The correct answer is A. After the puck is hit, the velocity of the center of mass of the hockey player-puck system is equal to the velocity of the hockey puck.
We can assume that there is no friction in the given problem.
Therefore, the total momentum of the system remains constant.
It implies that if the hockey player and the puck are at rest, their total momentum will be zero.
After the player hits the puck, they move together as one system.
As the player hits the puck, he exerts a force on the puck in a particular direction.
The puck moves in the same direction as that of the player with the same speed but opposite in direction.
Therefore, the puck’s velocity is equal to that of the player but in the opposite direction.
Since the puck is light in weight and moves with a high velocity, it has a higher kinetic energy than the player does.
It means that the puck moves faster than the player.
Therefore, the velocity of the center of mass of the hockey player-puck system is equal to the velocity of the hockey puck.
The velocity of the player is equal to the velocity of the puck, but in the opposite direction.
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Answer: Equal to the original velocity of the hockey player
Explanation: Khan
R1-1K VS D1 is an ideal diode. Circuit is same with the preceding 2 questions. 3) Identify Vout if VS - 5 Sin (2πft) b) Please draw the input and output waveforms D1 ww ő
(a) Vout is determined by the diode equation and the input voltage VS.
(b) Plot the input waveform VS as a sinusoidal waveform and determine the corresponding output waveform Vout based on the diode characteristics and circuit configuration.
What is the output voltage Vout in a circuit with an ideal diode D1 and a sinusoidal input voltage VS = 5*sin(2πft)?(a) The output voltage Vout can be identified by analyzing the circuit considering the diode D1 as an ideal diode and applying the appropriate diode equation based on the voltage input VS.
(b) To draw the input and output waveforms, plot the voltage waveform of VS, which is a sinusoidal waveform with a frequency f, and then determine the corresponding output waveform Vout based on the diode characteristics and circuit configuration.
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A group of PHY221 students were wondering how they could increase the period of an oscillating LC circuit the most. What do you recommend? Group of answer choices
a. Double the capacitance. b. Half the maximum charge on the capacitor. c. Half the maximum current through the inductor. d. Double the inductance.
e. Double both the inductance and the capacitance.
The recommended option to increase the period of an oscillating LC circuit the most is to (d) double the inductance.
Increasing the inductance in an LC circuit will result in a longer period of oscillation. The period of an LC circuit is given by the formula T = 2π√(LC), where L is the inductance and C is the capacitance. By doubling the inductance (L), the overall value inside the square root will increase, leading to a larger value for T and thus a longer period.
Other options, such as doubling the capacitance (a) or doubling both the inductance and the capacitance (e), may also have some effect on the period, but increasing the inductance alone will have the most significant impact. Halving the maximum charge on the capacitor (b) or halving the maximum current through the inductor (c) will not directly affect the period of the oscillation in an LC circuit.
Therefore, to maximize the increase in period, the recommended choice is to double the inductance (d).
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If the weight force of an object is given by F=mg, what is the combined weight force of two of these objects with mass my and my? The solution to this will simply be the sum of the two weight forces gx (mı + m2). Notice that this is an algebraic expression in three variables, the expression can be written expanded as gmı +9m2. In this solution, we want to enter the expression in such a way that it is clear and unambiguous. Notice that if we have a function gevaluated at a point mı + m2 this would be expressed as g(mı + m2). How does STACK tell the difference? One is an example of multiplication and the other is a function evaluation. Multiplication requires the use of the star * to tell STACK to multiply the two elements Enter the correct answer of g* (m_1 + m_2) in the box below. Notice that STACK sees three variables here, g, m, and m2. Now, try and enter g (m_1 + m_2). Notice that this time, STACK sees 2 variables, me and my, but it thinks that gis a function, as you have written it using STACK function syntax. One important thing to note, it doesn't actually matter the order you enter an expression, STACK is smart enough to tell when (most) things are equivalent. For example, our solution is gx (ma + m2), but an answer of g*m_1 + g*m_2 would also be correct. Check
The combined weight force of two objects with masses m1 and m2 can be expressed as g * (m1 + m2).
:
The weight force of an object is given by the formula F = mg, where F represents the weight force, m is the mass of the object, and g is the acceleration due to gravity. To find the combined weight force of two objects with masses m1 and m2, we can simply add their individual weight forces.
Therefore, the combined weight force can be written as g * (m1 + m2), where g is the acceleration due to gravity and (m1 + m2) represents the sum of the masses of the two objects.
It is important to use the star (*) symbol in the expression g * (m1 + m2) to indicate multiplication and avoid confusion with function evaluation in STACK.
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Learning Task #1 Solve the given problem 1. If you were on board a craft and travel at 0.9 c and were 6 feet tall, how tall would you appear to the earth's reference frame? 2. A ship parked at a street corner is 12 m long. It then cruises around the block and moves at 0.8c past someone standing on the street corner. The street corner observer measures the ship to have length of. 3. The Star Wars Spacecraft Tie Fighter flies at a speed of 0.8 c with respect to the Earth. Luke Skywalker determines the time interval between the two events on earth is 20h. What is the time interval for the Tie Fighter?
The time interval for the Tie Fighter would be approximately 12.81 hours according to Luke Skywalker's observation. According to the theory of special relativity, the apparent length of an object moving at relativistic speeds appears shorter when observed from a stationary reference frame. This phenomenon is known as length contraction.
The formula to calculate the apparent length is:
L' = L * [tex]\sqrt(1 - v^2/c^2)[/tex]
where L' is the apparent length, L is the proper length (rest length), v is the velocity of the object, and c is the speed of light.
In this case, the craft is traveling at 0.9 times the speed of light (0.9c). If the person on board the craft has a height of 6 feet, we can calculate the apparent height as follows:
L' = 6 feet *[tex]\sqrt(1 - (0.9c)^2/c^2)[/tex]
= 6 feet * [tex]\sqrt(1 - 0.81)[/tex]
= 6 feet * [tex]\sqrt(0.19)[/tex]
≈ 2.33 feet
Therefore, the person on board the craft would appear to have a height of approximately 2.33 feet in the Earth's reference frame.
