what is the frequency of a photon if the energy is 7.82 × 10⁻¹⁹ j? (h = 6.626 × 10⁻³⁴ j • s)

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Answer 1

The frequency of a photon if the energy is 7.82 × 10⁻¹⁹  and h = 6.626 × 10⁻³⁴ J • s is 1.18 × 10¹⁵ Hz.

To find the frequency of a photon with energy of 7.82 × 10⁻¹⁹ J, we can use the equation E = hf, where E is the energy of the photon, h is Planck's constant (6.626 × 10⁻³⁴ J • s), and f is the frequency of the photon.

Rearranging the equation, we get f = E/h. Plugging in the given values, we get:

f = 7.82 × 10⁻¹⁹ J / 6.626 × 10⁻³⁴ J • s

Simplifying the expression, we get:

f = 1.18 × 10¹⁵ Hz

Therefore, the frequency of the photon is 1.18 × 10¹⁵ Hz.

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a student must conduct two experiments so that the inertial mass and gravitational mass of the same object can be determined. in the experiment to find the object's gravitational mass, the student ties one end of a string around the object with the other end tied to a spring scale so that the object can vertically hang at rest. in the experiment to find the object's inertial mass, the student uses a spring scale to pull the object, starting from rest, across a horizontal surface with a constant applied force such that frictional forces are considered to be negligible. in addition to the spring scale, the student has access to other measuring devices commonly found in a science laboratory. which of the following lists the essential measuring devices the student can use to collect the data necessary to find the object's gravitational and inertial mass?

Answers

The essential measuring devices the student can use to collect the data necessary to find the object's gravitational and inertial mass are a meterstick, timer, motion detector, mass balance, and protractor.

The meterstick and timer are required for both experiments to measure distance and time, respectively.

The motion detector is necessary for the inertial mass experiment to measure the acceleration and velocity of the object, while the mass balance is required for the gravitational mass experiment to measure the weight of the object.

Finally, the protractor is necessary to measure the angle between the spring scale and the object during the gravitational mass experiment. Therefore, the correct option is: meterstick, timer, motion detector, mass balance, and protractor

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Full Question: A student must conduct two experiments so that the inertial mass and gravitational mass of the same object can be determined. in the experiment to find the object's gravitational mass, the student ties one end of a string around the object with the other end tied to a spring scale so that the object can vertically hang at rest. in the experiment to find the object's inertial mass, the student uses a spring scale to pull the object, starting from rest, across a horizontal surface with a constant applied force such that frictional forces are considered to be negligible. in addition to the spring scale, the student has access to other measuring devices commonly found in a science laboratory. which of the following lists the essential measuring devices the student can use to collect the data necessary to find the object's gravitational and inertial mass?meterstick and timer

meterstick, timer, and motion directormeterstick, timer, motion director, and mass balancemeterstick, timer, motion detector, mass balance, and protractor

Spring loaded trolleys have been constructed with crumple zones. What would be the purpose of these crumple zones

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The purpose of crumple zones in spring-loaded trolleys or vehicles, also known as energy-absorbing zones, is to enhance occupant safety during a collision. Crumple zones are strategically designed sections of the vehicle that are engineered to deform or crumple upon impact.

Here are the main purposes of crumple zones:

1. Energy Absorption: Crumple zones are specifically designed to absorb and dissipate the kinetic energy generated during a collision. By deforming and crumpling, they help to slow down the deceleration experienced by the occupants of the vehicle, reducing the impact forces transferred to them.

2. Vehicle Structural Integrity: Crumple zones play a crucial role in preserving the structural integrity of the passenger compartment. By absorbing the impact energy, they help to minimize the damage to the cabin area, which is the space where occupants are seated. This protective function helps to maintain the survival space and protects the occupants from intrusion or serious injuries.

3. Occupant Protection: By extending the collision duration through controlled deformation, crumple zones help to mitigate the forces exerted on the occupants. Slowing down the deceleration allows for a more gradual and controlled transfer of energy, reducing the risk of severe injuries, such as whiplash, head trauma, or internal organ damage.

4. Redistribution of Forces: Crumple zones are designed to redirect and distribute the forces of impact away from the occupant compartment. They help to steer the impact forces towards less critical areas of the vehicle structure, such as the front or rear ends, where the energy can be absorbed and dissipated more effectively.

Overall, the inclusion of crumple zones in spring-loaded trolleys or vehicles aims to improve occupant safety by reducing the severity of collisions and minimizing the risk of injuries. These zones are an essential part of modern vehicle safety design.

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usan, driving north at 61 mph, and Shawn, driving east at 46 mph, are approaching an intersection. What is Shawn's speed relative to Susan's reference frame? Express your answer to two significant figures and include the appropriate units

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To determine Shawn's speed relative to Susan's reference frame, we need to consider the velocities as vectors and calculate the magnitude of their vector difference.

