The slope of the line represents the acceleration, and the percent error can be calculated by comparing the measured and theoretical values. The graph helps determine if the acceleration is inversely proportional to the mass.
The slope of a line in a graph represents the rate of change between the variables plotted on the x-axis and y-axis. In this case, the x-axis represents the total mass (kg) and the y-axis represents the acceleration (m/s^2). Therefore, the slope of the line indicates how the acceleration changes with respect to the mass.
To calculate the percent error, the measured value of the slope can be compared to the value obtained from the graph. The percent error can be calculated using the formula:
Percent Error = ((Measured Value - Theoretical Value) / Theoretical Value) * 100
By substituting the measured and theoretical values of the slope into the formula, we can determine the percent error. This calculation helps us assess the accuracy of the measurements and determine the level of deviation between the measured and expected values.
Furthermore, by examining the graph, we can determine whether the acceleration is inversely proportional to the mass. If the graph shows a negative correlation, with a decreasing trend in acceleration as mass increases, then it suggests an inverse relationship. On the other hand, if the graph shows a positive correlation, with an increasing trend in acceleration as mass increases, it indicates a direct relationship. The visual representation of the data in the graph allows us to observe the relationship between acceleration and mass more effectively.
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A 70-kg professional cyclist is climbing a mountain road at an average speed of 23.3 km/h. The foad has an average slope of 3.7 ^7
and is 13.1 km long. If the cyclist's power output averages 350 W over the duration of the climb, how much energy E does he expead?
The cyclist expends approximately 196,949.25 Joules of energy during the climb.
To find the energy expended by the cyclist during the climb, we can use the formula:
Energy (E) = Power (P) × Time (t)
First, we need to find the time taken to complete the climb. We can use the formula:
Time (t) = Distance (d) / Speed (v)
Distance = 13.1 km = 13,100 m
Speed = 23.3 km/h = 23.3 m/s
Plugging in the values:
Time (t) = 13,100 m / 23.3 m/s
Time (t) ≈ 562.715 seconds
Now, we can calculate the energy expended:
Energy (E) = Power (P) × Time (t)
Energy (E) = 350 W × 562.715 s
Energy (E) ≈ 196,949.25 Joules
Therefore, the cyclist expends approximately 196,949.25 Joules of energy during the climb.
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Problem 104. Our universe is undergoing continuous uniform ex. pansion, like an expanding balloon. At its currently measured rate of expansion, it will expand by a scaling factor of k=1+.0005T in T million years. How long will it take to expand by 10% of its present size?
Given that the rate of expansion of the universe is k = 1 + 0.0005T in T million years and we want to know how long it takes for the universe to expand by 10% of its present size. We can write the equation for the rate of expansion as follows: k = 1 + 0.0005T
where T is the number of million years. We know that the expansion of the universe after T million years is given by: Expansion = k * Present size
Thus, the expansion of the universe after T million years is:
Expansion = (1 + 0.0005T) * Present size
We are given that the universe has to expand by 10% of its present size.
Therefore,
we can write: Expansion = Present size + 0.1 * Present size= 1.1 * Present size
Equating the two equations of the expansion,
we get: (1 + 0.0005T) * Present size = 1.1 * Present size
dividing both sides by Present size, we get:1 + 0.0005T = 1.1
Dividing both sides by 0.0005, we get: T = (1.1 - 1)/0.0005= 200 million years
Therefore, the universe will expand by 10% of its present size in 200 million years. Hence, the correct answer is 200.
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A certain boat traveling on a river displaces a volume of 6.7 m of water. The density of the water is 1000 kg/m2.) a. What is the mass of the water displaced by the boat? b. What is the weight of the boat?
According to the question (a). The mass of the water displaced by the boat is 6700 kg. (b). The weight of the boat is 65560 N.
a. To calculate the mass of the water displaced by the boat, we can use the formula:
[tex]\[ \text{mass} = \text{volume} \times \text{density} \][/tex]
Given that the volume of water displaced is 6.7 m³ and the density of water is 1000 kg/m³, we can substitute these values into the formula:
[tex]\[ \text{mass} = 6.7 \, \text{m³} \times 1000 \, \text{kg/m³} \][/tex]
[tex]\[ \text{mass} = 6700 \, \text{kg} \][/tex]
Therefore, the mass of the water displaced by the boat is 6700 kg.
b. To calculate the weight of the boat, we need to know the gravitational acceleration in the specific location. Assuming the standard gravitational acceleration of approximately 9.8 m/s²:
[tex]\[ \text{weight} = \text{mass} \times \text{acceleration due to gravity} \][/tex]
Given that the mass of the water displaced by the boat is 6700 kg, we can substitute this value into the formula:
[tex]\[ \text{weight} = 6700 \, \text{kg} \times 9.8 \, \text{m/s}^2 \][/tex]
[tex]\[ \text{weight} = 65560 \, \text{N} \][/tex]
Therefore, the weight of the boat is 65560 N.
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FM frequencies range between 88 MHz and 108 MHz and travel at
the same speed.
What is the shortest FM wavelength? Answer in units of m.
What is the longest FM wavelength? Answer in units of m.
The shortest FM wavelength is 2.75 m. The longest FM wavelength is 3.41 m.
Frequency Modulation
(FM) is a kind of modulation that entails altering the frequency of a carrier wave to transmit data.
It is mainly used for transmitting audio signals. An FM frequency
ranges
from 88 MHz to 108 MHz, as stated in the problem.
The wavelength can be computed using the
formula
given below:wavelength = speed of light/frequency of waveWe know that the speed of light is 3 x 10^8 m/s. Substituting the minimum frequency value into the formula will result in a maximum wavelength:wavelength = 3 x 10^8/88 x 10^6wavelength = 3.41 mSimilarly, substituting the maximum frequency value will result in a minimum wavelength:wavelength = 3 x 10^8/108 x 10^6wavelength = 2.75 mThe longer the wavelength, the better the signal propagation.
