Solar radiation pressure pushed gas and dust particles out of the solar nebula by the light from the sun.
The radiation pressure from the intense light of the newly formed sun pushed gas and dust particles out of the solar nebula, creating a void in the center which eventually led to the formation of the planets.
Scientists theorise that the solar system was created when a cloud of gas and dust in outer space was disturbed, possibly by the explosion of a nearby star (known as a supernova). The gas and dust cloud was compressed by the waves created by the explosion in space.
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If V=12 V, C1=470 μF, C2 =330 μF, C3 =100 μF, and C4 =10 μF, calculate the followings:1. the equivalent capacitance2. the charge stored in C23.the voltage across C34. the energy stored in C4.
1. Equivalent capacitance 910 μF
2. C2= 3,960 μC and C3 = 1,200 μC.
3. The energy stored in C4 is 0 J.
To calculate the requested values, we'll work step by step:
The equivalent capacitance (Ceq) can be found by adding the individual capacitances in parallel:
Ceq = C1 + C2 + C3 + C4
= 470 μF + 330 μF + 100 μF + 10 μF
= 910 μF
Therefore, the equivalent capacitance is 910 μF.
The charge stored in C2 and C3 can be calculated using the formula:
Q = C * V
For C2:
Q2 = C2 * V
= 330 μF * 12 V
= 3,960 μC
For C3:
Q3 = C3 * V
= 100 μF * 12 V
= 1,200 μC
Therefore, the charge stored in C2 is 3,960 μC and in C3 is 1,200 μC.
The voltage across C3 and C4 can be found by using the formula:
V = Q / C
For C3:
V3 = Q3 / C3
= 1,200 μC / 100 μF
= 12 V
For C4:
V4 = Q4 / C4
= 0 (since C4 does not have any charge stored initially) / 10 μF
= 0 V
Therefore, the voltage across C3 is 12 V, and the voltage across C4 is 0 V.
The energy stored in a capacitor can be calculated using the formula:
E = (1/2) * C * V^2
For C4:
[tex]E4 = (1/2) * C4 * V4^2[/tex]
[tex]= (1/2) * 10 \mu F * (0 V)^2[/tex]
= 0 J
Therefore, the energy stored in C4 is 0 J.
Note: It seems that there was no charge initially stored in C4, so there is no energy stored in it.
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If R is the relative density of the solid,prove that d1=R(d1-d2)
We can prove d1 = R(d1 - d2), accepting that d1 and d2 are the densities of two immiscible fluids and R is the relative thickness (i.e., thickness relative to that of the lower fluid) of a strong submerged within the lower fluid.
How to Prove d1 = R(d1 - d2)?Accepting that d1 and d2 are the densities of two immiscible fluids (with d1 being the thickness of the upper fluid and d2 being the thickness of the lower fluid) layered one over the other in a holder, and accepting that there's a strong with thickness R which is submerged within the lower fluid, we are able demonstrate that d1 = R(d1 - d2) utilizing the rule of buoyancy.
The buoyant drive acting on the strong is break even with to the weight of the uprooted fluid, which is break even with to the volume of the strong submerged within the fluid duplicated by the thickness of the fluid. Hence, able to type in:
Buoyant drive = Volume of submerged strong × Thickness of fluid
Since the strong is submerged within the lower fluid, ready to compose the volume of submerged strong as:
Volume of submerged solid = Volume of strong × (d2 / R)
where d2 / R is the proportion of the thickness of the lower fluid to the thickness of the strong.
Substituting this expression for the volume of submerged strong within the condition for the buoyant constrain, we get:
Buoyant constrain = (Volume of strong × d2 / R) × Thickness of fluid
Since the strong is in balance, the buoyant constrain must be break even with to the weight of the strong, which is given by:
Weight of strong = Volume of strong × Thickness of strong
Likening the buoyant constrain and the weight of the strong, we get:
(Volume of strong × d2 / R) × Thickness of fluid = Volume of strong × Thickness of strong
Canceling the volume of strong from both sides, we get:
d2 / R = (Thickness of strong) / (Thickness of fluid)
Improving this condition, we get:
R = (Thickness of strong) / (Thickness of fluid / d2)
Increasing both sides by d1 - d2, we get:
R(d1 - d2) = (Thickness of strong) / (Thickness of fluid / d2) × (d1 - d2)
Disentangling, we get:
R(d1 - d2) = Density of strong
Subsequently, we have demonstrated that d1 = R(d1 - d2), accepting that d1 and d2 are the densities of two immiscible fluids and R is the relative thickness (i.e., thickness relative to that of the lower fluid) of a strong submerged within the lower fluid.
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A lot is a section of land on which a house can be built. A beach town only has two oceanfront lots left to sell. Another five lots are available two blocks from the beach. Seven more lots are available two miles from the beach, and a dozen lots are available five miles from the beach. Each lot is the same size. The only differences are the distance from the beach and the number of lots available in each location.
Which lots are probably the most expensive?
the dozen lots located five miles from the beach
the seven lots located two miles from the beach
the five lots located two blocks from the beach
the two lots located along the oceanfront
Probably the most expensive lots are, (d). the two lots located along the oceanfront is the correct option.
The two lots closest to the water are probably the most expensive. This is due to the fact that oceanfront properties are normally extremely sought-after and desired, and the fact that there are currently just two coastal lots available suggests that there may be a large demand for them, which would increase their price.