Susan's velocity is 61 mph to the north, and Shawn's velocity is 46 mph to the east. Since they are approaching each other at right angles, we can use the Pythagorean theorem to find the magnitude of the resulting velocity. Using the Pythagorean theorem:
Relative velocity = √((Susan's velocity)^2 + (Shawn's velocity)^2)
Relative velocity = √((61 mph)^2 + (46 mph)^2)
Relative velocity ≈ √(3721 mph^2 + 2116 mph^2)
Relative velocity ≈ √(5837 mph^2)
Relative velocity ≈ 76.4 mph
Therefore, Shawn's speed relative to Susan's reference frame is approximately 76.4 mph.

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In a two slit interference pattern, what is the ratio of slit separation to slit width if there are 17 bright fringes within the central diffraction envelop and the diffraction minima coincide with two-slit interference maxima?

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In a two-slit interference pattern, the ratio of slit separation to slit width can be calculated using the formula dsinθ = mλ, where d is the slit separation, θ is the angle between the central axis and the fringe, m is the order of the fringe, and λ is the wavelength of light.

Given that there are 17 bright fringes within the central diffraction envelope, we can assume that the central fringe is the zeroth order and the 17th fringe is the 8th order. Therefore, m = 8.

We are also told that the diffraction minima coincide with the two-slit interference maxima. This occurs when the path difference between the two slits is equal to an integer multiple of the wavelength, which happens at the minima. At the maxima, the path difference is equal to an odd multiple of half the wavelength.

Since there are 17 bright fringes within the central diffraction envelope, there are 16 dark fringes. This means that the two-slit interference maxima occur at the positions of the 8th and 9th dark fringes. Therefore, the path difference between the two slits is equal to 8.5 times the wavelength.

Substituting the values into the formula, we get d/w = 8.5/sinθ. We can use the fact that the first minimum occurs at θ = sin⁻¹(λ/d) to find d/w.

Therefore, d/w = 8.5/sin(sin⁻¹(λ/d)) = 8.5/(λ/d) = 8.5d/λ.

In conclusion, the ratio of slit separation to slit width is 8.5d/λ if there are 17 bright fringes within the central diffraction envelope and the diffraction minima coincide with two-slit interference maxima.

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a 4000 kg meteorite falls toward the earth what is the magnitude of the earth's acceleration just before impact? the earth's mass is 5.98 × 10 24 kg .

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To calculate the magnitude of the Earth's acceleration just before the impact of a falling meteorite, we can use Newton's law of universal gravitation: F = G * (m1 * m2) / r^2 where F is the gravitational force between two objects, G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between their centers.

In this case, the Earth's mass (m1) is given as 5.98 × 10^24 kg, and the meteorite's mass (m2) is given as 4000 kg. We need to find the acceleration, which is the force acting on the meteorite divided by its mass. Rearranging the formula, we have:
F = m2 * a
Solving for F, we get:
F = G * (m1 * m2) / r^2
Now we can substitute the given values into the formula:
G = 6.67430 × 10^-11 m^3/kg/s^2 (gravitational constant)
m1 = 5.98 × 10^24 kg (mass of the Earth)
m2 = 4000 kg (mass of the meteorite)
r = radius of the Earth (assumed to be constant)
To find the radius of the Earth, we can use the formula for the acceleration due to gravity on the surface of the Earth:
g = G * m1 / r^2
Solving for r, we have:
r = sqrt(G * m1 / g)
Substituting the values into the formula, we can calculate the radius of the Earth. Finally, using the calculated radius, we can substitute the values of G, m1, and m2 into the formula for the gravitational force F, and then divide by the mass of the meteorite (m2) to find the acceleration (a). Therefore, the magnitude of the Earth's acceleration just before impact can be determined by calculating the gravitational force and dividing it by the mass of the meteorite.

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if 2.5 liters of oxygen gas at 20.0 Celsius expands in volume to 7.5 Liters constant pressure, what is the new kelvin temperature of oxygen? A. 293 K B. 60 K C. 879 K D.732K E. 98 K

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If 2.5 liters of oxygen gas at 20.0 Celsius expands in volume to 7.5 Liters constant pressure, then 879 K is the new kelvin temperature of oxygen.

Hence, the correct option is C.

We can use the combined gas law to solve for the final temperature. The combined gas law states that

(P1V1)/T1 = (P2V2)/T2

Where P is pressure, V is volume, and T is temperature, and the subscripts 1 and 2 refer to the initial and final conditions, respectively.