The FM
wavelength
ranges between 2.75 and 3.41 meters, which are relatively short. As a result, FM signals are unable to penetrate buildings and other structures effectively. It has a line-of-sight range of around 30 miles due to its short wavelength. FM is mainly used for local radio stations since it does not have an extensive range.
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13 Select the correct answer. Which missing item would complete this alpha decay reaction? + He 257 100 Fm → OA. 29C1 253 98 B. 255 C. 253 D. 22th 904 O E. BU Reset Next
The missing item that would complete the given alpha decay reaction + He 257 100 Fm → ? is option C. 253.
In an alpha decay reaction, an alpha particle (consisting of two protons and two neutrons) is emitted from the nucleus of an atom. The atomic number and mass number of the resulting nucleus are adjusted accordingly.
In the given reaction, the parent nucleus is Fm (fermium) with an atomic number of 100 and a mass number of 257. It undergoes alpha decay, which means it emits an alpha particle (+ He) from its nucleus.
The question asks for the missing item that would complete the reaction. Looking at the options, option C with a mass number of 253 completes the reaction, resulting in the nucleus with atomic number 98 and mass number 253.
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a 190-lb man carries a 20-lb can of paint up a helical staircase that encircles a silo with radius 15 ft. if the silo is 80 ft high and the man makes exactly four complete revolutions, how much work is done by the man against gravity in climbing to the top?
The work done by the man against gravity in climbing to the top is 9,480 foot-pounds.
To calculate the work done by the man, we need to determine the total change in potential energy as he climbs up the helical staircase that encircles the silo. The potential energy can be calculated using the formula PE = mgh, where m represents the mass, g represents the acceleration due to gravity, and h represents the height.
In this case, the mass of the man is 190 lb, and the height of the silo is 80 ft. Since the man makes exactly four complete revolutions around the silo, we can calculate the circumference of the helical staircase. The circumference of a circle is given by the formula C = 2πr, where r represents the radius. In this case, the radius of the silo is 15 ft.
To find the work done against gravity, we need to multiply the change in potential energy by the number of revolutions. The change in potential energy is obtained by multiplying the mass, the acceleration due to gravity (32.2 ft/s²), and the height. The number of revolutions is four.
Therefore, the work done by the man against gravity in climbing to the top can be calculated as follows:
Work = 4 * m * g * h
= 4 * 190 lb * 32.2 ft/s² * 80 ft
= 9,480 foot-pounds.
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For the following three vectors, what is 3C (2A× B)? A = 2.00 +3.00 - 7.00k B = -3.00 +7.00 Ĵ + 2.00k = 4.00 8.00
For the following three vectors,3C (2A × B) is equal to 660.00i + 408.00j + 240.00k.
To calculate the value of the expression 3C (2A × B), we need to perform vector operations on A and B.
Given:
A = 2.00i + 3.00j - 7.00k
B = -3.00i + 7.00j + 2.00k
First, let's calculate the cross product of 2A and B:
2A × B = 2(A × B)
To find the cross product, we can use the determinant method or the component method. Let's use the component method:
(A × B)_x = (Ay×Bz - Az × By)
(A × B)_y = (Az × Bx - Ax × Bz)
(A × B)_z = (Ax × By - Ay ×Bx)
Substituting the values of A and B into these equations, we get:
(A × B)_x = (3.00 × 2.00) - (-7.00 ×7.00) = 6.00 + 49.00 = 55.00
(A × B)_y = (-7.00 × (-3.00)) - (2.00 × 2.00) = 21.00 - 4.00 = 17.00
(A × B)_z = (2.00 × 7.00) - (2.00 × (-3.00)) = 14.00 + 6.00 = 20.00
Therefore, the cross product of 2A and B is:
2A × B = 55.00i + 17.00j + 20.00k
Now, let's calculate 3C (2A × B):
Given:
C = 4.00i + 8.00j
3C (2A × B) = 3(4.00i + 8.00j)(55.00i + 17.00j + 20.00k)
Expanding and multiplying each component, we get:
3C (2A × B) = 3(4.00 × 55.00)i + 3(8.00 ×17.00)j + 3(4.00 ×20.00)k
Simplifying the expression, we have:
3C (2A × B) = 660.00i + 408.00j + 240.00k
Therefore, 3C (2A × B) is equal to 660.00i + 408.00j + 240.00k.
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How long will it take for 30 grams of Rn-222 to decay to 7. 5g?
Half-Life: 3. 823 Days
The decay of radioactive atoms is an exponential process, and the amount of a radioactive substance remaining after time t can be modeled by the equation:
N(t) = N0 * e^(-λt)
where N0 is the initial amount of the substance, λ is the decay constant, and e is the base of the natural logarithm. The half-life of Rn-222 is given as 3.823 days, which means that the decay constant is:
λ = ln(2)/t_half = ln(2)/3.823 days ≈ 0.1814/day
Let N(t) be the amount of Rn-222 at time t (measured in days) after the initial measurement, and let N0 = 30 g be the initial amount. We want to find the time t such that N(t) = 7.5 g.
Substituting the given values into the equation above, we get:
N(t) = 30 * e^(-0.1814t) = 7.5
Dividing both sides by 30, we get:
e^(-0.1814t) = 0.25
Taking the natural logarithm of both sides, we get:
-0.1814t = ln(0.25) = -1.3863
Solving for t, we get:
t = 7.64 days
Therefore, it will take approximately 7.64 days for 30 grams of Rn-222 to decay to 7.5 grams.
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Two capacitors, C, = 6.10 MF and Cz = 3.18 F, are connected in parallel, then the combination is connected to a 250 V battery. When the capacitors are charged, each one is removed from the circuit. Next, the two charged capacitors are connected to each other so that the positive plate of one
capacitor is connected to the negative plate of the other capacitor. What is the resulting charge on each capacitor (in uC)?
