light with an intensity of 1 kw/m2 falls normally on a surface with an area of 1 cm and is completely reflected. the force of the radiation on the surface is

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Answer 1

The force exerted by the radiation on the surface can be found using the formula F = P/c, where c is the speed of light in m/s. In this specific case, the force is approximately 3.3 x 10^-10 N.

To calculate the force of the radiation on the surface, we first need to find the total power (P) that falls on the surface. Power is the rate at which energy is transferred, and is given by the formula:

P = I x A

where I is the intensity of the light in watts per square meter (W/m2) and A is the area of the surface in square meters (m2).

In this case, the intensity is given as 1 kW/m2, or 1000 W/m2 (since 1 kW = 1000 W). The area is given as 1 cm2, or 0.0001 m2 (since 1 m2 = 10,000 cm2).

So, we have:

P = I x A = 1000 W/m2 x 0.0001 m2 = 0.1 W

Next, we need to find the force (F) exerted by the radiation on the surface. This can be done using the formula:

F = P/c

where c is the speed of light, which is approximately 3 x 108 meters per second (m/s).

Substituting the values we have:

F = P/c = 0.1 W / 3 x 108 m/s = 3.3 x 10^-10 N

Therefore, the force of the radiation on the surface is approximately 3.3 x 10^-10 N.

In summary, the long answer is that the force of the radiation on the surface is found by first calculating the total power that falls on the surface using the formula P = I x A, where I is the intensity of the light in W/m2 and A is the area of the surface in m2. Next, the force exerted by the radiation on the surface can be found using the formula F = P/c, where c is the speed of light in m/s. In this specific case, the force is approximately 3.3 x 10^-10 N.

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Related Questions

in a double-slit experiment, the third-order maximum for light of wavelength 480 nm is located 16 mm from the central bright spot on a screen 1.6 m from the slits. light of wavelength 650 nm is then projected through the same slits. how far from the central bright spot will the second-order maximum of this light be located?

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The  second-order maximum for light with a wavelength of 650 nm will be located 8.35 × 10^-6 m, or 8.35 μm, from the central bright spot on the screen.

In a double-slit experiment, the location of the bright fringes can be determined using the equation:

d sin θ = mλ

where d is the distance between the slits, θ is the angle between the line from the center of the slits to the fringe and the line perpendicular to the screen, m is the order of the maximum, and λ is the wavelength of light.

For the third-order maximum of light with a wavelength of 480 nm, we have:

λ = 480 nm = 4.80 × 10^-7 m
m = 3
d = unknown
θ = sin^-1[(16 mm) / (1.6 m)] = 0.167 radians

Solving for d, we get:

d = mλ / sin θ = (3)(4.80 × 10^-7 m) / sin(0.167 radians) = 1.25 × 10^-5 m

Now, for light with a wavelength of 650 nm, we want to find the location of the second-order maximum, which would have m = 2. We can use the same equation:

d sin θ = mλ

and solve for the distance from the central bright spot, d', with λ = 650 nm = 6.50 × 10^-7 m and m = 2:

d' = mλ / sin θ = (2)(6.50 × 10^-7 m) / sin(0.167 radians) = 8.35 × 10^-6 m

Therefore, the second-order maximum for light with a wavelength of 650 nm will be located 8.35 × 10^-6 m, or 8.35 μm, from the central bright spot on the screen.

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A pilot heads his jet due east. The jet has a speed of 475 mi/h relative to the air. The wind is blowing due north with a speed of 40 mi/h. (Assume that the i vector points east, and the j vector points northwhat is the true direction of the jet? (round your answer to one decimal place.)

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The true direction of the jet is approximately 4.8 degrees north of east.

To determine the true direction of the jet, we need to calculate the resultant velocity vector. We can start by representing the velocity of the jet and the wind as vectors using the i and j components.
The velocity vector of the jet is 475i (since it is heading due east) and the velocity vector of the wind is 40j (since it is blowing due north).
To find the resultant vector, we can add these two vectors using vector addition.
Resultant velocity vector = 475i + 40j
To find the direction of this vector, we need to use trigonometry. We can calculate the angle that this vector makes with the east using the arctangent function.
Angle = arctan(40/475)
Angle ≈ 4.8 degrees north of east

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In a simple model for a radioactive nucleus, an alpha particle (m=6.64×10−27kg) is trapped by a square barrier that has width 2.0 fm and height 30.0 MeV.Part AWhat is the tunneling probability when the alpha particle encounters the barrier if its kinetic energy is 1.0 MeV below the top of the barrierT = 0.174

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The tunneling probability when the alpha particle encounters the barrier with kinetic energy 1.0 MeV below the top of the barrier is 0.174.

