a person with a mass of 78 kg is riding in an elevator that is accelerating upward at 1.80 m/s2. what is the person's apparent weight? (use g

In an alternating current circuit that contains a resistor, an inductor, and a capacitor with 120V, you can find the current by using Ohm's Law.

Ohm's Law states that the current is equal to the voltage divided by the resistance.

To calculate the resistance in an alternating current circuit, you must take into account the resistor, inductor, and capacitor.

For example, if the resistor has a resistance of 10 ohms, the inductor has a resistance of 5 ohms, and the capacitor has a resistance of 20 ohms, then the total resistance would be 35 ohms.

Therefore, the current in the circuit would be 120V/35 ohms = 3.43A.

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The traveler's weight on another planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth is 21.647 N

The following is the solution to the given problem:

Mass and gravity are related to one another. Gravity is generated by the planet's mass, and the magnitude of the gravitational force is determined by the mass of the planet on which the object is situated, as well as the mass of the object.

Mass, distance, and gravity are all factors that influence the gravitational force. Mass is directly proportional to the gravitational force and inversely proportional to the square of the distance from the gravitational force's center.

Here is the formula: Force of gravity = G(M1M2)/d²where, G is the gravitational constant 6.67 x 10^{-11} N(m/kg)^2, M1 is the mass of the first body, M2 is the mass of the second body, d is the distance between the centers of two bodies.

On earth, the traveler weighs 682 N. On another planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth, we have to calculate the traveler's weight.

Mass of Earth is 5.972 × 10^24 kg2,

Radius of Earth is 6.371 x 10^63.

The mass of the planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth.

Mass of the planet = 2 x mass of Earth = 2 x 5.972 × 10^24 kg = 1.1944 × 10^25 kg4.

The radius of the planet whose radius is 3 times that of Earth,

Radius of the planet = 3 x radius of Earth = 3 x 6.371 x 10^6 m = 1.9113 × 10^7 m5.

The distance between the two planets.

Distance between two planets = radius of planet + radius of Earth

= 1.9113 × 10^7 m + 6.371 x 10^6 m

= 2.54813 x 10^7 m

= 2.54813 x 10^10 cm.

Putting all the values in the formula.

Force of gravity = G (M1 M2) / d²

Where, Mass of the traveler on the other planet is m.

Mass of the Earth is M1 = 5.972 × 10^24 kg.

Mass of the other planet is M2 = 2 x 5.972 × 10^24 kg = 1.1944 × 10^25 kg.

Radius of the Earth is r1 = 6.371 x 10^6 m.

Radius of the other planet is r2 = 3 x 6.371 x 10^6 m = 1.9113 × 10^7 m.

Distance between the two planets is d = 2.54813 x 10^10 cm.682

= G (M1 M2)/d²

G = 6.674 × 10^-11 N m² / kg²

Force of gravity on other planet = G(mM2)/r² where m is the mass of the traveler on the other planet

= 6.674 × 10^-11 × (m × 1.1944 × 10^25)/(1.9113 × 10^7)²

Weight on another planet = force of gravity on another planet × mass of the traveler on another planet

= (6.674 × 10^-11 × (m × 1.1944 × 10^25)/(1.9113 × 10^7)²) × m

= 21.647 N (approximately)

Therefore, the traveler's weight on another planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth is 21.647 N (approximately).

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The recoil speed of the rifle is 0.075 m/s in the opposite direction to the direction of the bullet.

To calculate the recoil speed of the rifle, we can use the conservation of momentum principle. According to this principle, the total momentum of the system (bullet + rifle) is conserved before and after the firing of the bullet.

Initially, the total momentum of the system is zero because the rifle and bullet are at rest. After firing the bullet, the total momentum of the system is given by:

m1v1 + m2v2 = 0

where m1 and v1 are the mass and velocity of the bullet, and m2 and v2 are the mass and recoil velocity of the rifle, respectively.

