A meter stick swinging about its one end oscillates with time period T0. If bottom half of the stick is cut off, then its new oscillation period will be

Therefore, the charge is 1.20 x [tex]10^{-9[/tex] Coulombs.

The physical field that envelopes electrically charged particles and pulls or attracts all other charged particles in the vicinity is known as an electric field. Additionally, it describes the physical environment of a system of charged particles.  

An electric field, which is measured in Volts per metre (V/m), is an invisible force field produced by the attraction and repulsion of electrical charges (the source of electric flow). As you move away from the field source, the electric field's strength weakens.

The electric field due to a point charge at a distance r is given by:

E = k*q/[tex]r^{2}[/tex]

where k is the Coulomb constant (k = 8.99 x [tex]10^{-9[/tex] Nm/C) and q is the charge.

Rearranging the equation, we have:

q = E*[tex]r^{2}[/tex] 2/k

Substituting the given values, we get:

q = (3 V/m) * (0.6 m) / (8.99 x [tex]10^{-9[/tex] Nm/C)

q = 1.20 x [tex]10^{-9[/tex] C

Therefore, the charge is 1.20 x [tex]10^{-9[/tex] Coulombs.

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The spacing of the resulting lines on the screen will depend on the spacing of the diffraction grating and the wavelength of the light.

When light passes through a diffraction grating, it diffracts or bends as it interacts with the closely spaced slits in the grating.

The diffracted light waves interfere with each other, creating a pattern of bright and dark lines on a screen placed behind the grating. The spacing between the lines on the screen is determined by the distance between the slits in the grating and the wavelength of the light.
In the case of blue light with a wavelength of 434 nm, the spacing of the lines on the screen will be smaller than if a longer wavelength of light was used.

This is because shorter wavelengths of light diffract more than longer wavelengths, resulting in a wider spread of the light on the screen. Therefore, the lines on the screen will be closer together.
The spacing of the resulting lines on the screen will depend on the spacing of the diffraction grating and the wavelength of the light. Shorter wavelengths of light will produce lines that are closer together than longer wavelengths of light.

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Tapered roller bearings can withstand radial and thrust loads while requiring adjustment for proper clearance.

Tapered roller bearings are a type of automotive bearing designed to handle both radial and thrust loads, making them suitable for various applications such as wheels, transmissions, and differentials.

They consist of tapered rollers arranged between an inner and outer race, which allows them to effectively distribute the load across a larger contact area.

However, these bearings require proper clearance adjustment to ensure optimal performance and prevent premature wear.

By adjusting the clearance, you can control the bearing's operating conditions, reduce friction, and maintain the correct level of preload.

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The spectators will hear a frequency of approximately 6867.48 Hz.

The frequency heard by the spectators will be different from the frequency emitted by the airplane due to the Doppler effect. The Doppler effect is the change in frequency of a wave in relation to an observer who is moving relative to the source of the wave.

To find the frequency heard by the spectators, we can use the following formula:

[tex]$f' = f \left(\frac{v + v_0}{v + v_\text{s}}\right)$[/tex]

where:

f is the frequency emitted by the airplane (in Hz)

f' is the frequency heard by the spectators (in Hz)

v is the speed of sound (in m/s)

v₀ is the velocity of the airplane (in m/s)

vₛ is the velocity of the spectators (in m/s) - we assume this is zero since the spectators are stationary

First, we need to convert the velocity of the airplane from km/hr to m/s:

1200 km/hr = 1200000 m/hr

1200000 m/hr / 3600 s/hr = 333.33 m/s

Now we can plug in the values into the formula:

[tex]$f' = 3500 \text{ Hz} \left(\frac{342 \text{ m/s} + 333.33 \text{ m/s}}{342 \text{ m/s} + 0 \text{ m/s}}\right)$[/tex]

f' = 3500 Hz (675.33 / 342)

f' = 6867.48 Hz

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A refrigeration system is operating with a vapor charged thermostatic expansion valve. The thermal bulb is sensing a suction line temperature that is higher than the temperature that allows liquid to be present in the bulb. Any additional increases in the evaporator load will not result in an increase in refrigerant flow rate.