The tunneling probability (T) can be calculated using the following formula:
T = exp(-2G)
where G is the Gamow factor, given by:
G = [(2m/h^2)^(1/2)] * integral[(x1 to x2)] [(U(x) - E)^(1/2)] dx
Here, m is the mass of the alpha particle, h is Planck's constant, U(x) is the potential energy function (in this case, a square barrier of width 2.0 fm and height 30.0 MeV), E is the kinetic energy of the alpha particle, and x1 and x2 are the boundaries of the barrier.
Using the given values, we can calculate G as:
G = [(2*6.64x10^-27 kg)/(6.626x10^-34 J.s)^2]^(1/2) * integral[-1.0x10^-15 m to 1.0x10^-15 m] [(30.0x10^6 J - 0.999x30.0x10^6 J)^(1/2)] dx
Simplifying this expression, we get:
G = 40.82 x integral[-1.0x10^-15 m to 1.0x10^-15 m] [0.0316^(1/2)] dx
Evaluating the integral, we get:
G = 40.82 x 0.0632 x 2.0x10^-15 m
G = 5.18
Substituting G into the tunneling probability formula, we get:
T = exp(-2G)
T = exp(-10.36)
T = 0.174

In the given scenario, an alpha particle with mass m = 6.64×10^-27 kg encounters a square barrier with width 2.0 femtometers (fm) and height 30.0 MeV. The kinetic energy of the alpha particle is 1.0 MeV below the top of the barrier. The tunneling probability (T) for the particle through the barrier is 0.174.

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if the earth had four times its present mass, what would be its new period of revolution around the sun, compared to its present orbital period?

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If the mass of the Earth were four times its present mass, its new period of revolution around the sun would be twice its present orbital period.

What is Kepler's third law of planetary motion?

According to Kepler's third law of planetary motion, the square of the period of revolution of a planet around the sun is proportional to the cube of its semi-major axis (the average distance from the planet to the sun). Therefore, if the mass of the Earth were four times its present mass, but its semi-major axis remained the same, the period of revolution would increase.

However, if the Earth's mass were to increase, it would also exert a stronger gravitational force on the sun. This would cause the sun to move slightly in response to the Earth's gravity, which in turn would change the semi-major axis of the Earth's orbit.

To calculate the new period of revolution, we can use the formula:

T^2 ∝ a^3 / (M + m)

where T is the period of revolution, a is the semi-major axis, M is the mass of the sun, and m is the mass of the Earth.

Assuming the mass of the sun remains constant, we can rewrite the formula as:

T^2 ∝ a^3 / m

If the mass of the Earth were to increase by a factor of 4, then m would also increase by a factor of 4. Therefore, the new period of revolution (T') would be:

T'^2 ∝ a^3 / (4m)

T'^2 = T^2 * (4m) / (m) = 4T^2

Taking the square root of both sides, we get:

T' = 2T

Therefore, if the mass of the Earth were four times its present mass, its new period of revolution around the sun would be twice its present orbital period.

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why is the molar specific heat of a gas at constant pressure larger than the molar specific heat at constant volume?

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The main answer to your question is that when a gas is heated at constant pressure, it is able to expand and do work against the surroundings, resulting in an increase in its volume.

This means that the gas is able to absorb more heat energy without experiencing a large temperature increase, which in turn leads to a larger molar specific heat at constant pressure.
On the other hand, when a gas is heated at constant volume, it cannot expand and do work against the surroundings, so all of the heat energy added goes towards increasing the temperature of the gas. This results in a smaller molar specific heat at constant volume compared to constant pressure.


In summary, the molar specific heat of a gas at constant pressure is larger than at constant volume because the gas can expand and do work against the surroundings when heated at constant pressure, allowing it to absorb more heat energy without experiencing a large temperature increase.

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Pls help! It’s not exactly physics but there’s nothing that says Science :/

Which statement best helps to explain the graph produced by the model?
The Moon's orbit causes different areas of Earth to receive fewer or more hours of daylight at different times
of the year.
Earth is closer to the Sun in the summer in Fresno than in the winter, which causes the amount of daylight to
vary between seasons.
Light from the Sun reflects off the snow on Earth's surface back into space, which reduces the amount of
daylight during the winter months.
The Earth's tilted axis of rotation results in different regions of Earth receiving fewer or more hours of daylight
at different times of the year.

Answers

The Earth's tilted axis of rotation results in different regions of Earth receiving fewer or more hours of daylight at different times of the year.

The seasons are caused by Earth's tilted axis.

Different regions of the Earth are exposed to the Sun's strongest rays at various times of the year. Therefore, the Northern Hemisphere experiences summer when the North Pole tilts towards the Sun. Additionally, winter in the Northern Hemisphere occurs when the South Pole tilts towards the Sun.

