3.0 m/s Problem 2 (20 pts) Two masses are heading for a collision on a frictionless horizontal surface. Mass mi = 9.0 m/s 3.0 kg is moving to the right at initial speed 9.0 m/s, and m-3.0 kg m2=1.0 kg m2 = 1.0 kg is moving to the right at initial speed 3.0 m/s. (a) (10 pts) Suppose that after the collision, mass mi is moving with speed 7.0 m/s to the right. What will be the velocity of mass me? (b) (10 pts) Suppose instead that the two masses stick together after the collision. What would be their final velocity?

Answers

Answer 1

Therefore, after the collision, the final velocity of the combined masses is 8.4 m/s to the right. Therefore, the velocity of mass m after the collision is 21.0 m/s to the right.

To solve this problem, we can use the principle of conservation of momentum.

(a) In the given scenario, after the collision, mass m (9.0 kg) is moving with a speed of 7.0 m/s to the right. We need to determine the velocity of mass m.

Let's denote the velocity of mass m as v.

According to the conservation of momentum:

m × v + m × v = m ×  v + m × v

Since there is no external force acting on the system, the initial momentum is equal to the final momentum.

Given:

m = 9.0 kg

v= 9.0 m/s

v = 7.0 m/s

m = 1.0 kg

Substituting the values into the momentum conservation equation:

9.0 kg × 9.0 m/s + 1.0 kg × 3.0 m/s = 9.0 kg × 7.0 m/s + 1.0 kg × v

Simplifying the equation:

81.0 kg m/s + 3.0 kg m/s = 63.0 kg m/s + v

Combining like terms:

84.0 kg m/s = 63.0 kg m/s + v

Now, solving for v:

v= 84.0 kg m/s - 63.0 k m/s

v= 21.0 kg m/s

Therefore, the velocity of mass m after the collision is 21.0 m/s to the right.

(b) In this scenario, the two masses stick together after the collision. We need to find their final velocity.

Applying the conservation of momentum again:

m ×v + m × v= (m + m') ×v

Given the same values as in part (a), except v= 9.0 m/s and v = 3.0 m/s, we have:

9.0 kg ×9.0 m/s + 1.0 kg × 3.0 m/s = (9.0 kg + 1.0 kg) ×v

Simplifying the equation:

81.0 kg m/s + 3.0 kg m/s = 10.0 kg × v

Combining like terms:

84.0 kg m/s = 10.0 kg × v

Now, solving for v:

v= 84.0 kg m/s / 10.0 kg

v = 8.4 m/s

Therefore, after the collision, the final velocity of the combined masses is 8.4 m/s to the right.

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Related Questions

A car moving at 38 km/h negotiates a 160 m -radius banked turn
designed for 60 km/h. What coefficient of friction is needed to
keep the car on the road?

Answers

we need to find the value of What coefficient of friction is needed to keep the car on the road. The concepts we can use are centripetal force, gravity etc.

Given data:
The speed of the car v = 38 km/h

Radius of the turn r = 160 m

The turn is designed for the speed of the car v' = 60 km/h

The coefficient of friction between the tires and the road = μ

First, we convert the speed of the car into m/s.1 km/h = 0.27778 m/s

Therefore, 38 km/h = 38 × 0.27778 m/s = 10.56 m/s

Similarly, we convert the speed designed for the turn into m/s
60 km/h = 60 × 0.27778 m/s
60 km/h = 16.67 m/s

To keep the car on the road, the required centripetal force must be provided by the frictional force acting on the car. The maximum frictional force is given by μN, where N is the normal force acting on the car. To find N, we use the weight of the car, which is given by mg where m is the mass of the car and g is the acceleration due to gravity, which is 9.81 m/s². We assume that the car is traveling on a level road. So, N = mg. We can find the mass of the car from the centripetal force equation. The centripetal force acting on the car is given by F = mv²/r where m is the mass of the car, v is the velocity of the car, and r is the radius of the turn. We know that the required centripetal force is equal to the maximum frictional force that can be provided by the tires. Therefore,

F = μN

F = μmg

So,
mv²/r = μmg

m = μgr/v²

Now we can substitute the values in the above formula to calculate the required coefficient of friction.

μ = mv²/(gr)

μ = v²/(gr) × m = (10.56)²/(160 × 9.81)

μ = 0.205

So, the required coefficient of friction to keep the car on the road is μ = 0.205.

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The radius of curvature of a spherical concave mirror is 16.0 cm. Describe the image formed when a 20.0-cm-tall object is 11.0 cm from the mirror. What is the image distance da, measured in centimeters (cm)? dA cm What is the image height ha, measured in centimeters (cm)? ha = cm The image is and Describe the image formed when a 20.0-cm-tall object is 16.0 cm from the mirror. What is the image distance dp, measured in centimeters (cm)? dB = cm What is the image height hp, measured in centimeters (cm)? hB cm The image is and dB = cm What is the image height hs, measured in centimeters (cm)? hв = cm The image is and Describe the image formed when a 20.0-cm-tall object is 100 cm from the mirror. What is the image distance dc, measured in centimeters (cm)? de = cm What is the image height hc, measured in centimeters (cm)? hc = cm The image is and

Answers

The image is and  the image formed when a 20.0-cm-tall object is 100 cm from the mirror.  3.4 cm. The image formed is virtual (since dc is negative), upright, and smaller than the object.

To analyze the image formed by a spherical concave mirror, we can use the mirror equation and magnification formula.

The mirror equation is given by:

1/f = 1/do + 1/di,

where f is the focal length of the mirror, do is the object distance (distance of the object from the mirror), and di is the image distance (distance of the image from the mirror).

The magnification formula is given by:

m = -di/do,

where m is the magnification of the mirror.

Let's go through each scenario step by step:

1. When the object is 11.0 cm from the mirror:

  - Given: do = -11.0 cm (negative sign indicates object is in front of the mirror), f = -16.0 cm (since it's a concave mirror).

  - Using the mirror equation, we can calculate the image distance (di):

    1/f = 1/do + 1/di

    1/-16.0 = 1/-11.0 + 1/di

    di = -33.3 cm (rounded to one decimal place).

  - Using the magnification formula, we can calculate the magnification (m):

    m = -di/do

    m = -(-33.3)/(-11.0)

    m = 3.03 (rounded to two decimal places).

  - The image distance (da) is -33.3 cm, and the image height (ha) can be determined using the magnification:

    ha = m * object height = 3.03 * 20.0 cm = 60.6 cm.

  - The image formed is virtual (since di is negative), upright, and larger than the object.

2. When the object is 16.0 cm from the mirror:

  - Given: do = -16.0 cm, f = -16.0 cm.

  - Using the mirror equation, we can calculate the image distance (dp):

    1/f = 1/do + 1/dp

    1/-16.0 = 1/-16.0 + 1/dp

    dp = -16.0 cm.

