A rock is dropped from a 279 m high cliff. (a) how long does it take to fall the first 139.5 m?

Answers

Answer 1

it takes approximately 5.34 seconds for the rock to fall the first 139.5 meters.The time it takes for a rock to fall a certain distance can be calculated using the equation for free fall:

h = 1/2 * g * t^2

where:
h = distance fallen
g = acceleration due to gravity (approximately 9.8 m/s^2 on Earth)
t = time

In this case, the rock is dropped from a 279 m high cliff and we want to find the time it takes for the rock to fall the first 139.5 m.

First, we rearrange the equation to solve for time:

t^2 = (2 * h) / g

Substituting the given values:
t^2 = (2 * 139.5 m) / 9.8 m/s^2

t^2 = 28.47 s^2

Taking the square root of both sides, we get:
t = 5.34 s

Note: The time it takes for the rock to fall the remaining distance from 139.5 m to the bottom of the cliff would be the same, as long as there is no air resistance.

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Related Questions

Write the form of the partial fraction decomposition of the function (see example). do not determine the numerical values of the coefficients. (a) 4x (x 4)(3x 2)

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The given function is 4x / ((x+4)(3x+2)). We want to find the partial fraction decomposition of this function, without determining the numerical values of the coefficients.

To decompose the given function, we need to factorize the denominator first. The denominator can be factored as (x+4)(3x+2).

Now, let's express the given function as a sum of fractions with simpler denominators. We assume that the partial fraction decomposition has the following form:

4x / ((x+4)(3x+2)) = A / (x+4) + B / (3x+2)

To find the values of A and B, we can use a common denominator of (x+4)(3x+2) for both fractions on the right-hand side of the equation. This gives us:

4x = A(3x+2) + B(x+4)

Expanding the right-hand side, we get:

4x = 3Ax + 2A + Bx + 4B

Matching the coefficients of x on both sides of the equation, we have:

4x = (3A + B)x

Since the coefficients of x must be equal on both sides, we have:

3A + B = 4

Matching the constant terms on both sides of the equation, we have:

2A + 4B = 0

We now have a system of two equations with two unknowns (A and B). Solving this system will give us the values of A and B, which will allow us to complete the partial fraction decomposition.

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What are th magnitide and direction of acceleration of a proton where the electric field has agnitude 33 kn/c?

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The magnitude and direction of acceleration of a proton in an electric field can be determined using the equation:

a = qE/m

where a is the acceleration, q is the charge of the proton, E is the electric field, and m is the mass of the proton.

In this case, the magnitude of the electric field is given as 33 kN/C.

The charge of a proton is approximately 1.6 x 10^-19 C, and the mass of a proton is approximately 1.67 x 10^-27 kg.

Plugging in these values into the equation, we get:

a = (1.6 x 10^-19 C)(33 x 10^3 N/C) / (1.67 x 10^-27 kg)

Simplifying the calculation, we find that the magnitude of the acceleration is approximately 3.0 x 10^7 m/s^2.

The direction of the acceleration depends on the charge of the proton and the direction of the electric field. Since the proton has a positive charge, it will accelerate in the same direction as the electric field.

Therefore, the direction of the acceleration is the same as the direction of the electric field.

In summary, the magnitude of the acceleration of the proton is approximately 3.0 x 10^7 m/s^2, and the direction of the acceleration is the same as the direction of the electric field.

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(d) A 1.60-kg block of ice at 0°C is set sliding at 2.50 m/s over a sheet of copper at 0°C . Friction brings the block to rest. Find the mass of the ice that melts.

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The mass of the ice that melts is 0.150 kg (or 150 grams). The mass of the ice that melts can be found by considering the energy transferred due to friction.

First, let's calculate the initial kinetic energy of the block of ice. The formula for kinetic energy is given by KE = (1/2) * [tex]m * v^2,[/tex] where m is the mass and v is the velocity. Given that the mass of the block of ice is 1.60 kg and its initial velocity is 2.50 m/s, we can calculate the initial kinetic energy as follows:

KE_initial =[tex](1/2) * 1.60 kg * (2.50 m/s)^2[/tex]

Next, let's calculate the final kinetic energy of the block of ice when it comes to rest. Since the block of ice comes to rest, its final velocity is 0 m/s. Therefore, the final kinetic energy is:

KE_final = [tex](1/2) * 1.60 kg * (0 m/s)^2[/tex]

Now, the work done by friction can be calculated by subtracting the final kinetic energy from the initial kinetic energy:

Work_friction = KE_initial - KE_final

Since the block of ice comes to rest, all the initial kinetic energy is converted into heat energy, which results in the melting of the ice. The energy required to melt a certain mass of ice can be found using the specific latent heat of fusion for ice, which is 334,000 J/kg.

Therefore, the mass of the ice that melts can be calculated as:

Mass_melted = Work_friction / (specific latent heat of fusion for ice)

Let's substitute the values we have into the equation:

Mass_melted = (KE_initial - KE_final) / (specific latent heat of fusion for ice)

Mass_melted =[tex][(1/2) * 1.60 kg * (2.50 m/s)^2 - (1/2) * 1.60 kg * (0 m/s)^2] / 334,000 J/kg[/tex]

After simplifying the equation, we find:

Mass_melted =[tex](1/2) * 1.60 kg * (2.50 m/s)^2 / 334,000 J/kg[/tex]

Mass_melted = 0.150 kg

Therefore, the mass of the ice that melts is 0.150 kg (or 150 grams).

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Model air as a diatomic ideal gas with M = 28.9 g/mol. A cylinder with a piston contains 1.20kg of air at 25.0°C and 2.00×10⁵Pa . Energy is transferred by heat into the system as it is permitted to expand, with the pressure rising to 4.00×10⁵Pa . Throughout the expansion, the relationship between pressure and volume is given by

P = CV¹/²

where C is a constant. Find.(b) the final volume.