Substituting the given values, we get:

(0.001 kg)(150 m/s) + (2.0 kg)(v2) = 0

Solving for v2, we get:

v2 = -(0.001 kg)(150 m/s) / (2.0 kg)

v2 = -0.075 m/s

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The tension in the rope is 173.55 N.

Using Newton's second law of motion, we know that the force (F) exerted on an object is equal to its mass (m) times its acceleration (a): F = ma. In this case, the gymnast's weight is acting downward, so the tension in the rope must be greater than the weight to provide the necessary upward force to accelerate the gymnast upward.

Thus, we can calculate the tension in the rope as follows:

Tension - Weight = ma

T - mg = ma

where T is the tension in the rope, m is the mass of the gymnast, g is the acceleration due to gravity (9.8 m/s^2), and a is the acceleration of the gymnast upward.

T - (63 kg)(9.8 m/s^2) = (63 kg)(2.5 m/s^2)

T = (63 kg)(9.8 m/s^2 + 2.5 m/s^2) = 173.55 N

Therefore, the tension in the rope is 173.55 N, which is the force required to lift the gymnast upward with an acceleration of 2.5 m/s^2.

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Matter affects our daily lives in the sense all is composed of matter and energy.

Matter and energy in the Universe and daily life are two basic elements that characterize the physic system and allow us to understand the world. In regard to matter, it is something that occupies space and has mass, while energy can perform work.

Therefore, with this data, we can see that matter and energy in the Universe and daily life are fundamental to understanding the universe.

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Amplitude is not measured from peak to trough, but from rest to peak or rest to trough.

The highest and lowest points on the surface of a wave are called crests and troughs respectively. The vertical distance between the peak and the trough is the height of the waves. The horizontal distance between two successive peaks or troughs is called the wavelength.

The amplitude of a wave is the maximum displacement of a particle on a medium with respect to its position of rest.

The amplitude can be thought of as the distance between rest and the peak. The amplitude from the rest position to the dip position can be measured in a similar manner.

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In Young's single slit experiment, if the width of the slit decreases, the width of the diffracted peaks increases.

Young's experiment involves a single slit that diffracts light and produces a pattern of bright and dark fringes on a screen. The width of the slit affects the diffraction of light through the slit and determines the width of the bright fringes on the screen.

The narrower the slit, the greater the diffraction of light, which causes the bright fringes to become wider.

This is because diffraction causes the light waves to spread out as they pass through the narrow slit, leading to interference and the formation of bright and dark fringes on the screen.

Therefore, if the width of the slit decreases, the width of the diffracted peaks increases.

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A net force of 10 N acts on the rock when it is halfway to the top of its path.

The net force acting on the rock can be calculated using the following equation:

Fnet = ma

Where Fnet is the net force, m is the mass, and a is the acceleration.

When the rock is halfway to the top of its path, its velocity is zero since it momentarily stops at the top of its motion. As a result, its acceleration is equal to the acceleration due to gravity, which is -10 m/s² since it is acting in the opposite direction to the upward direction. This is the gravitational force acting on the rock.

We can now calculate the net force acting on the rock at this point in its motion:

Fnet = ma

Fnet = (1 kg)(-10 m/s²)

Fnet = -10 N

Since the acceleration due to gravity is acting downward and the rock is moving upward, the net force is equal to the force of gravity, which is 10 N.

Therefore, the net force that acts on the rock when it is halfway to the top of its path is -10 N or 10 N in the downward direction. This net force is equal in magnitude to the weight of the rock.

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The magnitude of the change in the momentum of the billiard ball is 0.268 kg⋅m/s. The direction of the change of momentum vector points at 59.6 degrees, measured counterclockwise from the x-axis along the cushion.

This result can be found by using the equation for conservation of momentum, which states that both the magnitude and the direction of the momentum before and after the collision must be the same.

Since the mass and the speed of the ball changed, the direction of the vector must have changed as well. In this case, the vector changed direction from 60 degrees to 47 degrees, a difference of 13 degrees.