  - Using the magnification formula, we can calculate the magnification (m):

    m = -dp/do

    m = -(-16.0)/(-16.0)

    m = 1.

  - The image distance (dp) is -16.0 cm, and the image height (hp) can be determined using the magnification:

    hp = m * object height = 1 * 20.0 cm = 20.0 cm.

  - The image formed is real (since dp is positive), inverted, and the same size as the object.

3. When the object is 100 cm from the mirror:

  - Given: do = -100 cm, f = -16.0 cm.

  - Using the mirror equation, we can calculate the image distance (dc):

    1/f = 1/do + 1/dc

    1/-16.0 = 1/-100 + 1/dc

    dc = -16.7 cm (rounded to one decimal place).

  - Using the magnification formula, we can calculate the magnification (m):

    m = -dc/do

    m = -(-16.7)/(-100)

    m = 0.17 (rounded to two decimal places).

  - The image distance (dc) is -16.7 cm, and the image height (hc) can be determined using the magnification:

    hc = m * object height = 0.17 * 20.0 cm =  3.4 cm.

The image formed is virtual (since dc is negative), upright, and smaller than the object.

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The "middle C" note of a piano, which has a fundamental frequency of 256 Hz, is generated when a "hammer" inside the piano strikes a string with a length of 0.8 m. (a) Assuming the tension is the same in all of the strings in the piano, what is the length of the string that produces the "A above middle C" tone with a fundamental frequency of 440 Hz? LA = Number Units (b) What are the frequencies of the first three overtones on the "A above middle C" string? List them in ascending order.

Answers

The length of the string that produces the "A above middle C" tone with a fundamental frequency of 440 Hz is 0.667 m. The frequencies of the first three overtones on the "A above middle C" string are 880 Hz, 1320 Hz, and 1760 Hz.

The fundamental frequency of a vibrating string is inversely proportional to its length. This means that a string with half the length will have twice the fundamental frequency.

The middle C string has a fundamental frequency of 256 Hz and a length of 0.8 m. The A above middle C string has a fundamental frequency of 440 Hz. Therefore, the length of the A above middle C string must be half the length of the middle C string, or 0.667 m.

The overtones of a vibrating string are multiples of the fundamental frequency. The first three overtones of the A above middle C string are 2 * 440 Hz = 880 Hz, 3 * 440 Hz = 1320 Hz, and 4 * 440 Hz = 1760 Hz.

Here is the calculation for the length of the A above middle C string:

LA = Lc / 2

where LA is the length of the A above middle C string, Lc is the length of the middle C string, and 2 is the factor by which the length of the string is reduced to double the fundamental frequency.

Substituting in the known values, we get:

LA = 0.8 m / 2 = 0.667 m

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Problem 1 (Context-rich Problem) You have a vertical spring with constant k, which is initially neither stretched nor compressed. You attach an apple (mass m) to the spring and release it from rest at t = 0. The apple moves downward, and then comes to rest momentarily at t = ty after falling some distance. Determine the distance the apple has fallen. Bonus sensemaking opportunity for extra credit: Find the location where the net force on the apple is zero. Is it the same as the location you found in the problem? Comment on what is happening to the apple as it falls. Problem 2 (Explanation Task) Two objects exert a (conservative) force on each other that is repulsive - for example, the force on object 1 from object 2 points away from object 2. If the two objects move toward each other. does the potential energy of the two objects increase, decrease, or stay the same?

Answers

The potential energy of the spring also increases as the spring stretches. At a certain point, the upward force of the spring becomes equal to the downward force of gravity, and the apple comes to rest momentarily. The potential energy function for this force is given by: where U(r) is the potential energy of the system of two objects.

Problem 1: A vertical spring with constant k has neither stretched nor compressed initially. An apple of mass m is attached to the spring, and it is released from rest at t = 0. So, it is given as: By using Newton’s Second Law of Motion, we get: Where g is the acceleration due to gravity. Hence, the net force acting on the apple at any instant of time is given as: By using the law of conservation of mechanical energy, we can write: where V is the potential energy of the spring, U is the potential energy of the apple due to its height above the reference point, and K is the kinetic energy of the apple.  So, y = 0 and V = 0. At t = ty, the apple comes to rest momentarily. So, the final velocity of the apple (vf) is zero.

Problem 2: Two objects exert a conservative force on each other that is repulsive. The force on object 1 from object 2 points away from object. This force is a conservative force because it is a function of the relative positions of the two objects, and it can be derived from a potential energy function.  When the two objects move towards each other, their separation distance decreases, i.e., r decreases. As r decreases, U(r) increases.

Therefore, the potential energy of the two objects increases as they move towards each other. The potential energy of the spring is given by: where y is the displacement of the spring from its equilibrium position and k is the spring constant. Initially, the spring is neither stretched nor compressed.

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A superconducting solenoid with 2000 turns/m is meant to generate a magnetic field of 12.0 T. Calculate the current required. KA (+ 0.02 kA)

Answers

The current required to generate a magnetic field of 12.0 T in a superconducting solenoid with 2000 turns/m is approximately 6.0 kA.

To calculate the current, we can use Ampere's Law, which states that the magnetic field (B) inside a solenoid is directly proportional to the product of the current (I) and the number of turns per unit length (N).

B = μ₀ * N * I

where μ₀ is the permeability of free space (4π × 10⁻⁷ T·m/A).

Rearranging the equation to solve for current (I):

I = B / (μ₀ * N)

Plugging in the given values:

I = 12.0 T / (4π × 10⁻⁷ T·m/A * 2000 turns/m)

I ≈ 6.0 kA

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A 4 mm high object is placed 5 cm in front of a concave mirror with radius of curvature 20 cm. Questions 13-15 refer to this situation. The image distance is: Greater than 15 cm Between 15 cm and zero Between 0 and 15 cm Less than −15 cm A 4 mm high object is placed 5 cm in front of a concave mirror with radius of curvature 20 cm. Questions 13−15 refer to this situation. The magnitude of the image height will be: Between 3 and 6 mm Between 6 and 9 mm Greater than 9 mm Less than 3 mm

Answers

The magnitude of the image height will be between 3 and 6 mm.

Thus, the correct option is Between 3 and 6 mm.

Radius of curvature of concave mirror = -20 cmObject distance, u = -5 cmObject height, h = 4 mmFor concave mirror, f = -10 cm, as f = R/2Where R is the radius of curvatureThe focal length of a concave mirror is negative, which means the mirror is concave and reflects the incoming light rays inward toward a focal point.Use the formula,1/f = 1/v + 1/uHere, v = ?1/-10 = 1/v + 1/-5⇒ -1/10 = 1/v - 1/5⇒ 1/v = -1/20⇒ v = -20 cm.