The thermostatic expansion valve (TXV) is a common type of refrigerant metering device used in refrigeration and air conditioning systems. The valve is designed to maintain a constant superheat at the evaporator outlet by regulating the flow of refrigerant to the evaporator. The thermal bulb of the TXV senses the temperature of the suction line and adjusts the valve opening accordingly. if the suction line temperature is higher than the temperature that allows liquid to be present in the bulb, the TXV will be fully open, and any additional increases in the evaporator load will not result in an increase in refrigerant flow rate.

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The distance from home to college is 283.4 km, and the college is 99.4 km away from home.

To calculate the distance from home to college, we first need to find out the distance covered while driving at 107 km/h.

This can be found by multiplying the speed by time, which gives us 107 km/h x 3.75 hours = 401.25 km.

Next, we need to find out the distance covered while driving at 56.3 km/h, which is 183 km - 401.25 km = -218.25 km.

The negative distance indicates that we went back towards home while driving slowly.

Finally, we need to add the distance covered at 56.3 km/h to the original distance from home to get the total distance.

Thus, the distance from home to college is 283.4 km, and the college is 99.4 km away from home.

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The pressure exerted by the reflected wave is [tex]1.25 * 10^-^9 Pa[/tex].

To calculate the pressure exerted by the reflected wave, we can use the formula P = (2I)/c, where P is pressure, I is the intensity of the wave, and c is the speed of light.

The intensity can be found using the equation I = (1/2)ε_0c[tex]E^2[/tex], where ε_0 is the electric constant, c is the speed of light, and E is the electric field amplitude.

Since the wave is linearly polarized, we know that the electric field amplitude is equal to the magnetic field amplitude, so E = Bc.

Plugging in the values given in the question, we find that I = [tex]6.25 * 10^-^1^5 W/m^2[/tex], and therefore P = [tex]1.25 * 10^-^9[/tex] Pa.

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The color of the fringes is in the red part of the visible spectrum since the wavelength of red light is around 700 nm.

The angle between adjacent fringes in Young's double slit experiment is given by:

θ = λ/d

where λ is the wavelength of light and d is the distance between the two slits. Solving for λ, we get:

λ = dθ

Plugging in the given values, we get:

λ = (0.20 mm)(3.4 × [tex]10^{-3}[/tex]rad) = 6.8 × [tex]10^{-7}[/tex]m = 680 nm.

The color of the fringes is in the red part of the visible spectrum since the wavelength of red light is around 700 nm.

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forklift operator should maintain a distance of at least three vehicle lengths from other powered industrial trucks. This is to ensure that there is enough space for each forklift to operate safely without the risk of collision or other accidents.

this distance requirement is that forklifts are heavy and powerful machines that can cause significant damage and injury in the event of a collision. By maintaining a safe distance from other forklifts, operators can reduce the risk of accidents and protect themselves and others from harm.

it is important for forklift operators to follow distance guidelines to maintain a safe workplace environment. By keeping a distance of at least three vehicle lengths from other powered industrial trucks, operators can ensure that they are able to perform their work safely and effectively.

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The ladybug is traveling at approximately 17,707.2 inches per minute.

Step 1: Find the circumference of the spinning disk.
The diameter of the disk is 88 inches. Use the formula for circumference: C = πd.
C = π × 88 inches ≈ 276.46 inches

Step 2: Calculate the total distance the ladybug travels in one revolution.
The ladybug is on the outer edge of the disk, so it travels the entire circumference in one revolution.
Distance per revolution = 276.46 inches

Step 3: Determine the total distance the ladybug travels in one minute.
The disk is spinning at 4040 revolutions per minute i.e., the frequency is to be multiplied by the distance per revolution by the number of revolutions per minute.
Total distance per minute [tex]= (276.46 inches/revolution)(4040 revolutions/minute)= 17,707.2 inches/minute[/tex]

So, the ladybug is traveling at approximately 17,707.2 inches per minute.

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When the charged particle's velocity doubles, the radius of the circular path becomes 2R.

The relationship between a charged particle's motion in a uniform magnetic field and the radius of its circular path can be described by the equation:

R = mv / (qB)

where R is the radius, m is the mass of the particle, v is its velocity, q is the charge of the particle, and B is the magnetic field strength.

Now, if the particle's velocity doubles (2v), the new radius (R') can be found using the same equation:

R' = m(2v) / (qB)

R' = 2mv / (qB)

Since mv / (qB) equals the initial radius R, we can substitute R back into the equation:

R' = 2R

So, when the charged particle's velocity doubles, the radius of the circular path becomes 2R.

