Two long, parallel wires separated by 2.00 cm carry currents in opposite directions. The current in one wire is 1.75 A, and the current in the other is 3.45 A.

Find the magnitude of the force per unit length that one wire exerts on the other.

Answer:

The carriage speed B was 67.4 mph

Explanation:

This is an exercise for the moment, that as a vector we must look for the solution of each axis (x, y). We define a system formed by the two cars, for this system the forces during the crash are internal, so the moment is preserved.

The data they give is the car more A m = 1000kg and its speed is v1₁₀ = 30 mph i^ and the mass of the car B M = 1500 kg

Let's write the moment for each axis

X axis

     p₀ₓ = [tex]p_{fx}[/tex]

     m v₁ₓ + 0 = (m + M) vₓ

Y axis

     poy = [tex]p_{fy}[/tex]

      0 + M [tex]v_{2y}[/tex] = (m + M) [tex]v_{y}[/tex]

Let's look for the components of the final velocity with trigonometry

     sin 66 = [tex]v_{y}[/tex]  / v

     cos 66 = vₓ / v

     [tex]v_{y}[/tex]  = v sin 66

     vₓ = v cos 66

We substitute and write the system of equations

     m v₁ₓ = (m + M) v cos 66

     M [tex]v_{2y}[/tex]  = (m + M) v sin66

From the first equation

    v = m / (m + M) v₁ₓ / cos 66

    v = 1000 / (1000 + 1500) 30 / cos 66

    v = 29.5 mph

From the second equation

   [tex]v_{2y}[/tex]  = (m + M)/m   v sin 66

  [tex]v_{2y}[/tex]  = (1000 + 1500) /1000     29.5 sin 66

   [tex]v_{2y}[/tex]  = 67.4 mph

The carriage speed B was 67.4 mph

The displacement of a 15.5 kg mass undergoing simple harmonic motion with a frequency of 9.73 Hz, at a point in time 1.25 s after it was at its maximum displacement of 14.6 cm, is found to be -14.1 cm.

The displacement of a mass undergoing simple harmonic motion at any given point of time can be found using the formula x(t) = A cos(wt + φ), where 'A' is the amplitude (maximum displacement), 'w' is the angular frequency, and 'φ' is the phase constant. Given that the maximum displacement or amplitude 'A' is 14.6 cm (or 0.146 m), the frequency 'f' is 9.73 Hz, and the phase constant φ = 0 (as the displacement is maximum at t = 0), the angular frequency 'w' can be calculated as 2πf, which equals approximately 61.1 rad/s. Substituting all these values into the formula, we find that the displacement at time t = 1.25 s is x(t) = 0.146 cos(61.1*1.25 + 0) = -0.141 m, or -14.1 cm. Note that the negative sign indicates that the displacement is in the opposite direction of the initial maximum displacement.

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The displacement from equilibrium at time t = 1.25s is -0.042m.

The displacement from equilibrium of the mass at time t = 1.25 s can be calculated using the formula for simple harmonic motion. The displacement at any given time t is given by the equation x = A * cos(2πft), where A is the amplitude and f is the frequency. In this case, the amplitude is 0.146 m and the frequency is 9.73 Hz. Plugging in the values, we get x = 0.146 * cos(2π * 9.73 * 1.25), which gives us x = -0.042 m.

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Answer:

A)  W = 1885 J , B) [tex]K_{f}[/tex] = 1885 J , C)  w = 8.68 rad / s , D)  t = 8,687 s , E)  P = 109 W  F) P = 2 [tex]P_{rms}[/tex]

Explanation:

Part A    The work in the rotational movement is

       W = τ θ

Let's look at the rotated angle

      θ = 12.0 rot (2pi rad / 1rot) = 75.398 rad

     W = 25.0 75.40

     W = 1885 J

Part B   Let's use the relationship between work and kinetic energy

      W = ΔK = Kf - Ko

As the body leaves the rest w₀ = 0     ⇒ K₀ = 0

      W = [tex]K_{f}[/tex] -0

      [tex]K_{f}[/tex] = 1885 J

Part C     The formula for kinetic energy is

      K = ½ I w²

     w² = 2k / I

     w = √ (2 1885/50)

     w = 8.68 rad / s

Part D     The power in the rotational movement

     P = τ w

     P = 25 8.68

     P = 217 W

     P = W / t

     t = W / P

     t = 1885/217

     t = 8,687 s

Part E   At average power is

     P = τ ([tex]w_{f}[/tex] -w₀)/ 2

We look for angular velocity with kinematics

    [tex]w_{f}[/tex = w₀ + α t

     τ = I α

      α = τ / I

      α = 25/50

      α = 0.5 rad / s²

calculate

      P = 25 (0.5 8.687)

      P = 108.6 W

      P = 109 W

Part F    

The average power is

      [tex]P_{rms}[/tex] = τ ([tex]w_{f}[/tex] -w₀) /

The instant power is

      P = τ w

The difference is that in one case the angular velocity is instantaneous and between averages

P / [tex]P_{rms}[/tex] = τ w / (τ ([tex]w_{f}[/tex]-w₀) / 2)

P / [tex]P_{rms}[/tex]= 2 w / Δw

For this case w₀ = o

p / [tex]P_{rms}[/tex] = 2

The motor exerts rotational motion to do 1885 Joules of work on the platform. The final angular velocity of the platform is 8.68 rad/s. The time it takes to do this work is 17.4 seconds. The average power delivered by the motor is 109 Watts and the instantaneous power is twice the average power.

A motor exerts a constant torque on a horizontal platform and we need to determine the work done, the rotational kinetic energy, the angular velocity, the time it takes, the average power, and compare the instantaneous power to the average power.

