Answer:
To make it around the circle, the tension in the string must provide the necessary centripetal force to keep the ball moving in a circle. At the top of the circle, the tension in the string must provide all the force to keep the ball moving in a circle. At the bottom of the circle, the tension in the string must provide the centripetal force in addition to the force of gravity.
We can use the centripetal force formula to solve for the minimum velocity: F_c = m * a_c
where F_c is the centripetal force, m is the mass of the ball, and a_c is the centripetal acceleration.
At the top of the circle, the centripetal force is equal to the tension in the string: F_c = T
where T is the tension in the string.
At the bottom of the circle, the centripetal force is equal to the sum of the tension in the string and the force of gravity:
F_c = T + mg
where m is the mass of the ball, g is the acceleration due to gravity (9.8 m/s^2), and T is the tension in the string.
The centripetal acceleration is given by: a_c = v^2 / r
where v is the velocity of the ball and r is the radius of the circle.
Since the circle has a radius of 0.33 m, we can substitute this into the equation for a_c: a_c = v^2 / 0.33
Combining these equations, we get:
At the top of the circle: T = m * v^2 / 0.33
At the bottom of the circle: T + mg = m * v^2 / 0.33
We can solve for the minimum velocity by using these two equations to eliminate the tension in the string: m * v^2 / 0.33 + mg = m * v^2 / 0.33
Simplifying this equation, we get: v = sqrt(0.33 * g)
Plugging in the values, we get: v = sqrt(0.33 * 9.8) = 1.81 m/s
Therefore, the minimum velocity that the ball must have to make it around the circle is 1.81 m/s
Green light has a wavelength of 5. 20 x 10^-7m. The speed of light is 3. 00 * 10^8 m/s. What is the frequency of green light waves? show your work
The required frequency of green light waves when the wavelength and the speed of light are specified is calculated to be 5.77× 10¹⁴ hz.
Wavelength of green light is given as 5.2 × 10⁻⁷ m.
The speed of light is given as 3× 10⁸ m/s.
We know the relation between wavelength, frequency and speed of light as,
λ = c/ν
where,
λ is wavelength
c is speed of light
ν is frequency
To find out frequency, let us make it as subject,
ν = c/λ = (3× 10⁸)/(5.2 × 10⁻⁷) = 0.577 × 10¹⁵ hz = 5.77× 10¹⁴ hz
Thus, the frequency is calculated to be 5.77× 10¹⁴ hz.
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besides the stars, what seven heavenly bodies could the ancient astronomers observe with the unaided eye?
The following are the seven heavenly bodies that the ancient astronomers could observe with the unaided eye: Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn
Step by step explanation:
Planets are some of the seven heavenly bodies that ancient astronomers could observe with the unaided eye besides the stars. The Greeks knew these seven as planets, which means wandering stars. In their nighttime skies, the planets, unlike the stars, moved. The names of the planets were taken from ancient Roman mythology. The Greeks, for example, identified the planet that could be seen moving back and forth across the sky as Hermes, their messenger god.
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since the moon cooled sooner than the earth, it is reasonable to assume that it no longer has a molten metal core. if that is the case, what conclusion would you draw about the magnetic fields around the moon?
The conclusion that could be drawn about the magnetic fields around the moon is that "the moon no longer has a magnetic field."
What causes magnetic fields around celestial objects?Planets like Earth that have a liquid metal outer core produce magnetic fields. It's said that the planet's rotation causes the magnetic field. When the planet spins, the molten metal in the core moves, producing an electric current. As a result of the moving electric current, a magnetic field is formed around the planet.
Moons that do not have a molten metal core cannot produce magnetic fields. The moon's magnetic field is significantly weaker than Earth's magnetic field. The surface of the moon is scorched by the sun's radiation due to the absence of a magnetic field. So, the conclusion that can be drawn about the magnetic fields around the moon is that the moon no longer has a magnetic field.
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Telescopes Homework . Unanswered Suppose we have a 1-m and 3-m diameter telescope. How does the light gathering power of the 3-m telescope compare to the 1-m telescope? Select an answer and submit. For keyboard navigation, use the up/down arrow keys to select an answer. a It is 9 times smaller b It is 3 times smaller c They are the same d It is 3 times bigger It is 9 times bigger
d.It is 3 times bigger It is 9 times bigger. The 3-m telescope has 9 times the light-gathering capacity of the 1-m telescope. It is nine times larger, to be precise.
The light-gathering power of a telescope is directly proportional to the square of its diameter. Therefore, a 3-m telescope has nine times the light-gathering power of a 1-m telescope. This is because the area of the 3-m telescope is nine times greater than the area of the 1-m telescope. In other words, a 3-m telescope can collect nine times more light in the same amount of time than a 1-m telescope. This increased light-gathering power enables the 3-m telescope to observe fainter and more distant objects than the 1-m telescope. Larger telescopes are, therefore, crucial for astronomers to study the most distant and faintest objects in the universe.
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True or False,the indirect method is used to determine total power in a parallel circuit when that power is determined from the total current, total resistance, and source voltage.
True, the indirect method is used to determine total power in a parallel circuit when that power is determined from the total current, total resistance, and source voltage.
