A _____ is that part of a rotating electric device that allows free movement. a. brush b. contact c. wye d. bearing

Answers

Answer 1

A bearing is that part of a rotating electric device that allows free movement. The correct option is D.

A bearing is an essential component of any rotating electric device. It is a device that supports and reduces friction between the moving parts of a machine, allowing them to rotate freely. Bearings are found in a wide range of devices, including electric motors, generators, turbines, and other machines. They are designed to support axial and radial loads and can be classified as either sliding or rolling bearings.

Rolling bearings are the most commonly used type of bearings in rotating electric devices. They consist of an outer race, an inner race, rolling elements (usually balls or rollers), and a cage. Rolling bearings are designed to reduce friction and allow for smooth operation even under heavy loads. They are available in a variety of sizes and designs to suit different applications.

In summary, a bearing is an essential component of a rotating electric device that allows for free movement. It is a device that supports and reduces friction between the moving parts of a machine, allowing them to rotate freely. Bearings are available in various types, designs, and sizes to suit different applications. The answer to your question is D.

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Related Questions

he star Jakondah has a distance of 20 light-years. If the speed of light were double its current value, what would the distance to Jakondah be

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The distance to Jakondah would remain the same at 20 light-years, as the speed of light doesn't affect distances.

While it may seem intuitive that doubling the speed of light would affect the distance to Jakondah, it's essential to understand that light-years measure distance, not time.

A light-year is the distance that light travels in a vacuum in one year.

Therefore, even if the speed of light were to double, the actual distance between Earth and Jakondah would remain the same, at 20 light-years.

However, it's worth noting that if the speed of light were indeed doubled, light from Jakondah would reach us in half the time it currently takes.

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Describe the variation of the net force on and the acceleration of a mass on a spring as it executes simple harmonic motion.

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The net force on a mass on a spring as it executes simple harmonic motion varies in magnitude and direction but always points towards the equilibrium position.

The force is directly proportional to the displacement of the mass from its equilibrium position. As the mass moves away from the equilibrium position, the net force increases, reaching its maximum when the mass is at the maximum displacement. Similarly, the acceleration of the mass on a spring also varies in magnitude and direction.

The acceleration is zero at the equilibrium position and reaches its maximum at the maximum displacement. The acceleration is directly proportional to the displacement and inversely proportional to the mass of the object.

The period of the oscillation is determined by the mass and the spring constant, and is independent of the amplitude of the oscillation.

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________ is the distance between one point on a wave and the nearest point just like it.
O Amplitude
O Crest Frequency
O Wavelength

Answers

Answer: wavelength

Explanation:

If the potential drop across an opening operating 300-watt floodlight is 120 volts, what is the current through the floodlight.

Answers

The current through the floodlight is 2.5 amperes.

The power P consumed by an electrical device can be expressed as:

P = V x I

where V is the voltage across the device, I is the current flowing through the device, and P is the power consumed by the device.

In this problem, the power consumed by the 300-watt floodlight is given as P = 300 W and the potential drop across the floodlight is V = 120 V. To find the current I flowing through the floodlight, we can rearrange the equation as follows:

I = P / V

Substituting the given values, we get:

I = 300 W / 120 V

I = 2.5 A

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The mass of an electric car is 900 kg including the passengers. A single motor mounted on the front wheels drives the car, and the radius of the wheel is 0.3 m. The car is going downhill at a speed of 50 km/hr, and the slope of the hill is 30 degree. The friction coefficient of the road surface at a given weather condition is 0.5. Ignore the motor losses and compute the power generated by the electric machine

Answers

The electric motor produces around 10.4 kW of power.

the following example: (900 kg x 9.81 m/s2 x sin(30) = 4414.5 N) The force operating on the car as it descends the slope is equal to the weight of the car multiplied by the sine of the slope angle. The friction force is calculated as follows: (900 kg x 9.81 m/s2 x 0.5) = 4414.5 N. The friction force is generated by the car's weight multiplied by the friction coefficient. As a result, there is no acceleration and there is no net force acting on the car. The frictional force times the vehicle's speed, or (4414.5 N) x (50 km/hr x 1000 m/km / 3600 s/hr), equals the power produced by the motor, or 10.4 kW.