Answers

[tex]P_{1} V_{1} = nRT_{1}[/tex]The final volume is approximately 2133.76 L is the answer.

To find the final volume, we can use the ideal gas law and the given relationship between pressure and volume during the expansion.

The ideal gas law is given by:

PV = nRT

where

P is the pressure,

V is the volume,

n = the number of moles of gas,

R is the ideal gas constant, and

T is the temperature.

Given:

Mass of air (m) = 1.20 kg = 1200 g

Molar mass of air (M) = 28.9 g/mol

Initial temperature (T1) = 25.0 °C = 298.15 K

Initial pressure (P1) = 2.00 × 10⁵ Pa

Final pressure (P2) = 4.00 × 10⁵ Pa

First, we need to calculate the number of moles of air using the mass and molar mass:

n = m / M

n = 1200 g / 28.9 g/mol

n ≈ 41.509 mol

Next, we can use the ideal gas law to find the initial volume (V1) using the initial conditions:

[tex]P_{1} V_{1} = nRT_{1}[/tex]

[tex]V_{1} = nRT_{1} / P_{1}[/tex]

[tex]V_{1}[/tex] = (41.509 mol)(8.314 J/(mol·K))(298.15 K) / (2.00 × 10⁵ Pa)

[tex]V_{1}[/tex] ≈ 533.44 L

Now, let's substitute the given relationship between pressure and volume (P = CV¹/²) into the ideal gas law equation:

(P/C)² = V

C²P² = V

Since C is a constant, we can rewrite it as C²P² = k, where k is another constant.

Now, we can use the initial and final conditions to find the final volume (V2):

C²P1² = [tex]V_{1}[/tex]

C²P2² = [tex]V_{2}[/tex]

So, by dividing the second equation by the first equation-

(P2² / P1²) = ([tex]V_{2}[/tex] / [tex]V_{1}[/tex])

By Substituting the known values:

(4.00 × 10⁵ Pa)² / (2.00 × 10⁵ Pa)² = [tex]V_{2}[/tex] / (533.44 L)

(16 / 4) = [tex]V_{2}[/tex] / (533.44 L)

4 = [tex]V_{2}[/tex] / (533.44 L)

Multiplying both sides by 533.44 L:

[tex]V_{2}[/tex] = 4 × 533.44 L

[tex]V_{2}[/tex] ≈ 2133.76 L

Therefore, the final volume is approximately 2133.76 L.

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Which planetary body has the fastest orbit, and which has the slowest orbit? Do you notice a general pattern here? Briefly explain a relationship between orbital velocity and orbital radius.

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The planetary body with the fastest orbit is Mercury, and the one with the slowest orbit is Neptune.

There is a general pattern between orbital velocity and orbital radius known as Kepler's second law of planetary motion. According to this law, a planet sweeps out equal areas in equal times as it orbits the Sun. This implies that planets closer to the Sun have smaller orbital radii and must travel faster to cover the same area in the same amount of time.

The relationship between orbital velocity and orbital radius can be expressed as v ∝ 1/r, where v represents the orbital velocity and r denotes the orbital radius. This relationship shows that as the orbital radius increases, the orbital velocity decreases. In other words, planets farther from the Sun have slower orbital velocities compared to those closer to the Sun.

This pattern is consistent with observations in our solar system. The inner planets, such as Mercury, have smaller orbital radii and faster orbital velocities, while the outer planets, like Neptune, have larger orbital radii and slower orbital velocities.

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(a) In the hydrogen atom, can the quantum number n increase without limit? (b) Can the frequency of possible discrete lines in the spectrum of hydrogen increase without limit? (c) Can the wavelength of possible discrete lines in the spectrum of hydrogen increase without limit?

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The quantum number n in a hydrogen atom can increase without limit, but the wavelength of possible discrete lines in the hydrogen spectrum cannot increase without limit.

For an electron in an atom, the allowed values of n are 1, 2, 3, ..., ∞. It follows that n can increase without limit in a hydrogen atom since its electron can be moved to higher energy levels as long as the energy is supplied to it.

A hydrogen atom's frequency of possible discrete lines in the spectrum can also increase without limit. A spectral line occurs when an atom changes energy levels, and the energy of the photon emitted corresponds to the energy level difference. Since the energy difference between two levels increases as the level number rises, the frequency of the emitted photon also rises. Therefore, the frequency of possible discrete lines in the spectrum of hydrogen can increase indefinitely.

The wavelength of possible discrete lines in the spectrum of hydrogen cannot increase without limit. The frequency of spectral lines is inversely proportional to their wavelength, as determined by the relation E = hf, where E is the energy of a photon, h is Planck's constant, and f is the frequency of the photon. As a result, a photon with a high frequency corresponds to a short wavelength, whereas a photon with a low frequency corresponds to a long wavelength. As a result, the wavelength of possible discrete lines in the hydrogen spectrum cannot rise indefinitely.

In a hydrogen atom, the principal quantum number (n) can have values of 1, 2, 3, 4, … and infinity. Hence, the quantum number n can increase without limit in a hydrogen atom. The possible discrete lines in the hydrogen spectrum are due to the transition of electrons from higher energy levels to lower energy levels, and the frequency of these lines is directly proportional to the energy difference between these levels.

Since the energy difference between two levels increases as the level number rises, the frequency of the emitted photon also rises. Therefore, the frequency of possible discrete lines in the spectrum of hydrogen can increase indefinitely. On the other hand, the wavelength of possible discrete lines in the hydrogen spectrum cannot increase without limit. The frequency of spectral lines is inversely proportional to their wavelength.

A photon with a high frequency corresponds to a short wavelength, whereas a photon with a low frequency corresponds to a long wavelength. As a result, the wavelength of possible discrete lines in the hydrogen spectrum cannot rise indefinitely.

