To find the magnitude of the initial acceleration of end B after the string on side B is cut,
1. Calculate the gravitational force acting on the rod: Fg = m * g, where m is the mass (1.6 kg) and g is the acceleration due to gravity (approximately 9.81 m/s²). Fg = 1.6 kg * 9.81 m/s² ≈ 15.7 N.
2. Find the torque τ about end A: τ = Fg * d, where d is the distance from the center of mass of the rod to end A. Since the rod is uniform, the center of mass is at the middle, so d = 55 cm / 2 = 27.5 cm = 0.275 m. τ = 15.7 N * 0.275 m ≈ 4.33 Nm.
3. Calculate the moment of inertia I of the rod about end A: I = (1/3) * m * L², where L is the length of the rod. I = (1/3) * 1.6 kg * (0.55 m)² ≈ 0.099 kg m².
4. Determine the angular acceleration α: α = τ / I. α = 4.33 Nm / 0.099 kg m² ≈ 43.7 rad/s².
5. Calculate the linear acceleration a of end B: a = α * L. a = 43.7 rad/s² * 0.55 m ≈ 24.03 m/s².
The magnitude of the initial acceleration of end B is approximately 24.03 m/s².
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What velocity of a body will you obtain from the position vs.
time graph for the following data: position from origin is 0 m, 10
m, 20 m, 30 m and 40 m at instants 0 s, 1 s, 2 s, 3 s, 4 s?
Answer:10 m/s
Explanation:
a girl weighing 455 n jumps from a tree, and her center of mass falls a vertical distance of 1.50 m. find the impulse necessary to bring her to rest.
The impulse necessary to bring her to rest is zero (0 Ns). Taking into account that the girl's momentum was maintained even as she fell, and since she started from rest, her final momentum should also be zero. So no additional push is needed beyond what gravity provides.
To find the impulse necessary to bring the girl to rest, we need to use the principle of conservation of momentum, which states that the total momentum of a system is conserved in the absence of external forces. In this case, we can assume that the girl is initially at rest, so her initial momentum is zero.
When the girl jumps from the tree, she is subject to the force of gravity, which causes her to accelerate downwards. We can use the equation for the gravitational potential energy to find the work done by gravity:
[tex]W = mgh[/tex]
Where W is the work done by gravity, m is the mass of the girl, g is the acceleration due to gravity, and h is the vertical distance that the center of mass falls.
Plugging in the given values, we get:
[tex]W = (455 N)(1,50 m)(9,81 m/s^2) \\W= 6.717,08 J[/tex]
This work done by gravity is equal to the change in kinetic energy of the girl, which can be expressed as the impulse required to bring her to rest:
J = ΔK
[tex]J= -mv[/tex]
where J is the impulse, ΔK is the change in kinetic energy, m is the mass of the girl, and v is her final velocity. Since the girl comes to a stop, her final velocity is zero, so we can simplify the equation to:
[tex]J = mv[/tex]
Plugging in the given mass and solving for the impulse, we get:
[tex]J = (455 N)(-0 m/s) \\J = 0 Ns[/tex]
Therefore, the impulse necessary to bring the girl to rest is zero.
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what is the purpose of wires in a circuit? why do we use wires to connect power supplies to resistors or other objects on a circuit board? why can't we just use power supplies and resistors?
The purpose of wires in a circuit is to provide a path for electric current to flow.
We use wires to connect power supplies to resistors or other objects on a circuit board because these objects do not have a direct electrical connection. If we did not use wires, electric current would not flow from the power supply to the resistor or other object.
Wires are essential components in a circuit because they provide the pathway for electricity to flow from one component to another. Without wires, the flow of electric current would be impossible, and a circuit would not work.In a circuit board, power supplies are connected to resistors and other objects using wires.
The power supply provides the voltage, while the resistor or other object provides the resistance. By connecting the power supply to the resistor or other object using wires, we create a complete circuit. Without wires, the power supply and resistor would be unable to communicate with each other, and the circuit would not function properly.
In conclusion, wires are an essential component of a circuit. They provide a pathway for electric current to flow, allowing power supplies and resistors to communicate with each other and create a complete circuit.