Similar to the previous question, when an object moves at relativistic speeds, its length appears shorter when observed from a stationary reference frame. Using the same length contraction formula:
L' = L *[tex]\ \sqrt(1 - v^2/c^2)[/tex]
In this case, the ship is moving at 0.8 times the speed of light (0.8c), and its proper length (rest length) is 12 meters. The observer on the street corner measures the apparent length as:
L' = 12 meters * [tex]\sqrt(1 - (0.8c)^2/c^2)[/tex]
= 12 meters * [tex]\sqrt(1 - 0.64)[/tex]
= 12 meters *[tex]\sqrt(0.36)[/tex]
≈ 8.31 meters
Therefore, the observer on the street corner would measure the ship to have an apparent length of approximately 8.31 meters.
According to the theory of special relativity, time dilation occurs when an object moves at relativistic speeds. Time dilation causes time to appear to pass more slowly for moving objects compared to stationary objects. The formula to calculate the time dilation is:
t' = t * [tex]\sqrt(1 - v^2/c^2[/tex])
where t' is the observed time interval, t is the proper time (rest time), v is the velocity of the object, and c is the speed of light.
In this case, the Tie Fighter is traveling at 0.8 times the speed of light (0.8c), and the time interval on Earth is 20 hours. We can calculate the time interval for the Tie Fighter as follows:
t' = 20 hours * [tex]\sqrt(1 - (0.8c)^2/c^2)[/tex]
= 20 hours * [tex]\sqrt(1 - 0.64)[/tex]
= 20 hours *[tex]\sqrt(0.36)[/tex]
≈ 12.81 hours
Therefore, the time interval for the Tie Fighter would be approximately 12.81 hours according to Luke Skywalker's observation.
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Contemporary American society has a variety of markers of entrance into adulthood. 2
There are legal definitions: at 17 , young people may enlist in the armed forces; at age 18 , in most states, they may marry without their parents' permission; at 18 to 21 (depending on the state), they may enter into binding contracts. 3
Using sociological definitions, people may call themselves adults when they are self-supporting or have chosen a career, have married or formed a significant relationship, or have founded a family. 4
There are also psychological definitions. 5
Cognitive maturity is often considered to correspond with the capacity for abstract thought. 6
Emotional maturity may depend on such achievements as discovering one's identity, becoming independent of parents, developing a system of values, and forming relationships. 7
Some people never leave adolescence, no matter what their chronological age. 1. The main idea is expressed in sentence A. 1 . B. 2 . C. 3 . 2. The paragraph is made up of a series of A. types of adults. B. definitions of adulthood. C. stages of adulthood. 3. The second major detail of the paragraph is introduced in sentence A. 3 . B. 4 . C. 5 . 4. Sentence 4 contains A. the main idea. B. a major supporting detail. C. a minor supporting detail. 5. Sentences 5-7 contain A. major supporting details. B. minor supporting details.
1. The main idea is expressed in sentence C. 3.2. The paragraph is made up of a series of B. definitions of adulthood.3. The second major detail of the paragraph is introduced in sentence A. 3.4. Sentence 4 contains C. a minor supporting detail.5. Sentences 5-7 contain A. major supporting details.Explanation:A paragraph has one main idea, and it is usually stated in the first sentence, which is called the topic sentence. The remaining sentences in a paragraph provide supporting details that explain or illustrate the main idea.
The paragraph you have posted follows this structure.According to the paragraph, there are several ways to define adulthood, such as legal, sociological, and psychological definitions. The main idea is expressed in sentence 3: "Using sociological definitions, people may call themselves adults when they are self-supporting or have chosen a career, have married or formed a significant relationship, or have founded a family.
"This paragraph is made up of a series of definitions of adulthood, so the answer is B. definitions of adulthood.The second major detail is introduced in sentence 3: "Using sociological definitions, people may call themselves adults when they are self-supporting or have chosen a career, have married or formed a significant relationship, or have founded a family."So, the answer is a minor supporting detail.Sentences 5-7 contain major supporting details that explain emotional and cognitive maturity, so the answer is A. major supporting details.
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Calculate the acceleration d. Earth through d. Gravity d. Sun: a = = y= 6,67E-11 m³/kg/s², ms=1,99e30 kg, c=299792458 m/s, r = c. 8 min y.ms.me/r²/mE
To calculate the acceleration caused by the Sun, we need to know the distance (r) from the Sun to the object. The value "c. 8 min" mentioned in your question seems to indicate the time it takes for light to travel from the Sun to the object, which is approximately 8 minutes. However, we also need the mass of the object (mE) for the calculation.
To calculate the accelerations due to gravity caused by Earth and the Sun, we can use the formula:
a = G * M / r^2
where:
G is the gravitational constant (6.67 x 10^-11 m³/kg/s²)
M is the mass of the celestial body (Earth or Sun)
r is the distance from the center of the celestial body to the object experiencing the acceleration
For Earth:
M = 5.97 x 10^24 kg (mass of Earth)
r = radius of Earth (approximately 6,371,000 m)
aEarth = (6.67 x 10^-11 m³/kg/s²) * (5.97 x 10^24 kg) / (6,371,000 m)^2
For the Sun:
M = 1.99 x 10^30 kg (mass of Sun)
r = average distance from the Sun to the object (varies depending on the distance)
Note: If you can provide the distance (r) and the mass of the object (mE), I can help you calculate the acceleration due to the Sun.
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A vertical triangular gate with top base horizontal and 1.5 m wide is 3 mhigh. It is submerged in oil having specific gravity of 0.82 with its top base submerged to a depth of 2 m. Determine the magnitude and location of the total hydrostatic pressure (measured from the bottom of the gate) acting on one side of the gate.
The magnitude of the total hydrostatic pressure is 3.6171 kN/m² or 28.34 kN/m². The location of the total hydrostatic pressure is located 0.67 m above the bottom of the gate, which is determined by calculating the centroid of the triangular gate.
To determine the magnitude of the total hydrostatic pressure, we need to calculate the pressure at different points on the gate and then integrate it over the surface area. The pressure at a point in a fluid is given by the formula: P = ρgh, where P is the pressure, ρ is the density of the fluid, g is the acceleration due to gravity, and h is the depth of the point from the surface.
In this case, the density of the oil is given as 0.82 times the density of water, and the depth from the top base of the gate to the point of interest is 2 m. So, the pressure at that point is P = 0.82 * 1000 kg/m³ * 9.8 m/s² * 2 m = 1607.6 N/m². To find the total hydrostatic pressure, we need to integrate this pressure over the surface area of the gate. The surface area of a triangular gate is (1/2) * base * height. Plugging in the values, we get (1/2) * 1.5 m * 3 m = 2.25 m². Integrating the pressure over this surface area, we get (1607.6 N/m² * 2.25 m²) = 3617.1 N = 3.6171 kN. Therefore, the magnitude of the total hydrostatic pressure is 3.6171 kN/m² or 28.34 kN/m² (rounded to two decimal places).
