Water flows steadily at a rate of 0.020f/s through the 0.75 -in-diameter galvanized iron pipe system shown below. The tee (branch flow) is threaded, the elbow or 90 ∘
smooth bend is threaded, and the reducer has a loss coefficient of 0.15 . The kinematic viscosity of water is 1.21(10) −5
f/s. Your boss suggests that friction losses in the straight pipe sections are negligible compared to losses in the threaded elbows and fittings of the system. Do you agree or disagree with your boss? Support your answer with appropriate calculations. What are the major and minor losses?

Answers

Answer 1

Water flows steadily at a rate of 0.020f/s through the 0.75 -in-diameter galvanized iron pipe system shown below. The tee (branch flow) is threaded, the elbow or 90 ∘ smooth bend is threaded, and the reducer has a loss coefficient of 0.15 . The kinematic viscosity of water is 1.21(10) −5 f/s. The major losses in the system are greater than the minor losses, and the boss's assumption that friction losses in the straight pipe sections are negligible compared to losses in the fittings is reasonable.

To determine whether friction losses in the straight pipe sections are negligible compared to losses in the fittings, we need to calculate the friction factor and the friction losses in the straight pipe sections and compare them to the losses in the fittings.

The Reynolds number for the flow can be calculated as

Re = (ρVD)/μ

Where ρ is the density of water, V is the velocity of water, D is the diameter of the pipe, and μ is the kinematic viscosity of water.

Substituting the given values, we get

Re = (1000 kg/[tex]m^{3}[/tex])(0.020 m/s)(0.01905 m)/(1.21 x [tex]10^{-5}[/tex] [tex]m^{2}[/tex]/s) = 3167.77

Since the flow is turbulent (Re > 4000), we can use the Colebrook equation to calculate the friction factor

1/[tex]\sqrt{f}[/tex] = -2.0log10((0.00015/3.7)(0.75/0.01905) + 2.51/(Re*[tex]\sqrt{f}[/tex] )

We can solve for f using an iterative numerical method, such as the Newton-Raphson method. For this problem, the solution is f = 0.0188.

The friction losses in the straight pipe sections can be calculated using the Darcy-Weisbach equation

hf = f(L/D)*([tex]V^{2}[/tex]/2g)

Where L is the length of the pipe section, D is the diameter of the pipe, and g is the acceleration due to gravity.

Assuming negligible losses in the straight pipe sections, we can set hf to zero and solve for the length of pipe required to have negligible losses

0 = f(L/D)*([tex]V^{2}[/tex]/2g)

L/D = 0

This means that any length of straight pipe will have negligible losses compared to the losses in the fittings.

The major losses in the system are due to the friction losses in the fittings, which can be calculated using the following equation

hf = K*([tex]V^{2}[/tex]/2g)

Where K is the loss coefficient of the fitting.

The minor losses in the system are due to changes in velocity and direction of flow, and can be calculated using the following equation

hf = K*([tex]V^{2}[/tex]/2g)

Where K is the loss coefficient of the minor loss.

For the given system, the major losses are due to the threaded tee and elbow, and can be calculated as

hftee = 1*([tex]V^{2}[/tex]/2g)

hfelbow = 1.5*([tex]V^{2}[/tex]/2g)

Where the loss coefficients for the threaded tee and elbow are assumed to be 1 and 1.5, respectively.

The minor losses are due to the smooth reducer and can be calculated as

hfreducer = 0.5*([tex]V^{2}[/tex]/2g)

Where the loss coefficient for the smooth reducer is assumed to be 0.5.

Therefore, the major losses in the system are greater than the minor losses, and the boss's assumption that friction losses in the straight pipe sections are negligible compared to losses in the fittings is reasonable.

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Related Questions

A certain ideal gas has a molar specific heat at constant pressure of 33.2 J/mol  K. Its molar specific heat at constant volume is closest to which of the following values? (R = 8.31J/mol  K) A) 24.9 J/mol  K B) 49.8 J/mol  K C) 41.9 J/mol  K D) 16.6 J/mol  K E) 25.1 J/mol  K

Answers

The relationship between the molar specific heat at constant pressure (Cp) and the molar specific heat at constant volume (Cv) for an ideal gas is Cp = Cv + R. Therefore, we can rearrange this equation to solve for Cv: Cv = Cp - R.

Using the given values, we have:

Cv = 33.2 J/mol  K - 8.31 J/mol  K
Cv = 24.9 J/mol  K

Therefore, the closest value for the molar specific heat at constant volume is A) 24.9 J/mol  K.

To find the molar specific heat at constant volume (Cv), we can use the relationship between molar specific heat at constant pressure (Cp) and the gas constant (R):

Cp = Cv + R

Given that Cp = 33.2 J/mol K and R = 8.31 J/mol K, we can solve for Cv:

Cv = Cp - R = 33.2 - 8.31 = 24.9 J/mol K

So, the closest value to the molar specific heat at constant volume is 24.9 J/mol K, which corresponds to option A) 24.9 J/mol K.

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what is the correct html for making a drop-down list?

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The correct HTML for creating a drop-down list is to use the `<select>` element along with the `<option>` elements. Here's an example:

[tex]```html < select > < option value="option1" > Option 1 < /option > < option value="option2" > Option 2 < /option > < option value="option3" > Option 3 < /option > < /select > ```[/tex]

In this example, the `<select>` element represents the drop-down list itself, and each `<option>` element represents an item within the list. The `value` attribute specifies the value associated with each option, while the content within the `<option>` tags represents the visible text for each item.

When a user interacts with the drop-down list, they can select one of the options. The selected option's value can then be retrieved using JavaScript or submitted as part of a form submission.