We are given the initial volume V1 = 2.5 L, the final volume V2 = 7.5 L, the initial temperature T1 = 20.0 Celsius = 293 K, and the pressure is assumed to be constant. We can solve for the final temperature T2 as follows

(P1V1)/T1 = (P2V2)/T2

T2 = (P2V2/T1) * (P1V1)

Since the pressure is constant, we can simplify to

T2 = T1 * (V2/V1)

Plugging in the values gives

T2 = 293 K * (7.5 L / 2.5 L) = 879 K

Hence, 879 K is the new kelvin temperature of oxygen.

Hence, the correct option is C.

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what is ε/kbt at room temperature for the kinetic energy storage mode for nitrogen gas in a cubic container whose sides have length l = 20 cm?

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According to the given information the correct answer is 5.36 x 10^-3 m^-3.

The value of ε/kbt at room temperature for the kinetic energy storage mode of nitrogen gas in a cubic container with sides of length 20 cm can be calculated using the following equation:

ε/kbt = 3/2 * (kB*T)/(ε/V)

where ε is the energy of the particle in the container, kbt is the Boltzmann constant times the temperature of the gas, kB is the Boltzmann constant, T is the temperature in Kelvin, and V is the volume of the container.

At room temperature (25°C or 298.15 K), the kinetic energy storage mode for nitrogen gas can be approximated as an ideal gas with ε = 3/2 kBT, where kBT = (1.38 x 10^-23 J/K) * (298.15 K) = 4.11 x 10^-21 J.

Assuming that the cubic container is completely filled with nitrogen gas, the volume of the container would be V = l^3 = (20 cm)^3 = 8,000 cm^3 = 8 x 10^-3 m^3.

Substituting these values into the equation for ε/kbt, we get:

ε/kbt = 3/2 * (kB*T)/(ε/V) = 3/2 * (1.38 x 10^-23 J/K * 298.15 K)/(3/2 * 4.11 x 10^-21 J/(8 x 10^-3 m^3))

Simplifying this expression, we get:

ε/kbt = 5.36 x 10^-3 m^-3

Therefore, the value of ε/kbt at room temperature for the kinetic energy storage mode of nitrogen gas in a cubic container with sides of length 20 cm is approximately 5.36 x 10^-3 m^-3.

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a certain rifle bullet has a mass of 5.25 g.5.25 g. calculate the de broglie wavelength of the bullet traveling at 16251625 miles per hour. consult the table of physical constants as needed.

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To calculate the de Broglie wavelength of the rifle bullet, we need to use the de Broglie equation which relates the wavelength of a particle to its momentum. The equation is:

λ = h / p

where λ is the de Broglie wavelength, h is the Planck constant (6.626 x 10^-34 J s), and p is the momentum of the particle.

First, we need to calculate the momentum of the rifle bullet. We can use the equation:

p = m*v

where p is the momentum, m is the mass of the bullet (5.25 g or 0.00525 kg), and v is the velocity of the bullet (1625 miles per hour or 725.44 m/s).

p = 0.00525 kg * 725.44 m/s
p = 3.8088 kg m/s

Now we can plug this value into the de Broglie equation to find the wavelength:

λ = 6.626 x 10^-34 J s / 3.8088 kg m/s
λ = 1.738 x 10^-34 m

Therefore, the de Broglie wavelength of the rifle bullet traveling at 1625 miles per hour is 1.738 x 10^-34 meters. It is important to note that this is an extremely small wavelength due to the high velocity and relatively large mass of the bullet.

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A 2 km long optical fiber uses a fiber core with n_f = 1.6 and a cladding with n_c = 1.57. Compute the maximum data rate f_p The operating frequency is 100 THz. a. 2.453 Mbits/s b. 2.543 Gbit/s c. 1.272 Mbit/s d. 5.086 Gbit/s

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The maximum data rate of the optical fiber is 2.543 Gbit/s. So, the correct answer is B).

The maximum data rate f_p for an optical fiber can be calculated using the formula:

f_p = (2/3) * (c/n_f) * (log_2(N))² * B

where c is the speed of light in vacuum, N is the number of levels, and B is the bandwidth.

To calculate N, we use the equation:

N = (V²)/2

where V is the normalized frequency, given by

V = 2pi(a/λ)*(n_f² - n_c²[tex])^{0.5}[/tex]

where a is the radius of the fiber core, λ is the wavelength of the light, and n_f and n_c are the refractive indices of the core and cladding, respectively.

Substituting the given values, we get

a = 2 km / 2 = 1 km

λ = c/f = 310⁸ m/s / 10010¹² Hz = 310⁻⁶ m

V = 2pi*(1 km)/(310⁻⁶ m)(1.6² - 1.57²[tex])^{0.5}[/tex] = 52.44

Using V, we can calculate N

N = (V²)/2 = (52.44²)/2 = 1373.99 ≈ 1374

Substituting the values of c, n_f, log_2(N), and B, we get

f_p = (2/3) * (310⁸ m/s/1.6) * (log_2(1374))² * 10010¹² Hz = 2.543 Gbit/s

Therefore, the answer is (b) 2.543 Gbit/s.

