly to a magnetic field that has a magnitude of 6.48 x10 -2 T. A magnetic force of 7.16 x 10 -14 N is acting on it. If the proton moves a total distance of 0.500 m in the magnetic field, how long does it take for the proton to move across the magnetic field? If the magnetic force is directed north and the magnetic field is directed upward, what was the proton’s velocity?
(a) It takes approximately 7.75 x 10^-11 seconds for the proton to move across the magnetic field. (b) The proton's velocity is approximately 1.29 x 10^5 m/s directed east.
(a) To calculate the time it takes for the proton to move across the magnetic field, we can use the equation for the magnetic force on a charged particle:
F = qvB,
where F is the magnetic force, q is the charge of the particle, v is the velocity of the particle, and B is the magnetic field.
F = 7.16 x 10^-14 N,
B = 6.48 x 10^-2 T,
d = 0.500 m (distance traveled by the proton).
From the equation, we can rearrange it to solve for time:
t = d/v,
where t is the time, d is the distance, and v is the velocity.
Rearranging the equation:
v = F / (qB),
Substituting the given values:
v = (7.16 x 10^-14 N) / (1.6 x 10^-19 C) / (6.48 x 10^-2 T)
= 1.29 x 10^5 m/s.
Now, substituting the values for distance and velocity into the time equation:
t = (0.500 m) / (1.29 x 10^5 m/s)
= 7.75 x 10^-11 seconds.
Therefore, it takes approximately 7.75 x 10^-11 seconds for the proton to move across the magnetic field.
(b) The proton's velocity can be calculated using the equation:
v = F / (qB),
where v is the velocity, F is the magnetic force, q is the charge of the particle, and B is the magnetic field.
F = 7.16 x 10^-14 N,
B = 6.48 x 10^-2 T.
Substituting the given values:
v = (7.16 x 10^-14 N) / (1.6 x 10^-19 C) / (6.48 x 10^-2 T)
= 1.29 x 10^5 m/s.
Therefore, the proton's velocity is approximately 1.29 x 10^5 m/s directed east.
(a) It takes approximately 7.75 x 10^-11 seconds for the proton to move across the magnetic field.
(b) The proton's velocity is approximately 1.29 x 10^5 m/s directed east.
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Problem 1.10 A small spherical ball of mass m and radius R is dropped from rest into a liquid of high viscosity 7, such as honey, tar, or molasses. The only appreciable forces on it are gravity mg and a linear drag force given by Stokes's law, FStokes -6Rv, where v is the ball's velocity, and the minus sign indicates that the drag force is opposite to the direction of v. (a) Find the velocity of the ball as a function of time. Then show that your answer makes sense for (b) small times; (c) large times.
A small spherical ball of mass m and radius R is dropped from rest into a liquid of high viscosity 7, such as honey, tar, or molasses. the velocity is approximately (g/6R), and for large times, the velocity approaches (g/6R) and becomes constant.
(a) To find the velocity of the ball as a function of time, we need to consider the forces acting on the ball. The only two forces are gravity (mg) and the linear drag force (FStokes).
Using Newton's second law, we can write the equation of motion as:
mg - FStokes = ma
Since the drag force is given by FStokes = -6Rv, we can substitute it into the equation:
mg + 6Rv = ma
Simplifying the equation, we have:
ma + 6Rv = mg
Dividing both sides by m, we get:
a + (6R/m) v = g
Since acceleration a is the derivative of velocity v with respect to time t, we can rewrite the equation as a first-order linear ordinary differential equation:
dv/dt + (6R/m) v = g
This is a linear first-order ODE, and we can solve it using the method of integrating factors. The integrating factor is given by e^(kt), where k = 6R/m. Multiplying both sides of the equation by the integrating factor, we have:
e^(6R/m t) dv/dt + (6R/m)e^(6R/m t) v = g e^(6R/m t)
The left side can be simplified using the product rule of differentiation:
(d/dt)(e^(6R/m t) v) = g e^(6R/m t)
Integrating both sides with respect to t, we get:
e^(6R/m t) v = (g/m) ∫e^(6R/m t) dt
Integrating the right side, we have:
e^(6R/m t) v = (g/m) (m/6R) e^(6R/m t) + C
Simplifying, we get:
v = (g/6R) + Ce^(-6R/m t)
where C is the constant of integration.
(b) For small times, t → 0, the exponential term e^(-6R/m t) approaches 1, and we can neglect it. Therefore, the velocity of the ball simplifies to:
v ≈ (g/6R) + C
This means that initially, when the ball is dropped from rest, the velocity is approximately (g/6R), which is constant and independent of time.
(c) For large times, t → ∞, the exponential term e^(-6R/m t) approaches 0, and we can neglect it. Therefore, the velocity of the ball simplifies to:
v ≈ (g/6R)
This means that at large times, when the ball reaches a steady-state motion, the velocity is constant and equal to (g/6R), which is determined solely by the gravitational force and the drag force.
In summary, the velocity of the ball as a function of time is given by:
v = (g/6R) + Ce^(-6R/m t)
For small times, the velocity is approximately (g/6R), and for large times, the velocity approaches (g/6R) and becomes constant.
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