Veronica’s velocity was measured as 4. 3 m/s. She displaced 20 meters in 4. 7 seconds. Which piece of information is missing for the correct calculation of velocity?

After the collision, the two objects stick together and move as one. Their total mass is m1 + m2 = 5 kg + m2.

In this case, we can apply the principle of conservation of linear momentum

The initial momentum of the first object (P1_initial) is given by its mass (m1) times its velocity (v1), which is [tex]5 kg * 4 m/s = 20 kg*m/s.[/tex]

Therefore, the total initial momentum [tex](P_{total_initial}) is P1_{initial} + P2_{initial} = 20 kg*m/s - m2 * 5 m/s.[/tex]

After the collision, the two objects stick together and move as one.

Their total mass is m1 + m2 = 5 kg + m2.

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The impulse imparted by the wall is -2 kg·m/s. The negative sign indicates a change in direction due to the rebound of the ball.

To determine the impulse imparted by the wall, we can use the principle of conservation of momentum. The impulse is equal to the change in momentum experienced by the ball.

The momentum of an object is given by the product of its mass and velocity:

Momentum = mass × velocity

Given:

Mass of the ball (m) = 0.10 kg

Initial velocity of the ball (v₁) = 10 m/s

Final velocity of the ball (v₂) = -10 m/s (negative sign indicates a change in direction)

The initial momentum of the ball is:

Initial momentum = m × v₁ = 0.10 kg × 10 m/s = 1 kg·m/s

The final momentum of the ball is:

Final momentum = m × v₂ = 0.10 kg × (-10 m/s) = -1 kg·m/s

The change in momentum is the difference between the final and initial momentum:

Change in momentum = Final momentum - Initial momentum = (-1 kg·m/s) - (1 kg·m/s) = -2 kg·m/s

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To determine the amount of energy lost due to air resistance, we can use the principle of conservation of mechanical energy. Initially, the Snickers bar has gravitational potential energy, and upon hitting the ground, it has kinetic energy.

The gravitational potential energy (PE) of an object is given by the equation:

PE = m * g * h

Where:

m is the mass of the object (3 kg)

g is the acceleration due to gravity (approximately 9.8 m/s^2)

h is the height of the Washington Monument (170 m)

Calculating the potential energy, we have:

PE = 3 kg * 9.8 m/s^2 * 170 m

PE = 4998 J (joules)

At the moment of impact, all the potential energy is converted into kinetic energy, given by:

KE = 1/2 * m * v^2

Where:

m is the mass of the object (3 kg)

v is the velocity at impact (52 m/s)

Calculating the kinetic energy, we have:

KE = 1/2 * 3 kg * (52 m/s)^2

KE = 4056 J (joules)

The energy lost due to air resistance is the difference between the initial potential energy and the final kinetic energy:

Energy Lost = PE - KE

Energy Lost = 4998 J - 4056 J

Energy Lost = 942 J (joules)

Therefore, the amount of energy lost due to air resistance is 942 joules.

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The length of the browser window (x) is 6. The dimensions of the screen are approximately 3 inches (width) and 18/13 inches (height).

Let's solve the equations step by step:

Part A:

The area of the browser window is given by the equation:

(x - 2) * x = 24

Expanding the equation:

[tex]x^{2}[/tex] - 2x = 24

Rearranging the equation to standard quadratic form:

[tex]x^{2}[/tex] -  2x - 24 = 0

Factoring the quadratic equation:

(x - 6)(x + 4) = 0

Setting each factor to zero:

x - 6 = 0 or x + 4 = 0

Solving for x:

x = 6 or x = -4

Since the length of the monitor cannot be negative, we discard the solution x = -4.

Therefore, the length of the browser window (x) is 6.

Part B:

The dimensions of the screen can be calculated using the length of the monitor (x+7) and the coverage ratio of the browser window (3/13).

The width of the screen is given by:

Width = (3/13) * (x + 7)

The height of the screen is given by:

Height = (3/13) * (x)

Substituting the value of x = 6:

Width = (3/13) * (6 + 7) = (3/13) * 13 = 3

Height = (3/13) * 6 = 18/13

Therefore, the dimensions of the screen are approximately 3 inches (width) and 18/13 inches (height).