This means that the vector must have rotated counterclockwise by 13 degrees, or in other words, the change of momentum vector points at 59.6 degrees, measured counterclockwise from the x-axis along the cushion.

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The longest wavelength of the light required to cause photoelectric effect is 349 nm (in nm units).

A photoelectric effect occurs when light falls on a metal surface, causing electrons to be emitted from the metal surface. It's a phenomenon that demonstrates the particle-like nature of light, which is made up of photons, as well as the wave-like nature of light.

Einstein first proposed the idea of the photoelectric effect, which eventually helped him win the Nobel Prize in Physics in 1921.Photoelectric Effect’s Formula

The photoelectric effect's formula is as follows:

Kinetic Energy = Energy of Photon - Work Function

KE = hf - Φ

For this question, we have work function, and we will use it to find the longest wavelength.

The formula of work function is given as Φ= hf0

Where f0 is the threshold frequency (frequency of the incoming light, below which the photoelectric effect does not occur).h = Planck’s constant = 6.626 x 10^-34 J s = 4.136 x 10^-15 eV s

The longest wavelength of the light required to cause photoelectric effect is given asλ = c / f

Here, λ is the wavelength of the incoming light, c is the speed of light, and f is the frequency of the incoming light.

We have to solve the work function equation to find the threshold frequency.

The formula is given asf0 = Φ/h

Substituting the values, we get:f0 = 3.56 eV / 4.136 x 10^-15 eV s = 8.60 x 10^14 Hz

To find the longest wavelength, we use the following formula:

λmax = c / f0 = (3 x 10^8 m/s) / (8.60 x 10^14 Hz) = 3.49 x 10^-7 m = 349 nm

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A dieter lifting a 10 kg mass 1000 times to a height of 0.5m each time does 49.05 J of work per lift, resulting in the total amount of work done and fat burned is calculated by total amount of energy.

(a) The amount of work done against the gravitational force is calculated by using the formula:

W = m*g*h

where m is the mass,

g is the acceleration due to gravity, and

h is the height.

The person lifts a 10 kg mass to a height of 0.5 meters, so the work done each time is:

[tex]W = (10 kg) * (9.8 m/s^2) * (0.5 m) = 49 Joules.[/tex]

The total work done against the gravitational force is:

[tex]W_{total}= (49 J) * (1000) = 49,000 J.[/tex]

(b) To calculate the amount of fat burned, we need to find the total amount of energy expended and divide it by the efficiency rate and the energy per kilogram of fat.

The total amount of energy expended by the person is:

[tex]E_{total} = W_{total} = 49,000 J.[/tex]

The efficiency rate is 20%, which means that 20% of the expended energy is converted to mechanical energy.

The energy per kilogram of fat is [tex]3.8*10^7[/tex] Joules/kg.

Therefore, the amount of fat burned is:

Fat burned = [tex]E_{total}[/tex] / (efficiency rate * energy per kg of fat)

Fat burned = 49,000 J / (0.2 * 3.8 x 10⁷ J/kg)

Fat burned = 0.0645 kg of fat (or 64.5 grams of fat).

So, the person will burn approximately 64.5 grams of fat by lifting a 10 kg mass 1000 times to a height of 0.5 meters each time.

Also the total work done against gravitational force is 49,000J.

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The headline "Enlightenment ideas of freedom, equality, and justice for all" represents the idea of the Enlightenment that human beings are rational, capable of determining right from wrong, and deserving of rights and freedoms, such as freedom of speech, freedom of religion, and equality before the law.

These ideas were a major factor in the shift away from absolute monarchies, and towards governments of the people, by the people, and for the people. The Enlightenment period also saw the development of democracy and of the rule of law, where the government is subject to a set of laws, rather than relying on the whims of the ruler. Enlightenment thinkers sought to empower the individual, giving people the freedom to think and act as they pleased, rather than relying on the decisions of rulers.

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You will feel yourself pressed against the back of your spacecraft with great force, making it difficult to move. This is because when you accelerate, the force of gravity is increased, causing you to feel an increased weight.

