4. A car with mass 1.50 x 10 kg traveling east at a speed of 25.0 m/s collides at an intersection with a 2.50 x 10°-kg van traveling north at a speed of 20.0 m/s, as shown in the Figure. Find the magnitude and direction of the velocity after the collision, assuming that the vehicles undergo a perfectly inelastic collision and assuming that friction between the vehicles and the road can be neglected. [4A)

i. The kinetic energy of the object when it is launched from the ground is 1600 J.

ii. The maximum height attained by the object is 44.2 m.

iii. The speed of the object when it is 12 m above the ground is 34.9 m/s.

The potential energy of an object with mass m is given by the formula mgh where g is acceleration due to gravity and h is the height above the reference level. When an object is launched, it has kinetic energy. The kinetic energy of an object with mass m moving at a velocity v is given by the formula KE= 1/2mv².

i. Initially, the object has no potential energy as it is launched from the ground. Therefore, the kinetic energy of the object when it is launched from the ground is 1600 J (KE=1/2mv²).

ii. The maximum height attained by the object can be determined using the formula h= (v²sin²θ)/2g.

iii. When the object is at a height of 12 m, the potential energy is mgh. Therefore, the total energy at that point is KE + PE = mgh + 1/2mv².

By using energy conservation, the speed of the object can be calculated when it is 12 m above the ground using the formula v= √(vo²+2gh).

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Answer:

i. The kinetic energy of the object when it is launched from the ground is 1600 J.

ii. The maximum height attained by the object is 44.2 m.

iii. The speed of the object when it is 12 m above the ground is 34.9 m/s.

Explanation:

The potential energy of an object with mass m is given by the formula mgh where g is acceleration due to gravity and h is the height above the reference level. When an object is launched, it has kinetic energy. The kinetic energy of an object with mass m moving at a velocity v is given by the formula KE= 1/2mv².

i. Initially, the object has no potential energy as it is launched from the ground. Therefore, the kinetic energy of the object when it is launched from the ground is 1600 J (KE=1/2mv²).

ii. The maximum height attained by the object can be determined using the formula h= (v²sin²θ)/2g.

iii. When the object is at a height of 12 m, the potential energy is mgh. Therefore, the total energy at that point is KE + PE = mgh + 1/2mv².

By using energy conservation, the speed of the object can be calculated when it is 12 m above the ground using the formula v= √(vo²+2gh).

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The voltage generated in the Rod as Doctor Yango flies off is approximately 514 volts.

As we know, the voltage induced in a conductor moving through a magnetic field is given by this formula;

v = Bl

voltage induced = magnetic field × length of conductor × velocity

Now, substituting the values given in the question;

v = (17 T) (0.33 m) (89.7 m/s) = 514 T⋅m/s ≈ 514 V

Therefore, the voltage generated in the Rod as Doctor Yango flies off is approximately 514 volts.

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The mass of water used to cool a 230 kg cast-iron car engine from 34°C to 6°C is approximately 3.86 kg. The heat given off during the cooling process is 4.3 x 10^6 J.

The calculation is based on the equation Q = mcΔT, where Q is the heat, m is the mass of water, c is the specific heat capacity, and ΔT is the change in temperature.

To find the mass of water used to cool the engine, we can use the equation:

Q = mcΔT

Where Q is the heat given off by the engine and water, m is the mass of water, c is the specific heat capacity of water (4.18 J/g°C), and ΔT is the change in temperature.

Given:

Q = 4.3 x 10^6 J

ΔT = (34°C - 6°C) = 28°C

c = 4.18 J/g°C

We can rearrange the equation to solve for mass:

m = Q / (cΔT)

Substituting the given values:

m = (4.3 x 10^6 J) / (4.18 J/g°C * 28°C)

m ≈ 3860 g

Therefore, approximately 3860 grams (or 3.86 kg) of water is used to cool the engine.

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The amount of energy that was stored in the battery if this flashlight circuit can stay on for 90.0 minutes is 57.5 J.

A flashlight is a circuit that consists of a battery and a light bulb. If we assume that the battery can maintain its 1.50 volt potential difference throughout its entire useful life.

The current that is passing through the circuit can be determined by using the Ohm's Law;

V= IR ⇒ I = V/R

Given,V = 1.50 V,

R = 212 Ω

⇒ I = V/R = (1.50 V) / (212 Ω) = 0.00708 A

The amount of charge that will flow in the circuit is given by;

Q = It = (0.00708 A)(90.0 min x 60 s/min) = 38.3 C

The energy that is stored in the battery can be calculated by using the formula for potential difference and the charge stored;

E = QV = (38.3 C)(1.50 V) = 57.5 J

Therefore, the amount of energy that was stored in the battery if this flashlight circuit can stay on for 90.0 minutes is 57.5 J.