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In a Class 2 circuit, because the power source of the circuit is limited, ____ overcurrent protection is required.

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In a Class 2 circuit, because the power source of the circuit is limited, extra overcurrent protection is required. This is because Class 2 circuits are designed to provide a limited amount of electrical energy and are often used to power low voltage devices such as sensors, LED lighting, and communication equipment.

Without proper overcurrent protection, these circuits could be at risk of overheating, short-circuiting, or even catching fire. Therefore, it is important to use appropriate overcurrent protection devices such as fuses or circuit breakers to protect the circuit and ensure safe operation.

A Class 2 circuit is a low-voltage electrical circuit that is designed to operate at a power level that is less than 100 watts and a maximum of 24 volts. It is commonly used for lighting and control systems in buildings.

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A baseball player slides into third base with an initial speed of 4.2 m/s . Part A If the coefficient of kinetic friction between the player and the ground is 0.50, how far does the player slide before coming to rest

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The baseball player slides for 1.8 meters before coming to rest. To determine how far the baseball player slides before coming to rest, we first need to calculate the acceleration due to friction.

We can use the formula a = μk * g, where μk is the coefficient of kinetic friction and g is the acceleration due to gravity (9.8 m/s²).

a = μk * g
a = 0.50 * 9.8
a = 4.9 m/s²

Next, we can use the kinematic equation vf² = vi² + 2ad, where vf is the final velocity (0 m/s), vi is the initial velocity (4.2 m/s), a is the acceleration due to friction (-4.9 m/s²), and d is the distance we are trying to find.

vf²= vi² + 2ad
0 = (4.2)² + 2(-4.9)d
0 = 17.64 - 9.8d
9.8d = 17.64
d = 1.8 meters

Therefore, the baseball player slides for 1.8 meters before coming to rest.

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What makes astronomers believe that the energy source in quasars is only a few light months across at maximum (the distance light travels in a few months)

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Astronomers believe that the energy source in quasars is only a few light months across at maximum due to several factors such as the brightness variability, immense energy output, and the compact nature of quasars.

Quasars, or quasi-stellar objects, are among the most luminous and energetic objects in the universe. They can emit immense amounts of energy, up to a thousand times that of our entire galaxy, within a relatively small region. The brightness of quasars can vary significantly over short time periods, sometimes as short as a few days. This rapid variability indicates that the energy source must be relatively small in size, as larger objects would take longer to exhibit such changes in brightness.

Based on these factors, astronomers have deduced that the energy source powering quasars must be compact, with a size on the order of a few light months across at maximum. This compact nature is consistent with the current understanding that quasars are powered by supermassive black holes at the centers of galaxies, with the energy output primarily coming from the accretion of matter onto the black hole.

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Worked Example 6 Two forces 10N and 20N are inclined at angle 60 to each other. Find the resultant force. Solution​

Answers

Used tip-to-toe method

Hope this helps :)

True or false. The period of a particle moving in a circle in a uniform B field is independent of the radius and speed of the particle.

Answers

Answer:

False. The period of a particle moving in a circle in a uniform B field is dependent on the radius and speed of the particle. Specifically, the period is given by T = 2πm/(qB), where m is the mass of the particle, q is its charge, B is the magnitude of the magnetic field, and the radius is given by R = mv/(qB), where v is the speed of the particle.

The period of a particle moving in a circle in a uniform B field is independent of the radius and speed of the particle is true because when a charged particle moves in a uniform magnetic field (B field), it experiences a magnetic force, which causes it to move in a circular path.