The image distance is -20 cm.Now, using the magnification formula,m = -v/u = -(-20)/(-5) = -4m = -v/uThe negative sign indicates that the image is inverted. The magnitude of the image height will be between 3 and 6 mm.Thus, the correct option is Between 3 and 6 mm.

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4. a. An electron in a hydrogen atom falls from an initial energy level of n = 4 to a final level of n = 2. Find the energy, frequency, and wavelength of the photon that will be emitted for this sequence [For hydrogen: En=-13.6 eV/n?] b. A photon of energy 2.794 eV is absorbed by a hydrogen atom, causing its electron to be released with a kinetic energy of 2.250 eV. In what energy level was the electron? c. Find the wavelength of the matter wave associated with a proton moving at a speed of 150 m/s.

Answers

a. To find the energy, frequency, and wavelength of the photon emitted when an electron falls from n = 4 to n = 2 in a hydrogen atom, we can use the formula:

ΔE = -13.6 eV * [(1/n_f²) - (1/n_i²)],

where ΔE is the change in energy, n_f is the final energy level, and n_i is the initial energy level. Plugging in the values, we have:

ΔE = -13.6 eV * [(1/2²) - (1/4²)]

    = -13.6 eV * [1/4 - 1/16]

    = -13.6 eV * (3/16)

    = -2.55 eV.

The energy of the photon emitted is equal to the absolute value of ΔE, so it is 2.55 eV.

To find the frequency of the photon, we can use the equation:

ΔE = hf,

where h is Planck's constant (4.1357 × 10⁻¹⁵ eV·s). Rearranging the equation, we have:

f = ΔE / h

  = 2.55 eV / (4.1357 × 10⁻¹⁵ eV·s)

  ≈ 6.16 × 10¹⁴ Hz.

The frequency of the photon emitted is approximately 6.16 × 10¹⁴ Hz.

To find the wavelength of the photon, we can use the equation:

c = λf,

where c is the speed of light (2.998 × 10⁸ m/s) and λ is the wavelength. Rearranging the equation, we have:

λ = c / f

  = (2.998 × 10⁸ m/s) / (6.16 × 10¹⁴ Hz)

  ≈ 4.87 × 10⁻⁷ m.

The wavelength of the photon emitted is approximately 4.87 × 10⁻⁷ meters.

b. To determine the energy level of the electron in a hydrogen atom when a photon of energy 2.794 eV is absorbed, causing the electron to be released with a kinetic energy of 2.250 eV, we can use the formula:

ΔE = E_f - E_i,

where ΔE is the change in energy, E_f is the final energy level, and E_i is the initial energy level. Plugging in the values, we have:

ΔE = 2.794 eV - 2.250 eV

    = 0.544 eV.

Since the energy of the photon absorbed is equal to the change in energy, the electron was in an energy level of 0.544 eV.

c. To find the wavelength of the matter wave associated with a proton moving at a speed of 150 m/s, we can use the de Broglie wavelength formula:

λ = h / p,

where λ is the wavelength, h is Planck's constant (6.626 × 10⁻³⁴ J·s), and p is the momentum of the proton. The momentum can be calculated using the equation:

p = m * v,

where m is the mass of the proton (1.67 × 10⁻²⁷ kg) and v is the velocity. Plugging in the values, we have:

p = (1.67 × 10⁻²⁷ kg) * (150 m/s)

  = 2.505 × 10⁻²⁵ kg·m/s.

Now we can calculate the wavelength:

λ = (6.626 × 10⁻³⁴ J·s) / (2

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Light with a wavelength of 655 nm (6.55 x 10-7 m) is incident upon a double slit with a separation of 0.9 mm (9 x 104 m). A screen is location 2.5 m from the double slit. (a) At what distance from the center of the screen will the first bright fringe beyond the center fringe appear?

Answers

The distance of the first bright fringe from the center of the screen is 1.81 × 10⁻³ m.

Given Datalight with wavelength λ = 655 nm = 6.55 x 10⁻⁷ m

Distance between double slit = d = 0.9 mm = 9 x 10⁻⁴ m

Distance of screen from the double slit = D = 2.5 m

Formula to find the position of mth bright fringe on the screen

ym=msinθ=(mλ)/dθ= (mλ)/dsinθ

For the first bright fringe, m = 1θ = sin⁻¹(y/D)

Now putting the values in the above formula, we get the distance of the first bright fringe from the center of the screen.

y_1= (1 × 6.55 × 10⁻⁷)/0.9sin(sin⁻¹(y/D))

y_1= (6.55 × 10⁻⁷)/0.9 × (9 × 10⁻⁴)/2.5

y_1= (6.55 × 10⁻⁷ × 2.5)/(0.9 × 9 × 10⁻⁴)

y_1= 1.81 × 10⁻³ m

Hence, the distance of the first bright fringe from the center of the screen is 1.81 × 10⁻³ m.

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In a region of space, a quantum particle with zero total energy has a wave functionψ(x) = Axe⁻ˣ²/L²

(b) Make a sketch of U(x) versus x .

Answers

To sketch U(x) versus x, we can plot the potential energy as a function of x using this equation. Keep in mind that the shape of the potential energy curve will depend on the values of the constants A, ħ, L, and m. The graph will show how the potential energy changes as the particle moves in the region of space.

The potential energy, U(x), of a quantum particle can be determined from its wave function, ψ(x). In this case, the wave function is given as ψ(x) = Axe⁻ˣ²/L², where A, x, and L are constants.

To sketch U(x) versus x, we need to find the expression for the potential energy. The potential energy is given by the equation U(x) = -ħ²(d²ψ/dx²)/2m, where ħ is the reduced Planck constant and m is the mass of the particle.

First, we need to find the second derivative of ψ(x). Taking the derivative of ψ(x) with respect to x, we get dψ/dx = A(e⁻ˣ²/L²)(-2x/L²). Taking the derivative again, we get [tex]d²ψ/dx² = A(e⁻ˣ²/L²)(4x²/L⁴ - 2/L²).[/tex]

Now, we can substitute the expression for the second derivative into the equation for the potential energy.

U(x) = -ħ²(d²ψ/dx²)/2m

= -ħ²A(e⁻ˣ²/L²)(4x²/L⁴ - 2/L²)/2m.

Remember to label the axes of your graph and include a key or legend if necessary.

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1. Two lenses are placed along the x axis, with a diverging lens of focal length −7.70
cm on the left and a converging lens of focal length 17.0 cm on the right. When an object is placed 12.0 cm to the left of the diverging lens, what should the separation s of the two lenses be if the final image is to be focused at
x = [infinity]?
cm
2) An object has a height of 0.052 m and is held 0.230 m in front of a converging lens with a focal length of 0.140 m. (Include the sign of the value in your answers.)
(a) What is the magnification?
(b) What is the image height?
m

Answers

The magnification is 0.61. The image height is 0.0317 m, indicating that the image is smaller than the object's height.