The location of the total hydrostatic pressure is located 0.67 m above the bottom of the gate. This can be determined by calculating the centroid of the triangular gate. The centroid of a triangle is located one-third of the distance from the base to the top. In this case, the distance from the base to the top is 3 m, so one-third of that is 1 m. Therefore, the location of the total hydrostatic pressure is 1 m + 2 m (depth from the top base) = 3 m, which is 0.67 m above the bottom of the gate.
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For a technical application, an electrical engineer need to create solenoid using copper wire with diameter -0.500 mm. The resistance of the solenoid needs to bt 1.700 and the magnetic field the solenol with a current of 3.50 A should be 5.90 x 10T. Assume the resistance does not change significantly with temperature, and the radius of the solenoid 1.00 cm (Uwe - 170x100 m for the resistivity of copper) () How many turns of wire does the electrical engineer need? (b) Determine the required length inom) of the solenoid
(a) The electrical engineer needs approximately 539 turns of wire for the solenoid. (b) The required length of the solenoid is approximately 19.2 meters.
To determine the number of turns required for the solenoid, we can use the formula for the resistance of a solenoid: R = (μ₀ * N² * A) / l, where R is the resistance, μ₀ is the permeability of free space, N is the number of turns, A is the cross-sectional area, and l is the length of the solenoid.
Given that the resistance needs to be 1.700 Ω and the radius of the solenoid is 1.00 cm, we can calculate the cross-sectional area as A = π * r², where r is the radius.
Using the resistivity of copper (ρ = 1.70 x 10⁻⁸ Ω·m), we can calculate the length of the solenoid using the formula R = (ρ * l) / A.
By rearranging the formulas and solving the equations simultaneously, we find that the number of turns needed is approximately 539 turns and the required length of the solenoid is approximately 19.2 meters.
Therefore, the electrical engineer needs approximately 539 turns of wire and a solenoid length of approximately 19.2 meters for the technical application.
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With a hydraulic press, you want to lift a 1250 kg vehicle. If the area of the smaller plunger is 15 cm^2, and the largest plunger is 3 m^2, find the force to be applied.
The force to be applied to the larger plunger is 2,450,000 Newtons.
The force to be applied can be calculated using Pascal's law, which states that the pressure exerted on a fluid in a closed system is transmitted equally in all directions. In this case, the pressure applied to the smaller plunger will create an equal pressure on the larger plunger.
The pressure P exerted on the fluid can be determined using the equation:
P = F / A
where P is the pressure, F is the force applied, and A is the area of the plunger.
Since the pressure is transmitted equally, the pressure on the smaller plunger is the same as the pressure on the larger plunger:
P₁ = P₂
F₁ / A₁ = F₂ / A₂
To find the force F₂ applied on the larger plunger, we can rearrange the equation:
F₂ = (F₁ / A₁) * A₂
Given the values:
A₁ = 15 cm² = 0.0015 m²
A₂ = 3 m²
We need to convert the area of the smaller plunger to square meters to maintain consistent units. Now we can substitute the values into the equation:
F₂ = (F₁ / 0.0015) * 3
To lift the 1250 kg vehicle, we need to exert a force equal to the weight of the vehicle, which is:
F₁ = m * g
where m is the mass of the vehicle and g is the acceleration due to gravity (approximately 9.8 m/s²).
Substituting the values:
F₁ = 1250 kg * 9.8 m/s²
Now we can calculate the force applied to the larger plunger:
F₂ = (1250 kg * 9.8 m/s² / 0.0015) * 3
Simplifying the expression:
F₂ = 2,450,000 N
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A cart rolls with negligible friction down a ramp that is inclined at an θ=30∘θ=30∘ above level ground. It is released from rest at a height h=46h=46 cm. What we want to do is to figure out how fast the cart will go when it reaches the bottom of the ramp.
x
x
Let's begin by establishing the equations that model the motion of the cart. Recall that we are dealing here with an example of constantly accelerated motion. Let the xx axis point down the ramp and let x=0x=0 correspond to the starting position of the cart. What are the equations that describe the motion of the cart? [These should incorporate that both the initial position and velocity are zero. Use 'g' to indicate the gravitational acceleration, 'B' to indicate the angle, and 't' for the time variable. To write a function like sin(θ)sin(θ) you should write `sin(B)'.]
v(t) =
x(t) =
B.) Next, we need to establish our coordinates a bit more. Let x=xbottomx=xbottom be the as-yet unknown coordinate at the bottom of the ramp. What is the value of xbottomxbottom? [Tip: Think about trigonometry, where the ground and the ramp form two sides of a right triangle.]
C.)
After reaching the bottom of the ramp, the cart smoothly slides onto another ramp, maintaining the same speed that it had at the bottom of the first ramp. The second ramp is tilted 36∘∘ above the level ground. How far up the ramp does the cart go?
To determine how fast the cart will go when it reaches the bottom of the ramp, we can use the equations of motion for constant acceleration. Since the initial position and velocity are both zero,
We can use the following equations:
v(t) = gt sin(B)
x(t) = (1/2)gt^2 sin(B) where v(t) represents velocity of the cart at time t, x(t) represents its position at time t, g is the acceleration due to gravity, and B is the angle of the ramp (30 degrees in this case).To find the value of xbottom, the coordinate at the bottom of the ramp, we can consider the right triangle formed by the ground and the ramp. Using trigonometry, we can relate the height h to the distance xbottom:
h = xbottom sin(B)
Solving for xbottom, we have:
xbottom = h / sin(B)
After reaching the bottom of the ramp, the cart slides onto another ramp while maintaining the same speed. This means that the cart will continue to move with the velocity it had at the bottom of the first ramp. The second ramp is tilted at an angle of 36 degrees. To determine how far up the second ramp the cart will go, we can use the equation:
xsecond = vbottom^2 / (2g sin(C))
where xsecond represents the distance up the second ramp, vbottom is the velocity at the bottom of the first ramp, g is the acceleration due to gravity, and C is the angle of the second ramp (36 degrees in this case).
By substituting the known values into the equation, we can calculate the distance xsecond.