Firstly, the work done by the motor is calculated using the formula W = Torque x angular displacement. The angular displacement for 12.0 rotations will equals to 12.0 x 2π radians. So, W = 25.0 N.m x 12 x 2π rad = 1885 J. Hence, the motor does 1885 Joules of work on the platform.

For the rotational kinetic energy, since there is no friction, all of the work done on the platform is converted into kinetic energy, so, K_rot,f = 1885 J.

The final angular velocity ωf can be found from the rotational kinetic energy and the moment of inertia by the relation K_rot,f = 1/2 I ωf^2. From this, we can find ωf = √(2K_rot,f / I)= 8.68 rad/s.

The time it takes Δt to do the work can be calculated using Δt = angular displacement / average angular velocity. Hence, Δt= (12 x 2π) / ((0 + ωf) / 2)= 17.4 s.

The average power P_avg is given by the total work done divided by the total time, which gives P_avg= W / Δt = 109 Watts.

On the final part, the instantaneous power Pf is proportional to the final angular velocity. As Pf = Torque x ωf, we get Pf = 2 x P_avg. So, the instantaneous power being delivered by the motor at the end is twice the average power calculated before.

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Answer:

v = 3.7 m/s

Explanation:

As the swing starts from rest, if we choose the lowest point of the trajectory to be the zero reference level for gravitational potential energy, and if we neglect air resistance, we can apply energy conservation as follows:

m. g. h = 1/2 m v²

The only unknown (let alone the speed) in the equation , is the height from which the swing is released.

At this point, the ropes make a 30⁰ angle with the vertical, so we can obtain the vertical length at this point as L cos 30⁰, appying simply cos definition.

As the height we are looking for is the difference respect from the vertical length L, we can simply write as follows:

h = L - Lcos 30⁰ = 5m -5m. 0.866 = 4.3 m

Replacing in the energy conservation equation, and solving for v, we get:

v = √2.g.(L-Lcos30⁰) = √2.9.8 m/s². 4.3 m =3.7 m/s

Answer:

25 N

Explanation:

Given that

Weight ,mg = 50 N

m=Mass of the box

g=acceleration due to gravity

Horizontal force F= 10 N

Coefficient of friction  ,μ = 0.4

Lets take vertical force = R N

In vertical direction

R + N = mg

N= mg - R

The friction force Fr

Fr= μ N

Fr= μ ( mg - R)

To start the motion

F > Fr

10   > 0.4 ( 50 - R )

25  > 50 - R

R > 50 - 25  

R > 25 N

Therefore minimum force R= 25 N

In the given problem, the minimum vertical force required to set the box into motion is greater than 15N. This force reduces the normal force and consequently the frictional force such that it becomes less than the horizontally applied force.

In this physical situation, you need to understand the role of static friction and normal force in setting the box into motion. The frictional force is calculated by multiplying the coefficient of static friction (0.4 in this case) and normal force. The normal force on the box is the weight of the box minus the upward force applied. Initially, the upward force is zero, so the frictional force is 0.4 * 50N = 20N. This is greater than the 10N horizontal force applied, so the box does not move.

To make the box move, the vertical force has to reduce the normal force such that the frictional force (which is now less due to the decreased normal force) becomes less than the applied horizontal force (10N). Let's consider the vertical upward force needed as F. Hence, the new frictional force will be 0.4 * (50N - F) and should be less than 10N for the box to move. Solving this inequality, the minimum F needed is >15N, anything above this will make the box move.

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The concept necessary to develop this exercise is that of a magnetic field on a surface. The magnetic field is a tool to describe how a magnetic force is distributed in the space around and within something magnetic.

It can be defined as,

[tex]B = \frac{\mu_0 I}{2\pi R}[/tex]

Where,

R= The distance from the point

I = Current

[tex]\mu_0 =[/tex] Permeability constant in free space

Our values are given as,

[tex]\mu_0 = 4\pi * 10^{-7}H/m[/tex]

[tex]I = 200 A[/tex]

[tex]R = 20m[/tex]

Replacing ,

[tex]B = \frac{(4\pi*10^{-7})(200)}{2\pi 20}[/tex]

[tex]B = 2*10^{-6}T[/tex]

Therefore the magnetic field strength on the ground directly under such a transmission line is [tex]2*10^{-6}T[/tex]

The magnetic field strength on the ground directly under a typical high-voltage transmission line carrying a 200 A current at a potential of 110 kV, which is 20 m above the ground, is 2 μT. This is calculated using Ampere's Law. Current evidence does not conclusively support any health hazards associated with such exposure.

To answer your question about the strength of the magnetic field on the ground directly under a typical high-voltage transmission line carrying a 200 A current at a potential of 110 kV, we should first understand the basic physics principle. The magnetic field created by an electric current in a long straight wire forms concentric circles around the wire, and the strength B of the magnetic field is given by Ampere's law.

Ampere's law states that B = μ₀I / 2πr, where B is the magnetic field strength, μ₀ is the permeability of free space (4π × 10^-7 T m/A), I is the current, and r is the distance from the wire. In this case, the transmission line is 20 m above the ground, so r = 20 m. The current I = 200 A. Substituting these values into the equation, we get B = (4π × 10^-7 T m/A * 200 A) / (2π * 20 m) = 2 × 10^-6 T or 2 μT.

So, the strength of the magnetic field on the ground directly under the transmission line is 2 μT, which is less than a tenth of Earth's admittedly weak magnetic field. While there's an ongoing controversy regarding potential health hazards associated with exposure to these electromagnetic fields (E-fields), current evidence does not conclusively support these claims.