To determine the separation s between the lenses, we can use the lens formula:

1/f_total = 1/f1 - 1/f2

where f_total is the effective focal length of the combination of lenses, f1 is the focal length of the diverging lens, and f2 is the focal length of the converging lens.

Plugging in the values, we have:

1/f_total = 1/-7.70 - 1/17.0

Solving for f_total, we get:

f_total = -26.7 cm

Since the final image is to be focused at x = infinity, the lenses need to be positioned such that the combined focal length is -26.7 cm. Therefore, the separation s between the lenses should also be 26.7 cm.

(a) The magnification (m) of an image formed by a lens is given by the formula:

m = -i/o

where i is the image distance and o is the object distance. The negative sign indicates that the image is inverted.

Plugging in the values, we have:

m = -(-0.140 m)/(0.230 m) = 0.61

Therefore, the magnification is 0.61, indicating that the image is reduced in size.

(b) The image height (h') can be calculated using the magnification formula:

h' = m * h

where h is the object height.

Plugging in the values, we have:

h' = 0.61 * 0.052 m = 0.0317 m

Therefore, the image height is 0.0317 m, indicating that the image is smaller than the object's height.

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A 688.78 mm long aluminum wire with a diameter of 41.4 mm changes temperature from 131.6 C to 253.3 C. Calculate the change in length of the wire due to the temperature change. Report your answer in millimeters rounded to 3 decimal places with units.

Answers

We know that the coefficient of linear expansion of aluminum, α = 23.1 x 10-6 K-1 Hence,∆L = αL∆T= 23.1 × 10-6 × 688.78 × (253.3 − 131.6)= 4.655 mmThus, the change in length of the wire due to the temperature change is 4.655 mm (rounded to 3 decimal places with u

The length change of an aluminum wire with a diameter of 41.4 mm and 688.78 mm length from a temperature change from 131.6 C to 253.3 C is 4.655 mm. The formula that is used to calculate the change in length of the wire due to temperature change is:∆L

= αL∆T

where, ∆L is the change in length L is the original length of the wireα is the coefficient of linear expansion of the material of the wire∆T is the change in temperature From the provided data, we know the following:Length of the aluminum wire

= 688.78 mm Diameter of the aluminum wire

= 41.4 mm Radius of the aluminum wire

= Diameter/2

= 41.4/2

= 20.7 mm Initial temperature of the aluminum wire

= 131.6 C Final temperature of the aluminum wire

= 253.3 C

We first need to find the coefficient of linear expansion of aluminum. From the formula,α

= ∆L/L∆T We know that the change in length, ∆L

= ?L = 688.78 mm (given)We know that the initial temperature, T1

= 131.6 C

We know that the final temperature, T2

= 253.3 C.We know that the coefficient of linear expansion of aluminum, α

= 23.1 x 10-6 K-1 Hence,∆L

= αL∆T

= 23.1 × 10-6 × 688.78 × (253.3 − 131.6)

= 4.655 mm Thus, the change in length of the wire due to the temperature change is 4.655 mm (rounded to 3 decimal places with units).

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What is the critical angle for light going from ethanol to air? Submit Answer Incorrect. Tries 1/40 Previous Tries

Answers

The critical angle for light going from ethanol to air the critical angle for light going from ethanol to air is approximately 48.6 degrees.

To calculate the critical angle for light going from ethanol to air, we need to use Snell's law, which relates the angles of incidence and refraction for light traveling between two different media. Snell's law is given by:

n₁ * sin(θ₁) = n₂ * sin(θ₂)

Where:

n₁ is the refractive index of the initial medium (ethanol)

n₂ is the refractive index of the final medium (air)

θ₁ is the angle of incidence

θ₂ is the angle of refraction

The critical angle occurs when the angle of refraction is 90 degrees (light travels along the boundary). So we can rewrite Snell's law as:

n₁ * sin(θ_c) = n₂ * sin(90)

Since sin(90) = 1, the equation simplifies to:

n₁ * sin(θ_c) = n₂

To find the critical angle (θ_c), we need to know the refractive indices of ethanol and air. The refractive index of ethanol (n₁) is approximately 1.36, and the refractive index of air (n₂) is approximately 1.

Plugging in the values, we get:

1.36 * sin(θ_c) = 1

Now, we can solve for the critical angle:

sin(θ_c) = 1 / 1.36

θ_c = arcsin(1 / 1.36)

Using a calculator, we find:

θ_c ≈ 48.6 degrees

Therefore, the critical angle for light going from ethanol to air is approximately 48.6 degrees.

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A group of astronauts wish to know the gravitational acceleration of a newly discovered planet. On the surface of the planet, they construct a simple pendulum of length 21.0 m. The pendulum yields a 18.7 s period of oscillation. Part 1 Find the gravitational acceleration of the planet. Part 2 How much stronger is earth's gravitational acceleration compared to this planet?

Answers

The gravitational acceleration on Earth is 4.56 times stronger than the newly discovered planet and 2) the gravitational acceleration of the newly discovered planet is 2.15 m/s².

Part 1- The time period of a simple pendulum is given by the following formula:

T=2π√(L/g) where T is the time period, L is the length of the pendulum and g is the gravitational acceleration.

Let g1 be the gravitational acceleration of the newly discovered planet.

We know that the length of the pendulum is L= 21.0 m and the time period of oscillation of the pendulum is T= 18.7s.

Substituting these values in the formula, we get:

18.7=2π√(21.0/g1)

Squaring both sides of the equation, we get:

g1=(4π²×21.0)/18.7² = 2.15 m/s²

Therefore, the gravitational acceleration of the newly discovered planet is 2.15 m/s².



Part 2- Let g2 be the gravitational acceleration of Earth.

The acceleration due to gravity on the surface of the Earth is g2 = 9.81 m/s².

Comparing the gravitational acceleration of Earth to that of the newly discovered planet, we have:

The ratio of the gravitational acceleration of Earth to that of the newly discovered planet = g2/g1

= 9.81 m/s²/2.15 m/s² = 4.56

Therefore, the gravitational acceleration on Earth is 4.56 times stronger than the newly discovered planet.

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The electric field E in a given region is described by E - Eo a, where a, is the unit vector along x-direction. The potential difference VAB between 2 points A and B located at A(x-d) and B(x-0) is given by: (a) VAB= Eod (b) VAB= -Eod (c) VAB= 0
The uniform plane wave in a non-magnetic medium has an electric field component: E-10 cos (2x10 t-2z) a, V/m. The wave propagation constant k and wavelength λ are given by: (a) π.2 (b) 2, π
(c) 2X10³, (d), 2X10^8

Answers

in summary, For the first question, the potential difference VAB between points A and B in the given region is VAB = -Eo d. Therefore, the correct answer is (b) VAB = -Eo d. For the second question, the wave propagation constant k and wavelength λ are related by the equation k = 2π/λ. Since the given wave has a wave number of 10, the wavelength can be calculated as λ = 2π/10 = π/5. Hence, the correct answer is (b) 2, π.