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Calculate the de Broglie wavelength of (a) a 0.998 keV electron (mass = 9.109 x 10-31 kg), (b) a 0.998 keV photon, and (c) a 0.998 keV neutron (mass = 1.675 x 10-27 kg). (a) Number Units (b) Number Units (c) Number Units

Answers

(a) The de Broglie wavelength of a 0.998 keV electron can be calculated using the formula λ = h / p, where λ is the wavelength, h is the Planck constant, and p is the momentum of the electron.

Plugging in the values, we get:

[tex]λ = h / p = h / √(2mE)[/tex]

where m is the mass of the electron, E is its energy, and h is the Planck constant.

Substituting the values, we get:

[tex]λ = 6.626 x 10^-34 J.s / √(2 x 9.109 x 10^-31 kg x 0.998 x 10^3 eV x 1.602 x 10^-19 J/eV)[/tex]

[tex]λ = 3.86 x 10^-11 m[/tex]

Therefore, the de Broglie wavelength of a 0.998 keV electron is 3.86 x 10^-11 meters.

(b) For a photon, the de Broglie wavelength can be calculated using the formula λ = h / p, where p is the momentum of the photon. Since photons have no rest mass, their momentum can be calculated using the formula p = E / c, where E is the energy of the photon and c is the speed of light.

Plugging in the values, we get:

[tex]λ = h / p = h / (E / c)[/tex]

[tex]λ = hc / E[/tex]

Substituting the values, we get:

[tex]λ = (6.626 x 10^-34 J.s x 3 x 10^8 m/s) / (0.998 x 10^3 eV x 1.602 x 10^-19 J/eV)[/tex]

λ = 2.48 x 10^-10 m

Therefore, the de Broglie wavelength of a 0.998 keV photon is 2.48 x 10^-10 meters.

(c) The de Broglie wavelength of a 0.998 keV neutron can be calculated using the same formula as for an electron: λ = h / p, where p is the momentum of the neutron. However, since the mass of the neutron is much larger than that of an electron, its de Broglie wavelength will be much smaller.

Plugging in the values, we get:

[tex]λ = h / p = h / √(2mE)[/tex]

Substituting the values, we get:

[tex]λ = 6.626 x 10^-34 J.s / √(2 x 1.675 x 10^-27 kg x 0.998 x 10^3 eV x 1.602 x 10^-19 J/eV)[/tex]

[tex]λ = 2.20 x 10^-12 m[/tex]

Therefore, the de Broglie wavelength of a 0.998 keV neutron is 2.20 x 10^-12 meters.

In summary, the de Broglie wavelength of a 0.998 keV electron is 3.86 x 10^-11 meters, the de Broglie wavelength of a 0.998 keV photon is 2.48 x 10^-10 meters, and the de Broglie wavelength of a 0.998 keV neutron is 2.20 x 10^-12 meters.

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A two lens combination consisting of a diverging Lens (#1) with a focal length of -20 cm and a converging Lens (#2) with a focal length of +30 cm is used to view the image of an object, 6 cm high, placed 30 cm in front of the first lens. The two lenses are separated by 40.0 cm. Which of the following characteristics does the final image have?

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The final image formed by the two-lens combination has the following characteristics: 1. Real image 2. Inverted 3. Image distance of 60 cm from the converging lens 4. Image height of 18 cm

The final image in a two-lens combination can be determined by first finding the image formed by the first lens (diverging lens) and then using that image as the object for the second lens (converging lens).
For the diverging lens (#1), with a focal length of -20 cm and object distance (p1) of 30 cm, we can find the image distance (q1) using the lens formula: 1/f1 = 1/p1 + 1/q1. Solving for q1, we get an image distance of -60 cm. The negative sign indicates that the image is virtual and on the same side as the object. The image height (h1) can be found using the magnification formula: h1/h0 = q1/p1, which gives us h1 = -12 cm (negative sign indicates an inverted image).
Now, we will treat the virtual image formed by lens #1 as the object for lens #2 (converging lens). The object distance (p2) for lens #2 is the distance between the virtual image and the converging lens, which is 40 cm - 60 cm = -20 cm. Using the lens formula for lens #2: 1/f2 = 1/p2 + 1/q2, we find the final image distance (q2) to be 60 cm. The positive sign indicates that the final image is real and on the opposite side of the converging lens.
Lastly, we can find the final image height (h2) using the magnification formula: h2/h1 = q2/p2, which gives us h2 = -18 cm. The negative sign indicates that the final image is inverted.
In summary, the final image formed by the two-lens combination has the following characteristics:
1. Real image
2. Inverted
3. Image distance of 60 cm from the converging lens
4. Image height of 18 cm

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in the case of reflection from a planar surface, use fermat's principle to prove that the incident and reflected rays share a common plane with the normal to the surface, i.e. the plane of incidence.

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Fermat's principle is a fundamental principle of optics that states that light travels from one point to another along the path that requires the least time.

When light reflects from a planar surface, it follows this principle, taking the path that minimizes the time of travel.
To prove that the incident and reflected rays share a common plane with the normal to the surface, we must first consider the path of the light rays. Let us assume that the incident ray and the reflected ray are both in the same plane, which is the plane of incidence. This plane is perpendicular to the surface of the mirror.
Now, let us consider a point P on the incident ray and a point Q on the reflected ray. According to Fermat's principle, the path taken by the light between P and Q is the path that requires the least time. This path can be shown to lie in the same plane as the incident and reflected rays, i.e., the plane of incidence.
To see this, we can consider the path of the light ray between P and Q. Since the angle of incidence is equal to the angle of reflection, the path of the light ray can be represented by the angle of incidence, the angle of reflection, and the normal to the surface. These three vectors lie in the same plane, which is the plane of incidence.
Therefore, we have proved that the incident and reflected rays share a common plane with the normal to the surface, i.e., the plane of incidence. This is a fundamental principle of optics that is used to explain the reflection of light from a planar surface.