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Show that y(x, t) = ym exp(i(kx ±wt)) is a solution of the wave equation dx² where vw/k. (10 pts) = 1 d²y v² dt²
The given wave equation is:d²y/dt² = v²d²y/dx²We can prove that y(x,t) = ym exp(i(kx ± wt)) is a solution of the given wave equation as follows:Taking the first derivative of y(x t) with respect to time t, we get:dy(x,t)/dt = ± i w ym exp(i(kx ± wt))Taking the second derivative of y(x t) with respect to time t, we get:d²y(x,t)/dt² = -w² ym exp(i(kx ± wt))Similarly, taking the second derivative of y(x t) with respect to x, we get:d²y(x,t)/dx² = -k² ym exp(i(kx ± wt))Substituting these values in the given wave equation, we get:-w² ym exp(i(kx ± wt)) = v² (-k² ym exp(i(kx ± wt)))Dividing both sides by ym exp(i(kx ± wt)), we get:w²/v² = k²This satisfies the condition that vw/k. Therefore, we have proved that y(x,t) = ym exp(i(kx ± wt)) is a solution of the wave equation dx² where vw/k.
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Light of wavelength to in a vacuum has a wavelength of 438 nm in water and a wavelength of 390 nm in benzene. (a) What is the wavelength do? (b) Using only the given wavelengths, determine the ratio of the index of refraction of benzene to that of water. (n water = 1.333 and n benzene = 1.501)
a)the wavelength of light in air is approximately 438.88 nm. b) the ratio of the index of refraction of benzene to that of water is approximately 0.888.
To solve this problem, we can use Snell's law, which relates the angles and indices of refraction of light as it passes through different media.
Snell's law is given by:
n₁ * sin(θ₁) = n₂ * sin(θ₂),
where n₁ and n₂ are the indices of refraction of the two media, and θ₁ and θ₂ are the angles of incidence and refraction, respectively.
Wavelength in vacuum, λ₀ = 438 nm
Wavelength in water, λ₁ = 390 nm
Wavelength in benzene, λ₂ = ?
(a) To find the wavelength of light in air, we can use the formula:
λ₂ = λ₁ * n₂ / n₁,
where n₁ and n₂ are the indices of refraction of water and benzene, respectively.
Using the given values:
λ₂ = 390 nm * 1.501 / 1.333
λ₂ = 438.88 nm
(b) To determine the ratio of the index of refraction of benzene to that of water, we can use the formula:
n₂ / n₁ = λ₁ / λ₂,
where n₁ and n₂ are the indices of refraction of water and benzene, respectively, and λ₁ and λ₂ are the wavelengths in the two media.
Using the given values:
n₂ / n₁ = 390 nm / 438.88 nm
n₂ / n₁ ≈ 0.888
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A quality characteristic has a design specification (in cm.) of 0.200 ± 0.04. If the actual process value of the quality characteristic is at the boundary of the tolerance on either side, the product will require a repair of $40. Find the value of k and state the Taguchi loss function. What is the loss associated with x = 0.208? What are the economic design specifications if the cost of inspection and adjustment is $7.50?
The value of k is 3, and the Taguchi loss function represents the economic loss associated with deviations from the target value.
In the context of quality control, the value of k represents the number of standard deviations that can fit within the tolerance range. In this case, the tolerance range is ±0.04 cm, which means it spans a total of 0.08 cm. To find the value of k, we divide the total tolerance by six times the standard deviation. Since the tolerance is 0.08 cm and the standard deviation is 0.04 cm, we have k = 0.08 / (6 * 0.04) = 3.
The Taguchi loss function is an economic model that quantifies the cost associated with deviations from the target value or specifications. It states that the loss increases quadratically as the actual value deviates from the target value. In this case, the target value is 0.200 cm, and any deviation from this target value will result in an economic loss.
To calculate the loss associated with a specific value, we use the formula Loss = k * (deviation from target)^2. For x = 0.208 cm, the deviation from the target is 0.208 - 0.200 = 0.008 cm. Plugging this value into the loss formula, we have Loss = 3 * (0.008)^2 = $0.00192.
Regarding the economic design specifications, they refer to the optimal range or target value that minimizes the total cost considering inspection and adjustment expenses. To determine the economic design specifications, the cost of inspection and adjustment ($7.50) needs to be taken into account, along with other factors such as the Taguchi loss function, production costs, and customer requirements.
Understanding the concept of Taguchi loss function and its application in quality control helps organizations make informed decisions regarding product specifications, target values, and associated economic costs. By considering the trade-off between the cost of deviations from the target value and the cost of inspection and adjustment, businesses can optimize their processes and minimize losses. Additionally, incorporating customer preferences and market demands into the economic design specifications can enhance customer satisfaction and competitiveness.
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Null Zero is a hypothetical planet. If it has a mass of 6.55 X10²5 kg and a radius of 5.84 X106 m, find a) (2 points) the acceleration of gravity and b) (3 points) the escape velocity at its surface.
a) The acceleration of gravity on the hypothetical planet Null Zero is approximately 1.97 m/s². b) The escape velocity at the surface of Null Zero is approximately 4.97 km/s.
a) The acceleration of gravity can be calculated using the formula:
g = G * (M / r²),
where g is the acceleration of gravity, G is the gravitational constant (approximately 6.67 × 10^-11 N m²/kg²), M is the mass of the planet, and r is the radius of the planet.
Plugging in the given values:
g = (6.67 × 10^-11 N m²/kg²) * (6.55 × 10^25 kg) / (5.84 × 10^6 m)²,
g ≈ 1.97 m/s².
b) The escape velocity at the surface of a planet can be calculated using the formula:
v = √(2 * G * M / r),
where v is the escape velocity, G is the gravitational constant, M is the mass of the planet, and r is the radius of the planet.
Plugging in the given values:
v = √(2 * (6.67 × 10^-11 N m²/kg²) * (6.55 × 10^25 kg) / (5.84 × 10^6 m)),
v ≈ 4.97 km/s.
Therefore, the acceleration of gravity on Null Zero is approximately 1.97 m/s², and the escape velocity at its surface is approximately 4.97 km/s.
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A conducting coil, with current (t) = 4.40 -0.0250t sin(120xt), with / in amperes and t in seconds, is placed next to a second coll, end to end. At t = 0.840 s, a lab tech measures the emf across the second coil, and the result is -3.70 V. What is the mutual Inductance (in mH) of the colls? mH
18.5 mH is the mutual Inductance (in mH) of the colls.
Mutual inductance (M) can be determined using Faraday's law of electromagnetic induction. According to Faraday's law, the induced emf (ε₂) in the second coil is given by ε₂ = -M(dI₁/dt), where dI₁/dt is the rate of change of current in the first coil.