Additionally, because to the desirable position and picturesque views, being right on the beachfront frequently attracts a higher price. In contrast, due to their distance from the beach and likely lesser demand, the other lots situated further away from it (two blocks, two miles, and five miles) may be less expensive.
Therefore ,the correct option is (d).
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the ____-conductor ide cable has half the number of pins as it has wires.
The answer to your question is the 40-conductor IDE cable. This cable has 40 pins and 80 wires, meaning that it has twice as many wires as pins. The extra wires are included to support features such as cable selection and faster data transfer rates.
However, the newer 80-conductor IDE cable has 80 pins and 80 wires, with each wire having a specific function. The extra pins are used for grounding and shielding purposes to reduce crosstalk and interference. In conclusion, the 40-conductor IDE cable has half the number of pins as it has wires, while the 80-conductor IDE cable has an equal number of pins and wires.
The 40-conductor IDE cable has half the number of pins as it has wires. This is because each pin in the IDE cable is connected to a corresponding wire, and the 40-conductor IDE cable consists of 80 wires.
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if you dribble a basketball with a frequency of 1.90 hz , how much time does it take for you to complete 14 dribbles?
It would take approximately 7.3682 seconds to complete 14 dribbles at a frequency of 1.90 Hz.
If you dribble a basketball with a frequency of 1.90 Hz, it means that you complete 1 full dribble cycle in 1/1.90 seconds or approximately 0.5263 seconds.
To find the time it takes to complete 14 dribbles, we need to multiply the time for one dribble cycle by 14:
Time for one dribble cycle = 0.5263 seconds
Time for 14 dribble cycles = 14 x 0.5263 seconds = 7.3682 seconds (rounded to four decimal places)
Therefore, it would take approximately 7.3682 seconds to complete 14 dribbles at a frequency of 1.90 Hz.
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a yo-yo has a rotational inertia of 950 g'cmz and a mass of 120 g. its axle radius is 3.2 ffiffi, and its string is 120 cm long. the yo-yo rolls from rest down to the end of the string. (a) what is the magnitude of its linear acceleration? (b) how long does it take to reach the end of the string? as it reaches the end of the string, what are its (c) linear speed, (d) translational kinet
To solve this problem, we can use the principle of conservation of energy, which states that the initial potential energy of the yo-yo is converted into kinetic energy as it rolls down the string.
(a) The magnitude of the linear acceleration can be found using the formula:
a = g(sinθ - μcosθ)
where g is the acceleration due to gravity, θ is the angle the string makes with the vertical, and μ is the coefficient of kinetic friction. Since the yo-yo is rolling without slipping, we can use the relationship between linear and angular acceleration:
a = Rα
where R is the radius of the yo-yo and α is its angular acceleration. Combining these equations, we get:
α = g/R(sinθ - μcosθ)
The moment of inertia of the yo-yo about its center is:
I = 1/2MR^2 + 1/4mR^2
where M is the mass of the yo-yo and m is the mass of the string. Substituting the given values, we get:
I = 0.0024 kg·m^2
The torque acting on the yo-yo due to the tension in the string is:
τ = Iα
At the bottom of the string, the tension in the string is equal to the weight of the yo-yo, so we have:
τ = (1/2)mgR
Setting these two expressions for τ equal to each other and solving for α, we get:
α = (1/2)mgR/I = 51.5 rad/s^2
Finally, we can use the relationship between linear and angular acceleration to find the magnitude of the linear acceleration:
a = Rα = 164.8 m/s^2
(b) The time it takes for the yo-yo to reach the end of the string can be found using the kinematic equation:
y = (1/2)at^2
where y is the length of the string and a is the linear acceleration. Substituting the given values, we get:
t = sqrt(2y/a) = 2.12 s
(c) At the end of the string, the linear speed of the yo-yo is equal to the product of its radius and angular velocity:
v = ωR
The final angular velocity can be found using the kinematic equation:
θ = ωi t + (1/2)αt^2
where θ is the angle through which the yo-yo rotates, ωi is its initial angular velocity (zero), and α is its angular acceleration. The angle θ is equal to the length of the string, so we have:
θ = 2π = ωf t + (1/2)αt^2
Solving for ωf, we get:
ωf = (2π - (1/2)αt^2)/t = 45.5 rad/s
Substituting this value into the equation for linear speed, we get:
v = ωfR = 145.6 cm/s
(d) The translational kinetic energy of the yo-yo at the end of the string is:
K = (1/2)mv^2 = 0.052 J
where m is the mass of the yo-yo. The rotational kinetic energy is:
K' = (1/2)Iω^2 = 0.163 J
The total kinetic energy is the sum of these two terms:
Ktotal = K + K' = 0.215 J
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Plane monochromatic waves with wavelength 520 nmnm are incident normally on a plane transmission grating having 330 slits/mmslits/mm .Find the angles of deviation in the first, second, and third orders.
The angles of deviation for the first, second, and third orders of diffraction are approximately 9.78 degrees, 19.44 degrees, and 30.29 degrees, respectively.
The angle of deviation for a diffraction grating is given by the equation:
sinθ = mλ/d
where θ is the angle of deviation, m is the order of diffraction, λ is the wavelength of light, and d is the distance between adjacent slits on the grating.