The period of this motion can be determined by the following equation:
T = 2πm / (qB)

In this equation:


- T represents the period of the particle's motion.
- m is the mass of the particle.
- q is the charge of the particle.
- B is the magnitude of the magnetic field.

As you can see, the period (T) is determined only by the mass (m), charge (q), and magnetic field strength (B). The radius and speed of the particle do not appear in this equation, which means the period is independent of these factors.

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To navigate, a porpoise emits a sound wave that has a wavelength of 1.4 cm. The speed at which the wave travels in seawater is 1522 m/s. Find the period of the wave.

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The period of the sound wave emitted by the porpoise is 9.19 microseconds.

The period of a wave is the time it takes for one complete cycle of the wave. It is related to the frequency of the wave by the equation:

T = 1/f

where T is the period and f is the frequency.

The speed of the wave can be expressed as the product of its wavelength and frequency:

v = λf

where v is the speed, λ is the wavelength, and f is the frequency.

We can rearrange this equation to solve for the frequency:

f = v/λ

In this case, the wavelength is 1.4 cm, which we can convert to meters:

λ = 1.4 cm = 0.014 m

The speed is 1522 m/s, so we can plug in these values and solve for the frequency:

f = 1522 m/s / 0.014 m = 108714 Hz

Now we can use the equation for the period to find the answer:

T = 1/f = 1 / 108714 Hz = 9.19 μs

Therefore, the period of the sound wave emitted by the porpoise is 9.19 microseconds.

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What is the height of a student whose z-score is 3? 55"" 53"" 47"" 43""

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The mean height of the students in the group is 47 inches.

To find the mean height of the students in the group, we need to sum up all the heights and divide by the total number of students. Using the given table, we have:

Total height = 45 + 48 + 49 + 40 + 53 = 235 inches

Total number of students = 5

Mean height = Total height / Total number of students

= 235 / 5

= 47 inches

Therefore, the mean height of the students in the group is 47 inches.

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Full Question: What is the mean height of the students in the group? 1-47 inches 2-49 inches 3-51 inches 4-53 inches The table shows the heights of students in a group. Student Height (in inches) A 45 B. 48 49 D. 40 53 E.

Answer:

55

Explanation:

A certain radioactive material is known to decay at a rate proportional to the amount present. If after one hour it is observed that 10 percent of the material has decayed, find the half-life (period of time it takes for the amount of material to decrease by half) of the material (in hrs.).

a.6.58

b.8.58

c.10.58

d.12.58

Answers

Certain radioactive material is known to decay at a rate proportional to the amount present. If after one hour it is observed that 10 percent of the material has decayed, the half-life of the material is 10.58 hrs.

We can use the formula for exponential decay, which states that the amount of material remaining after time t is given by:

N(t) = [tex]N0 e^{(-kt)}[/tex]

where N0 is the initial amount of material, k is the decay constant, and e is the base of the natural logarithm.

If 10% of the material has decayed after one hour, then the remaining amount of material is 90% of the initial amount, or N(1) = 0.9 N0.

These values are entered into the exponential decay equation to produce the following results:

0.9 N0 = [tex]N0 e^{(-k)}[/tex]

We can divide both sides by N0 to make things simpler:

0.9 = [tex]e^{(-k)}[/tex]

After calculating the natural logarithm of both sides, we arrive at:

ln(0.9) = -k

Solving for k, we get:

k = -ln(0.9)

The half-life is the time it takes for the amount of material to decrease by half. Let's call this time T. Then, we can write:

N(T) = 0.5 N0

Substituting into the exponential decay equation, we get:

0.5 N0 = [tex]N0 e^{(-kT)}[/tex]

We can divide both sides by N0 to make things simpler:

0.5 = [tex]e^{(-kT)}[/tex]

If we take the natural logarithm of both sides, we obtain:

ln(0.5) = -kT

When we replace the value of k we discovered earlier, we obtain:

ln(0.5) = ln(0.9) T

Solving for T, we get:

T = ln(2) / ln(0.9)

Using a calculator, we find:

T ≈ 10.58

Therefore, the half-life of the material is approximately 10.58 hours. Answer: (c)

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A particular linearly polarized electromagnetic wave has a peak magnetic field of 5.0 x 10^{-6} T, which is about one-tenth the magnitude of the Earth's magnetic field. If this wave reflects straight back from a mirror, what is the pressure the wave exerts on the mirror

Answers

The pressure exerted by the reflected wave is [tex]1.25 * 10^-^9 Pa[/tex].