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Answer:

The elastic potential energy stored in the elastic band can be calculated using the formula:

Elastic Potential Energy = 0.5 x Spring Constant x (Extension)^2

where the spring constant is 20.5 N/m and the extension is 0.9 m.

Plugging in the values, we get:

Elastic Potential Energy = 0.5 x 20.5 N/m x (0.9 m)^2 = 8.29 J

Therefore, the elastic potential energy stored in the elastic band is 8.29 Joules.

A. Indirect sound reflections refer to the sound waves that bounce off surfaces in a room before reaching the listener.

The major concern involved in architectural acoustics is how indirect sound reflections change sound quality.

These reflections can affect the sound quality by altering the characteristics of the sound, such as its clarity, intelligibility, and reverberation.

Architectural acoustics aims to optimize the design and arrangement of spaces to control and manage these indirect sound reflections.

This involves techniques such as the strategic placement of sound-absorbing materials, the use of diffusers to scatter sound waves, and the control of room dimensions and shapes to minimize undesirable echoes and reverberation.

While direct sound reflections can also influence the sound quality, they are often less of a concern in architectural acoustics compared to indirect reflections.

Direct sound refers to the sound that reaches the listener without any significant interaction with the room's surfaces. However, the design of architectural spaces can still consider the control of direct reflections to improve sound clarity and intelligibility in specific scenarios.

Therefore, among the given options, A. indirect sound reflections changing sound quality is the primary concern in architectural acoustics.

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For an object infinitely far away, the lens should be at the focal length. For a specific distance, use the lens equation.

When focusing an object that is infinitely far away, the incoming light rays are parallel with the principal axis of the system.

In this case, the lens should be at its focal length to achieve focus.

This is because parallel rays of light converge to a single point at the focal length of the lens.

For objects at specific distances, the lens equation can be used to determine the required distance between the lens and the film or CCD chip.

The lens equation is 1/f = 1/s + 1/s', where f is the focal length of the lens, s is the distance from the lens to the object, and s' is the distance from the lens to the image.

By rearranging the equation, the distance from the lens to the image can be calculated.

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The solenoid should carry approximately 1.17 A of current to produce a magnetic field of 4.65 mT at its center.

To find the current needed for a 30.0-cm-long solenoid with 1.25 cm in diameter to produce a field of 4.65 mT at its center and has 935 turns of wire, proceed as follows:

1. First, we need to use the formula for the magnetic field B at the center of a solenoid:

B = μ₀ * n * I,

where μ₀ is the permeability of free space (4π × 10⁻⁷ T·m/A), n is the number of turns per unit length (turns/m), and I is the current (A).

2. Convert the length of the solenoid to meters:

30.0 cm = 0.3 m.

3. Calculate the number of turns per unit length (n):

n = total turns / length = 935 turns / 0.3 m = 3116.67 turns/m.

4. Rearrange the formula for the magnetic field to solve for current:

I = B / (μ₀ * n).

5. Plug in the values for B, μ₀, and n:

I = (4.65 × 10⁻³ T) / ((4π × 10⁻⁷ T·m/A) * 3116.67 turns/m).

6. Calculate the current:

I ≈ 1.17 A.

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The vertical shear of the zonal winds (i.e., the east-west winds) is given by the rate of change of the zonal winds with respect to height. We can calculate it as follows:

Vertical shear of zonal winds = (change in zonal winds) / (change in height)

At the surface, the zonal winds are calm, so the change in zonal winds over 10 km is simply the zonal wind at 10 km. Therefore, the vertical shear of the zonal winds is:

Vertical shear of zonal winds = (40 m/s - 0 m/s) / (10,000 m) = 0.004 s^-1

Note that the units of the vertical shear of the zonal winds are s^-1, which is the same as the inverse of the units of height.

Similarly, the vertical shear of the meridional winds (i.e., the north-south winds) is given by the rate of change of the meridional winds with respect to height. We can calculate it as follows:

Vertical shear of meridional winds = (change in meridional winds) / (change in height)

At the surface, the meridional winds are also calm, so the change in meridional winds over 10 km is simply the meridional wind at 10 km. Therefore, the vertical shear of the meridional winds is:

Vertical shear of meridional winds = (0 m/s - 0 m/s) / (10,000 m) = 0 s^-1

Note that the units of the vertical shear of the meridional winds are also s^-1. In this case, the result is zero because the meridional winds are constant with height.