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The loss of heat energy when a 6.4 kg cloud of steam at 150 degrees Celsius hits you and cools to 100 degrees Celsius is 13,440,000 Joules.

To calculate the heat energy loss, we can use the formula:

Q = mcΔT

Where Q represents heat energy, m is the mass of the steam cloud (6.4 kg), c is the specific heat capacity of water (4,186 J/kg°C), and ΔT is the change in temperature (150°C - 100°C = 50°C).

Plugging in the values, we have:

Q = (6.4 kg) × (4,186 J/kg°C) × (50°C)

Q = 13,440,000 Joules

Therefore, the loss of heat energy when the steam cools from 150°C to 100°C is 13,440,000 Joules.

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the car is experiencing a centripetal force of 3411.1 N.

The speed at which the 900 kg car is moving while taking a turn with a radius of 9.5 m while experiencing a centripetal acceleration of 3.79 m/s² can be calculated using the formula given below:

v = √(r × a)

Where:

v is the speed at which the car is moving

r is the radius of the turn

a is the centripetal acceleration

v = √(r × a) = √(9.5 × 3.79) = 7.08 m/s

Therefore, the car is moving at a speed of 7.08 m/s.

The centripetal force that the car is experiencing can be calculated using the formula given below:

F = m × a

Where:

F is the force the car is experiencing

m is the mass of the car (900 kg)

a is the centripetal acceleration

F = m × a = 900 × 3.79 = 3411.1 N

Therefore, the car is experiencing a centripetal force of 3411.1 N.

The force responsible for creating this centripetal motion in the car is the frictional force between the tires of the car and the road surface.

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An object emits a range of electromagnetic energy wavelengths because it has a temperature that is above absolute zero. This results in the emission of thermal radiation, which is a type of electromagnetic radiation. When an object is heated, the atoms and molecules within it gain energy and begin to move more quickly. This results in the release of electromagnetic radiation in the form of photons of light. The wavelength of this light depends on the temperature of the object.

The relationship between temperature and wavelength is described by Wien's Law, which states that the wavelength of the peak emission of thermal radiation is inversely proportional to the temperature of the object. This means that the hotter an object is, the shorter the wavelength of the peak emission of its thermal radiation.

The range of electromagnetic energy wavelengths emitted by an object is called its electromagnetic spectrum. This spectrum can range from radio waves with long wavelengths to gamma rays with short wavelengths. Different objects emit different parts of the electromagnetic spectrum depending on their temperature and composition.

For example, the Sun emits a range of electromagnetic energy wavelengths, including visible light, ultraviolet radiation, and infrared radiation. The Earth also emits thermal radiation in the form of infrared radiation.

In addition to thermal radiation, objects can emit other types of electromagnetic radiation depending on their composition and state. For example, stars emit light at specific wavelengths depending on the elements present in their atmosphere. X-ray machines emit high-energy X-rays that can pass through soft tissue but are absorbed by denser materials like bone.

In conclusion, an object emits a range of electromagnetic energy wavelengths because of its temperature, which causes it to emit thermal radiation. The specific wavelengths emitted depend on the temperature and composition of the object. Other factors, such as the object's state and composition, can also influence the types of electromagnetic radiation emitted.

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To determine the time it would take Susie to complete the marathon, we can use the formula: Time = Distance / Speed

Given that the distance of the marathon is 26 miles and Susie's steady rate is 8 mph, we can substitute these values into the formula. Time = 26 miles / 8 mph. To calculate the time, we divide 26 miles by 8 mph: Time = 3.25 hours. Since there are 60 minutes in an hour, we can convert the decimal part of the time to minutes: 0.25 hours * 60 minutes/hour = 15 minutes.  Therefore, it would take Susie approximately 3 hours and 15 minutes to complete the marathon.

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Violet is the most likely color of the light whose second-order bright band forms an angle of 13.5°.