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a radio station broadcasts with a power of 90.13 kw. how many photons are produced each second if that station broadcasts at a frequency of 101.2 m hz

Answers

The radio station produces approximately 5.6 x [tex]10^2^4[/tex] photons every second at a frequency of 101.2 MHz with a power of 90.13 kW.

What is the estimated number of photons produced per second?

The number of photons produced by a radio station is determined by its power output and frequency. The formula used to calculate the number of photons produced per second is given by the equation:

n = (P/E) x Avogadro's number

Where n is the number of photons, P is the power in watts, E is the energy per photon (Planck's constant x frequency), and Avogadro's number is the number of particles per mole (6.022 x [tex]10^2^3[/tex]).

Using the given values of power (90.13 kW) and frequency (101.2 MHz), we can calculate the energy per photon to be 1.24 x [tex]10^-^2^5[/tex] joules. Substituting these values into the equation, we get:

n = (90.13 x [tex]10^3[/tex] / 1.24 x [tex]10^-^2^5[/tex]) x 6.022 x [tex]10^2^3[/tex]

n = 5.6 x [tex]10^2^4[/tex] photons/second

Therefore, a radio station broadcasting with a power of 90.13 kW at a frequency of 101.2 MHz produces approximately 5.6 x [tex]10^2^4[/tex] photons per second.

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A 20o full-depth steel spur pinion with 18 teeth is to transmit 2.5 hp at a speed of 600 rev/min. Determine appropriate values for the face width and diametral pitch based on an allowable bending stress of 10kpsi.

Answers

The appropriate values for the face width and diametral pitch are 0.02 in and 7.73 teeth/in, respectively.

To determine the face width and diametral pitch of a 200 full-depth steel spur pinion with 18 teeth that can transmit 2.5 hp at a speed of 600 rev/min, we must first consider the allowable bending stress of 10kpsi.

Using the equation P = (2πNT)/60, where P is the power transmitted, N is the speed in revolutions per minute, and T is the torque, we can solve for T.

Thus, T = (P x 60)/(2πN).

Substituting the given values, we get T = (2.5 x 60)/(2π x 600) = 0.0631 lb-ft.

Next, we can use the equation T = (π/2)σb[(d²)/dp], where σb is the allowable bending stress, d is the pitch diameter, and dp is the diametral pitch.

Rearranging the equation, we get dp = (π/2)σb(d²)/T.

Substituting the given values and solving for dp, we get dp = 7.73 teeth/in.

To determine the face width, we can use the equation F = (2KTb)/(σbY), where F is the face width, K is the load distribution factor, Tb is the transmitted torque, and Y is the Lewis form factor.

Substituting the given values, we get F = (2 x 1.25 x 0.0631)/(10 x 0.154) = 0.0195 in or approximately 0.02 in.

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The spool has a mass of 64kg and a radius of gyration kG = 0.3m If it is released from rest, determine how far its center descends down the plane before it attains an angular velocity omega = 10 rad / s Neglect the mas of the cord which is wound around the central core.
The coefficient of kinetic friction between the spool and plane at A is μk = 0.2

Answers

The spool center will descend up to 0.468 m  before it attains an angular velocity omega = 10 rad / s

The Normal force can be calculated on a surface inclined by angle theta

Normal force = mass × gravitational acceleration × cos(theta)

since the angle of the plane is not mentioned, we will consider theta equal to 0.

Normal force = mass × gravitational acceleration × cos(theta)

Normal force = 64 kg × 9.8 m/s^2 × cos(0°)

Normal force = 627.2 N

The friction force can be calculated using the coefficient of kinetic friction:

Friction force = μk × Normal force

Friction force = 0.2 * 627.2 N

Friction force = 125.44 N

The work done by friction is equal to the change in kinetic energy,

Since the initial kinetic energy is 0:

Work done by friction = (1/2) × I × ω² - 0

Work done by friction =  (1/2) × I × ω²

= (1/2) ×  (64 kg ×  (0.3 m)^2) ×  (10 rad/s)^2

Work done by friction = 288 J

To find the height h, we can now set the work done by friction equal to the gravitational potential energy:

Work done by friction = m × g × h

h = Work done by friction / (m × g)

h = 288 J / (64 kg ×9.8 m/s^2)

h ≈ 0.468 m

Therefore, the center of the spool descends approximately 0.468 meters down the plane before attaining an angular velocity of 10 rad/s.

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A torque of 50.0 n-m is applied to a grinding wheel ( i=20.0kg-m2 ) for 20 s. (a) if it starts from rest, what is the angular velocity of the grinding wheel after the torque is removed?

Answers

The angular velocity of the grinding wheel after the torque is removed is 50 rad/s.

We can use the rotational version of Newton's second law, which states that the net torque acting on an object is equal to the object's moment of inertia times its angular acceleration:

τ = I α

where τ is the torque, I is the moment of inertia, and α is the angular acceleration.

Assuming that the grinding wheel starts from rest, its initial angular velocity is zero, so we can use the following kinematic equation to find its final angular velocity:

ω = α t

where ω is the final angular velocity and t is the time for which the torque is applied.

Substituting the given values, we have:

τ = I α

[tex]α = τ / I = 50.0 N-m / 20.0 kg-m^2 = 2.5 rad/s^2[/tex]

[tex]ω = α t = 2.5 rad/s^2 x 20 s = 50 rad/s[/tex]

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The photons used in microwave ovens have a momentum of 5.2×10−33 kg⋅m/s.(a) What is their wavelength?(b) How does the wavelength of the microwaves compare with the size of the holes in the metal screen on the door of the oven?

Answers

The wavelength of the microwaves is 0.127 meters, or 127 millimeters. The wavelength of the microwaves is much larger than the size of the holes.