To calculate the pressure exerted by the reflected wave, we can use the formula P = (2I)/c, where P is pressure, I is the intensity of the wave, and c is the speed of light.

The intensity can be found using the equation I = (1/2)ε_0c[tex]E^2[/tex], where ε_0 is the electric constant, c is the speed of light, and E is the electric field amplitude.

Since the wave is linearly polarized, we know that the electric field amplitude is equal to the magnetic field amplitude, so E = Bc.

Plugging in the values given in the question, we find that I = [tex]6.25 * 10^-^1^5 W/m^2[/tex], and therefore P = [tex]1.25 * 10^-^9[/tex] Pa.

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A wire carrying a current of 0.25 A is 0.5 m long. If the wire is perpendicular to a magnetic field of 0.6 T, how much is the magnetic force on the wire

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The magnetic force on a current-carrying wire in a magnetic field can be calculated using the formula F = BIL, where F is the magnetic force, B is the magnetic field, I am the current, and L is the length of the wire. In this case, the wire is perpendicular to the magnetic field, so we can simplify the equation to F = BIL. F = 0.075 N


The magnetic force on the wire carrying a current of 0.25 A and perpendicular to a magnetic field of 0.6 T is 0.075 N. It is important to note that the direction of the magnetic force is perpendicular to both the direction of the current and the direction of the magnetic field. To find the magnetic force on a wire carrying a current in a perpendicular magnetic field, we can use the following formula Magnetic Force (F) = Current (I) × Length of wire (L) × Magnetic Field (B) × sin(θ)
Here, θ is the angle between the current direction and the magnetic field. Since the wire is perpendicular to the magnetic field, the angle θ is 90 degrees. The sine of a 90-degree angle is 1, so sin(θ) = 1. Current (I) = 0.25 A Length of wire (L) = 0.5 m Magnetic Field (B) = 0.6 T Magnetic Force (F) = (0.25 A) × (0.5 m) × (0.6 T) × sin (90°) F = (0.25 A) × (0.5 m) × (0.6 T) × 1 F = 0.075 N The magnetic force on the wire is 0.075 N.

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A point of light located in the upper left of the visual field is projected to the _______ part of the retina. qukzet

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The point of light located in the upper left of the visual field is projected to the lower right part of the retina.


The human eye is a complex organ that is capable of detecting light and converting it into neural signals that the brain can interpret.

When a point of light is located in the upper left of the visual field, it is projected to the lower right part of the retina. This is because of the way that light rays enter the eye and are refracted by the cornea and lens.

The retina is a thin layer of cells at the back of the eye that contains specialized cells called photoreceptors. These cells convert light into electrical signals that are sent to the brain via the optic nerve.

The brain then interprets these signals as visual images.

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Suppose you were looking at two stars, both at the same distance, but while star A is a G5 I, star B is a G5 III. How would they look different to you in a telescope

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In a telescope, star A and star B would appear equally bright, since they are at the same distance.

However, star B would appear larger and redder than star A, due to its larger size and cooler temperature as a giant star (III) compared to a main-sequence star (I).To elaborate, the Roman numeral following the spectral class (G5) indicates the luminosity class or size of the star. "I" means it's a main-sequence star (like our sun), while "III" means it's a giant star. Giant stars have a larger diameter than main-sequence stars, and they are cooler, which makes them appear more reddish in color. Therefore, star B would appear larger and redder than star A in a telescope, despite being equally bright.