What is an indirect method?The indirect method of calculating power in a parallel circuit is used when it is not feasible to measure the current flowing through each individual resistor. It is found by multiplying the total resistance of the circuit (RT) by the square of the total current (IT), or by using the total voltage (VT) squared and dividing by the total resistance (RT).
The indirect method is used to determine total power in a parallel circuit when that power is determined from the total current, total resistance, and source voltage. The equation to use for this is Power = Voltage x Current. Therefore, the total power in a parallel circuit can be determined by multiplying the source voltage by the total current, divided by the total resistance.
The formula to calculate power is given by P = IV, where P stands for power, I stands for current, and V stands for voltage. Power is usually measured in watts (W), current is measured in amperes (A), and voltage is measured in volts (V).A parallel circuit consists of multiple paths, each containing a resistor.
The current through each resistor in a parallel circuit varies, and each resistor has its own voltage drop. The total resistance of a parallel circuit is less than the smallest resistance in the circuit.
The formula for calculating total power in a parallel circuit is
P = IT² × RT,
where IT is the total current and RT is the total resistance.
This formula assumes that the total voltage of the circuit is known. The formula can also be written as
P = VT²/RT,
where VT is the total voltage in the circuit.
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Suppose a neutron star with a mass of about 1.5MSun and a radius of 10 kilometers suddenly appeared in your hometown. How thick a layer would Earth form as it wraps around the neutron star's surface? Assume that the layer formed by Earth has the same average density as the neutron star. (Hint: Consider the mass of Earth to be distributed in a spherical shell over the surface of the neutron star and then calculate the thickness of such a shell with the same mass as Earth. The volume of a spherical shell is approximately its surface area times its thickness: Vshell=4πr^2×h. Because the shell will be thin, you can assume that its radius is the radius of the neutron star.)Express your answer to two significant figures and include the appropriate units.
Earth would form a layer around the neutron star with a thickness of 6.2 km.
Mass of the neutron star = 1.5 MSun. Radius of the neutron star = 10 km. Let's assume that the layer formed by Earth has the same average density as the neutron star. Since the mass of the neutron star is 1.5 MSun, this means that Earth will wrap around the neutron star's surface in a spherical shell over the surface of the neutron star whose mass is equal to the mass of the Earth.
Let's first calculate the volume of the neutron star, VNS:VNS = (4/3)πr³= (4/3)π(10 km)³= 4,188.8 km³. We can now calculate the mass of the neutron star, MNS, using its average density, D, which is:
D = MNS / VNS 1.5 MSun = MNS / 4,188.8 km³. Therefore, MNS = (1.5 MSun)(4,188.8 km³) = 6,283.2 MSun.We know that the thickness, h, of the shell is needed to calculate the volume, Vshell, of the spherical shell with the same mass as Earth. The volume of a spherical shell is approximately its surface area times its thickness: Vshell=4πr^2.h, so we can now use the above equation to calculate h.h = Vshell / (4πr²)= MEarth / (D × 4πr²). Where MEarth is the mass of the Earth. MEarth = 5.97 × 10²⁴ kgD = MNS / VNS = (6,283.2 MSun) / (4,188.8 km³) = 1.50 × 10¹⁷ kg/km³r = 10 km. Putting in these values:h = (5.97 × 10²⁴ kg) / (1.50 × 10¹⁷ kg/km³ × 4π(10 km)²) = 6.2 km.
Therefore, Earth would form a layer around the neutron star with a thickness of 6.2 km.
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If E an is absolutely convergent and (bn) is bounded sequence show that convergent. Gabn is absolutely Give an example to show that if the convergence 0l (n is conditional and (bn) is bounded sequence then anbn may diverge. Liii) Give A example of a convergent series (n,Such that 02 is not convergent
First, let's prove that if [tex]$\sum_{n=1}^\infty |a_n|$[/tex] is absolutely convergent and [tex]$(b_n)$[/tex] is a bounded sequence, then [tex]$\sum_{n=1}^\infty a_n b_n$[/tex] is convergent.
Since [tex]$(b_n)$[/tex] is bounded, there exists some positive constant [tex]$M$[/tex] such that [tex]$|b_n| \leq M$[/tex] for all [tex]$n \in \mathbb{N}$[/tex]. Then, for any [tex]$n \in \mathbb{N}$[/tex], we have:
[tex]$$|a_n b_n| \leq |a_n| \cdot |b_n| \leq M \cdot |a_n|$$[/tex]
Since [tex]$\sum_{n=1}^\infty |a_n|$[/tex] is absolutely convergent, we know that [tex]$\sum_{n=1}^\infty M|a_n|$[/tex] is also convergent, by comparison. Thus, by the comparison test, we can conclude that [tex]$\sum_{n=1}^\infty |a_n b_n|$[/tex] is convergent.
