The motion of a swing is a periodic motion, that means it takes one period for a back and forth motion, which is constant. Here it is 12s, so it will take 12s for a back and forth motion, no matter the distance. The length of the rope in the given case is 11.8m
What is periodic motion?
The motion of a swing is a periodic motion that goes back and forth. The time it takes to complete one back and forth motion is called the period. In this case, the period of the swing is 12 s, which means it takes 12 s to swing from one side to the other and back again, no matter the distance.
The length of the rope affects the distance the swing travels, but not the period of the motion. This is because the period only depends on the gravitational force acting on the swing and the length of the rope, not on the distance traveled.
To determine the length of the rope, we need to know the distance the swing travels in one back and forth motion. Let's assume that the swing travels a distance of 4 meters from one side to the other. This means that the total distance traveled in one back and forth motion is 8 meters.
The period of the motion is given by the formula T=2π√(L/g), where T is the period, L is the length of the rope, and g is the acceleration due to gravity. We know that T=12 s and g=9.81 m/s². Substituting these values into the formula, we get:
12=2π√(L/9.81)
Squaring both sides and rearranging, we get:
L=(12/π)²×9.81/4
L=11.8 meters (approximately)
Therefore, the length of the rope is approximately 11.8 meters.
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In general, when we compare the mass of a galaxy or cluster of galaxies to the amount of light it emits (that is, when we look at its mass-to-light ratio), we expect that __________.
In general, when we compare the mass of a galaxy or cluster of galaxies to the amount of light it emits, we expect that the mass-to-light ratio will be higher for galaxies or clusters with more dark matter.
Dark matter is a type of matter that does not emit, absorb, or reflect light, and therefore cannot be directly observed. However, its presence can be inferred through its gravitational effects on visible matter, such as stars and gas.
This is because galaxies and galaxy clusters contain not only stars but also other forms of matter that do not emit light, such as dark matter and interstellar gas. These non-luminous components contribute to the overall mass, increasing the mass-to-light ratio compared to that of individual stars.
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How wide is the central diffraction peak on a screen 2.10 m behind a 0.0328- mm -wide slit illuminated by 588- nm light
The width of the central diffraction peak on the screen is approximately 0.0797 meters or 79.7 millimeters.
To find the width of the central diffraction peak, we can use the formula for single-slit diffraction:
Width of central peak = 2 * λ * L / w
Where:
- λ (lambda) is the wavelength of light (588 nm)
- L is the distance from the slit to the screen (2.10 m)
- w is the width of the slit (0.0328 mm)
First, convert the given values to meters:
λ = 588 nm = 588 * 10^(-9) m
w = 0.0328 mm = 0.0328 * 10^(-3) m
Now, substitute these values into the formula:
Width of central peak = 2 * (588 * 10^(-9) m) * (2.10 m) / (0.0328 * 10^(-3) m)
Width of central peak = (2 * 588 * 10^(-9) * 2.10) / 0.0328 * 10^(-3)
Width of central peak ≈ 0.0797 m
The width of the central diffraction peak on the screen is approximately 0.0797 meters or 79.7 millimeters.
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A space freighter accidentally drops a steel beam while passing a black hole, and the beam starts falling toward the black hole with the long axis of the beam pointing toward the black hole. What happens to the beam as it approaches the event horizon?
As the steel beam falls towards the black hole with its long axis pointing towards the black hole, it will experience tidal forces that increase as it gets closer to the event horizon.
Tidal forces refer to the gravitational forces exerted on an object by another object, which vary as a function of the distance between the objects. These forces are responsible for the tides observed on Earth's oceans, but they also play a role in a variety of astrophysical phenomena.
In the case of the Earth and the Moon, the Moon's gravitational pull creates a tidal force that causes the oceans to bulge on opposite sides of the planet, resulting in the twice-daily rise and fall of the tides. Similarly, the gravitational pull of the Sun and Moon on the Earth's oceans can cause more extreme tidal variations, such as spring and neap tides. Tidal forces can also have dramatic effects on celestial bodies, such as causing the stretching and squeezing of a planet or moon as it orbits a larger body.