The resulting charge on each capacitor, both when connected in parallel to the battery and when connected to each other in series, is approximately 2.32 µC.
When capacitors are connected in parallel, the voltage across them is the same. Therefore, the voltage across the combination of capacitors in the first scenario (connected in parallel to the battery) is 250 V.
For capacitors connected in parallel, the total capacitance (C_total) is the sum of individual capacitances:
C_total = C1 + C2
Given:
C1 = 6.10 µF = 6.10 × 10^(-6) F
C2 = 3.18 F
C_total = C1 + C2
C_total = 6.10 × 10^(-6) F + 3.18 × 10^(-6) F
C_total = 9.28 × 10^(-6) F
Now, we can calculate the charge (Q) on each capacitor when connected in parallel:
Q = C_total × V
Q = 9.28 × 10^(-6) F × 250 V
Q ≈ 2.32 × 10^(-3) C
Therefore, the resulting charge on each capacitor when connected in parallel to the battery is approximately 2.32 µC.
When the capacitors are disconnected from the circuit and connected to each other in series, the charge remains the same on each capacitor.
Thus, the resulting charge on each capacitor when they are connected to each other in series is also approximately 2.32.
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Vertically polarized light of intensity lo is incident on a polarizer whose transmission axis is at an angle of 70° with the vertical. If the intensity of the transmitted light is measured to be 0.34W/m² the intensity lo of the incident light is 0.43 W/m 1.71 W/m 2.91 W/m 0.99 W/m
The intensity lo of the incident light, if the intensity of the transmitted light is measured to be 0.34W/m² is 1.050 W/m². So none of the options are correct.
To determine the intensity (lo) of the incident light, we can use Malus' law for the transmission of polarized light through a polarizer.
Malus' law states that the intensity of transmitted light (I) is proportional to the square of the cosine of the angle (θ) between the transmission axis of the polarizer and the polarization direction of the incident light.
Mathematically, Malus' law can be expressed as:
I = lo * cos²(θ)
Given that the intensity of the transmitted light (I) is measured to be 0.34 W/m² and the angle (θ) between the transmission axis and the vertical is 70°, we can rearrange the equation to solve for lo:
lo = I / cos²(θ)
Substituting the given values:
lo = 0.34 W/m² / cos²(70°)
The value of cos²(70°) as approximately 0.3236. Plugging this value into the equation:
lo = 0.34 W/m² / 0.3236
lo = 1.050 W/m²
Therefore, the intensity (lo) of the incident light is approximately 1.050 W/m².
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CI Photo Credit Cameron Out A 1.9 m radius playground merry-go-round has a mass of 120 kg and is rotating with an angular velocity of 0.400 rev/s. What is its angular velocity after a 22.0 kg child gets onto it by grabbing its outer edge? a The added child is initially at rest. Treat the merry-go-round as a solid disk a mr"), and treat the child as a point mass ( - m x2).
When a 22.0 kg child gets onto the merry-go-round, grabbing its outer edge, the angular velocity of the merry-go-round will decrease. The angular momentum added by the child is L_child = (22.0 kg)(1.9 m)^2 × 0 rev/s.
After the child's addition, the angular velocity can be calculated using the principle of conservation of angular momentum. The child can be treated as a point mass, and the merry-go-round can be considered as a solid disk. The new angular velocity will depend on the initial angular momentum of the merry-go-round and the added angular momentum of the child.
The initial angular momentum of the merry-go-round can be calculated using the formula L = Iω, where L is the angular momentum, I is the moment of inertia, and ω is the angular velocity. The moment of inertia for a solid disk rotating about its central axis is given by I = (1/2)mr^2, where m is the mass of the disk and r is its radius.
Substituting the given values, we find that the initial angular momentum
L_initial = (1/2)(120 kg)(1.9 m)^2 × 0.400 rev/s.
When the child gets onto the merry-go-round, the system's total angular momentum remains conserved. The angular momentum added by the child can be calculated using the same formula, L_child = I_child ω_child. Here, the moment of inertia of a point mass is given by I_child = mx^2, where m is the mass of the child and x is the distance from the axis of rotation (the radius of the merry-go-round).
Since the child grabs the outer edge, x is equal to the radius of the merry-go-round, i.e., x = 1.9 m. Therefore, the angular momentum added by the child is L_child = (22.0 kg)(1.9 m)^2 × 0 rev/s.
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Given an object distance of 12 cm and a lens with focal length
of magnitude 4 cm, what is the image distance for a concave lens?
Give your answers in cm.
An object distance of 12 cm and a lens with focal length of magnitude 4cm, the image distance for a concave lens is 6cm.
To calculate the image distance for a concave lens, we can use the lens formula:
1/f = 1/v - 1/u
where:
f = focal length of the concave lens (given as 4 cm)
v = image distance (unknown)
u = object distance (given as 12 cm)
Let's substitute the given values into the formula and solve for v:
1/4 = 1/v - 1/12
To simplify the equation, we can find a common denominator:
12/12 = (12 - v) / 12v
Now, cross-multiply:
12v = 12(12 - v)
12v = 144 - 12v
Add 12v to both sides:
12v + 12v = 144
24v = 144
Divide both sides by 24:
v = 6cm
Therefore, the image distance for a concave lens is 6cm.
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An air bubble at the bottom of a lake 41,5 m doep has a volume of 1.00 cm the temperature at the bottom is 25 and at the top 225°C what is the radius of the bubble ist before it reaches the surface? Express your answer to two significant figures and include the appropriate units.
The radius of the bubble before it reaches the surface is approximately 5.4 × 10^(-4) m
The ideal gas law and the hydrostatic pressure equation.
Temperature at the bottom (T₁) = 25°C = 25 + 273.15 = 298.15 K
Temperature at the top (T₂) = 225°C = 225 + 273.15 = 498.15 K
Using the ideal gas law equation: PV = nRT, where P is the pressure, V is the volume, n is the number of moles, R is the gas constant, and T is the temperature in Kelvin.
