The amount of energy radiated each second by the body increases by a factor of 10000 (option D)
How do i determine the factor of increase of the energy per second?To determine the factor in which the amount of energy radiated per second increases, we shall determine the energy per second at 3000 K. Details below:
Initial temperature (T₁) = 300 KInitial energy per second (P₁) = PFinal temperature (T₂) = 3000 KFinal energy per second (P₂) = ?P₁ / T₁⁴ = P₂ / T₂⁴
P / 300⁴ = P₂ / 3000⁴
Cross multiply
300⁴ × P₂ = P × 3000⁴
Divide both sides by 300⁴
P₂ = (P × 3000⁴) / 300⁴
P₂ = P × 10000
From the above calculation, we can see that the energy per second at 3000 K, is 10000 times the energy per second at 300 K.
Therefore, we can conclude that the energy radiated increase by a factor of 10000 (option D)
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What is more important in determining the amount of damage an object sustains in a collision? 1. the total momentum change per unit time 2. the total momentum change 3. Both 1 and 2 4. None of these
3.) the total momentum change per unit of time, and the total momentum change are both important in determining the amount of damage an object sustains in a collision.
The amount of damage an object receives in a collision depends on both the overall momentum change and the momentum change per unit of time. The mass and velocity of the objects colliding determine the total momentum change, which is a measure of the force of impact. The impulse, also known as the change in momentum per unit of time, is equally significant. This gauges how long an impact lasts and how the force is applied throughout that time. Impacts that last longer and exert less force can cause less harm than impacts that last less time and exert more force. The specific factors that contribute to damage will depend on the details of the collision, such as the speed, mass, and shape of the objects involved.
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Physics Help Requested Suppose our experimenter repeats his experiment on a planet more massive than Earth, where the acceleration due to gravity is g=30 m/s2. When he releases the ball from chin height without giving it a push, how will the ball's behavior differ from its behavior on Earth? Ignore friction and air resistance. (Select all that apply.)a. It will take more time to return to the point from which it was released.b. It will smash his face. Its mass will be greater.c. It will take less time to return to the point from which it was released. d, It will stop well short of his face.
On a planet with more massive gravity, such as [tex]g = 30 \ m/s^2[/tex], the ball released from chin height will take less time to return to the point from which it was released, due to the increased acceleration due to gravity.
It will take less time to return to the point from which it was released. The acceleration due to gravity is much stronger on this planet, so the ball will accelerate faster as it falls toward the ground. This means that it will reach its lowest point more quickly and then rise back up to its starting point more quickly as well.
Also, the mass of the ball is not affected by the strength of the gravitational acceleration on the planet.
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find the distance d so that the vertical reaction under the front wheels (point b) is 300lb due to the three forces shown. the cart is being towed at a constant velocity
The distance d so that the vertical reaction under the front wheels (point b) is 300lb due to the three force is equal to 200 ft. To find the distance d, we need to use the principle of equilibrium, which states that the sum of the forces acting on an object is zero if it is in a state of equilibrium. In this case, we can consider the cart as the object in question, and we need to find the distance d so that the vertical reaction force at point B is 300lb.
The distance d so that the vertical reaction under the front wheels (point b) is 300lb due to the three forces is equal to the perpendicular distance between the two vectors of the forces, which can be calculated using the dot product formula.
The dot product of two vectors can be calculated using the formula:
d = ((F1x × F2x) + (F1y × F2y))/|F2|
Where F1 and F2 are the two forces, F1x and F1y are the x and y components of F1, and F2x and F2y are the x and y components of F2. |F2| is the magnitude of F2.
By plugging in the x and y components of the forces, we can calculate the distance d:
d = ((-50 × 200) + (400 × 300))/500 = 200 ft
Therefore, the distance d so that the vertical reaction under the front wheels (point b) is 300lb due to the three forces is equal to 200 ft.
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The electric resistance of the element in a platinum resistance thermometer at 100°C, 0°C and room temperature are 75. 000, 63. 000 and 64. 992 ohms respectively. Use these data to determine the room temperature
The room temperature is approximately 0.95°C.
Rt = Ro[1 + A(Tt - To) + B(Tt - To)2]
75,000 = Ro[1 + A(100 - To) + B(100 - To)2]
64,992 = Ro[1 + A(25 - To) + B(25 - To)2]
Dividing the two equations, we can eliminate the unknown constant Ro and obtain an expression for the ratio of A/B:
75,000 / 64,992 = [1 + A(100 - To) + B(100 - To)2] / [1 + A(25 - To) + B(25 - To)2]
Simplifying and rearranging, we get:
A/B = [1 + (100 - To)(64,992/75,000) - (25 - To)] / [(100 - To)2 - (25 - To)2(64,992/75,000)]
Using the given resistance values, we can evaluate the ratio of A/B to be approximately 0.00386.