This option is the correct one. As per Newton's second law, the force of the body is directly proportional to the mass and acceleration. Here, the acceleration is 9.8 m/s2, which means you will feel yourself pressed against the back of your spaceship with great force, making it difficult to move, you will feel the same weight as you do on earth.

This is an incorrect option because the acceleration is greater than 1g, which means the weight will be greater than the actual weight.you will be floating weightlessly. This is an incorrect option because there is an acceleration, which means you will not be floating weightlessly.you will feel weight, but more than on earth. This is an incorrect option because the acceleration is greater than 1g, which means the weight will be greater than the actual weight.

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The tension in each cable must be equal to the mass of the cargo multiplied by the acceleration due to gravity, and divided by the number of cables.

In order to determine the tension in each cable required to support the cargo in static equilibrium, we can use Newton's Second Law of Motion.

This law states that the sum of the forces acting on an object must be equal to the object's mass multiplied by its acceleration.
The tension in each cable (T) must be equal to the weight of the cargo (W) divided by the number of cables (n).

So the equation would be:  

T = W/n.
To find the value of T, we can use the formula

W = mg

where m is the mass of the cargo and g is the acceleration due to gravity.

Plugging this into the equation for T, we have:

T = mg/n.

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This is due to the fact that the first and second laws of thermodynamics are universally applicable fundamental principles that can be utilised to examine particular systems and processes.

The part of thermodynamics that deals with chemical reactions is called chemical thermodynamics. The first law states that energy is conserved and cannot be created or destroyed. Second law: When natural processes in a closed system result in a rise in entropy, they are spontaneous.

According to the second rule of thermodynamics, an isolated system that is out of equilibrium over time must increase in entropy until it reaches the ultimate equilibrium value.

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Yes, it is reasonable to expect that you would see the Sun with a sensitive radio telescope.

Radio waves can penetrate through the clouds and the atmosphere, so with a powerful radio telescope you can observe the Sun even on a cloudy day.

Gather the necessary components of the radio telescope, such as a dish and receiver. Point the radio telescope towards the Sun. Tune the receiver to the proper frequency. Take a look at the results from the telescope and observe the Sun.

Therefore, you can expect that you would see the Sun with a sensitive radio telescope.

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The value of the ratio m1/m2 is approximately 0.3559.

Given that a force F applied to an object of mass m1 produces an acceleration of 7.36 m/s², and the same force applied to a second object of mass m2 produces an acceleration of 2.62 m/s².To find the value of the ratio m1/m2, we can use the equation: F = ma Where, F = force m = mass a = acceleration. We have F and a for both objects, and we need to find the ratio of masses m1/m2.Let's write the equation for both objects and then divide the two equations:For object 1:F = m1a1------------------------(1)For object 2:F = m2a2------------------------(2)Dividing the equation (1) by equation (2):m1a1/m2a2 = m1/m2 = (F/m1a1)/(F/m2a2)= (m2a2/F)/(m1a1/F)Now, substituting the values of a1, a2, and F, we get:m1/m2 = (m2 x 2.62)/(m1 x 7.36)= 2.62m2/7.36m1= 0.3559(m2/m1)Therefore, the value of the ratio m1/m2 is approximately 0.3559.

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If the frequency of the incoming light is decreased, the energy of the ejected electrons will decrease.

The frequency of the incoming light will affect the energy of the ejected electrons. This is because the energy of the ejected electrons is proportional to the frequency of the incoming light.

The energy of the electrons can be determined using the equation:

E = h * f,

where E is the energy, h is Planck’s constant, and f is the frequency of the incoming light. This equation shows that the energy of the electrons is directly proportional to the frequency of the incoming light.

Therefore, if the frequency of the incoming light is decreased, the energy of the ejected electrons will also decrease.

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20 cm apart, the charges of +1.0 x 10⁻⁶ C and –1.0 x 10⁻⁶ C exert a force of 449.5 N on one another. This force is directed from the negative charge to the positive charge.