(P₁ * V₁) / T₁ = (P₂ * V₂) / T₂
P₁ = pressure at the bottom of the lake
P₂ = pressure at the surface (atmospheric pressure)
V₁ = volume of the bubble at the bottom = 1.00 cm³ = 1.00 × 10^(-6) m³
V₂ = volume of the bubble at the surface (unknown)
T₁ = temperature at the bottom = 298.15 K
T₂ = temperature at the top = 498.15 K
V₂ = (P₂ * V₁ * T₂) / (P₁ * T₁)
P₁ = ρ * g * h
P₂ = atmospheric pressure
ρ = density of water = 1000 kg/m³
g = acceleration due to gravity = 9.8 m/s²
h = height = 41.5 m
P₁ = 1000 kg/m³ * 9.8 m/s² * 41.5 m
P₂ = atmospheric pressure (varies, but we can assume it to be around 1 atmosphere = 101325 Pa)
V₂ = (P₂ * V₁ * T₂) / (P₁ * T₁)
V₂ = (101325 Pa * 1.00 × 10^(-6) m³ * 498.15 K) / (1000 kg/m³ * 9.8 m/s² * 41.5 m * 298.15 K)
V₂ ≈ 1.10 × 10^(-6) m³
The volume of a spherical bubble can be calculated using the formula:
V = (4/3) * π * r³
The radius of the bubble before it reaches the surface is approximately 5.4 × 10^(-4) m
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1. An oil drop is balanced in a Millikan apparatus. The drop has a mass of 1.8 10-18 kg. The plates have a potential difference of 920 V, are separated by 3.6 cm, and the lower plate is positive. Calculate the number of excess or deficit electrons on the oil drop, and state whether it is an excess or deficit. [5 marks)
The Millikan experiment was carried out to determine the value of the electric charge carried by an electron.'
The method was to suspend oil droplets in a uniform electric field between two metal plates by adjusting the voltage applied to the plates such that the force on the droplet was balanced by the force of gravity. The excess or deficit charge on the droplet could then be calculated and from this,
The charge carried by an electron could be determined.What is an oil drop?An oil drop is a charged droplet of oil that is formed in a high voltage field. An oil droplet carries an electric charge because when it comes into contact with an ion.
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Juan loves the movie "Titanic". So after he gets his Pfizer booster he takes a Disney Cruise to Newfoundland, Canada (where the real Titanic sank) and is on the look out for icebergs. However, due to global warming all the ice he sees are roughly 1 m cubes. If ice has a density of 917 kg/m^3 and the ocean water has a density of 1,025 kg/m^3, how high will the 1 m^3 "icebergs" above the water so that Juan can see them?
Group of answer choices
A. 0.4 m
B. 1.0 m
C. 0.6 m
D. 0.1 m
The fraction of the ice above the water level is 0.6 meters (option c).
The ice floats on water because its density is less than that of water. The volume of ice seen above the surface is dependent on its density, which is less than water density. The volume of the ice is dependent on the water that it displaces. An ice cube measuring 1 m has a volume of 1m^3.
Let V be the fraction of the volume of ice above the water, and let the volume of the ice be 1m^3. Therefore, the volume of water displaced by ice will be V x 1m^3.The mass of the ice is 917kg/m^3 * 1m^3, which is equal to 917 kg. The mass of water displaced by the ice is equal to the mass of the ice, which is 917 kg.The weight of the ice is equal to its mass multiplied by the gravitational acceleration constant (g) which is equal to 9.8 m/s^2.
Hence the weight of the ice is 917kg/m^3 * 1m^3 * 9.8m/s^2 = 8986.6N.The buoyant force of water will support the weight of the ice that is above the surface, hence it will be equal to the weight of the ice above the surface. Therefore, the buoyant force on the ice is 8986.6 N.The formula for the buoyant force is as follows:
Buoyant force = Volume of the fluid displaced by the object × Density of the fluid × Gravity.
Buoyant force = V*1m^3*1025 kg/m^3*9.8m/s^2 = 10002.5*V N.
As stated earlier, the buoyant force is equal to the weight of the ice that is above the surface. Hence, 10002.5*V N = 8986.6
N.V = 8986.6/10002.5V = 0.8985 meters.
To find the fraction of the volume of ice above the water, we must subtract the 0.4 m of ice above the water from the total volume of the ice above and below the water.V = 1 - (0.4/1)V = 0.6 meters.
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A satellite revolving around Earth has an orbital radius of 1.5 x 10^4 km. Gravity being the only force acting on the satele calculate its time period of motion in seconds. You can use the following numbers for calculation: Mass of Earth = 5.97 x 10^24 kg Radius of Earth = 6.38 x 10^3 km Newton's Gravitational Constant (G) = 6.67 x 10^-11 N m^2/kg^2 Mass of the Satellite = 1050 kg O a. 1.90 x 10^4 s O b. 4.72 x 10^3 s O c. 11.7 x 10^7 s O d. 3.95 x 10^6 s O e. 4.77 x 10^2 s O f. 2.69 x 10^21 s
The time period of motion of a satellite revolving around Earth with an orbital radius of 1.5 x 10^4 km is 67805.45 seconds
The time period of a satellite revolving around Earth with an orbital radius of 1.5 x 10^4 km can be calculated as follows: Given values are:
Mass of Earth (M) = 5.97 x 10^24 kg
Radius of Earth (R) = 6.38 x 10^3 km
Newton's Gravitational Constant (G) = 6.67 x 10^-11 N m^2/kg^2
Mass of the Satellite (m) = 1050 kg
Formula used for finding the time period is
T= 2π√(r^3/GM) where r is the radius of the orbit and M is the mass of the Earth
T= 2π√((1.5 x 10^4 + 6.38 x 10^3)^3/(6.67 x 10^-11 x 5.97 x 10^24))T = 2π x 10800.75T = 67805.45 seconds
The time period of motion of the satellite is 67805.45 seconds.