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The length of your spaceship is getting shorter.

This phenomenon occurs due to a concept called length contraction, which is a result of special relativity. As the speed of the spaceship approaches the speed of light, an observer inside the spaceship would perceive its length to be shorter.

This occurs because the relative motion between the spaceship and the observer affects the way distances are measured.

However, it is important to note that this effect is only noticeable at speeds close to the speed of light.

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To determine the thermal energy created, we need additional information such as friction coefficients and the object's mass.

To calculate the thermal energy generated during the ascent of a 12-m-high, 60-m-long slope, we would require more information such as the mass of the object and the friction coefficients between the object and the slope, as well as between the object and the tube.

Thermal energy is produced due to the work done against friction, which converts mechanical energy into heat.

Once we have the necessary information, we could use the formula for work done (W = F × d × cosθ) to determine the work done against friction, and that value would represent the thermal energy created.

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The rotational kinetic energy of the propeller is approximately 54674.29 J (joules).


To find the rotational kinetic energy, we'll follow these steps:
1. Convert the frequency from rpm (revolutions per minute) to Hz (revolutions per second).
2. Calculate the angular velocity (ω) in radians per second.
3. Determine the moment of inertia (I) of the propeller.
4. Calculate the rotational kinetic energy (K) using the formula K = 0.5 * I * ω^2.
Step 1: Convert frequency to Hz
Frequency = 2470 rpm / 60 = 41.167 Hz
Step 2: Calculate angular velocity
ω = 2 * π * frequency = 2 * π * 41.167 ≈ 258.63 rad/s
Step 3: Determine the moment of inertia
For a rod (propeller) of length L = 1.992 m and mass M = 19.16 kg rotating about one end, the moment of inertia is given by:
I = (1/3) * M * L^2 ≈ (1/3) * 19.16 * (1.992^2) ≈ 26.46 kg*m^2
Step 4: Calculate the rotational kinetic energy
K = 0.5 * I * ω^2 ≈ 0.5 * 26.46 * (258.63^2) ≈ 54674.29 J

So, the rotational kinetic energy of the propeller is approximately 54674.29 J.

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Infrared radiation. The electromagnetic spectrum is the range of all types of electromagnetic radiation, and infrared radiation falls just below visible red light on this spectrum.

Although we cannot see infrared radiation with our eyes, we can feel it as heat. Infrared radiation has a longer wavelength than visible light, and it is used in many applications such as thermal imaging, remote sensing, and communication.

Infrared radiation is also used in infrared heaters, which provide warmth by emitting heat directly to objects in a room rather than heating the air.

Overall, infrared radiation is an important part of the electromagnetic spectrum and has many practical uses in our daily lives.

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The estimated mass of the supermassive black hole at the center of this galaxy would be approximately 3.6 billion solar masses.

The mass of the supermassive black hole at the center of a bulge in a galaxy can be estimated using the bulge's velocity dispersion.

Assuming the M-sigma relation holds for this galaxy, we can use the following equation to estimate the mass of the supermassive black hole at the center:

M_bh = ([tex]sigma^2[/tex] * R) / G

where M_bh is the mass of the black hole, sigma is the velocity dispersion of stars in the bulge, R is the radius of the bulge, and G is the gravitational constant.

Assuming a velocity dispersion of 200 km/s and a bulge radius of 5 kpc (kiloparsecs), we get:

M_bh = (200 km/s[tex])^2[/tex] * 5 kpc * (3.086 × 10^19 m/kpc) / (6.674 × [tex]10^-11[/tex]N*(m/kg[tex])^2[/tex])

= 3.6 x [tex]10^9[/tex]solar masses

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the surface area of the big sphere is half the combined surface area of the eight little spheres.

Surface area is the measure of the total area that the surface of an object occupies in three-dimensional space.

A sphere is a three-dimensional geometrical object that is perfectly round in shape, like a ball, with every point on its surface equidistant from its center.

According to the given information:

When eight little spheres of mercury coalesce to form a single sphere, the surface area of the big sphere is smaller than the combined surface areas of the eight little spheres. This is because as the volume stays constant, the surface area decreases when the spheres merge into one larger sphere, minimizing the overall surface tension.

When eight spheres of equal radius are combined to form a single sphere of the same material, the total surface area of the resulting sphere can be found by:

A_big = 4πR^2

where R is the radius of the big sphere.