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Compared to a landscape that develops in a cool, dry climate, a landscape that develops in a warm, rainy climate will most likely weather and erode a. Slower, so the landforms are more angular b. Slower, so the landforms are more rounded c. Faster, so the landforms are more angular d. Faster, so the landforms are more rounded
A landscape that develops in a warm, rainy climate will most likely weather and erode faster, so the landforms are more rounded.
This is because in a warm, rainy climate, there is more water available to weather and erode the landforms. The water can penetrate cracks and crevices in the rocks, dissolve minerals, and carry away sediments. Over time, this can lead to the rounding of edges and the smoothing of surfaces, resulting in more rounded landforms.
In contrast, in a cool, dry climate, there is less water available to weather and erode the landforms. This can result in slower rates of erosion and less rounding of the landforms.
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how do the light-collecting area and best possible angular resolution of telescope with a 10-meter diameter mirror compare to that of a telescope with a 5-meter diameter mirror?
Angular resolution and light-collecting area:
The light-collecting area of a telescope is the amount of light that the mirror can collect. It is critical in astronomy because the brighter the star or galaxy you are looking at, the more information you can gather.
The angular resolution, on the other hand, is a measurement of the minimum angle between two stars that can be distinguished using a telescope. A high angular resolution means that you can see objects more clearly.
A telescope with a 10-meter diameter mirror has a four times larger light-collecting area and twice the best possible angular resolution compared to a telescope with a 5-meter diameter mirror. Therefore, a larger telescope will provide better images of objects in space because it gathers more light and can see more clearly.
The light-collecting area and best possible angular resolution of the telescope depending on the size of the mirror or lens used. This is why larger telescopes are better suited for astronomical observation than smaller ones.
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b) what happens to the reaction rate when the concentration (absorbance) of the reactants is quadrupled? determine the reaction order by solving the following equations. show a sample computation in your lab notebook.
Rate 4/ Rate 2 = [CV 4]’/[CV 2]’ <-> X = ________ Rate 5/ Rate 3 = [CV 5]’/[CV 3]’ <-> X = ________
When the concentration of the reactants is quadrupled, the reaction rate depends on the reaction order. To determine the reaction order, we can solve the given equations:
1.[tex]Rate 4 / Rate 2 = [CV 4]'^x / [CV 2]'^x[/tex]
2.[tex]Rate 5 / Rate 3 = [CV 5]'^x / [CV 3]'^x[/tex]
To find the reaction order (x), we first need to know the values of the rates (Rate 4, Rate 2, Rate 5, Rate 3) and the concentrations (CV 4, CV 2, CV 5, CV 3). Once you have these values, you can plug them into the equations and solve for x.
For example, let's say the given values are:
Rate 4 = 8, Rate 2 = 2, Rate 5 = 10, Rate 3 = 1
CV 4 = 4, CV 2 = 1, CV 5 = 5, CV 3 = 2
Now plug these values into the equations:
1.[tex]8 / 2 = (4^x) / (1^x)[/tex]
2. [tex]10 / 1 = (5^x) / (2^x)[/tex]
Solve for x:
1. [tex]4 = 4^x[/tex]
2. [tex]10 = (5^x) / (2^x)[/tex]
From equation 1, we can deduce that x = 1 (since 4^1 = 4). Thus, the reaction order is 1, which means the reaction rate is directly proportional to the concentration of the reactants. Therefore, when the concentration of the reactants is quadrupled, the reaction rate will also be quadrupled.
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every atom (other than hydrogen and helium) that you see around us, making up everything including the earth, is literally group of answer choices from the big bang star stuff, from stars
Every atom other than hydrogen and helium that we see around us is actually the result of nucleosynthesis, a process of nuclear fusion in stars that creates heavier elements.
During nucleosynthesis, two hydrogen atoms collide and form helium, which is then subjected to intense pressures and temperatures that allow the helium to fuse into heavier elements such as,
oxygen, nitrogen, and carbon. This process repeats until the heavier elements that form the core of stars, like iron and nickel, are created.
The process of fusion is ongoing and eventually the star runs out of fuel and explodes in a supernova, releasing the material that was created within it.
This material is then scattered across the universe, eventually forming clouds of gas and dust that coalesce to create planets, moons, and other bodies, including Earth.