The quantum number n in a hydrogen atom can increase without limit, but the wavelength of possible discrete lines in the hydrogen spectrum cannot increase without limit.

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A reverse-biased silicon diode is connected in series with a 12 v source and a resistor. the voltage across the diode is:________

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The voltage drop across the diode is minimal and can be considered as zero or approximately 12 V.Consequently, the voltage across the diode is negligible or approximately 12 V.

In the given problem, a reverse-biased silicon diode is connected in series with a 12 V source and a resistor. We need to find the voltage across the diode. To determine the voltage across the diode, we need to know about the reverse-biased diode and how it operates. In a reverse-biased diode, the p-type region of the diode is connected to the negative terminal of the battery, and the n-type region is connected to the positive terminal. In this way, a potential barrier is formed across the diode. A voltage applied in the forward direction increases the current flow, while a voltage in the reverse direction reduces the current flow and impedes it.

Due to this reason, the resistance of the diode in a reverse-biased condition is very high. The value of this resistance depends on the characteristics of the diode and can be of the order of millions of ohms or even more. Thus, in a reverse-biased silicon diode connected in series with a 12 V source and a resistor, the voltage across the diode is approximately 12 V as the diode offers very high resistance in the reverse direction, and a minimal amount of current flows through it. the voltage across the diode is approximately 12 V.

We know that a reverse-biased silicon diode is connected in series with a 12 V source and a resistor. When the diode is reverse-biased, it offers very high resistance, and a minimal amount of current flows through it. Therefore, the voltage drop across the diode is minimal and can be considered as zero or approximately 12 V. Consequently, the voltage across the diode is negligible or approximately 12 V.

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if a box on a pan balance reads 10 kg, you can be confident that the number represents the object's .(2 points)hardnessmasstemperatureweight

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When a box on a pan balance reads 10 kg, it indicates the object's weight, which is the force of gravity acting on it.

If a box on a pan balance reads 10 kg, you can be confident that the number represents the object's weight. Weight refers to the force of gravity acting on an object. It is different from mass, which is the amount of matter in an object. The weight of an object can vary depending on the strength of the gravitational field it is in. For example, an object that weighs 10 kg on Earth would weigh less on the Moon due to the Moon's weaker gravitational pull.

To understand this concept, imagine placing the box on a pan balance in different locations. If the box reads 10 kg on Earth, it would be heavier compared to the Moon. This is because the Earth has a stronger gravitational force than the Moon. However, the box's mass would remain the same, as mass is an intrinsic property of an object and does not change with the gravitational field.

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Assume an object of mass M is suspended from the bottom of the rope of mass m and length L in Problem 58 .(b) What If? Show that the expression in part (a) reduces to the result of Problem 58 when M=0 . (c) Show that for m<

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If the object mass is zero then the acceleration due to gravity acting on the rope will be (1/2)gL.

What if M = 0?The expression in part (a) becomes mLg/(2m) = (1/2)gL when M=0 which is the same result obtained in problem 58.

For m << M The expression in part (a) reduces toMgL/2M = g/2 which is independent of the mass of the rope.

This is the acceleration due to gravity acting on the object when the mass of the rope is negligible and can be ignored.

The expression in part (a) becomes (1/2)gL when M=0. For m << M, the expression reduces to g/2, independent of the mass of the rope.

Given that, a rope of mass m and length L is hung with a mass M. The rope has a uniform linear density.

We have to determine the effect on tension and the acceleration due to gravity when an object of mass M is suspended from the bottom of the rope and for m << M.

Let's look at both cases below(b) What if M = 0?

When the object mass M=0, the expression in part (a) becomes

mLg/(2m) = (1/2)gL

when M=0 which is the same result obtained in problem 58.

Hence, we can conclude that if the object mass is zero then the acceleration due to gravity acting on the rope will be (1/2)gL.

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Calculate the wavelength of x-rays scattering from a crystal lattice with a distance between crystal layers of 0.025 nm, scattering angle of 25 degrees, and first order diffraction.

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The wavelength of X-rays scattering from a crystal lattice with a distance between crystal layers of d and scattering angle of θ and first-order diffraction can be calculated using Bragg's law. The wavelength of the X-rays scattering from the crystal lattice is approximately 0.02095 nm.

To calculate the wavelength of X-rays scattering from a crystal lattice, we can use Bragg's Law:

nλ = 2dsinθ

where:

n = order of diffraction (first order diffraction in this case, so n = 1)

λ = wavelength of the X-rays (unknown)

d = distance between crystal layers (0.025 nm)

θ = scattering angle (25 degrees)

First, we need to convert the scattering angle from degrees to radians:

θ_radians = 25 degrees * (π/180)

Next, we can substitute the known values into Bragg's Law:

1 * λ = 2 * 0.025 nm * sin(25 degrees * (π/180))

Simplifying:

λ = 0.05 nm * sin(0.4363)

Calculating the sine value:

sin(0.4363) ≈ 0.419

Now, substituting this value into the equation:

λ ≈ 0.05 nm * 0.419

λ ≈ 0.02095 nm

Therefore, the wavelength of the X-rays scattering from the crystal lattice is approximately 0.02095 nm.

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The pressure regulator valve keeps the pressure at a regulated level by exhausting excess pressure back to the _________________.

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The pressure regulator valve is responsible for maintaining a regulated level of pressure. When the pressure exceeds the desired level, the valve exhausts the excess pressure back to the source.

To better understand this concept, let's use an analogy. Imagine a balloon being filled with air. As the air pressure inside the balloon increases, it reaches a certain point where it becomes too high, risking the balloon's rupture.

In this scenario, the pressure regulator valve acts like a safety mechanism. It senses the excessive pressure and releases some of the air back into the environment, ensuring that the balloon remains intact.