The volume of the big sphere can be found by adding up the volumes of the eight little spheres:

V_big = 8(4/3 πr^3) = 32/3 πr^3

Since the density of mercury is constant, the mass of the big sphere is equal to the sum of the masses of the eight little spheres:

m_big = 8m

where m is the mass of each little sphere.

The radius of the big sphere can be found using the formula for the volume of a sphere:

V_big = 4/3 πR^3

R = (3V_big/4π)^(1/3)

Substituting V_big = 32/3 πr^3 and solving for R, we get:

R = 2r

Therefore, the radius of the big sphere is twice the radius of the little spheres.

Substituting R = 2r in the equation for the surface area of the big sphere, we get:

A_big = 4π(2r)^2 = 16πr^2

The combined surface area of the eight little spheres can be found using the formula for the surface area of a sphere:

A_little = 8(4πr^2) = 32πr^2

The ratio of the surface area of the big sphere to the combined surface area of the eight little spheres is:

A_big/A_little = (16πr^2)/(32πr^2) = 1/2

Therefore, the surface area of the big sphere is half the combined surface area of the eight little spheres.

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The heaviest vehicle that can be lifted with the given hydraulic lift is about 5.59 × [tex]10^{6}[/tex] kg, or 5,590 metric tons.

We can use the formula for pressure in a hydraulic system:

P = F/A

F = P × A

The area of the output line can be calculated using the formula for the area of a circle:

A = π[tex]r^2[/tex]

We are given the diameter of the output line, so we can calculate the radius as:

r = d/2 = 19.5 cm/2 = 9.75 cm

Substituting the values into the formula, we get:

A = π(9.75 cm[tex])^2[/tex] = 298.3 [tex]cm^2[/tex]

The force that the hydraulic lift can generate is therefore:

F = (17.9 atm) × (1.013 × [tex]10^5[/tex]Pa/atm) × (298.3 [tex]cm^2[/tex]) = 5.48 × [tex]10^7[/tex] N

To find the heaviest vehicle that can be lifted, we need to divide the force by the weight of the vehicle:

W = F/g

where W is the weight of the vehicle, and g is the acceleration due to gravity (9.8 m/[tex]s^2[/tex]).

Converting the force to newtons, we get:

F = 5.48 × [tex]10^7[/tex] N

Dividing by the acceleration due to gravity, we get:

W = 5.48 × [tex]10^7[/tex] N/9.8 m/[tex]s^2[/tex] = 5.59 × [tex]10^6[/tex]10^6 kg

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The magnitude of the electric field is [tex]$E = 5.76 \times 10^6 \mathrm{N/C}$[/tex]

We can use the formula for the force on a charged particle in an electric field, and the formula for acceleration to solve for the electric field.

The force on a charged particle in an electric field is given by:

F = qE

where F is the force, q is the charge, and E is the electric field.

The formula for acceleration is:

a = F/m

where a is the acceleration, F is the force, and m is the mass.

Substituting F from the first equation into the second equation, we get:

a = qE/m

Solving for E, we get:

E = ma/q

Substituting the given values, we get:

[tex]$E = \frac{(1.5 \times 10^{-15} \mathrm{kg}) \times (6.33 \times 10^7 \mathrm{m/s}^2)}{1.65 \times 10^{-9} \mathrm{C}}$[/tex]

Simplifying, we get:

[tex]$E = 5.76 \times 10^6 \mathrm{N/C}$[/tex]

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The reading on voltage probe VPA will be a negative peak, followed by a positive peak, and then a return to zero.

This is because when the magnet is moved quickly into the coil, it induces a current in the coil in one direction, which generates a voltage with a negative sign. When the magnet is moved quickly out of the coil, it induces a current in the opposite direction, generating a voltage with a positive sign. The voltage then returns to zero once the magnet is stationary outside the coil. This phenomenon is known as electromagnetic induction, and is the basis for the operation of electric generators and motors.

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When the 50 watt bulb is observed from a distance that is 5 times of the distance of the 2 watt bulb, both the bulbs will appear to be equally bright.

The square of the distance from the source has an inverse relationship with the Brightness of object. The observer must alter their distance from each bulb so that the ratio of their squared distances equals the ratio of their luminosities in order for the 50-watt and 2-watt bulbs to seem equally bright.

Since 50/2 in this case equals 25, the space between the 50 watt and 2-watt bulbs should be five times higher (since 5 squared = 25).