Now, to give an example to show that if [tex]$\sum_{n=1}^\infty a_n$[/tex] is conditionally convergent and [tex]$(b_n)$[/tex] is a bounded sequence, then [tex]$\sum_{n=1}^\infty a_n b_n$[/tex] may diverge, consider the following:
Let [tex]$a_n = \frac{(-1)^n}{n}$[/tex] and [tex]$b_n = 1$[/tex] for all [tex]$n \in \mathbb{N}$[/tex]. Then [tex]$\sum_{n=1}^\infty a_n = -\ln(2)$[/tex] is conditionally convergent, and [tex]$(b_n)$[/tex] is clearly a bounded sequence. However,
[tex]$\sum_{n=1}^\infty a_n b_n = \sum_{n=1}^\infty \frac{(-1)^n}{n} = \ln(2)$[/tex]
which diverges.
Finally, to give an example of a convergent series [tex]$\sum_{n=1}^\infty a_n$[/tex] that [tex]$\sum_{n=1}^\infty |a_{2n}|$[/tex] diverges, consider the following:
Let [tex]$a_n = \frac{(-1)^n}{n}$[/tex] for all [tex]$n \in \mathbb{N}$[/tex]. Then [tex]$\sum_{n=1}^\infty a_n$[/tex] converges conditionally to [tex]$-\ln(2)$[/tex], but [tex]$\sum_{n=1}^\infty |a_{2n}| = \sum_{n=1}^\infty \frac{1}{2n}$[/tex] diverges.
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Lab: Electromagnetic Induction: Instructions Click the links to open the resources below. These resources will help you complete the assignment. Once you have created your file(s) and are ready to upload your assignment, click the Add Files button below and select each file from your desktop or network folder. Upload each file separately. Your work will not be submitted to your teacher until you click Submit.
To complete the lab assignment on Electromagnetic Induction, first click the links to open the resources provided.
This will help you complete the task.
After creating the file(s) and once you are ready to submit your assignment,
click the 'Add Files' button and select each file from your desktop or network folder.
Remember to upload each file separately. Once you have uploaded the files, click 'Submit' to submit your work to your teacher.
In this lab, you are expected to understand and apply the concept of Electromagnetic Induction.
Electromagnetic Induction is a process where a varying magnetic field creates an electric field.
The electric field then induces a current in a nearby circuit. This current is caused by Faraday's law of induction.
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a clean nickel surface is exposed to light with a wavelength of 241 nm n m . the photoelectric work function for nickel is 5.10 ev e v . for related problem-solving tips and strategies, you may want to view a video tutor solution of a photoelectric-effect experiment. part a what is the maximum speed of the photoelectrons emitted from this surface?
The maximum speed of the photoelectrons emitted from the clean nickel surface is 6.70 × 10⁵ m/s.
Calculate the energy of a photon.E = hc/λwhere, h = Planck’s constant = 6.626 × 10⁻³⁴ Js, c = speed of light = 3 × 10⁸ m/sE = 6.626 × 10⁻³⁴ × 3 × 10⁸/241 × 10⁻⁹E = 8.21 × 10⁻¹⁸ J
Calculate the kinetic energy of the photoelectrons.
K.E. = E – W₀K.E. = 8.21 × 10⁻¹⁸ J – 5.10 × 1.6 × 10⁻¹⁹ J = 7.09 × 10⁻¹⁹ J
K.E. = 1/2 mv² where, m = mass of photoelectron, v = velocity of photoelectron, and K.E. = kinetic energy of photoelectronv = √(2K.E./m) = √[(2 × 7.09 × 10⁻¹⁹ J)/(9.1 × 10⁻³¹ kg)]v = 6.70 × 10⁵ m/s or 0.224c
So, the maximum speed of the photoelectrons emitted from this surface is 6.70 × 10⁵ m/s.
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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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an early submersible craft for deep-sea exploration was raised and lowered by a cable from a ship. when the craft was stationary, the tension in the cable was 5500 n . when the craft was lowered or raised at a steady rate, the motion through the water added an 1800 n drag force.
Part A
What was the tension in the cable when the craft was being lowered to the seafloor?
Express your answer to two significant figures and include the appropriate units.
Part B
What was the tension in the cable when the craft was being raised from the seafloor?
Express your answer to two significant figures and include the appropriate units.
Part A: When the craft is being lowered, the tension in the cable is 6387 N
Part B: When the craft is being raised, the tension in the cable is 5227 N
The weight of the craft will be equal to the force of gravity acting on it, which can be calculated using the mass of the craft and the acceleration due to gravity (g = 9.81 m/s²).
Therefore, the tension in the cable when the craft is being lowered is:
Tension = weight + drag force
Tension = (mass x g) + drag force
Tension = (unknown mass x 9.81 m/s²) + 1800 N
Tension = (unknown mass x 9.81) + 1800 N
Part A When the craft is stationary, the tension in the cable is 5500 N. This means that the weight of the craft is equal to the tension in the cable when it's not moving,
Solving for the mass:
5500 N = (mass x 9.81) + 0 N
mass = 5500 N / 9.81 m/s²
mass = 560.3 kg
Now we can substitute the mass into the expression for tension when the craft is being lowered:
Tension = (mass x 9.81) + 1800 N
Tension = (560.3 kg x 9.81 m/s²) + 1800 N
Tension = 6387 N
Therefore, the tension in the cable when the craft is being lowered to the seafloor is 6387 N.
Part B: When the craft is being raised at a steady rate, the tension in the cable will be equal to the weight of the craft minus the drag force due to the motion through the water.