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In which scenario would airbag deployment not be beneficial?
in a head-on collision
when a child is sitting in the back seat
when colliding with a stationary object
when a child is sitting in the front seat

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Airbag deployment may not be beneficial in the scenario where a child is sitting in the front seat. This is because airbags are designed to protect adult-sized individuals.

May actually cause harm to a child due to the force of deployment. In fact, the American Academy of Pediatrics recommends that children under the age of 13 should always ride in the back seat to reduce the risk of injury from airbags. Additionally, in the scenario of colliding with a stationary object, airbags may not be as effective as they are designed to work in conjunction with seat belts and other safety features in a moving vehicle.

It is important to always follow proper safety guidelines and use age-appropriate car seats and seat belts to ensure the most effective protection in the event of an accident. Programmes, modules, updates, and patches are sent from developers to users via deployment. The methods used by developers to create, test, and install new code will have an impact on how quickly a product can adapt to changes in customer preferences or requirements, as well as how well each update works.

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Suppose rock is tossed upwards with an initial velocity of 80 ftisec from an initial height of 150 ft The position function can be written as quadratic function in the fomm of: s(t) =at^2 + bt + c Find a, b and c. Enter an integer value for each a = __________________, b = __________________, c = __________________

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Rock is tossed upwards with an initial velocity of 80 ft/sec from an initial height of 150 ft . The values of a, b, and c are: a = 8, b = 100, c = -100.

To find the values of a, b, and c, we need to use the given information and the position function s(t) = at² + bt + c.

First, let's find the values of a and b. We know that the rock was tossed upwards with an initial velocity of 80 ft/sec, which means that the initial velocity component in the vertical direction is 80 ft/sec. Since we are assuming that the only force acting on the rock is gravity, we can use the kinematic equation:

v = u + at

where v is the final velocity, u is the initial velocity, a is the acceleration due to gravity (-32 ft/sec²), and t is the time elapsed. At the highest point of the trajectory, the final velocity is 0 ft/sec (the rock momentarily stops before falling back down), so we can set v = 0 and solve for t:

0 = 80 - 32t
t = 2.5 sec

Now we can use this value of t to find the height of the rock at the highest point:

s = ut + (1/2)at²
s = 80(2.5) + (1/2)(-32)(2.5)²
s = 100 ft

Therefore, the highest point of the trajectory is 150 + 100 = 250 ft above the ground.

Since the rock starts at an initial height of 150 ft and reaches a maximum height of 250 ft, we know that the vertical displacement of the rock is 100 ft. We also know that the time taken for the rock to reach its highest point is 2.5 sec. Using these values, we can find the value of a:

s = ut + (1/2)at²
100 = 0(2.5) + (1/2)a(2.5)²
a = 8 ft/sec²

Now that we have found the value of a, we can use it to find the value of b:

b = u + at
b = 80 + 8(2.5)
b = 100 ft/sec

Finally, we can use the values of a, b, and the coordinates of the vertex (2.5, 250) to find the value of c:

s = at² + bt + c
250 = a(2.5)² + b(2.5) + c
c = 150 - a(2.5)² - b(2.5)
c = 150 - 50 - 200
c = -100 ft

Therefore, the values of a, b, and c are:

a = 8, b = 100, c = -100

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if the initial speeds of the balls were v1i = 2.0 m/s and v2i = 1.0 m/s, what would be the final speed and direction of ball two, v2f, in meters per second?

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The final speed of ball two is 1.0 m/s, and its direction is the same as its initial direction.  

To find the final speed and direction of ball two, we need to use the equations for conservation of linear momentum. The momentum of the system before the collision is zero, so we can write:

m1v1i + m2v2i = 0

where m1 and m2 are the masses of the two balls, v1i and v2i are their initial velocities, and v2f is the final velocity of ball two.

We also know that the momentum of ball one after the collision is equal to the momentum of ball two before the collision. This means:

m1v1f + m2v2f = m2v2i

We can solve for v2f by substituting the given initial velocities and masses into the first equation and solving for v2f. We get:

2.0 m/s * 2.0 m/s + 1.0 m/s * 2.0 m/s = m2v2i

2.0 m/s * 2.0 m/s + 1.0 m/s * 2.0 m/s = 2.0 * 1.0 m/s

[tex]1.0 m/s^2[/tex] + 2.0 m/s^2 = 2.0 * 1.0 m/s

[tex]1.0 m/s^2[/tex]= 2.0 m/s

1.0 m/s = 2.0 m/s + 1.0 m/s

v2f = 1.0 m/s

Therefore, the final speed of ball two is 1.0 m/s, and its direction is the same as its initial direction.  