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If Both bulbs could appear equally bright it depends on the inverse square law, which states that the intensity of light is inversely proportional to the square of the distance from the source.

The brightness or luminosity of a light bulb is directly related to its wattage, which is a measure of its power consumption. In this case, a 50-watt light bulb has a wattage that is 25 times greater than a 2-watt light bulb (50 watts / 2 watts = 25). As a result, the 50-watt light bulb will produce more light and appear brighter compared to the 2-watt light bulb.  In simpler terms, as the distance from a light source increases, the brightness of the light decreases.

For both bulbs to appear equally bright, the observer would need to be positioned at different distances from each light bulb. Specifically, the observer would have to be closer to the 2-watt light bulb and farther away from the 50-watt light bulb. By adjusting the distance between the observer and each light bulb, the perceived brightness of both bulbs can be equalized, even though their actual luminosity is significantly different.

In summary, a 50-watt light bulb is 25 times more luminous than a 2-watt light bulb due to its higher power consumption. However, both bulbs can appear equally bright if the observer is positioned at different distances from each light source, following the inverse square law.

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The instantaneous velocity of the elevator after 1.4 s if an elevator starting at rest accelerates upward at 0.69 m/s² is 0.966 m/s.

To find the instantaneous velocity of the elevator after 1.4 seconds, you can use the formula v = u + at, where v is the final velocity, u is the initial velocity, a is the acceleration, and t is the time. In this case, u = 0 m/s (starting at rest), a = 0.69 m/s² (upward acceleration), and t = 1.4 s.

The instantaneous velocity of the elevator after 1.4 seconds is calculated as follows:

Step 1: Identify the given values:

u = 0 m/s

a = 0.69 m/s²

t = 1.4 s

Step 2: Use the formula v = u + at:

v = (0 m/s) + (0.69 m/s² × 1.4 s)

Step 3: Calculate the final velocity:

v = 0 + (0.966 m/s)

v = 0.966 m/s

Therefore, the instantaneous velocity of the elevator after 1.4 seconds is 0.966 m/s.

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The power that can be generated from water going over a 10 m waterfall at a rate of 100 kg per second can be calculated using the formula P = mgh, where P is power, m is mass, g is the acceleration due to gravity (9.81 m/s^2), and h is the height of the waterfall.

Using the given values, we can calculate the power as follows:

P = (100 kg/s) x (9.81 m/s^2) x (10 m)
P = 9,810 watts or 9.81 kilowatts

Therefore, it is possible to receive up to 9.81 kilowatts of power from water going over a 10 m waterfall at a rate of 100 kg per second.

1. Calculate the gravitational potential energy (PE): PE = m * g * h
  Here, m = 100 kg (mass), g = 9.81 m/s² (gravitational acceleration), and h = 10 m (height).
  PE = 100 kg * 9.81 m/s² * 10 m = 9810 J (joules)

2. The energy is converted into kinetic energy, which can be used to calculate the power (P) generated. To calculate the power, divide the energy by time (t).
  Since the rate is 100 kg per second, the time (t) is 1 second.

3. Calculate the power (P): P = PE / t
  P = 9810 J / 1 s = 9810 W (watts)

So, the maximum power possible to receive from water going over a 10-meter waterfall at a rate of 100 kg per second is 9810 watts.

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The current through the floodlight is 2.5 amperes.

The power P consumed by an electrical device can be expressed as:

P = V x I

where V is the voltage across the device, I is the current flowing through the device, and P is the power consumed by the device.

In this problem, the power consumed by the 300-watt floodlight is given as P = 300 W and the potential drop across the floodlight is V = 120 V. To find the current I flowing through the floodlight, we can rearrange the equation as follows:

I = P / V

Substituting the given values, we get:

I = 300 W / 120 V

I = 2.5 A

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Do not point the laser beam at the fish as it could harm its eyesight.

It is not recommended for the fisherman to point the laser beam directly at the fish as it could potentially harm its eyesight.

Laser beams are known to cause damage to the retina, which is the part of the eye responsible for processing visual information.

Moreover, the fish could be disturbed or frightened by the sudden appearance of the laser beam, which could affect its behavior and swimming patterns.

If the fisherman wishes to use a laser beam for fishing purposes, he should do so in a safe and responsible manner, avoiding pointing it directly at the fish or any other living creatures.

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