Using the same mass of the craft that we calculated in Part A, we can calculate the tension in the cable when the craft is being raised:
Tension = weight - drag force
Tension = (mass x g) - drag force
Tension = (560.3 kg x 9.81 m/s²) - 1800 N
Tension = 5227 N
Therefore, the tension in the cable when the craft is being raised from the seafloor is 5227 N.
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it is proposed that future space stations create an artificial gravity by rotating. suppose a space station is constructed as a 1600-m -diameter cylinder that rotates about its axis. the inside surface is the deck of the space station. you may want to review (pages 186 - 189) .
The speed of rotation which is required to simulate the Earth's gravity in this space station is approximately 88.4 m/s.
What is the speed of rotation?When future space stations rotate, they create an artificial gravity. Let's suppose a space station is constructed as a cylinder with a diameter of 1600 m that rotates about its axis, with the inside surface being the deck of the space station.
The centripetal force of the rotation provides the artificial gravity. The magnitude of this force is:
F = mv²/r,
where, m is the mass of the object, v is the speed of rotation, and r is the radius of rotation. The force is perpendicular to the direction of motion and towards the center of rotation.
To calculate the speed of rotation required to simulate Earth's gravity (g = 9.81 m/s²), we need to first find the radius of rotation. The radius is half the diameter of the cylinder, so it is r = 800 m.
F = mv²/r
mg = mv²/r
v² = gr
v = √(gr)
v = √(9.81 m/s² × 800 m)
v = 88.4 m/s
Therefore, the speed of rotation required to simulate Earth's gravity in this space station is 88.4 m/s.
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A 2 kg mass and a 6 kg mass are attached to either end of a 3 m long massless rod.
Find the rotational inertia (I) of the system when rotated about:
a.) Find the center of mass of the system.
b.) the end with the 2 kg mass.
c.) the end with the 6 kg mass.
d.) the center of the rod.
e.) the center of mass of the system.
The center of mass of the system is 2.75 meters from the 2 kg mass. The rotational inertia of the system at the end with the 2 kg mass is 6 kg. This can be calculated with the help of mass and distance.
The total mass of the system, the total mass is: 2 kg + 6 kg = 8 kg.
To find the center of mass, we will divide the mass of each end by the total mass and multiply it by the length of the rod. For the 2 kg mass, we get:
(2/8) × 3m = 0.75m.
For the 6 kg mass, we get (6/8) × 3m = 2.25m.
The center of mass is the sum of the two distances, or 2.75m from the 2 kg mass.
The rotational inertia of the system when rotated about the end with the 2 kg mass is:
I = (1/3) × 2 kg × (3m)² = 6 kg m².
The rotational inertia of the system when rotated about the end with the 6 kg mass is:
I = (1/3) × 6 kg × (3m)² = 18 kg m².
The rotational inertia of the system when rotated about the center of the rod is:
I = (1/2) × 8 × (1.5m)² = 12 kg m².
The rotational inertia of the system when rotated about the center of mass is:
I = (1/2) × 8 kg × (2.75m)² = 24.5 kg m².
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A 5 kg particle moves along an x axis, being propelled by a variable force directed along that axis. Its position is given by x = 3 m + (5 m/s)t + ct2 - (4 m/s3)t3 with x in meters and t in seconds.The factor c is a constant. At t = 3 s the force on the particle has a magnitude of 33 N and is in the negative direction of the axis. What is c?
To answer this question, we need to determine the acceleration of the particle by differentiating its position equation twice with respect to time. After finding the acceleration, we can use the force-mass-acceleration relationship to calculate c.
We have the Mass of particle = m = 5 kg
Position of particle, x = 3 + 5t + ct² - 4t³ m
Force on the particle at t = 3 s, F = -33 N (negative direction of the axis)
Using the given equation, we can differentiate to get the acceleration of the particle with respect to time. Taking the Derivative of x with respect to time, we get the velocity of the particle:
v = dx/dt= 5 + 2ct - 12t² ... (i)
Taking the derivative of v with respect to time, we get the acceleration of the particle:
a = dv/dt= 2c - 24t ... (ii)
Now, we can use the relation F = ma to get c.
Therefore, a=F/m
a=-33/5
5(2c - 24t) = 5a
=> 2c - 24t = -33/5
At t = 3 s,
2c - 72 = -33/5
=> c = [(-33/5) + 72]/2= 32.7 m/s²
Therefore, the value of c is 32.7 m/s².
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A 0.45 kg dodge ball is thrown at an opposing player at a velocity of 38 m/s to the right. Unfortunately, it misses the player and bounces off the wall at 28 m/s to the left.
What is the impulse of the ball hitting the wall?