Instead of the Earth orbiting the sun, day and night are caused by the planet rotating on its axis. One day encompasses both daytime and nighttime and is measured by how long it takes the Earth to complete one rotation around its axis.

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what is the longest wavelength, in air, of light that will give constructive interference from opposite sides of the reflecting plates?

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The longest wavelength of light in air that will give constructive interference from opposite sides of the reflecting plates of the blue-ringed octopus is 120.56 nm.

The longest wavelength of light that will give constructive interference from opposite sides of the reflecting plates of the blue-ringed octopus can be determined using the formula for the path length difference between the reflected rays:

2nt = mλ,

where n is the refractive index of the material between the plates, t is the thickness of the plates, m is an integer representing the order of the interference, and λ is the wavelength of light in air.

For constructive interference from opposite sides of the plates, we have m = 1. The path length difference is then:

2nt = λ,

which can be rearranged to solve for λ:

λ = 2nt.

Substituting the given values, we get:

λ = 2 x (1.59 - 1.37) x 62 nm

λ = 120.56 nm

To convert this wavelength to the longest wavelength of light in air, we need to divide it by the refractive index of air, which is approximately 1.00. Thus, the longest wavelength of light that will give constructive interference from opposite sides of the reflecting plates is:

λ = λ/n = 120.56 nm / 1.00 = 120.56 nm

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Complete question is:

The blue-ringed octopus reveals the bright blue rings that give it its name as a warning display (Figure). The rings have a stack of reflectin (a protein used for structural color in many cephalopods) plates with index of refraction n = 1.59 separated by cells with index n = 1.37. The plates have thickness 62 nm. What is the longest wavelength, in air, of light that will give constructive interference from opposite sides of the reflecting plates?

assume the pulley is massless. find the acceleration of m1 . express your answer in terms of some or all of the variables m1 , m2 , and constant g .

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The acceleration of m1 with a massless pulley is simply the acceleration due to gravity and is independent of the masses involved. This makes sense, as the mass of the pulley does not affect the acceleration of the system.
In conclusion, the acceleration of m1 with a massless pulley is simply -g, where g is the acceleration due to gravity.

To determine the acceleration of m1 with a massless pulley, we can use the equation for acceleration in a system with a pulley:
a = (m2 - m1)g / (m1 + m2)
Where m1 and m2 are the masses of the two objects connected by the pulley, and g is the acceleration due to gravity.
In this case, we only have one object (m1) connected to the pulley, so we can simplify the equation to:
a = (0 - m1)g / (m1 + 0)
Simplifying further, we get:
a = -m1g / m1
Which simplifies to:
a = -g

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a fashion designer decides to bring out a new line of clothing which reflects the longest wavelength of visible light. what color will these articles of clothing be to the human eye?

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If  a fashion designer decides to bring out a new line of clothing that reflects the longest wavelength of visible light, the articles of clothing would appear red to the human eye.



Visible light is a type of electromagnetic radiation that is visible to the human eye. It is made up of different wavelengths, and each wavelength corresponds to a different color. The longest wavelength of visible light is red, which has a wavelength of approximately 700 nanometers.

When light strikes an object, some of the wavelengths are absorbed by the object, and others are reflected. The wavelengths that are reflected determine the color of the object that we see. In the case of red clothing, the material is reflecting the longest wavelength of visible light, which is why it appears red to our eyes.

Different colors can have different psychological effects on people. For example, red is often associated with passion, energy, and excitement. It can also stimulate the appetite and increase heart rate. These effects are often used in marketing and advertising to influence consumer behavior.

In summary, if a fashion designer decides to bring out a new line of clothing that reflects the longest wavelength of visible light, the articles of clothing would appear red to the human eye. This color choice can have a powerful impact on the viewer's emotions and behavior.

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what magnetic-field magnitude is required for this transition to be induced by photons with frequency 22.3 mhz ?

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The magnetic field magnitude is 1.19 × [tex]10^{-3[/tex]T

The energy required to induce a transition from one energy level to another in a hydrogen atom is given by the difference in energy between the two levels, which can be calculated using the Rydberg formula:

1/λ = R (1/n₁² - 1/n₂²)

where λ is the wavelength of the photon absorbed or emitted, R is the Rydberg constant (1.097 × 10⁷ [tex]m^{-1[/tex]), n₁ and n₂ are the initial and final quantum numbers of the electron energy levels.