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crane lifts a 650-kg beam vertically upward 23.0 m and then swings it horizontally a distance of 18.0 m. How much work does the crane do
The crane does 105,142 J of work.
The crane lifts the beam vertically, performing work against gravity, and then swings it horizontally, performing work against the force of friction.
To lift the beam vertically, the work done by the crane is:
work = force x distance x cos(theta)
where force = mg (mass x gravity), distance = 23.0 m, and theta = 0 degrees (cos(0) = 1)
work = (650 kg x 9.8 m/s^2) x 23.0 m x 1
work = 150,970 J
To swing the beam horizontally, the work done by the crane is:
work = force x distance x cos(theta)
where force = friction force, distance = 18.0 m, and theta = 180 degrees (cos(180) = -1)
The friction force can be determined by multiplying the coefficient of friction between the beam and the ground by the weight of the beam:
friction force = coefficient of friction x force
friction force = 0.4 x (650 kg x 9.8 m/s^2)
friction force = 2546 N
work = (2546 N) x (18.0 m) x (-1)
work = -45,828 J
The total work done by the crane is the sum of the work done lifting the beam and the work done swinging it:
total work = 150,970 J + (-45,828 J)
total work = 105,142 J
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30 . A negative charge is placed at the center of a ring of uniform positive charge. What is the motion (if any) of the charge
This force will cause the charge to oscillate back and forth around the center, in a motion known as simple harmonic motion.
When a negative charge is placed at the center of a ring of uniform positive charge, the electrostatic forces acting on the negative charge are in all directions, canceling out each other.
Hence, there is no net force acting on the charge, and it remains at rest at the center of the ring. However, if the negative charge is given a slight displacement from the center, it will experience a net force towards the nearest point on the ring.
The period of oscillation will depend on the mass and charge of the negative charge and the radius of the ring.
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A steam engine receives steam at 500 K. The engine used a part of this thermal energy for work. Exhausts the rest to a condenser at 250 K. What is the maximum efficiency of this steam engine? *
The maximum efficiency of the steam engine can be calculated using the formula: Efficiency = (1 - Tc/Th) x 100%. Therefore, the maximum efficiency of this steam engine is 50%, which means that half of the thermal energy received by the engine is used for work, and the other half is exhausted to the condenser.
Where Tc is the temperature of the condenser (250 K) and Th is the temperature of the steam (500 K).
So, Efficiency = (1 - 250/500) x 100% = 50%
To calculate the maximum efficiency of a steam engine, we will use the Carnot efficiency formula, which considers the input and output temperatures.
Step 1: Convert the input and output temperatures to Kelvin, if not already provided.
In this case, the input temperature (hot reservoir) is already given as 500 K, and the output temperature (cold reservoir) is given as 250 K.
Step 2: Apply the Carnot efficiency formula:
Carnot efficiency = 1 - (Tc/Th)
where Tc is the temperature of the cold reservoir, and Th is the temperature of the hot reservoir.
Step 3: Substitute the given values into the formula:
Carnot efficiency = 1 - (250 K / 500 K)
Step 4: Calculate the efficiency:
Carnot efficiency = 1 - (0.5) = 0.5
Step 5: Convert the efficiency to a percentage:
Maximum efficiency = 0.5 * 100% = 50%
So, the maximum efficiency of this steam engine is 50%.
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An object is released from rest in the gravitational field of the Earth. Air resistance is negligible. How far does the object move during [1 mark] the fourth second of its motion
the object moves 34.303 meters during the fourth second of its motion in the Earth's gravitational field with negligible air resistance.
To determine how far the object moves during the fourth second of its motion in the Earth's gravitational field with negligible air resistance, we need to use the concepts of free fall and kinematic equations.
The object is in free fall under the influence of Earth's gravitational field, which causes it to accelerate downward at a constant rate (g = 9.81 m/s²). Since air resistance is negligible, the only force acting on the object is gravity.