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The star named Capella has an apparent magnitude of 0, whereas the star named Polaris has an apparent magnitude of 2, which means that Capella appears __________ Polaris in the night sky.

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In the context of magnitude, a lower value represents a brighter object. Therefore, the star Capella appears brighter than Polaris in the night sky.

Based on the given information, the star named Capella has an apparent magnitude of 0, whereas the star named Polaris has an apparent magnitude of 2.

A lower value in the context of magnitude denotes a brighter item. Polaris and Capella are hence more visible in the night sky.

Polaris and Capella are two stars that can be seen in the night sky. About 42 light-years from Earth, in the constellation Auriga, is a yellow giant star called Capella. The star, which is among the brightest in the sky, is actually a system of four stars that revolve around a single mass centre. A yellow-white supergiant star called Polaris, sometimes referred to as the North Star or Pole Star, may be found in the constellation Ursa Minor, around 323 light-years from Earth. It has been used for navigation by seafarers and astronomers for millennia and is renowned for its close alignment with the Earth's rotational axis.


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In a choir practice room, two parallel walls are 6.50 m apart. The singers stand against the north wall. The organist faces the south wall, sitting 0.820 m away from it. To enable her to see the choir, a flat mirror 0.600 m wide is mounted on the south wall, straight in front of her. What width of the north wall can the organist see

Answers

In this scenario, the organist is sitting 0.820 m away from the south wall and there is a mirror mounted on the south wall that is 0.600 m wide. The mirror is placed in such a way that it reflects the image of the B standing against the north wall towards the organist. Therefore, the organist can see the reflection of the choir through the mirror.
 
To calculate the width of the north wall that the organist can see, we need to use the concept of similar triangles. The distance between the north and south walls is 6.50 m, and the distance between the mirror and the choir is the same as the distance between the organist and the mirror (0.820 m). Let's call the width of the north wall that the organist can see "x".
Using similar triangles, we can set up the following equation:  x/0.820 = 0.600/6.50
Solving for "x", we get:  x = 0.057 m or 5.7 cm
Therefore, the organist can see a width of 5.7 cm of the north wall through the mirror.

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If you carry a heavy bag of groceries and bang your hand against the wall, the concept that best explains why your hand hurts is gravity. inertia. resistance. none of the above g

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The concept that best explains why your hand hurts is inertia.

When you carry a heavy bag of groceries and accidentally bang your hand against a wall, the concept that best explains why your hand hurts is inertia.

Inertia is the tendency of an object to resist changes in its state of motion, which includes changes in speed and direction.

When your hand hits the wall, it suddenly stops moving while the rest of your body is still in motion, causing a force to be exerted on your hand.

This sudden change in motion results in a painful sensation in your hand.

While gravity and resistance may play a role in other physical scenarios, inertia is the most relevant concept to explain this specific situation.

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How much energy is required to move a 1250 kg object from the Earth's surface to an altitude twice the Earth's radius

Answers

The amount of energy required to move a 1250 kg object from the Earth's surface to an altitude twice the Earth's radius is approximately 10.2 x [tex]10^9[/tex] joules.

The formula for gravitational potential energy is:

U = mgh

The height above the Earth's surface is therefore:

h = 12,742 km - 6,371 km = 6,371 km

Next, we need to calculate the acceleration due to gravity at this height. The acceleration due to gravity decreases with distance from the Earth's surface, so we need to use the formula:

g = G*M/r²

At a height of 6,371 km, the distance from the center of the Earth is:

r = 6,371 km + 6,371 km = 12,742 km

The mass of the Earth is approximately 5.97 x [tex]10^{24[/tex] kg, and the gravitational constant is approximately 6.67 x [tex]10^{-11[/tex]N*(m/kg)². Plugging these values into the formula gives:

g = (6.67 x [tex]10^{-11[/tex] N*(m/kg)²)*(5.97 x [tex]10^{24[/tex] kg)/(12,742 km)²

= 1.31 m/s²

Finally, we can plug in the values of m, g, and h into the formula for gravitational potential energy:

U = mgh

= (1250 kg)(1.31 m/s²)(6,371 km * 1000)

= 10.2 x [tex]10^9[/tex] J

Potential energy is a type of energy that an object possesses by virtue of its position or configuration relative to other objects in its surroundings. It is the energy that is stored within an object, and it can be released to perform work when the object undergoes a change in position or configuration.