To determine the color of the light whose second-order bright band forms an angle of 13.5°, we can use the formula for the angle of diffraction:

sinθ = mλ/d

where θ is the angle of diffraction, m is the order of the bright band, λ is the wavelength of light, and d is the spacing between the lines of the diffraction grating.In this case, we are looking for the second-order bright band (m = 2), and the angle of diffraction is given as 13.5°. The diffraction grating has 175 lines per mm, so the spacing between the lines (d) can be calculated as:

d = 1 / (number of lines per unit length)

= 1 / (175 lines/mm)

= 0.00571 mm

Now, we can rearrange the formula to solve for the wavelength (λ):

λ = d * sinθ / m

λ = (0.00571 mm) * sin(13.5°) / 2

Calculating this value, we find that λ is approximately 0.001585 mm.

Different colors of light have different wavelengths. Among the given options, the color with a wavelength closest to 0.001585 mm is violet. Therefore, violet is the most likely color of the light whose second-order bright band forms an angle of 13.5°.

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A call can supply circuit of 0. 4A and 0. 2A through a 4ohms and 10 ohms resistor respectively what is the internal resistant of the cellThe internal resistance of the cell is 3 ohms.

According to Ohm's Law, the current in a circuit can be determined using the equation I = V/R, where I is the current, V is the voltage, and R is the resistance. In this case, we have two resistors connected in parallel. Let's assume the voltage of the cell is V.

For the 4-ohm resistor, the current is given as 0.4A. Using Ohm's Law, we can calculate the voltage across the resistor as V1 = I1 * R1 = 0.4A * 4ohms = 1.6V.

For the 10-ohm resistor, the current is given as 0.2A. Using Ohm's Law, we can calculate the voltage across the resistor as V2 = I2 * R2 = 0.2A * 10ohms = 2V.

Since the resistors are in parallel, the voltage across both resistors is the same, so V1 = V2. This means the internal resistance of the cell can be calculated as V = I * r, where r is the internal resistance. Substituting the values, we have 1.6V = 0.4A * r, which gives us r = 1.6V / 0.4A = 4 ohms.

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In the experiment, measuring the total time for 20 complete revolutions and dividing it by 20 to obtain the period of rotation is done to reduce errors and improve the accuracy of the measurement.

Measuring the time for one complete revolution directly can be subject to human reaction time and potential errors in starting and stopping the stopwatch precisely at the beginning and end of each revolution. These errors can accumulate and affect the accuracy of the measurement.

By measuring the total time for 20 complete revolutions and then dividing it by 20, we are essentially averaging out these potential errors over multiple revolutions. This helps to minimize the impact of any individual timing error and provides a more reliable and accurate measurement of the period of rotation.

Additionally, by taking multiple measurements (in this case, 20), we increase the sample size and reduce the influence of outliers or irregularities in any individual measurement. This improves the overall precision and reliability of the calculated period.

Therefore, measuring the total time for multiple revolutions and dividing by the number of revolutions allows for a more accurate determination of the period of rotation in the experiment.

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As the particles of an object become more compact and closer together, the kinetic energy of the particles will generally decrease.

This is because kinetic energy is associated with the motion of particles, and when particles become more compact and closer together, their freedom of motion and average speed tends to decrease.

As a result, the overall kinetic energy of the particles decreases.

Hence, As the particles of an object become more compact and closer together, the kinetic energy of the particles will generally decrease.

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Answer:

The mechanical advantage of the screwdriver is 3.

Explanation:

The mechanical advantage can be calculated using the formula: mechanical advantage = output force / input force. In this case, the output force is 75 N (the force applied by the screwdriver to the lid), and the input force is 25 N (the force applied to the screwdriver).

Therefore, the mechanical advantage is:

mechanical advantage = 75 N / 25 N = 3.

Hence, the mechanical advantage of the screwdriver is 3.

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The minimum coefficient of friction required to keep the car from sliding off the road is approximately 0.285. This can be calculated using the equation: coefficient of friction = (v^2) / (g * r).

Where v is the velocity of the car, g is the acceleration due to gravity, and r is the radius of curvature of the curve.