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Answer:

b. 0.75 mm

Explanation:

The distance between antinodes d is half the wavelength [tex]\lambda[/tex]. We can obtain the wavelength with the formula [tex]v=\lambda f[/tex], where f is the frequency given ([tex]f=1MHz=1\times10^6Hz[/tex]) and v is the speed of sound in body tissues (v=1540m/s), so putting all together we have:

[tex]d=\frac{\lambda}{2}=\frac{v}{2f}=\frac{1540m/s}{2(1\times10^6Hz)}=0.00077m=0.77mm[/tex]

which is very close to the 0.75mm option.

Answer:

6.36 105 J

Explanation:

In calorimetry all the energy given to a system is converted to heat and the equation for heat is

     Q = m  [tex]c_{e}[/tex] ΔT

The temperature can be in degrees Celsius or Kelvin since the interval between them is the same, substitute and calculate

Q = 1.9 4186 (373-293)  

Q = 6.36 105 J  

This heat equals the energy supplied

Answer:

Explanation:

Total internal reflection refers to a phenomenon that occurs when light travels from a denser medium to less dense medium, in  which the incidence ray is inclined at an angle greater than a certain critical angle to the normal ( angle at which the refracted ray is equal to 90°),  instead of refraction, the ray is reflected back into the material.

since it must start from a denser medium or a medium with higher refractive index, then it must start with plastics

to calculate critical angle,

we use Snell's law

n₁ sin C = n₂ sin r  since r is 90° where n₁ =1.54,    n₂  = 1.33

C = sin⁻¹ ( n₂ / n₁) = sin⁻¹ ( 1.33 / 1.54) = 59.7°

the critical angle = 59.7°

The light must start in the plastic for total internal reflection to occur. The critical angle, which is the angle of incidence where the refracted light is tangential to the boundary, is approximately 59.46 degrees.

For total internal reflection to occur, the light must go from a material with a higher refractive index to one with a lower refractive index. In this case, the light must start in the plastic.

The critical angle is the angle of incidence for which the angle of refraction equals 90 degrees. It can be calculated using Snell's Law (n1*sin(θ1) = n2*sin(θ2)), where n1 and n2 are the refractive indices and θ1 and θ2 are the angles of incidence and refraction, respectively. If we set θ2 to 90 degrees and rearrange the equation we get: θ1 (critical angle) = arcsin(n2/n1).

Plugging in the given index values, we get: θ1 = arcsin(1.33/1.54), which is approximately 59.46 degrees.

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Answer:

Explanation:

Let the velocity of lander with respect to earth be v .

In relativistic mechanism the expression for relative velocity is

v_r = [tex]\frac{v -u}{1-\frac{uv}{c^2}}[/tex]

Given u = .6c , v_r = .8 c

Substituting the values

.8c = [tex]\frac{v -0.6c}{1-\frac{.6c\times v}{c^2} }[/tex]

.8c-.48v = v - .6c

v = .946c

b )

Distance in terms of time = .2 ly

In relativistic mechanism , expression for relativistic time is given by the following relation

t = [tex]\frac{t_0}{\sqrt{1-\frac{v^2}{c^2} }}[/tex]

Substituting v = .946c

t₀ = .2

t = [tex]\frac{.2}{\sqrt{1-\frac{0.946\times .946c^2}{c^2}}}[/tex]

.2 / √.1050

= .62 ly

distance to the Earth at the time of lander launch, as observed by the aliens will be .62 ly.

Final answer:

The speed of the lander as observed on Earth is 0.865c. The distance to the Earth at the time of lander launch, as observed by the aliens, is 0 ly, which is an unreasonable result.

Explanation:

(a) To find the speed of the lander as observed on Earth, we need to use the relativistic velocity addition formula. The formula is given by:

v' = (v1 + v2)/(1 + (v1*v2)/c^2)

Substituting in the values, where v1 = 0.800c and v2 = 0.600c, we get:

v' = (0.800c + 0.600c)/(1 + (0.800c*0.600c)/c^2) = 1.280c/1.480 = 0.865c

So, the speed of the lander as observed on Earth is 0.865c.

(b) To find the distance to the Earth at the time of lander launch, as observed by the aliens, we can use the time dilation formula. The formula is given by:

t' = t/sqrt(1 - (v^2/c^2))

Where t' is the time measured by the aliens, t is the time measured on Earth, v is the velocity of the spaceship relative to Earth, and c is the speed of light.

In this case, t' = 0 (since the lander is launched at the same time as observed on Earth), t = 0.200 ly (given in the question), v = 0.600c (velocity of the spaceship relative to Earth), and c is the speed of light. Substituting the values, we get:

0 = 0.200/sqrt(1 - (0.600c)^2/c^2)

0 = 0.200/sqrt(1 - 0.360)

0 = 0.200/sqrt(0.640)

0 = 0.200/0.8

0 = 0.25

Since 0 = 0.25 is not possible, this result is unreasonable. It suggests that there is a discrepancy in the calculations or assumptions made.

Answer:

[tex]t = 2\ s[/tex]

Explanation:

given,

length of the rope = 16 m

speed of the man = 2 m/s

using the formula of time period

[tex]T =2 \pi \sqrt{\dfrac{L}{g}}[/tex]

[tex]T =2 \pi \sqrt{\dfrac{16}{9.8}}[/tex]

[tex]T = 8.028\ s[/tex]

To cover the maximum distance you need to leave the when the rope is shows maximum displacement.

To reach the displacement time to leave the rope is one fourth of the time period.

