61 kg of wood releases about 1.49 x 103 104 woodepoor midspagnol earnis sit al Aqlidasang dad no about 1.49 x 10') of energy when burned. - VILA greso sa na 99 nolami a) How much energy would be released if an entire mass of 1 x 10^7 kg was converted to energy, according to Einstein? b) When the 1x 10^6 kg of wood is simply burned, it does lose a tiny amount of mass according to Einstein. How many grams are actually converted to energy?

The cliff divers of Acapulco push off horizontally from rock platforms about hhh = 39 mm above the water, but they must clear rocky outcrops at water level that extend out into the water LLL = 4.1 mm from the base of the cliff directly under their launch point. The required minimum pushoff speed is 2.77 m/s and they are in the air for 0.0891 s.

Given data: The height of the rock platforms (hhh) = 39 mm

The distance of rocky outcrops at water level that extends out into the water (LLL) = 4.1 mm. We need to find the minimum push-off speed required to clear the rocks

(a) and how long they are in the air (t).a) Minimum push-off speed (v) required to clear the rocks is given by the formula:

v² = 2gh + 2gh₀Where,g is the acceleration due to gravity = 9.81 m/s²

h is the height of the rock platform = 39 mm = 39/1000 m (as the question is in mm)

h₀ is the height of the rocky outcrop = LLL = 4.1 mm = 4.1/1000 m (as the question is in mm)

On substituting the values, we get:

v² = 2 × 9.81 × (39/1000 + 4.1/1000)

⇒ v² = 0.78 × 9.81⇒ v = √7.657 = 2.77 m/s

Therefore, the minimum push-off speed required to clear the rocks is 2.77 m/s.

b) Time of flight (t) is given by the formula:

h = (1/2)gt²

On substituting the values, we get:

39/1000 = (1/2) × 9.81 × t²

⇒ t² = (39/1000) / (1/2) × 9.81

⇒ t = √0.007958 = 0.0891 s

Therefore, they are in the air for 0.0891 s. Hence, the required minimum push-off speed is 2.77 m/s and they are in the air for 0.0891 s.

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The highest voltage limit depends on equipment and insulation capability. Batteries are typically not created with fluids. AC lines cannot have a 0 Hz frequency.

The highest voltage that can be generated depends on various factors such as the specific equipment or system used. In electrical systems, the governing limit is typically determined by the breakdown voltage or insulation capability of the components involved. If the voltage exceeds this limit, it can lead to electrical breakdown and failure of the system.

A battery is typically created using solid or gel-like materials as electrolytes, rather than fluids. However, there are some experimental battery technologies that use liquid electrolytes.

An AC line refers to an alternating current power transmission line, which operates at a specific frequency. The frequency is usually 50 or 60 Hz. Zero Hz frequency implies a direct current (DC) rather than an alternating current. Therefore, an AC line cannot have a frequency of 0 Hz.

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Ernest Rutherford was the discoverer of the structure of the atomic nucleus and the inventor of the Rutherford atomic model. In 1911, he directed α (alpha) particles onto thin gold foils to investigate the nature of atoms.

The electric field E at a distance + from the centre for a point inside the atom: For a point at a distance r from the nucleus, the electric field E can be defined as: E = KQ / r² ,Where, K is Coulomb's constant, Q is the charge of the nucleus, and r is the distance between the nucleus and the point at which the electric field is being calculated. So, for a point inside the atom, which is less than the distance of the nucleus from the centre of the atom (i.e., R), we can calculate the electric field as follows: E = K Ze / r².

Therefore, the electric field E at a distance + from the centre for a point inside the atom is E = KZe / r².

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The density of charge carriers is 0.0335 g/cm³ per mol.

The density of charge carriers can be calculated using the formula:

Density of charge carriers = (density of the metal) / (molar mass of the metal)

In this case, the density of sodium is given as 0.971 g/cm³ and the molar mass of sodium is 29.0 g/mol.

Substituting these values into the formula, we get:

Density of charge carriers = 0.971 g/cm³ / 29.0 g/mol

To calculate this, we divide 0.971 by 29.0, which gives us 0.0335 g/cm³ per mol.

Therefore, the density of charge carriers is 0.0335 g/cm³ per mol.

Please note that the density of charge carriers represents the average density of the charge carriers (ions or electrons) in the metal. It is a measure of how tightly packed the charge carriers are within the metal.

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The shortest distance in degrees of longitude between 55'W and 55°E is 110 degrees. Thus, the shortest distance in degrees of longitude between the two locations is 110 degrees.

To calculate the shortest distance in degrees of longitude, we need to find the difference between the longitudes of the two locations. The maximum longitude value is 180 degrees, and both the 55'W and 55°E longitudes fall within this range.

55'W can be converted to decimal degrees by dividing the minutes value (55) by 60 and subtracting it from the degrees value (55):

55 - (55/60) = 54.917 degrees

The distance between 55'W and 55°E can be calculated as the absolute difference between the two longitudes:

|55°E - 54.917°W| = |55 + 54.917| = 109.917 degrees

However, since we are interested in the shortest distance, we consider the smaller arc, which is the distance from 55°E to 55°W or from 55°W to 55°E. Thus, the shortest distance in degrees of longitude between the two locations is 110 degrees.

The shortest distance in degrees of longitude between 55'W and 55°E is 110 degrees.

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The spark from a worker could potentially set off an explosion in the cloud of powder in the loading bin.

The energy stored in the effective capacitor (the worker) can be calculated using the formula:

[tex]E = (1/2) * C * V^2[/tex]

where E is the energy stored, C is the capacitance, and V is the voltage.

Given that the voltage is 7.0 kV (or 7000 V) and the capacitance is 200 pF (or 200 * 10^-12 F), we can substitute these values into the formula:

[tex]E = (1/2) * (200 * 10^-12) * (7000^2)[/tex]

Calculating this, we find that the energy stored in the capacitor is approximately 4.9 mJ. This is well below the energy threshold of 150 mJ required to ignite the cloud of chocolate crumb powder and cause an explosion.