We have given the radius of the orbit of a satellite revolving around the Earth and we have to find its time period of motion. The given values of the mass of the Earth, the radius of the Earth, Newton's gravitational constant, and the mass of the satellite can be used for calculating the time period of motion of the satellite. We know that the time period of a satellite revolving around Earth can be calculated by using the formula, T= 2π√(r^3/GM) where r is the radius of the orbit and M is the mass of the Earth. Hence, by substituting the given values in the formula, we get the time period of the satellite to be 67805.45 seconds.
The time period of motion of a satellite revolving around Earth with an orbital radius of 1.5 x 10^4 km is 67805.45 seconds.
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A school building has a design heat loss coefficient of 0.025MW/K and an effective thermal capacity of 2500 MJ/K. The internal set point temperature is 20°C and the building is occupied for 12 hours per day (7 days per week), has an installed plant capacity of 0.5 MW. For a mean monthly outdoor temperature of 5°C (when the preheat time is 5.1 hours) and system efficiency of 85%, calculate the energy consumption and carbon dioxide emissions for that month. (Assume 0.31kgCO2 per kWh of gas). Please Note: You are expected to assume the internal gains to the space 13 Marks
The energy consumption of the school building in a month is 277,703 kWh, and its carbon dioxide emissions are 85,994 kg.CO₂.
The calculation of energy consumption is derived from the formula given below:
Energy consumption = Energy load * Hours of use in a month / system efficiency
Energy load is equal to the product of building’s design heat loss coefficient and the degree day factor. Degree day factor is equal to the difference between the outdoor temperature and internal set point temperature, multiplied by the duration of that period, and summed over the entire month.
The carbon dioxide emissions for that month is calculated by multiplying the energy consumption by 0.31 kg.CO₂/kWh of gas.
As per the given data, energy load = 0.025MW/K * (20°C-5°C) * (24h-5.1h) * 30 days = 10,440 MWh, and the degree day factor is 15°C * (24h-5.1h) * 30 days = 10,818°C-day.
Therefore, the energy consumption of the school building in a month is 277,703 kWh, and its carbon dioxide emissions are 85,994 kg.CO₂.
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EM radiation has an average intensity of 1700 W/m2. Which of the following statements about the E or B fields in this radiation is correct? Erms = 800.2 N/C Bmax = 4.42 x 10-6 T Brms = 2.29 x 10-6 T Emax = 1500.0 N/C At a certain place on the surface of the earth, the sunlight has an intensity of about 1.8 x 103 W/m². What is the total electromagnetic energy from this sunlight in 5.5 m³ of space? (Give your answer in joules but don't include the units.) Click Submit to complete this assessment. Question 12 of
The correct statement about the E or B fields in radiation is that Erms = 800.2 N/C.
EM (electromagnetic) radiation has an average intensity of 1700 W/m². As a result, the electrical field (Erms) is related to the average intensity through the equation E = cB, where E is the electric field, B is the magnetic field, and c is the speed of light.
Erms is related to the average intensity I (in W/m²) through the formula Erms = sqrt(2 I / c ε) which is approximately equal to 800.2 N/C.
For a 5.5 m³ space on the earth's surface, the total electromagnetic energy from sunlight with an intensity of 1.8 x 103 W/m² is 9.9 x 106 J.
The formula for calculating the energy is E = I × A × t, where E is the energy, I is the intensity, A is the area, and t is the time.
Here, the area is 5.5 m³ and the time is 1 second, giving an energy of 9.9 x 106 J.
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S For each of the following systems and time intervals, write the appropriate expanded version of Equation 8.2, the conservation of energy equation.(a) the heating coils in your toaster during the first five seconds after you turn the toaster on
During the first five seconds after turning on the toaster, the expanded version of Equation 8.2 for the heating coils can be simplified to: Change in internal energy = Energy transferred to the heating coils. The equation can be simplified to focus on the internal energy change.
The conservation of energy equation, Equation 8.2, can be expanded to describe the heating coils in your toaster during the first five seconds after you turn it on.
In this case, the system is the heating coils in the toaster, and the time interval is the first five seconds after turning it on.
Equation 8.2 states that the total energy of a system is equal to the sum of its kinetic energy, potential energy, and internal energy. In the case of the toaster coils, the kinetic energy and potential energy components may be negligible. Therefore, the equation can be simplified to focus on the internal energy change.
Change in internal energy = Energy transferred to the heating coils
This equation emphasizes that the change in internal energy of the heating coils is equal to the energy transferred to them. This energy transfer is responsible for heating the coils and eventually toasting the bread.
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Enter only the last answer c) into moodle.
A solid sphere of mass M and radius R rolls without slipping to the right with a linear speed of v
a) Find a simplified algebraic expression using symbols only for the tolal kinetic energy Kior of the ball in terms of M and R
b) IfM = 7.5 kg. R = 10,8 cm and v = 4.5 m/s find the moment of inertia of the bail.
c) Plug in the numbers from part b) into your formula from part a) to get the value of the total kinetic energy
The total kinetic energy of the rolling ball, taking into account both its translational and rotational kinetic energy, is approximately 100.356 Joules. This is calculated by considering the mass, linear speed, radius, moment of inertia, and angular velocity of the ball.
a) The total kinetic energy of the rolling ball can be expressed as the sum of its translational kinetic energy and rotational kinetic energy.
The translational kinetic energy (Kt) is given by the formula: Kt = 0.5 * M * v^2, where M is the mass of the ball and v is its linear speed.
The rotational kinetic energy (Kr) is given by the formula: Kr = 0.5 * I * ω^2, where I is the moment of inertia of the ball and ω is its angular velocity.
Since the ball is rolling without slipping, the linear speed v is related to the angular velocity ω by the equation: v = R * ω, where R is the radius of the ball.