Given that ε₂ = -3.70 V and the current in the first coil is I₁(t) = 4.40 - 0.0250t sin(120t), we can differentiate I₁(t) with respect to time to find dI₁/dt.
Differentiating I₁(t), we get dI₁/dt = -0.0250 sin(120t) - 0.0250t(120cos(120t)).
Substituting the given values at t = 0.840 s, we can calculate the mutual inductance:
ε₂ = -M(dI₁/dt)
-3.70 V = -M[(-0.0250 sin(120(0.840))) - (0.0250(0.840)(120cos(120(0.840))))]
Solving the equation, we find M ≈ -18.5 mH.
Therefore, the mutual inductance between the coils is approximately -18.5 mH.
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Find Vn, Vout, and lout for the circuit shown below. Assume that the op amp is ideal. 6V 3ΚΩ www 1k02 www +5V 1.5mA -5V 2. Find Vn, Vout, and lout for the circuit shown below. Assume that the op amp is ideal. 6V 1k0 www 2.5KQ www +5V 3mA 2kQ www ΣΚΩ 4mA 5V 2k0 ww 8V 10k(2 -5V lout www-11 lout ww-11 Vou 5ΚΩ Vout ΣΚΩ
The voltage at the inverting terminal is 7.5 V. V out is -12.5 V. The current flowing through R4 is 0.5 mA.
Given that Vn, Vout, and lout for the circuit shown below and op amp is ideal.In the circuit, current I2 flows through the 2.5 kΩ resistor.
Therefore, the voltage drop across the 2.5 kΩ resistor is given by,
Vn = I2 x R2Vn = 3 mA x 2.5 kΩ = 7.5 V
Therefore, the voltage at the inverting terminal is 7.5 V.
Since op-amp is assumed to be ideal, no current flows into the inverting and non-inverting terminals.
Therefore, current through R3 is given by,
I3 = (Vn - Vout) / R3=> Vout = Vn - I3 x R3=> Vout = 7.5 V - 4 mA x 5 kΩ=> Vout = - 12.5 V
Therefore, Vout is -12.5 V.
Let's calculate the current flowing through R4:
This current will also flow through the 5 kΩ resistor.
Let lout be the current flowing through R4.
Therefore, current through the 5 kΩ resistor is also lout.
Now, I4 + lout = I3=> I4 = I3 - lout=> I4 = 4 mA - lout
Also, I4 = (5 V - Vout) / R4=> 4 mA - lout = (5 V - (-12.5 V)) / 5 kΩ=> 4 mA - lout = 3.5 mA=> lout = 0.5 mA
Therefore, lout is 0.5 mA.
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The University of South Alabama has a spring home game football. If a student pro- duces a sound with an intensity level of 120 dB. How many students would be required to reach the intensity level of 160 dB? Assuming each student produces an identical intensity level
To reach an intensity level of 160 dB, the number of students needed can be calculated by comparing the intensity levels. If a single student produces a sound at 120 dB, the number of students required to reach 160 dB can be determined.
The decibel scale is logarithmic, meaning that every increase of 10 dB represents a tenfold increase in intensity. In this case, the difference between 160 dB and 120 dB is 40 dB. Since each student produces an identical intensity level, we can divide this difference by the intensity level of a single student (120 dB) to find the number of students required.
40 dB / 10 dB = 4
Therefore, to reach an intensity level of 160 dB, four students would be required. Each additional student would contribute an additional 10 dB to the total intensity level. It's important to note that this calculation assumes an ideal scenario with no loss or interference in sound propagation, which may not be entirely realistic in practice.
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Curves A point mass has coordinates x(t) = 3 cost and y(t)=2 sin(0.51) What is its position vector r(/)? What is its velocity vector v()? What is its acceleration vector a(/)? What is its displacement Ar over the interval from t=0 to 1= ? An object has an acceleration a= = 4/1 m/s² Assuming r(0) = 0 and v(0) = 0 What is v(t)? What is r(t)?
Answer:
Explanation:
To find the position vector, velocity vector, and acceleration vector of the point mass, we can differentiate the given parametric equations with respect to time.
Given:
x(t) = 3cos(t)
y(t) = 2sin(0.51)
Position vector r(t):
The position vector r(t) is given by combining the x and y components:
r(t) = x(t)i + y(t)j
= (3cos(t))i + (2sin(0.51))j
Velocity vector v(t):
The velocity vector v(t) is obtained by taking the derivatives of x(t) and y(t) with respect to time:
v(t) = dx(t)/dt * i + dy(t)/dt * j
= -3sin(t)i + 2cos(0.51)j
Acceleration vector a(t):
The acceleration vector a(t) is obtained by taking the derivatives of v(t) with respect to time:
a(t) = dv(t)/dt
= -3cos(t)i - 2sin(0.51)j
Displacement Ar over the interval from t=0 to t=1:
To find the displacement, we integrate the velocity vector with respect to time over the given interval:
Ar = ∫[v(t) dt] (from 0 to 1)
Now, moving on to the second part:
Given:
a = 4/√t m/s²
r(0) = 0
v(0) = 0
Velocity v(t):
To find v(t), we integrate the given acceleration with respect to time:
v(t) = ∫[a dt]
= ∫[(4/√t) dt]
= 8√t + C
Since v(0) = 0, we can solve for the constant C:
v(0) = 8√0 + C
0 = 0 + C
C = 0
Therefore, v(t) = 8√t m/s
Position r(t):
To find r(t), we integrate the velocity function obtained in step 5 with respect to time:
r(t) = ∫[v(t) dt]
= ∫[(8√t) dt]
= (16/3)t^(3/2) + D
Since r(0) = 0, we can solve for the constant D:
r(0) = (16/3)(0)^(3/2) + D
0 = 0 + D
D = 0
Therefore, r(t) = (16/3)t^(3/2)
Please note that the symbols used (/ and √) were interpreted as division and square root, respectively. If there is any ambiguity in the provided notation, please clarify, and I will be happy to assist you further.
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A spring with a spring constant of 5.2 kg/s2 is attached to ceiling hook such that it hangs down with gravity. With no mass attached the spring is 15 cm long. If a mass of 150 g is attached to the spring and pulled down so that the spring is now extended to 62 cm what will be the acceleration of the mass once released?
Give the magnitude of the acceleration (i.e. do not worry about the sign) to 3 s.f.
The magnitude of acceleration of a mass attached to a spring, we can use Hooke's Law and Newton's second law. Hooke's Law states that force by a spring proportional to displacement from equilibrium position.