Substituting the given values, we get:
d = 1/330 mm = 0.00303 mm
λ = 520 nm = 0.00052 mm
For the first order of diffraction (m = 1):
sinθ = (1)(0.00052 mm)/(0.00303 mm) = 0.169
θ = 9.78 degrees
For the second order of diffraction (m = 2):
sinθ = (2)(0.00052 mm)/(0.00303 mm) = 0.338
θ = 19.44 degrees
For the third order of diffraction (m = 3):
sinθ = (3)(0.00052 mm)/(0.00303 mm) = 0.506
θ = 30.29 degrees
When light passes through a grating, it diffracts and produces a pattern of bright and dark fringes. The angle at which these fringes occur depends on the wavelength of light, the spacing of the grating, and the order of diffraction. The equation used to calculate the angle of deviation, sinθ = mλ/d, relates all of these factors.
In this problem, we are given the wavelength of light (520 nm) and the spacing of the grating (330 slits/mm).
We use these values to calculate the distance between adjacent slits on the grating (d = 1/330 mm = 0.00303 mm). We then use this value along with the equation sinθ = mλ/d to calculate the angles of deviation for the first, second, and third orders of diffraction.
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what happens to the power level of a lens if i double the focal length of the same lens? (f0 is the original focal length and f1 is the new focal length)
When you double the focal length of a lens from f0 to f1, the power level of the lens decreases by a factor of 2. This is because the power of a lens is inversely proportional to its focal length. Mathematically, the power of the lens can be calculated using the formula P = 1/f, where P is the power of the lens in diopters and f is the focal length of the lens in meters.
Therefore, if you double the focal length of the lens, the power of the lens becomes half of its original power.
When you double the focal length of a lens, the power level of the lens will decrease. The power (P) of a lens is given by the formula P = 1/f, where f is the focal length. If the original focal length is f0 and the new focal length is f1 (f1 = 2 * f0), then the new power level will be P1 = 1/f1. Since f1 is twice f0, the new power level will be half the original power level.
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Doubling the focal length of a lens will result in the power being halved.
The power of a lens is inversely proportional to its focal length. Mathematically, the power (P) of a lens is given by the formula:
P = 1/f
where f represents the focal length of the lens.
If we double the focal length of a lens (from f0 to f1), the power of the lens will decrease. Let's compare the power of the lens before and after doubling the focal length:
P0 = 1/f0 (original power)
P1 = 1/f1 (new power)
If we double the focal length, f1 = 2f0. Substituting this value into the formula, we have:
P1 = 1/(2f0)
Comparing P0 and P1, we can see that P1 is half of P0:
P1 = (1/2)P0
Therefore, doubling the focal length of a lens will result in the power being halved.
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a negative particle is put near a stationary negative charge. is the electric potential positive or negative?
When a negative particle is put near a stationary negative charge, the electric potential at the location of the negative particle is negative.
The electric potential is a scalar quantity that represents the amount of electric potential energy per unit charge at a given point in space. The sign of the electric potential depends on the sign of the charge creating the electric field.
In this case, the stationary negative charge creates an electric field that is directed away from it. When the negative particle is placed near the stationary negative charge, it will experience a repulsive force due to the electric field. The negative particle will therefore have to do work against the electric field to move away from the stationary charge.
Since the negative particle has to do work to move away from the stationary charge, the electric potential energy of the negative particle increases. As a result, the electric potential at the location of the negative particle is negative.
In summary, when a negative particle is put near a stationary negative charge, the electric potential at the location of the negative particle is negative.
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Light traveling in air is incident on the surface of a block of plastic at an angle of
62. 7° to the normal and is bent so that it makes a 48. 1° angle with the normal in the
plastic. Find the speed of light in the plastic.
Note: Your answer is assumed to be reduced to the highest power possible.
Light traveling in air is incident on the surface of a block of plastic at an angle of 62. 7° to the normal and is bent so that it makes a 48. 1° angle with the normal in the plastic.
Assuming the block of plastic is surrounded by air, we can use Snell's law to relate the incident angle to the refracted angle.
n1 sinθ1 = n2 sinθ2
Where n1 is the index of refraction of air (approximately 1), θ1 is the incident angle, n2 is the index of refraction of the plastic, and θ2 is the refracted angle.
Rearranging the equation, we get
n2 = n1 sinθ1 / sinθ2
By putting these values given, we get
n2 = sin(62.7°) / sin(48.1°)
n2 = 1.456
This means that the speed of light in the plastic is
v2 = c/n2
Where c is the speed of light in a vacuum (approximately 3x[tex]10^{8}[/tex] m/s).
By putting these values, we get
v2 = 3x[tex]10^{8}[/tex] m/s / 1.456
v2 = 2.06x[tex]10^{8}[/tex] m/s
Hence, the speed of light in the plastic is approximately 2.06x[tex]10^{8}[/tex] m/s.
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A certain digital camera having a lens with focal length 7.50cm focuses on an object 1.60m tall that is 4.30m from the lens. How far must the lens be from the photocells?
The lens of the digital camera must be approximately 15.74 cm away from the photocells.
To calculate this distance, we can use the lens formula, which relates the object distance (u), image distance (v), and focal length (f) of a lens. The lens formula is given by:
1/f = 1/v - 1/u
Given that the focal length (f) of the lens is 7.50 cm, the object height (h) is 1.60 m, and the object distance (u) is 4.30 m, we can use the lens formula to find the image distance (v) where the photocells are located.