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The linear momentum of the ball is 1.534 kg m/s.

The mass of the ball is 100 g, and the height from which it is dropped is 12.0 m. We have to calculate the linear momentum of the ball when it strikes the ground. To find the velocity of the ball, we have used the third equation of motion which relates the final velocity, initial velocity, acceleration, and displacement of an object.

Let's substitute the given values in the equation, we get:

v² = u² + 2asv² = 0 + 2 × 9.8 × 12.0v² = 235.2v = √235.2v ≈ 15.34 m/s

Now we can find the linear momentum of the ball by using the formula p = mv. We get:

p = 0.1 × 15.34p = 1.534 kg m/s

Therefore, the ball's linear momentum when it strikes the ground is 1.534 kg m/s.

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To calculate the work done by the boy in lifting the box, we need to use the formula:

Work = Force × Distance × cos(θ)

In this case, the force exerted by the boy is equal to the weight of the box, which can be calculated using the formula:

Force = mass × acceleration due to gravity

Given that the mass of the box is 1 kg and the acceleration due to gravity is 10 m/s² (as given in the question), the force exerted by the boy is:

Force = 1 kg × 10 m/s² = 10 N

The distance lifted by the boy is given as 40 cm, which is 0.4 meters. Plugging in these values into the work formula:

Work = 10 N × 0.4 m × cos(0°)

Since the box is lifteverticall y, the angle θ between the force and the displacement is 0°, and the cosine of 0° is 1. So we have:

Work = 10 N × 0.4 m × 1 = 4 J

Therefore, the work done by the boy in lifting the 1-kg box vertically by 40 cm is 4 joules.

The correct option is (c) 4.

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Part A: The speed of the block when it is a distance of 16.8 m from its starting point is 6.80 m/s. Part B: The time it takes for the block to slide 16.8 m from its starting point is 2.47 seconds.

To find the speed of the block when it is a distance of 16.8 m from its starting point, we can use the equations of motion. Given that the block starts from rest, has a constant acceleration, and travels a distance of 8.40 m, we can find the acceleration using the equation v^2 = u^2 + 2as. Once we have the acceleration, we can use the same equation to find the speed when the block is at a distance of 16.8 m. For part B, to find the time it takes to slide 16.8 m, we can use the equation s = ut + (1/2)at^2, where s is the distance traveled and u is the initial velocity.

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a) The rate of heat transfer (W) by conduction through the wall is 14.40 W.

b) The total heat (J) transferred through the wall in 45 minutes is 32,400 J.


Given, Length (l) = 3.0 m, Breadth (b) = 2.0 m, Thickness of brick (d) = 8.0 cm = 0.08 m, Thermal conductivity of brick (k) = 0.15 W/m-K, Temperature inside the room (T1) = 15 degC, Temperature outside the room (T2) = -9.5 degC, Time (t) = 45 minutes = 2700 seconds

(a) Rate of heat transfer (Q/t) by conduction through the wall is given by:

Q/t = kA (T1-T2)/d, where A = lb = 3.0 × 2.0 = 6.0 m2

Substituting the values, we get:

Q/t = 0.15 × 6.0 × (15 - (-9.5))/0.08 = 14.40 W

Therefore, the rate of heat transfer (W) by conduction through the wall is 14.40 W.

(b) The total heat (Q) transferred through the wall in 45 minutes is given by: Q = (Q/t) × t

Substituting the values, we get: Q = 14.40 × 2700 = 32,400 J

Therefore, the total heat (J) transferred through the wall in 45 minutes is 32,400 J.

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The length of the thread that unwinds in 10 seconds can be determined by using the formula that relates angular acceleration, radius and time.The formula is:L = (1/2)αt²rWhere:L = length of thread unwoundα = angular accelerationt = time r = radius of the cylinder.

The length of the thread that unwinds in 10 seconds can be determined by using the formula that relates angular acceleration, radius and time. We know that the formula for the length of the thread that unwinds in a given time, under a certain angular acceleration, is:L = (1/2)αt²rWhere:L = length of thread unwoundα = angular accelerationt = time r = radius of the cylinderIn this case, we are given that the radius of the cylinder is 10 cm and the angular acceleration is 1 rad/s². We need to find the length of the thread that unwinds in 10 seconds.