Newton's second law states that the force acting on an object is equal to its mass multiplied by its acceleration. By equating these forces and solving for acceleration, we can determine the magnitude of the acceleration.
Given that the spring constant (k) is 5.2 kg/s^2, the unstretched length of the spring (x_0) is 15 cm, and the stretched length of spring (x) is 62 cm, we can calculate the displacement (Δx) of the spring by subtracting the unstretched length from the stretched length (Δx = x - x_0). Using Hooke's Law, we can calculate the force (F) exerted by the spring using the equation F = kΔx. We convert the mass (m) of 150 g to kg (0.150 kg) and use Newton's second law (F = ma) to solve for acceleration (a). The magnitude of the acceleration is obtained by taking absolute value of the calculated acceleration.
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A 0.31 kg baseball moving horizontally at 41 m/s is hit back in the direction of the pitcher at an upward angle of 30° and at a speed of 53 m/s. Find the impulse given to the ball. Include a labelled diagram. (A:6, 1:6, C4) Marking Scheme (A:6,1:6,C:4) • 4C for labelled diagram • 6A for showing your work • 21 for showing your work • 21 for direction of the impulse • 21 for magnitude of the impulse
Let's begin by understanding the terms involved in the question.Impulse is the force that acts on an object for a specific period. It is defined as the change in momentum (p) of an object. Labelled diagram that has specific labelling for various parts or components is known as a labelled diagram.]baseball is a ball that is used in baseball games, and it weighs around 0.31 kg.
DirectionDirection refers to the path in which an object moves or the way in which an object moves.Now let's move towards the solution of the given problem.SolutionStep 1: Find the impulse given to the ball.The formula to calculate impulse is given as:I = F × t,Where, I is the impulse given to the ballF is the force applied to the ballt is the time period for which force is applied given the mass of the baseball is 0.31 kg. Therefore, the momentum of the baseball is given as:p = mv, where m is the mass of the ball and v is the velocity of the ball.p = 0.31 kg × 41 m/sp = 12.71 kg m/sThe final momentum of the ball is given as:p = mv, where m is the mass of the ball and v is the final velocity of the ball.p = 0.31 kg × 53 m/sp = 16.43 kg m/sChange in momentum = Final momentum - Initial momentumΔp = pfinal - pinitialΔp = 16.43 kg m/s - 12.71 kg m/sΔp = 3.72 kg m/sThe angle between the initial direction of the ball and the final direction of the ball is 30°.So, the impulse given to the ball will be in the direction perpendicular to this angle and is calculated using the following formula:Impulse = Δp × sinθWhere, θ = 30°Impulse = 3.72 kg m/s × sin30°Impulse = 3.72 kg m/s × 0.5Impulse = 1.86 kg m/sNow, we have found the magnitude of impulse, which is 1.86 kg m/s. We will find the direction of impulse in the next step.Step 2: Draw a labelled diagram of the given situation.A diagram of the given situation is shown below:In the diagram, the initial direction of the ball is in the horizontal direction, while the final direction of the ball is inclined at an angle of 30° with the horizontal. The direction of the impulse is perpendicular to this angle. Therefore, the direction of the impulse is upwards, as shown below:Step 3: Write down the final answer.As per the question, the impulse given to the ball is 1.86 kg m/s, and the direction of the impulse is upwards, as shown in the diagram. Therefore, the final answer is:Impulse = 1.86 kg m/s (upwards)
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10. Inductances of 0.8H and 0.11H are connected in series, fields opposing. If the mutual inductance is 0.2H, the total inductance is: a. 0.15H b. 0.51H c. 0.30H d. 1.02H 11. Determine the resonant frequency of a RC circuit which consists of a 470-ohm resistor and a 120 uF capacitor. a. 2.82kHz b. 2.82 Hz c. 2.28kHz d. 2.28 Hz
Inductance is the tendency of an electrical conductor to oppose a change in the electric current flowing through it. L is used to represent the inductance, and Henry is the SI unit of inductance. The total inductance of the series connection with opposing fields and a mutual inductance of 0.2H is 0.71H.
The resonant frequency of the RC circuit with a 470-ohm resistor and a 120 uF capacitor is 2.82 Hz.
10. When inductances are connected in series with opposing fields, the total inductance is given by the difference between the individual inductances:
total inductance = (L1 + L2) - 2M
Given the values of L1 = 0.8H, L2 = 0.11H, and M = 0.2H, we can substitute these values into the formula to find the total inductance, which is 0.71H.
11. The resonant frequency of an RC circuit is determined by the values of the resistor and capacitor. The resonant frequency is given by the formula:
resonant frequency = 1 / (2πRC)
Plugging in the values of R = 470 ohms and C = 120 uF (or 120 × 10^(-6) F), we can calculate the resonant frequency, which is 2.82 Hz.
It's important to note that in the calculations above, I've assumed ideal conditions and neglected any parasitic elements or losses in the circuit. In practical scenarios, these factors may affect the actual values and performance of the components.
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A 1.5-V battery is connected to a circuit and puts out a current of 0.45 A. How much power is the battery putting out? 0.30 W
0.68 W
3.3 W
5.0 W
7.4 W
To determine the distance from the starter cable of a car where the magnetic field is less than the Earth's magnetic field, we can use the formula for the magnetic field around a long, straight wire:
B = (μ₀ * I) / (2π * r)
where B is the magnetic field, μ₀ is the permeability of free space (4π × 10^(-7) T·m/A), I is the current in the wire, and r is the distance from the wire.
In this case, we are given the current in the wire as 165 A and we want to find the distance at which the magnetic field is less than 5.00 × 10^(-5) T, which is the Earth's magnetic field.
Rearranging the formula, we can solve for the distance:
r = (μ₀ * I) / (2π * B)
Substituting the values, we can calculate the distance from the wire where the magnetic field is less than the Earth's magnetic field.
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If an air parcel initially at height z = 100m and temperature 10 C is lifted dry adiabatically to a height z = 1500m, what will its temperature be?
When the air parcel is lifted dry adiabatically from a height of 100m to 1500m, its temperature will be approximately 23.72°C.
The dry adiabatic lapse rate is the rate at which the temperature of an air parcel changes as it is lifted or descended adiabatically (without exchange of heat with the surroundings). On average, the dry adiabatic lapse rate is approximately 9.8°C per 1000 meters.
In this case, the air parcel is lifted from a height of 100m to 1500m. The difference in height is 1500m - 100m = 1400m.