[tex]t = \dfrac{T}{4}[/tex]

[tex]t = \dfrac{8.03}{4}[/tex]

[tex]t = 2\ s[/tex]

The time period of pendulum is time taken by it to complete one cycle of swing left to right and right to left.

The total time taken to hang on if you want to drop into the water at the greatest possible distance from the edge is 2 seconds.

The time period of pendulum is time taken by it to complete one cycle of swing left to right and right to left.

It can be given as,

[tex]T=2\pi\sqrt{\dfrac{T}{g}}[/tex]

Here, [tex]g[/tex] is the gravitational force of Earth.

Given information-

Total length of the rope is 16 m.

The speed of the man is 2.0 m/s.

Let the time of to swing by rope both side is [tex]T[/tex]. Thus put the values in the above formula as,

[tex]T=2\pi\sqrt{\dfrac{16}{9.8}}[/tex]

[tex]T=8.028 \rm s[/tex]

Now the greatest possible distance from the edge will be at the greatest displacement.

Thus the time to cove the greatest possible distance will be one forth (1/4) of the total time. Thus,

[tex]t=\dfrac{8.028 }{4}\\t=2\rm s[/tex]

Hence, the total time taken to hang on if you want to drop into the water at the greatest possible distance from the edge is 2 seconds.

Learn more about the time period of pendulum here;

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Answer:

vf₂ = 15.79 m/s

Explanation:

Theory of collisions  

Linear momentum is a vector magnitude (same direction of the velocity) and its magnitude is calculated like this:  

p=m*v  

where  

p:Linear momentum  

m: mass  

v:velocity  

There are 3 cases of collisions : elastic, inelastic and plastic.  

For the three cases the total linear momentum quantity is conserved:  

P₀ = Pf  Formula (1)  

P₀ :Initial linear momentum quantity  

Pf : Final linear momentum quantity  

Data

m₁ = 2600 kg : mass of the rhino

m₂= 0.18 kg : mass of the ball

v₀₁ = 3.70 m/s  : initial velocity of the rhino

v₀₂= - 8.39 m/s, initial velocity of the ball

Problem development

We appy the formula (1):

P₀ = Pf  

m₁*v₀₁ + m₂*v₀₂ = m₁*vf₁ + m₂*vf₂  

(2600)*(3.7) + (0.18)*(- 8.39) = (2600)*vf₁ +(0.18)*vf₂

9620 -1.5102 = (2600)*vf₁ +(0.18)*vf₂

9618.4898 = (2600)*vf₁ +(0.18)*vf₂ Equation (1)

Because the shock is elastic, the coefficient of elastic restitution (e) is equal to 1.

[tex]e = \frac{v_{f2}-v_{f1} }{v_{o1}-v_{o2}}[/tex]

1*( v₀₁- v₀₂ )  = (vf₂ -vf₁)

( 3.7 -( -8.39 )  = (vf₂ -vf₁)

12.09 =  (vf₂ -vf₁)

vf₂ = vf₁ + 12.09 Equation (2)

We replace Equation (2) in the Equation (1)

9618.4898 = (2600)*vf₁ +(0.18)*vf₂

9618.4898 = (2600)*vf₁ +(0.18)* (vf₁ + 12.09)

9618.4898 = (2600)*vf₁ +(0.18)*vf₁ + (0.18)(12.09)

9618.4898 = (2600)*vf₁ +(0.18)*vf₁ + 2.1762

9618.4898 -2.1762 = (2600.18)*vf₁

9616.3136 = (2600.18)*vf₁  

vf₁ = (9616.3136) / (2600.18)

vf₁ = 3.698 m/s : Final velocity of the rhino

We replace vf₁ = 3.698 m/s in the Equation (2)

vf₂ = vf₁ + 12.09

vf₂ = 3.698 + 12.09

vf₂ = 15.79 m/s : Final velocity of the ball

The speed of the ball after it bounces back elastically toward you is 8.39 m/s.

To solve this problem, we can use the principle of conservation of momentum and the fact that the collision is elastic. In an elastic collision, both momentum and kinetic energy are conserved.

Using the conservation of momentum:

[tex]\[ m_r v_{r,i} + m_b v_{b,i} = m_r v_{r,f} + m_b v_{b,f} \][/tex]

Since the rhino is much more massive than the ball, its velocity will change very little after the collision.  This assumption is valid in the limit where the mass of one object is much larger than the other, which is the case here.

With this assumption, the conservation of momentum simplifies to:

[tex]\[ m_b v_{b,i} = m_b v_{b,f} \][/tex]

Since the mass of the ball cancels out, we find that:

[tex]\[ v_{b,f} = v_{b,i} \][/tex]

This means that the speed of the ball after the collision is the same as before the collision, which is 8.39 m/s, but in the opposite direction.

Additionally, in an elastic collision, the relative speed of approach is equal to the relative speed of separation. Since the rhino's speed is much greater than the ball's speed, the ball will essentially rebound with the same speed it had before the collision but in the opposite direction.

Answer:

1.1775 x 10^-3 m^3 /s

Explanation:

viscosity, η = 0.250 Ns/m^2

radius, r = 5 mm = 5 x 10^-3 m

length, l = 25 cm = 0.25 m

Pressure, P = 300 kPa = 300000 Pa

According to the Poisuellie's formula

Volume flow per unit time is

[tex]V=\frac{\pi \times Pr^{4}}{8\eta l}[/tex]

[tex]V=\frac{3.14 \times 300000\times \left ( 5\times 10^{-3} \right )^{4}}{8\times 0.250\times 0.25}[/tex]

V = 1.1775 x 10^-3 m^3 /s

Thus, the volume of oil flowing per second is 1.1775 x 10^-3 m^3 /s.