Similarly, in various systems such as pneumatic or hydraulic systems, the pressure regulator valve monitors the pressure and prevents it from exceeding a predetermined level.

By opening a pathway for the excess pressure to escape, the valve helps maintain a safe and regulated pressure, protecting the system from damage.

In summary, the pressure regulator valve exhausts excess pressure back to the source or the environment, ensuring that the pressure remains within a safe and regulated range.

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a railroad wagon accelerates from rest. a small metallic sphere of mass m is suspended at the end of a light string which attached to the wagon’s ceiling and makes an angle θ with the vertical.

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When a railroad wagon accelerates from rest, a small metallic sphere of mass m suspended at the end of a light string attached to the wagon's ceiling will make an angle θ with the vertical.

To analyze this situation, we can consider the forces acting on the sphere. The gravitational force mg will act vertically downward, while the tension in the string will act along the string and have both a horizontal and vertical component. The vertical component of the tension balances the weight of the sphere, so Tsinθ = mg.

The horizontal component of the tension provides the centripetal force required for the sphere to move in a circular path.

Since the wagon is accelerating, there must be a horizontal net force acting on the sphere. This net force is provided by the horizontal component of the tension, which equals ma (mass of the sphere times the acceleration of the wagon).

Therefore, we have:

Tsinθ = mg
Tcosθ = ma

Dividing the two equations, we get:

tanθ = a/g

This equation shows that the acceleration of the wagon can be determined by measuring the angle θ and the acceleration due to gravity g.

In summary, when a railroad wagon accelerates, the angle θ between the suspended sphere and the vertical can be used to determine the acceleration of the wagon using the equation tanθ = a/g.

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A 200-g block is attached to a horizontal spring and executes simple harmonic motion with a period of 0.250 s . The total energy of the system is 2.00 J . Find (a) the force constant of the spring.

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A 200-g block is attached to a horizontal spring and executes simple harmonic motion with a period of 0.250 s . The force constant of the spring is [tex]128π^2 N/m.[/tex]

To find the force constant of the spring, we can use the formula for the total energy of a system in simple harmonic motion:

[tex]Total Energy = 1/2 * k * A^2[/tex]

where k is the force constant of the spring and A is the amplitude of the oscillation.

Given that the total energy of the system is 2.00 J, we can substitute this value into the equation:

[tex]2.00 J = 1/2 * k * A^2[/tex]

Since the problem provides the period of oscillation, we can use the relationship between period and angular frequency:

[tex]T = 2π/ω[/tex]

where T is the period and ω is the angular frequency.

From this equation, we can solve for ω:

[tex]ω = 2π/T = 2π/0.250 s = 8π rad/s[/tex]

Next, we can use the relationship between angular frequency and force constant:

[tex]ω = √(k/m)[/tex]

where m is the mass of the block.

Rearranging the equation, we can solve for k:

[tex]k = ω^2 * m = (8π rad/s)^2 * 0.200 kg = 128π^2 N/m[/tex]

Thus, the force constant of the spring is [tex]128π^2 N/m.[/tex]

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An electromagnetic wave with a peak magnetic field magnitude of 1.50x10⁻⁷ T has an associated peak electric field of what magnitude? (a) 0.500x10⁻¹⁵ N/C (b) 2.00x10⁻⁵ N/C (c) 2.20x10⁴ N/C (d) 45.0 N/C (e) 22.0 N/C

Answers

An electromagnetic wave consists of both an electric field and a magnetic field that oscillate perpendicular to each other and to the direction of wave propagation. The magnitude of the electric field is directly related to the magnitude of the magnetic field. The correct answer is (d) 45.0 N/C.

To find the peak electric field magnitude associated with a given peak magnetic field magnitude, we can use the equation:

E = c * B

where E is the electric field magnitude, B is the magnetic field magnitude, and c is the speed of light in a vacuum (approximately 3.00 x 10^8 meters per second).

In this case, we are given a peak magnetic field magnitude of 1.50 x 10^-7 T. Plugging this value into the equation, we get:

[tex]E = (3.00 \times 10^8 m/s) * (1.50 \times 10^{-7} T)[/tex]
[tex]E = 4.50 \times 10^1 N/C[/tex]

Therefore, the peak electric field magnitude associated with the given peak magnetic field magnitude is 4.50 x 10^1 N/C.

In the provided answer choices, the closest magnitude to 4.50 x 10^1 N/C is 45.0 N/C, which corresponds to option (d).

To summarize, the correct answer is (d) 45.0 N/C.

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Solution is required 54. The area of the ellipse is 62. 83 m². The semi- minor axis is 0. 8 times the semi-major axis. Find the perimeter of the ellipse 55. The perimeter of ellipse is 21. 3m. The semi- major axis is 4m. What is the length of the latus rectum 56. The distance between the foci of an ellipse is 6m. The semi-minor axis is 4m long. Find the length of the latus rectum in meters 57. Determine the eccentricity of ellipse whose diameters are 10m and 8m long

Answers

Answer: the eccentricity of the ellipse is approximately 0.9487.