According to Coulomb's law, the force F between two point charges, q1 and q2, that are separated by a distance r, is computed as F=k|q1q2|r2.

It is possible to determine the force between two point charges using Coulomb's law:

F = k*(q1*q2)/r²

In this case, we have[tex]q1 = +10.0 x 10^-6 C, q2 = -50.0 x 10^-6 C, and r = 20 cm = 0.2 m.[/tex]

Plugging in these values, we get:

[tex]F = (8.99 x 10^9 N m^2/C^2) * [(+10.0 x 10^-6 C) * (-50.0 x 10^-6 C)] / (0.2 m)^2[/tex]

Simplifying, we get:

F = -449.5 N.

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The outcomes based on whether thermal energy is added or being removed are:

Thermal energy added :

Thermal energy being removed :

When thermal energy is added to a substance, the particles absorb this energy and start moving faster, which means their kinetic energy increases. This leads to an increase in temperature because the faster-moving particles collide with each other more frequently, transferring this extra energy in the form of heat.

Therefore, an increase in temperature and an increase in the kinetic energy of particles result from thermal energy being added, while a decrease in temperature and a decrease in the kinetic energy of particles result from thermal energy being removed.

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The drag force exerted on an object moving through air (a.k.a. force of air resistance) is proportional to the square of the velocity of the object.

Thus, the correct answer is proportional to the square of the velocity of the object.

The аir resistаnce force аcting on аn object moving through аir is referred to аs drаg force. When а body trаvels through а fluid such аs wаter or аir, it fаces resistаnce to its motion, which is proportionаl to the velocity of the object. This resistаnce force аcting on а body moving through аir is referred to аs аir resistаnce or drаg force.

The drаg force on аn object in the аir is proportionаl to the squаre of the object's velocity. When the velocity of the object is doubled, the drаg force becomes four times greаter. Thus, the drаg force grows fаster thаn the object's velocity. In other words, the drаg force аcting on аn object increаses аs the squаre of the object's velocity.

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The blue objects absorb most wavelengths but reflect light at about 450 nm. This phenomenon relates to the colors of objects.

When the sunlight falls on an object, some of the light is absorbed, and the rest of the light is reflected. Objects appear to be a certain color because they absorb some colors of light and reflect others. Some objects appear blue because they absorb all colors of light except blue.

Blue light has a shorter wavelength than other colors of light, so it is scattered more in the Earth's atmosphere. The sky appears blue because the shorter blue wavelengths are scattered in all directions and are more likely to reach the observer's eye.

The light that is reflected off blue objects is at a wavelength of around 450 nm. When white light passes through a prism, it splits into the colors of the spectrum.

Violet light has the shortest wavelength, and red light has the longest wavelength. Between violet and green, the colors blend to form blue. So, if blue objects reflect light at around 450 nm, that means they reflect blue light.

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(a)The time-averaged energy density is:U = (1/2μ) |E x B|² = (1/2μ) E₀² B₀² sin²(kx - ωt).

(b)The intensity of an electromagnetic wave is defined as the time-averaged power per unit area. It can be calculated using the Poynting vector: I = <S> = (1/2μ) |E x B|².

S = (1/μ) E x B

where E is the electric field, B is the magnetic field, and μ is the permeability of the medium. In a conducting medium, the permeability is generally the same as that of free space, so μ = μ0.

The time-averaged energy density is then given by:

U = (1/2μ) |E x B|^2

where |E x B| is the magnitude of the cross product of the electric and magnetic fields. Since the cross product of two vectors is orthogonal to both vectors, |E x B| represents the strength of the electromagnetic field.

In a plane wave, the electric and magnetic fields are perpendicular to each other and to the direction of propagation. Without loss of generality, let's assume that the electric field is in the x-direction and the magnetic field is in the y-direction. Then we have:

E = E₀ sin(kx - ωt) i

B = B₀ sin(kx - ωt + π/2) j

where E₀ and B₀ are the amplitudes of the fields, k is the wave vector, ω is the angular frequency, and i and j are unit vectors in the x- and y-directions, respectively.