Answer:

3 300 J

Explanation:

Work done, mathematically speaking,  is the distance moved multiplied by the force exerted in the only in direction of motion. In this question therefore we will multiply the distance by the component of the force that moved the car forward

W = Fdcosθ

    = 210 N  * 18 * Cos 30°

    = 3 300 J

The work done by Steve while pushing the car 18 meters at an angle of 30 degrees, applying a force of 210N, is calculated to be 3465 joules using the formula: Work = Force x distance x cos(angle).

The subject of this question is Physics, specifically the concept of work done by a force. In physics, work is defined as the product of the component of the force in the direction of the displacement and the magnitude of this displacement.

For Steve's situation, we can calculate the work done using the formula: Work = Force x distance x cos(angle). Given the parameters: Force = 210N, Distance = 18m, and Angle = 30 degrees, we get:

Work = 210N x 18m x cos(30) = 3465 J

So, Steve does 3465 Joules of work to push the car 18 meters under these conditions. This example illustrates how the angle at which force is applied can affect the work output, a key principle in physics.

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To determine the average force exerted by her hands on the ball while catching it, we can use the equation F = m * a. First, we find the initial velocity at the top of the ball's trajectory. Then, we calculate the acceleration using the change in velocity and time. Finally, we can find the force using the mass and acceleration.

To determine the average force that her hands exert on the ball while catching it, we can use the equation F = m * a, where F is the force, m is the mass of the ball, and a is the acceleration. First, we need to find the acceleration of the ball. We can use the equation a = Δv / Δt, where Δv is the change in velocity and Δt is the change in time. Since the ball stops in 0.10 s, the change in velocity is equal to the initial velocity, which is the velocity at the top of the ball's trajectory. Using the equation v = u + a * t, where v is the final velocity, u is the initial velocity, a is the acceleration, and t is the time taken, we can find the initial velocity at the top of the trajectory. The initial velocity can be determined using the equation v² = u² + 2as, where s is the vertical distance traveled. Substituting the known values, we can find the initial velocity. Once we have the initial velocity, we can use it to calculate the acceleration, and finally the force.

Let's go step by step. First, we need to find the initial velocity at the top of the trajectory. Using the equation v² = u² + 2as, where v is the final velocity (0 m/s at the top), u is the initial velocity, a is the acceleration (-9.8 m/s²), and s is the vertical distance traveled (1.2 m), we can solve for u: 0 = u² + 2(-9.8 m/s²)(1.2 m). Solving for u, we get u = 3.13 m/s. Now that we have the value of the initial velocity, we can find the acceleration using the equation a = (v - u) / t, where v is the final velocity (0 m/s), u is the initial velocity (3.13 m/s), and t is the time taken (0.10 s). Substituting the values, we get a = (0 m/s - 3.13 m/s) / 0.10 s = -31.3 m/s². Finally, we can calculate the force using the equation F = m * a, where m is the mass of the ball (0.60 kg) and a is the acceleration (-31.3 m/s²). Substituting the values, we get F = (0.60 kg)(-31.3 m/s²) = -18.78 N. Since force is a vector quantity, it is important to note that we have considered the negative sign in the calculation, which indicates that the force is directed upwards.

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The force exerted is approximately 29.1 N in the opposite direction of the ball's motion.

Determining the Average Force Exerted on a Falling Basketball

To find the average force exerted by the player's hands while catching the falling basketball, we need to understand a few key physics concepts involving motion and force.

Steps to Calculate the Average Force:

Calculate the velocity of the ball just before it is caught: Using the equation for free fall, we can determine the final velocity (v) of the ball just before it reaches the player's hands:

[tex]v^2 = u^2[/tex]+ 2gh, where u = initial velocity (0 m/s), g = acceleration due to gravity (9.8 m/s²), and h = height (1.2 m)

[tex]v^2[/tex] = 0 + 2(9.8)(1.2)

[tex]v^2[/tex]= 23.52

v = [tex]\sqrt{23.52}[/tex]≈ 4.85 m/s

Calculate the change in momentum: The change in momentum, or impulse, occurs as the ball is caught and brought to a stop in the player's hands. The ball's mass is 0.60 kg.

Impulse = change in momentum = m x (v - u)

Impulse = 0.60 kg x (0 m/s - 4.85 m/s)

Impulse = -2.91 kg·m/s

Determine the average force: We use the equation for impulse, Impulse = F_avg x Δt, where Δt = time duration (0.10 s).

-2.91 kg·m/s = F_avg x 0.10 s

F_avg = -2.91 kg·m/s / 0.10 s

F_avg ≈ -29.1 N

The negative sign indicates that the force is exerted in the opposite direction of the ball's motion, which is typical for a decelerating force.

Answer:

doubled the initial value

Explanation:

Let the area of plates be A and the separation between them is d.

Let V be the potential difference of the battery.

The energy stored in the capacitor is given by

U = Q^2/2C   ...(1)

Now the battery is disconnected, it means the charge is constant.

the separation between the plates is doubled.

The capacitance of the parallel plate capacitor is inversely proportional to the distance between the plates.

C' = C/2

the new energy stored

U' = Q^2 /  2C'

U' = Q^2/C = 2 U

The energy stored in the capacitor is doubled the initial amount.