Answer:
The impulse of the ball hitting the wall can be calculated using the impulse-momentum theorem, which states that the impulse of a force is equal to the change in momentum it produces:
Impulse = Change in momentum
The change in momentum of the ball can be calculated as follows:
Change in momentum = Final momentum - Initial momentum
The final momentum of the ball can be calculated using the mass and velocity of the ball after bouncing off the wall:
Final momentum = mass x velocity
Final momentum = 0.45 kg x (-28 m/s) (since the ball is moving to the left)
Final momentum = -12.6 kg m/s
The initial momentum of the ball can be calculated using the mass and velocity of the ball before hitting the wall:
Initial momentum = mass x velocity
Initial momentum = 0.45 kg x 38 m/s (since the ball is moving to the right)
Initial momentum = 17.1 kg m/s
Therefore, the change in momentum of the ball is:
Change in momentum = -12.6 kg m/s - 17.1 kg m/s
Change in momentum = -29.7 kg m/s
Since impulse is equal to the change in momentum, the impulse of the ball hitting the wall is:
Impulse = Change in momentum
Impulse = -29.7 kg m/s
Therefore, the impulse of the ball hitting the wall is 29.7 kg m/s to the left.
Explanation:
A student wants to use the output from the aux port on their phone to play music from their speakers. The aux port supplies 5v and a max current of 0.015A, but the speakers need 12v and a max current of 1.5A. You decide to use a power transistor to amplify the signal from the aux port. What does the beta value of your chosen transistor need to be to amplify the current enough?
pls explain or elaborate the answer if u can!!
Answer:The beta value of a transistor represents the current gain, which is the ratio of the collector current to the base current. In this case, we want to use the transistor as an amplifier to increase the current from the 0.015A supplied by the phone to the 1.5A required by the speakers.
The required current gain can be calculated using the following formula:
Beta = (Ic / Ib)
Where:
Beta is the current gain of the transistor
Ic is the collector current (output current)
Ib is the base current (input current)
To find the required beta value, we need to first calculate the base current required to drive the transistor. We can use Ohm's Law to do this:
Ib = V / R
Where:
Ib is the base current
V is the voltage supplied by the phone (5V)
R is the input resistance of the transistor circuit
Assuming an input resistance of 1kΩ, the base current required is:
Ib = V / R = 5 / 1000 = 0.005A (5mA)
Now, we can calculate the required collector current using the maximum current required by the speakers:
Ic = 1.5A
Finally, we can calculate the required beta value:
Beta = Ic / Ib = 1.5 / 0.005 = 300
Therefore, we need to choose a power transistor with a beta value of at least 300 to amplify the current from the aux port enough to drive the speakers.
Explanation:
g as a prank, someone drops a water-filled balloon out of a window. the balloon is released from rest at a height of 10.0 m above the ears of a man who is the target. then, because of a guilty conscience, the prankster shouts a warning after the balloon is released. the warning will do no good, however, if shouted after the balloon reaches a certain point, even if the man could react infinitely quickly. assuming that the air temperature is 20 c and ignoring the effect of air resistance on the balloon, determine how far above the man's ears this point is.
The point at which the warning will do no good is 7.50 m above the man's ears.
When a water-filled balloon is released from rest at a height of 10.0 m above the ears of a man, the warning will do no good if shouted after the balloon reaches a certain point. Assuming that the air temperature is 20°C and ignoring the effect of air resistance, this point is 7.50 m above the man's ears.
The vertical displacement (d) can be determined using the equation [tex]d = \frac{vf2}{2g}[/tex], where vf is the final velocity and g is the acceleration due to gravity (9.81 m/s2).
Since the balloon was released from rest, the initial velocity is 0 m/s. Therefore, [tex]d = \frac{02 }{ 2} (\frac{9.81 m}{s2} ) = 0[/tex]m. Since the initial height was 10.0 m, the final height is 10.0 m + 0 m = 10.0 m.
The point at which the warning will do no good is 7.50 m above the man's ears, so the final height of the balloon must be 10.0 m - 7.50 m = 2.50 m.
Therefore, the point at which the warning will do no good is 7.50 m above the man's ears.
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blocks with masses of 2 kg , 4 kg , and 6 kg are lined up in a row on a frictionless table. all three are pushed forward by a 56 n force applied to the 2 kg block. part a how much force does the 4 kg block exert on the 6 kg block? express your answer to two significant figures and include the appropriate units. activate to select the appropriates template from the following choices. operate up and down arrow for selection and press enter to choose the input value typeactivate to select the appropriates symbol from the following choices. operate up and down arrow for selection and press enter to choose the input value type f
The force exerted by the 4 kg block on the 6 kg block can be is 0 N
Step-by-step explanation:
Newton's Third Law states that for every action there is an equal and opposite reaction. This means that the force exerted by the 4 kg block on the 6 kg block is equal in magnitude and opposite in direction to the force exerted by the 6 kg block on the 4 kg block.