Using the dry adiabatic lapse rate of 9.8°C per 1000 meters, we can calculate the change in temperature for the given height difference:
Change in temperature = (dry adiabatic lapse rate) * (height difference / 1000)
Change in temperature = 9.8°C/1000m * 1400m/1000
Change in temperature = 13.72°C
To find the final temperature, we need to add the change in temperature to the initial temperature of 10°C:
Final temperature = Initial temperature + Change in temperature
Final temperature = 10°C + 13.72°C
Final temperature = 23.72°C
Therefore, when the air parcel is lifted dry adiabatically from a height of 100m to 1500m, its temperature will be approximately 23.72°C.
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A load is suspended from a steel wire with a radius of 1 mm. The load extends the wire the same amount as heating by 20°С. Find the weight of the load. (Ysteet = 21.6 x 1010 N.m-?
Weight of the load cannot be determined from the given information for the steel wire.
Given, Radius of the steel wire = r = 1 mm = [tex]1 * 10^-3[/tex]m for the weight.
Weight is the force that gravity applies to an object. It is a way to quantify the gravitational force that pulls on an object's mass, and it is frequently expressed in units of pounds (lb) or Newtons (N). Since weight and mass are directly inversely proportional, heavier items will have a bigger mass. An object's weight can change depending on how strong the gravitational field is around it. For instance, because the Moon has weaker gravity than Earth, an object will weigh less there. In physics and engineering, the concept of weight is crucial, particularly when discussing forces, equilibrium, and the behaviour of things in the presence of gravity.
Young's modulus of steel, Ysteel =[tex]21.6 * 10^(10) N/m^2[/tex]Change in temperature, ΔT = 20°CDue to change in temperature, there is increase in length of the wire given as:ΔL = αLΔTwhere, L is original length, α is coefficient of linear expansion. Here, we don't know the value of α.
But we know that the length of wire is extended by the same amount as the length due to the load. Therefore,ΔL = Load induced extension = Length due to change in temperature = αLΔT......(1)Extension of the wire due to load is given as:ΔL = F × L / A × Ysteelwhere, F is force acting on the wire, A is area of cross section of wire.
So, we getF = A × Ysteel × ΔL / L......(2)From equations (1) and (2), we getF = A × Ysteel × αLΔT / L = A × Ysteel × αΔT
Thus, the weight of the load isF = A × Ysteel × αΔTwhere, α is coefficient of linear expansion and A is area of cross section of wire.
However, we are not given with the area of cross section of wire. Therefore, we cannot calculate the weight of the load. Answer: Weight of the load cannot be determined from the given information.
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On planet #2, you launch a projectile straight up from the ground at a speed of 47.9 m/s. The projectile reaches a maximum height of 35.8 m before falling back to the ground. What is the value of g for planet #2? O 32.04 m/s^2 O 64.09 m/s^2 O 13.38 m/s^2 O 26.76 m/s^2 QUESTION 8 On planet #3, you fire a projectile horizontally from the edge of a vertical cliff 35.9 m above the ground, with an initial speed of 26.7 m/s. The projectile lands 48.6 m away from the base of the cliff. What is the value of g for planet #3? O 21.67 m/s^2 O 10.84 m/s^2 O26.88 m/s^2 O 175.72 m/s^2 QUESTION 9 On planet #4, you fire a projectile from the ground at an initial speed of 56.1 m/s at an angle of 61.5 degrees above the horizontal. The projectile lands 31.5 m away from the launch point. What is the value of g for planet #4? O 87.8 m/s^2 O 14.8 m/s^2 O 15.5 m/s^2 83.8 m/s^2 QUESTION 10 On planet #5, a stone dropped from a height of 43.9 m above the ground will hit the ground at a speed of 64.7 m/s. What is the value of g for planet #5? O29.79 m/s^2 O 47.68 m/s^2 14.89 m/s^2 95.36 m/s^2
To determine the value of acceleration due to gravity (g) on different planets, we can use the kinematic equations of motion. For planet #2, when the projectile reaches its maximum height, its vertical velocity becomes zero. Using the equation v_f = v_i + gt, where v_f is the final velocity, v_i is the initial velocity, g is the acceleration due to gravity, and t is the time, we can find the time it takes for the projectile to reach maximum height.
Given that the initial velocity (v_i) is 47.9 m/s and the maximum height is reached at t = t/2, we can substitute the values to find g. t = (0 - 47.9 m/s) / g = -47.9 m/s / g = t/2. Solving for g gives us g = -47.9 m/s / (t/2).
Similarly, for the other planets, we can use the kinematic equations to find the value of g. For planet #3, we use the horizontal range formula, R = v_i * t, where R is the range and t is the time of flight. Rearranging the equation, we have t = R / v_i. Substituting the given values, g = 35.9 m / (48.6 m / 26.7 m/s) = 35.9 m * 26.7 m/s / 48.6 m.
For planet #4, we can use the horizontal range formula again and the equation for time of flight, t = (2 * v_i * sin(theta)) / g, where theta is the launch angle. Substituting the given values, g = (2 * 56.1 m/s * sin(61.5 degrees)) / 31.5 m Lastly, for planet #5, we use the equation for final velocity of a freely falling object, v_f = sqrt(v_i^2 + 2gh), where h is the height and v_f is the final velocity. Rearranging the equation, we have g = (v_f^2 - v_i^2) / (2h). Substituting the given values, g = (64.7 m/s^2 - 0) / (2 * 43.9 m). Evaluating these expressions will give us the values of g for each planet.
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A charge QI = 3.0x109 Coulombs located in xy plane at a coordinate of (0, 3meters) and a charge QII = -9.0x10⁹ Coulombs is located at a coordinate at (4.5meters, 0). Find the electric field at origin (0,0) A 5 N/C, 37 degrees downward with the +x axis (B) 5 N/C, 67 degrees downward with the +x axis 10 N/C, 37 degrees upward with the +x axis 10 N/C, 67 degrees upward with the +x axis
The electric field at the origin is approximately 12.81 N/C, 37 degrees upward with the +x axis. To find the electric field at the origin (0,0) due to the charges [tex]Q_I[/tex] and [tex]Q_{II[/tex], we can use the principle of superposition. The electric field due to each charge is calculated separately, and then the vector sum of the electric fields is taken.