Plugging in the values, we get:
1/7.50 = 1/v - 1/4.30
Solving for v, we find:
v ≈ 15.74 cm
This is the distance at which the lens of the digital camera must be positioned from the photocells in order to focus on an object that is 1.60 m tall and located 4.30 m away from the lens. It's important to note that this is a simplified calculation and other factors such as the depth of field, lens characteristics, and camera design may also affect the actual positioning of the lens in a real camera system.
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retroreflective chevrons on the back of new fire apparatus and ambulances should be oriented in which direction according to nfpa standards?
According to NFPA standards, retroreflective chevrons on the back of new fire apparatus and ambulances should be oriented in a downward-facing direction.
This means that the angle of the chevron should be pointing downwards towards the ground. This orientation helps to increase the visibility of the vehicle when viewed from a higher angle, such as from the perspective of a driver in a taller vehicle. The downward orientation helps to reduce glare and improve the contrast of the chevron, making it easier for other drivers to see and avoid the vehicle.
Additionally, the chevrons should be a contrasting color to the background of the vehicle, and should be placed on both the left and right sides of the vehicle to ensure maximum visibility from all angles.
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you place a 100 g piece of iron and a 100g piece of lead inside a well insulated container. the initial temp of the lead is 30 degrees celsius, but you do not know the initial temperature of the iron. You seal the insulated container and wait until the lead and iron reach a common final temperature of 177 degrees Celcius. What was the initial temperature of the iron?
The initial temperature of the iron was approximately 94.3 degrees Celsius.
To solve this problem, we can use the principle of conservation of energy, which states that the total energy of a closed system is constant.
We can assume that the insulated container and its contents form a closed system, and that the heat lost by the lead is gained by the iron until they reach a common final temperature.
We can use the following equation to relate the heat gained or lost by a substance to its mass, specific heat, and change in temperature:
Q = mcΔT
where
Q is the heat gained or lost,
m is the mass,
c is the specific heat, and
ΔT is the change in temperature.
Since the insulated container is well insulated, we can assume that no heat is lost to the surroundings, so the total heat gained by the iron must equal the total heat lost by the lead:
[tex]m_{iron} * c_{iron} * (T_{final} - T_{initial}) = m_{lead} * c_{lead} * (T_{initial} - T_{lead})[/tex]
where
[tex]m_{iron}[/tex] and [tex]c_{iron}[/tex] are the mass and specific heat of iron,
[tex]T_{final[/tex] is the common final temperature of the iron and lead,
[tex]T_{initial[/tex] is the initial temperature of the iron,
[tex]m_{lead[/tex] and [tex]c_{lead[/tex] are the mass and specific heat of lead, and
[tex]T_{lead[/tex] is the initial temperature of the lead.
We can substitute the given values into the equation and solve for [tex]T_{initial[/tex]:
[tex]100 g * c_{iron} * (177°C - T_{initial}) = 100 g * c_{lead} * (T_{initial} - 30C)[/tex]
Dividing both sides by 100 g and rearranging:
c_iron * (177°C - T_initial) = c_lead * (T_initial - 30°C)
c_iron * 177°C - c_iron * T_initial = c_lead * T_initial - c_lead * 30°C
(c_iron + c_lead) * T_initial = c_iron * 177°C + c_lead * 30°C
T_initial = (c_iron * 177°C + c_lead * 30°C) / (c_iron + c_lead)
Substituting the specific heat values for iron and lead (0.45 J/g°C and 0.13 J/g°C, respectively):
T_initial = (0.45 J/g°C * 177°C + 0.13 J/g°C * 30°C) / (0.45 J/g°C + 0.13 J/g°C)
T_initial = 94.3°C
Therefore, the initial temperature of the iron was approximately 94.3 degrees Celsius
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as particle shape becomes non-spherical, there is a chance that, upon drying, they will reorient in nonrandom directions. how will the x-ray diffraction pattern change for alignment of cds particles along specific directions: [100], [001], [110]?
As particles become non-spherical and align along specific directions, the X-ray diffraction pattern will show more intense peaks corresponding to the aligned planes due to the constructive interference of X-ray waves.
When particle shape becomes non-spherical, the alignment of the particles can indeed impact the X-ray diffraction pattern. Here's how the pattern would change for alignment of CdS particles along specific directions:
1. [100] alignment: When particles are aligned along the [100] direction, the diffraction pattern will show strong and well-defined peaks corresponding to planes parallel to the [100] direction. This is because the X-ray waves will constructively interfere, producing higher intensities in those directions.
2. [001] alignment: Similarly, for the [001] alignment, the diffraction pattern will display strong peaks corresponding to planes parallel to the [001] direction. The constructive interference will occur along this direction, leading to more intense peaks.
3. [110] alignment: For particles aligned along the [110] direction, the diffraction pattern will exhibit prominent peaks for planes parallel to the [110] direction. This alignment will also cause constructive interference, resulting in higher intensity peaks for the [110] direction.
In conclusion, as particles become non-spherical and align along specific directions, the X-ray diffraction pattern will show more intense peaks corresponding to the aligned planes due to the constructive interference of X-ray waves.
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a copper wire carries 1 amp of electric current. what kind of charge does the electron flow create in the wire? 1. positive 2. negative 3. no charge
The electron flow in a copper wire carrying 1 amp of electric current creates a negative charge.