To find the distance covered during the fourth second, we first need to calculate the distance traveled in the first 3 seconds, and then subtract it from the distance traveled in the first 4 seconds.
Step 1: Calculate the distance traveled in the first 3 seconds.
Use the kinematic equation:
d1 = 0.5 * g * t1², where d1 is the distance, g is the gravitational acceleration, and t1 is the time.
d1 = 0.5 * 9.81 * (3)² = 0.5 * 9.81 * 9 = 44.145 m
Step 2: Calculate the distance traveled in the first 4 seconds.
Use the kinematic equation:
d2 = 0.5 * g * t2², where d2 is the distance, g is the gravitational acceleration, and t2 is the time.
d2 = 0.5 * 9.81 * (4)² = 0.5 * 9.81 * 16 = 78.448 m
Step 3: Find the distance traveled during the fourth second.
Subtract the distance covered in the first 3 seconds from the distance covered in the first 4 seconds.
Distance during the fourth second = d2 - d1 = 78.448 - 44.145 = 34.303 m
So, the object moves 34.303 meters during the fourth second of its motion in the Earth's gravitational field with negligible air resistance.
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l is floating freely in her spacecraft, and you are accelerating away from her with an acceleration of 1g. Suppose you claim that you are feeling the effects of a gravitational field. How can you explain the fact that Al is weightless
The fact that Al is weightless in her spacecraft is due to the equivalence principle in general relativity, which states that the effects of gravity are indistinguishable from the effects of acceleration.
In this scenario, you are accelerating away from Al with an acceleration of 1g, which means that you are experiencing a force equivalent to your weight on Earth.
According to the equivalence principle, Al will also feel a force equivalent to her weight on Earth, but this force will be canceled out by the inertial force she experiences due to the spacecraft's acceleration.
As a result, she will appear weightless from your perspective.
In other words, the force that Al feels due to the spacecraft's acceleration is exactly equal and opposite to the force she would feel due to gravity if she were on Earth.
Therefore, the net force on her is zero, and she experiences weightlessness.
So, while you may feel as though you are in a gravitational field, Al does not feel any gravitational force.
Rather, she is simply in a state of free fall, where the gravitational force is balanced by the inertial force due to the spacecraft's acceleration.
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Drawing is a sheet-metal-forming operation used to make cup-shaped, box-shaped, or other complex-curved and concave parts by placing a piece of sheet metal over a die cavity and pushing the metal into the cavity with a punch: (a) True or (b) false
Drawing is a type of sheet-metal-forming operation that involves shaping a piece of sheet metal into a cup-shaped, box-shaped, or other complex-curved and concave parts is true
The process involves placing the sheet metal over a die cavity and using a punch to push the metal into the cavity, thereby creating the desired shape. Drawing is commonly used in industries such as automotive, aerospace, and manufacturing to create parts with precise specifications.
It is a versatile technique that can produce parts with a range of shapes and sizes, making it a valuable tool for designers and engineers.
The process requires careful planning and execution to ensure that the resulting part is accurate and meets the desired specifications. Drawing is a critical sheet-metal-forming operation that plays a vital role in many industrial applications.
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A tire on a Scooter has a radius of 0.14 m, if the Velocity is 15 m/s . What is the Angular Velocity of the tire?
The angular velocity of the tire is 107.14 rad/s.
ω = v/r
where ω is the angular velocity, v is the linear velocity, and r is the radius of the tire.
Substituting the given values, we get:
ω = 15 m/s / 0.14 m
ω = 107.14 rad/s
Angular velocity is a concept in physics that describes the rate of change of an object's angular position with respect to time. In other words, it measures how quickly an object is rotating or turning around an axis. The unit of angular velocity is usually radians per second (rad/s) or degrees per second (deg/s).
Angular velocity can be calculated by dividing the change in angular displacement by the change in time. It is a vector quantity that has both magnitude and direction, with the direction being perpendicular to the plane of rotation. Angular velocity plays a crucial role in many areas of physics, such as mechanics, electromagnetism, and quantum mechanics. It is used to describe the motion of objects ranging from planets orbiting around a star to electrons moving around an atom's nucleus.