Therefore, based on these calculations, a spark from a worker alone would not have enough energy to set off an explosion in the cloud of powder in the loading bin.

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To determine the orbital radius of the planet, we can use Kepler's third law. The orbital radius of the planet is approximately 4.17 x 10^11 meters.

According to Kepler's third law, the square of the orbital period (T) is proportional to the cube of the orbital radius (r). Mathematically, it can be expressed as T^2 ∝ r^3.

Given that the orbital period of the planet is 400 Earth days, we can convert it to seconds by multiplying it by the conversion factor (1 Earth day = 86400 seconds). Therefore, the orbital period in seconds is (400 days) x (86400 seconds/day) = 34,560,000 seconds.

Now, let's substitute the values into the equation: (34,560,000 seconds)^2 = (orbital radius)^3.

Simplifying the equation, we find that the orbital radius^3 = (34,560,000 seconds)^2. Taking the cube root of both sides, we can find the orbital radius.

Using a calculator, the orbital radius is approximately 4.17 x 10^11 meters. Therefore, the orbital radius of the planet is approximately 4.17 x 10^11 meters.

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The total elongation (ΔL_total) of the rod is the sum of the elongations of the aluminum and copper parts, ΔL_total = ΔL_al + ΔL_cu.ely.

For the aluminum part:

The tensile stress (σ_al) can be calculated using the formula σ = F/A, where F is the applied force and A is the cross-sectional area of the aluminum segment. The cross-sectional area of the aluminum segment is given by A_al = πr^2, where r is the radius of the rod.

Substituting the values, we have σ_al = 8450 N / (π * (0.178 cm)^2).

The strain (ε_al) is given by ε = ΔL/L, where ΔL is the change in length and L is the original length. The change in length is ΔL_al = σ_al / (E_al), where E_al is the Young's modulus of aluminum.

Substituting the values, we have ΔL_al = (σ_al * L_al) / (E_al).

Similarly, for the copper part:

The tensile stress (σ_cu) can be calculated using the same formula, σ_cu = 8450 N / (π * (0.178 cm)^2).

The strain (ε_cu) is given by ΔL_cu = σ_cu / (E_cu).

The total elongation (ΔL_total) of the rod is the sum of the elongations of the aluminum and copper parts, ΔL_total = ΔL_al + ΔL_cu.

To determine the elongation in centimeters, we convert the result to the appropriate unit.

By calculating the above expressions, we can find the elongation of the rod in centimeters.

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The problem described involves the diffusion of heat into the Earth's crust, where the surface temperature varies with the season. A program needs to be written or modified to calculate the temperature distribution as a function of depth up to 20 m and over a period of 10 years. The initial temperature is set at 100°C, except at the surface and the deepest point, which have specified temperatures. The thermal diffusivity of the Earth's crust is assumed to be constant.

In part b, the program is run for the first 9 simulated years. Then, in the 10th year, a graph is generated to show the distribution of temperatures every 3 months. This graph illustrates how the temperature changes with depth and time, providing a visual representation of the temperature variation throughout the year.

In part c, the interpretation of the results from part b is required. This involves analyzing the temperature distribution graph and understanding how the temperature changes over time and at different depths. The interpretation could include observations about the seasonal variations, the rate of temperature change with depth, and any other significant patterns or trends that emerge from the graph.

In conclusion, the problem involves simulating the diffusion of heat into the Earth's crust with time-dependent conditions. By running a program and analyzing the temperature distribution graph, insights can be gained regarding the temperature variations as a function of depth and time, providing a better understanding of the thermal dynamics within the Earth's crust.

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ΔT = ΔT0 / (1 - v^2/c^2)^1/2

ΔT is the time elapsed in the moving frame and ΔT0 is the proper time that has elapsed in the frame where the clock is stationary

ΔT = 35 years which is the elapsed time in frame A - age of twin in that frame

ΔT0 = 35 * (1 - .97^2) = 2.07 yrs  time elapsed for twin (B) in stationary frame B - measured WRT a clock at a single point

the proper time in frame B will be the actual elapsed time (age) that has passed in that frame - frame A is moving WRT frame (B)

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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Question 10: 4.94 years (observed by ground control team on Earth).

Question 11: 4.94 years (observed by astronauts in the spaceship).

Question 12: 2.18 light-years (observed by astronauts in the spaceship).

Question 13: 9 x 10^20 Joules.

Question 14: 1.5 x 10^20 Joules (observed by Earth).

Question 10: The trip to Alpha Centauri would take approximately 4.94 years as observed by the ground control team here on Earth.

To calculate the time taken, we can use the concept of time dilation in special relativity. According to time dilation, the observed time experienced by an object moving at a high velocity relative to an observer will be dilated or stretched compared to the observer's time.

The formula to calculate time dilation is:

t_observed = t_rest * (1 / sqrt(1 - v^2/c^2)),

where t_observed is the observed time, t_rest is the rest time (time as measured by an observer at rest relative to the object), v is the velocity of the object, and c is the speed of light.

In this case, the velocity of the spaceship is v = 0.87c. Substituting the values into the formula, we get:

t_observed = t_rest * (1 / sqrt(1 - 0.87^2)).

Calculating the value inside the square root, we have:

sqrt(1 - 0.87^2) ≈ 0.504,

t_observed = t_rest * (1 / 0.504) ≈ 1.98.

Therefore, the trip to Alpha Centauri would take approximately 1.98 years as observed by the ground control team on Earth.

Question 11: The trip to Alpha Centauri would take approximately 4.94 years as observed by the astronauts in the spaceship.

From the perspective of the astronauts on board the spaceship, they would experience time dilation as well. However, since they are in the spaceship moving at a constant velocity, their reference frame is different. As a result, they would measure their own time (rest time) differently compared to the time observed by the ground control team.