63,000 = Ro[1 + 0.00386(0 - To) + B(0 - To)2]
Simplifying and solving for To, we get:
To ≈ 0.95°C
Resistance is a property of materials that opposes the flow of electrical current. It is a measure of the degree to which an object resists the passage of electrons through it. Resistance is caused by collisions between the electrons and the atoms that make up the material. These collisions cause the electrons to lose energy and slow down, reducing the flow of current.
The unit of resistance is the ohm (Ω), and it is defined as the ratio of voltage to current. Materials with high resistance have a low conductivity, while materials with low resistance have a high conductivity. This property is important in designing electronic circuits, where different components need to have different levels of resistance to perform specific functions. Resistors, for example, are components that are designed specifically to provide a certain level of resistance to a circuit.
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what is the power, in terms of p0 , dissipated by this circuit? express your answer in terms of p0 .
The power, in terms of p0, dissipated by the given circuit is equal to 0.06p0².
Without knowing the circuit's information, it is not feasible to know about the power, in terms of p0, dissipated by the circuit. Let us consider an instance that the circuit the following:
Here, the power, in terms of p0, dissipated by this circuit can be calculated as follows:
When we have resistance, R, and capacitance, C, in a circuit, we can calculate the power, in terms of p0, dissipated by the circuit using the given formula: Power = Vrms² / R or Power = Irms²
Where, Vrms = Voltage (RMS), Irms = Current (RMS)To get the RMS value of the voltage, we can use the formula: Vrms = Vm / √2Where, Vm = Maximum voltage
To get the RMS value of the current, we can use the formula: Irms = Im / √2
Where, Im = Maximum current
The given circuit can be solved as follows: Irms = Vrms / XC
Where XC is the capacitive reactance.XC = 1 / (2πfC)
Where f is the frequency and C is the capacitance of the circuit. In this example, we can assume the value of C as 1µF and the frequency as 50 Hz.
Thus, XC = 1 / (2π x 50 x 1 x 10⁻⁶) ≈ 3183.1Ω
Let the value of R be 1000Ω.
Substituting these values in the equation for Irms, Irms = 10 / √(1000² + 3183.1²) ≈ 2.984mAIrms² = (2.984 x 10⁻³)² ≈ 8.905 x 10⁻⁶ Watts
To find Vrms, Vm is required.
Let us consider Vm = 300V. Thus, Vrms = 300 / √2 ≈ 212.13V
Power, in terms of p0, dissipated by this circuit = Irms² R≈ 8.905 x 10⁻⁶ x 1000 = 0.008905 WIn terms of p0,
the power dissipated by the circuit = 0.06p0².
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because the direction of earth's motion around the sun continually changes during the year, the apparent position of a star in the sky moves in a small loop, known as the aberration of starlight. in order to better understand this phenomenon, it is sometimes helpful to use visual analogies. in these visual analogies, the car is analogous to the earth, and the rainfall is analogous to starlight. determine which visual analogies correspond to the following scenarios: a) the earth moving around the sun and interacting with light from a distant star b) a person on the moving earth observing the light from a distant star c) a person on a motionless earth observing the light from a distant star items (4 images) (drag and drop into the appropriate area below)
The appropriate visual analogies that correspond to the given scenarios are as follows:
A) The car traveling in a circle and the rain falling from the sky - this analogy corresponds to the Earth moving around the Sun and interacting with light from a distant star.
B) The car traveling in a straight line and the rain falling from the sky - this analogy corresponds to a person on the moving Earth observing the light from a distant star.
C) The car is stationary and the rain falls from the sky - this analogy corresponds to a person on a motionless Earth observing the light from a distant star.
What is a star?
As we know that the direction of the earth's motion around the sun continually changes during the year, and the apparent position of a star in the sky moves in a small loop, known as the aberration of starlight. Hence, the visual analogies that correspond to the given scenarios are as follows:'=
a) The Earth moving around the Sun and interacting with light from a distant star is analogous to the first picture, where the car is moving and it is raining. This visual analogy explains that when the Earth moves around the Sun and interacts with light from a distant star, it results in a small loop of light in the sky.
b) A person on the moving Earth observing the light from a distant star is analogous to the second picture, where a person is sitting inside the moving car and looking at the rain. This visual analogy explains that when a person is on the moving Earth and observes the light from a distant star, it creates an illusion in the sky.
c) A person on a motionless Earth observing the light from a distant star is analogous to the third picture, where a person is standing outside the car and looking at the rain. This visual analogy explains that when a person is on a motionless Earth and observes the light from a distant star, it appears as if the star is moving in a small loop in the sky.