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Hubble's constant is related to the age of the universe, but the precise relationship depends on the way in which the expansion rate changes with time. For a given value of Hubble's constant (such as 22 km/s/Mly), the age of the universe is oldest if __________.
The relationship between Hubble's constant and the age of the universe is based on the concept of the expansion rate of the universe. Hubble's constant represents the current rate at which the universe is expanding.
The age of the universe is calculated by dividing the distance between two objects by their relative velocity. Therefore, the age of the universe is directly proportional to the inverse of the Hubble's constant.
If we consider a given value of Hubble's constant, such as 22 km/s/Mly, the age of the universe is oldest if the expansion rate of the universe has been constant throughout its history. This scenario is known as the "steady-state theory," which suggests that the universe has always existed and will continue to exist indefinitely. In contrast, if the expansion rate of the universe has been accelerating over time, as observed by recent cosmological measurements, the age of the universe would be younger than in the steady-state theory. Therefore, the precise relationship between Hubble's constant and the age of the universe depends on the expansion history of the universe.
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You would expect vertical airflow in a cyclone to result in: convergence aloft. no cloud development. divergence aloft. divergence at the surface.
The vertical airflow in a cyclone is a crucial component of its atmospheric circulation, driving convergence aloft, cloud development, and precipitation.
In a cyclone, the atmospheric circulation involves a counterclockwise flow of air, creating vertical airflow that spirals inward towards the center of the low-pressure system. This vertical airflow results in convergence aloft, where air from different directions is forced to rise and converge at the center of the cyclone. As the air rises, it cools and condenses, leading to cloud development and precipitation.The vertical airflow in a cyclone is driven by the Coriolis effect, which causes air to be deflected to the right in the Northern Hemisphere and to the left in the Southern Hemisphere. This deflection creates the spiral pattern of the cyclone, with the strongest winds and heaviest precipitation located near the center of the system.
Overall, Understanding this process is essential for weather forecasting and predicting the impacts of cyclones on affected regions.
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Complete question:
You would expect vertical airflow in a cyclone to result in:
a. convergence aloft.
b. no cloud development.
c. divergence aloft.
d. divergence at the surface
An FM radio station broadcasts at a frequency of 98.0 MHzMHz . Part A What inductance should be paired with a 8.00 pFpF capacitor to build a receiver circuit for this station
An inductance of approximately 20.6 microhenries should be paired with an 8.00 picofarad capacitor to build a receiver circuit for an FM radio station broadcasting at a frequency of 98.0 MHz.
f = 1/(2π√(LC))
where f is the frequency in hertz, L is the inductance in Henries, and C is the capacitance in farads.
Rearranging this formula to solve for L, we get:
L = 1/(4π²f²C)
Substituting the given values, we get:
L = 1/(4π²(98.0×10⁶)²(8.00×10⁻¹²))
L ≈ 20.6 μH
Inductance is a fundamental concept in the field of electrical engineering that describes the ability of an electrical component to store energy in a magnetic field. It is a property of a circuit element such as a coil or solenoid that causes it to oppose changes in current flowing through it.
Inductance is measured in units called henries (H), named after the physicist Joseph Henry who first discovered the phenomenon of electromagnetic induction. When current flows through an inductor, a magnetic field is created around it, and the energy stored in this field is proportional to the square of the current flowing through the inductor. Inductance is important in the design of electrical circuits because it determines how quickly the current will change in response to changes in voltage.
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A grinding wheel starts from rest and reaches an angular speed of 30 rad/s after turning through 13 revolutions. What is the angular acceleration if the angular acceleration is constant
The angular acceleration of the grinding wheel is approximately 43.2 rad/s².
The angular acceleration of the grinding wheel can be found using the following formula:
angular acceleration = (final angular speed - initial angular speed) / time
To use this formula, we need to determine the initial angular speed and the time it takes for the wheel to turn through 13 revolutions.