Mass of first block ([tex]m_1[/tex]) = 2 kg
Mass of second block ([tex]m_2[/tex]) = 4 kg
Mass of third block ([tex]m_3[/tex]) = 6 kg
Force applied (F) = 56 N
To find: The force exerted by the 4 kg block on the 6 kg block
Let's assume that the blocks are numbered 1, 2, and 3 from left to right. Then, the force applied to the 2 kg block is given as: [tex]F_1[/tex] = 56 N
According to Newton's Third Law of Motion, the force exerted by block 1 on block 2 ([tex]F_1[/tex] on 2) and the force exerted by block 2 on block 1 ([tex]F_2[/tex] on 1) will be equal and opposite in direction. This means that:
[tex]F_1[/tex] on 2 = [tex]- F_2[/tex] on 1
This can be rearranged to give: [tex]F_2[/tex] on 1 = [tex]- F_1[/tex] on 2
Substituting the values, we get: [tex]F_2[/tex] on 1 = -56 N
Similarly, the force exerted by block 2 on block 3 ([tex]F_2[/tex] on 3) and the force exerted by block 3 on block 2 ([tex]F_2[/tex] on 2) will be equal and opposite in direction. This means that: [tex]F_2[/tex] on 3 = [tex]- F_3[/tex] on 2
This can be rearranged to give: [tex]F_3[/tex] on 2 = [tex]- F_2[/tex] on 3
Now, to find the force exerted by the 4 kg block on the 6 kg block ([tex]F_4[/tex] on 6), we need to determine the force exerted by the 6 kg block on the 4 kg block ([tex]F_6[/tex] on 4). Since the force exerted by the 4 kg block on the 6 kg block is equal in magnitude and opposite in direction to the force exerted by the 6 kg block on the 4 kg block, we can use the value of [tex]F_6[/tex] on 4
to find [tex]F_4[/tex] on 6. Using Newton's Second Law of Motion,
we know that : F = ma
Where F is the force applied,
m is the mass of the object, and
a is the acceleration produced by the force.
[tex]F_1[/tex] on 2 = -56 N is the net force on block 2 since no other external forces are acting on it.
Using the same equation for blocks 2 and 3: [tex]F_2[/tex] on 3 = [tex]-F_1[/tex] on 2 = 56 N
Since the blocks are on a frictionless surface, the net force on the system of three blocks is equal to:
[tex]F_n_e_t[/tex] = [tex]F_1 + F_2 + F_3[/tex] = m * a
Where, [tex]F_1[/tex] = 56 N (force applied to the 2 kg block)
[tex]F_2[/tex] = -56 N (force exerted by the 2 kg block on the 4 kg block)
[tex]F_3[/tex] = 56 N (force exerted by the 4 kg block on the 6 kg block)
m = 2 + 4 + 6 = 12 kg (total mass of the three blocks)
a = [tex]F_N_e_t[/tex]/m = (56 - 56 + 56) / 12 = 0 N/kg
Since the system is frictionless, the force required to accelerate each block is the same. This means that the force exerted by block 6 on block 4 ([tex]F_6[/tex] on 4) is equal in magnitude and opposite in direction to the force exerted by block 4 on block 6 ([tex]F_4[/tex] on 6).
Using the same equation as before:
[tex]F_4[/tex] on 6 = [tex]-F_6[/tex] on 4
Now, to find [tex]F_6[/tex] on 4,
we use the same equation that we used earlier: F = ma
The mass (m) is now 4 kg since we are considering blocks 4 and 6.
[tex]F_6[/tex] on 4 = m * a
Since the force required to accelerate each block is the same, the acceleration produced by the force applied (56 N) is the same for all three blocks.
Therefore, we can use the value of a that we obtained earlier.
a = 0 N/kg (since the blocks are on a frictionless surface)
[tex]F_6[/tex] on 4 = 4 kg * 0 N/kg = 0 N
Therefore, [tex]F_4[/tex] on 6 = - [tex]F_6[/tex] on 4 = 0 N.
Answer: 0 N.
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what is the single most important property of a star that will determine its evolution?
The single most important property of a star that determines its evolution is its mass.
A star's mass determines its internal temperature, pressure, and nuclear reactions, which drive its energy production and ultimately its evolution. Low-mass stars, like red dwarfs, have relatively low internal temperatures and undergo a slow process of fusion that can last for trillions of years. On the other hand, high-mass stars, like blue giants, have much higher internal temperatures and undergo fusion much more quickly, leading to a shorter lifespan.
The mass of a star also determines whether it will eventually evolve into a white dwarf, neutron star, or black hole, making it the single most important factor in a star's evolution.
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the circular structures on the surface of the moon are the result of
The circular structures on the surface of the Moon are the result of impact craters formed by the impact of asteroids or comets.
The Moon's lack of atmosphere and tectonic activity means that its surface has remained largely unchanged for billions of years, preserving evidence of the impacts that have occurred over its history. When an object collides with the Moon's surface, it creates a shock wave that radiates outward, blasting away material and creating a circular depression.
The size and shape of the resulting crater depends on the size, speed, and angle of impact, as well as the properties of the target material. These craters provide valuable information about the history of the Moon and the Solar System, as well as insights into the formation and evolution of planetary bodies.
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bright streak of light in the sky as air is heated by debris falling from space called
A bright streak of light in the sky as air is heated by debris falling from space is called a meteor or shooting star.
Meteors are created when small pieces of interplanetary debris, such as fragments of comets or asteroids, enter the Earth's atmosphere at high speed. As these pieces of debris encounter the Earth's atmosphere, they collide with air molecules and are heated to extremely high temperatures, causing them to emit light and appear as bright streaks in the sky.
Most meteors burn up completely before reaching the ground, although larger fragments may survive and strike the Earth's surface as meteorites. Meteors are a common occurrence and can be observed during meteor showers, which occur when the Earth passes through a trail of debris left behind by a comet or asteroid.
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Can we use our brainly points.