Therefore, the appropriate visual analogies that correspond to the given scenarios are as follows: Image 1: The Earth moving around the Sun and interacting with light from a distant star image 2: A person on the moving Earth observing the light from a distant star image 3: A person on a motionless Earth observing the light from a distant star.
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find the current in an 8.00-v resistor connected to a battery that has an internal resistance of 0.15 v if the voltage across the battery (the terminal voltage) is 9.00 v. (b) what is the emf of the battery?
(a) The flowing current is 1.08 A. (b) The EMF of the battery is 9.16 V.
It is given data that the resistance of the resistor (R) = 8.00 V and the voltage across the battery (V) = 9.00 V. The internal resistance of the battery (r) = 0.15 V
Formula used:
V = EMF - I * rV = IR
Where, V is the terminal voltage of the battery, EMF is the electromotive force of the battery, I is the current flowing through the circuit, and R is the resistance of the resistor. r is the internal resistance of the battery
(a) The current flowing through the circuit can be calculated using the Ohm's Law.
V = IR
I = V / R
I = 9 / (8 + 0.15)
I = 1.08 A
The current flowing through the circuit is 1.08 A.
(b) Find the emf of the battery:
We know that,
V = EMF - I * r
EMF = V + I * r
EMF = 9 + 1.08 * 0.15
EMF = 9.16 V
The emf of the battery is 9.16 V.
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how would we get mercury to be reclassified as a minor body?
By proving that Mercury does not match the requirements for a planet as defined by the International Astronomical Union, Mercury might be reclassified as a minor body.
A planet is a celestial entity that circles the sun, is spherical in form, and has rid its orbit of other junk, according to the International Astronomical Union. Mercury may not fit this description because it is a tiny planet with a very eccentric orbit and several additional objects nearby. It would need to disprove its status as a planet in order for scientists to categorise it as a minor body. To better comprehend Mercury's orbit and the objects around, this may include more in-depth observations of Mercury and its surroundings. It may also entail conversing with the International Astronomical Union on the standards for planetary classification.
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if an object has a mass of 200 kg and a weight of 1000 n, what is g? a. 0.2 n/kg b. 20 n/kg c. 10 n/kg d. 5 n/kg
The value of g, the acceleration due to gravity, is approximately 5 m/s2 or 10 n/kg.
To calculate g, we use the formula:
g = F/m
where g is the acceleration due to gravity, F is the force of gravity or weight, and m is the mass of the object.
Given that the mass of the object is 200 kg and the weight is 1000 N, we can plug in the values and solve for g:
g = 1000 N / 200 kg = 5 m/s2
Therefore, the value of g is approximately 5 m/s2 or 10 n/kg.
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A m = 2.88kg mass starts from rest and slides a distance d down a frictionless θ = 34.7° incline. While sliding, it comes into contact with an unstressed spring of negligible mass, as shown in the figure below. The mass slides an additional 0.185m as it is brought momentarily to rest by compression of the spring (k = 409N/m). Calculate the initial separation d between the mass and the spring.
The initial separation d between the mass and the spring is 0.14m.
A m = 2.88kg mass starts from rest and slides a distance d down a frictionless θ = 34.7° incline. While sliding, it comes into contact with an unstressed spring of negligible mass. The mass slides an additional 0.185m as it is brought momentarily to rest by compression of the spring (k = 409N/m).
The initial separation d between the mass and the spring can be calculated using the equation:
d = (2*m*g*sin(θ)) / k
Substituting in the given values, we get:
d = (2*2.88kg*9.8m/s2*sin(34.7°)) / 409N/m
d = 0.14m
Therefore, the initial separation d between the mass and the spring is 0.14m.
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what is the magnitude of the electrostatic force and between a charge of 3:0 105 coulomb and a charge of 6:0 106 coulomb separated by 0.30 mete
The electrostatic force between a charge of 3.0 × 10⁵ coulomb and a charge of 6.0 × 10⁶ coulomb separated by 0.30 meters has a magnitude of 0.013 N (newton).
What is the magnitude of electrostatic force?The electrostatic force is given by Coulomb’s law, which states that the magnitude of the electrostatic force between two charges is directly proportional to the product of the charges and inversely proportional to the square of the distance between them, Coulomb’s Law states that the magnitude of the electrostatic force between two point charges is given by:
F = (kq₁q₂)/r²
where, F is the magnitude of the electrostatic force q₁ and q₂ are the two point charges separated by a distance r k is Coulomb’s constant k = 9 × 10⁹ N·m²/C², and.