(a) Using the de Broglie relation, λ = h/p, where h is the Planck constant and p is the momentum, we have: λ = h/p = 6.626 x[tex]10^{-34}[/tex] Js / 5.2 x [tex]10^{-33}[/tex] kgm/s = 0.127 meters. So the wavelength of the microwaves is 0.127 meters, or 127 millimeters.

(b) The size of the holes in the metal screen on the door of the oven is typically on the order of millimeters, so the wavelength of the microwaves is much larger than the size of the holes. This means that the microwaves are not significantly blocked by the screen and can pass through to heat the food inside the oven.

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What conditions must n satisfy to make x^2 test valid?
N must be equal to 10 or more
N must be equal to 5 or more
N must be large enough so that for every cell the expected cell count will be equal to 10 or more
N must be large enough so that for every cell the expected cell count will be equal to 5 or more

Answers

For the chi-square (x^2) test to be valid, N must be large enough so that for every cell the expected cell count will be equal to 5 or more.

To make the x^2 test valid, N must be large enough so that for every cell the expected cell count will be equal to 5 or more. In other words, N must be such that each cell in the contingency table has a sufficient number of observations to ensure that the test is reliable. Some guidelines suggest that N should be at least 10 or more, while others suggest that N should be at least 5 or more. However, the most important consideration is to ensure that the expected cell count is not too low, as this can lead to inaccurate or misleading results. Therefore, the key condition for a valid x^2 test is to have a sufficiently large sample size to ensure that each cell has an expected count of at least 5.

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consider an oscillating lc circuit with inductance l and capacitance c. at time t=0 the current maximum at i. what is the maximum charge on the capacitor during the oscillations?

Answers

The maximum charge on the capacitor during the oscillations is equal to i/ω.

At time t=0, the current in the oscillating lc circuit with inductance L and capacitance C is at its maximum value of i. As the circuit oscillates, the charge on the capacitor varies periodically, resulting in a back-and-forth flow of energy between the inductor and the capacitor. During each oscillation, the maximum charge on the capacitor occurs when the current is at its zero crossing.

To determine the maximum charge on the capacitor, we can use the equation Q = CV, where Q is the charge, C is the capacitance, and V is the voltage across the capacitor. At the point where the current is at its zero crossing, the voltage across the capacitor is at its maximum value, which is given by V = i/(ωC), where ω = 1/√(LC) is the angular frequency of the oscillation. Substituting this into the equation for Q, we get:

Qmax = CVmax = C(i/(ωC)) = i/ω

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consider a 250-m2 black roof on a night when the roof’s temperature is 31.5°c and the surrounding temperature is 14°c. the emissivity of the roof is 0.900.

Answers

The Stefan-Boltzmann rule, which states that the energy radiated by an object is proportional to the fourth power of its temperature and emissivity, can be used to determine how quickly the black roof radiates heat into its surroundings. Consequently, the following is the formula for the power the roof radiates:

P = εσA(T^4 - T_0^4)

where P is the power radiated, E is the emissivity (in this case, 0.900), S is the Stefan-Boltzmann constant (5.67 x 10-8 W/m2K), A is the roof's surface area (250 m2), T is the roof's temperature in Kelvin (31.5 + 273 = 304.5 K), and T_0 is the temperature outside in K (14 + 273 = 287 K).

When we enter the values, we obtain:

P is equal to 0.900 x 5.67 x 10-8 x 250 x (304.54 - 287.4) = 10747 W.

As a result, the black roof is dispersing 10747 W of heat onto the area around it. This is an estimate of the radiation-related energy loss from the roof.

Using a white or reflective roof surface would reflect more of the incoming solar radiation and lessen the amount of heat that the roof absorbs as a way to mitigate this energy loss. Insulating the roof is another choice that would lessen the amount of heat transfer from the roof to the building below.

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To calculate the radiative heat transfer between the black roof and its surroundings, we can use the Stefan-Boltzmann law:

Q = σεA(Tᴿ⁴ - Tₛ⁴)

Where:

Q is the rate of radiative heat transfer (in watts)

σ is the Stefan-Boltzmann constant (5.67 x 10⁻⁸ W/m²K⁴)

ε is the emissivity of the black roof

A is the surface area of the roof (250 m²)

Tᴿ is the temperature of the black roof in Kelvin (315°C + 273.15 = 588.15 K)

Tₛ is the temperature of the surroundings in Kelvin (14°C + 273.15 = 287.15 K)

Substituting these values into the equation, we get:

Q = 5.67 x 10⁻⁸ x 0.900 x 250 x (588.15⁴ - 287.15⁴)

Q = 5.12 x 10⁴ W

Therefore, the rate of radiative heat transfer from the black roof to the surroundings is 5.12 x 10⁴ watts.

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A series circuit has an impedance of 61.0 Ω and a power factor of 0.715 at a frequency of 54.0 Hz . The source voltage lags the current. Part A What circuit element, an inductor or a capacitor, should be placed in series with the circuit to raise its power factor? - inductor - capacitor Part B What size element will raise the power factor to unity?

Answers

Therefore, a capacitor of approximately 0.0185 farads should be placed in series with the circuit to raise the power factor to unity.

Part A: A capacitor should be placed in series with the circuit to raise its power factor.
Part B: To raise the power factor to unity, the size of the capacitor needed can be calculated using the formula:
C = 1 / (2πfZtan(θ))
where C is the capacitance in farads, f is the frequency in hertz, Z is the impedance in ohms, and θ is the angle between the voltage and current phasors.
In this case, f = 54.0 Hz, Z = 61.0 Ω, and θ = cos⁻¹(0.715) = 44.4°. Plugging these values into the formula gives:
C = 1 / (2π x 54.0 x 61.0 x tan(44.4°)) ≈ 0.0185 F
Therefore, a capacitor of approximately 0.0185 farads should be placed in series with the circuit to raise the power factor to unity.
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You are flying at 0.97 c with respect to Kara. At the exact instant you pass Kara, she fires a very short laser pulse in the same direction you're heading.After 1.0 s has elapsed on Kara's watch, what does Kara say the distance is between you and the laser pulse?