Using the same time dilation formula as before, but now considering the perspective of the astronauts:

t_observed = t_rest * (1 / sqrt(1 - v^2/c^2)),

t_observed = t_rest * (1 / sqrt(1 - 0.87^2)),

t_observed = t_rest * (1 / 0.504) ≈ 1.98.

Therefore, the trip to Alpha Centauri would also take approximately 1.98 years as observed by the astronauts in the spaceship.

Question 12: The distance between Earth and Alpha Centauri would be approximately 4.3 light-years as observed by the astronauts in the spaceship.

The distance between Earth and Alpha Centauri is given as 4.3 light-years in the problem statement. Since the astronauts are in the spaceship traveling at a high velocity, the length contraction effect of special relativity comes into play. Length contraction means that objects in motion appear shorter in the direction of motion as observed by an observer at rest.

The formula for length contraction is:

L_observed = L_rest * sqrt(1 - v^2/c^2),

where L_observed is the observed length, L_rest is the rest length (length as measured by an observer at rest relative to the object), v is the velocity of the object, and c is the speed of light.

In this case, since the spaceship is moving relative to Earth, we need to calculate the length contraction for the distance between Earth and Alpha Centauri as observed by the astronauts. Using the formula:

L_observed = 4.3 ly * sqrt(1 - 0.87^2),

L_observed ≈ 4.3 ly * 0.507 ≈ 2.18 ly.

Therefore, the distance between Earth and Alpha Centauri would be approximately 2.18 light-years as observed by the astronauts in the spaceship.

Question 13: The rest energy of the spaceship (including the astronauts) with a mass of 10^4 kg would be 9 x 10^20 Joules.

The rest energy of an object can be calculated using Einstein's mass-energy equivalence principle, which states that energy (E) is equal to mass (m) times the speed of light (c) squared (E = mc^2).

In this case, the mass of the spaceship (including the astronauts) is given as 10^4 kg. Substituting the values into the equation:

Rest energy = (10^4 kg) * (3 x 10^8 m/s)^2,

Rest energy ≈ 10^4 kg * 9 x 10^16 m^2/s^2,

Rest energy ≈ 9 x 10^20 Joules.

Therefore, the rest energy of the spaceship would be approximately 9 x 10^20 Joules.

Question 14: The total energy of the spaceship (with a mass of 10^4 kg) when moving at v = 0.75c as observed by Earth would be approximately 1.5 x 10^20 Joules.

To calculate the total energy of the spaceship when moving at a velocity of 0.75c as observed by Earth, we need to use the relativistic energy equation:

Total energy = rest energy + kinetic energy,

where kinetic energy is given by:

Kinetic energy = (gamma - 1) * rest energy,

and gamma (γ) is the Lorentz factor:

gamma = 1 / sqrt(1 - v^2/c^2).

In this case, the velocity of the spaceship is v = 0.75c. Substituting the values into the equations, we have:

gamma = 1 / sqrt(1 - 0.75^2) ≈ 1.5,

Kinetic energy = (1.5 - 1) * 9 x 10^20 Joules = 9 x 10^20 Joules.

Therefore, the total energy of the spaceship when moving at v = 0.75c as observed by Earth would be approximately 1.5 x 10^20 Joules.

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Equation 37.25 relating to the Doppler effect's validity depends on specific conditions that should be specified in the source material.

The Doppler effect describes the observed shift in frequency or wavelength of a wave when there is relative motion between the source of the wave and the observer.

The equation you mentioned, Equation 37.25, may be specific to the source you referenced, and without the context or details of the equation, it is difficult to determine its exact validity.

In general, equations related to the Doppler effect are valid under certain assumptions and conditions, which may include:

1. The source of the wave and the observer are in relative motion.

2. The relative motion is along the line connecting the source and the observer (the line of sight).

3. The source and observer are not accelerating.

4. The speed of the wave is constant and known.

It is important to consult the specific source or reference material to understand the conditions under which Equation 37.25 is valid, as it may have additional factors or constraints specific to that equation.

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Answer:The phase difference between the two interfering waves on a screen at a point 2.50 mm from the central bright fringe is 1.31 radians.The ratio of the intensity at this point to the intensity at the center of a bright fringe is I_max/I = 1.90 or I = 1.90 I_max.

(a) The phase difference between the two interfering waves on a screen at a point 2.50 mm from the central bright fringe is 1.31 radian.

We can use the formula:δ = (2π/λ)dsinθFor a bright fringe, the angle θ is very small, so we can use the approximation sinθ = θ, where θ is in radians.

δ = (2π/λ)dsinθ

= (2π/570 x 10⁻⁹ m) x 0.850 x 10⁻³ m x (2.50 x 10⁻³ m/2.60 m)

= 1.31 radian

(b) The ratio of the intensity at this point to the intensity at the center of a bright fringe is

Imax/I = cos²(δ/2)

= cos²(0.655)

= 0.526.

Therefore, I/Imax = 1.90 or

I = 1.90 I max.

More explanation:Two narrow parallel slits separated by 0.850 mm are illuminated by 570−nm light and the screen is 2.60 m away from the slits.

Let the angle between the central bright fringe and the point be θ.The phase difference between the two waves at the point on the screen is given by

δ = (2π/λ)dsinθ

We can assume that sinθ is approximately equal to θ in radians because the angle is very small.From the equation given above, we know that

δ = (2π/λ)dsinθ

We have the values as

λ = 570−nm

= 570 x 10⁻⁹ m.

θ = (2.50 mm/2.60 m)

= 2.50 x 10⁻³ m.

From the above equation, we can get the value ofδ = 1.31 radians.The intensity at a distance x from the center of the central bright fringe is given by:

I = I_max cos²πd sinθ/λ

Where d is the separation of the slits and I_max is the intensity of the bright fringe at the center.

From the equation given above, we know thatI = I_max cos²πd sinθ/λ We have the values as

d = 0.850 mm

= 0.850 x 10⁻³ m,

λ = 570−nm

= 570 x 10⁻⁹ m and

θ = (2.50 mm/2.60 m)

= 2.50 x 10⁻³ m.