What did the triangle say to the circle?
Your pointless
Answer:
i actually giggled at that oml.
Explanation:
that was good
Burl and Paul have a total weight of 1300 N. The tensions in the ropes that support the scaffold they stand on add to 1800 N. The weight of the scaffold itself must beA. 400 NB. 500 NC. 600 ND. 800 N
Burl and Paul have a total weight of 1300 N. The tensions in the ropes that support the scaffold they stand on add to 1800 N. The weight of the scaffold itself must be 500 N.
What is a scaffold?A scaffold is a temporary structure that is erected to support workers and their equipment when they are performing a job at a height above the ground. In the construction sector, it is widely used, and it is made up of one or more platforms that are supported by a system of frames and poles.
In order to solve the given problem, we'll have to use some mathematical concepts such as addition and subtraction. The total weight of Burl and Paul = 1300 N
The tensions in the ropes that support the scaffold they stand on = 1800 N
Let us suppose that the weight of the scaffold is x.
So, from the given data, we can write down the following equation:
Total weight of Burl, Paul, and the scaffold = Tensions in the ropes + weight of the scaffold
1300 + x = 1800x = 1800 - 1300= 500 N
Therefore, the weight of the scaffold is 500 N.
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a waterbed heater uses 450 w of power. it is on 35 % of the time, off 65 % . part a what is the annual cost of electricity at a billing rate of $0.13 per kwhr ? express your answer using two significant figures.
The annual cost of electricity at a billing rate of $0.13 per kWhr for a waterbed heater that uses 450 W of power is $36.51.
What is the usage of the waterbed heater in a day?For the calculation of the energy consumed, one must know the energy consumed by the heater per day. The energy consumed in one day can be calculated by multiplying the power consumed by the hours the heater is used. The power consumed by the heater is 450 W.
The heater is used 35% of the time and is off 65% of the time. The percentage of time the heater is used is calculated using the formula:
Percentage of time the heater is used = (Time heater is on/Total time) × 100
Percentage of time the heater is used = (35/100) × 100
Percentage of time the heater is used = 35%
The percentage of time the heater is off is calculated using the formula:
Percentage of time the heater is off = (Time heater is off/Total time) × 100
Percentage of time the heater is off = (65/100) × 100
Percentage of time the heater is off = 65%
Thus, the heater is used for 8.4 hours per day (i.e., 24 hours × 35%) and is off for 15.6 hours per day (i.e., 24 hours × 65%).
The energy consumed per day can be calculated by multiplying the power consumed by the time the heater is on. Energy consumed per day = Power consumed × Time heater is on
Energy consumed per day = 450 W × 8.4 hours
Energy consumed per day = 3780 Wh
Energy consumed per day = 3.78 kWh
The annual cost of electricity can be calculated by multiplying the energy consumed per year by the cost of electricity per kWh.
Annual cost of electricity = Energy consumed per year × Cost of electricity per kWh
Annual cost of electricity = 3.78 kWh × $0.13/kWh
Annual cost of electricity = $0.4914/day
Annual cost of electricity = $179.31/year
Hence, the annual cost of electricity at a billing rate of $0.13 per kWhr for a waterbed heater that uses 450 W of power is $36.51.
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We think that extrasolar Neptune-sized planets likely have big compositional differences when compared to our own Neptune because they O probably have a different formation history O have measured densities that span a factor of 1000 O have migrated so that we can see them O all formed closer to their stars
Extrasolar Neptune-sized planets likely have big compositional differences when compared to our own Neptune because they have measured densities that span a factor of 1000.
Neptune is the fourth-largest planet in our solar system, and it is a gas giant similar to Jupiter, Saturn, and Uranus. An extrasolar Neptune-sized planet (also known as an exo-Neptune) is a planet that is Neptune-sized but orbits a star other than the sun.
Exo-Neptunes are often observed using the transit technique, in which the planet passes in front of the star, causing a small drop in brightness that can be detected by telescopes on Earth. As a result, their densities can be calculated by measuring their mass and size.
Exo-Neptunes have measured densities that span a factor of 1000, meaning that their compositions can be vastly different from that of our own Neptune, which has a density of 1.64 g/cm³. This suggests that they may have different formation histories, be composed of different materials, or have different atmospheric conditions.
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Sam (85 kg) takes off up a 50-m-high, 10 degree frictionless slope on his jet-powered skis. The skis have a thrust of 220 N. He keeps his skis tilted at 10 degree after becoming airborne. How far does Sam land from the base of the cliff?
Sam (85 kg) takes off up a 50-m-high, 10 degree frictionless slope on his jet-powered skis. The skis have a thrust of 220 N. He keeps his skis tilted at 10 degree after becoming airborne. Sam lands about 109.9 meters from the base of the cliff.
To solve this problem, we can use the conservation of energy principle. At the bottom of the slope, all of Sam's energy is in the form of potential energy:
Potential energy = mgh
where m is Sam's mass (85 kg), g is the acceleration due to gravity [tex](9.81 m/s^2)[/tex], and h is the height of the slope (50 m).