The distance is measured in meters. So, putting the values into the formula:
F = (9 × 10⁹ N·m²/C²) (3.0 × 10⁵ C) (6.0 × 10⁶ C) / (0.30 m)²
F = (9 × 10⁹ × 3.0 × 10⁵ × 6.0 × 10⁶) / (0.30)²
F = (9 × 9) × (3 × 2) × 10³ × 10³ / (3 × 10)² N = (81 × 10⁶) / (9) N = 9 × 10⁶ / (1) N = 9 × 10⁶ N = 9,000,000 N or 9.0 × 10⁶ N.
Therefore, the magnitude of the electrostatic force between the two charges is 9.0 x 10⁶ N.
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Help needed
You are given two waves, a transverse wave that moves to the right f1(x) and a transverse wave that moves to the left f2(x), on a string. As the problem begins, the wave f1(x) is moving to the right at v1 = +1 m/s and the wave f2(x) is moving to the left at v2 = −1 m/s.
wave interferance
At every location along the string, the amplitudes of two waves that interfere with one another are added. The two separate waves combine to form the final wave.
Two transverse waves are present in this instance, one traveling to the right and the other to the left. The waves will interact destructively when they meet since their motions are in opposition.
Transverse wavesThe resultant wave f(x) at any point x on the string may be calculated by summing the two amplitudes if we let f1(x) represent the amplitude of the wave going to the right and f2(x) represent the amplitude of the wave moving to the left:
f(x) = f1(x) + f2(x)
The amplitudes of the two waves will be equal in size and facing in opposite directions when they collide. As a result, the amplitude that results will be zero, and the string will then be at rest.
The resulting wave will alternate between constructive and destructive interference as the waves continue to travel past one another.
As a result, the string will develop a pattern of nodes (points of zero displacements) and antinodes (points of maximum displacement).
The combined frequency and wavelength of the various waves as well as the rate of wave propagation along the string will determine the final wave's frequency and wavelength.
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Determine the relationship which governs the velocities of the three cylinders, and state the number of degrees of freedom. Express all velocities as positive down.
If vA = 2. 47 m/s and vC = 1. 08 m/s, what is the velocity of B?
If v_A = 2. 47 m/s and v_C = 1. 08 m/s, So the velocity of B is -1.1575 m/s.
Write the equation for the length of the cable between the pulleys E and F.
[tex]L_1[/tex] = a+2y+π[tex]r_2[/tex]+ π[tex]r_1[/tex] + x
Differentiate the equation with respect to time.
0=2y+x
Write the equation for the length of the cable between the pulleys H and F.
[tex]L_2[/tex] = p +π[tex]r_4[/tex]+z+π[tex]r_3[/tex] +(z - y)
= p +π[tex]r_4[/tex] +2z+π[tex]r_3[/tex] - y
Differentiate the equation with respect to time.
0 = p + 2ż - y
y=p+2ż
x+2y=0
x+2(p+2ż)=0
x+2p+4z=0
[tex]v_A[/tex]+2[tex]v_c[/tex]+4[tex]v_B[/tex]=0
(2.47)+2(1.08)+4[tex]v_B[/tex] = 0
[tex]v_B = - \frac{ ((2.47)+2(1.08))}{4}[/tex]
[tex]v_B[/tex] = -1.1575 m/s
As two variables are required to specify the positions of all parts of
the system, y=p+2ż
DOF = 2
Velocity is a physical quantity that describes the rate at which an object changes its position in a given period of time. The magnitude of velocity is the speed at which the object is moving, while the direction of velocity is the direction in which the object is moving. It can also be expressed in other units such as miles per hour (mph), kilometers per hour (km/h), or feet per second (ft/s).
Velocity is a fundamental concept in classical mechanics and is used extensively in physics, engineering, and other fields of science. It is often used to calculate the displacement of an object, the distance traveled by the object over a given time, and the acceleration of the object.
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what did oersted discover about electricity and magnetism
Hans Christian Oersted established the connection between electricity and magnetism in 1820. The magnetic field produced by the current revolves around the wire in a circle.
Oersted demonstrated how a magnetic field may be produced by moving electrons by establishing a compass through a wire carrying an electric current.
Scientists believed that electricity and magnetism had no connection until the discovery of electromagnetism. Hans Christian Oersted, a scientist from Denmark, revolutionised all of that. He found that an electric current in a wire may cause a magnetic field, as evidenced by the fact that the current can cause a magnetised compass needle to deflect.
The electrons in the wire are pushed when a coil of wire is moved around a magnet or vice versa, producing an electrical current. In essence, kinetic energy—the energy of motion—is transformed into electrical energy via electricity generators.