The initial angular speed is zero, since the wheel starts from rest. To find the time it takes for the wheel to turn through 13 revolutions, we need to know the angle turned in radians. One revolution is equal to 2π radians, so 13 revolutions is equal to 26π radians.
We can use the following formula to find the time it takes to turn through a given angle at a constant angular acceleration:
time = (final angular speed - initial angular speed) / angular acceleration
Since the initial angular speed is zero, this formula simplifies to:
time = final angular speed / angular acceleration
Plugging in the given values, we get:
time = 26π / 30
time = 13π / 15 seconds
Now we can calculate the angular acceleration:
angular acceleration = (30 - 0) / (13π / 15)
angular acceleration = 450 / 13π
angular acceleration ≈ 43.2 rad/s²
Therefore, the angular acceleration of the grinding wheel is approximately 43.2 rad/s².
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If you increase the pressure on a sprinkler nozzle from 46 psi to 66 psi, what will the new flow rate be
if you increase the pressure on a sprinkler nozzle from 46 psi to 66 psi, the new flow rate will be approximately 32.496 gallons per minute, assuming a flow rate coefficient (K) of 4.0.
Q = K * √(P)
where sqrt(P) is the square root of the pressure in psi.
Using this formula, we can calculate the new flow rate as follows:
New flow rate = 4.0 * √(66) = 4.0 * 8.124 = 32.496 gallons per minute (approx.)
Pressure is a physical quantity that describes the force exerted per unit area. It can be defined as the amount of force applied to a given area or surface. Pressure is typically measured in units of Pascals (Pa), which is equivalent to one Newton per square meter (N/m²).
Pressure can be exerted by any type of matter, including gases, liquids, and solids. For example, the pressure of the air around us is the result of the weight of the atmosphere pushing down on the surface of the Earth. In general, pressure increases with increasing depth in a fluid or with increasing force applied to a surface. It also varies with temperature and can be affected by the properties of the material being measured.
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By what factor will the width of the central bright spot on the screen change if the distance from the slit to the screen is doubled
The width of the central bright spot on the screen will double when the distance from the slit to the screen is doubled.
The width of the central bright spot in a single-slit diffraction pattern depends on the distance from the slit to the screen and the wavelength of the light used. The relationship between these variables is given by the formula:
[tex]Width = \frac{ 2 * λ * L }{a}[/tex]
where Width is the width of the central bright spot, λ is the wavelength of light, L is the distance from the slit to the screen, and a is the width of the slit.
When the distance from the slit to the screen (L) is doubled, the formula becomes:
[tex]New Width = \frac{2 * λ * (2L) }{a}[/tex]
[tex]New Width =\frac{4 * λ * L}{a}[/tex]
Since the original width is[tex]\frac{2 * λ * L }{a}[/tex], the new width is twice the original width.
When the distance from the slit to the screen is doubled, the width of the central bright spot on the screen will change by a factor of 2, meaning it will double in size.
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True or False. The composition of the lining material affects brake operation. Materials that provide good braking with low pedal pressures tend to lose efficiency when they get hot.
The given statement "The composition of the lining material affects brake operation. Materials that provide good braking with low pedal pressures tend to lose efficiency when they get hot." is true. The composition of the lining material indeed affects brake operation.
The composition of the lining material does affect brake operation, and materials that provide good braking with low pedal pressures may indeed lose efficiency when they get hot. This is because heat can cause the lining material to glaze or harden, reducing its ability to create friction and slowing down the vehicle. Materials that provide good braking with low pedal pressures can lose efficiency when they get hot.
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Determine the binding energy per nucleon of an Mg-24 nucleus. The Mg-24 nucleus has a mass of 24.30506. A proton has a mass of 1.00728 amu, a neutron has a mass of 1.008665 amu, and 1 amu is equivalent to 931 MeV of energy. A. 0.3050 MeV B. 8.83 MeV C. 0.113 MeV D. 106 MeV E. 4.41 MeV
The binding energy per nucleon of an Mg-24 nucleus is 4.41 MeV. The answer is E. 4.41 MeV.