Explanation:

55. Given the semi-major axis, a = 4 m and the perimeter, P = 21.3 m, we can use the formula for the perimeter of an ellipse, which is given by:P = 4aE(1 - e²/4)where E is the complete elliptic integral of the second kind and e is the eccentricity of the ellipse.To find the eccentricity, we can use the fact that the semi-minor axis, b, is related to the semi-major axis by:b = 0.8aSubstituting this into the formula for the area of an ellipse, A = πab, we get:62.83 m² = πa(0.8a)a² = 78.54 m²a = √(78.54/π) ≈ 4.00 mSubstituting this into the formula for the perimeter, we get:21.3 m = 4(4)E(1 - e²/4)21.3 m/16 = E(1 - e²/4)1.33125 = E(1 - e²/4)We can use a numerical method, such as Newton's method, to solve for e. Alternatively, we can make an initial guess for e and iterate using the formula for E until we get a value that is close enough to 1.33125. For example, we can start with e = 0.5 and iterate using the following formula:e ← e + (1.33125 - E(1 - e²/4))/((e² - 4)E')where E' is the derivative of E. After a few iterations, we get:e ≈ 0.8891Therefore, the length of the latus rectum is given by:l = 2b²/a ≈ 1.024 m56. Given the distance between the foci, c = 6 m and the semi-minor axis, b = 4 m, we can use the formula for the length of the latus rectum, which is given by:l = 2b²/aSubstituting the formula for the distance between the foci, c = √(a² - b²), we get:l = 2b²/√(a² - b²)Squaring both sides, we get:l² = 4b⁴/(a² - b²)Substituting the formula for the area of an ellipse, A = πab, we get:62.83 m² = πa(4)²a² = 83.78 m²a = √(83.78/π) ≈ 5.15 mSubstituting this into the formula for the length of the latus rectum, we get:l ≈ 5.95 m57. Given the diameters of the ellipse, we can find the lengths of the semi-major and semi-minor axes:a = 10/2 = 5 mb = 8/2 = 4 mThe eccentricity of an ellipse is given by:e = √(a² - b²)/aSubstituting the values of a and b, we get:e = √(5² - 4²)/5 = √9/5 ≈ 0.9487Therefore, the eccentricity of the ellipse is approximately 0.9487.

A wood-framed single-family detached residence in Houston, Texas, has a south-facing wall with a net exposed area of 100ft2. The wall has an Rt of 15.1 hr*ft2*°F/Btu. Determine the sensible heat transmission component of the cooling load for this wall.

2. A wood-framed single-family detached residence in Austin, Texas, has a south-facing wall with a net exposed area of 100ft2. The wall has an Rt of 15.1 hr*ft2*°F/Btu. Determine the sensible heat transmission component of the cooling load for this wall.

Answers

The sensible heat transmission component of the cooling load for the south-facing wall in both Houston and Austin is approximately 132.45 Btu/hr. The values remain the same for both locations as the given data for the wall remains constant in the provided scenario.

The sensible heat transmission component of the cooling load for the south-facing wall in both Houston and Austin can be determined using the same formula:

Q = U × A × ΔT

Where:

Q is the sensible heat transmission (cooling load) in Btu/hr

U is the overall heat transfer coefficient in Btu/hrft²°F

A is the net exposed area of the wall in ft²

ΔT is the temperature difference in °F

Given that the net exposed area of the south-facing wall is 100 ft² and the overall heat transfer coefficient (Rt) is 15.1 hrft²°F/Btu, we need to calculate the temperature difference (ΔT).

Assuming a typical indoor-outdoor temperature difference of around 20°F during the cooling season for both Houston and Austin, we can substitute the values into the formula:

Q = (1 / Rt) × A × ΔT

ΔT = 20°F

Q = (1 / 15.1 hrft²°F/Btu) × 100 ft² × 20°F

Calculating the expression:

Q = (1 / 15.1) × 100 × 20 Btu/hr

Q ≈ 132.45 Btu/hr

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For the following questions, choose from the following possibilities: (a) yes; water (b) no; water (c) yes; air (d) no; air.(i) Can light undergo total internal reflection at a smooth interface between air and water? If so, in which medium must it be traveling originally?

Answers

Yes, light can undergo total internal reflection at a smooth interface between air and water. It must be travelling in water initially.

Total internal reflection occurs when light travelling in a denser medium reaches a boundary with a less dense medium and is reflected back into the denser medium instead of being transmitted. In this case, the denser medium is water and the less dense medium is air.

When light travels from the water towards the air, it reaches the boundary between the two mediums. The critical angle is the angle of incidence at which the refracted angle becomes 90 degrees, resulting in the light being totally reflected back into the water. This phenomenon occurs due to the difference in the refractive indices of air and water.

The refractive index of water is higher than that of air, which means that light travels slower in water than in air. As the angle of incidence increases beyond the critical angle, the light is no longer able to refract into the air and is completely reflected back into the water.

Therefore, light can undergo total internal reflection at a smooth interface between air and water, and it must be travelling in water initially for this phenomenon to occur.

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Robert Hofstadter won the 1961 Nobel Prize in Physics for his pioneering work in studying the scattering of 20 -GeV electrons from nuclei. (d) State how the wavelength compares with the diameter of an atomic nucleus, typically on the order of . 10⁻¹⁴ m

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Robert Hofstadter used 20 GeV electrons with a wavelength on the order of 10⁻¹² meters to study atomic nuclei, which are typically on the order of 10⁻¹⁴ meters in diameter. This allowed him to probe the internal structure of nuclei with great precision, revolutionizing our understanding of matter.

Robert Hofstadter's pioneering work on the scattering of 20 GeV electrons from atomic nuclei revolutionized our understanding of the structure of matter. One of the remarkable aspects of his research was the comparison between the wavelength of the electrons and the diameter of atomic nuclei.

The wavelength of the 20 GeV electrons used by Hofstadter in his experiments is determined by the de Broglie equation, which relates the momentum of a particle to its wavelength. With such high electron energies, the corresponding wavelengths are on the order of 10⁻¹² meters. This is significantly smaller than the typical diameter of an atomic nucleus, which is on the order of 10⁻¹⁴ meters.

This size difference is crucial for understanding the significance of Hofstadter's work. By using high-energy electrons with wavelengths much smaller than the size of the nucleus, he was able to probe the internal structure of atomic nuclei with unprecedented detail. The scattering patterns of these electrons provided valuable insights into the distribution of charge and the spatial extent of nuclear forces within the nucleus.