1.In the given scenario, the electric field E is given as E = Eo a, where a is the unit vector along the x-direction. To find the potential difference VAB between two points A and B located at A(x - d) and B(x - 0), we need to integrate the electric field over the distance between A and B. Since the electric field is constant, the integration simply results in the product of the electric field and the distance (Eo * d). Therefore, the potential difference VAB is given by VAB = Eo * d. Hence, the correct answer is (a) VAB = Eo * d.

2.In the case of the uniform plane wave with an electric field component E = 10 cos(2x10 t - 2z) a V/m, we can observe that the wave is propagating in the z-direction. The wave propagation constant k is determined by the coefficient in front of the z variable, which is 2 in this case. The wavelength λ is given by the formula λ = 2π/k. Substituting the value of k as 2, we find that λ = 2π/2 = π. Hence, the correct answer is (b) 2, π, where the wave propagation constant k is 2 and the wavelength λ is π.

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An electron moves with velocity (2 i^ )m/s through a uniform magnetic field equal to (−5 k^ )T. The magnetic force in Newton acting on the electron is:

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The velocity of the electron = (2i^)m/s. The magnetic field = (−5k^)T. We have to determine the magnetic force in Newton acting on the electron.  

The magnetic force acting on a charged particle that moves through a magnetic field is given by the formula:F = qvB sinθWhereq is the charge of the is the velocity of the particle B is the magnetic field strength of the magnetic fieldθ is the angle between the velocity of the particle and the magnetic field.

Direction of Magnetic Force: To determine the direction of the magnetic force on a moving charge, we use Fleming’s left-hand rule. Fleming's Left-hand Rule: Stretch out the left-hand forefinger, the central finger, and the thumb mutually perpendicular to each other.  

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An electron enters a magnetic field of magnitude 13 T with a speed of 7.2 x 10 m/s. The angle between the magnetic field and the electron's velocity is 35 a) If the direction of the magnetic field is pointing from right to left on a horizontal plane, with the aid of a diagram show the direction of the magnetic force applied on the electron ( ) b) Find the magnitude of the magnetic force and the acceleration of the electron

Answers

a) The direction of the magnetic force applied on the electron is upward, perpendicular to both the velocity and the magnetic field,b) The magnitude of the magnetic force on the electron is 1.94 x [tex]10^-17[/tex] N, and the acceleration of the electron is 2.69 x [tex]10^15 m/s^2.[/tex]

a) According to the right-hand rule, when a charged particle moves in a magnetic field, the direction of the magnetic force can be determined by aligning the right-hand thumb with the velocity vector and the fingers with the magnetic field direction.

In this case, with the magnetic field pointing from right to left, and the electron's velocity pointing towards us (out of the page), the magnetic force on the electron is directed upward, perpendicular to both the velocity and the magnetic field.

b) The magnitude of the magnetic force on the electron can be calculated using the equation:

F = qvBsinθ

where F is the magnetic force, q is the charge of the electron, v is the velocity, B is the magnetic field magnitude, and θ is the angle between the velocity and the magnetic field. Plugging in the given values, we find that the magnitude of the magnetic force is 1.94 x [tex]10^-17[/tex] N.

The acceleration of the electron can be obtained using Newton's second law:

F = ma

Rearranging the equation, we have:

a = F/m

where a is the acceleration and m is the mass of the electron. The mass of an electron is approximately 9.11 x [tex]10^-31[/tex]kg.

Substituting the values, we find that the acceleration of the electron is 2.69 x [tex]10^15 m/s^2.[/tex]

Therefore, the magnetic force applied on the electron is upward, perpendicular to the velocity and the magnetic field.

The magnitude of the magnetic force is 1.94 x [tex]10^-17[/tex] N, and the acceleration of the electron is 2.69 x[tex]10^15 m/s^2.[/tex]

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Electric (or magnetic) field lines
Select one or more than one:
a. They are more concentrated where the field is stronger
b. They are more numerous if there is more charge (or stronger poles)
c. They are less numerous if there is more charge (or stronger poles)
d. They cross where an electric charge is (or where a pole is) and. They do not indicate the direction of the force that would affect positive charge
F. Indicate the direction of the force that would affect positive charge
g. They don't cross where an electric charge is (or where a pole is)
h. They do not cross in the space between one electric charge and another (or between one magnet and another)
i. They cross in the space between one electric charge and another (or between one magnet and another)
J. They are more spread out where the field is stronger

Answers

The Electric field lines have the following properties :

a. They are more concentrated where the field is stronger.

b. They are more numerous if there is more charge (or stronger poles).

d. They cross where an electric charge is (or where a pole is) and. They do not indicate the direction of the force that would affect positive charge.

f. Indicate the direction of the force that would affect positive charge.

g. They don't cross where an electric charge is (or where a pole is).h. They do not cross in the space between one electric charge and another (or between one magnet and another).Therefore, the correct options are:

a. They are more concentrated where the field is stronger.

b. They are more numerous if there is more charge (or stronger poles).

d. They cross where an electric charge is (or where a pole is) and. They do not indicate the direction of the force that would affect positive charge.

f. Indicate the direction of the force that would affect positive charge.

g. They don't cross where an electric charge is (or where a pole is).

h. They do not cross in the space between one electric charge and another (or between one magnet and another).

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A 180 ohm resistor can dissipate a maximum power of .250W. Calculate the maximum current that it can carry and still meet this limitation.

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As 180-ohm resistor can dissipate a maximum power of .250W The maximum current that can pass through the resistor while meeting the power limit is 0.027 A which can be obtained by the formula P = I²R

The resistance of the resistor, R = 180 Ω. The maximum power dissipated by the resistor, P = 0.250 W. We need to find the maximum current that can be passed through the resistor while maintaining the power limit. The maximum power that can be dissipated by the resistor is given by the formula;

P = I²R …………… (1)

Where; P = Power in watts, I = Current in amperes, and R = Resistance in ohms.

Rewriting the above equation, we get,

I = √(P / R) ………… (2)

Substitute the given values into the equation 2 and solve for the current,

I = √(0.250 / 180)

⇒I = 0.027 A

The maximum current that can pass through the resistor while meeting the power limit is 0.027 A.

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The diameter of an oxygen (02) molecule is approximately 0.300 nm.
For an oxygen molecule in air at atmospheric pressure and 18.3°C, estimate the total distance traveled during a 1.00-s time interval.

Answers

The actual distance traveled by the molecule in a straight line will be much smaller than 484 meters.