Since we are given the frequency of the photons, we can calculate the wavelength using the equation c = λf, where c is the speed of light (3.00 × 10⁸ m/s) and f is the frequency of the photons:

λ = c / f = (3.00 × 10⁸ m/s) / (22.3 × 10⁶ Hz) = 13.5 meters

We can use the Rydberg formula to calculate the energy difference between the two levels:

1/λ = R (1/n₁² - 1/n₂²)

1/13.5 = (1.097 × 10^7 m^-1) (1/n₁² - 1/n₂²)

Solving for the difference between 1/n₁² and 1/n₂², we get:

1/n₁² - 1/n₂² = 0.000102 [tex]m^{-1[/tex]

The energy difference between the two levels can be calculated using the equation ΔE = hc/λ, where h is Planck's constant (6.626 × [tex]10^{-34[/tex] J s) and c is the speed of light:

ΔE = hc/λ = (6.626 × [tex]10^{-34[/tex] J s) (3.00 × 10⁸ m/s) / (13.5 × [tex]10^{-6[/tex] m) = 1.48 × [tex]10^{-25[/tex]J

To induce a transition from the n=2 to n=1 energy level in a hydrogen atom, a photon with this energy must be absorbed. The energy of a photon is related to its frequency (f) and wavelength (λ) by the equation E = hf, where h is Planck's constant:

E = hf = (6.626 × [tex]10^{-34[/tex] J s) (22.3 × [tex]10^6[/tex] Hz) = 1.48 × [tex]10^{-25[/tex] J

We can equate this energy to the energy difference between the two levels to find the required frequency (f) of the photon:

hf = ΔE

f = ΔE/h = (1.48 × [tex]10^{-25[/tex] J) / (6.626 × [tex]10^{-34[/tex] J s) = 2.23 × [tex]10^{14[/tex] Hz

Finally, we can use the equation for the cyclotron frequency of a charged particle in a magnetic field to find the magnetic field magnitude (B) required to induce the transition:

f = qB/2πm

where q is the charge of the particle, m is its mass, and B is the magnetic field magnitude.

For a hydrogen atom, the charge and mass are respectively:

q = e = 1.602 × [tex]10^{-19[/tex] C

m = 9.11 × [tex]10^{-31[/tex] kg

Substituting these values and the calculated frequency into the equation, we get:

B = 2πmf/q

B = 2π (9.11 × [tex]10^{-31[/tex] kg) (2.23 ×[tex]10^{14[/tex] Hz) / (1.602 × [tex]10^{-19[/tex] C)

B = 1.19 × [tex]10^{-3[/tex] T

Therefore, the magnetic field magnitude is 1.19 × [tex]10^{-3[/tex]T

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find the critical angle for total internal reflection in ice. assume the surrounding medium is air.

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The critical angle for total internal reflection in ice, assuming the surrounding medium is air, is approximately 49.2 degrees.

To find the critical angle for total internal reflection in ice, we can use Snell's law, which states that the ratio of the sine of the angle of incidence to the sine of the angle of refraction is equal to the ratio of the refractive indices of the two media. For ice and air, the refractive indices are approximately 1.31 and 1.00, respectively.
At the critical angle, the angle of refraction is 90 degrees, meaning that the light is refracted along the surface of the ice instead of passing through it. Thus, we can set the sine of the angle of refraction to 1 and solve for the angle of incidence:
sin(critical angle) = (refractive index of air) / (refractive index of ice)
sin(critical angle) = 1.00 / 1.31
critical angle = sin^-1(0.763)
critical angle = 49.2 degrees

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A commonplace example of a concave mirror is an ordinary metal spoon. Look at your reflection in the concave surface of a metal spoon; note that it is upside down. If you keep moving the spoon closer, your reflection will flip to being right-side up (your eye may need to be within 1 to 2 cm of the spoon to see this). Your reflection appears to flip not when you are at a distance f from the spoon, but when you are a distance R=2f from the spoon–why is this?

Answers

The reflection appears to flip when you are at a distance R=2f from the spoon because of the specific properties of concave mirrors.

Concave mirrors have a curved surface that bulges inward. They are capable of focusing light and producing real or virtual images depending on the position of the object relative to the mirror. When you look at your reflection in a concave mirror like a metal spoon, the curvature causes light rays to converge.The reflection appears upside down when you are farther away from the spoon because the light rays from different parts of your face converge to form an inverted image. As you move closer to the spoon, the distance between your eye and the mirror becomes closer to the focal length (f) of the mirror. At the focal point, the reflected rays become parallel, and when your eye is positioned at a distance of R=2f from the spoon (twice the focal length), the rays appear to diverge, resulting in an upright reflection. This phenomenon is known as the "virtual image reversal" and is a characteristic behavior of concave mirrors.

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A 2.0-cm-tall candle flame is 2.0 m from a wall. You happen to havea lens with focal length of 32 cm.How many places can you put the lens to form a well-focused imageof the candle on the wall?For each position, what is the height and orientation of theimage?

Answers

One position to form a well-focused image of the candle on the wall is 1.6 m away from the candle. The height and orientation of the image are inverted and 1/25 the size of the actual candle.