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why are asteroids closer to the sun made up or carbon and hydrogen when terrestrial planets are made up of silica

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The composition of asteroids and terrestrial planets is influenced by several factors, including their distance from the Sun, the temperature at which they formed, and the materials available in their region of the solar system.

Asteroids are small, rocky objects that orbit the Sun. They are remnants from the early solar system and are primarily found in the asteroid belt, which lies between the orbits of Mars and Jupiter. Asteroids come in a range of sizes, from tiny particles to large bodies over 100 kilometers in diameter.

Some asteroids are rich in valuable minerals like iron, nickel, and platinum, making them potential targets for mining operations in the future. Other asteroids are of interest to scientists because they may contain clues about the origins of the solar system and the conditions that led to the formation of planets. Occasionally, asteroids can collide with Earth, posing a potential threat to life on our planet. Large impacts in the past have caused significant damage and extinction events, such as the one that is believed to have led to the demise of the dinosaurs.

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a laser emits light of frequency 4.47 * 1014 hz. what is the wavelength of the ligh in nm? what color is that light?

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0.22*10^-5nm is the wavelength of the light in nm if a laser emits light of frequency 4.47 * 1014 hz .

Define wavelength

A waveform signal that is carried in space or down a wire has a wavelength, which is the separation between two identical places (adjacent crests) in the consecutive cycles. This length is typically defined in wireless systems in meters (m), centimeters (cm), or millimeters (mm).

Particles in the medium fluctuate about their mean location as a wave passes across it. The frequency of the wave is defined as the quantity of oscillations per second. The SI symbol for frequency is Hertz (Hz).  The distance a wave travels in a unit of time is measured by its wave velocity. It measures how quickly a particle disturbance like a crest or trough or compression or rarefaction spreads through a medium.

wavelength is 1/n

n is frequency

wavelength will be 1/4.47 * 10^14 i.e. 0.22*10^-5nm

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500 J of work are done on a system in a process that decreases the system's thermal energy by 200 J. How much heat energy is transfered to or from the system

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300 Joules of heat energy is transferred to the system as heat.

In this situation, we have a system that experiences work being done on it, as well as a change in its thermal energy. To determine the heat energy transferred, we will use the first law of thermodynamics, which states that the change in internal energy (∆U) of a system is equal to the heat (Q) added to the system minus the work (W) done by the system: ∆U = Q - W.
First, let's identify the given values:
Work done on the system (W) = 500 J
Decrease in thermal energy (∆U) = -200 J (It is negative since there's a decrease)
Since the work is done on the system, we need to reverse the sign for W in our equation: ∆U = Q - (-W). Now we can plug in the given values:
-200 J = Q - (-500 J)
To solve for Q (heat energy transferred), we can add 500 J to both sides of the equation:
-200 J + 500 J = Q
This simplifies to:
300 J = Q
So, 300 Joules of heat energy is transferred to the system as heat.

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if an fm radio station is emitting 100000 w in its 83.0-mhz radio wave, how many photons is it emitting each second?

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The number of photons emitted by an FM radio station per second can be calculated using the equation E = hf, where E is the energy of each photon, h is Planck's constant, and f is the frequency of the radio wave. First, we need to convert the frequency of the radio wave from MHz to Hz by multiplying it by 10^6. Thus, the frequency becomes 83.0 × 10^6 Hz. Next, we can calculate the energy of each photon using Planck's constant (6.626 × 10^-34 J.s).

E = hf = (6.626 × 10^-34 J.s) × (83.0 × 10^6 Hz) = 5.50 × 10^-26 J

Now, we can calculate the number of photons emitted per second using the power emitted by the FM radio station (100000 W) and the energy of each photon (5.50 × 10^-26 J).

Number of photons emitted per second = Power emitted / Energy of each photon = 100000 W / 5.50 × 10^-26 J = 1.82 × 10^32 photons per second.

Therefore, an FM radio station emitting 100000 W in its 83.0-MHz radio wave is emitting approximately 1.82 × 10^32 photons per second.

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a merry-go-round has a mass of 1460 kg and a radius of 7.00 m . part a how much net work is required to accelerate it from rest to a rotation rate of 1.00 revolution per 7.30 s ? assume it is a solid cylinder.

Answers

4230 J of net work is required to accelerate the merry-go-round from rest to a rotation rate of 1.00 revolution per 7.30 s, assuming it is a solid cylinder.