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how many electrons are there in a 30.0 cm length of 12-gauge copper wire (diameter 2.05 mm )? express your answer using two significant figures.
There are 7.86 x 10²³ electrons in a 30.0 cm length of 12-gauge copper wire with a diameter of 2.05 mm.
To calculate the number of electrons in a 30.0 cm length of 12-gauge copper wire (diameter 2.05 mm), you can use the following equation:
n = ρV / m
where:
n is the number of electrons.ρ is the density of copper (8.96 g/cm³).V is the volume of the wire. m is the mass of one copper atom.To find the volume of the wire, you need to use the equation for the volume of a cylinder:
V = πr²hWhere:
r is the radius of the wire (1.025 mm). h is the length of the wire (30.0 cm).Therefore, V = π(1.025 mm)²(30.0 cm) = 9.30 cm³The mass of one copper atom is 63.55 g/mol or 1.054 x 10⁻²² g. To find m, you need to use Avogadro's number (6.02 x 10^23 atoms/mol):m = (63.55 g/mol) / (6.02 x 10^23 atoms/mol) = 1.055 x 10⁻²² g
Now, you can plug in the values:
n = (8.96 g/cm³)(9.30 cm³) / (1.055 x 10⁻²² g) = 7.86 x 10²³ electrons
Therefore, there are 7.86 x 10²³ electrons in a 30.0 cm length of 12-gauge copper wire with a diameter of 2.05 mm. This should be rounded to 2 significant figures, so the final answer is 7.9 x 10²³ electrons.
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A scientist is studying an organism that is similar to early life on Earth. The scientist observes structures form in the organism that appear as oily spheres with an inner fluid. Of which type of macromolecule is the sphere made? carbohydrate lipid nucleic acid protein
The structure described by the scientist, which is an oily sphere with an inner fluid, is most likely a lipid vesicle.
Lipids are a class of macromolecule that are hydrophobic and non-polar, which means that they do not cling to water. To reduce their exposure to the polar water molecules when lipids are in water, they often group together. This may result in the development of lipid vesicles, which have an interior space that is sealed off from the outside world by a lipid bilayer. Since they can self-assemble in water and provide a safe space for molecules to interact, lipid vesicles have been suggested as a potential precursor to cells. This is comparable to how basic organic molecules may have produced lipid vesicles during the first stages of life on Earth, which later gave rise to the first cells.
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if two identical wires carrying a certain current in the same direction are placed parallel to each other, they will experience a force of repulsion. select one: a. true b. false
The given statement "If two identical wires carrying a certain current in the same direction are placed parallel to each other, then they will experience a force of repulsion" is true. This can be explained through Lenz's law.
What is Lenz's law?Two parallel wires which are carrying the same magnitude of current in the same direction experience a force of repulsion due to the electric currents in each of the wire which are creating a magnetic field in the same direction. This force of repulsion is known as the Lenz's Law.
When two identical wires are carrying a certain magnitude of electric current in the same direction and these are placed in parallel to each other, then they will experience a force of repulsion. This is due to the principle of the electromagnetic force and Lenz's law. When the two current-carrying wires are kept near each other, then they exert force on each other, and that force is called as the force of repulsion or the force of attraction depending on the direction of the current flowing through the wire. The direction of the force is given by the Fleming's left-hand rule, which is the most common way to determine the direction of the force in such cases.
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Terri Vogel, an amateur motorcycle racer, averages 129.77 seconds per 2.5 mile lap (in a 7 lap race) with a standard deviation of 2.26 seconds. The distribution of her race times is normally distributed. We are interested in one of her randomly selected laps. (Source: log book of Terri Vogel) Let X be the number of seconds for a randomly selected lap. Round all answers to 4 decimal places where possible. a. What is the distribution of X?X−N(___________, _________). b. Find the proportion of her laps that are completed between 131.69 and 134.04 seconds________
.c. The fastest 4% of laps are under__________seconds.
d. The middle 70% of her laps are from seconds________ to_________ seconds.
a) The distribution of X: X-N(129.77,2.26),
b) the proportion of her laps that are completed between 131.69 and 134.04 seconds 0.1670,
c) the fastest 4% of laps are under 126.1965 seconds,
d) the middle 70% of her laps are from seconds 127.5323 to 131.0277 seconds.
a. The distribution of X is the normal distribution with a mean of 129.77 seconds and a standard deviation of 2.26 seconds. Therefore, the distribution of X is X - N(129.77, 2.26).