Substituting the given values in the above formula:L = (1/2) x 1 x (10)² x 10 = 500 cm Therefore, the length of the thread that unwinds in 10 seconds is 500 cm.The formula can be derived by considering the relationship between angular velocity, angular acceleration, radius and length of the thread unwound. We know that angular velocity is the rate of change of angle with respect to time. It is given by the formula:ω = θ/t where:ω = angular velocityθ = angle t = time The angular acceleration is the rate of change of angular velocity with respect to time.

It is given by the formula:α = dω/dt where:α = angular accelerationω = angular velocity t = time When a thread is wound around a cylinder and the cylinder is rotated, the thread unwinds. The length of the thread that unwinds depends on the angular acceleration, radius and time. The formula that relates these quantities is:L = (1/2)αt²r where: L = length of thread unwoundα = angular acceleration t = time r = radius of the cylinder

Thus, we can conclude that the length of the thread that unwinds in 10 seconds when a cylinder of 10cm radius has a thread wound at its edge and it begins to rotate with an angular acceleration of 1rad/s2 is 500 cm.

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The minimum distance (absolute value) from the central maximum is approximately 8.55 × 10−5 mm.

(a)Fraction of maximum intensity at a distance of 600 cm from the central maximum of the interference. Consider that monochromatic light of wavelength λ is incident on and perpendicular to two slits separated by a distance d. This causes an interference pattern on a screen some distance away.

The pattern will have alternating light and dark fringes, with the central maximum being the brightest and the fringe intensities decreasing with distance from the central maximum.

The distance from the central maximum to the first minimum (the first dark fringe) is given by:$$sin\theta_1=\frac{\lambda}{d}$$$$\theta_1=\sin^{-1}\frac{\lambda}{d}$$Similarly, the distance from the central maximum to the nth minimum is given by:$$sin\theta_n=n\frac{\lambda}{d}$$$$\theta_n=\sin^{-1}(n\frac{\lambda}{d})$$At a distance x from the central maximum, the intensity of the interference pattern is given by:$$I(x)=4I_0\cos^2(\frac{\pi dx}{\lambda D})$$where I0 is the maximum intensity, D is the distance from the slits to the screen, and x is the distance from the central maximum. At a distance of 600 cm (or 6 m) from the central maximum, we have x = 6 m, λ = 656.3 nm = 6.563 × 10−7 m, d = 0.200 mm = 2 × 10−4 m, and we can assume that D ≈ 1 m (since the distance to the screen is much larger than the distance between the slits).

Substituting these values into the equation for intensity gives:$$I(6\ \text{m})=4I_0\cos^2(\frac{\pi (2\times 10^{-4})(6.563\times 10^{-7})}{(1)})$$$$I(6\ \text{m})=4I_0\cos^2(0.000412)$$$$I(6\ \text{m})=4I_0\times 0.999998$$$$I(6\ \text{m})\approx 4I_0$$Therefore, the intensity at a distance of 600 cm from the central maximum is approximately 4 times the maximum intensity.(b) Minimum distance (absolute in mm) from the central maximum where the intensity is at the value found in part (a)At the distance from the central maximum where the intensity is 4I0, we have x = 6 m and I(x) = 4I0.

Substituting these values into the equation for intensity gives:$$4I_0=4I_0\cos^2(\frac{\pi (2\times 10^{-4})(6.563\times 10^{-7})}{(1)})$$$$1=\cos^2(0.000412)$$$$\cos(0.000412)=\pm 0.999997$$$$\frac{\pi dx}{\lambda D}=0.000412$$$$d=\frac{0.000412\lambda D}{\pi x}$$$$d=\frac{0.000412(656.3\times 10^{-9})(1)}{\pi(6)}$$$$d\approx 8.55\times 10^{-8}$$The minimum distance from the central maximum where the intensity is 4 times the maximum intensity is approximately 8.55 × 10−8 m = 0.0855 μm = 8.55 × 10−5 mm.

Therefore, the minimum distance (absolute value) from the central maximum is approximately 8.55 × 10−5 mm.

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The total energy of the helium atom to the first order approximation is given by:

E = 2T + J - K

Calculating the energy of the excited states of the helium atom to the first order of approximation involves considering the Coulomb and exchange integrals. Let's denote the wavefunctions of the two electrons in helium as ψ₁ and ψ₂.

The Coulomb integral represents the electrostatic interaction between the electrons and is given by:

J = ∫∫ ψ₁*(r₁) ψ₂*(r₂) 1/|r₁ - r₂| ψ₁(r₁) ψ₂(r₂) dr₁ dr₂,

Where r₁ and r₂ are the positions of the first and second electrons, respectively. This integral represents the repulsion between the two electrons due to their electrostatic interaction.