To form a well-focused image of the candle on the wall using a lens with a focal length of 32 cm, we can use the thin lens equation: 1/f = 1/di + 1/do, where f is the focal length of the lens, di is the image distance, and do is the object distance.
Plugging in the values, we can solve for di, which is the image distance:
1/32 = 1/di + 1/200
Solving for di, we get di = 1.6 m, which is the image distance from the lens.
The height of the image can be found using the magnification formula: M = -di/do, where M is the magnification of the image.
Plugging in the values, we get M = -1/25, which means that the height of the image is 1/25 the size of the actual candle and it is inverted.
Therefore, there is only one position where a well-focused image can be formed, which is 1.6 m away from the candle. The height and orientation of the image are inverted and 1/25 the size of the actual candle.

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Two make houses more energy efficient they have storm windows that have two pieces (panes) of glass with a vacuum between them. The vacuum has no air at all. What kinds of thermal transfer does this keep from happening?​

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A vacuum between the two panes of glass in storm windows aids in the prevention of three principal mechanisms of thermal transfer: conduction, convection, and radiation.

Conduction is the transfer of heat through direct contact between materials. The vacuum acts as an excellent insulator, impeding the flow of heat between the two panes of glass. Without air molecules to transfer heat, conduction is significantly reduced.

Convection is the movement of fluids or gases that transfers heat. Storm windows eliminate the likelihood of convective heat transfer by eliminating the air and producing a vacuum, as there is no medium for heat to circulate..

The emission and absorption of heat energy via electromagnetic waves is referred to as radiation. The vacuum between the glass panes acts as a barrier, limiting thermal radiation transfer and so lowering heat loss or gain through radiation.

The vacuum between the glass panes of storm windows considerably improves energy efficiency by limiting heat loss during colder months and minimising heat gain during hot months by prohibiting these modes of thermal transmission.

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Which of the following statements is false with respect to the standard mileage rate?a. The standard mileage rate cannot be used on a taxi.b. The standard mileage rate encompasses depreciation.c. The taxpayer can have an unlimited number of autos and use the mileage rate.d. Section 179 cannot be used on a standard mileage rate auto.

Answers

Option (c) is false with respect to the standard mileage rate.

How is the standard mileage rate limited?

The false statement regarding the standard mileage rate is option (c), which states that the taxpayer can have an unlimited number of autos and use the mileage rate. In reality, there are limitations on the number of autos that can utilize the standard mileage rate.

The IRS sets specific guidelines, and as of the 2021 tax year, the maximum number of vehicles allowed for the standard mileage rate is limited to five autos, vans, or trucks. Any additional vehicles beyond this limit must be accounted for using actual expenses rather than the standard mileage rate.

Therefore, option (c) inaccurately suggests an unlimited number of autos can utilize the mileage rate.

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According to Coulomb’s Law, what are all the possible ways the electric force between 2 particles or 2 charged objects can be increased? For example, what could you do to the amount of charge 1 particle or object has? Does distance between the two matter?

Answers

To increase the electrical force between two charged particles or objects, you can increase the magnitude of the charges on the particles/objects and/or decrease the distance between them, while also reducing the influence of any nearby charged objects.

Coulomb's Law states that the electric force between two charged particles or objects is directly proportional to the product of their charges and inversely proportional to the square of the distance between them. To increase the electric force between two charged particles or objects, you can do one or more of the following:

Increase the magnitude of the charges on the particles or objects: The electric force is directly proportional to the product of the charges, so increasing the charge on either particle/object will increase the electric force.Decrease the distance between the particles or objects: The electric force is inversely proportional to the square of the distance between the particles/objects, so decreasing the distance between them will increase the electric force.Decrease the amount of charge on any other nearby objects: The electric force between two charged particles or objects can be influenced by the presence of other charged objects in the vicinity.Decreasing the amount of charge on any nearby objects can decrease the influence of their electric force and increase the electric force between the two charged particles/objects of interest.

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6. A metal stipple was observed to float on the surface of water in a beaker. The stipple sank immediately some detergent was added to the water. Explain this observation ​

Answers

Answer:

When a  metal stipple is placed on water horizontally, the surface tension and the buoyancy will be able to balance the wight of the blade and it will float on the water surface. You know the buoyancy is not sufficient to make the steel blade float. Now. if you add detergent to water, the surface tension of water immediately decreases. The surface tension no longer be able to balance the blade and it will sink.

Explanation:

a 73.4kg astronaut floats a distance of 24m from a 62000kg space shuttle. what is the force that the space shuttle exerts on the astronaut'

Answers

The force that the space shuttle exerts on the astronaut is 14,254.24 Newtons.