On substituting the values in the equation, we get,I/I_max = 0.526.

Therefore, I_max/I = 1.90 or

I = 1.90 I_max.

Therefore,The phase difference between the two interfering waves on a screen at a point 2.50 mm from the central bright fringe is 1.31 radians.The ratio of the intensity at this point to the intensity at the center of a bright fringe is I_max/I = 1.90 or

I = 1.90 I_max.

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A crate of mass m-12.4 kg is pulled by a massless rope up a 36.9° ramp. The rope passes over an ideal pulley and is attached to a hanging crate of mass m2-16.3 kg. Total Work = Work₁ + Work₂

To find the total work done on the sliding crate, we need to consider the work done by different forces acting on it.

The work done by the tension in the rope (T) can be calculated using the formula:

Work₁ = T * displacement₁ * cos(θ₁)

where displacement₁ is the distance the sliding crate moves along the ramp and θ₁ is the angle between the displacement and the direction of the tension force.

In this case, the displacement₁ is given as 1.50 m and the tension force T is given as 121.5 N. The angle θ₁ is the angle of the ramp, which is 36.9°. Therefore, we can calculate the work done by the tension force as:

Work₁ = 121.5 * 1.50 * cos(36.9°)

Next, we need to consider the work done by the frictional force (f) acting on the sliding crate. The work done by the frictional force is given by:

Work₂ = f * displacement₂

where displacement₂ is the distance the crate moves horizontally. In this case, the frictional force f is given as 22.8 N. The displacement₂ is equal to the displacement₁ because the crate moves horizontally over the same distance.

Therefore, we can calculate the work done by the frictional force as:

Work₂ = 22.8 * 1.50

Finally, the total work done on the sliding crate is the sum of the work done by the tension force and the work done by the frictional force:

Total Work = Work₁ + Work₂

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The volume of the air in the middle ear will decrease to 4.3 cm^3 when the pressure is 0.83 x 10^5 N/m^2.

We can use the ideal gas law to calculate the new volume, V2, of the air in the middle ear. The ideal gas law states that:

PV = nRT

 Where:

P is the pressure of the gas

V is the volume of the gas

n is the number of moles of gas

R is the ideal gas constant

T is the temperature of the gas

In this case, the pressure, number of moles, and temperature of the gas remain constant. The only thing that changes is the pressure.

We can rearrange the ideal gas law to solve for V2:

V2 = V1 * (P1 / P2)

Where:

V1 is the initial volume of the gas

P1 is the initial pressure of the gas

P2 is the final pressure of the gas

Plugging in the values, we get:

V2 = 5.4 cm^3 * (1.0 x 10^5 N/m^2 / 0.83 x 10^5 N/m^2) = 4.3 cm^3

Therefore, the volume of the air in the middle ear will decrease to 4.3 cm^3 when the pressure is 0.83 x 10^5 N/m^2.

As you mentioned, if the volume of the middle ear does not change, then the air will have to escape the chamber. This is what causes our ears to "pop" when we go to high altitudes.

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a) The amount of liquid before the boiler is 90 kg mol/h.

To calculate the amount of liquid before the boiler, we need to determine the liquid flow rate in the feed stream that enters the distillation column.

Given that the feed flow rate is 100 kg mol/h and it contains 45 mol% benzene and 55 mol% toluene, we can calculate the moles of benzene and toluene in the feed:

Moles of benzene = 100 kg mol/h × 0.45 = 45 kg mol/h

Moles of toluene = 100 kg mol/h × 0.55 = 55 kg mol/h

Since the average heat capacity of the feed is 140 kJ/kg mol·K, we can convert the moles of benzene and toluene to mass:

Mass of benzene = 45 kg mol/h × 78.11 g/mol = 3519.95 kg/h

Mass of toluene = 55 kg mol/h × 92.14 g/mol = 5067.7 kg/h

Now, we can calculate the total mass of the liquid before the boiler:

Total mass before the boiler = Mass of benzene + Mass of toluene = 3519.95 kg/h + 5067.7 kg/h = 8587.65 kg/h

Converting the mass to moles:

Moles before the boiler = Total mass before the boiler / Average molecular weight = 8587.65 kg/h / (45.09 g/mol) = 190.67 kg mol/h

Therefore, the amount of liquid before the boiler is approximately 190.67 kg mol/h.

b) The amount of returned vapor to the distillation column from the boiler is 9 kg mol/h.

To calculate the amount of returned vapor from the boiler, we need to determine the vapor flow rate in the distillate stream.

Given that the distillate contains 95 mol% benzene and 5 mol% toluene, and the total flow rate of the distillate is 100 kg mol/h, we can calculate the moles of benzene and toluene in the distillate:

Moles of benzene in the distillate = 100 kg mol/h × 0.95 = 95 kg mol/h

Moles of toluene in the distillate = 100 kg mol/h × 0.05 = 5 kg mol/h

Therefore, the amount of returned vapor to the distillation column from the boiler is 95 kg mol/h - 5 kg mol/h = 90 kg mol/h.

c) The number of theoretical trays in the stripping section, equivalent to the packed bed height of column 1.95, is 60.

To calculate the number of theoretical trays in the stripping section, we can use the concept of tray efficiency and the reflux ratio.

The number of theoretical trays is given by:

Number of theoretical trays = (Height of column / Tray height) × (1 - Tray efficiency) + 1

Given that the packed bed height of the column is 1.95, we can substitute the values into the equation:

Number of theoretical trays = (1.95 / 1) × (1 - 1/41) + 1 = 60

Therefore, the number of theoretical trays in the stripping section, equivalent to the packed bed height of column 1.95, is 60.

d) The value of g for the q-line section is 16.6.

To calculate the value of g for the q-line section, we can use the equation:

g = (slope of q-line) / (slope of operating line)

Given that the slope of the q-line is 8.3, we need to determine the slope of the operating line.

The operating line slope is given by:

Slope of operating line = (yD - yB) / (xD - xB)

Where yD and xD are the mole fractions of benzene in the distillate and xB is the mole fraction of benzene in the bottoms.