Hofstadter's groundbreaking research paved the way for further studies in nuclear physics and laid the foundation for our understanding of the fundamental properties of atomic nuclei. His work demonstrated the importance of using particles with extremely short wavelengths to investigate structures on the atomic scale, allowing us to unravel the mysteries of the microscopic world.

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select all that apply select all the places where light of the same wavelength from two sources would interfere constructively.

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Constructive interference occurs at points along the central axis between the sources, points equidistant from both sources, and points where the path difference is an odd multiple of half the wavelength. These are the places where light waves from two sources of the same wavelength interfere constructively.

When light waves from two sources interfere constructively, it means that they align and reinforce each other, resulting in a stronger combined wave. To determine where this constructive interference occurs, we need to consider the concept of path difference. Path difference is the difference in distance traveled by the waves from the two sources to a specific point.

For constructive interference to happen, the path difference should be a whole number multiple of the wavelength (λ) of the light. This occurs at certain locations, such as:

1. Points along the central axis between the sources: At these points, the path difference is zero because the waves have traveled the same distance. Therefore, constructive interference occurs here.

2. Points equidistant from both sources: At these points, the path difference is an integer multiple of the wavelength. As a result, the waves align and constructively interfere.

3. Points where the path difference is an odd multiple of half the wavelength: In these cases, the waves will be perfectly out of phase and then perfectly in phase again. Constructive interference occurs at these points.

It's important to note that constructive interference happens for light of the same wavelength from two sources. If the sources emit light of different wavelengths, the interference pattern will be more complex.

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In conclusion, places where light of the same wavelength from two sources would interfere constructively are determined by the path difference between the sources being an integer multiple of the wavelength

To determine the places where light of the same wavelength from two sources would interfere constructively, we need to understand the concept of constructive interference.

Constructive interference occurs when two waves meet in phase, meaning their crests and troughs align, resulting in a stronger combined wave.

For constructive interference to happen, the path difference between the two sources must be an integer multiple of the wavelength.

This occurs at specific points called nodes.

Here are a few examples of places where constructive interference may occur:

1. On a screen, the points equidistant from the two sources along a straight line connecting them.

These points will experience constructive interference.


2. Along the line connecting the two sources, there will be regions of constructive interference where the path difference between the two sources is equal to an integer multiple of the wavelength.
3. If the two sources are separated by a distance equal to an integer multiple of the wavelength, there will be constructive interference at all points along the line connecting the sources.

Remember, for constructive interference to occur, the path difference between the sources must be an integer multiple of the wavelength.

These are just a few examples, and there may be other scenarios depending on the specific situation.

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Travel agents collected data from recent travelers about their modes of transportation for their vacations, They found that 37% traveled by airplane, 8% traveled by train, and 7% traveled by airplane and train. Let A be the event that the mode of travel was airplane and let T be the event that the mode of travel was train.

koi zinda hai kya?

✌✌✌​

Answers

37% traveled by airplane

This means the probability of traveling by airplane (P(A)) is 0.37

8% traveled by train

This means the probability of traveling by train (P(T)) is 0.08

7% traveled by airplane and train

This double counts the people who traveled by both airplane and train.

We need to subtract this 7% from both the airplane and train percentages to get the correct probabilities.

So the corrected probabilities are:

P(A) = 0.37 - 0.07 = 0.30

P(T) = 0.08 - 0.07 = 0.01

Let's verify that these corrected probabilities add up to 1 (100%):

P(A) + P(T) = 0.30 + 0.01 = 0.31

Since the problem states only 37% traveled by airplane and 8% by train, with 7% by both, the remaining 48% must have traveled by other means.

So we can add that to get a total probability of 1:

P(A) + P(T) + P(other) = 0.30 + 0.01 + 0.48 = 0.79

Therefore, the corrected probabilities are:

P(A) = 0.30

P(T) = 0.01

P(other) = 0.48

As discussed in Chapter 27, the conductivity of metals decreases with increasing temperature due to electron collisions with vibrating atoms. In contrast, the conductivity of semiconductors increases with increasing temperature. What property of a semiconductor is responsible for this behavior? (a) Atomic vibrations decrease as temperature increases.(b) The number of conduction electrons and the number of holes increase steeply with increasing temperature.(c) The energy gap decreases with increasing temperature. (d) Electrons do not collide with atoms in a semiconductor.

Answers

In semiconductors, the increase in the number of charge carriers outweighs the impact of electron collisions, resulting in increased conductivity with increasing temperature.

The property of a semiconductor responsible for its conductivity increasing with increasing temperature is (b) The number of conduction electrons and the number of holes increase steeply with increasing temperature.

In semiconductors, the valence band is filled with electrons, and the conduction band is empty at absolute zero temperature. However, as the temperature increases, thermal energy causes some electrons to gain enough energy to jump from the valence band to the conduction band. This process creates additional charge carriers in the form of conduction electrons. Simultaneously, some electrons from the valence band leave behind "holes," which are essentially vacant positions in the valence band.

As the temperature rises further, more electrons gain sufficient energy to jump to the conduction band, and the number of conduction electrons increases steeply. At the same time, the number of holes in the valence band also increases. These additional charge carriers contribute to an increase in conductivity.

This behavior is different from metals because in metals, increasing temperature leads to increased electron collisions with vibrating atoms, which hampers electron flow and reduces conductivity. However, in semiconductors, the increase in the number of charge carriers outweighs the impact of electron collisions, resulting in increased conductivity with increasing temperature.

So, option (b) is the correct answer.

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The average (mean) age of people who respond to a particular survey is an example of a parameter?

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The average age of people who respond to a particular survey is an example of a statistic, as it describes a characteristic of the sample and not the entire population.

The average (mean) age of people who respond to a particular survey is an example of a statistic, not a parameter. In statistics, a parameter refers to a characteristic of a population, while a statistic refers to a characteristic of a sample.