There are several types of potential energy, including gravitational potential energy, elastic potential energy, and electric potential energy. Gravitational potential energy is the energy that an object possesses by virtue of its position in a gravitational field. Elastic potential energy is the energy that is stored in a stretched or compressed spring or other elastic material. Electric potential energy is the energy that is stored in an electrically charged object.

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A garden hose of inner radius 1.2 cm carries water at 2.0 m/s. The nozzle at the end has radius 0.28 cm. How fast does the water move through the nozzle

Answers

The water moves through the nozzle at a velocity of 36.8 m/s.

The continuity equation states that the product of the cross-sectional area of a pipe and the fluid velocity is constant, assuming that the fluid is incompressible and there are no leaks in the system. Mathematically, this can be expressed as:

A1v1 = A2v2

where A1 and A2 are the cross-sectional areas of the pipe at two different points, and v1 and v2 are the fluid velocities at those points.

In this problem, we can use the continuity equation to find the velocity of water through the nozzle. We can assume that the volume flow rate of water is constant along the hose, so the product of the cross-sectional area and velocity at any point must be the same.

Let's call the cross-sectional area of the hose A1 and the cross-sectional area of the nozzle A2. The radius of the hose is 1.2 cm, so its cross-sectional area is:

A1 = πr1² = π(1.2 cm)² = 4.52 cm²

The radius of the nozzle is 0.28 cm, so its cross-sectional area is:

A2 = πr2² = π(0.28 cm)² = 0.246 cm²

We know that the water velocity in the hose is 2.0 m/s. To find the velocity through the nozzle, we can rearrange the continuity equation to solve for v2:

v2 = A1v1 / A2

Substituting the values we found above, we get:

v2 = (4.52 cm²)(2.0 m/s) / 0.246 cm²

v2 = 36.8 m/s

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When you look at a very dim star, you sometimes need to look to the side of the star and view it with peripheral vision. Why?

Answers

The reason you need to look to the side of a very dim star and view it with peripheral vision is because the rod cells, which are more sensitive to low light, are more abundant in the peripheral areas of the retina.

In our eyes, there are two types of photoreceptor cells: rod cells and cone cells.

Rod cells are responsible for vision in low light conditions, while cone cells are responsible for color vision and visual acuity in bright light. The rod cells are more abundant in the peripheral regions of the retina, while cone cells are concentrated in the central area called the fovea.
When you look directly at a dim star, the light falls on the fovea, where there are fewer rod cells. By looking slightly to the side of the star, you allow the light to fall on the peripheral retina, where there is a higher concentration of rod cells. This makes it easier for you to detect the dim light from the star with your peripheral vision.
In order to see a dim star more clearly, it is helpful to use peripheral vision by looking to the side of the star. This is because the rod cells, which are sensitive to low light, are more concentrated in the peripheral areas of the retina, allowing you to detect faint light more effectively.

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A series RLC circuit has a 190 kHz resonancefrequency.

What is the resonance frequency if the resistor value isdoubled?

What is the resonance frequency if thecapacitor value is doubled?

Answers

A series RLC circuit has a 190 kHz resonance frequency. Resistor Resonance frequency is same and capacitor resonance frequency is 380kHz.