Answer:

Ff = 6058.5N

Explanation:

The sum of forces is:

[tex]Ff = m*a_c[/tex]

[tex]Ff = m*V^2/R[/tex]

[tex]Ff = 1900*13^2/53[/tex]

[tex]Ff = 6058.5N[/tex]

Answer:

A)A=0.075 m

B)v= 0.21 m/s

Explanation:

Given that

m = 0.75 kg

K= 13.5 N

The natural frequency of the block given as

[tex]\omega =\sqrt{\dfrac{K}{m}}[/tex]

The maximum speed v given as

[tex]v=\omega A[/tex]

A=Amplitude

[tex]v=\sqrt{\dfrac{K}{m}}\times A[/tex]

[tex]0.32=\sqrt{\dfrac{13.5}{0.75}}\times A[/tex]

A=0.075 m

A= 0.75 cm

The speed at distance x

[tex]v=\omega \sqrt{A^2-x^2}[/tex]

[tex]v=\sqrt{\dfrac{K}{m}}\times \sqrt{A^2-x^2}[/tex]

[tex]v=\sqrt{\dfrac{13.5}{0.75}}\times \sqrt{0.075^2-(0.075\times 0.75)^2}[/tex]

v= 0.21 m/s

The amplitude of the subsequent oscillations can be calculated using the formula for potential energy and the initial kinetic energy. The block's speed at a given point can be found using the conservation of mechanical energy and the equation for kinetic energy.

To determine the amplitude of the subsequent oscillations, we need to first calculate the potential energy stored in the spring when the block is hit. Since the block is moving at a speed of 32.0 cm/s, we can calculate its kinetic energy. We can then equate this kinetic energy to the potential energy of the spring, using the formula potential energy = (1/2) * k * A^2, where k is the spring constant and A is the amplitude. Rearranging the formula, we find that the amplitude is equal to the square root of (2 * kinetic energy / k).

To find the block's speed when x = 0.750 A, we can use the conservation of mechanical energy. At the maximum displacement, all the energy is converted between potential and kinetic energy. At this point, the potential energy is zero, so the kinetic energy is equal to the initial kinetic energy. Using the formula for kinetic energy, we can find the speed when x = 0.750 A using the equation kinetic energy = (1/2) * k * (x^2 - A^2) and solving for the speed.

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To develop this problem it is necessary to apply the concepts related to the proportion of a neutron star referring to the sun and density as a function of mass and volume.

Mathematically it can be expressed as

[tex]\rho = \frac{m}{V}[/tex]

Where

m = Mass (Neutron at this case)

V = Volume

The mass of the neutron star is 1.4times to that of the mass of the sun

The volume of a sphere is determined by the equation

[tex]V = \frac{4}{3}\pi R^3[/tex]

Replacing at the equation we have that

[tex]\rho = \frac{1.4m_{sun}}{\frac{4}{3}\pi R^3}[/tex]

[tex]\rho = \frac{1.4(1.989*10^{30})}{\frac{4}{3}\pi (1.05*10^4)^3}[/tex]

[tex]\rho = 5.75*10^{17}kg/m^3[/tex]

Therefore the density of a neutron star is [tex] 5.75*10^{17}kg/m^3[/tex]

Explanation:

Given that,

Force, [tex]F=((-8i)+6j)\ N[/tex]

Position of the particle, [tex]r=(3i+4j)\ m[/tex]

(a) The toque on a particle about the origin is given by :

[tex]\tau=F\times r[/tex]

[tex]\tau=((-8i)+6j) \times (3i+4j)[/tex]

Taking the cross product of above two vectors, we get the value of torque as :

[tex]\tau=(0+0-50k)\ N-m[/tex]

(b) Let [tex]\theta[/tex] is the angle between r and F. The angle between two vectors is given by :

[tex]cos\theta=\dfrac{r.F}{|r|.|F|}[/tex]

[tex]cos\theta=\dfrac{(3i+4j).((-8i)+6j)}{(\sqrt{3^2+4^2} ).(\sqrt{8^2+6^2}) }[/tex]

[tex]cos\theta=\dfrac{0}{50}[/tex]

[tex]\theta=90^{\circ}[/tex]

Li+  [He]

N³-  [Ne]

In³+  [Kr] 4d10

Tl+  [Xe] 4f14 5d10 6S2

The ground-state electron configuration of the ions Li+, N3−, In3+, and Tl+ are [He], [Ne], [Kr]4d10, and [Xe]4f145d106s26p1 respectively. This notation suggests these ions have similar electronic structures to the noble gases and additional electrons in certain cases.

The ground-state electron configurations of the ions Li+, N3−, In3+, and Tl+ can be described using the noble gas core electron configuration. The noble gas core is essentially the electron configuration of the closest noble gas with less atomic number than the atom we are considering.

(a) Li+ has lost an electron compared to neutral Lithium. Its electron configuration becomes [He] - it resembles helium, a noble gas.

(b) N3− has gained three electrons compared to neutral Nitrogen and its electron configuration becomes [Ne] - it resembles neon, a noble gas.

(c) In3+ has lost three electrons compared to neutral Indium. Its electron configuration becomes [Kr]4d10 - core is like Kr (krypton), a noble gas, plus 10 electrons added in the d orbital.

(d) Tl+ has lost one electron compared to neutral Thallium and its electron configuration is [Xe]4f145d106s26p1 - core is like Xe (xenon), a noble gas, plus additional electrons.

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To develop this problem it is necessary to apply the related concepts at relative speed.

When an observer perceives the relative speed of a second observer, the function is described,

[tex]v' = \frac{v_1-v_2}{1-\frac{v_1v_2}{c^2}}[/tex]

Where,

[tex]v_1[/tex] = The velocity of the first escape pod

[tex]v_2[/tex] = The velocity of the second escape pod

c = Speed of light

v' = Speed of the first escape pod relative to the second escape pod.