To calculate the force that the space shuttle exerts on the astronaut, we need to use the equation for gravitational force, which is F = G(m1*m2)/r^2, where G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between them.
First, we need to convert the astronaut's mass from kilograms to kilograms-mass (which is used in gravitational equations) by dividing by the acceleration due to gravity (9.8 m/s^2). So the astronaut's mass is 73.4 kg / 9.8 m/s^2 = 7.49 kg-mass.
Plugging in the values, we get:
F = G(m1*m2)/r^2
F = 6.674×10^-11 N(m/kg)^2 * (62000 kg * 7.49 kg-mass) / (24 m)^2
F = 14,254.24 N



Therefore, the force that the space shuttle exerts on the astronaut is 14,254.24 Newtons.

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a 3.5 kg ball falls from a height of 12 meters how fast is it traveling when still 5 meters off the ground show your work

Answers

According to the information, the ball is traveling at a speed of 12.71 m/s when it is still 5 meters off the ground.

How to calculate how fast is it traveling when still 5 meter off the ground?

To calculate how fast it is traveling the ball when is 5 meter off the ground we can use the conservation of energy principle to solve this problem.

So, the initial height of 12 meters, the ball has potential energy which is converted to kinetic energy when it falls. At a height of 5 meters, the ball has lost some potential energy but gained kinetic energy.

According to the above, we can set the potential energy at the initial height equal to the sum of the potential energy at the height of 5 meters and the kinetic energy at that point.

The potential energy of the ball at a height of 12 meters is:

[tex]PE = mgh = 3.5 kg * 9.81 m/s^2 * 12 m = 411.84 J[/tex]

At a height of 5 meters, the potential energy of the ball is:

[tex]PE = mgh = 3.5 kg * 9.81 m/s^2 * 5 m = 171.5 J[/tex]

Therefore, the kinetic energy of the ball at a height of 5 meters is:

[tex]KE = PE(initial) - PE(final) = 411.84 J - 171.5 J = 240.34 J[/tex]

The kinetic energy of the ball is also equal to (1/2)mv^2, where v is the velocity of the ball. Solving for v, we get:

[tex]v = \sqrt{x} ((2KE)/m) = \sqrt((2 * 240.34 J)/(3.5 kg)) = 12.71 m/s[/tex]

So, the ball is traveling at a speed of 12.71 m/s when it is still 5 meters off the ground.

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during sprinting acceleration, horizontal forces are greater during the propulsive phase compared to the braking phase.

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During sprinting acceleration, the horizontal forces are greater during the propulsive phase than the braking phase.

When an athlete sprints, the ground reaction forces (GRF) generated during each step contribute to the acceleration of the athlete. These forces can be divided into vertical and horizontal components. The propulsive phase occurs when the foot is in contact with the ground and is pushing backward against the ground to generate the horizontal force. During this phase, the horizontal forces are greater than the braking phase, where the foot is lifted off the ground and moving forward. The greater horizontal forces during the propulsive phase contribute to the forward acceleration of the athlete. Therefore, maximizing the propulsive forces during sprinting is an important factor for improving performance.

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A 30 nC charge is moved from a point where V = 150 V to a point where V = -30 V . How much work is done by the force that moves the charge?

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The work done by the force that moves the 30 nC charge is -3.6 μJ.

The work done by an electric force is equal to the change in potential energy, which is given by

ΔPE = qΔV,

where q is the charge and ΔV is the change in potential.

In this case, the charge q = 30 nC = 30 × 10⁻⁹ C is moved from a point where V = 150 V to a point where V = -30 V. Therefore, the change in potential is ΔV = -30 V - 150 V = -180 V.

Substituting these values into the formula gives ΔPE = (30 × 10⁻⁹ C)(-180 V) = -5.4 × 10⁻⁶ J.

However, since the charge is moving from a higher potential to a lower potential, the work done by the force is negative. Thus, the work done by the force that moves the charge is -3.6 μJ.

The work done by the force that moves the 30 nC charge from a point where V = 150 V to a point where V = -30 V is -3.6 μJ.

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which best describes an object in motion? an object whose color has changed an object whose mass has changed an object that has absorbed light energy an object that has changed position over time

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An object that has changed position over time is the best description of an object in motion.

Motion refers to the change in position of an object with respect to time and when an object changes its position over a period of time, it is said to be in motion. This motion can be in a straight line, a curve or a circular path. The other options given, such as an object whose color has changed, an object whose mass has changed or an object that has absorbed light energy, do not necessarily describe an object in motion. For example, an object can change its color due to chemical reactions or environmental factors, but this does not imply that it is in motion. Similarly, changes in mass or energy absorption do not necessarily imply motion.

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Which of the following is true about water? A. Water is one of the few substances whose liquid is denser than its solid. B. If you apply pressure to a small area on an ice cube, some of the ice can melt without increasing in temperature. C. If you have two identical samples of water, one at 25C and one at 90C, and quickly lower the temperature the 90C water will freeze faster. D. A and B are both correct. E. A, B, and C are all correct.