Electric current is the flow of charged particles, such as electrons, through a conductor. In a copper wire, the negatively charged electrons move through the wire, creating a flow of current. Since the electrons are negatively charged, their movement through the wire creates a negative charge.
To further explain, it is important to understand that in a metal conductor like copper, the electrons are free to move throughout the material. When a voltage is applied across the wire, it creates an electric field that causes the electrons to move in a particular direction. In this case, the electrons move from the negative terminal of the voltage source, through the wire, and towards the positive terminal. This movement of electrons is what creates the electric current.
Since electrons are negatively charged, their movement through the wire creates a negative charge. This is why when you touch a metal object that is connected to a live wire, you can receive an electric shock. The excess electrons flow through your body, creating a negative charge that can cause discomfort or even injury.
In summary, the electron flow in a copper wire carrying 1 amp of electric current creates a negative charge due to the movement of negatively charged electrons through the wire.
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n which phase of the throwing motion is maximum external rotation achieved? wind-up cocking acceleration deceleration
Maximum external rotation is achieved in the acceleration phase of the throwing motion.
At which phase of the throwing motion is maximum external rotation attained: wind-up, cocking, acceleration, or deceleration?During the wind-up phase of the throwing motion, the pitcher starts with his or her hands together in front of the body and begins to lift the leg on the opposite side of the throwing arm. In the cocking phase, the pitcher moves the throwing arm back behind the body, and the hand rotates inward, so the ball faces the ground. In the acceleration phase, the pitcher starts moving the arm forward, and the ball begins to face forward. During this phase, the pitcher generates a significant amount of power to throw the ball. Finally, in the deceleration phase, the pitcher slows down the arm after the ball has been released.
The maximum external rotation is achieved during the acceleration phase, just before the forward acceleration of the arm. During this phase, the pitcher's arm rotates externally, allowing the arm to reach maximum speed just before the release of the ball.
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what quantity/quantities change when a light wave move from air to water, and how does it/do they change? (select all that apply.)
When a light wave moves from air to water, the following quantities change:
- wavelength (decreases)
- frequency (stays constant)
- speed (decreases)
- direction (bends or refracts)
When a light wave moves from air to water, the quantities that change are the speed, wavelength, and direction of the light wave. The speed of the light wave decreases in water compared to air due to the higher refractive index of water. Consequently, the wavelength of the light wave also becomes shorter in water. The change in speed causes the light wave to change direction, a phenomenon known as refraction.
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The complete question : What quantity/quantities change when a light wave move from air to water, and how does it/do they change? (Select all that apply.)
A) its speed increases
B) its frequency decreases
C) its wavelength decreases
D) its frequency increases
E) its speed decreases
F) its wavelength increases
what is the pressure if an additional 29.7 kg of nitrogen is added without changing the temperature?
If an additional 29.7 kg of nitrogen is added without changing the temperature, if the gas was already under high pressure or in a small volume, the pressure increase could be much more significant.
Assuming that the nitrogen is added to a closed system with a fixed volume, the pressure will increase proportionally to the increase in the number of gas molecules. This is described by the ideal gas law, which states that PV = nRT, where P is the pressure, V is the volume, n is the number of moles of gas, R is the gas constant, and T is the temperature in Kelvin.
Since the temperature is constant, the equation simplifies to PV = constant. Adding 29.7 kg of nitrogen is equivalent to adding approximately 1 mole of nitrogen gas (based on the molar mass of nitrogen, which is approximately 28 g/mol). Therefore, the pressure will increase by a factor of 1/1, or simply by the ratio of the initial number of moles to the final number of moles:
Pfinal = (ninitial + 1)/ninitial * Pinitial
where Pinitial is the initial pressure and ninitial is the initial number of moles of nitrogen gas.
Without knowing the initial pressure or volume, it is not possible to calculate the final pressure precisely. However, we can make some general observations based on the ideal gas law. If the initial pressure and volume were such that the gas was not already at high pressure or density (i.e. not close to its critical point), then adding 1 mole of gas should increase the pressure by less than a factor of 2. For example, if the initial pressure was 1 atm, adding 1 mole of nitrogen would increase the pressure to approximately 1.5 atm. However, if the gas was already under high pressure or in a small volume, the pressure increase could be much more significant.
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pascal's principle: a container consists of two vertical cylindrical columns of different diameter connected by a narrow horizontal section, as shown in the figure. the open faces of the two columns are closed by very light plates that can move up and down without friction. the tube diameter at a is 44 cm and at b it is 13 cm. this container is filled with oil of density 0.820 g/cm3. if a 132-kg object is placed on the larger plate at a, how much mass in kg, should be placed on the smaller plate at b to balance it?
According to Pascal's principle, pressure applied to a confined fluid is transmitted equally in all directions. In this case, the pressure applied to the larger plate at a will be transmitted to the oil in the container and will also push the smaller plate at b upwards.