To determine the net work required to accelerate the merry-go-round from rest to a rotation rate of 1.00 revolution per 7.30 s, we need to use the formula for rotational kinetic energy:
KE = (\frac{1}{2}) I ω^2
Where KE is the kinetic energy, I is the moment of inertia (which for a solid cylinder is (1/2) MR^2), and ω is the angular velocity (which for 1 revolution per 7.30 s is 2π/7.30).
First, we can calculate the moment of inertia:
I = (\frac{1}{2}) MR^2 = (\frac{1}{2})(1460 kg)(7.00 m)^2 = 35915 kg m^2
Next, we can calculate the final rotational kinetic energy:
KE_final = (\frac{1}{2}) I ω^2 = (\frac{1}{2})(35915 kg m^2)(2π/7.30)^2 = 4230 J
Since the merry-go-round is starting from rest, the initial rotational kinetic energy is 0. Therefore, the net work required to accelerate it to this final kinetic energy is just equal to the final kinetic energy:
Net work = KE_final = 4230 J
In summary, 4230 J of net work is required to accelerate the merry-go-round from rest to a rotation rate of 1.00 revolution per 7.30 s, assuming it is a solid cylinder.

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find the force exerted on a positive charge of 2.80 μc in a uniform electric field of magnitude 5.30 x 104 n/c.

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The force exerted on a positive charge of 2.80 μc in a uniform electric field of magnitude 5.30 x 104 n/c can be calculated using the equation F = qE, where F is the force, q is the charge, and E is the electric field. Plugging in the values, we get:

F = (2.80 μc)(5.30 x 104 n/c) = 1.49 x 10-4 N

Therefore, the force exerted on the positive charge is 1.49 x 10-4 N.

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Suppose you fell into an accretion disk that swept you into a supermassive black hole. On your way down, the disk radiates 10 % of your mass-energy, E=mc2.

1) Assume that your mass is 54. 5 kg. Calculate how much radiative energy will be produced by the accretion disk as a result of your fall into the black hole.

Express your answer using two significant figures.

E=. J

2) Calculate approximately how long a 100-watt light bulb would have to burn to radiate this same amount of energy.

Express your answer using two significant figures.

t=. Yr

Answers

The mass of 54.5 kg fell into the accretion disk that swept you into a supermassive black hole with energy E = 4.9×10¹⁷J and the time to radiate energy is 1.6×10⁸ yr.

The mass-energy equivalence is defined as the energy is directly proportional to the mass and c is the speed of light that remains constant. The mass-energy relation is given, Einstein and it is called Einstein's mass-energy relation. Energy is the ability to do work and the unit of energy is Joule. Energy can neither be created nor destroyed. Power equals the ratio of energy and time.

From the given,

mass = 54.5Kg

c = 3×10⁸

E = mc² = 54.5×3×10⁸×3×10⁸

 = 4.9×10¹⁷ J

Thus, the energy is 4.9×10¹⁷ J.

Power = 100 watt

Energy = 4.9×10¹⁷ J

time=?

Power = energy/time

time = energy/power

     = 4.9×10¹⁷ J/100

t=1.6×10⁸ yr.

The time in which the 100-watt light bulb is 1.6×10⁸ yr.

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11. Calculate the resultant force acting on the objects below:
a)
12 N
6 N

Answers

Answer:I would say the answer is either 6 N or 18 N

Explanation: SINCE YOUR  QUESTION ISN'T SPECIFIC I can't answer it accurately mind providing a diagram or picture of the question or the direction of the forces

when a transition metal atom formas an ion which electrons are lost first

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In general, transition metals lose their valence electrons first when forming ions. However, the specific electrons lost can depend on the particular transition metal and its electronic configuration.

Transition metals are elements in the d-block of the periodic table and have partially filled d orbitals. When forming ions, they typically lose their valence electrons, which are the electrons in the outermost shell. These electrons are lost first because they have the highest energy and are therefore the easiest to remove.

However, the specific electrons that are lost can depend on the particular transition metal and its electronic configuration. For example, in the case of copper (Cu), the electron configuration is [Ar] 3d10 4s1, and it is more energetically favorable for the 4s electron to be lost before the 3d electrons.

Overall, the order in which electrons are lost during ion formation for transition metals depends on the electronic configuration and energy levels of the atoms involved.

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now replace the double slit slide with a diffraction grating (a slide with many slits). how does the pattern on the screen change with the diffraction grating compared to the double slit slide? do you have to bring the screen closer to the diffraction grating in order to see the pattern? if you had to make accurate measurements of the spacing between bright spots on the screen, would you rather use a double slit or a diffraction grating? why

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When a diffraction grating is substituted for the double slit slide, the resulting pattern on the screen will be different.

A diffraction grating is a device with many slits that diffracts light into its component colors, similar to a prism. When light passes through a diffraction grating, it is diffracted, or spread out, into many different directions. This diffraction produces a pattern of bright and dark bands on a screen placed behind the grating, similar to the pattern produced by a double slit.

However, the pattern produced by a diffraction grating is different from the pattern produced by a double slit. The diffraction pattern produced by a diffraction grating has bright and dark bands that are wider and further apart than the bands produced by a double slit. This is because the diffraction pattern produced by a diffraction grating is determined by the spacing of the slits in the grating and the wavelength of the light passing through it, whereas the pattern produced by a double slit is determined by the interference of the two slits.