The exchange integral accounts for the quantum mechanical effect called electron exchange and is given by:

K = ∫∫ ψ₁*(r₁) ψ₂*(r₂) 1/|r₁ - r₂| ψ₂(r₁) ψ₁(r₂) dr₁ dr₂,

Where ψ₂(r₁) ψ₁(r₂) represents the probability amplitude for electron 1 to be at position r₂ and electron 2 to be at position r₁. The exchange integral represents the effect of the Pauli exclusion principle, which states that two identical fermions cannot occupy the same quantum state simultaneously.

The total energy of the helium atom to the first order approximation is given by:

E = 2T + J - K,

Where T is the kinetic energy of a single electron.

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The correct option is: a) 0.25

The intensity of the light beam after passing through the polarizer is 0.25.

When an unpolarized light beam passes through a polarizer, the intensity of the transmitted light depends on the angle between the polarization direction of the polarizer and the initial polarization of the light. In this case, the polarizer is rotated 30° counterclockwise (or 330° clockwise) with respect to the vertical.

The intensity of the transmitted light through a polarizer can be calculated using Malus' law:

I_transmitted = I_initial * cos²(θ)

Where:

I_transmitted is the intensity of the transmitted light

I_initial is the initial intensity of the light

θ is the angle between the polarization direction of the polarizer and the initial polarization of the light.

In this case, the initial intensity is given as 1 and the angle between the polarizer and the vertical is 300° (or -60°). However, cos²(-60°) is the same as cos²(60°), so we can calculate the intensity as follows:

I_transmitted = 1 * cos²(60°)

= 1 * (0.5)²

= 1 * 0.25

= 0.25

Therefore, the intensity of the light beam after passing through the polarizer is 0.25. Thus, the correct option is a. 0.25.

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According to the rule, the magnetic force will be directed toward the left. The correct answer is B. toward the left.

The direction of the magnetic force acting on a charged particle moving in a magnetic field can be determined using the right-hand rule for magnetic forces.

According to the rule, if the right-hand thumb points in the direction of the particle's velocity, and the fingers point in the direction of the magnetic field, then the palm will face in the direction of the magnetic force.

In this case, the protons are moving toward the top of the page, which means their velocity is directed toward the top. The uniform magnetic field points directly into the page. Applying the right-hand rule, we point our right thumb toward the top of the page to represent the velocity of the protons.

Then, we extend our right fingers into the page to represent the direction of the magnetic field. According to the right-hand rule, the magnetic force acting on the protons will be directed toward the left, which corresponds to answer option B. toward the left.

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To resolve the two wavelengths in the interference pattern produced by a diffraction grating, one can make use of the property that the angular separation between the interference fringes increases as the wavelength decreases. Here's how the resolution can be achieved:

Replace the diffraction grating by one with more lines per mm.

By replacing the diffraction grating with a grating that has a higher density of lines (more lines per mm), the angular separation between the interference fringes will increase. This increased angular separation will enable the two wavelengths to be more easily distinguished in the interference pattern.

Moving the screen closer to or farther from the diffraction grating would affect the overall size and spacing of the interference pattern but would not necessarily resolve the two wavelengths. Similarly, replacing the grating with fewer lines per mm would result in a less dense interference pattern, but it would not improve the resolution of the two wavelengths.

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In the given scenario, a gear cog is subjected to four forces (F1, F2, F3, and F4) at different positions. We need to determine the net torque about the axle, identify the force that generates the biggest torque, and determine which force should be removed to maximize the net torque in one direction.

(i) To calculate the net torque about the axle, we need to consider the torque produced by each individual force. The torque produced by a force is given by the equation τ = r × F, where r is the distance from the point of rotation to the line of action of the force, and F is the magnitude of the force. The direction of torque follows the right-hand rule, where the thumb points in the direction of the force and the fingers curl in the direction of the torque.

(ii) To identify the force that generates the biggest torque in any one direction, we compare the magnitudes of the torques produced by each force. By calculating the torques produced by F1, F2, F3, and F4, we can determine which force results in the largest magnitude of torque. The direction of the torque can be determined based on the right-hand rule.

(iii) To determine which force should be removed to maximize the net torque in one direction, we need to analyze the torques produced by each force. By removing one force, we alter the torque balance. We can compare the torques produced by the remaining three forces and identify which combination of forces generates the maximum net torque in one specific direction.