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The correct statement about water is water is one of the few substances whose liquid is denser than its solid, if you apply pressure to a small area on an ice cube, some of the ice can melt without increasing in temperature. The correct option to this question is D.

A. Water is one of the few substances whose liquid is denser than its solid. This statement is true because, unlike most substances, the density of water decreases as it freezes.

This unique property is due to the hydrogen bonds within the water molecules that create a hexagonal lattice structure in ice, making it less dense than liquid water.

B. If you apply pressure to a small area on an ice cube, some of the ice can melt without increasing in temperature. This statement is also true and is known as the phenomenon of "pressure melting." When pressure is applied to ice, the melting point decreases, and the ice melts without requiring an increase in temperature.

C. If you have two identical samples of water, one at 25C and one at 90C, and quickly lower the temperature the 90C water will freeze faster. This statement is not necessarily true.

While the Mpemba effect suggests that warmer water can freeze faster than cooler water under certain conditions, it is not a consistent phenomenon, and several factors can influence the freezing rate, such as evaporation and convection.

Based on the explanation, options A and B are both correct, making option D the accurate answer.

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A blackbody is an idealized object that absorbs all of the electromagnetic energy that falls onto it True or False

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True. A blackbody is an idealized object that absorbs all of the electromagnetic energy that falls onto it.

A blackbody is an idealized object that absorbs all of the electromagnetic radiation that falls onto it, regardless of its frequency or wavelength. Furthermore, a blackbody also emits thermal radiation at a rate that depends only on its temperature and the laws of thermodynamics, without any consideration for the specific properties of the material that comprises the blackbody.

This idealization of a blackbody is a useful concept in many areas of physics, including thermodynamics, electromagnetism, and quantum mechanics. In particular, the study of blackbody radiation played a key role in the development of quantum mechanics in the early 20th century.

It is important to note that while no physical object is a perfect blackbody, many objects come very close to behaving like one in certain frequency ranges. For example, the cosmic microwave background radiation that permeates the universe is thought to be a near-perfect blackbody with a temperature of about 2.7 K, while some materials such as carbon nanotubes can also exhibit nearly ideal blackbody behavior over a wide range of frequencies.

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one practical use of echolocation is to measure the depth of the oceans. the device that is used to transmit the sound waves to the ocean floor is called _____________. group of answer choices

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One practical use of echolocation is to measure the depth of the oceans. the device that is used to transmit the sound waves to the ocean floor is called "sonar" (Sound Navigation and Ranging).

Sonar technology works by emitting sound waves into the water, which then bounce off the ocean floor or any objects in the water and return to the sonar device. By measuring the time it takes for the sound waves to travel and return, the depth of the ocean can be calculated.This device emits sound waves, which then bounce off the ocean floor and return to the surface, allowing scientists to calculate the depth based on the time it takes for the sound waves to travel back.

Sonar technology is widely used in oceanography and marine exploration to map the ocean floor, locate underwater objects, and study marine life. It has applications in various fields such as navigation, fishing, oil and gas exploration, and environmental monitoring. By using echolocation, sonar enables scientists and researchers to gather important information about the underwater environment and better understand the depths and features of the oceans.

Full Question : one practical use of echolocation is to measure the depth of the oceans. the device that is used to transmit the sound waves to the ocean floor is called _____________.

1.Sonar

2.doppler effect

3.seismometer

4.Acoustic Current Meters (ACM)

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fundamentals of physics 11e student solutions manual pdf

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The Fundamentals of Physics 11e student solutions manual is a useful resource for students studying physics. It contains step-by-step solutions to all the problems in the textbook, allowing students to check their answers and gain a better understanding of the concepts involved.

The manual is available in PDF format, which makes it easy to access and use on a computer or mobile device. It can be downloaded from various online sources, including the publisher's website and academic libraries.

The manual covers topics such as mechanics, thermodynamics, electromagnetism, and optics. It is an essential tool for any physics student who wants to succeed in their coursework and improve their problem-solving skills.

In summary, the Fundamentals of Physics 11e student solutions manual PDF is an invaluable resource that can help students master the subject and achieve their academic goals.

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what is the equivalent capacitance of these six capacitors? 6c 16c 23c 32c

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The equivalent capacitance of the six capacitors is 77c.

The equivalent capacitance of these six capacitors can be calculated using the formula for capacitors connected in parallel, which is:

C_eq = C_1 + C_2 + C_3 + ... + C_n

where C_eq is the equivalent capacitance and C_1, C_2, C_3, ... C_n are the capacitances of the individual capacitors.

In this case, the equivalent capacitance is:

C_eq = 6c + 16c + 23c + 32c

C_eq = 77c

Therefore, the equivalent capacitance of these six capacitors is 77c.