Therefore, the total kinetic energy (Kior) of the ball can be expressed as: Kior = Kt + Kr = 0.5 * M * v^2 + 0.5 * I * (v/R)^2.
b) To find the moment of inertia (I) of the ball, we can rearrange the equation for ω in terms of v and R: ω = v / R.
Substituting the values, we have: ω = 4.5 m/s / 0.108 m = 41.67 rad/s.
The moment of inertia (I) can be calculated using the equation: I = (2/5) * M * R^2.
Substituting the values, we have: I = (2/5) * 7.5 kg * (0.108 m)^2 = 0.08712 kg·m².
c) Plugging in the values from part b) into the formula from part a) for the total kinetic energy (Kior):
Kior = 0.5 * M * v^2 + 0.5 * I * (v/R)^2
= 0.5 * 7.5 kg * (4.5 m/s)^2 + 0.5 * 0.08712 kg·m² * (4.5 m/s / 0.108 m)^2
= 91.125 J + 9.231 J
= 100.356 J.
Therefore, the total kinetic energy of the ball, with the given values, is approximately 100.356 Joules.
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Two spheres with uniform surface charge density, one with a radius of 7.1 cm and the other with a radius of 4.2 cm, are separated by a center-to-center distance of 38 cm. The spheres have a combined charge of + 55jC and repel one another with a
force of 0.71 N. Assume that the chargo of the first sphote is
eator than the charge o the second sobore
What is tho surface chargo density on the sobero bi radicie 7 12
The surface charge density can be calculated by using the formula:σ=q/A, where σ = surface charge density, q = charge of a spherical object A = surface area of a spherical object. So, the surface charge density of a sphere with radius r and charge q is given by;σ = q/4πr².
The total charge of the spheres, q1 + q2 = 55 μC. The force of repulsion between the two spheres, F = 0.71 N.
To find, The surface charge density on the sphere with radius 7.1 cm,σ1 = q1/4πr1². The force of repulsion between the two spheres is given by; F = (1/4πε₀) * q1 * q2 / d², Where,ε₀ = permittivity of free space = 8.85 x 10^-12 N^-1m^-2C²q1 + q2 = 55 μC => q1 = 55 μC - q2.
We have two equations: F = (1/4πε₀) * q1 * q2 / d²σ1 = q1/4πr1². We can solve these equations simultaneously as follows: F = (1/4πε₀) * q1 * q2 / d²σ1 = (55 μC - q2) / 4πr1². Putting the values in the first equation and solving for q2:0.71 N = (1/4πε₀) * (55 μC - q2) * q2 / (38 cm)²q2² - (55 μC / 0.71 N * 4πε₀ * (38 cm)²) * q2 + [(55 μC)² / 4 * (0.71 N)² * (4πε₀)² * (38 cm)²] = 0q2 = 9.24 μCσ1 = (55 μC - q2) / 4πr1²σ1 = (55 μC - 9.24 μC) / (4π * (7.1 cm)²)σ1 = 23.52 μC/m².
Therefore, the surface charge density on the sphere with radius 7.1 cm is 23.52 μC/m².
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Onsider a turbojet engine mounted on a stationary test stand at sea level. The inlet and exit areas are 1. 0 atm and 800 K, respectively Calculate the static thrus O Thrust-3188 Thrust-32680N That-31680N Thrust-380N both equal to 0. 45 m². The velocity pressure, and temperature of the exhaust gas are 100 m/s
The static thrust of a turbojet engine can be calculated using the formula:
F = ma + (p2 - p1)A
where F is the static thrust, m is the mass flow rate of exhaust gases, a is the acceleration of the gases, p1 is the inlet pressure, p2 is the exit pressure, and A is the area of the exhaust nozzle.
Given that the inlet and exit areas are both 0.45 m², the area A equals 0.45 m².
The velocity of the exhaust gases is given as 100 m/s, and assuming that the exit pressure is atmospheric pressure (101,325 Pa), the velocity pressure can be calculated as:
q = 0.5 * ρ * V^2 = 0.5 * 1.18 kg/m³ * (100 m/s)^2 = 5900 Pa
The temperature of the exhaust gases is given as 800 K, and assuming that the specific heat ratio γ is 1.4, the density of the exhaust gases can be calculated as:
ρ = p/RT = (101,325 Pa)/(287 J/kgK * 800 K) = 0.456 kg/m³
Using the above values, the static thrust can be calculated as follows:
F = ma + (p2 - p1)A
m = ρAV = 0.456 kg/m³ * 0.45 m² * 100 m/s = 20.52 kg/s
a = (p2 - p1)/ρ = (101,325 Pa - 1 atm)/(0.456 kg/m³) = 8367.98 m/s^2
Therefore,
F = 20.52 kg/s * 8367.98 m/s^2 + (101,325 Pa - 1 atm)*0.45 m² = 31680 N
Hence, the static thrust of the turbojet engine is 31680 N.
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What is the pressure inside a 310 L container holding 103.9 kg of argon gas at 21.0 ∘ C ? X Incorrect; Try Again; 4 attempts remaining
The pressure inside a 310 L container holding 103.9 kg of argon gas at 21.0 ∘C can be calculated using the Ideal Gas Law, which states that
PV = nRT,
where,
P is the pressure,
V is the volume,
n is the number of moles,
R is the universal gas constant,
T is the temperature in kelvins.
We can solve forP as follows:P = nRT/V .We need to first find the number of moles of argon gas present. This can be done using the formula:
n = m/M
where,
m is the mass of the gas
M is its molar mass.
For argon, the molar mass is 39.95 g/mol.
n = 103.9 kg / 39.95 g/mol
= 2.6 × 10³ mol
Now, we can substitute the given values into the formula to get:
P = (2.6 × 10³ mol)(0.0821 L·atm/mol·K)(294.15 K) / 310 L
≈ 60.1 atm
Therefore, the pressure inside the container is approximately 60.1 atm.