To understand this distinction, let's break it down step-by-step:

1. Parameter: A parameter is a characteristic that describes a whole population. For example, if you wanted to know the average age of all people in a country, you would need to collect data from every single person in that country. The average age calculated from this complete data set would be a parameter.

2. Statistic: On the other hand, a statistic is a characteristic that describes a sample, which is a subset of the population. In practice, it is often not feasible to collect data from an entire population. Instead, we take a smaller representative group, called a sample, and use it to make inferences about the larger population. In the case of a survey, the average age calculated from the responses of the people who participated in the survey would be a statistic.

In summary, the average age of people who respond to a particular survey is an example of a statistic, as it describes a characteristic of the sample and not the entire population.

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A piston in a gasoline engine is in simple harmonic motion. The engine is running at the rate of 3600 rev/min. Taking the extremes of its position relative to its center point as ±5.00cm , find the magnitudes of the (b) maximum acceleration of the piston.

Answers

The maximum acceleration of the piston in simple harmonic motion is approximately 188.5 m/s², calculated using the formula a = -ω²x, where ω is the angular frequency and x is the displacement from the center position.

To find the maximum acceleration of the piston, we can use the equation for simple harmonic motion (SHM):

a = -ω²x

Where:

a is the acceleration

ω is the angular frequency

x is the displacement from the center position

The angular frequency (ω) can be calculated from the engine's rotational speed (ω) using the formula:

ω = 2πf

Where:

f is the frequency (revolutions per minute in this case)

Given:

Displacement (x) = ±5.00 cm = ±0.05 m

Rotational speed (f) = 3600 rev/min

First, we need to convert the rotational speed to angular frequency:

ω = 2π(3600 rev/min) * (1 min / 60 s)

   = 120π rad/s

Now we can calculate the maximum acceleration using the formula:

a = -ω²x

Substituting the values:

a = -(120π rad/s)² * (0.05 m)

Calculating the value:

a ≈ -188.5 m/s²

Since the acceleration is a vector quantity, the magnitude of the maximum acceleration is 188.5 m/s².

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a 40 kg child is sitting on a swing. the swing is attached to a tree branch by a single 2.40m long rope.

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Now we can calculate the torque by multiplying the weight by the perpendicular distance: torque = weight × distance = 392 N × 1.20 m = 470.4 Nm.

Therefore, the torque exerted by the child on the swing is 470.4 Nm.

The swing is attached to the tree branch by a single 2.40m long rope. The child's mass is 40 kg. To answer this question, we can use the concept of torque.

Torque is the rotational force exerted on an object. In this case, the torque exerted by the child on the swing can be calculated by multiplying the child's weight (mg) by the perpendicular distance (r) between the point of rotation (tree branch) and the child.

The child's weight can be calculated using the formula weight = mass × acceleration due to gravity. Since the child's mass is 40 kg, and acceleration due to gravity is approximately 9.8 m/s^2, the weight of the child is 40 kg × 9.8 m/s^2 = 392 N.

To find the perpendicular distance, we can use the length of the rope, which is 2.40m. Since the rope is attached to the tree branch, the perpendicular distance is half of the rope length, which is 2.40m ÷ 2 = 1.20m.

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How would you change a tree to convert an apomorphy to a plesiomorphy and why does this change work?

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To convert an apomorphy to a plesiomorphy in a tree, one would need to modify the tree structure by repositioning the branch that represents the apomorphic trait. This change works because apomorphies are derived traits that have evolved more recently in a particular lineage, whereas plesiomorphies are ancestral traits shared by multiple lineages.

In order to convert an apomorphy to a plesiomorphy, the branch representing the apomorphic trait would need to be moved higher up the tree, closer to the common ancestor of the lineages involved. By doing so, the apomorphic trait would now be present in multiple lineages, indicating its ancestral nature rather than a derived characteristic unique to a specific lineage. This change helps align the tree with the concept of plesiomorphy, where a trait is shared among multiple lineages due to inheritance from a common ancestor.

Overall, modifying the tree structure to reposition the branch representing the apomorphic trait to a higher position helps convert the apomorphy into a plesiomorphy by indicating its ancestral nature shared by multiple lineages.

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the nardo ring is a circular test track for cars. it has a circumference of 12.5 km. cars travel around the track at a constant speed of 100 km/h. a car starts at the easternmost point of the ring and drives for 7.5 minutes at this speed. what is the speed of the car in m/s ?

Answers

There are two types of quantities in physical science. both the scalar and vector quantities. While the vector quantity has both the magnitude and direction, the scalar quantity just has the magnitude. The displacement is equal to zero.

Thus, The distance between an object's beginning point and ending position is known as displacement.

The formula D = s x t

This can be used to determine how far an object has travelled. D stands for distance, s for speed, and t for time.

It is important to correctly convert the specified dimensions in order to remove the units from the fraction's denominator and numerator

   D = (12.5 km) = (100 km/h)(7.5 min)(1 h/60 min)

This indicates that the object had recently returned to its original location. The displacement is therefore equal to ZERO.

Thus, There are two types of quantities in physical science. both the scalar and vector quantities. While the vector quantity has both the magnitude and direction, the scalar quantity just has the magnitude. The displacement is equal to zero.

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What is the height of the resultant wave formed by the interference of the two waves at the position x = 0.5 m at time t = 0.2 s?

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The resultant wave formed by the interference of the two waves at the position x = 0.5 m at time t = 0.2 s has a height of 1.14 cm.

When two waves meet, they either enhance or decrease each other's amplitude based on their phase difference. If the phase difference between two waves is an even multiple of pi, they are in phase, and their amplitudes add up, resulting in constructive interference. In contrast, if the phase difference is an odd multiple of pi, the waves will be out of phase, and their amplitudes will cancel out, resulting in destructive interference.