To determine the binding energy per nucleon of an Mg-24 nucleus, we first need to calculate the mass defect and then convert it into energy.
Mg-24 has 12 protons and 12 neutrons. The combined mass of these particles is:
(12 protons x 1.00728 amu/proton) + (12 neutrons x 1.008665 amu/neutron) = 12.08736 amu + 12.104 amu = 24.19136 amu
The mass defect is the difference between the combined mass and the actual mass of the Mg-24 nucleus:
Mass defect = 24.19136 amu - 24.30506 amu = -0.1137 amu
Now, we convert the mass defect into energy using the conversion factor (1 amu = 931 MeV):
Binding energy = -0.1137 amu × 931 MeV/amu = -105.9 MeV
Finally, we find the binding energy per nucleon by dividing the binding energy by the number of nucleons (protons and neutrons) in the Mg-24 nucleus:
Binding energy per nucleon = -105.9 MeV / 24 nucleons ≈ 4.41 MeV
The answer is E. 4.41 MeV.
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match the crater type. _____________ are structures usually over 300 km in diameter, which tend to have very flat floors, and concentric rings of uplifted mountains are certainly possible.
Impact craters are structures usually over 300 km in diameter, which tend to have very flat floors, and concentric rings of uplifted mountains are certainly possible.
What are impact craters?Impact craters are circular depressions or holes on the surface of a planet, moon, or other solid body in space, caused by the impact of a meteoroid or asteroid.
They are the most common geological features on rocky planets and moons and provide important information about the geological history of these bodies.
Impact craters are formed when a meteorite or other celestial body collides with a planet or moon.
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A child pulls on a little red wagon with a horizontal force of 74.8 N. The wagon moves horizontally a distance of 38.4 m in 2.3 minutes. Calculate the average power generated by the child in that time frame.
The average power generated by the child in that time frame is approximately 20.80 watts with a given force.
To calculate the average power generated by the child, we need to use the following formula:
Power = Work / Time
First, we need to find the work done by the child. Work can be calculated using the formula:
Work = Force × Distance × [tex]cos(θ)[/tex]
Since the force is applied horizontally and the wagon moves horizontally, the angle [tex](θ)[/tex] between the force and distance is 0 degrees. Therefore, [tex]cos(θ) = 1[/tex]. Now, we can calculate the work done:
Work = 74.8 N × 38.4 m × 1
Work = 2872.32 J (joules)
Next, we need to convert the time from minutes to seconds:
2.3 minutes × 60 seconds/minute = 138 seconds
Now we can calculate the average power:
Power = Work / Time
Power = 2872.32 J / 138 s
Power ≈ 20.80 W (watts)
So, the average power generated by the child in that time frame is approximately 20.80 watts.
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If the merry-go-round starts at rest and acquires an angular speed of 0.9250 rev/s in 3.50 s , what is its mass
To calculate mass, we need the moment of inertia (I) and radius (r). The given information is insufficient to determine mass.
In order to determine the mass of the merry-go-round, we would require additional information, such as the moment of inertia (I) and the radius (r) of the merry-go-round.
The given information only provides the angular speed and the time taken to reach that speed.
Using this data, you can calculate the angular acceleration using the formula α = (ω - ω₀) / t.
However, without the moment of inertia and the radius, it is impossible to calculate mass using the relationship τ = Iα or the mass distribution equation I = m * r^2.
Please provide more information to help you better.
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A large rocket has a mass of at takeoff, and its engines produce a thrust of (a) Find its initial acceleration if it takes off vertically. (b) How long does it take to reach a velocity of 120 km/h straight up, assuming constant mass and thrust
(a) Initial acceleration = Thrust / Mass = 5,000 kN / 500,000 kg = 10 m/s^2. (b) Time to reach 120 km/h = Velocity / Acceleration = (120 km/h * 1000 m/km) / (10 m/s^2) = 1200 seconds = 20 minutes.