Given that the distillate contains 95 mol% benzene and the bottoms contain 10 mol% benzene, we can substitute the values into the equation:

Slope of operating line = (0.95 - 0.10) / (0.95 - 0.45) = 1.6

Now we can calculate the value of g:

g = 8.3 / 1.6 = 16.6

Therefore, the value of g for the q-line section is 16.6.

e) The height equivalent for the stripping section is 98.25.

To calculate the height equivalent for the stripping section, we can use the equation:

Height equivalent = (Number of theoretical trays - 1) × Tray height

Given that the number of theoretical trays in the stripping section is 60 and the tray height is not provided, we cannot calculate the exact value of the height equivalent. However, since the number of theoretical trays is equivalent to the packed bed height of column 1.95, we can assume that the tray height is 1.95 / 60.

Height equivalent = (60 - 1) × (1.95 / 60) ≈ 1.95

Therefore, the height equivalent for the stripping section is approximately 1.95.

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The linear speed of a hollow sphere that rolls down a 25 cm high ramp from rest can be determined as follows:

Given data: mass of the sphere (m) = 20 g = 0.02 kg

The radius of the sphere (r) = 1.5 cm = 0.015 m

height of the ramp (h) = 25 cm = 0.25 m

Acceleration due to gravity (g) = 9.81 m/s².

Let's use the conservation of energy principle to calculate the linear speed of the sphere at the bottom of the ramp.

The initial potential energy (U₁) is given by: U₁ = mgh where m is the mass of the sphere, g is the acceleration due to gravity, and h is the height of the ramp.

U₁ = 0.02 kg × 9.81 m/s² × 0.25 m = 0.049 J.

The final kinetic energy (K₂) is given by: K₂ = (1/2)mv² where m is the mass of the sphere and v is the linear speed of the sphere.

K₂ = (1/2) × 0.02 kg × v².

Let's equate the initial potential energy to the final kinetic energy, that is:

U₁ = K₂0.049 = (1/2) × 0.02 kg × v²0.049

= 0.01v²v² = 4.9v = √(4.9) = 2.21 m/s (rounded to two decimal places).

Therefore, the sphere's linear speed at the bottom of the ramp is approximately 2.21 m/s.

Hence, the closest option (d) to this answer is 2.05 m/s.

The sphere's linear speed is 2.05 m/s.

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The velocity of the center of the rod in vector form is approximately 24.85 m/s. The angular velocity of the rod after the collision is 24844.087 rad/s. The increase in internal energy of the objects is -103.347 J.

(a) Velocity of center of the rod: The velocity of the center of the rod can be calculated by applying the principle of conservation of momentum. Since the system is isolated, the total momentum of the system before the collision is equal to the total momentum of the system after the collision. Using this principle, the velocity of the center of the rod can be calculated as follows:

Let v be the velocity of the center of the rod after the collision.

m1 = 1.7 kg (mass of the rod)

m2 = 0.09 kg (mass of the meteorite)

v1 = 0 m/s (initial velocity of the rod)

u2 = 245 m/s (initial velocity of the meteorite)

i1 = 0° (initial angle of the rod)

i2 = 26° (initial angle of the meteorite)

j1 = 0° (final angle of the rod)

j2 = 82° (final angle of the meteorite)

v2 = 60 m/s (final velocity of the meteorite)

The total momentum of the system before the collision can be calculated as follows: p1 = m1v1 + m2u2p1 = 1.7 kg × 0 m/s + 0.09 kg × 245 m/sp1 = 21.825 kg m/s

The total momentum of the system after the collision can be calculated as follows: p2 = m1v + m2v2p2 = 1.7 kg × v + 0.09 kg × 60 m/sp2 = (1.7 kg)v + 5.4 kg m/s

By applying the principle of conservation of momentum: p1 = p221.825 kg m/s = (1.7 kg)v + 5.4 kg m/sv = (21.825 kg m/s - 5.4 kg m/s)/1.7 kg v = 10.015 m/s

To represent the velocity in vector form, we can use the following equation:

vCM = (m1v1 + m2u2 + m1v + m2v2)/(m1 + m2)

m1 = 1.7 kg (mass of the rod)

m2 = 0.09 kg (mass of the meteorite)

v1 = 0 m/s (initial velocity of the rod)

u2 = 245 m/s (initial velocity of the meteorite)

v = 10.015 m/s (velocity of the rod after the collision)

v2 = 60 m/s (velocity of the meteorite after the collision)

Substituting these values into the equation, we have:

vCM = (1.7 kg * 0 m/s + 0.09 kg * 245 m/s + 1.7 kg * 10.015 m/s + 0.09 kg * 60 m/s) / (1.7 kg + 0.09 kg)

Simplifying the equation:

vCM = (0 + 22.05 + 17.027 + 5.4) / 1.79

vCM = 44.477 / 1.79

vCM ≈ 24.85 m/s

Therefore, the velocity of the center of the rod in vector form is approximately 24.85 m/s.

(b) Angular velocity of the rod: To calculate the angular velocity of the rod, we can use the principle of conservation of angular momentum. Since the system is isolated, the total angular momentum of the system before the collision is equal to the total angular momentum of the system after the collision. Using this principle, the angular velocity of the rod can be calculated as follows:

Let ω be the angular velocity of the rod after the collision.I = (1/12) m L2 is the moment of inertia of the rod about its center of mass, where L is the length of the rod.m = 1.7 kg is the mass of the rod

The angular momentum of the system before the collision can be calculated as follows:

L1 = I ω1 + m1v1r1 + m2u2r2L1 = (1/12) × 1.7 kg × (0.9 m)2 × 0 rad/s + 1.7 kg × 0 m/s × 0.2 m + 0.09 kg × 245 m/s × 0.7 mL1 = 27.8055 kg m2/s

The angular momentum of the system after the collision can be calculated as follows:

L2 = I ω + m1v r + m2v2r2L2 = (1/12) × 1.7 kg × (0.9 m)2 × ω + 1.7 kg × 10.015 m/s × 0.2 m + 0.09 kg × 60 m/s × 0.7 mL2 = (0.01395 kg m2)ω + 2.1945 kg m2/s

By applying the principle of conservation of angular momentum:

L1 = L2ω1 = (0.01395 kg m2)ω + 2.1945 kg m2/sω = (ω1 - 2.1945 kg m2/s)/(0.01395 kg m2)

Here,ω1 is the angular velocity of the meteorite before the collision. ω1 = u2/r2

ω1 = 245 m/s ÷ 0.7 m

ω1 = 350 rad/s

ω = (350 rad/s - 2.1945 kg m2/s)/(0.01395 kg m2)

ω = 24844.087 rad/s

The angular velocity of the rod after the collision is 24844.087 rad/s.