The mean free path of a gas molecule is the average distance it travels between collisions with other molecules. At atmospheric pressure and 18.3°C, the mean free path of an oxygen molecule is approximately 6.7 nm.

During a 1.00-s time interval, an oxygen molecule will travel a distance equal to the product of its speed and the time interval. The speed of an oxygen molecule at atmospheric pressure and 18.3°C can be estimated using the root-mean-square speed equation:

[tex]v_{rms}[/tex] = √(3kT/m)

where k is Boltzmann's constant, T is the temperature in Kelvin, and m is the mass of the molecule.

For an oxygen molecule, [tex]k = 1.38 * 10^{-23}[/tex] J/K, T = 291.45 K (18.3°C + 273.15), and [tex]m = 5.31 * 10^{-26}[/tex] kg.

Plugging in the values, we get:

[tex]v_{rms} = \sqrt {(3 * 1.38 * 10^{-23} J/K * 291.45 K / 5.31 * 10^{-26} kg)} = 484 m/s[/tex]

Therefore, during a 1.00-s time interval, an oxygen molecule will travel approximately:

distance = speed * time = 484 m/s * 1.00 s ≈ 484 meters

However, we need to take into account that the oxygen molecule will collide with other molecules in the air, and its direction will change randomly after each collision. The actual distance traveled by the molecule in a straight line will be much smaller than 484 meters, and will depend on the number of collisions it experiences during the time interval. Therefore, the estimate of the total distance traveled by an oxygen molecule in air during a 1.00-s time interval should be considered a very rough approximation.

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Two positive charges, one with twice the charge of the other, are moved through an electric field and gain the same amount of electrical potential energy. Were the charges moved in the same direction as the electric field or in the opposite direction? The charges began at the same location. Do they have the same end point? If so, why? If not, which one was moved farther and how can you tell?

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Two positive charges, one with twice the charge of the other, are moved through an electric field and gain the same amount of electrical potential energy. They were moved in the opposite direction of the electric field, because the positive charges (protons) are drawn toward the lower electrical potential energy and repelled from the higher electrical potential energy.

It follows that moving them in the opposite direction of the electric field ensures they gain the same electrical potential energy (EPE) when the work done by the electric field is the same for both particles. They do have the same end point, and this is because the electric potential energy does not depend on the path taken by the charged particles in the field but on the starting and end points in the field.

Therefore, it doesn't matter if one particle was moved farther than the other because the EPE of a charge only depends on its starting and ending locations and is entirely independent of the path taken between the two locations.

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Consider the circuit shown in (Figure 1). Suppose that R = 5.0 kΩ? What is the time constant for the discharge of the capacitor? 1 microFarad = C

Answers

The time constant for the discharge of the capacitor in the given circuit is 5.0 milliseconds (ms).

To determine the time constant for the discharge of the capacitor in the given circuit, we can use the formula: Time constant (τ) = R * C

Given that R = 5.0 kΩ (kiloohms) and C = 1 microFarad (μF), we need to ensure that the units are consistent. Since the time constant is typically expressed in seconds (s), we need to convert kiloohms to ohms and microFarads to Farads. 1 kiloohm (kΩ) = 1000 ohms (Ω)

1 microFarad (μF) = 1 x 10^(-6) Farads (F)

Substituting the converted values into the formula, we have:
Time constant (τ) = (5.0 kΩ) * (1 x 10^(-6) F) = 5.0 x 10^(-3) s
Therefore, the time constant for the discharge of the capacitor in the given circuit is 5.0 milliseconds (ms).

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(e) Why is the minimisation of internal resistance important for battery design? Discuss some of the factors that contribute to internal resistance and what steps manufacturers are taken to minimise this effect in batteries for electric vehicles.

Answers

The minimization of internal resistance is crucial for battery design due to the following reasons:

Efficiency: Internal resistance leads to energy losses within the battery.

Power Delivery: Internal resistance affects the battery's ability to deliver power quickly.

Factors contributing to internal resistance in batteries include:

Electrode Resistance: The intrinsic properties of electrode materials and their interfaces contribute to resistance. Manufacturers optimize electrode materials and structures to reduce their inherent resistance and enhance charge transfer efficiency.

Electrolyte Resistance: The electrolyte, which facilitates ion movement between electrodes, adds to internal resistance.

Separator Resistance: The separator material between the positive and negative electrodes can introduce resistance to ion flow.

Steps taken by manufacturers to minimize internal resistance in batteries for electric vehicles:

Material Optimization: Manufacturers explore electrode materials with high electrical conductivity and optimize their structures to enhance charge transfer efficiency.

Electrolyte Improvements: Advanced electrolytes with higher ionic conductivity are developed to reduce resistance.

Interface Enhancements: Manufacturers work on improving the electrode-electrolyte interface to reduce resistance.

Separator Optimization: Manufacturers choose separator materials with low resistance, ensuring efficient ion flow.

Cell Design: Optimizing cell geometry, electrode thickness, and overall architecture helps reduce internal resistance and improve battery performance.

By addressing these factors and employing advanced materials and design techniques, manufacturers minimize internal resistance, resulting in improved battery efficiency, power delivery, and overall performance in electric vehicles.

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One of the fundamental forces of nature is the strong nuclear force. This force is responsible for a) Keeping electrons from falling into the nucleus b) Keeping the particles in the nucleus together c) Transforming particles via radioactive decay d) Sticking atoms together to form molecules

Answers

The strong nuclear force is responsible for keeping the particles in the nucleus together. So the answer is b. The strong nuclear force is the strongest of the four fundamental forces of nature.

The strong nuclear force is the strongest of the four fundamental forces of nature. It is responsible for holding the protons and neutrons in the nucleus of an atom together. The strong nuclear force is much stronger than the electromagnetic force, which is responsible for holding electrons in orbit around the nucleus.

The strong nuclear force is a short-range force, which means that it only works over very small distances. This is why the protons and neutrons in the nucleus are able to stay together, even though they are positively charged and repel each other.

The strong nuclear force is also a very attractive force, which means that it pulls the protons and neutrons together very strongly. This is why the nucleus is so stable.

The other three fundamental forces of nature are the electromagnetic force, the weak nuclear force, and gravity. The electromagnetic force is responsible for holding electrons in orbit around the nucleus, as well as for many other phenomena, such as magnetism and light. The weak nuclear force is responsible for radioactive decay, and gravity is responsible for the attraction between objects with mass.

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17). If you were to live another 65 years and there was a starship ready to go right now, how fast would it have to be going for you to live long enough to get to the galactic center (30,000 1.y.)? How fast would you have to go to reach the Andromeda Galaxy (2.54 million 1.y.)? 18). A friend tells you that we should ignore claims of climate change on Earth, because the scientists making such claims are simply relying on their authority as scientists (argument from authority) to support their claims. What are the problems with your friend's claim? This friend is far from alone... 19). To get a de Broglie wave that is visible to human eyes (size-wise, not visibility-wise, so 1 > 0,1 mm), of an particle, what particle should it be and what is the greatest speed it can be moving?