To calculate the minimum coefficient of friction, we can use the equation:

coefficient of friction = (v^2) / (g * r)

Given:

Mass of the car (m) = 890 kg

Velocity of the car (v) = 25 m/s

Radius of curvature (r) = 220 m

Acceleration due to gravity (g) ≈ 9.8 m/s^2

Plugging in the values, we have:

coefficient of friction = (25^2) / (9.8 * 220)

≈ 625 / 2156

≈ 0.289

Therefore, the minimum coefficient of friction required to keep the car from sliding off the road is approximately 0.285. This means that the friction between the car's tires and the road must provide at least this much resistance to prevent the car from losing traction and sliding off the road during the turn.

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The common velocity of masses m and M after the impact is v = mv / sqrt(m (m + M)). A pendulum consists of a mass m hanging at the bottom end of a massless rod of length l, which has a frictionless pivot at its top end. A mass m, moving as shown in the figure with velocity v impacts m and becomes embedded.

The given figure shows the before and after impact of two masses m and M with velocities v and 0, respectively, where mass M is hanging with the help of a rod and performing simple harmonic motion. Therefore, the given system of masses is an example of an inelastic collision. As per the principle of conservation of linear momentum in physics, the momentum of a system is conserved if the net external force acting on it is zero. As the given system of masses has no external force acting on it, its momentum is conserved.

The initial momentum of the system can be calculated as:pi = mv + 0Since mass M is at rest, its initial momentum is zero. Therefore, the total initial momentum of the system ispi = mv. The final momentum of the system can be calculated as:pf = (m + M)V. Here, V is the common velocity of masses m and M after the impact, which can be calculated using the principle of conservation of mechanical energy.

As the given system of masses is an example of an inelastic collision, some energy is lost during the impact due to deformation of the masses. Therefore, the conservation of mechanical energy can be written as:

1/2 mv² = (1/2) (m + M) V²

Solving for V, we get:V² = mv² / (m + M)V = v * sqrt(m / (m + M))

Therefore, the final momentum of the system can be calculated as:pf = (m + M) v * sqrt(m / (m + M)) = v * sqrt(m (m + M))

Therefore, applying the principle of conservation of linear momentum, we have:pi = pfmv = v * sqrt(m (m + M))v = mv / sqrt(m (m + M))

Hence, the common velocity of masses m and M after the impact is v = mv / sqrt(m (m + M)).

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The amplitude of the emf in the coil is 62.8 V. We can use the formula below to determine the amplitude of the emf in the coil.E = NBAω

We know that the cross-sectional area of the coil is 20.0 cm² and the number of turns in the coil is 1000.

Therefore, we have N = 1000. Also, the magnetic field in the coil is given as B = 0.5 T.

Let's recall the formula for the amplitude of the emf in the coil given as:E = NBAω,

where, E is the emf in the coil N is the number of turns in the coil, B is the magnetic field,

A is the cross-sectional area of the coil, ω is the angular frequency of the coil.

Using the given values, we can find the amplitude of the emf in the coil as follows:

E = NBAω= 1000 × 0.5 × 20.0 × π × 50= 62,832.0 V= 62.8 V (to 3 significant figures).

Hence, the amplitude of the emf in the coil is 62.8 V.

Therefore, the amplitude of the emf in the coil is 62.8 V.

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The initial velocity of a projectile launched horizontally can be calculated using the equation of distance covered horizontally (x) = Initial velocity (u)  Time of flight (t). The horizontal component of the initial velocity can be determined by x = u  t, t = 1.63 s, x = 6.5 mu = x / t = 6.5 m / 1.63 su = 3.99 m/s  4.00 m/s.

The initial velocity of the projectile that was launched horizontally can be calculated using the equation below: Distance covered horizontally (x) = Initial velocity (u) × Time of flight (t) where, Time of flight (t) can be found using the formula below: t = [2 × vertical height (h)] / g where ,g is the acceleration due to gravity = 9.8 m/s².The vertical height (h) of the projectile is 8.0 m. So the time of flight of the projectile will bet = [2 × 8.0 m] / 9.8 m/s²t = 1.63 s Therefore, the horizontal component of the projectile’s initial velocity can be determined by: x = u × tt = 1.63 s, x = 6.5 mu = x / t = 6.5 m / 1.63 su = 3.99 m/s ≈ 4.00 m/s. So, the projectile was launched horizontally with a velocity of 4.00 m/s (rounded to the nearest hundredth).Content loaded: The term “content loaded” is used to indicate that the contents of a webpage or app have finished loading and are ready for viewing or use.