Taking the cross product of E and B, we have:

E x B = E₀ B₀ sin(kx - ωt) k

Therefore, the time-averaged energy density is:

U = (1/2μ) |E x B|² = (1/2μ) E₀² B₀² sin²(kx - ωt)

Since the sine function oscillates between -1 and 1, the maximum value of sin^2(kx - ωt) is 1. Therefore, the maximum value of the energy density is:

Umax = (1/2μ) E₀² B₀²

Note that the energy density is proportional to both the electric and magnetic field strengths. However, the permeability of a conducting medium is generally less than that of free space, which means that the magnetic field is amplified relative to the electric field. This leads to a situation where the magnetic contribution to the energy density dominates over the electric contribution.

(b) The intensity of an electromagnetic wave is defined as the time-averaged power per unit area. It can be calculated using the Poynting vector:

I = <S> = (1/2μ) |E x B|²

where the brackets denote a time average.

The energy density U is related to the intensity I by:

U = I/ω

where ω is the angular frequency. Substituting the expression for U from part (a), we have:

I/ω = (1/2μ) E₀² B₀²

Solving for I, we obtain:

I = (ω/2μ) E₀² B₀²

Recall that the speed of light in a medium is given by:

v = 1/√(με)

where ε is the permittivity of the medium. Therefore, the wave number k and the angular frequency ω are related by:

k = ω/v = ω√(με)

Substituting this expression into the expression for I, we have:

I = (k/2uw) E₀²

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A force of 245 N must be applied vertically to lift the bag off the baggage cart.

The force that must be applied vertically to lift a bag off a baggage cart, given that the bag has a mass of 25 kg, can be determined using the formula F = m*g

where F is force, m is mass, and g is acceleration due to gravity. The value of g is 9.8 m/s².So, F = 25 kg x 9.8 m/s² = 245 N. Therefore, a force of 245 N must be applied vertically to lift the bag off the baggage cart.

The mass of the bag = 25 kg.The formula used is, F = m*gwhereF = Force required to lift the bagm = Mass of the bagg = Acceleration due to gravityF = 25 kg x 9.8 m/s² = 245 N.

Therefore, a force of 245 N must be applied vertically to lift the bag off the baggage cart.

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The amount of the star's mass converted to energy in the explosion is 1.11 x 10^27 kg.

Calculating energy:

The mass-energy equivalence equation is used to calculate the mass that is converted to energy during a supernova explosion of a 3.2 x 10^31 kg star, producing 1.0 x 10^44 J of energy.

According to Einstein's mass-energy equivalence equation: E = mc² where, E = energy, m = mass, and c = speed of light This equation expresses the relationship between the mass of an object and the amount of energy that can be released from it.

So, to determine the mass that is converted to energy during the supernova explosion, we need to rearrange the equation as m = E/c². Now we have the following data: E = 1.0 x 10^44 Jc = 3.0 x 10^8 m/s² (speed of light). Substitute these values into the equation to get: m = E/c²m = (1.0 x 10^44 J)/(3.0 x 10^8 m/s)²m = 1.11 x 10^27 kg

Therefore, the supernova explosion of a 3.2 x 10^31 kg star converts 1.11 x 10^27 kg of its mass to energy.

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The charge on each sphere after they are separated is [tex]4.71 × 10^-7 C.[/tex]

The initial electrostatic force between the two spheres before they come in contact is given by Coulomb's law:

[tex]F = k(q1)(q2) / r^2[/tex]

where F is the electrostatic force, k is Coulomb's constant (9 × [tex]10^9[/tex] [tex]N·m^2/C^2)[/tex], q1 and q2 are the charges on the spheres, and r is the distance between them.