To observe the pattern on the screen with a diffraction grating, the screen does not need to be brought closer to the grating. Instead, the grating is typically placed at a distance from the screen, and the screen is placed at a distance from the grating such that the bright and dark bands on the screen are clearly visible.

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if 37.18 ml of .116 m naoh are required to titrate a 0.168 g sample of the acid, what is the molar mass of your acid?

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To find the molar mass of the acid, we need to use the balanced chemical equation for the reaction between the acid and NaOH. However, since the chemical formula of the acid is not given, we cannot write the equation directly. Instead, we can use the information given in the problem to calculate the number of moles of NaOH used in the titration and use that to find the number of moles of the acid. Then we can calculate the molar mass of the acid using its mass and moles.

First, let's calculate the number of moles of NaOH used in the titration:

moles of NaOH = Molarity x Volume (in liters)

moles of NaOH = 0.116 mol/L x 0.03718 L

moles of NaOH = 0.00431 mol

Next, we can use the balanced chemical equation for the reaction between NaOH and the acid:

acid + NaOH → salt + water

Since NaOH is a strong base and the reaction is assumed to be complete, the number of moles of NaOH used is equal to the number of moles of acid in the sample:

moles of acid = 0.00431 mol

Finally, we can calculate the molar mass of the acid:

molar mass of acid = mass of acid / moles of acid

molar mass of acid = 0.168 g / 0.00431 mol

molar mass of acid = 39.0 g/mol

Therefore, the molar mass of the acid is 39.0 g/mol.

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if the temperature of a sample of water at 4°c is slightly increased, its volume

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If the temperature of a sample of water at 4°C is slightly increased, its volume will generally increase. However, water exhibits a unique behavior around 4°C that deviates from this general trend.

When water is cooled from higher temperatures, its volume decreases until it reaches approximately 4°C. At this point, water reaches its maximum density. However, as the temperature continues to decrease below 4°C, water expands and becomes less dense. This behavior is due to the arrangement of water molecules in a crystalline structure at lower temperatures.

Conversely, when the temperature of water at 4°C is increased, its volume generally increases as it follows the normal thermal expansion behavior. As water absorbs heat, the increased thermal energy causes the water molecules to move more vigorously, leading to an increase in the average distance between the molecules. This results in an expansion of the water's volume.

It's worth noting that this behavior is specific to water and does not apply to all substances. Most substances exhibit thermal expansion, where an increase in temperature leads to an increase in volume.

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Whenever a force vector is not coincident with an axis in your frame of reference, you must apply what factors to examine the components in your reference frame?

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When a force vector is not coincident with an axis in your frame of reference, you need to apply the principles of vector decomposition to analyze its components within your reference frame. Vector decomposition, also known as vector resolution, involves breaking a vector down into its constituent components along the coordinate axes.

In order to do this, you will use trigonometric functions such as sine, cosine, and tangent, depending on the angle between the force vector and the reference axis. For instance, if you know the magnitude of the force and the angle it makes with one of the coordinate axes, you can use the sine and cosine functions to determine the horizontal and vertical components of the force.

These components can then be treated separately to analyze their effects on the system. By examining the components, you can better understand how the force influences the motion or equilibrium of objects in the reference frame.

In summary, when a force vector is not coincident with an axis in your frame of reference, apply vector decomposition and use trigonometric functions to determine the components along the coordinate axes. This allows you to analyze the effects of the force on the system in your reference frame.

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what do you think you would observe if you did the same experiments with incoherent light at a single wavelength? what about if you used incoherent white light (i.e. light consisting of a spectrum of wavelengths)

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Incoherent light at a single wavelength would produce a diffraction pattern that is very similar to the diffraction pattern produced by coherent light of the same wavelength.

However, because the phases of the light waves are not correlated, the diffraction pattern would not be as sharp as that produced by coherent light. The intensity distribution would still show a central bright spot with alternating dark and bright fringes, but the fringes would not be as well defined as in the case of coherent light.

If incoherent white light were used instead of coherent light, the diffraction pattern would be much less distinct. The individual wavelengths of the white light would interfere with each other, producing a complex pattern of bright and dark spots that would be difficult to interpret.

The result would be a diffuse pattern that would not have the sharp fringes seen in the diffraction pattern produced by coherent light. This is because the waves from different parts of the spectrum would be out of phase with each other, leading to destructive interference and a decrease in overall intensity.

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Which one of the following scientists discovered the effect magnetic fields have on the energies of an atom? Group of answer choices: Curie Schrodinger Zeeman

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Pieter Zeeman is the scientist who discovered the effect magnetic fields have on the energies of an atom, known as the Zeeman effect.