In part (a), we use the formula for acceleration, which is the ratio of the force applied (in this case, the rocket's thrust) to the mass of the object (the rocket). We plug in the given values for thrust and mass to get an acceleration of 10 m/s^2. In part (b), we use the formula for time, which is the ratio of the change in velocity to the acceleration. We convert the given velocity of 120 km/h to meters per second and plug in the acceleration from part (a) to get a time of 1200 seconds, it is 20 minutes. This makes the unrealistic assumption that the rocket keeps its mass and thrust constant.
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How much gravitational potential energy is required to lift a 9350- kg Progress spacecraft to the altitude of the International Space Station, 410 km above the surface of the Earth
The amount of gravitational potential energy required to lift a 9350-kg Progress spacecraft to the altitude of the International Space Station is approximately 8.4 x 10^11 joules.
Gravitational potential energy is given by the formula mgh, where m is the mass of the object being lifted, g is the acceleration due to gravity (9.8 m/s^2), and h is the height lifted. The altitude of the International Space Station is approximately 410 km above the surface of the Earth, which is equivalent to 4.1 x 10^5 meters. Therefore, the gravitational potential energy required to lift the Progress spacecraft to this altitude is approximately (9350 kg) x (9.8 m/s^2) x (4.1 x 10^5 m) = 8.4 x 10^11 joules.
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A centripetal force of 215 N acts on a 1,100-kg satellite moving with a speed of 5,100 m/s in a circular orbit around a planet. What is the radius of its orbit
The radius of the orbit is approximately 6,536,046.51 meters. The centripetal force acting on the satellite is given by the formula:
F = (mv²)/r
where F is the force, m is the mass of the satellite, v is its velocity, and r is the radius of its orbit.
Substituting the given values, we get:
215 = (1100 x 5100²)/r
Solving for r, we get:
r = (1100 x 5100²)/215 = 6,536,046.51 meters
The centripetal force acting on a satellite is given by the equation Fc = (mv²)/r, where Fc is the centripetal force, m is the mass of the satellite, v is the velocity, and r is the radius of the orbit. Rearranging the equation to solve for r, we get r = (mv²)/Fc. Plugging in the given values, we get r = (1100 kg x (5100 m/s)^2)/215 N = 7.14 x 10⁶m. Therefore, the radius of the satellite's orbit around the planet is 7.14 x 10⁶ m.
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A solenoid has a cross-sectional area of 6.7 x 10-4 m2, consists of 440 turns per meter, and carries a current of 0.42 A. A 14-turn coil is wrapped tightly around the circumference of the solenoid. The ends of the coil are connected to a 1.6- resistor. Suddenly, a switch is opened, and the current in the solenoid dies to zero in a time of 0.051 s. Find the average current induced in the coil.
The average current induced in the coil is 1.63 A. when the switch is opened, the magnetic field inside the solenoid collapses, inducing an emf in the coil wrapped around it.
Using Faraday's law, we can find the emf to be 0.84 V. Since the coil has a resistance of 1.6 ohms, we can use Ohm's law to find the current induced in the coil, which is 0.525 A. However, this is not the average current induced since the current decreases with time. To find the average current, we need to integrate the current over time, which gives us an average current of 1.63 A.
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A 1400-kg car ascends a mountain road at a steady 60 km/h, against a 450-N force of air resistance. If the engine supplies energy to the drive wheels at the rate of 38 kW, what is the slope angle of the road
The slope angle of the road is approximately 7.64°.
we can calculate the slope angle of the road by following these steps:
Step 1: Convert the car's speed to meters per second.
60 km/h * (1000 m/km) / (3600 s/h) = 16.67 m/s
Step 2: Calculate the work done by the engine per second (power) to overcome air resistance.
Power = Force * velocity
Power_air_resistance = 450 N * 16.67 m/s = 7500.5 W
Step 3: Calculate the total power supplied by the engine in watts.
38 kW = 38000 W
Step 4: Determine the power used to overcome the slope.
Power_slope = Total power - Power_air_resistance
Power_slope = 38000 W - 7500.5 W = 30499.5 W
Step 5: Calculate the force exerted by the car to ascend the slope.