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The following are the steps to solve the given problem:

1. Let us consider the two blocks as A and B, where A is the 4.0 kg block and B is the 5.0 kg block.

We can now use the formula F = m * a to calculate the acceleration produced in each block due to the applied force.

Substituting the values of m(A) = 4.0 kg and m(B) = 5.0 kg in step 10, we geta(B) / a(A) = 5.0 / 4.0a(B) = (5.0 / 4.0) * a(A)

we geta(B) = (5.0 / 4.0) * a(B)a(B) = 1.25 * a(B)

Solving for a(B), we geta(B) = F / m(B)a(B) = F / 5.0 kg

Substituting the value of a(B) from step 15 in step 14, we get

F / 5.0 kg = 1.25 * Fa(B) = (5.0 / 4.0) * F

we know that F(A on B) = - F(B on A). Hence, we can write

F(B on A) = - (5.0 / 4.0) * F

The force acting on block B due to block A is the force that we need to calculate. Hence,

F(B on A) = (5.0 / 4.0) * F

The 4.0 kg block exerts a force of (5.0 / 4.0) * F on the 5.0 kg block.

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The relationship when a function of the form y = ab^x is used to fit the data is called an exponential relationship or exponential function.

In this equation, "a" represents the initial value or y-intercept, "b" is the base of the exponential function, and "x" is the independent variable. The exponential function is commonly used to model situations where the dependent variable, y, changes exponentially with respect to the independent variable, x. A function is a mathematical concept that relates input values (called the domain) to output values (called the range). It represents a specific relationship between variables or quantities. A function takes one or more inputs and produces a unique output for each input. It can be represented by an equation, a formula, a graph, or a verbal description.

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The electric potential energy of the particle with a charge of 5nC, located 0.5m away from a charge of 9.5nC, is 1.9 J.

To calculate the electric potential energy, we can use the formula:

Electric potential energy = (k * q1 * q2) / r

Where:

k is the electrostatic constant (9 x 10^9 N m^2/C^2),

q1 and q2 are the charges of the two particles (in this case, 5nC and 9.5nC, respectively),

r is the distance between the charges (0.5m).

Substituting the given values into the formula:

Electric potential energy = (9 x 10^9 N m^2/C^2) * (5 x 10^-9 C) * (9.5 x 10^-9 C) / 0.5m

Calculating the expression:

Electric potential energy ≈ 1.9 J

Therefore, the electric potential energy of the particle is approximately 1.9 Joules.

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Inertia refers to the natural tendency of every object to resist any change in either speed or direction. Every object tends to maintain its state of motion until an external force acts on it.

Inertia is an essential concept in physics, and it can be observed in everyday life. Here is how you can observe inertia in your everyday life:

When you are in a moving car, and the driver suddenly stops, your body tends to move forward. This is because of inertia. Your body is already in motion, and when the car stops, your body tends to keep moving in the same direction. The seatbelt helps to prevent this movement by exerting a force on your body in the opposite direction.

When you are on a merry-go-round and it starts spinning, you tend to feel a force pushing you away from the center of the ride. This is also due to inertia. Your body is already in motion, and when the ride starts spinning, your body tends to keep moving in the same direction. The force that pushes you away from the center of the ride is known as the centrifugal force.

When you are playing a game of pool, and you hit the cue ball, it tends to keep moving until it comes into contact with another ball or hits the wall of the table. This is also due to inertia. The cue ball is already in motion, and it tends to maintain its state of motion until it comes into contact with another object or hits the wall of the table.

These are just a few examples of how you can observe inertia in your everyday life.

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Assuming a constant density, the size of an object scales as its mass raised to the power of 1/3 (one-third).