Potential energy = [tex](85 kg) \times (9.81 m/s^2) \times (50 m) = 41,287.5 J[/tex]
As Sam takes off up the slope, his potential energy is converted to kinetic energy and then to a combination of kinetic and potential energy as he becomes airborne. We can use the conservation of energy to find Sam's speed at the top of the slope:
Potential energy at bottom = Kinetic energy at top
[tex]mgh = (1/2)mv^2[/tex]
where v is Sam's speed at the top of the slope.
[tex]v = \sqrt{(2gh)} = \sqrt{(2 \times 9.81 m/s^2 \times 50 m)} = 31.3 m/s[/tex]
Now, we can use Sam's speed and the angle of his skis to find his horizontal velocity:
Horizontal velocity = v cos(theta)
where theta is the angle of the skis after becoming airborne (10 degrees).
Horizontal velocity = 31.3 m/s x cos(10 degrees) = 30.2 m/s
Finally, we can use the horizontal velocity and Sam's hang time to find the distance he travels:
Distance = Horizontal velocity x Hang time
where hang time is the time Sam spends in the air. Hang time can be found using the formula:
Hang time = (2v sin(theta)) / g
Hang time = (2 x 31.3 m/s x sin(10 degrees)) / 9.81 [tex]m/s^2[/tex] = 3.64 s
Distance = 30.2 m/s x 3.64 s = 109.9 m
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A 900.0kg car is traveling at 11.0m/s. What is the momentum of this car?
The momentum of the car is 9900 kg m/s.
What is momentum?
The momentum of an object is defined as the product of its mass and velocity. In this case, the momentum of the car can be calculated using the following formula:
Momentum = mass x velocity
Here, the mass of the car is 900.0 kg and its velocity is 11.0 m/s. Substituting these values into the formula, we get:
Momentum = 900.0 kg x 11.0 m/s
Momentum = 9900 kg m/s
Therefore, the momentum of the car is 9900 kg m/s.
Note that the units of momentum are kilogram meters per second (kg m/s), which are derived from the units of mass (kg) and velocity (m/s). Momentum is a vector quantity, meaning it has both magnitude and direction, and its direction is the same as the direction of motion of the object.
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discuss whether the values found in parts (a) and (b) seem consistent with the fact that tidal effects with earth have caused the moon to rotate with one side always facing earth.
Yes, the values found in parts (a) and (b) are consistent with the fact that tidal effects with earth have caused the moon to rotate with one side always facing earth.
This is because part (a) states that the moon rotates on its axis in the same amount of time it takes to complete one orbit around the Earth, which is a phenomenon known as tidal locking. Part (b) further indicates that the same side of the moon always faces the Earth, further supporting the notion that tidal effects have caused the moon to rotate with one side always facing Earth.
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Three dimensions. Three point particles are fixed in place in any xyz coordinate system. Particle A, at the origin, has mass m A . Particle B, at xyz , coordinates (2.00d,2.00d), has mass 2.00 m A , and particle C, at coordinates ( - 1.00d , 2.00d, -3.00d ), has mass the other particles. In terms of distance d, at what (a) x, (b) y, and (c) z coordinate should D be placed so that the net gravitational force on A from B, C, and D is zero
In order for the net gravitational force on particle A from particles B, C, and D to be zero, particle D must be placed at x = 0, y = 4d, and z = 0.
This can be calculated using Newton's law of universal gravitation, which states that the gravitational force between two objects is directly proportional to the product of their masses, and inversely proportional to the square of the distance between them. Therefore, the net gravitational force can be calculated by considering the gravitational force between each pair of particles and summing the results.
For particle A, the gravitational force due to B, C, and D will be:
FAB = (G*m*2m) / (d²) ,
FAC = (G*m*2m) / ((-d)²) ,
FAD = (G*m*2m) / ((y-d)²).
For particle D, the gravitational force due to B, C, and A will be:
FDB = (G*2m*m) / (d²) ,
FDC = (G*2m*m) / ((-d)²) ,
FDA = (G*2m*m) / ((y-d)²).
Adding these forces together and equating them to zero yields the coordinates for particle D: x = 0, y = 4d, and z = 0.
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a pump is to move water from a lake into a large, pressurized tank as shown in the figure at a rate of 1000 gal in 10 min or less. will a pump that adds 3 hp to the water work for this purpose? support your answer with appropriate calculations. repeat the problem if the tank were pressurized to 3, rather than 2, atmospheres.
A 3 hp pump would be used to move water from a lake into a large, pressurized tank.
To solve,
P = F × V,
where P is the power, F is the force, and V is the velocity of the water.
We know the power is 3 hp and the velocity is 1000 gal/10 min, so we can solve for F:
F = P ÷ V = 3 hp ÷ 1000 gal/10 min
= 0.003 hp/gal/min.
Now, if the tank is pressurized to 3 atmospheres, the pressure will increase the force needed to move the water.
So, the equation for pressure is P = F × A, where P is the pressure, F is the force, and A is the area.
We know the pressure is 3 atmospheres and the force is 0.003 hp/gal/min, so we can solve for A:
A = P ÷ F = 3 atmospheres ÷ 0.003 hp/gal/min
= 1000 gal/10 min/3 atmospheres.
Therefore, a 3 hp pump will work for this purpose, even if the tank is pressurized to 3 atmospheres.
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