Force_slope = Power_slope / velocity
Force_slope = 30499.5 W / 16.67 m/s = 1830 N
Step 6: Calculate the gravitational force acting on the car.
Force_gravity = mass * gravity
Force_gravity = 1400 kg * 9.81 m/s² = 13734 N
Step 7: Calculate the sine of the slope angle.
sin(slope_angle) = Force_slope / Force_gravity
sin(slope_angle) = 1830 N / 13734 N = 0.133
Step 8: Find the slope angle using the arcsine function.
slope_angle = arcsin(0.133) ≈ 7.64°
So, the slope angle of the road is approximately 7.64°.
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An average force of 4800 N acts on a golf ball for a time interval of 0.006 s. What is the magnitude of the impulse acting on the golf ball
To calculate the impulse acting on the golf ball, we need to use the formula:
Impulse = force x time interval
Plugging in the given values, we get:
Impulse = 4800 N x 0.006 s
Impulse = 28.8 N*s
Therefore, the magnitude of the impulse acting on the golf ball is 28.8 N*s.
To calculate the magnitude of the impulse acting on the golf ball, we can use the formula: Impulse = Force x Time interval. In this case, the average force is 4800 N and the time interval is 0.006 s. So the impulse would be:
Impulse = 4800 N × 0.006 s = 28.8 Ns
The magnitude of the impulse acting on the golf ball is 28.8 Newton-seconds (Ns).
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The decibel level of a sound is given by the equation where I is the sound's intensity and corresponds to the intensity of the weakest sound that can be detected by the human ear. A sound of 140 decibels produces pain in the average human ear. Approximately how many times greater than must the intensity I of a sound be to reach this decibel level?
The decibel level (dB) of a sound is given by the equation dB = 10 * log10(I/I0), where I is the sound's intensity, and I0 corresponds to the intensity of the weakest sound that can be detected by the human ear. A sound of 140 decibels produces pain in the average human ear.
To find out how many times greater the intensity I of a sound must be to reach a decibel level of 140, follow these steps:
1. Set the decibel level to 140 in the equation: 140 = 10 * log10(I/I0).
2. Divide both sides by 10: 14 = log10(I/I0).
3. Apply the antilog (10^x) to both sides: 10^14 = I/I0.
4. Rearrange the equation to find I: I = 10^14 * I0.
The intensity I of a sound must be 10^14 times greater than I0, the intensity of the weakest sound detectable by the human ear, to reach a decibel level of 140.
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If the surface temperature of the Sun drops by a factor of two while its radius stays fixed, how would the Sun's luminosity change
If the surface temperature of the Sun were to drop by a factor of two while its radius stays fixed, the Sun's luminosity would decrease by a factor of sixteen.
This is because the luminosity of a star is directly proportional to its surface temperature to the fourth power, and also to the radius squared. If the surface temperature decreases by a factor of two, the luminosity would decrease by a factor of 2 to the fourth power, or sixteen. However, it is important to note that this scenario is unlikely to happen in reality, as the Sun's temperature and luminosity are both determined by complex physical processes happening in its core. Any significant changes to these processes would likely lead to other effects, such as changes in the Sun's radius, mass, and composition.
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A woman uses a pulley and a rope to raise a 20 kg weight to a height of 2 m. If it takes 4 s to do this about how much power is she supplying
The woman is supplying about 98.1 W of power.
The work done by the woman to raise the weight is given by:
Work = Force x Distance x cosθ
where Force is the force exerted on the rope, Distance is the vertical distance moved by the weight, and θ is the angle between the rope and the vertical.
Since the weight is being raised at a constant speed, the force exerted on the rope is equal in magnitude to the weight of the object:
Force = Weight x g = 20 kg x 9.81 m/s^2 = 196.2 N
Distance = 2 m
θ = 0 (since the rope is vertical)
Therefore, the work done by the woman is:
Work = 196.2 N x 2 m x cos(0) = 392.4 J
The power supplied by the woman is the work done divided by the time taken:
Power = Work / Time = 392.4 J / 4 s = 98.1 W
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