In a series RLC circuit, the resonance frequency is the frequency at which the capacitive and inductive reactances cancel out, leaving only the resistance. It can be calculated using the formula:
[tex]f=\frac{1}{2\pi \sqrt{LC} }[/tex]
Where f is the resonance frequency, L is the inductance, and C is the capacitance.
Now, let's answer the questions:
1. If the resistor value is doubled, the resonance frequency of the circuit will not change. This is because the resistor does not affect the capacitance or inductance of the circuit, which are the factors that determine the resonance frequency.
2. If the capacitance value is doubled, the resonance frequency of the circuit will decrease. This is because the capacitance is in the denominator of the formula for resonance frequency, which means that increasing the capacitance will decrease the resonance frequency. The new resonance frequency can be calculated using the same formula as before, but with the new capacitance value:
[tex]f=\frac{1}{2\pi \sqrt{L(2C)} }[/tex]
Where 2C is the new capacitance value.

So F = 380kHz

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Determine the rate of heat transferred from the hot surface through each fin and the fin effectiveness. Is the use of fins justified? Why?

Answers

Heat transfer rate through fins and fin effectiveness must be determined to justify their use in a system.

To determine the rate of heat transferred from a hot surface through each fin, it is necessary to consider the material properties of the fin, its geometry, and the flow characteristics of the medium in which it operates.

Additionally, the fin effectiveness must be evaluated to determine whether the use of fins is justified.

Fin effectiveness is a measure of how well a fin increases the heat transfer rate, and is influenced by factors such as the fin thickness, surface area, and spacing.

If the fin effectiveness is high enough, it justifies the use of fins as they increase the heat transfer rate and improve the system's efficiency.

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An electromagnet is a coil of wire with a current running through it. This creates an electromagnetic field. An additional magnet and its poles interact with the electromagnet, causing an electromagnetic motor to turn. What are some ways you could make an electromagnetic motor stronger, and how could you apply these principles to everyday life

Answers

i) An electromagnetic motor can be made stronger by focusing on three key aspects: increasing the current, using more wire turns in the coil, and employing a better core material.

ii) These principles can be applied in various ways. For instance, electric vehicles and public transportation systems benefit from stronger electromagnetic motors, as they provide improved efficiency and torque.


Firstly, increasing the current running through the wire will amplify the strength of the electromagnetic field. This can be achieved by utilizing a higher voltage power source or reducing the resistance in the circuit.

Secondly, incorporating more wire turns in the coil can enhance the electromagnetic field generated by the electromagnet. The additional turns strengthen the field, which in turn increases the motor's overall power.

Lastly, using a core material with high magnetic permeability, such as soft iron or ferrite, will help concentrate the magnetic field and boost the motor's effectiveness. The core material must be easily magnetized and demagnetized, allowing the electromagnet to rapidly switch poles as needed for optimal performance.

In the medical field, magnetic resonance imaging (MRI) machines use powerful electromagnets to generate detailed images of the body, which aids in diagnosis and treatment. Furthermore, enhanced electromagnetic motors in industrial machinery can lead to increased productivity and reduced energy consumption.

By optimizing these factors, we can create stronger electromagnetic motors and harness their capabilities to improve multiple aspects of our daily lives.

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Light of wavelength 687 nm is incident on a single slit 0.75 mm wide. At what distance from the slit should a screen be placed if the second dark fringe in the diffraction pattern is to be 1.7 mm from the center of the screen

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The screen should be placed about 1.54 m from the slit to observe the second dark fringe at a distance of 1.7 mm from the center of the screen.

[tex]y_n[/tex] = (n λ L) / w

Plugging in the values, we get:

1.7 mm = (2)(687 nm)(L) / 0.75 mm

Solving for L, we get:

L = (1.7 mm)(0.75 mm) / (2)(687 nm)

L ≈ 1.54 m

A screen is a surface that displays visual information, usually in electronic form, for the purpose of communication, entertainment, or information. Screens come in various sizes and types, including LCD, LED, OLED, and CRT. They are commonly used in electronic devices such as televisions, computers, smartphones, tablets, and digital signage.