To balance the object at a, an equal force must be applied to the smaller plate at b. The first step is to calculate the pressure exerted by the object on the oil in the container. The formula for pressure is P = F/A, where P is pressure, F is force, and A is area. The area of the larger plate at a is (22 cm)^2 x π = 1,518.72 cm^2. Therefore, the pressure exerted by the 132-kg object is:
P = F/A = (132 kg x 9.8 m/s^2) / 1,518.72 cm^2 = 0.865 kPa
Since the oil has a density of 0.820 g/cm^3, its mass per unit volume is 0.820 kg/L or 820 kg/m^3. The pressure transmitted by the object will cause the oil to rise to a certain height in the narrower column at b. The height difference between the oil levels in the two columns is h and can be calculated using the formula P = ρgh, where ρ is the density of the fluid, g is the acceleration due to gravity, and h is the height difference. Rearranging the formula gives:
h = P / (ρg) = 0.865 kPa / (820 kg/m^3 x 9.8 m/s^2) = 0.000111 m = 1.11 cm
Therefore, the smaller plate at b will rise by 1.11 cm. The area of the smaller plate at b is (6.5 cm)^2 x π = 132.73 cm^2. To balance the object at a, an equal force must be applied to the smaller plate at b. The formula for force is F = ma, where F is force, m is mass, and a is acceleration. The acceleration in this case is due to gravity, so a = g = 9.8 m/s^2. Rearranging the formula gives:
m = F/a = (132 kg x 9.8 m/s^2) / 132.73 cm^2 = 98.82 kg
Therefore, to balance the object at a, a mass of 98.82 kg should be placed on the smaller plate at b.
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4) imagine measuring the local gravitational acceleration at the surface of a solid aluminum sphere the size of the moon. if you used a simple pendulum of length 1 m, what would you measure the period to be?
Therefore, if we used a simple pendulum of length 1 m to measure the local gravitational acceleration at the surface of a solid aluminum sphere the size of the moon, we would measure the period to be 3.92 seconds.
The period of a simple pendulum depends on the length of the pendulum and the local gravitational acceleration. The formula for the period of a simple pendulum is:
T = 2π√(L/g)
where T is the period, L is the length of the pendulum, and g is the local gravitational acceleration.
Assuming the aluminum sphere has the same density as solid aluminum (2,700 kg/m³), its mass would be approximately 7.35 x 10²² kg, which is the mass of the moon. The radius of the sphere would be approximately 1,737 km, which is also the radius of the moon.
The local gravitational acceleration at the surface of the sphere can be calculated using the formula:
g = G(M/r²)
where G is the gravitational constant, M is the mass of the sphere, and r is the radius of the sphere.
Substituting the values, we get:
g = 6.67 x 10⁻¹¹ N(m/kg)² * 7.35 x 10²² kg / (1.737 x 10⁶ m)²
= 1.62 m/s²
Using this value of g and a length of 1 m, we can calculate the period of the simple pendulum:
T = 2π√(L/g)
= 2π√(1/1.62)
= 3.92 s
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A92 238U atom has measured mass of 238.050785 u. what is the binding energy per nucleon?
The binding energy per nucleon for a 238U atom with a measured mass of 238.050785 u is approximately 7.6 MeV.
To calculate the binding energy per nucleon, first determine the mass defect by subtracting the measured mass (238.050785 u) from the total mass of its individual nucleons (protons and neutrons).
Next, convert the mass defect to energy using Einstein's mass-energy equivalence formula, E=mc², where E is the energy, m is the mass defect, and c is the speed of light.
Finally, divide the binding energy by the total number of nucleons (A = 238) to find the binding energy per nucleon.
Summary: By calculating the mass defect, converting it to energy, and dividing by the total number of nucleons, we find that the binding energy per nucleon for a 238U atom with a measured mass of 238.050785 u is approximately 7.6 MeV.
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the plucked string produces a tone. what is the fundamental frequency, in hertz, of the tone under the given conditions?
The fundamental frequency, in hertz, of the new tone that is produced when the string is plucked is 168.84 Hz
The fundamental frequency, in hertz, of the new tone that is produced when the string is plucked is 168.84 Hz
Let assume that the oscillating length on the guitar is 0.62 m,
If the guitarist shortens the oscillating length of the properly tuned D-string by 0.15 m.
Then the new length of the oscillating string L' = (0.62 - 0.15 )m = 0.47 m
The fundamental frequency of the new tone can be computed by using the formula:
where;
mass (m) is assumed to be 1.5× 10⁻³ kg, and;
tension T = 4Lf² m
T = 4× 0.62× 147 × 1.5× 10⁻³ (assuming old fundamental frequency = 147)
T = 4× 0.62× 147 × 1.5× 10⁻³
T = 80.39 N
f = 168.84 Hz
Therefore, the fundamental frequency, in hertz, of the new tone that is produced when the string is plucked is 168.84 Hz
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Full Question
The guitarist shortens the oscillating length of the properly tuned D-string by 0.15 m by pressing on the string with a finger. What is the fundamental frequency, in hertz, of the new tone that is produced when the string is plucked?
Access Solid state Physics 1st Edition Chapter 12 solutions now. Our solutions are written by experts so you can be assured of the highest quality!
For free electrons ε(k) = ℏ^2k^2/2m. Calculate ∂A(ε, kz)/∂ε and show that the general expression (12.42) for the period in a magnetic field reduces to the free electron result (12.43).
Therefore, we have shown that the general expression (12.42) for the period in a magnetic field reduces to the free electron result (12.43) when evaluated for free electrons.
To start, we have:
A(ε,kz) = (eB/2πℏ)∫dkx exp[i(kxx + kzz + (2m/ℏ)(ε - ℏ^2k^2/2m)t)]∂A(ε,kz)/∂ε = (eB/2πℏ)∫dkx expi(kxx + kzz + (2m/ℏ)(ε - ℏ^2k^2/2m)t)
= (eB/πℏ)∫dkx expi(kxx + kzz + (2m/ℏ)εt)^1/2
Now we can use this expression to derive the general expression for the period in a magnetic field. From equation (12.41) in the textbook, we have:
T = (2π/ωc)(∂A/∂ε)
where ωc = eB/m is the cyclotron frequency.