The mass, density, and volume of an object are related by the equation:

ρ = m/Vwhere ρ is the density, m is the mass, and V is the volume.

We can write this equation as

V = m/ρThis equation can be used to find the relationship between the mass and volume of an object of constant density.

Assume that we have two objects of the same material with masses m1 and m2.

We can find the ratio of their volumes by taking the ratio of their masses and density as follows:

V1/V2 = m1/ρ / m2/ρV1/V2 = m1/m2V1/V2 = (m1/m2)^(1/3)

This shows that the ratio of the volumes of two objects with the same density is proportional to the cube root of the ratio of their masses.

This relationship can be expressed as:

V ∝ m^(1/3)

This relationship can also be expressed as the size of an object scales as its mass raised to the power of 1/3.

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To determine the crate's final velocity after 0.5 seconds, we can use the concept of Newton's second law of motion, which states that the net force acting on an object is equal to its mass multiplied by its acceleration.

In this scenario, the stevedore applies a horizontal force of 175 N to move the crate along the dock. However, there is also an opposing force of friction acting in the opposite direction, which has a magnitude of 120 N. The net force is the difference between these two forces, so we can calculate it as follows:

Net force = Applied force - Frictional force

Net force = 175 N - 120 N

Net force = 55 N

Now, using Newton's second law of motion, we can determine the acceleration of the crate. Rearranging the equation, we have:

Net force = mass * acceleration

55 N = 50 kg * acceleration

Solving for acceleration:

acceleration = 55 N / 50 kg

acceleration = 1.1 m/s²

Since we know the initial velocity of the crate is zero (as it starts from rest), and we want to find the final velocity after 0.5 seconds, we can use the equation of motion:

final velocity = initial velocity + (acceleration * time)

Plugging in the values:

final velocity = 0 + (1.1 m/s² * 0.5 s)

final velocity = 0.55 m/s

Therefore, the crate's final velocity after 0.5 seconds is 0.55 m/s. This means that after being subjected to a 175 N force and experiencing 120 N of friction, the crate gains a velocity of 0.55 m/s in the direction of the applied force.

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When solving the problem of pool game and calculating the magnitude of the final velocity of the cue ball, the correct option is 0.56 m/s.

The following method: Use the principle of conservation of momentum, i.e. momentum before the collision is equal to the momentum after the collision, which is mathematically written as: [tex]$$mv_1+Mv_2=(m + M)v_3$$[/tex]

Where, m is the mass of the cue ball,

M is the mass of the striped ball,

v1 is the velocity of the cue ball before the collision,

v2 is the velocity of the striped ball before the collision, and

v3 is the velocity of the cue ball after the collision.

Using the above formula, we get the final velocity of the cue ball as:

[tex]$$v_3=frac {mv_1+Mv_2}{m+M}$$[/tex]

Plug in the given values, we get,

[tex]$$v_3=frac{0.4*0.80+0.4*0.38}{0.4+0.4}$$[/tex]

Solving for v3, we get [tex]$v_3=0.59$[/tex] m/s Therefore, the magnitude of the final velocity of the cue ball is 0.59 m/s.

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The initial velocity of the ball is (b) 31 m/s. This is the velocity of the ball at point B, which is the point where it just hits the ground.

The velocity of the ball at point B, just before it hits the ground, can be determined using the principles of projectile motion and considering the effects of gravity.

Calculate the velocity of the ball at point B by using the following equation:

v = u + at

Where:

v = final velocity

u = initial velocity

a = acceleration

t = time

In this case:

v = 31 m/s

a = 9.8 m/s²

t = 0 (the ball is just about to hit the ground)

Solve for u (the initial velocity) as follows:

31 = u + 9.8 × 0

31 = u

Therefore, the initial velocity of the ball is 31 m/s. This is the velocity of the ball at point B, which is the point where it just hits the ground.

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Complete question:

A ball is thrown upward with an initial velocity of 31 m/s. At position B, where the ball just exactly before it hit the ground, how fast is the ball at point B?

(a) 980 m/s

(b) 31 m/s

(c) 980 m/s²

(d) 31 m/s²