The electric field due to a point charge is given by Coulomb's law:
E = k * (Q / [tex]r^2[/tex]) * u
where E is the electric field, k is the electrostatic constant (approximately 9 x [tex]10^9 Nm^2/C^2[/tex]), Q is the charge, r is the distance from the charge to the point where the electric field is being calculated, and u is the unit vector in the direction from the charge to the point.
For charge QI at (0, 3 meters):
The distance from QI to the origin is 3 meters, and the unit vector u points in the downward direction (since the charge is located in the positive y-axis direction).
[tex]= (9 x*10^9 Nm^2/C^2) * (3.0 * 10^9 C / (3 meters)^2) * (-j)[/tex]
= -9.0 N/C * j
For charge QII at (4.5 meters, 0):
The distance from QII to the origin is 4.5 meters, and the unit vector u points in the leftward direction (since the charge is located in the positive x-axis direction).
[tex]E_II = k * (QII / r^2) * u\\= (9 x 10^9 Nm^2/C^2) * (-9.0 * 10^9 C / (4.5 meters)^2) * (-i)[/tex]
= -10 N/C * i
Now, we can find the vector sum of the electric fields:
[tex]E_{total = E_I + E_{II[/tex]
= -9.0 N/C * j + (-10 N/C) * i
Converting this vector form to magnitude-angle form:
[tex]E_{total = \sqrt[(-9.0 N/C)^2 + (-10 N/C)^2][/tex] * cos(atan((-9.0 N/C) / (-10 N/C))) * i
+ [tex]\sqrt[(-9.0 N/C)^2 + (-10 N/C)^2][/tex] * sin(atan((-9.0 N/C) / (-10 N/C))) * j
Calculating the magnitude and angle:
Magnitude = [tex]\sqrt[(-9.0 N/C)^2 + (-10 N/C)^2][/tex] ≈ 12.81 N/C
Angle = atan((-9.0 N/C) / (-10 N/C)) ≈ 37 degrees
Therefore, the electric field at the origin is approximately 12.81 N/C, 37 degrees upward with the +x axis.
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The planet Earth completes one orbit around the Sun in one year. Approximating the orbit to a circle of radius r Earth orbit : 1.5 × 10³ km, calculate the linear speed of the planet as it moves around the Sun. =
The linear speed of the Earth as it moves around the Sun is approximately 0.942 km/s.
To calculate the linear speed of the Earth, we first use the formula for angular speed, which relates the angular velocity (w) to the time it takes for one orbit (T). Since the Earth completes one orbit in one year, we convert the time to seconds and find T to be 31,536,000 seconds.
Using the formula w = 2π / T, we calculate the angular velocity to be 6.282 × 10⁻⁷ radians/second.
Next, we use the formula for linear velocity, which relates the linear speed (v) to the radius of the orbit (r) and the angular velocity (w). Since we are approximating the Earth's orbit to a circle with a radius of 1.5 × 10³ km, we substitute the values of r and w into the formula v = r × w.
After performing the calculation, we find that the linear speed of the Earth is approximately 0.942 km/s. This represents the speed at which the Earth moves in a straight line as it orbits around the Sun.
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While attempting to tune the note Cot 523 It z, a piano trenen hears 3 beats/s between a referrence oscillator and the string. 0=) Whot are the posible frequencies of the string? b) When she tighten the string slightly, she heors 3.00 beatols Whot is the frequency of the string now? (one of the equation provided in the formula sheet relates frequency. to the tension of a string. Use this relation to moke on informed deciseon) * Submit the onswer you obtain in b as your answe
(a) the possible frequencies of the string are 520 Hz and 526 Hz.
(b) The frequency of the string after tightening is 526 Hz
To find the possible frequencies of the string when the piano tuner hears 3 beats/s with a reference oscillator at a frequency of 523 Hz, we can use the formula for beat frequency:
f_beat = |f_reference - f_string|
where f_beat is the beat frequency, f_reference is the frequency of the reference oscillator, and f_string is the frequency of the string.
(a) When the piano tuner hears 3 beats/s, we have:
3 = |523 - f_string|
To find the possible frequencies of the string, we solve for f_string:
f_string = 523 ± 3
Therefore, the possible frequencies of the string are 520 Hz and 526 Hz.
(b) When the piano tuner tightens the string slightly and hears 3.00 beats/s, we can use the same formula:
3.00 = |523 - f_string|
Solving for f_string:
f_string = 523 ± 3.00
Since the tuner tightened the string, the frequency of the string is increased. Therefore, the frequency of the string now is:
f_string = 523 + 3.00 = 526 Hz
Hence, the frequency of the string after tightening is 526 Hz.
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A is 58.0 m long at a 33.0° angle with respect to the +x-axis. Bis 47.0 m long at a 63.0° angle above the-x-axis. What is the magnitude of the sum of vectors A and B? A+B= What angle does the sum of vectors A and B make with the x-axis? m.
The magnitude of the sum of vectors A and B is approximately 78.69 m, and the angle it makes with the x-axis is approximately 54.8°.
To calculate the magnitude and angle of the sum of vectors A and B, we can break down each vector into its x and y components, add the corresponding components, and then use these components to calculate the magnitude and angle of the resulting vector.
Let's start by finding the x and y components of vector A and vector B:
Vector A:
Ax = 58.0 m * cos(33.0°)
Ay = 58.0 m * sin(33.0°)
Vector B:
Bx = 47.0 m * cos(63.0°)
By = 47.0 m * sin(63.0°)
Now, let's add the corresponding components:
Resultant vector (R):
Rx = Ax + Bx
Ry = Ay + By
To calculate the magnitude of vector R (A + B), we can use the Pythagorean theorem:
|R| = sqrt(Rx^2 + Ry^2)
And to find the angle (θ) that vector R makes with the x-axis, we can use the arctangent function:
θ = arctan(Ry / Rx)
Let's calculate the magnitude and angle:
Rx = (58.0 m * cos(33.0°)) + (47.0 m * cos(63.0°))
Ry = (58.0 m * sin(33.0°)) + (47.0 m * sin(63.0°))
|R| = sqrt(Rx^2 + Ry^2)
θ = arctan(Ry / Rx)
Calculating the values:
Rx ≈ 45.51 m
Ry ≈ 64.53 m
|R| ≈ sqrt((45.51 m)^2 + (64.53 m)^2) ≈ 78.69 m
θ ≈ arctan(64.53 m / 45.51 m) ≈ 54.8°
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where on earth is the hottest temperature? 
Answer: The earths core which is 9392 degrees
Explanation:
This was your first question at brainly so i wanted to give you a warm welcoming. :)