Answers

Kara would say that the distance between someone and the laser pulse is 0.243 meters after 1.0 second has elapsed on someone's watch.

According to special relativity, the time dilation effect occurs when an object is moving relative to an observer. The moving object experiences time slower than the stationary observer.

The equation for length contraction in special relativity is given by:

L' = L / γ

Where:

L' is the contracted length observed by the moving observer.

L is the rest length of the object at rest.

γ (gamma) is the Lorentz factor given by γ = 1 / [tex]\sqrt{ (1 - v^{2} /c^{2})}.[/tex]

The laser pulse is emitted at the exact instant you pass Kara and travels in the same direction as you. Let's assume the rest length of the laser pulse is 1 meter (L = 1 meter) in Kara's frame of reference.

γ = 1 / [tex]\sqrt{(1 - v^{2}/c^{2})}[/tex]

= 1 / [tex]\sqrt{(1 - 0.97^{2})}[/tex]

= 1 / [tex]\sqrt{(0.0591)}[/tex]

= 1 / 0.2429

= 4.11

L' = L / γ

= 1 meter / 4.11

= 0.243 meters

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Oxygen-15 is used in PET imaging and is a beta-plus emitter.What is the daughter nucleus of this decay?
A) Fluoride-15
B) Nitrogen- 15
C) Nitrogen-14
D) Oxygen-15

Answers

The daughter nucleus of this decay Fluoride-15. The correct option is A.

Oxygen-15 is a radioactive isotope of oxygen that is commonly used in PET (positron emission tomography) imaging. In PET imaging, a small amount of a radioactive substance such as Oxygen-15 is injected into the body and then detected by a scanner, which creates images of the internal organs and tissues.

Oxygen-15 is a beta-plus emitter, which means it undergoes a decay process in which a proton in the nucleus is converted into a neutron, emitting a positron (a positively charged particle) and a neutrino in the process. The positron quickly interacts with an electron in the body, resulting in the annihilation of both particles and the emission of two gamma rays in opposite directions.

The daughter nucleus of the decay of Oxygen-15 is Fluoride-15. This is because the beta-plus decay process converts one proton in the nucleus into a neutron, changing the atomic number by one but leaving the mass number unchanged. Oxygen-15 has 8 protons and 7 neutrons, while Fluoride-15 has 9 protons and 6 neutrons. Thus, the decay of Oxygen-15 results in the production of Fluoride-15. The daughter nucleus of this decay Fluoride-15. The correct option is A.

To summarize, Oxygen-15 is a beta-plus emitter used in PET imaging, and its decay process results in the production of Fluoride-15 as the daughter nucleus. This decay process is important in medical imaging as it allows the detection of the distribution and metabolism of various compounds in the body, including glucose and other substances involved in cancer and other diseases.

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A 1,100 kg horse is walking at 2. 0 m/s.


What type of energy is being described?

Answers

The type of energy being described in this scenario is kinetic energy. Kinetic energy is the energy possessed by an object due to its motion.

In this case, the horse is walking at a velocity of 2.0 m/s. The formula to calculate kinetic energy is [tex]\( KE = \frac{1}{2}mv^2 \)[/tex], where m represents the mass of the object and v represents its velocity. Plugging in the given values, the kinetic energy of the horse can be calculated as follows:

[tex]\[KE = \frac{1}{2} \times 1100 \, \text{kg} \times (2.0 \, \text{m/s})^2 = 2200 \, \text{J}\][/tex]

Therefore, the horse has a kinetic energy of 2200 Joules. Kinetic energy is a form of mechanical energy, which is associated with the motion of an object. As the horse moves, its kinetic energy represents the energy of its motion.

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compared to the earth, planet x has twice the mass and twice the radius. this means that compared to the earth’s surface gravity, the surface gravity on planet x is:

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Compared to the surface gravity of Earth, the surface gravity on planet X is approximately 2.63 times greater. This means that objects on planet X would feel much heavier than they would on Earth.

Surface gravity is defined as the force that pulls objects towards the center of a celestial body. The force of gravity is determined by the mass and size of the object. In the case of planet X, it has twice the mass and twice the radius of Earth.

To calculate the surface gravity of planet X compared to Earth, we can use the formula:

Surface gravity = G(Mass of celestial body) / (Radius of celestial body)²

where G is the gravitational constant.

For Earth, the mass is approximately 5.97 x 10²⁴ kg and the radius is approximately 6,371 km.

Plugging in these values, we get:

Surface gravity of Earth = (6.67 x 10⁻¹¹ N(m² /kg² )) (5.97 x 10²⁴ kg) / (6,371 km)²

Surface gravity of Earth = 9.81 m/s²  

This means that the force of gravity on Earth's surface is 9.81 m/s² .

For planet X, the mass is twice that of Earth, or approximately 1.19 x 10²⁵ kg, and the radius is also twice that of Earth, or approximately 12,742 km.

Plugging in these values, we get:

Surface gravity of planet X = (6.67 x 10⁻¹¹ N(m²/kg² )) (1.19 x 10²⁵ kg) / (12,742 km)²  

Surface gravity of planet X = 25.8 m/s²  

Therefore, compared to the surface gravity of Earth, the surface gravity on planet X is approximately 2.63 times greater. This means that objects on planet X would feel much heavier than they would on Earth.