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a) The speed of light in glass can be found using the formula v = c/n, where v is the speed of light in the medium (glass), c is the speed of light in vacuum (approximately 3x10^8 m/s), and n is the refractive index of glass (1.5). Therefore, the speed of light in glass is approximately 2x10^8 m/s.

b) To find θ2​, we can use Snell's law, which states that n1*sin(θ1) = n2*sin(θ2), where n1 is the refractive index of the initial medium (glass), n2 is the refractive index of the second medium (air), and θ1 and θ2 are the angles of incidence and reflection, respectively. Given that θ1 is 36∘ and n1 is 1.5, we can solve for θ2:

1.5*sin(36∘) = 1*sin(θ2)

θ2 ≈ 23.49∘

c) To find θ3​, we can use Snell's law again, but this time with the refractive index of air (approximately 1) and the refractive index of glass (1.5). Given that θ2 is 23.49∘ and n1 is 1.5, we can solve for θ3:

1*sin(23.49∘) = 1.5*sin(θ3)

θ3 ≈ 15.18∘

d) The critical angle is the angle of incidence at which the refracted angle becomes 90∘. Using Snell's law with n1 (glass) and n2 (air), we can find the critical angle (θc):

n1*sin(θc) = n2*sin(90∘)

1.5*sin(θc) = 1*sin(90∘)

θc ≈ 41.81∘

Therefore, the critical angle is approximately 41.81∘.

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The entrance velocity is approximately 10.62 m/s, the exit velocity is approximately 95.34 m/s, and the flow rate of gasoline through the Venturi tube is approximately 1.15 m³/s.

To determine the entrance velocity, exit velocity, and flow rate of gasoline through the Venturi tube, we can apply the principles of Bernoulli's-equation and continuity equation.

Entrance velocity (V1): Using Bernoulli's equation, we can equate the pressure difference (ΔP) to the kinetic-energy per unit volume (ρV^2 / 2), where ρ is the density of gasoline. Rearranging the equation, we get:

ΔP = (ρV1^2 / 2) - (ρV2^2 / 2)

Substituting the given values: ΔP = 15,000 Pa and ρ = 700 kg/m³, we can solve for V1. The entrance velocity (V1) is approximately 10.62 m/s.

Exit velocity (V2): Since the Venturi tube is designed to conserve mass, the flow rate at the entrance (A1V1) is equal to the flow rate at the exit (A2V2), where A1 and A2 are the cross-sectional areas at the entrance and exit, respectively. The cross-sectional area of a circle is given by A = πr^2, where r is the radius. Rearranging the equation, we get:

V2 = (A1V1) / A2

Substituting the given values: A1 = π(0.03 m)^2, A2 = π(0.01 m)^2, and V1 = 10.62 m/s, we can calculate V2. The exit velocity (V2) is approximately 95.34 m/s.

Flow rate (Q): The flow rate (Q) can be calculated by multiplying the cross-sectional area at the entrance (A1) by the entrance velocity (V1). Substituting the given values: A1 = π(0.03 m)^2 and V1 = 10.62 m/s, we can calculate the flow rate (Q). The flow rate is approximately 1.15 m³/s.

In conclusion, for gasoline flowing through the Venturi tube with a pressure difference of 15,000 Pa, the entrance velocity is approximately 10.62 m/s, the exit velocity is approximately 95.34 m/s, and the flow rate is approximately 1.15 m³/s.

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Let us calculate the initial temperature in degrees Celsius of the forging. We know that the hot metal forging has a mass of 70.3 kg and a specific heat capacity of 434 J/(kg C°).

Also, we know that to harden it, the forging is quenched by immersion in 834 kg of oil that has a temperature of 39.9°C and a specific heat capacity of 2680 J/(kg C°).

The final temperature of the oil and forging at thermal equilibrium is 68.5°C. Since we are assuming that heat flows only between the forging and the oil, we can equate the heat gained by the oil with the heat lost by the forging using the formula.

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The initial velocity of the second mass (m₂) is 0 as it is stationary. To find the initial velocity of the first mass (m₁), we will use the equation for kinetic energy.Kinetic energy = 1/2 mv²where m is the mass of the object and v is its velocity.

The kinetic energy of the first mass can be found by converting its velocity from km/hr to m/s.Kinetic energy = 1/2 (8.775 kg) (48.38 km/hr)² = 1/2 (8.775 kg) (13.44 m/s)² = 797.54 JSo the total initial kinetic energy of the two masses is the sum of the kinetic energies of the individual masses: 797.54 J + 0 J = 797.54 JThe final velocity of the two masses can be found using the law of conservation of momentum.