Substituting in the expression we just derived for ∂A/∂ε:
T = (2π/ωc)(eB/πℏ)∫dkx expi(kxx + kzz + (2m/ℏ)εt)^1/2
= (2πℏ/ωc)(1/eB)(∂A(ε,kz)/∂ε)
= (2πℏ/ωc)(1/eB)(eB/πℏ)∫dkx expi(kxx + kzz + (2m/ℏ)εt)^1/2
= (2π/ωc)∫dkx expi(kxx + kzz + (2m/ℏ)εt)^1/2
which is the general expression for the period in a magnetic field.
Now, to show that this reduces to the free electron result (12.43), we need to evaluate the integral assuming free electrons. In this case, we have:
ε = ℏ^2k^2/2m
and therefore:
∂ε/∂k = ℏ^2k/m
Substituting this into the expression for T:
T = (2π/ωc)∫dkx exp[i(kxx + kzz + ℏk^2t/m)]
= (2π/ωc)exp(-iωct)∫dkx exp[i(kxx + kzz + ℏk^2t/m)]
= (2π/ωc)exp(-iωct)∫dkx exp[i(kxx + kzz + 2πi(ℏ/m)(kxx + kzz)t)]
= (2π/ωc)exp(-iωct)∫dkx exp[i(kxx + kzz)] = (2π/ωc)δ(kz) = 2πm/ωcℏ
which is the free electron result (12.43).
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what happens to the reading on the galvanometer when the switch in circuit 1 is a) first closed, b) kept closed, and c) opened again?
When the switch in circuit 1 is first closed (a), current begins to flow through the circuit, creating a magnetic field around the inductor. This change in magnetic field induces an electromotive force (EMF) in the coil, which causes a deflection in the galvanometer needle, indicating a momentary current flow.
When the switch is kept closed (b), the current in the circuit reaches a steady state, and the magnetic field around the inductor becomes constant. As a result, the induced EMF drops to zero, causing the galvanometer needle to return to its original position, indicating no current flow in the secondary coil.
Finally, when the switch is opened again (c), the current in the circuit stops abruptly, and the magnetic field around the inductor begins to collapse. This change in magnetic field once again induces an EMF in the secondary coil, causing the galvanometer needle to deflect in the opposite direction. This indicates a momentary current flow in the opposite direction compared to when the switch was first closed.
Thus the reading on the galvanometer will show a momentary deflection when the switch is first closed or opened, but no deflection when the switch is kept closed. The direction of the deflection will depend on the change in the magnetic field.
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use the information in the table about four different electric circuits to answer the question. circuit resistance (ohms) voltage (v) 1 0.5 20 2 0.5 40 3 0.25 40 4 0.25 60 which circuit will have the greatest electric current?
Comparing the calculated currents, we can see that Circuit 4 has the greatest electric current, which is 240A.
The circuit with the least resistance will have the greatest electric current according to Ohm's Law (I=V/R).
Therefore, Circuit 4 with a resistance of 0.25 ohms and a voltage of 60 volts will have the greatest electric current.
use Ohm's Law, which states that the current (I) equals the voltage (V) divided by the resistance (R). The formula is I = V/R.
Using the given information, we can calculate the current for each circuit:
1. Circuit 1: Resistance = 0.5 ohms, Voltage = 20V
I1 = V1/R1 = 20/0.5 = 40A
2. Circuit 2: Resistance = 0.5 ohms, Voltage = 40V
I2 = V2/R2 = 40/0.5 = 80A
3. Circuit 3: Resistance = 0.25 ohms, Voltage = 40V
I3 = V3/R3 = 40/0.25 = 160A
4. Circuit 4: Resistance = 0.25 ohms, Voltage = 60V
I4 = V4/R4 = 60/0.25 = 240A
Comparing the calculated currents, we can see that Circuit 4 has the greatest electric current, which is 240A.
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the ankylosis of the bones of the middle ear resulting in a conductive hearing loss is known as
The ankylosis of the bones of the middle ear resulting in a conductive hearing loss is known as otosclerosis.
Otosclerosis is a condition in which the bones of the middle ear, particularly the stapes bone, become fixed in place due to abnormal bone growth. This can interfere with the transmission of sound waves from the eardrum to the inner ear, resulting in a conductive hearing loss. Otosclerosis typically affects both ears and can occur in anyone, but it most commonly affects women in their 20s to 40s. Symptoms include hearing loss, tinnitus (ringing in the ears), and dizziness. Treatment options include hearing aids and surgery to replace the affected bones with prosthetic devices.
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A CD test is performed on a sand specimen. The consolidation pressure in the test, oc 30.0 kPa. The peak deviator stress was, AO peak = 128.7 kPa. The ultimate deviator stress was, Aoult = 96.1 kPa. What is the peak effective friction angle, ¢, for the sand? peak A) 43.0° B) 38.0° C) 39.4° D) 44.0° E) None of the above
The peak effective friction angle for the sand is approximately 35.9°, which is closest to option B) 38.0°.