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Part A Calculate the displacement current Ip between the square platos, 6.8 cm on a side of a capacitor if the electric field is changing at a rate of 2.1 x 10% V/m. Express your answer to two significant figures and include the appropriate units. lo =
the displacement current between the square plates of the capacitor is 9694 A. To calculate displacement current, we convert the units appropriately and perform the multiplication.
In this case, the square plates have a side length of 6.8 cm, which gives us an area of (6.8 cm)^2. The electric field is changing at a rate of 2.1 x 10^6 V/m.
The displacement current (Ip) between the square plates of a capacitor can be calculated by multiplying the rate of change of electric field (dE/dt) by the area (A) of the plates.
The area of the square plates is (6.8 cm)^2 = 46.24 cm^2. Converting this to square meters, we have A = 46.24 cm^2 = 0.004624 m^2.
Now, we can calculate the displacement current (Ip) by multiplying the rate of change of electric field (dE/dt) by the area (A):
Ip = (dE/dt) * A = (2.1 x 10^6 V/m) * (0.004624 m^2) = 9694 A
Therefore, the displacement current between the square plates of the capacitor is 9694 A.
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A police car is moving to the right at 27 m/s, while a speeder is coming up from behind at a speed 36 m/s, both speeds being with respect to the ground. The police officer points a radar gun at the oncoming speeder. Assume that the electromagnetic wave emitted by the gun has a frequency of 7.5×109 Hz. Find the difference between the frequency of the wave that returns to the police car after reflecting from the speeder's car and the frequency emitted by the police car.
In this scenario, a police car is moving to the right at 27 m/s, and a speeder is approaching from behind at 36 m/s.
The police officer points a radar gun at the speeder, emitting an electromagnetic wave with a frequency of 7.5×10^9 Hz. The task is to find the difference between the frequency of the wave that returns to the police car after reflecting from the speeder's car and the frequency emitted by the police car.
The frequency of the wave that returns to the police car after reflecting from the speeder's car is affected by the relative motion of the two vehicles. This phenomenon is known as the Doppler effect.
In this case, since the police car and the speeder are moving relative to each other, the frequency observed by the police car will be shifted. The Doppler effect formula for frequency is given by f' = (v + vr) / (v + vs) * f, where f' is the observed frequency, v is the speed of the wave in the medium (assumed to be the same for both the emitted and reflected waves), vr is the velocity of the radar gun wave relative to the speeder's car, vs is the velocity of the radar gun wave relative to the police car, and f is the emitted frequency.
In this scenario, the difference in frequency can be calculated as the observed frequency minus the emitted frequency: Δf = f' - f. By substituting the given values and evaluating the expression, the difference in frequency can be determined.
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Two capacitors are connected parallel to each
other. Let C1 = 3.50 F .C2 = 5.10 pF be their
capacitances, and Vat = 57.0 V the potential
difference across the system.
a) Calculate the charge on each capacitor (capacitor 1 and 2)
b) Calculate the potential difference across each capacitor (capacitor 1 and 2)
The charge on capacitor 1 is approximately 199.5 C, and the charge on capacitor 2 is approximately 2.907 × 10⁻¹⁰ C. The potential difference across capacitor 1 is approximately 57.0 V, and the potential difference across capacitor 2 is approximately 56.941 V.
a) To calculate the charge on each capacitor, we can use the formula:
Q = C × V
Where:
Q is the charge on the capacitor,
C is the capacitance, and
V is the potential difference across the capacitor.
For capacitor 1:
Q1 = C1 × Vat
= 3.50 F × 57.0 V
For capacitor 2:
Q2 = C2 × Vat
= 5.10 pF × 57.0 V
pF stands for picofarads, which is 10⁻¹² F.
Therefore, we need to convert the capacitance of capacitor 2 to farads:
C2 = 5.10 pF
= 5.10 × 10⁻¹² F
Now we can calculate the charges:
Q1 = 3.50 F × 57.0 V
= 199.5 C
Q2 = (5.10 × 10⁻¹² F) × 57.0 V
= 2.907 × 10⁻¹⁰ C
Therefore, the charge on capacitor 1 is approximately 199.5 C, and the charge on capacitor 2 is approximately 2.907 × 10⁻¹⁰ C.
b) To calculate the potential difference across each capacitor, we can use the formula:
V = Q / C
For capacitor 1:
V1 = Q1 / C1
= 199.5 C / 3.50 F
For capacitor 2:
V2 = Q2 / C2
= (2.907 × 10⁻¹⁰ C) / (5.10 × 10⁻¹² F)
Now we can calculate the potential differences:
V1 = 199.5 C / 3.50 F
= 57.0 V
V2 = (2.907 × 10⁻¹⁰ C) / (5.10 × 10⁻¹² F)
= 56.941 V
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If calcium has a 0.647 in specific heat and has been added 5.0 more does that mean it has a high temperature in specific heat?
Calcium has a specific heat capacity of 0.647. This means that it requires 0.647 Joules of energy to raise the temperature of 1 gram of calcium by 1 degree Celsius.
If calcium has a 0.647 in specific heat and has been added 5.0 more does that mean it has a high temperature in specific heat? Adding 5.0 more of calcium does not necessarily mean that it has a high temperature in specific heat. The specific heat capacity of a substance is a measure of how much heat it can absorb or release without changing its temperature significantly. It is not directly related to the temperature of the substance. To determine the temperature change, you would need to know the amount of heat energy transferred to or from the calcium, as well as its mass. Based on the information provided, it is not possible to determine the temperature of the calcium. Calcium has a specific heat capacity of 0.647. This means that it requires 0.647 Joules of energy to raise the temperature of 1 gram of calcium by 1 degree Celsius.
The specific heat capacity of calcium is 0.647, but without more information, we cannot determine its temperature.