According to the law of conservation of momentum, the momentum before the collision is equal to the momentum after the collision.m₁v₁ + m₂v₂ = (m₁ + m₂)vfwhere m₁ is the mass of the first object, v₁ is its velocity before the collision, m₂ is the mass of the second object, v₂ is its velocity before the collision, vf is the final velocity of both objects after the collision.

Since the second mass is stationary before the collision, its velocity is 0.m₁v₁ = (m₁ + m₂)vf - m₂v₂Substituting the given values in the above equation and solving for v₁, we get:v₁ = [(m₁ + m₂)vf - m₂v₂]/m₁= [(8.775 kg + 4.944 kg)(0 m/s) - 4.944 kg (0 m/s)]/8.775 kg = 0 m/sSo the initial velocity of the first mass is 0 m/s.

The momentum of the system after the collision is:momentum = (m₁ + m₂)vfThe total final kinetic energy of the system can be found using the equation:final kinetic energy = 1/2 (m₁ + m₂) vf²Substituting the given values in the above equation, we get:final kinetic energy = 1/2 (8.775 kg + 4.944 kg) (0.9707 m/s)² = 25.28 JThe mechanical energy lost due to this collision is the difference between the initial kinetic energy and the final kinetic energy:energy lost = 797.54 J - 25.28 J = 772.26 JThus, the mechanical energy lost due to this collision is 772.26 J.

Initial velocity of the first mass = 0 m/sInitial velocity of the second mass = 0 m/sFinal velocity of the two masses = 0.9707 m/sTotal initial kinetic energy of the two masses = 797.54 JTotal final kinetic energy of the two masses = 25.28 JEnergy lost due to this collision = 772.26 J.

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A jet engine emits sound uniformly in all directions, radiating an acoustic power of 2.85 x 105 W. The intensity of the sound at a distance of 57.3 m from the engine is 6.91 W/m^2, and the corresponding sound intensity level is 128.4 dB.

The intensity of sound I is inversely proportional to the square of the distance from the source. The sound intensity level B is calculated using the following formula:

B = 10 log10(I/I0)

where I0 is the reference intensity of 10^-12 W/m^2.

Here is the calculation in detail:

Intensity I = 2.85 x 105 W / (4 * pi * (57.3 m)^2) = 6.91 W/m^2

Sound intensity level B = 10 log10(6.91 W/m^2 / 10^-12 W/m^2) = 128.4 dB

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The magnitude of the magnetic force on the smoke particle is 9.0x10^(-4) N with the direction of the force towards the East.

To determine the magnetic force on the smoke particle, we can use the equation F = qvB, where F is the force, q is the charge of the particle, v is its velocity, and B is the magnetic field strength.

Given that the charge of the smoke particle is -9.0x10^(-1) C, its velocity is 2.0 mm/s (which can be converted to 2.0x10^(-3) m/s), and the magnetic field strength is 0.50 T, we can calculate the magnetic force.

Using the equation F = qvB, we can substitute the values: F = (-9.0x10^(-1) C) x (2.0x10^(-3) m/s) x (0.50 T). Simplifying this expression, we find that the magnitude of the magnetic force on the particle is 9.0x10^(-4) N.

The direction of the magnetic force can be determined using the right-hand rule. Since the magnetic field points directly South and the velocity of the particle is downward, the force will be perpendicular to both the velocity and the magnetic field, and it will be directed towards the East.

Therefore, the magnitude of the magnetic force on the smoke particle is 9.0x10^(-4) N, and the direction of the force is towards the East.

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Weight and mass are not directly proportional to each other. Weight and mass are two different physical quantities. The given statement is false

Mass refers to the amount of matter an object contains, while weight is the force exerted on an object due to gravity. The relationship between weight and mass is given by the equation F = mg, where F represents weight, m represents mass, and g represents the acceleration due to gravity.

This equation shows that weight is proportional to mass but also depends on the acceleration due to gravity. Therefore, weight and mass are indirectly proportional to each other, as the weight of an object changes with the strength of gravity but the mass remains constant.

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To solve y' + 2 = 0 using an integrating factor, we multiply by e^(2x) and integrate. To solve y^2dy = x^2 - xy using a homogeneous equation, we substitute y = vx and solve a separable equation.