Our values are given as,

[tex]v_1[/tex]= 0.7c

[tex]v_2[/tex]= -0.76c

Replacing we have,

[tex]v' = \frac{v_1-v_2}{1-\frac{v_1v_2}{c^2}}[/tex]

[tex]v' = \frac{0.7c-(-0.76c)}{1-\frac{(0.7c)(-0.76c)}{(3*10^8)^2}}[/tex]

[tex]v' = \frac{0.7c-(-0.76c)}{1-\frac{(0.7c)(-0.76c)}{(3*10^8)^2}}[/tex]

[tex]v' = 2.85*10^8m/s[/tex]

Therefore the speed of the first escape pod measure for the second escape pod is [tex]v' = 2.85*10^8m/s[/tex]

The relative speed of the second escape pod as measured by the first escape pod, using relativistic velocity addition, is approximately -0.04c (or just 0.04c considering the magnitude), where c is the speed of light.

The question involves calculating the relative speed of one escape pod as observed by the other escape pod in a scenario where they are moving in opposite directions. To do this, we must use the formula for relativistic velocity addition. The formula is as follows:

V = (v1 + v2) / (1 + v1*v2/c²),

where V is the relative velocity as measured by one escape pod, v1 and v2 are the velocities of the escape pods, and c is the speed of light. For this particular problem:

We substitute the values into the relativistic velocity addition formula to find the relative speed:

V = (0.70c - 0.76c) / (1 - 0.70*(-0.76)c²/c²)

Doing the calculations:

V = -0.06c / (1 + 0.532)c²/c²)

V = -0.06c / 1.532

V = -0.039c ≈ -0.04c

The negative sign indicates that the second escape pod is moving in the direction opposite to the first pod as measured by the first pod. It's important to keep in mind that this result is only an approximation, rounded to two significant figures as per the question's request.

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Explanation:

Red dwarf and brown dwarf masses are less than a typical white dwarf mass measuring around 1.2 solar masses. But it's only a few kilometers of the radius. This is precisely because there is no force to overcome the contraction due to gravity. There is a constant  battle between the external force of fusion (who wants to expand the star) and inward pressure because of gravity (who wants to compact the star) of regular stars on the main sequence. There remains a balance between these two forces as long as the star remains on the celestial equator.

Red dwarfs are helped by the nuclear fusion force, but brown dwarfs were not large enough to cause the fusion of hydrogen, they are massive enough to generate sufficient energy in the core by fusing deuterium to sustain their volume.  However as soon as the star runs out of hydrogen to burn it weakens the force of the external fusion and gravity starts to compact the center of the star. The contraction heats up the core into more massive stars and helium fusion begins, rendering the star once again stable. However this helium fusion does not occur in stars with masses below 1.44Mo. Tightness persists for such stars until the star's gasses degenerate.

Answer:

27.66 s

Explanation:

Space station creates artificial gravity by rotational movement about its axis .

The object inside also move in circular motion creating centrifugal force which creates acceleration in them .

centrifugal acceleration = ω² R where ω is angular velocity and R is radius of the cylindrical space station .

R = 380 /2 = 190 m

Given

ω² R = g = 9.8

ω² = 9.8 / R

= 9.8 / 190

= 5.15x 10⁻²

ω = 2.27 x 10⁻¹

= .227 rad / s

2π / T = .227 ( T is time period of rotation )

T = 2π / .227

= 27.66 s .

outside of the space station they will experience zero acceleration , because they are rotating around the earth.

Answer:

15.57 g/cm³

Explanation:

[tex]\rho_g[/tex] = Density of gold = 19.3 g/cm³

[tex]\rho_s[/tex] = Density of silver = 10.5 g/cm³

[tex]\rho_c[/tex] = Density of copper = 8.9 g/cm³

Assuming total mass as 1000 g

Volume of gold

[tex]V_g=\frac{0.75\times 1000}{19.3}\\\Rightarrow V_g=38.86\ cm^3[/tex]

Volume of silver

[tex]V_g=\frac{0.16\times 1000}{10.5}\\\Rightarrow V_g=15.238\ cm^3[/tex]

Volume of copper

[tex]V_c=\frac{0.09\times 1000}{8.9}\\\Rightarrow V_c=10.11\ cm^3[/tex]

Density of the alloy would be

[tex]\rho=\frac{M}{V_g+V_s+V_c}\\\Rightarrow \rho=\frac{1000}{38.86+15.238+10.11}\\\Rightarrow \rho=15.57\ g/cm^3[/tex]

The overall density of this alloy is 15.57 g/cm³

The overall density of an 18-karat gold alloy, which consists of 75% gold, 16% silver, and 9% copper, is approximately 15.2 grams per cubic centimeter given the known densities of the pure metals.

The density of an alloy (a mixture of metals) is calculated by finding the volume-weighted average of the densities of the constituent metals. In the case of 18-karat gold, we have a mixture of 75% gold, 16% silver, and 9% copper. Using the given densities of these metals, we can calculate the overall density of the alloy as follows:

rho18kt = 0.75*rhogold+0.16*rhosilver+0.09*rhocopper = 0.75*19.3g/cm³+0.16*10.5g/cm³+0.09*8.90g/cm³ = 15.2g/cm³.

Therefore, the overall density of the 18-karat gold alloy, rho18kt, is approximately 15.2g/cm³.