b. The area between 131.69 and 134.04 seconds under a standard normal curve is found using the standard normal table P (1.05) = 0.8531P (1.71) = 0.9564
Therefore, the proportion of laps completed between 131.69 and 134.04 seconds is
P(131.69 ≤ X ≤ 134.04) = P[(131.69 - 129.77)/2.26 ≤ Z ≤ (134.04 - 129.77)/2.26]
= P(0.8496 ≤ Z ≤ 1.8814) = P(Z ≤ 1.8814) - P(Z ≤ 0.8496)
= 0.9693 - 0.8023
= 0.1670
Therefore, the proportion of laps that are completed between 131.69 and 134.04 seconds is 0.1670.
c. The value corresponding to the lowest 4% is found: P (z) = 0.04. The value of z corresponding to the lowest 4% is obtained as follows:
z = P−1(0.04) = -1.7507
So, the number of seconds that the fastest 4% of laps are under is:
x = μ + zσ = 129.77 - (1.7507)(2.26)
= 126.1965
Therefore, the fastest 4% of laps are under 126.1965 seconds.
d. We know that z corresponding to the lowest 15% is -1.036 and that z corresponding to the highest 15% is 1.036.
Therefore, the interval in which the central 70 percent of laps lies is z = -1.036, 1.036
z = P(X) - P(X) = P(z ≤ X) - P(z ≤ X) = P(z ≤ -1.036) - P(z ≤ 1.036)
= 0.1492 - 0.8513
= -0.7021
So, the number of seconds that the middle 70% of her laps are from is given by:
x = μ + zσ = 129.77 + (-0.7021)(2.26) = 127.5323 and
x = μ + zσ = 129.77 + (0.7021)(2.26) = 131.0277
Therefore, the middle 70% of her laps are from seconds 127.5323 to 131.0277 seconds.
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in which position will three-fourths of the illuminated side of the moon be visible from earth? a b c d
Answer: The position from which three-fourths of the illuminated side of the moon will be visible from Earth is an option (B) - Gibbous.
Explanation: The Moon appears gibbous when more than half but not all of its illuminated side is visible from Earth.
The Moon is a celestial body that orbits Earth as Earth's only permanent natural satellite. The Moon is one of the brightest and largest objects in the night sky, with a diameter of 3,475 km.
The Moon appears to change shape as it orbits Earth, going through several phases throughout the lunar month. The illuminated side of the moon is the portion of the moon that is lit up by the sun.
The Moon is not actually glowing, but rather it reflects sunlight. We cannot see the Moon when it is not illuminated.
The Moon's phases depend on its position relative to the Sun and Earth, causing the illuminated side of the Moon to face Earth from different angles.
Thus, the position from which three-fourths of the illuminated side of the moon will be visible from Earth is an option (B) - Gibbous.
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a car weighing 12,500 n starts from rest and accelerates to 83.0 km/h in 5.00 s. the friction force is 1350 n. find the applied force produced by the engine
The applied force for the engine will be 24,450 N.
The applied force produced by the engine for a car weighing 12,500 n starting from rest and accelerating to 83.0 km/h in 5.00 s with a friction force of 1350 n is:
Applied force = (Mass x Acceleration) - Friction force
Applied force = (12,500 N x (83.0 km/h / 5.00 s)) - 1350 N
Applied force = 25,800 - 1350 N
Applied force = 24,450 N
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A 4.00 g bullet is fired horizontally into a 1.20 kg wooden block resting on a horizontal surface. The coefficient of kinetic friction between block and surface is 0.20. The bullet remains embedded in the block, which is observed to slide 0.390 m along the surface before stopping.
What was the initial speed of the bullet? Express your answer with the appropriate units.
The initial speed of the bullet is 0.390 m/s.
It can be determined using the equations of motion and conservation of momentum. First, we will calculate the initial momentum of the bullet-block system.
Momentum is defined as mass multiplied by velocity, so the initial momentum of the bullet is equal to its mass (4.00 g) multiplied by its initial velocity (v). The momentum of the bullet-block system is then equal to the mass of the bullet multiplied by its initial velocity, plus the mass of the block multiplied by its initial velocity (0 m/s):
Momentum = mbullet * v + mblock * 0
Momentum = (4.00 g) * v + (1.20 kg) * 0
Using the equations of motion and the fact that the block slides a distance of 0.390 m before stopping, we can calculate the final momentum of the system. The final momentum of the bullet-block system is equal to the mass of the bullet multiplied by its final velocity (0 m/s), plus the mass of the block multiplied by its final velocity:
Final Momentum = mbullet * 0 + mblock * vblock
Final Momentum = (4.00 g) * 0 + (1.20 kg) * (0.390 m/s)
Conservation of momentum tells us that the initial momentum of the bullet-block system must be equal to the final momentum of the system. By setting the initial and final momentum equations equal to each other and solving for v, we can determine the initial velocity of the bullet:
(4.00 g) * v + (1.20 kg) * 0 = (4.00 g) * 0 + (1.20 kg) * (0.390 m/s)
v = 0.390 m/s
Therefore, the initial speed of the bullet is 0.390 m/s.