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An airtight box, having a lid of area 80cm2, is partially evacuated (i.e., has low pressure than outside atmosphere). Atmosphere pressure is 1.01×10 5
Pa. A force of 600N is required to pull the lid off the box. What was the pressure in the box?

Answers

The pressure in the box was 100 Pa.

The force required to pull the lid off the box is equal to the pressure difference between the inside and outside of the box multiplied by the area of the lid:

F = (P_outside - P_inside) * A_lid

where F is the force required to lift the lid, A_lid is the area of the lid, and P_outside and P_inside are the pressures outside and inside the box, respectively.

Solving for P_inside, we get:

P_inside = P_outside - F/A_lid

Substituting the given values, we get:

P_inside = 1.01×10^5 Pa - 600 N / (80 cm^2 * (1 m/100 cm)^2)

P_inside = 1.01×10^5 Pa - 750 Pa

P_inside = 100 Pa

Therefore, the pressure inside the box was 100 Pa.

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10-4. calculate the required diameter for certified-capacity liquid rupture discs for the following conditions. assume a liquid specific gravity of 1.2 for all cases. Liquid flow Set pressure Overpressure Backpressure a. 500 gpm b. 100 gpm c. 5 m/s d. 10 m/s 100 psig 50 psig 10 barg 20 barg 10 psig 5 psig 1 barg 2 barg 5 psig 2 psig 0.5 barg 1 barg

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The required diameter for certified-capacity liquid rupture discs for the given conditions are 6.08 inches for 500 gpm, 3.07 inches for 100 gpm, 1.29 inches for 5 m/s, and 1.60 inches for 10 m/s.

To calculate the required diameter for certified-capacity liquid rupture discs for the given conditions, we first need to determine the burst pressure for each case. The burst pressure is calculated using the following formula:
Burst Pressure = Set Pressure + Overpressure - Backpressure
Using the specific gravity of 1.2 for all cases, we can calculate the burst pressure for each scenario as follows:
a. 500 gpm: Burst Pressure = 100 psig + 50 psig - 10 psig = 140 psig
b. 100 gpm: Burst Pressure = 100 psig + 50 psig - 5 psig = 145 psig
c. 5 m/s: Burst Pressure = 10 barg + 1 barg - 0.5 barg = 10.5 barg
d. 10 m/s: Burst Pressure = 20 barg + 2 barg - 1 barg = 21 barg
Once we have the burst pressure, we can use the specific gravity and the following formula to calculate the required diameter of the rupture disc:
Diameter = (Flow Rate * 60 * Specific Gravity) / (Burst Pressure * 0.8 * 3.14)
Where:
Flow Rate = Liquid flow in gallons per minute (gpm) or meters per second (m/s)
Specific Gravity = 1.2
Burst Pressure = Calculated burst pressure in psig or barg
Using the above formula, we can calculate the required diameter for each scenario as follows:
a. 500 gpm: Diameter = (500 * 60 * 1.2) / (140 * 0.8 * 3.14) = 6.08 inches
b. 100 gpm: Diameter = (100 * 60 * 1.2) / (145 * 0.8 * 3.14) = 3.07 inches
c. 5 m/s: Diameter = (5 * 60 * 1.2) / (10.5 * 0.8 * 3.14) = 1.29 inches
d. 10 m/s: Diameter = (10 * 60 * 1.2) / (21 * 0.8 * 3.14) = 1.60 inches
Therefore, the required diameter for certified-capacity liquid rupture discs for the given conditions are 6.08 inches for 500 gpm, 3.07 inches for 100 gpm, 1.29 inches for 5 m/s, and 1.60 inches for 10 m/s.

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Light traveling through medium 3 (n3 3.00) is incident on the interface with medium 2 (n2- 2.00) at angle θ. If no light enters into medium 1 (n,-1.00), what can we conclude about 0? a) θ> 19.5° b) θ< 19.5° c) θ> 35.3。 d) θ < 35.3。 e) θ may have any value from 0° to 90° n,Ei n3 53

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Answer:Main answer:

The critical angle for total internal reflection at the interface between medium 2 and medium 3 is 19.5 degrees, so if no light enters into medium 1, we can conclude that the angle of incidence θ is greater than 19.5 degrees. Therefore, the correct answer is (a) θ > 19.5°.

Supporting answer:

The critical angle for total internal reflection at an interface between two media is given by the equation sin θc = n2/n3, where n2 and n3 are the refractive indices of the two media. Plugging in the given values, we get sin θc = 2/3, which gives us a critical angle of 19.5 degrees.

If the angle of incidence is less than the critical angle, some light will refract into medium 2, but if the angle of incidence is greater than the critical angle, all of the light will reflect back into medium 3. Therefore, if no light enters into medium 1, we can conclude that the angle of incidence must be greater than the critical angle, which is 19.5 degrees.

It's important to note that the refractive index of a medium is a measure of how much the speed of light is reduced when it passes through the medium, and this value depends on the properties of the medium.

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explain the difference between the diffraction and interference of light. describe the physics of both.

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Diffraction and interference are two important concepts in physics related to the behavior of light. Diffraction refers to the bending of light waves around an obstacle or through a small opening, resulting in a spread of light beyond the shadow region.

This phenomenon can be observed in everyday life, such as the appearance of a fringed pattern when light passes through a narrow slit or the spread of light around the edge of a door.

Interference, on the other hand, occurs when two or more light waves meet and combine to form a new wave with a different amplitude and direction. This can produce patterns of constructive or destructive interference, depending on the relative phase of the waves. Interference is commonly observed in experiments involving lasers and thin films, as well as in natural phenomena like the iridescent colors of soap bubbles and oil slicks.

The physics behind diffraction and interference can be explained by the wave nature of light, which is described by its wavelength, frequency, and amplitude. When light waves encounter an obstacle or a narrow opening, they diffract or bend around it, resulting in a spread of light beyond the shadow region. This effect is more pronounced for longer wavelengths, such as those of red and infrared light, and can be minimized by using smaller openings or higher frequencies.