1. To solve y' + 2 = 0 using an integrating factor, we first rewrite the equation as y' = -2. Then, we multiply both sides by the integrating factor e^(2x):

e^(2x)*y' = -2e^(2x)

We recognize the left-hand side as the product rule of (e^(2x)*y)' and integrate both sides with respect to x:

e^(2x)*y = -e^(2x)*C1 + C2

where C1 and C2 are constants of integration. Solving for y, we get:

y = -C1 + C2*e^(-2x)

where C1 and C2 are arbitrary constants.

2. To solve y^2dy = x^2 - xy using a homogeneous equation, we first rewrite the equation in the form:

dy/dx = (x^2/y - x)

This is a homogeneous equation because both terms have the same degree of homogeneity (2). We then substitute y = vx and dy/dx = v + xdv/dx into the equation, which gives:

v + xdv/dx = (x^2)/(vx) - x

Simplifying, we get:

vdx/x = (1 - v)dv

This is a separable equation that we can integrate to get:

ln|x| = ln|v| - v + C

where C is the constant of integration. Rearranging and substituting back v = y/x, we get:

ln|y| - ln|x| - y/x + C = 0

This is the general solution of the homogeneous equation.

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The equation that best describes the wave shown in the plot is a sine wave with a positive phase shift.

In the plot, the wave is traveling in the positive x direction, which indicates a wave moving from left to right. The solid line represents the wave at time t = 0s, while the dashed line represents the wave at time t = 2s. This indicates that the wave is progressing in time.

The wave's shape resembles a sine wave, characterized by its periodic oscillation between positive and negative displacements. Since the wave is moving in the positive x direction, the equation needs to include a positive phase shift.

Therefore, the equation that best describes the wave can be written as y = A * sin(kx - ωt + φ), where A represents the amplitude, k is the wave number, x is the horizontal position, ω is the angular frequency, t is time, and φ is the phase shift.

Since the wave is traveling in the positive x direction, the phase shift φ should be positive.

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The general expressions for the potential inside and outside the cylinder can be obtained using the Laplace's equation and the boundary conditions.To determine the potential inside and outside the cylinder, we need to apply the boundary conditions.

a. Ignoring end effects, the general expressions for the potential inside and outside the cylinder can be written as:

Inside the cylinder (r < a):

ϕ_inside = ϕ0 + E * r

Outside the cylinder (r > a):

ϕ_outside = ϕ0 + E * a^2 / r

Here, ϕ_inside and ϕ_outside are the potentials inside and outside the cylinder, respectively. ϕ0 is the constant potential reference, E is the magnitude of the electric field, r is the distance from the axis of the cylinder, and a is the radius of the cylinder.

b. To determine the potential inside and outside the cylinder, substitute the given values into the general expressions:

Inside the cylinder (r < a):

ϕ_inside = ϕ0 + E * r

Outside the cylinder (r > a):

ϕ_outside = ϕ0 + E * a^2 / r

c. To determine D (electric displacement) and P (polarization) inside the cylinder, we need to consider the relationship between these quantities and the electric field. In a linear dielectric material, the electric displacement D is related to the electric field E and the polarization P through the equation:

D = εE + P

where ε is the permittivity of the material. Since the cylinder is in a vacuum, ε = ε0, the permittivity of free space. Therefore, inside the cylinder, we have:

D_inside = ε0E + P_inside

where D_inside and P_inside are the electric displacement and polarization inside the cylinder, respectively.

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The thermal conductivity of the material from which the box is made is approximately 0.84 W/(m·K).

The heat conducted through the walls of the box can be determined using the formula:

Q = k * A * (ΔT / d)

Where:

Q is the heat conducted through the walls,

k is the thermal conductivity of the material,

A is the surface area of the walls,

ΔT is the temperature difference between the inside and outside of the box, and

d is the thickness of the walls.

Given that the temperature difference ΔT is (29.2 °C - (-91.7 °C)) = 121.7 °C and the heat conducted Q is 3.02 x [tex]10^{6}[/tex] J, we can rearrange the formula to solve for k:

k = (Q * d) / (A * ΔT)

The surface area A of the walls can be calculated as:

A = 6 * [tex](side length)^{2}[/tex]

Substituting the given values, we have:

A = 6 * (0.284 m)2 = 0.484 [tex]m^{2}[/tex]

Now we can substitute the values into the formula:

k = (3.02 x [tex]10^{6}[/tex] J * 3.62 x [tex]10^{-2}[/tex] m) / (0.484 [tex]m^{2}[/tex] * 121.7 °C)

Simplifying the expression, we find:

k = 0.84 W/(m·K)

Therefore, the thermal conductivity of the material from which the box is made is approximately 0.84 W/(m·K).