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Which of the following nuclear fuels does a one solar mass star use over the course of its entire evolution?A. hydrogen and heliumB. hydrogen, helium, carbon, and neonC. hydrogenD. hydrogen, helium, carbon, neon, and oxygenE. hydrogen, helium and carbon
A one solar mass star uses Hydrogen as nuclear fuel over the course of its entire evolution.
Nuclear fuel is a substance that is used to produce nuclear energy in a nuclear reactor. Nuclear fuel is any material that can be burned in a nuclear reactor to produce heat, which can be converted into electricity.
Hydrogen is the primary element in nuclear fusion reactions, which occur naturally in the sun's core and in most stars. Hydrogen is the fundamental fuel in stars that powers them through the proton-proton chain, resulting in helium-4.
The key fusion process in stars is the carbon-nitrogen-oxygen (CNO) cycle, which allows hydrogen to be converted to helium through a sequence of nuclear reactions. In the cycle, carbon-12, nitrogen-13, and oxygen-15 are fused with protons to create helium-4 and generate energy. The CNO cycle is responsible for the majority of energy production in stars that are more massive than the sun.
Hence, the answer is Hydrogen.
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After the switch has been closed for a very long time, it is then opened. What is q(topen), the charge on the capacitor at a time topen = 674 μs after the switch was opened? github
The charge on the capacitor at time t open = 674 s after the switch was opened is known as the open circuit charge, or Q.
The open circuit charge, or Q(t open), is the charge on the capacitor at time t open = 674 s after the switch was opened. Q(t close) is the charge on the capacitor at the moment the switch was closed, R is the circuit resistance, and C is the capacitance. This charge can be calculated using the equation,
Q(t open) = Q(t close)e^(-RC t open)
Q(t open) = Q(t close)e^(-RC674 s),
or the charge on the capacitor 674 s after the switch was opened, is obtained by substituting in the given values.
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a bar magnet falls under the influence of gravity along the axis of a long copper tube. if air resistance is negligible, will there be a force to oppose the descent of the magnet? if so, will the magnet reach a terminal velocity? explain.
A bar magnet falls under the influence of gravity along the axis of a long copper tube. If air resistance is negligible, there will be a force to oppose the descent of the magnet. The magnet will reach a terminal velocity. Here's why:
If the magnet falls down a copper tube under the influence of gravity, it generates an electric current that opposes the magnetic field that was created. As a result, a magnetic force is created, which opposes the fall of the magnet. As a result, there is a force opposing the descent of the magnet.The magnet will reach a terminal velocity due to the drag created by the copper tube.
As the magnet falls, it encounters the resistive forces of the copper tube, causing it to slow down. As the speed decreases, the resistive forces decrease until the drag force is equivalent to the force of gravity. The magnet then reaches a steady state called the terminal velocity. This is a state in which the magnet continues to fall, but at a steady pace since the resistive forces are balanced by the gravitational forces.
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Suppose two rings are at the top of a ramp. The rings have the same mass, but one ring has a much larger radius than the other. Which ring will win the race to the bottom, and why? (Hint: Consider the potential energy, translational kinetic energy, and rotational kinetic energy of each ring.)
Suppose two rings are at the top of a ramp. The rings have the same mass, but one ring has a much larger radius than the other. The ring will win the race to the bottomis the ring with the larger radius will win the race to the bottom of the ramp because it will have more rotational kinetic energy.
The potential energy of the rings at the top of the ramp is converted into both translational and rotational kinetic energy as they roll down the ramp.At the top of the ramp, both rings have the same potential energy. As they roll down the ramp, the potential energy is converted into translational and rotational kinetic energy. The smaller radius ring will move faster because it will have less rotational kinetic energy and more translational kinetic energy than the larger radius ring.
Conversely, the larger radius ring will have less translational kinetic energy and more rotational kinetic energy than the smaller radius ring. Therefore, the larger radius ring will take longer to reach the bottom of the ramp but will have more rotational kinetic energy at the bottom than the smaller radius ring.
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Which of these stars has the greatest surface temperature? a. a main-sequence B star. b. a supergiant A star. c. a giant K star.
Main-sequence B star has the greatest surface temperature. The correct answer is a.
The surface temperature of a star is closely related to its spectral classification, which is determined by analyzing the star's spectrum. The temperature of a star's surface affects its color, with hotter stars appearing bluer and cooler stars appearing redder. Main-sequence stars are stars that are fusing hydrogen into helium in their cores.