Interference, on the other hand, results from the superposition of two or more waves, which can either reinforce or cancel each other out depending on their relative phase. This effect is commonly observed in experiments involving lasers and thin films, as well as in natural phenomena like the iridescent colors of soap bubbles and oil slicks.

diffraction and interference are two important concepts in physics related to the behavior of light. While diffraction refers to the bending of light waves around an obstacle or through a small opening, interference occurs when two or more light waves meet and combine to form a new wave with a different amplitude and direction. Both phenomena can be explained by the wave nature of light and have important applications in a wide range of fields, including optics, telecommunications, and materials science.

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A cylindrical capacitor has inner and outer radii at 5 mm and 15 mm, respectively, and the space between the conductors is filled with a dielectric material with relative permittivity of 2.0. The inner conductor is maintained at a potential of 100 V while the outer conductor is grounded. Find: (a) the voltage midway between the conductors, (b) the electric field midway between the conductors, and c) the surface charge density on the inner and outer conductors.

Answers

The surface charge density on the outer conductor is zero, since it is grounded and has no net charge.

(a) The voltage midway between the conductors can be calculated using the formula V = V1 - V2, where V1 is the voltage on the inner conductor and V2 is the voltage on the outer conductor. So, V = 100 V - 0 V = 100 V.
(b) The electric field midway between the conductors can be calculated using the formula E = V/d, where V is the voltage and d is the distance between the conductors. Here, the distance is the average of the inner and outer radii, which is (5 mm + 15 mm)/2 = 10 mm = 0.01 m. So, E = 100 V/0.01 m = 10,000 V/m.
(c) The surface charge density on the inner conductor can be calculated using the formula σ = ε0εrE, where ε0 is the permittivity of free space, εr is the relative permittivity, and E is the electric field. Here, σ = ε0εrE(1/r), where r is the radius of the inner conductor. So, σ = (8.85 x 10^-12 F/m)(2.0)(10,000 V/m)(1/0.005 m) = 3.54 x 10^-7 C/m^2.
The surface charge density on the outer conductor is zero, since it is grounded and has no net charge.

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A constant horizontal force of 150 N is applied to a lawn roller in the form of a uniform solid cylinder of radius 0.4 m and mass 13 kg . If the roller rolls without slipping, find the acceleration of the center of mass. The acceleration of gravity is 9.8 m/s^2. Answer in units of m/s^2. Then, find the minimum coefficient of friction necessary to prevent slipping.

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The acceleration of the center of mass of the lawn roller is 1.21 m/s². The minimum coefficient of friction necessary to prevent slipping is 0.27.

The torque due to the applied force causes the lawn roller to undergo both linear and angular acceleration. Since the lawn roller rolls without slipping, the acceleration of the center of mass is related to the angular acceleration as a = αr, where α is the angular acceleration and r is the radius of the cylinder.

The net torque on the lawn roller is given by τ = Fr, where F is the applied force. Equating τ to Iα, where I is the moment of inertia of the cylinder, gives us α = F/(I+mr²), where m is the mass of the cylinder. Substituting the given values, we get α = 2.63 rad/s². Therefore, a = αr = 1.21 m/s².

In order for the lawn roller to not slip, the force of static friction between the roller and the ground must be greater than or equal to the maximum static friction force, which is equal to the coefficient of static friction μs multiplied by the normal force.

The normal force is equal to the weight of the cylinder, which is mg, where g is the acceleration due to gravity. Therefore, we need μs ≥ F/(mg) = 0.27, where F is the applied force, m is the mass of the cylinder, and g is the acceleration due to gravity.

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a small, square loop carries a 41 a current. the on-axis magnetic field strength 48 cm from the loop is 6.8 nt .What is the edge length of the loop?

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The edge length of the small, square loop carrying a 41 A current is approximately 2.88 mm. This is found by using the formula for magnetic field strength and solving for the area of the loop

To solve this problem, we need to use the formula for the magnetic field created by a current-carrying loop at a distance from the center of the loop. The formula is:
B = (μ0 * I * A) / (2 * R)
Where B is the magnetic field strength, μ0 is the permeability of free space (4π × 10^-7 T·m/A), I is the current in the loop, A is the area of the loop, and R is the distance from the center of the loop to the point where the magnetic field is measured.
In this problem, we know that the current in the loop is 41 A, the magnetic field strength at a distance of 48 cm from the loop is 6.8 nT (which is 6.8 × 10^-9 T), and the distance from the center of the loop to the point where the magnetic field is measured is R = 48 cm = 0.48 m.
Solving for the area of the loop, we get:
A = (2 * R * B) / (μ0 * I)
A = (2 * 0.48 m * 6.8 × 10^-9 T) / (4π × 10^-7 T·m/A * 41 A)
A = 8.32 × 10^-6 m^2
Now, since the loop is square, we can find the length of one of its edges by taking the square root of its area:
Edge length = √A
Edge length = √(8.32 × 10^-6 m^2)
Edge length = 0.00288 m or 2.88 mm
Therefore, the edge length of the loop is approximately 2.88 mm.
The edge length of the small, square loop carrying a 41 A current is approximately 2.88 mm. This is found by using the formula for magnetic field strength and solving for the area of the loop, which is then used to find the length of one of its edges.

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A standing wave is formed on a string that is 37 m long, has a mass per unit length 0.00874 kg/m, and is stretched to a tension of 15 N.1) Find the fundamental frequency. Answer in units of cycles/s.2) Find the next frequency that could cause a standing wave pattern.Answer in units of cycles/s.

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The fundamental frequency is approximately 0.36 cycles/s and the next frequency is approximately 0.72 cycles/s.