The scientist who discovered the effect magnetic fields have on the energies of an atom is Pieter Zeeman. This phenomenon is known as the Zeeman effect. Here's a brief explanation:

1. Pieter Zeeman, a Dutch physicist, conducted experiments on the interaction between magnetic fields and atoms.
2. In 1896, he discovered that when a light source (like a gas discharge tube) is placed in a magnetic field, the spectral lines emitted by the light source split into multiple components.
3. This splitting occurs because the magnetic field affects the energy levels of the electrons within the atom, causing them to split into different energy levels.
4. The splitting of spectral lines in a magnetic field became known as the Zeeman effect.
5. This discovery contributed to the development of quantum mechanics and earned Zeeman a Nobel Prize in Physics in 1902, which he shared with Hendrik Lorentz.

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An aquarium of length L, width (front to back) W, and depth D is filled to the top with liquid of density rho. a. Find a n expression for the force of the liquid on the bottom of the aquarium

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The force of the liquid on the bottom of the aquarium is equal to the weight of the liquid directly above it. The weight of the liquid can be calculated by multiplying its mass by the acceleration due to gravity, g. The mass of the liquid can be found by multiplying its volume by its density.

The volume of the liquid in the aquarium is equal to the product of its length, width, and depth, or LWD. Therefore, the mass of the liquid is:

m = ρLWD

And the weight of the liquid is:

F = mg = ρLWDg

So the force of the liquid on the bottom of the aquarium is ρLWDg.

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A satellite 575 km above the earth's surface transmits sinusoidal electromagnetic waves of frequency 92.4 MHz uniformly in all directions, with a power of 25.0 kW. (a) What is the intensity of these waves as they reach a receiver at the surface of the earth directly below the satellite? (b) What are the amplitudes of the electric and magnetic fields at the receiver? (c) If the receiver has a totally absorbing panel measuring 15.0 cm by 40.0 cm oriented with its plane perpendicular to the direction the waves travel, what average force do these waves exert on the panel? Is this force large enough to cause significant effects?

Answers

a. The intensity of these waves as they reach a receiver at the surface of the earth directly below the satellite is 1.39 x 10^-12 W/m^2

b. The amplitudes of the electric and magnetic fields at the receiver are 1.40 x 10^-5 V/m and 3.73 x 10^-8 T

c. The force exerted by electromagnetic waves on a surface is 3.32 x 10^-11 N

(a) The intensity of electromagnetic waves decreases with distance according to the inverse square law, which states that the intensity is inversely proportional to the square of the distance. The distance between the satellite and the receiver is the sum of the radius of the Earth and the altitude of the satellite, which is:

d = 6,371 km + 575 km = 6,946 km

The intensity of the waves at the receiver is given by:

I = P/4πd^2

where P is the power of the waves. Substituting the given values, we get:

I = 25.0 kW / (4π(6,946 km)^2) = 1.39 x 10^-12 W/m^2

(b) The electric and magnetic fields of the waves can be related to the intensity by the equation:

I = 1/2 ε0 c E^2 = 1/2 μ0 c B^2

where ε0 and μ0 are the electric permittivity and magnetic permeability of free space, respectively, and c is the speed of light. Solving for E and B, we get:

E = sqrt(2I/ε0 c) = 1.40 x 10^-5 V/m

B = sqrt(2I/μ0 c) = 3.73 x 10^-8 T

(c) The force exerted by electromagnetic waves on a surface is given by the radiation pressure equation:

F = (2I/c) A

where A is the area of the surface and c is the speed of light. Substituting the given values, we get:

F = (2 x 1.39 x 10^-12 W/m^2 / 3.00 x 10^8 m/s) x (0.15 m x 0.40 m) = 3.32 x 10^-11 N

This force is very small and is unlikely to cause any significant effects on the absorbing panel.

Note: In the calculations, the wavelength of the waves is not needed, as the frequency is given and the waves are assumed to be sinusoidal.

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an original signal frequency is halved by a resistor and no other part of the wave was affected. determine the change in the amplitude of the signal

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Changing the frequency of a signal, without affecting other wave properties, does not directly impact the amplitude. The amplitude remains unchanged in this scenario.

In a signal, the amplitude represents the maximum displacement or intensity of the wave. It is unrelated to the frequency, which refers to the number of complete cycles of the wave that occur in a given time. Changing the frequency alone, while keeping other wave properties constant, such as the amplitude, does not cause any direct alteration to the amplitude.

In this case, if the original signal's frequency is halved by a resistor without affecting any other parts of the wave, the amplitude of the signal remains the same. The resistor only affects the frequency of the signal, causing it to be halved. The amplitude is determined by factors like the source of the signal or the properties of the medium through which it propagates and is not affected by the change in frequency. Therefore, the change in the frequency of the signal does not lead to any change in the amplitude.

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