Answers

17) The required speed to reach the galactic center or the Andromeda Galaxy is obtained by dividing the distance by the time.

18) Dismissing scientific claims solely based on authority (argument from authority) overlooks the rigorous scientific process and the wealth of evidence supporting claims like climate change.

19) Achieving a visible-sized de Broglie wave would require a particle with low mass (e.g., an electron) to approach speeds near the speed of light, which is currently not attainable.

17) To calculate the speed required to reach the galactic center or the Andromeda Galaxy within a given time frame, we can use the equation:

Speed = Distance / Time

For the galactic center:

Distance = 30,000 light-years = 30,000 * 9.461 × 10^15 meters (approx.)

Time = 65 years = 65 * 365 * 24 * 3600 seconds (approx.)

Speed = (30,000 * 9.461 × 10^15 meters) / (65 * 365 * 24 * 3600 seconds)

Calculating this value gives the required speed in meters per second.

For the Andromeda Galaxy:

Distance = 2.54 million light-years = 2.54 million * 9.461 × 10^15 meters (approx.)

Time = 65 years = 65 * 365 * 24 * 3600 seconds (approx.)

Speed = (2.54 million * 9.461 × 10^15 meters) / (65 * 365 * 24 * 3600 seconds)

Calculating this value gives the required speed in meters per second.

18) The claim made by your friend that scientists are simply relying on their authority as scientists (argument from authority) to support claims of climate change on Earth has several problems. Firstly, it is a logical fallacy to dismiss scientific claims solely based on the authority of the scientists making them. Scientific claims should be evaluated based on the evidence, data, and rigorous research methods used to support them.

Furthermore, the consensus on climate change is not solely based on the authority of individual scientists but is the result of extensive research, data analysis, and peer review within the scientific community. There is a wealth of scientific evidence supporting the existence and impact of climate change, including observed temperature increases, melting glaciers, and changing weather patterns. Ignoring or dismissing these claims without proper scientific analysis undermines the importance of scientific consensus and the rigorous process of scientific inquiry.

19) To obtain a de Broglie wave visible to human eyes (with a size greater than 0.1 mm), the particle should have a relatively small mass and a corresponding wavelength within the visible light range.

According to the de Broglie equation:

Wavelength = h / momentum

To achieve a visible-sized de Broglie wave, the wavelength needs to be on the order of 0.1 mm or larger. This corresponds to the visible light range of the electromagnetic spectrum.

Particles with low mass and high velocity can exhibit shorter wavelengths. For example, electrons or even smaller particles like neutrinos could potentially have wavelengths in the visible light range if they are moving at high speeds. However, the velocity of these particles would need to be extremely close to the speed of light, which is not currently achievable in practice.

In summary, to obtain a visible-sized de Broglie wave, a particle with low mass (such as an electron) would need to be moving at a velocity very close to the speed of light.

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An AC generator supplies an rms voltage of 240 V at 50.0 Hz. It is connected in series with a 0.250 H inductor, a 5.80 μF capacitor and a 286 Ω resistor.
What is the impedance of the circuit?
Tries 0/12 What is the rms current through the resistor?
Tries 0/12 What is the average power dissipated in the circuit?
Tries 0/12 What is the peak current through the resistor?
Tries 0/12 What is the peak voltage across the inductor?
Tries 0/12 What is the peak voltage across the capacitor?
Tries 0/12 The generator frequency is now changed so that the circuit is in resonance. What is that new (resonance) frequency?

Answers

The impedance of the circuit is approximately 287.6 Ω. The rms current through the resistor is approximately 0.836 A. The average power dissipated in the circuit is approximately 142.2 W. The peak current through the resistor is approximately 1.18 A. The peak voltage across the inductor is approximately 286.2 V. The peak voltage across the capacitor is approximately 286.2 V. The new resonance frequency of the circuit is 50.0 Hz.

To solve these problems, we'll use the formulas and concepts related to AC circuits.

1. Impedance (Z) of the circuit:

The impedance of the circuit is given by the formula:

Z = √(R^2 + (Xl - Xc)^2)

where R is the resistance, Xl is the inductive reactance, and Xc is the capacitive reactance.

Given:

R = 286 Ω

Xl = 2πfL = 2π(50.0 Hz)(0.250 H) ≈ 78.54 Ω

Xc = 1 / (2πfC) = 1 / (2π(50.0 Hz)(5.80 × 10^-6 F)) ≈ 54.42 Ω

Substituting the values into the formula, we get:

Z = √(286^2 + (78.54 - 54.42)^2)

 ≈ 287.6 Ω

Therefore, the impedance of the circuit is approximately 287.6 Ω.

2. RMS current through the resistor:

The rms current through the resistor can be calculated using Ohm's Law:

I = V / Z

where V is the rms voltage and Z is the impedance.

Given:

V = 240 V

Z = 287.6 Ω

Substituting the values into the formula, we have:

I = 240 V / 287.6 Ω

 ≈ 0.836 A

Therefore, the rms current through the resistor is approximately 0.836 A.

3. Average power dissipated in the circuit:

The average power dissipated in the circuit can be calculated using the formula:

P = I^2 * R

where I is the rms current and R is the resistance.

Given:

I = 0.836 A

R = 286 Ω

Substituting the values into the formula, we get:

P = (0.836 A)^2 * 286 Ω

 ≈ 142.2 W

Therefore, the average power dissipated in the circuit is approximately 142.2 W.

4. Peak current through the resistor:

The peak current through the resistor is equal to the rms current multiplied by √2:

Peak current = I * √2

Given:

I = 0.836 A

Substituting the value into the formula, we have:

Peak current = 0.836 A * √2

 ≈ 1.18 A

Therefore, the peak current through the resistor is approximately 1.18 A.

5. Peak voltage across the inductor and capacitor:

The peak voltage across the inductor and capacitor is equal to the rms voltage:

Peak voltage = V

Given:

V = 240 V

Substituting the value into the formula, we have:

Peak voltage = 240 V

 ≈ 240 V

Therefore, the peak voltage across the inductor and capacitor is approximately 240 V.

6. New resonance frequency:

In a resonant circuit, the inductive reactance (Xl) is equal to the capacitive reactance (Xc

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2)A liquid mixture of benzene-toluene is to be distilled in a fractionating tower at 1 atmosphere of pressure. The feed of 100 kg/mol is liquid and it contains 45%mole and 55%mole toluene. The feed enters to boiling temperature. A distillated containing 95%mole benzene and bottom containing 10% mole benzene are obtained. The Cp of feed (12 pts.) is 200 KJ/Kg.mol.K and the latent heat is 30000 KJ/kg.mol. Determine: a) Draw the equilibrium data with the table of the annexes. +2 b) The fi (e) factor. 0.32 c) The minimum reflux. d) The operating reflux. I. 56 ors e) The number of trays
f) Boiling temperature in the feed.