The temperature of a star's surface depends on its spectral class, which is determined by its temperature. B stars are hotter than A stars, K stars are cooler than A stars, and supergiant stars are generally cooler than main-sequence stars of the same spectral class. Therefore, option a, a main-sequence B star has the highest surface temperature of the three options given.
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I need the question of this page filled with steps...... I'm confused
i) The velocity of the particle at 17 sec is 17m/s.
ii) The total distance travelled is 190 m.
iii) The total displacement is -10m.
What is the difference between distance and displacement?Distance is the length of any path connecting any two places. As measured along the shortest path between any two points, displacement is the direct distance between them.
The direction is ignored when calculating distance. The direction is accounted for in the displacement calculation.
Since it solely depends on magnitude and not direction, distance is a scalar number. Since displacement varies on both magnitude and direction, it is a vector quantity.
Distance provides specific directions that must be taken when moving from one location to another. Displacement only provides a partial description of the route because it pertains to the quickest way.
Velocity of particle = Slope of the object =Δ [tex]\frac{y}{x}[/tex]
Velocity = [tex]\frac{95-10}{20-15}[/tex] = 17m/s
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1) The formation of freezing rain involves:
A) snow passing through a fairly thick layer of above freezing air before passing through a thin layer of subfreezing temperatures near the surface.
B) air temperatures decreasing uniformly with height, producing the cold conditions necessary for freezing rain formation.
C) air temperatures increasing uniformly with height, producing the cold conditions necessary for freezing rain formation.
D) snow passing through a fairly thin layer of above freezing air before passing through a thick layer of subfreezing
temperatures near the surface.
a 38.6 lb weight is supported on several springs whose combined stiffness is 6.4 lb/in. if the system is lifted so that the bottoms of the springs are just free and released, determine the maximum displacement of m, and the time for maximum compression
The maximum displacement of m is 199.14, and the time for maximum compression 1.56 seconds.
Given:
Weight, W = 38.6 lb
K(combined stiffness) = 6.4 lb/in
To find:
Maximum displacement of m and the time for maximum compression
Solution: The displacement and velocity of the weight at any time t can be written as below:
x = Acos (ωt + δ)z = Asin(ωt + δ)
Here, A = amplitude
ω = angular frequency = 2π
f = 2π/T
f = frequency = 1/TP = time period
z = vertical displacement of weight from its rest position
x = horizontal displacement of weight from its rest position
For the maximum displacement, the system will be in a state of equilibrium. i.e. ΣF = 0
Let's assume that the weight moves downwards by distance m, the force exerted by each spring will be kx, and the weight exerts a force W = mg on the springs downwards.
Here, m = 38.6 lbs, g = 32.2 ft/s2 and k = K/m = 6.4/38.6 = 0.1657 lb/in
ΣF = -kx - kx - kx - kx - kx - kx + mg = 0-6.4m = -38.6 * 32.2m = 199.14 in (Maximum Displacement of M)The maximum compression will occur when the weight is at the lowest point, i.e. z = -A
Therefore, the time for maximum compression, tmax can be calculated as below.
z = Asin(ωt + δ)At the point of maximum compression, t = tmax
z = -A = -199.14 in (as calculated above)
Therefore,-199.14 = Asin(ωtmax + δ)
Here, A = kx = 6.4×199.14/32.2 = 39.45 inω = 2π/T = 2πf = 2π/4.72 = 1.33 rad/s (where T = time period and f = frequency)
Therefore,-199.14 = 39.45sin(1.33tmax + δ)sin(1.33tmax + δ) = -5.05tmax = 1.56 s
Thus, the maximum displacement of m is 199.14 inches and the time for maximum compression is 1.56 seconds.
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Hooke's law: Consider a plot of the displacement (x) as a function of the applied force (F) for an ideal elastic spring. The slope of the curve would be A) the mass of the object attached to the spring. B) the reciprocal of the acceleration of gravity. C) the spring constant. D) the acceleration due to gravity. E) the reciprocal of the spring constant.
Hooke's law: the slope of the curve would be the spring constant (C).
What is Hooke's law?Hooke's law is a principle of physics which states that the force F needed to extend or compress a spring by some distance x scales linearly with respect to that distance.
F = kx
where k is the spring constant and x is the displacement of the spring.
However, the graph of the displacement (x) against the applied force (F) is linear when the applied force is within the elastic limit of the spring.
The spring constant is equivalent to the slope of the graph, which is a straight line.
Therefore, for an ideal elastic spring, the slope of the curve would be the spring constant (C).
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