The peak effective friction angle, φ, can be calculated using the following formula:
tan φ = (Aoult - Ao peak)/(2oc)
Substituting the given values, we get:
tan φ = (96.1 - 128.7)/(2 x 30.0) = -0.727
Taking the inverse tangent, we get:
[tex]φ = tan^-1(-0.727) = -35.9°[/tex]
However, since the effective friction angle cannot be negative, we need to add 180° to the angle:
φ = 180 - 35.9 = 144.1°
Since this angle is greater than 90°, we need to subtract it from 180° to get the peak effective friction angle:
φ = 180 - 144.1 = 35.9°
Therefore, the peak effective friction angle for the sand is approximately 35.9°, which is closest to option B) 38.0°.
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1. (25 points) A parallel plate capacitor consists of two metal plates with an area A = 542 mm? separated by a distance d = 0.36 mm. If the capacitor is connected to 9 Volt-battery (a) What is the charge Q on the capacitor? (b) What is the electric field between the plates? (e) Calculate the electric potential energy and energy density of the capacitor.
(a) The charge on the capacitor is 1.20 x 10⁻⁸ coulombs.
(b) The electric field between the plates is 2.5 x 10⁷ volts per meter.
(e) The electric potential energy of the capacitor is 5.4 x 10⁻⁷ joules. The energy density of the capacitor is 2.77 joules per cubic meter.
(a) To find the charge Q on the capacitor, we use the formula Q = CV, where C is the capacitance of the capacitor and V is the voltage applied to the capacitor.
The capacitance of a parallel plate capacitor is given by the formula C = εA/d, where ε is the permittivity of the medium between the plates, A is the area of the plates, and d is the distance between the plates.
For air, the permittivity is approximately ε = 8.85 x 10⁻¹² F/m.
Converting the area to square meters, we have A = 5.42 x 10⁻⁴ m².
Converting the distance to meters, we have d = 3.6 x 10⁻⁴ m.
Therefore, the capacitance of the capacitor is:
C = εA/d = (8.85 x 10⁻¹² F/m)(5.42 x 10⁻⁴ m²)/(3.6 x 10⁻⁴ m) = 1.33 x 10⁻⁹ F
Now, using the formula Q = CV, we have:
Q = (1.33 x 10⁻⁹ F)(9 V) = 1.20 x 10⁻⁸ C
(b) To find the electric field between the plates, we use the formula E = V/d, where V is the voltage applied to the capacitor and d is the distance between the plates.
Using the same values as before, we have:
E = 9 V/0.36 mm = 2.5 x 10⁷ V/m
(e) To calculate the electric potential energy of the capacitor, we use the formula U = (1/2)CV², where C is the capacitance of the capacitor and V is the voltage applied to the capacitor.
Using the same values as before, we have:
U = (1/2)(1.33 x 10⁻⁹ F)(9 V)² = 5.4 x 10⁻⁷ J
To calculate the energy density of the capacitor, we use the formula u = U/V, where U is the electric potential energy of the capacitor and V is the volume of the space between the plates.
The volume of the space between the plates is given by V = Ad, where A is the area of the plates and d is the distance between the plates. Using the same values as before, we have:
V = (5.42 x 10⁻⁴ m²)(3.6 x 10⁻⁴ m) = 1.95 x 10⁻⁷ m³
Therefore, the energy density of the capacitor is:
u = U/V = (5.4 x 10⁻⁷ J)/(1.95 x 10⁻⁷ m³) = 2.77 J/m³
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when the mass of an object exceeds the oppenheimer-volkov limit, the object is believed to collapse to form a(n)
When the mass of an object exceeds the Oppenheimer-Volkov limit, the object is believed to collapse to form a black hole.
The Oppenheimer-Volkov limit is the maximum mass that a neutron star can have before it collapses into a black hole due to the overwhelming force of gravity. The event horizon of a black hole is an area of spacetime where gravity is so intense that nothing, not even light or other electromagnetic waves, have the energy to cross it. According to general relativity theory, a compact enough mass can bend spacetime into a black hole. The event horizon is the line beyond which there is no escape. Despite having a significant impact on the outcome and circumstances of an object traversing it, general relativity states that it lacks any locally observable characteristics. A black hole functions in many ways like an ideal black body because it doesn't reflect any light.
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What are the different components of a steam power plant working on Rankine cycle?
The different components of a steam power plant working on Rankine cycle include the boiler, turbine, condenser, feed pump, and various auxiliary devices.
The boiler is responsible for generating steam by heating water using the heat produced from fuel combustion. The steam produced is then sent to the turbine, which converts the thermal energy of the steam into mechanical work, this work is used to drive an electric generator to produce electricity. Next, the steam exits the turbine and enters the condenser, where it is cooled by a cooling medium (usually water or air) and converted back into liquid form, this condensed water, called condensate, is then pumped back to the boiler using a feed pump, completing the cycle. The feed pump increases the pressure of the condensate to match the boiler's pressure, ensuring efficient operation.
Auxiliary devices in a steam power plant working on Rankine cycle play a crucial role in maintaining the efficiency and safety of the system. These devices include heaters, coolers, pressure regulators, and various monitoring and control systems. They assist in optimizing the operation of the power plant, maintaining the desired temperature and pressure levels, and ensuring the system functions safely and effectively. The different components of a steam power plant working on Rankine cycle include the boiler, turbine, condenser, feed pump, and various auxiliary devices.
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