(c) Increase in internal energy of the objects

The increase in internal energy of the objects can be calculated using the following equation:ΔE = 1/2 m1v1² + 1/2 m2u2² - 1/2 m1v² - 1/2 m2v2²

Here,ΔE is the increase in internal energy of the objects.m1v1² is the initial kinetic energy of the rod.m2u2² is the initial kinetic energy of the meteorite.m1v² is the final kinetic energy of the rod. m2v2² is the final kinetic energy of the meteorite.Using the given values, we get:

ΔE = 1/2 × 1.7 kg × 0 m/s² + 1/2 × 0.09 kg × (245 m/s)² - 1/2 × 1.7 kg × (10.015 m/s)² - 1/2 × 0.09 kg × (60 m/s)²ΔE = -103.347 J

Therefore, the increase in internal energy of the objects is -103.347 J.

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(a) The mass of the block is 39.6 g.

(b) The block floats partially submerged because its weight is not entirely balanced by the upward buoyant force, resulting in some part of the block being submerged.

(c) Forces acting on the block:

- Weight of the block acting downward (mg)

- Buoyant force acting upward

(d) The buoyant force acting on the block is equal to the weight of the block.

(e) The source of the buoyant force is the pressure difference between the top and bottom surfaces of the submerged or partially submerged object

(f) The volume of the fluid displaced by the block is equal to the volume of the block.

a. To find the mass of the block, we can use the formula:

mass = density * volume.

Given the density of the block is 0.88 g/cm³ and the volume is 45 cm³:

mass = 0.88 g/cm³ * 45 cm³.

Calculating the mass:

mass = 39.6 g.

Therefore, the mass of the block is 39.6 g.

b. When the block is placed in the oil of density 0.92 g/cm³, it floats partially submerged because the density of the block is less than the density of the oil.

According to Archimedes' principle, an object will float if the buoyant force acting on it is equal to or greater than the weight of the object. In this case, the buoyant force exerted by the oil on the block is sufficient to counteract the weight of the block, causing it to float. The block floats partially submerged because its weight is not entirely balanced by the upward buoyant force, resulting in some part of the block being submerged.

c. A Free Body Diagram (FBD) of the block in this scenario would show the following forces acting on the block:

- Weight of the block acting downward (mg)

- Buoyant force acting upward

d. The buoyant force acting on the block is equal to the weight of the fluid displaced by the block. If the block is floating partially submerged, it means that the buoyant force is equal to the weight of the block. This is because the block is in equilibrium, with the upward buoyant force balancing the downward force due to gravity (weight of the block). So, the buoyant force acting on the block is equal to the weight of the block.

e. The source of the buoyant force is the pressure difference between the top and bottom surfaces of the submerged or partially submerged object. The fluid exerts a greater pressure on the lower surface of the object compared to the top surface, resulting in an upward force known as the buoyant force.

f. According to Archimedes' principle, the volume of fluid displaced by a submerged object is equal to the volume of the object itself. So, in this case, the volume of the fluid displaced by the block is equal to the volume of the block.

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The absorbed dose in Gray and Rad is 10 Gy and 1000 Rad, respectively. The dose equivalent in Sievert and rem is 200 Sv and 20000 Rem, respectively.

Given data:Mass of the tumor = 10 g

Total energy absorbed = 0.5 J

Energy absorbed by tumor, E = 0.5 J

Mass of tumor, m = 10 g

= 0.01 kg

Absorbed Dose = E/m
= 0.5 J / 0.01 kg

= 50 Gy

Dose Equivalent

= Absorbed dose × Quality factor = 50 × 1

= 50 Sievert (Sv)

So, absorbed dose in Gray and Rad is 50 Gy and 5000 Rad, respectively. The dose equivalent in Sievert and rem is 50 Sv and 5000 Rem, respectively.b) Given data:Energy absorbed by the tumor,

E = 0.10 JRBE (Relative Biological Effectiveness) of alpha particle

= 20

Absorbed Dose = E/m

= 0.10 J / 0.01 kg

= 10 Gy

Dose Equivalent = Absorbed dose × Quality factor

= 10 Gy × 20

= 200 Sievert (Sv)

So, the absorbed dose in Gray and Rad is 10 Gy and 1000 Rad, respectively. The dose equivalent in Sievert and rem is 200 Sv and 20000 Rem, respectively.

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c. The velocity of the muon in the electron's frame is approximately equal to the speed of light (c) =  [tex]3 * 10^8 m / s[/tex]

d.  muon's momentum in electron's frame = 1 / √(0) = undefined

(c)

Velocity of electron (v1) = 0.996c

Velocity of muon (v2) = 0.93c

We apply the relativistic velocity addition formula:

v' = (v1 + v2) / (1 + (v1*v2)/c²)

= (0.996c + 0.93c) / (1 + (0.996c * 0.93c) / c²)

≈ 1.926c / (1 + 0.996 * 0.93)

= 1.926c / 1.926

c = [tex]3 * 10^8 m / s[/tex]

(d) Momentum of muon in electron's frame:

Mass of muon (m) = [tex]1.9 * 10^-^2^8 kg[/tex]

Velocity of muon in electron's frame (v') = c

Using the relativistic momentum formula:

p = γ * m * v

where γ is the Lorentz factor,  γ = 1 / √(1 - (v²/c²))

The velocity of the muon in the electron's frame (v') is equal to the speed of light (c), we can substitute v' = c into the formula:

γ = 1 / √(1 - (c²/c²))

= 1 / √(1 - 1)

= 1 / √(0)

= undefined

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c) The velocity of muon in the electron's frame is 0.93c.

d) The muon's momentum in the electron's frame is 5.29 × 10^-20 kg m/s.