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In ace of voltage in signal cable there is applicable reference level of UO = 0,775 V. The voltage corresponding to a level of 12 dB is approximately 1.947 V.

a. To compute the level value in decibels for different voltage values, we can use the formula: Level [dB] = 20 * log10(Vin / Vref)

Where: Vin is the input voltage.

Vref is the reference voltage (0.775 V in this case).

Let's calculate the level values for the given voltage values:

For U = 1 mV:

Level [dB] = 20 * log10(1 mV / 0.775 V)

Level [dB] = 20 * log10(0.00129)

Level [dB] ≈ -59.92 dBu

For U = 5 mV:

Level [dB] = 20 * log10(5 mV / 0.775 V)

Level [dB] = 20 * log10(0.00645)

Level [dB] ≈ -45.76 dBu

For U = 20 µV:

Level [dB] = 20 * log10(20 µV / 0.775 V)

Level [dB] = 20 * log10(0.0000258)

Level [dB] ≈ -95.44 dBu

b. To compute the voltage corresponding to a level of 12 dB, we rearrange the formula:

Level [dB] = 20 * log10(Vin / Vref)

Let's solve for Vin:

12 = 20 * log10(Vin / 0.775 V)

0.6 = log10(Vin / 0.775 V)

Now, we can convert it back to exponential form:

10^0.6 = Vin / 0.775 V

Vin = 0.775 V * 10^0.6

Vin ≈ 1.947 V

So, the voltage corresponding to a level of 12 dB is approximately 1.947 V.

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When a point dipole is situated at the center of a conducting spherical shell connected to the land, the potential inside the shell can be determined using zonal harmonics that are regular at the origin to satisfy the boundary conditions.

To find the potential inside the conducting spherical shell, we can make use of the method of images. By placing an image dipole with opposite charge at the center of the shell, we create a symmetric system. This allows us to satisfy the boundary conditions on the shell surface. The potential inside the shell can be expressed as a sum of two contributions: the potential due to the original dipole and the potential due to the image dipole.

The potential due to the original dipole can be calculated using the standard expression for the potential of a point dipole. The potential due to the image dipole can be found by taking into account the image dipole's distance from any point inside the shell and the charges' signs. By summing these two contributions, we obtain the total potential inside the shell.

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The first diffraction minimum of electrons passing through a 1.20 nm single slit with a 2.25 pm wavelength will be found at an angle of 0.115 radians.

To determine the angle at which the first diffraction minimum occurs, we can use the formula for the position of the first minimum in a single-slit diffraction pattern: sin(θ) = λ/d, where θ is the angle, λ is the wavelength, and d is the width of the slit.

First, let's convert the given values to meters: 2.25 pm = 2.25 × 10^(-12) m and 1.20 nm = 1.20 × 10^(-9) m.

Substituting the values into the formula, we get sin(θ) = (2.25 × 10^(-12) m) / (1.20 × 10^(-9) m).

Taking the inverse sine of both sides, we find θ = sin^(-1)((2.25 × 10^(-12) m) / (1.20 × 10^(-9) m)).

Evaluating this expression, we obtain θ ≈ 0.115 radians. Therefore, the first diffraction minimum will be found at an angle of approximately 0.115 radians.

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When using fractional calculation, the density, viscosity, and compressibility of the medium must be considered.

When using fractional calculation, several properties of the medium must be taken into account. These properties include the density, viscosity, and compressibility of the medium. Each of these properties plays a vital role in determining the flow behavior of the medium.
Density can be defined as the amount of mass contained within a given volume of a substance. In the case of fluids, it is the mass of the fluid per unit volume. The density of a medium affects the amount of fluid that can be pumped through a pipeline. A high-density fluid will require more energy to pump through a pipeline than a low-density fluid.
Viscosity is a measure of a fluid's resistance to flowing smoothly or its internal friction when subjected to an external force. It is influenced by the size and shape of the fluid molecules. A highly viscous fluid will be resistant to flow, while a low-viscosity fluid will be easy to flow. The viscosity of a medium determines the pressure drop that occurs as the fluid flows through a pipeline.
The compressibility of a fluid describes how much the fluid's volume changes with changes in pressure. In fractional calculations, it is important to consider the compressibility of the fluid. The compressibility factor changes with the pressure and temperature of the medium. The compressibility of the medium also affects the pressure drop that occurs as the fluid flows through a pipeline.
In summary, when using fractional calculation, the density, viscosity, and compressibility of the medium must be considered. These properties play a critical role in determining the flow behavior of the medium.

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