To find the fundamental frequency of the standing wave on the string, we can use the equation:
f = (1/2L) √(T/μ)
Where L is the length of the string, T is the tension, μ is the mass per unit length, and f is the frequency. Plugging in the given values, we get:
f = (1/2*37) √(15/0.00874) = 42.9 cycles/s
So the fundamental frequency is 42.9 cycles/s.
To find the next frequency that could cause a standing wave pattern, we can use the formula:
f2 = 2f1
Where f1 is the fundamental frequency and f2 is the next frequency. Plugging in the value of f1, we get:
f2 = 2*42.9 = 85.8 cycles/s
So the next frequency that could cause a standing wave pattern is 85.8 cycles/s.
In summary, the fundamental frequency of the standing wave on the string is 42.9 cycles/s and the next frequency that could cause a standing wave pattern is 85.8 cycles/s.

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What is most likely the color of the light whose second-order bright band forms an angle of 13. 5° if the diffraction grating has 175 lines per mm? green red violet yellow.

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The second-order bright band of a diffraction grating with 175 lines per mm forming an angle of [tex]13.5^0[/tex] is most likely violet.

The angle at which the bright band forms can be determined using the equation for diffraction: [tex]m\lamba = d sin\theta[/tex], where m is the order of the bright band,[tex]\lambda[/tex] is the wavelength of light, d is the spacing between the grating lines and [tex]\theta[/tex] is the angle. In this case, m = 2, d = 1/175 mm = 0.00571 mm, and [tex]\theta =[/tex] [tex]13.5^0[/tex].

Rearranging the equation, we have [tex]\lambda = d sin\theta / m[/tex]. Plugging in the values, we find [tex]\lambda = (0.00571 mm)(sin(13.5^0))/(2) = 0.001293 mm = 1.293 nm[/tex]. Comparing this value to the visible light spectrum, we find that violet light has a wavelength ranging from approximately 380 to 450 nm. Since the calculated wavelength of 1.293 nm falls within this range, it is most likely that the colour of the light is violet.

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a 8.0 μfμf capacitor, a 11 μfμf capacitor, and a 16 μfμf capacitor are connected in parallel. part a what is their equivalent capacitance?

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Three capacitors with capacitance values of 8.0 μf, 11 μf, and 16 μf are connected in parallel. The equivalent capacitance is calculated by adding up the individual capacitances, resulting in a total of 35 μf.

When capacitors are connected in parallel, the equivalent capacitance is equal to the sum of individual capacitances. Therefore, to find the equivalent capacitance of the given capacitors, we simply add their capacitance values.

C_eq = C_1 + C_2 + C_3

C_eq = 8.0 μF + 11 μF + 16 μF

C_eq = 35 μF

The equivalent capacitance of the three capacitors connected in parallel is 35 μF.

In parallel connection, the positive plate of all capacitors is connected together and the negative plate of all capacitors is also connected together. When capacitors are connected in parallel, the voltage across each capacitor is the same and equal to the voltage across the entire circuit. The total capacitance of the circuit is increased, which results in an increase in the amount of charge that can be stored in the circuit.

In practical applications, capacitors are often connected in parallel to increase the capacitance of a circuit. For example, in an audio system, capacitors are used to filter out unwanted noise from the signal. By connecting multiple capacitors in parallel, the amount of noise that can be filtered out is increased, resulting in a cleaner audio signal.

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calculate the range of wavelengths (in m) for x-rays given their frequency range is 30,000 to 3.0 ✕ 107 thz. Smaller Value ___________ mLarger Value ____________ m

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The range of wavelengths (in meters) for x-rays with a frequency range of 30,000 THz to 3.0 × 10⁷ THz is approximately 1.0 × 10⁻¹¹ m to 1.0 × 10⁻⁸ m.


To calculate the range of wavelengths, we use the formula:
Wavelength (λ) = Speed of light (c) / Frequency (f)

The speed of light (c) is approximately 3.0 × 10⁸ m/s.

For the smaller value, use the higher frequency (3.0 × 10⁷ THz):

λ = (3.0 × 10⁸ m/s) / (3.0 × 10⁷ THz × 10¹² Hz/THz)
λ ≈ 1.0 × 10⁻¹¹ m

For the larger value, use the lower frequency (30,000 THz):

λ = (3.0 × 10⁸ m/s) / (30,000 THz × 10¹² Hz/THz)
λ ≈ 1.0 × 10⁻⁸ m


The range of wavelengths for x-rays is approximately 1.0 × 10⁻¹¹ m to 1.0 × 10⁻⁸ m.

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A street performer tosses a ball straight up into the air (event 1) and then catches it in his mouth (event 2).For each of the following observers, state whether the time they measure between these two events is the proper time or the dilated time.-the street performer-a stationary observer on the other side of the street-a person sitting at home watching the peformance on tv-a person observing the performance from a moving car

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The proper time is the time interval between two events that occur at the same location in space, while the dilated time is the time interval measured by an observer who is moving relative to the events.

For the events of the street performer tossing a ball straight up into the air and then catching it in his mouth, the time measured by each observer is as follows:

The street performer: Since the events are happening to the performer, he can measure the proper time between the two events.

A stationary observer on the other side of the street: The observer is not moving relative to the events, and is located at the same position for both events, so he can measure the proper time between the two events.

A person sitting at home watching the performance on TV: The TV signal takes time to travel to the person's TV set, so there is a delay between the actual events and the time the person sees them.

The person is not located at the same position for both events, so he cannot measure the proper time between the two events.

A person observing the performance from a moving car: The person is moving relative to the events, so he will measure the dilated time between the two events.

This is because the events appear to be happening at different positions due to the motion of the observer, and the time interval will appear longer than the proper time.

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