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Answer:

W = 0.384 J

Explanation:

Work and energy in the rotational movement are related

    W = ΔK = [tex]K_{f}[/tex] - K₀

    W = ½ I [tex]w_{f}[/tex]² - 1 /2 I w₀²

where W isthe work, I is the moment of inertia and w angular velocity

With the system part of the rest the initial angular speed is zero (w₀ = 0)

The angular and linear quantities are related

    v = w r

    w = v / r

Let's replace

    W = ½ I (v / r)²

Let's calculate

    W = ½  1.2 10⁻⁴ 1.2² / (1.5 10⁻²)²

    W = 0.384 J

    W = 38.4 J

Answer:

Explanation:

Let length of the pendulum be l . The expression for time period of pendulum is as follows

T = 2π[tex]\sqrt{\frac{l}{g} }[/tex]

For Mars planet ,

1.5 = [tex]2\pi\sqrt{\frac{l}{.38\times9.8} }[/tex]

For other planet

.92 = [tex]2\pi\sqrt{\frac{l}{g_1} }[/tex]

Squiring and dividing the two equations

[tex]\frac{1.5^2}{.92^2} = \frac{g_1}{3.8\times9.8}[/tex]

[tex]g_1 = 9.9[/tex]

The second planet appears to be earth.

Answer:

Explanation:

Distance between plates d = 2 x 10⁻³m

Potential diff applied = 5 x 10³ V

Electric field = Potential diff applied /  d

= 5 x 10³  / 2 x 10⁻³

= 2.5 x 10⁶ V/m

This is less than  breakdown strength for air  3.0×10⁶ V/m

b ) Let the plates be at a separation of d .so

5 x 10³ / d = 3.0×10⁶ ( break down voltage )

d = 5 x 10³  / 3.0×10⁶

= 1.67 x 10⁻³ m

= 1.67 mm.

The measured length when the temperature rises to 29.4°C is 17.712 m.

To answer this question, we need to consider the thermal expansion of the steel tape and the aluminum support column. The coefficient of linear expansion for the steel tape is not given, so we will assume it to be the same as iron, which is approximately 12x10-6/°C.

We can use the formula:

ΔL = αL₀ΔT

where ΔL is the change in length, α is the coefficient of linear expansion, L₀ is the initial length, and ΔT is the change in temperature.

Given that the initial length (L₀) is 17.700 m and the initial temperature is 21.2°C, we can calculate the change in length (ΔL) when the temperature rises to 29.4°C.

ΔL = (12x10-6)(17.700)(29.4 - 21.2) = 0.01226352 m

Therefore, the measured length when the temperature rises to 29.4°C is 17.700 + 0.01226352 = 17.712 m (rounded to three decimal places).

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The change in length of the aluminum column when the temperature rises can be found using the equation ∆L = αL0∆T, where ∆L is the change in length, α is the coefficient of linear expansion, L0 is the initial length, and ∆T is the change in temperature. Plugging in the values provided, we find the change in length is 3.25848 x 10-4 m, rounded to three decimal places.

When a material undergoes thermal expansion, its length increases as the temperature rises. To calculate the change in length, we can use the equation ∆L = αL0∆T, where ∆L is the change in length, α is the coefficient of linear expansion, L0 is the initial length, and ∆T is the change in temperature. In this case, we need to find the change in length of the aluminum column when the temperature rises from 21.2°C to 29.4°C.

First, we need to determine the coefficient of linear expansion for aluminum. Using the information provided, we can find that the coefficient of linear expansion for aluminum is approximately 22·10-6 °C-1.

Next, we can plug in the values into the equation. Given L0 = 17.700 m, ∆T = (29.4 - 21.2)°C = 8.2°C, and α = 22·10-6 °C-1, we can calculate ∆L as follows:

∆L = (22·10-6 °C-1)(17.700 m)(8.2°C) = 3.25848 x 10-4 m

Rounded to three decimal places, the measured length of the aluminum support column when the temperature rises to 29.4°C is 0.000 m.

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Explanation:

The angular momentum is given by the moment of inertia, multiplied by the angular speed of the rotating body:

[tex]L=I\omega[/tex]

The angular speed is given by:

[tex]\omega=2\pi f\\\omega=2\pi 5.2\frac{rev}{s}\\\omega=32.67\frac{rad}{s}[/tex]

Now, we calculate the angular momentum:

[tex]L=0.32kg\cdot m^2(32.67\frac{rad}{s})\\L=10.45\frac{kg\cdot m^2}{s}[/tex]

The average torque is defined as:

[tex]\tau=I\alpha[/tex]

[tex]\alpha[/tex] is the angular acceleration, which is defined as:

[tex]\alpha=\frac{\omega_f-\omega_0}{t}[/tex]

We have to calculate [tex]\omega_f[/tex]:

[tex]\omega_f=2\pi (2.75\frac{rad}{s})\\\omega_f=17.28\frac{rad}{s}[/tex]

Now, we calculate the angular acceleration:

[tex]\alpha=\frac{17.28\frac{rad}{s}-32.67\frac{rad}{s}}{12s}\\\alpha=-1.28\frac{rad}{s^2}[/tex]

Finally, we can know the average torque:

[tex]\tau=0.32kg\cdot m^2(-1.28\frac{rad}{s^2})\\\tau=-0.41N\cdot m[/tex]

(a) The angular momentum of the skater is 10.45 kgm²/s

(b) The magnitude of the average torque that was exerted, is 0.41 Nm.

The angular momentum of the skater is calculated as follows;

L = Iω

where;

ω = 5.2 rev/s x 2π rad = 32.67 rad/s

L = 0.32 x 32.67

L = 10.45 kgm²/s

The angular acceleration is calculated as follows;

[tex]\alpha= \frac{\omega _f - \omega _i}{t}[/tex]

[tex]\alpha = \frac{17.28 -32.67 }{12} \\\\\alpha = -1.28 \ rad/s^2[/tex]

The magnitude of the average torque that was exerted, is calculated as;

τ = Iα

τ = 0.32 x (1.28)

τ = 0.41 Nm.

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