Screens can display a wide range of content, including text, images, videos, and interactive applications. They allow users to interact with information through touch, gestures, or input devices such as a keyboard or mouse. Screens have revolutionized the way we consume and access information, enabling us to communicate, learn, work, and entertain ourselves in ways that were not possible before.

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Hubble's law says that Group of answer choices more massive galaxies rotate faster the more distant a galaxy is, the faster it appears to be receding from us. the larger a galaxy is, the faster is receding from us.

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In Hubble's Law demonstrates that as the distance between a galaxy and us increases, the speed at which it appears to recede also increases. This observation supports the idea of an expanding universe, which is a key aspect of the current understanding of the cosmos.

Hubble's Law states that the more distant a galaxy is, the faster it appears to be receding from us. This observation is based on the redshift of light emitted by distant galaxies, which is the stretching of the wavelength of light towards the red end of the spectrum as the galaxy moves away from us. The relationship between the recessional velocity (how fast a galaxy is moving away) and its distance can be described by the equation:
Recessional velocity = Hubble constant × Distance
The Hubble constant (H0) is a value that represents the rate of expansion of the universe, measured in kilometers per second per megaparsec (km/s/Mpc).
In Hubble's Law demonstrates that as the distance between a galaxy and us increases, the speed at which it appears to recede also increases. This observation supports the idea of an expanding universe, which is a key aspect of the current understanding of the cosmos.

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Explain why in both parts of the experiment the leaf of the electroscope goes back to its original position after the rod is removed.

Answers

In an electroscope, the leaf is initially deflected when a charged object (such as a rod) is brought close to it. This happens because the charges on the rod induce opposite charges in the leaf, causing it to be attracted to the rod and move away from its original position.


In the experiment involving an electroscope and a rod, the electroscope's leaf goes back to its original position after the rod is removed due to the following reasons:

1. When the charged rod is brought near the electroscope, it induces an opposite charge on the nearest part of the electroscope, causing the electroscope's leaf to repel away from the metal stem.

2. Once the rod is removed, the charges in the electroscope redistribute themselves, returning to a balanced state. This causes the leaf to go back to its original position since there is no longer any net charge to cause repulsion.

In both parts of the experiment, the leaf returns to its original position after the rod is removed because the removal of the rod eliminates the charge imbalance that initially caused the leaf to move.

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What value of inductance should be used in series with a capacitor of 0.9 pF to form an oscillating circuit that will radiate a wavelength of 7.9 m

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The value of inductance that should be used in series with a capacitor of 0.9 pF to form an oscillating circuit that will radiate a wavelength of 7.9 m is 1.26 x 10⁻⁷ H.

We can use the formula for the resonant frequency of an LC circuit to calculate the inductance required to form an oscillating circuit that will radiate a wavelength of 7.9 m. The resonant frequency of an LC circuit is given by:

f = 1 / (2π√(LC))

where f is the frequency of oscillation, L is the inductance in henries, and C is the capacitance in farads.

The speed of light is given by:

c = fλ

where c is the speed of light (approximately 3 x [tex]10^8[/tex] m/s), f is the frequency of oscillation, and λ is the wavelength of radiation.

We want the oscillating circuit to radiate a wavelength of 7.9 m, so we can write:

f = c / λ = (3 x [tex]10^8[/tex]m/s) / (7.9 m) = 3.80 x [tex]10^8[/tex] Hz

We are given that the capacitance is 0.9 pF, or 9 x 10^-13 F. Substituting these values into the equation for resonant frequency, we get:

3.80 x[tex]10^7[/tex] Hz = 1 / (2π√(L (9 x [tex]10^-13[/tex]F)))

Solving for L, we get:

L = 1 / (4π²(3.80 x 10⁷ Hz)²(9 x 10⁻¹³ F)) = 1.26 x 10⁻⁷ H

Therefore, the value of inductance that should be used in series with a capacitor of 0.9 pF to form an oscillating circuit that will radiate a wavelength of 7.9 m is 1.26 x 10⁻⁷ H.

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