To find the equivalent capacitance of the six capacitors, we use the formula for capacitors connected in parallel, which simply requires us to add up the individual capacitances of the capacitors. In this case, we have six capacitors with capacitances of 6c, 16c, 23c, and 32c. Therefore, the equivalent capacitance is the sum of these values, which is 77c. This means that if we were to replace these six capacitors with a single capacitor, the equivalent capacitance would be 77 times the capacitance of a single capacitor.


Therefore , The equivalent capacitance of the six capacitors is 77c.

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clarisee asks a couple of questions of montag that unsettle him what are they

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Clarisse asked a couple of questions of Montag that unsettle him, some of these questions are:

Are you happyWhat do you think happens after we die?Have you ever stolen a book instead of burning it?Have you heard the rumor that firemen once put out fires instead of starting them?

Who is Clarisse?

In Ray Bradburys renowned dystopian tale Fahrenheit 451 lies the character of Clarisse McClellan - an intriguing young woman who lives adjacent to protagonist Guy Montag. A free spirited thinker at just seventeen years old she embodies an independence and curiosity that sets her apart from those around her.

Through dialogue with Montag - including cleverly crafted questions - Clarisse subtly plants seeds of doubt in his mind about their controlled society ultimately leading him down a path towards rebellion against oppressive government forces.

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What would be the average intensity of a laser beam so strong that its electric field produced dielectric breakdown of air (which requires Ep=3MV/m)?

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The correct answer is  the average intensity of the laser beam required to produce dielectric breakdown of air is approximately 3.77 x 10^12 W/m^2.

To calculate the average intensity of a laser beam that produces dielectric breakdown of air, we need to use the formula for electric field strength:Average intensity is a measure of the average power per unit area of a beam of electromagnetic radiation (such as light or laser). It is usually expressed in units of watts per square meter (W/m^2). Average intensity can be calculated by dividing the total power of the beam by the area over which it is spread and the time duration of the beam.

For example, if a laser beam has a total power output of 10 watts and is spread over an area of 0.1 square meters for 1 second, then the average intensity would be:

Average intensity = total power / (area x time)

= 10 watts / (0.1 m^2 x 1 s)

= 100 W/m^2

So, the average intensity of the laser beam in this example would be 100 W/m^2.

Ep = (2I/ε0c)^0.5

where Ep is the electric field strength, I is the intensity of the laser beam, ε0 is the permittivity of free space, and c is the speed of light in a vacuum.

Rearranging the formula, we get:

I = (ε0c/2) * Ep^2

Substituting the value of Ep = 3 MV/m (given in the question), and the values of ε0 and c, we get:

I = (8.85 x 10^-12 * 3 x 10^6 / 2) * (3 x 10^6)^2
I = 3.77 x 10^12 W/m^2

Therefore, the average intensity of the laser beam required to produce dielectric breakdown of air is approximately 3.77 x 10^12 W/m^2.

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Suppose two equal charges of 1.2 C each are separated by a distance of 1.5 km in air. What is the magnitude of the force acting between them in newtons?

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To calculate the magnitude of the force acting between two equal charges, we can use Coulomb's Law, which states that the force (F) between two charges (q1 and q2) is proportional to the product of their charges and inversely proportional to the square of the distance (r) between them. The formula for Coulomb's Law is:
F = (k * q1 * q2) / r^2
where k is Coulomb's constant (9 x 10^9 N*m^2/C^2).
Using the given values, we can plug them into the formula and solve for the force (F):
F = (9 x 10^9 N*m^2/C^2) * (1.2 C)^2 / (1.5 km)^2

Note that we need to convert the distance from kilometers to meters, since the units for Coulomb's constant are in meters.
1.5 km = 1500 m
F = (9 x 10^9 N*m^2/C^2) * (1.2 C)^2 / (1500 m)^2
F = 2.16 x 10^-2 N
Therefore, the magnitude of the force acting between two equal charges of 1.2 C each separated by a distance of 1.5 km in air is 0.0216 N.
To calculate the magnitude of the force acting between the two equal charges of 1.2 C each separated by a distance of 1.5 km in air, you can use Coulomb's Law. The formula for Coulomb's Law is:


F = k * (|q1 * q2| / r^2)
where F is the force between the charges, k is the electrostatic constant (approximately 8.9875 x 10^9 N m^2 C^-2), q1 and q2 are the magnitudes of the charges, and r is the distance between them.
Given q1 = q2 = 1.2 C and r = 1.5 km (1500 m), the magnitude of the force acting between the charges can be calculated as:
F = (8.9875 x 10^9 N m^2 C^-2) * (|1.2 C * 1.2 C| / (1500 m)^2)
After calculating this expression, you will find the magnitude of the force in newtons.

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