The collision between electrons accelerated to 0.996c and a nucleus produces a muon which moves in the direction of the electron with a speed of 0.93c. Given the mass of muon is 1.9×10^-28 kg.

(c) Velocity of muon in electron's frame, Let us use the formula:β = v/cwhere:β = velocityv = relative velocityc = speed of light

The velocity of muon in the electron's frame can be determined by:β = v/cv = βcWhere v = velocity, β = velocity of muon in electron's frame, c = speed of light

Then, v = 0.93cβ = 0.93

(d) Muon's momentum in electron's frame Let us use the formula for momentum: p = mv

where: p = momentum, m = mass, v = velocity, The momentum of muon in the electron's frame can be determined by: p = mv

where p = momentum, m = mass of muon, v = velocity of muon in electron's frame

Given that m = 1.9 × 10^-28 kg and v = 0.93c

We first find v:β = v/cv = βc = 0.93 × 3 × 10^8v = 2.79 × 10^8 m/s

Now,p = mv = (1.9 × 10^-28 kg) × (2.79 × 10^8 m/s) = 5.29 × 10^-20 kg m/s.

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The component of the longer vector along the line of the shorter vector is approximately 15.2 (option b). We can use the concept of vector projection.

To find the component of the longer vector along the line of the shorter vector, we can use the concept of vector projection.

Let's denote the longer vector as A (magnitude of 32) and the shorter vector as B (magnitude of 9.6). The angle between them is given as 61.7°.

The component of vector A along the line of vector B can be found using the formula:

Component of A along B = |A| * cos(theta)

where theta is the angle between vectors A and B.

Substituting the given values, we have:

Component of A along B = 32 * cos(61.7°)

Using a calculator, we can evaluate this expression:

Component of A along B ≈ 15.2

Therefore, the component of the longer vector along the line of the shorter vector is approximately 15.2 (option b).

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H2 has higher vibrational entropy due to larger energy spacing and more available energy states.

Problem 1:

To calculate kg T for T = 500 K in various units:

[tex]erg: kg T = 1.3807 × 10^-16 erg/K * 500 K eV: kg T = 8.6173 × 10^-5 eV/K * 500 K cm-t: kg T = 1.3807 × 10^-23 cm-t/K * 500 K Wavelength: kg T = (6.626 × 10^-34 J·s) / (500 K) Degrees Kelvin: kg T = 500 K Hertz: kg T = (6.626 × 10^-34 J·s) * (500 Hz)[/tex]

Problem 2:

To determine which molecule has higher vibrational entropy without performing a calculation:

The vibrational entropy (Svib) is directly related to the number of available energy states or levels. In this case, the vibrational energy for H2 is given by Ev = ħw(v + 1/2) with ħw = 4401 cm^-1, and for 12 it is given by Ev = ħw(v + 1/2) with ħw = 214.52 cm^-1.

Since the energy spacing (ħw) is larger for H2 compared to 12, the energy levels are more closely spaced. This means that there are more available energy states for H2 and therefore a higher number of possible vibrational states. As a result, H2 is expected to have a higher vibrational entropy compared to 12.

By considering the energy spacing and the number of available vibrational energy states, we can conclude that H2 has a higher vibrational entropy.

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Given: Velocity of the airplane, v = 247 m/altitude, h = 395 mime of flight, t = ?Distance, d = We know that, the equation of motion for an object under the acceleration due to gravity is given as:-h = 1/2 gt²     .....(i)where g is the acceleration due to gravity and t is the time of flight.

We know that the horizontal distance, d travelled by the airplane is given aside = vt    ......(ii)Now, from equation (i) we can find time of flight t as: -h = 1/2 gt² => 2h/g = t² => t = sqrt(2h/g)

Now, we know that the acceleration due to gravity g is 9.8 m/s². On substituting the given values of h and g we get:-t = sqrt (2 x 395/9.8) => t = 8.019 snow, from equation.

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To calculate the total resistance of a circuit, you can use the following formulas:

For resistors connected in series: R_total = R1 + R2 + R3 + ...

For resistors connected in parallel: (1/R_total) = (1/R1) + (1/R2) + (1/R3) + ...

Resistors connected in series:

For three 80.0 Ω lightbulbs and three 100.0 Ω lightbulbs connected in series:

R_total = 80.0 Ω + 80.0 Ω + 80.0 Ω + 100.0 Ω + 100.0 Ω + 100.0 Ω

R_total = 540.0 Ω

Therefore, the total resistance of the circuit when the lightbulbs are connected in series is 540.0 Ω.

Resistors connected in parallel:

For the same three 80.0 Ω lightbulbs and three 100.0 Ω lightbulbs connected in parallel:

(1/R_total) = (1/80.0 Ω) + (1/80.0 Ω) + (1/80.0 Ω) + (1/100.0 Ω) + (1/100.0 Ω) + (1/100.0 Ω)

(1/R_total) = (1/80.0 + 1/80.0 + 1/80.0 + 1/100.0 + 1/100.0 + 1/100.0)

(1/R_total) = (3/80.0 + 3/100.0)

(1/R_total) = (9/200.0 + 3/100.0)

(1/R_total) = (9/200.0 + 6/200.0)

(1/R_total) = (15/200.0)

(1/R_total) = (3/40.0)

R_total = 40.0/3

Therefore, the total resistance of the circuit when the lightbulbs are connected in parallel is approximately 13.33 Ω (rounded to two decimal places).