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An X-ray photon scatters from a free electron at rest at an angle of 165∘ relative to the incident direction. Use h=6.626⋆10−34 Js for Planck constant. Use c=3.00⋆108 m/s for the speed of light in a vacuum. Part A - If the scattered photon has a wavelength of 0.310 nm, what is the wavelength of the incident photon? Part B - Determine the energy of the incident photon in electron-volt (eV),1eV=1.6×10−19 J Part C - Determine the energy of the scattered photon. Part D - Find the kinetic energy of the recoil electron. Unit is eV. Keep 1 digit after the decimal point. Learning Goal: An X-ray photon scatters from a free electron at rest at an angle of 165∘ relative to the incident direction. Use h=6.626⋆10−34Js for Planck constant. Use c=3.00∗108 m/s for the speed of light in a vacuum.
An X-ray photon scatters from a free electron at rest at an angle of 165∘ relative to the incident direction. Use h=6.626×10⁻³⁴ J s for Planck constant. Use c=3.00×10⁸ m/s for the speed of light in a vacuum.
Part A - If the scattered photon has a wavelength of 0.310 nm, the wavelength of the incident photon is 0.310 nm.
Part B - The energy of the incident photon in electron-volt is 40.1 eV.
Part C - The energy of the scattered photon is 40.1 eV.
Part D - The kinetic energy of the recoil electron is 0 eV.
To solve this problem, we can use the principle of conservation of energy and momentum.
Part A: To find the wavelength of the incident photon, we can use the energy conservation equation:
Energy of incident photon = Energy of scattered photon
Since the energies of photons are given by the equation E = hc/λ, where h is Planck's constant, c is the speed of light, and λ is the wavelength, we can write:
hc/λ₁ = hc/λ₂
Where λ₁ is the wavelength of the incident photon and λ₂ is the wavelength of the scattered photon. We are given λ₂ = 0.310 nm. Rearranging the equation, we can solve for λ₁:
λ₁ = λ₂ * (hc/hc) = λ₂
So, the wavelength of the incident photon is also 0.310 nm.
Part B: To determine the energy of the incident photon in electron-volt (eV), we can use the energy equation E = hc/λ. Substituting the given values, we have:
E = (6.626 × 10⁻³⁴ J s * 3.00 × 10⁸ m/s) / (0.310 × 10⁻⁹ m) = 6.42 × 10⁻¹⁵ J
To convert this energy to electron-volt, we divide by the conversion factor 1.6 × 10⁻¹⁹ J/eV:
E = (6.42 × 10⁻¹⁵ J) / (1.6 × 10⁻¹⁹ J/eV) ≈ 40.1 eV
So, the energy of the incident photon is approximately 40.1 eV.
Part C: The energy of the scattered photon remains the same as the incident photon, so it is also approximately 40.1 eV.
Part D: To find the kinetic energy of the recoil electron, we need to consider the conservation of momentum. Since the electron is initially at rest, its initial momentum is zero. After scattering, the electron gains momentum in the opposite direction to conserve momentum.
Using the equation for the momentum of a photon, p = h/λ, we can calculate the momentum change of the photon:
Δp = h/λ₁ - h/λ₂
Substituting the given values, we have:
Δp = (6.626 × 10⁻³⁴ J s) / (0.310 × 10⁻⁹ m) - (6.626 × 10⁻³⁴ J s) / (0.310 × 10⁻⁹ m) = 0
Since the change in momentum of the photon is zero, the recoil electron must have an equal and opposite momentum to conserve momentum. Therefore, the kinetic energy of the recoil electron is zero eV.
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Explain the photoelectric effect. Again, diagrams are important
to the explanation.
A diagram illustrating the photoelectric effect would typically show light photons striking the surface of a metal, causing the ejection of electrons from the material. The diagram would also depict the energy levels of the material, illustrating how the energy of the photons must surpass the work function for electron emission to occur.
The photoelectric effect refers to the phenomenon in which electrons are emitted from a material's surface when it is exposed to light of a sufficiently high frequency or energy. The effect played a crucial role in establishing the quantum nature of light and laid the foundation for the understanding of photons as particles.
Here's a simplified explanation of the photoelectric effect:
1. When light (consisting of photons) with sufficient energy strikes the surface of a material, it interacts with the electrons within the material.
2. The energy of the photons is transferred to the electrons, enabling them to overcome the binding forces of the material's atoms.
3. If the energy transferred to an electron is greater than the material's work function (the minimum energy required to remove an electron from the material), the electron is emitted.
4. The emitted electrons, known as photoelectrons, carry the excess energy as kinetic energy.
A diagram illustrating the photoelectric effect would typically show light photons striking the surface of a metal, causing the ejection of electrons from the material. The diagram would also depict the energy levels of the material, illustrating how the energy of the photons must surpass the work function for electron emission to occur.
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a A simple refractor telescope has an objective lens with a focal length of 1.6 m. Its eyepiece has a 3.80 cm focal length lens. a) What is the telescope's angular magnification?
The telescope's angular magnification is approximately -42.11, indicating an inverted image.
Angular magnification refers to the ratio of the angle subtended by an object when viewed through a magnifying instrument, such as a telescope or microscope, to the angle subtended by the same object when viewed with the eye. It quantifies the degree of magnification provided by the instrument, indicating how much larger an object appears when viewed through the instrument compared to when viewed without it.
The angular magnification of a telescope can be calculated using the formula:
Angular Magnification = - (focal length of the objective lens) / (focal length of the eyepiece)
Given:
Focal length of the objective lens (f_objective) = 1.6 mFocal length of the eyepiece (f_eyepiece) = 3.80 cm = 0.038 mPlugging these values into the formula:
Angular Magnification = - (1.6 m) / (0.038 m)
Simplifying the expression:
Angular Magnification ≈ - 42.11
Therefore, the angular magnification of the telescope is approximately -42.11. Note that the negative sign indicates an inverted image.
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