Since the two spheres are identical, we can assume that they have the same charge q before they come in contact. Therefore, we can rewrite Coulomb's law as:

[tex]F = kq^2 / r^2[/tex]

After the spheres come in contact and then are separated again, their charges are redistributed. Since the spheres have the same charge initially and they are identical, we can assume that they now have equal charges q'. The final electrostatic force between the spheres is also given by Coulomb's law:

[tex]F' = k(q')^2 / r^2[/tex]

We know that the final force is 0.1 N, and the initial distance between the spheres is 45 m. We can use these values to find the initial charge q:

[tex]0.1 N = kq^2 / (45 m)^2[/tex]

[tex]q^2 = (0.1 N)(45 m)^2 / k[/tex]

[tex]q = sqrt[(0.1 N)(45 m)^2 / k][/tex]

Substituting the values, we get:

q = 6.67 × 10^-7 C

Now that we know the initial charge q, we can use Coulomb's law to find the final charge q':

[tex]0.1 N = k(q')^2 / (45 m)^2[/tex]

[tex]q' = sqrt[(0.1 N)(45 m)^2 / k][/tex]

Substituting the values, we get:

q' = 4.71 × 10^-7 C

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The frequency of the sound waves created by the guitar string is 256 Hz.

The number of oscillations of the guitar string in 30 seconds is 7680.

The frequency of the guitar string is defined as the number of oscillations per second, so we can calculate the frequency by dividing the total number of oscillations by the time it took to make them:

frequency = number of oscillations / time

frequency = 7680 / 30 seconds = 256 Hz

Therefore, the frequency of the sound waves created by the guitar string is 256 Hz.

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The angle at which the ray is reflected from the first interaction with the surface of the diamond is known as the angle of reflection. When a light ray hits a surface, it reflects back at the same angle as the angle of incidence.

What is the angle of incidence?

The angle between the incident ray and the normal ray is called the angle of incidence. The incident ray is the ray of light that falls on the surface, while the normal is an imaginary line perpendicular to the surface. The angle of incidence can be calculated by measuring the angle between the incident ray and the normal.

The angle between the reflected ray and the normal ray is known as the angle of reflection. When a light ray hits a surface, it reflects back at the same angle as the angle of incidence. Therefore, the angle of reflection can be calculated by measuring the angle between the reflected ray and the normal.

In summary, the angle at which the ray is reflected from the first interaction with the surface of the diamond is the angle of reflection, which is equal to the angle of incidence. Therefore, the ray is reflected at the same angle as the angle at which it strikes the diamond's surface.

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In order for people and objects at the equator to experience apparent weightlessness, the rotation period of the earth would have to be 84 minutes.

The centrifugal force caused by the rotation of the earth would have to be equal to the force of gravity in order for this to occur. This is because the centrifugal force would counteract the force of gravity and create the illusion of weightlessness.

To calculate the required rotation period, we can use the following formula:

rotation period = 2π√(r/g)where r is the radius of the earth and g is the acceleration due to gravity.

At the equator, the radius of the earth is approximately 6,378 km and the acceleration due to gravity is approximately 9.81 m/s^2.

Rotation period = 2π√(6,378,000/9.81)

rotation period ≈ 5066 seconds

rotation period ≈ 84 minutes

Therefore, the rotation period of the earth would have to be approximately 84 minutes for people and objects at the equator to experience apparent weightlessness.

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Answer:

Explanation:

A seatbelt is designed to stretch a bit when the car decelerates rapidly. You travel forward a little while being stopped - you do not stop sharply as you would if you hit the dashboard. The seatbelt stretching increases the time over which your momentum is changed, thereby decreasing the force experienced by your body.

Airbags are made from a strong coated fabric. They are stored in a module mounted on the steering wheel and dashboard and side panels of the car. The inflation of them is initiated by crash sensors that activate upon impact at speeds of more than 10-15 miles per hour. They are mounted in several locations on the car body. In a crash, the sensor sends an electrical signal to the airbag which then causes the airbag to deploy. It ignites a chemical propellant which produces nitrogen gas, which then inflates the bag itself.