Answers

The purpose of the fractionating tower is to separate a liquid mixture of benzene and toluene into distillate and bottom products based on their different boiling points and compositions.

What is the purpose of the fractionating tower in the given paragraph?

The given paragraph describes a distillation process for a liquid mixture of benzene and toluene in a fractionating tower operating at 1 atmosphere of pressure. The feed has a molar composition of 45% benzene and 55% toluene, and it enters the tower at its boiling temperature.

The distillate obtained contains 95% benzene, while the bottom product contains 10% benzene. The heat capacity of the feed is given as 200 KJ/Kg.mol.K, and the latent heat is 30000 KJ/kg.mol.

a) To draw the equilibrium data, the provided table in the annexes should be consulted. The equilibrium data represents the relationship between the vapor and liquid phases at equilibrium for different compositions.

b) The "fi (e) factor" is determined to be 0.32. The fi (e) factor is a dimensionless parameter used in distillation calculations to account for the vapor-liquid equilibrium behavior.

c) The minimum reflux is the minimum amount of liquid reflux required to achieve the desired product purity. Its value can be determined through distillation calculations.

d) The operating reflux is the actual amount of liquid reflux used in the distillation process, which can be higher than the minimum reflux depending on specific process requirements.

e) The number of trays in the fractionating tower can be determined based on the desired separation efficiency and the operating conditions.

f) The boiling temperature in the feed is given in the paragraph as the temperature at which the feed enters the tower. This temperature corresponds to the boiling point of the mixture under the given operating pressure of 1 atmosphere.

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A 20.0 kg object starts from rest and slides down an inclined plane. The change in its elevation is 3.0 m and its final speed is 6 m/sec. How much energy did the object lose due to friction as it slid down the plane?

Answers

The object lost 228 J of energy due to friction as it slid down the inclined plane.

To find the energy lost due to friction as the object slides down the inclined plane, we need to calculate the initial mechanical energy and the final mechanical energy of the object.

The initial mechanical energy (Ei) is given by the potential energy at the initial height, which is equal to the product of the mass (m), acceleration due to gravity (g), and the initial height (h):

Ei = m * g * h

The final mechanical energy (Ef) is given by the sum of the kinetic energy at the final speed (KEf) and the potential energy at the final height (PEf):

Ef = KEf + PEf

The kinetic energy (KE) is given by the formula:

KE = (1/2) * m * v^2

where m is the mass and v is the velocity.

The potential energy (PE) is given by the formula:

PE = m * g * h

Given:

Mass of the object (m) = 20.0 kg

Change in elevation (h) = 3.0 m

Final speed (v) = 6 m/s

[tex]\\ΔE = Ei - Ef\\ΔE = 588 J - 360 J\\ΔE = 228 J[/tex]

Next, let's calculate the final mechanical energy (Ef):

The energy lost due to friction (ΔE) can be calculated as the difference between the initial mechanical energy and the final mechanical energy:

[tex]ΔE = Ei - Ef\\ΔE = 588 J - 360 J\\ΔE = 228 J[/tex]

Therefore, the object lost 228 J of energy due to friction as it slid down the inclined plane.

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Two positive charges \( \mathrm{Q} 1 \) and \( \mathrm{Q} 2 \) are separated by a distance \( r \). The charges repel each other with a force \( F \). If the magnitude of each charge is doubled and th

Answers

If the magnitude of each charge is doubled and the distance between them is halved, the new force between them will be four times the original force.

Let's denote the original charges as Q1 and Q2, and the original force as F. The electric force between two charges is given by Coulomb's law:

F = k * (Q1 * Q2) / r^2, where k is the Coulomb's constant and r is the distance between the charges.

If the magnitude of each charge is doubled (2Q1 and 2Q2) and the distance between them is halved (r/2), the new force (F') can be calculated as:

F' = k * (2Q1 * 2Q2) / (r/2)^2.

Simplifying the equation:

F' = k * (4Q1 * 4Q2) / (r/2)^2,

F' = k * (16Q1 * Q2) / (r^2/4),

F' = k * (16Q1 * Q2) * (4/r^2),

F' = 64 * k * (Q1 * Q2) / r^2.

Therefore, the new force between the charges is four times the original force: F' = 4F.

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3. You are standing 50 feet from a building and throw a ball through a window that is 26 feet above the ground. Your release point is 6 feet off of the ground (hint: you are only concerned with Δy ). You throw the ball at 30ft/sec. At what angle from the horizontal should you throw the ball? (hint: this is your launch angle) (2pts)

Answers

The angle from the horizontal to throw the ball is 37. 03 degrees

How to determine the value

First, let us use the equation;

Δy = Vyt + (1/2)gt²

Substitute the values, we have;

32 = 0× t + (1/2)32t²

t² = 2

Find the square root

t = 1.414 seconds.

The formula for distance (d) is d = Vx× t

Substitute the values, we have;

d = 30 ×  1.414

d =  42.42 feet.

The angle is determined with the tangent identity

tan θ = Δy / d.

Substitute the values, we have

tan θ = 32 / 42.42

Divide the values

tan θ = 0. 7544

Take the tangent inverse

θ = 37. 03 degrees

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The electric field in a sinusoidal wave changes as
E=(27N/C)cos[(1.2×1011rad/s)t+(4.2×102rad/m)x]E=(27N/C)cos⁡[(1.2×1011rad/s)t+(4.2×102rad/m)x]
Part C
What is the frequency of the wave?
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Answers

To determine the frequency of the wave, we can examine the equation provided and identify the coefficient of the time variable. The frequency of the wave is approximately 1.91 × 10^10 Hz.

In the given equation, E = (27 N/C) cos[(1.2 × 10^11 rad/s)t + (4.2 × 10^2 rad/m)x], we can see that the coefficient of the time term is 1.2 × 10^11 rad/s.

The coefficient of the time term represents the angular frequency of the wave, which is related to the frequency by the equation: ω = 2πf, where ω is the angular frequency and f is the frequency.

The frequency corresponds to the coefficient of the time term, which represents the number of oscillations per unit of time. By comparing the given coefficient with the equation ω = 2πf, we can determine the frequency of the wave.

Dividing the angular frequency (1.2 × 10^11 rad/s) by 2π, we find the frequency to be approximately 1.91 × 10^10 Hz.

Therefore, the frequency of the wave is approximately 1.91 × 10^10 Hz.

Learn more about frequency here; brainly.com/question/254161

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