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The force experienced by an object with a charge in an electric field can be calculated using the equation F = q * E, where F is the force, q is the charge of the object, and E is the electric field strength.

In this case, the electric field strength in the region is 1900 N/C, and the charge of the object is 0.0035 C. By substituting these values into the equation, we can find the force on the object.

The force on the object is given by:

F = 0.0035 C * 1900 N/C

Multiplying the charge of the object (0.0035 C) by the electric field strength (1900 N/C) gives us the force on the object. The resulting force will be in newtons (N), which represents the strength of the force acting on the charged object in the electric field. Therefore, the force on the object is equal to 6.65 N.

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The speed of the water as it comes out of the pipe is approximately 7.94 m/s (meters per second). To determine the speed of the water as it comes out of the pipe, we can apply the Bernoulli's equation, which relates the pressure, velocity, and height of a fluid in a streamline flow.

The equation can be written as:

P + (1/2) * ρ * v^2 + ρ * g * h = constant

where P is the pressure, ρ is the density of the fluid, v is the velocity, g is the acceleration due to gravity, and h is the height.

In this case, we are given the diameter of the pipe, which can be used to calculate the radius (r) as:

r = diameter / 2 = 10.16 cm / 2 = 5.08 cm = 0.0508 m

The flow rate (Q) can be calculated as:

Q = A * v

where A is the cross-sectional area of the pipe and v is the velocity.

The cross-sectional area of a pipe can be determined using the formula:

A = π * r^2

Now, let's calculate the cross-sectional area:

A = π * (0.0508 m)^2 ≈ 0.008125 m^2

The pressure can be converted from atm to Pascal (Pa):

P = 2.20 atm * 101325 Pa/atm ≈ 223095 Pa

Next, we can rearrange the Bernoulli's equation to solve for the velocity (v):

v = √((2 * (P - ρ * g * h)) / ρ)

Since the height (h) is not given, we can assume it to be zero for water flowing horizontally.

Substituting the given values:

v = √((2 * (223095 Pa - ρ * g * 0)) / ρ)

The density of water (ρ) is approximately 1000 kg/m^3, and the acceleration due to gravity (g) is approximately 9.8 m/s^2.

v = √((2 * (223095 Pa - 1000 kg/m^3 * 9.8 m/s^2 * 0)) / 1000 kg/m^3)

Simplifying the equation:

v = √(2 * (223095 Pa) / 1000 kg/m^3)

v ≈ √(446.19 m^2/s^2)

v ≈ 21.12 m/s

However, this value represents the velocity when the pipe is fully open. Since the water is flowing out of the pipe, the velocity will decrease due to the contraction of the flow.

Using the principle of continuity, we know that the flow rate (Q) remains constant throughout the pipe.

Q = A * v

0.04256 m^3/s = 0.008125 m^2 * v_out

Solving for v_out:

v_out = 0.04256 m^3/s / 0.008125 m^2

v_out ≈ 5.23 m/s

Therefore, the speed of the water as it comes out of the pipe is approximately 5.23 m/s.

The speed of the water as it comes out of the pipe is determined to be approximately 5.23 m/s. This is calculated by applying Bernoulli's equation and considering the given pressure, flow rate, and diameter of the pipe. The principle of continuity is also used to account for the decrease in velocity due to the contraction of the flow.

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The magnitude of the force F3 required to make the object move in uniform linear motion in the direction of F1 is 50 N, given that F1 = 30 N and F2 = 40 N with a 90° angle between them.

To find the magnitude of the force F3 required to make the object move in uniform linear motion in the direction of F1, we can use vector addition. Since the angle between F1 and F2 is 90°, we can treat them as perpendicular components.

We can represent F1 and F2 as vectors in a coordinate system, where F1 acts along the x-axis and F2 acts along the y-axis. The force F3 will also act along the x-axis to achieve uniform linear motion in the direction of F1.

By using the Pythagorean theorem, we can find the magnitude of F3:

F3 = √(F1² + F2²).

Substituting the given values:

F1 = 30 N,

F2 = 40 N,

we can calculate the magnitude of F3:

F3 = √(30² + 40²).

F3 = √(900 + 1600).

F3 = √2500.

F3 = 50 N.

Therefore, the magnitude of the force F3 required to make the object move in uniform linear motion in the direction of F1 is 50 N.

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The final velocity when you and your friend reach the bottom of the hill cannot be determined without additional information about the coefficient of friction on the hill or other factors affecting the motion.

To calculate the final velocity when you and your friend reach the bottom of the hill, we can apply the principles of conservation of momentum and conservation of mechanical energy.

Given:

First, let's calculate the initial momentum before colliding with your friend:

Initial momentum (p_initial) = m1 * v1

Next, we calculate the frictional force on the sidewalk:

Frictional force (f_friction1) = μ1 * (m1 + m2) * 9.8 m/s^2

The work done by friction on the sidewalk can be calculated as:

Work done by friction on the sidewalk (W_friction1) = f_friction1 * d1

Since the work done by friction on the sidewalk is negative (opposite to the direction of motion), it results in a loss of mechanical energy. Thus, the change in mechanical energy on the sidewalk is:

Change in mechanical energy on the sidewalk (ΔE1) = -W_friction1

After colliding with your friend, the total mass becomes (m1 + m2).

Now, let's calculate the potential energy at the top of the hill:

Potential energy at the top of the hill (PE_top) = (m1 + m2) * g * h

Since there is no friction on the hill, the total mechanical energy is conserved. Therefore, the final kinetic energy at the bottom of the hill is equal to the initial mechanical energy minus the change in mechanical energy on the sidewalk and the potential energy at the top of the hill:

Final kinetic energy at the bottom of the hill (KE_final) = p_initial - ΔE1 - PE_top

Finally, we can calculate the final velocity (v_final) at the bottom of the hill:

Final velocity at the bottom of the hill (v_final) = sqrt(2 * KE_final / (m1 + m2))

After performing the calculations using the given values, you can determine the final velocity when you and your friend reach the bottom of the hill.

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