Here, the phase difference is

[tex]0.2 * 2 * \pi / 0.005 - \pi / 2[/tex]

= 77.75 degrees

= 1.36 rad.

The amplitude of the resultant wave is given by

A = A1 + A2 + 2 A1 A2 cos (phi) where phi is the phase difference between the two waves,

A1 and A2 are the amplitudes of the two waves.

In this problem, the amplitude of the two waves is 1 cm each.

Therefore,

A = 1 + 1 + 2 * 1 * 1 * cos (1.36)

= 2 + 0.28

= 2.28 cm

Therefore, the height of the resultant wave formed by the interference of the two waves at the position x = 0.5 m at time t = 0.2 s is 1.14 cm.

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Q|C A firebox is at 750K , and the ambient temperature is 300K. The efficiency of a Carnot engine doing 150 J of work as it transports energy between these constant-temperature baths is 60.0%. The Carnot engine must take in energy 150 J 0.600=250 J from the hot reservoir and must put out 100 J of energy by heat into the environment. To follow Carnot's reasoning, suppose some other heat engine S could have an efficiency of 70.0%. (i) Let the engines operate together through one cycle as in part (d). Find the change in entropy of the Universe.

Answers

The change in entropy of the Universe is 0.667 J/K.

To find the energy input and work output of engine S as it puts out exhaust energy of 100 J, we can use the efficiency formula:

[tex]\[ \text{Efficiency} = \frac{\text{WO}}{\text{EI}} \times 100 \][/tex]

Given the efficiency of engine S is 70.0% and the exhaust energy output is 100 J, we can rearrange the formula to solve for the energy input:

[tex]\[ \text{EI} = \frac{\text{WO}}{\text{Efficiency}} \][/tex]

Substituting the given values:

[tex]\[ \text{EI} = \frac{100 \, \text{J}}{0.700} \]\\\\\ \text{EI} \approx 142.86 \, \text{J} \][/tex]

To find the work output, we multiply the energy input by the efficiency:

[tex]\[ \text{WO} = \text{WI} \times \text{Efficiency} \]\\\\\\ \text{WO} = 142.86 \, \text{J} \times 0.700 \]\\\\\ \text{WO} \approx 100 \, \text{J} \][/tex]

Therefore, the energy input of engine S is approximately 142.86 J and the work output is approximately 100 J.

(i) To find the change in entropy of the Universe, we can use the formula:

[tex]\[ \Delta S_{\text{Universe}} = \frac{\textEO}}{\text{Temperature of the cold reservoir}} \][/tex]

In this case, the energy output is the total energy transferred to the environment, which is 200 J, and the temperature of the cold reservoir is 300 K.

Substituting these values:

[tex]\[ \Delta S_{\text{Universe}} = \frac{200 \, \text{J}}{300 \, \text{K}} \]\\\\\ \Delta S_{\text{Universe}} = 0.667 \, \text{J/K} \][/tex]

Therefore, the change in entropy of the Universe is 0.667 J/K.

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three equal point charges, each with charge 1.00 μc , are placed at the vertices of an equilateral triangle whose sides are of length 0.700 m . what is the electric potential energy u of the system? (take as zero the potential energy of the three charges when they are infinitely far apart.)

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The electric potential energy of the system is approximately 38.64 Joules.

To calculate the electric potential energy (U) of the system, we can use the formula for the potential energy of a system of point charges:

U = k * (q₁ * q₂ / r₁₂ + q₁ * q₃ / r₁₃ + q₂ * q₃ / r₂₃)

Where:

U is the electric potential energy

k is the electrostatic constant (8.99 × [tex]10^9[/tex] N m²/C²)

q₁, q₂, q₃ are the charges

r₁₂, r₁₃, r₂₃ are the distances between the charges

Given:

Charge of each point charge (q₁ = q₂ = q₃) = 1.00 μC = 1.00 × [tex]10^-^6[/tex] C

Side length of the equilateral triangle (a) = 0.700 m

The distances between the charges can be calculated using the properties of an equilateral triangle:

r₁₂ = r₁₃ = r₂₃ = a

Now we can substitute the given values into the formula for electric potential energy:

U = (8.99 × [tex]10^9[/tex] N m²/C²) * [(1.00 × [tex]10^-^6[/tex] C)² / (0.700 m) + (1.00 × [tex]10^-^6[/tex] C)² / (0.700 m) + (1.00 × [tex]10^-^6[/tex] C)² / (0.700 m)]

Simplifying the expression:

U = (8.99 × [tex]10^9[/tex] N m²/C²) * [(1.00 ×[tex]10^-^6[/tex] C)² * 3 / (0.700 m)]

U = (8.99 × [tex]10^9[/tex] N m²/C²) * [(1.00 ×[tex]10^-^6[/tex] C)² * 3 / (0.700 m)]

U ≈ 38.64 J

Therefore, the electric potential energy of the system is approximately 38.64 Joules.

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The boiling point of liquid hydrogen is 20.3K at atmospheric pressure. What is this temperature on(a) the Celsius scale.

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The boiling point of liquid hydrogen is 20.3K at atmospheric pressure. To convert this temperature to the Celsius scale, we need to use the formula: Therefore, the temperature of liquid hydrogen at its boiling point on the Celsius scale is approximately -252.85°C.

°C = K - 273.15

Using this formula, we can calculate the temperature on the Celsius scale.

°C = 20.3K - 273.15

Simplifying the equation, we have:

°C = -252.85


It's important to note that this is a very low temperature. In fact, it is close to absolute zero, which is the coldest temperature possible. At this temperature, hydrogen exists in its liquid state, but it would rapidly turn into a gas if the pressure is released. Liquid hydrogen is commonly used as rocket fuel because it has a high energy density, which means it can provide a lot of power for its weight.

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