All of the atoms that make up our planet, from oxygen to iron, are the direct result of this process, which began in the big bang and continues to the present day.
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65. a 150-w lightbulb emits 5% of its energy as electromagnetic radiation. what is the radiation pressure on an absorbing sphere of radius 10 m that surrounds the bulb?
The radiation pressure on an absorbing sphere of radius 10 m that surrounds the lightbulb is approximately 3.98 x 10^-13 Pa.
The radiation pressure on an absorbing sphere can be calculated using the formula,
P = (2 * I) / c
where P is the radiation pressure, I is the intensity of the radiation, and c is the speed of light.
First, we need to calculate the intensity of the radiation emitted by the lightbulb. The energy emitted per second by the lightbulb is 150 W, and 5% of this energy is emitted as electromagnetic radiation. Therefore, the energy emitted as radiation is,
E = 150 W * 0.05 = 7.5 W
The intensity of the radiation is the power per unit area, and can be calculated by dividing the energy emitted per second by the surface area of a sphere with a radius of 10 m,
I = E / (4 * pi * r^2) = 7.5 W / (4 * pi * 10^2 m^2) = 5.98 x 10^-5 W/m^2
Now we can calculate the radiation pressure, P = (2 * I) / c = (2 * 5.98 x 10^-5 W/m^2) / 3 x 10^8 m/s = 3.98 x 10^-13 Pa
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in august of 2006, the iau (international astronomical union) published an official definition what it means to be a planet. what criteria is needed for that classification? why is pluto no longer considered a full fledged planet?
In August of 2006, the International Astronomical Union (IAU) published an official definition of what it means to be a planet.
The criteria required for that classification are:
The object must be in orbit around the sun.The object must be spherical or nearly spherical.The object must have cleared the neighborhood around its orbit.Pluto is no longer considered a full-fledged planet because it has not satisfied the third condition mentioned above. According to the IAU, Pluto has not cleared the neighborhood around its orbit.
That is, Pluto shares its orbit with numerous other objects in the Kuiper Belt region and therefore does not have a clear path around the sun. This led to the IAU redefining Pluto as a dwarf planet in 2006, which means that it is still classified as a planet but is no longer considered a full-fledged planet.
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Air at atmospheric pressure of inside a of Hg is trapped availaible 760mm. container piston. The piston is so that the volume 100 km² to 150 dm³. the with a moveable pulled out slowly is increased from temperature remaining constant. What will be presture of the air?answer of this numerical?????
If the piston is positioned so that the volume is between 100 km² and 150 dm³, the air pressure within the container is 506.67 mm Hg. the from a moveable drawn out slowly while the temperature stays the same.
How do you determine air pressure?We can rewrite the equation as P = nRT/V using the ideal gas law, where PV = nRT, where P is pressure, V is volume, n is number of moles of gas, R is ideal gas constant, and T is temperature.
We can assume that n, R, and T are constants because the temperature doesn't change. Hence, we can write:
P1V1 = P2V2
P1(100) = P2 x (150)
Upon solving for P2, we obtain:
P2 = (P1 x V1) / V2
P2 = 506.67 mmHg
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What is the magnitude of the applied electric field inside an aluminum wire of radius 1. 0 mm
that carries a 4. 0- A
current? [
σaluminum
= 3. 6 ×
10 7
A/(V⋅m)
]
The following formula may be used to determine how large the electric field is within the aluminium wire:
E = J/σ
E, J, and are the electric field, the current density, and the conductivity of aluminium, respectively.
where A is the wire's cross-sectional area and I is the current.
The following formula may be used to get the cross-sectional area of the wire:
A = πr^2
where r is the wire's radius.
We obtain the following by substituting the aluminum's electrical conductivity value from the problem:
E = J/σ
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true or false: energy is the capacity to do work and work is anything that involves moving matter against an opposing force.
The given statement "Energy is the capacity to do work and work is anything that involves moving matter against an opposing force" is TRUE. Energy is the capacity to do work, which is defined as any action that requires the application of a force to move matter. This includes tasks such as lifting a book, pushing a door open, or running.
Energy refers to the capacity of a physical system to perform work. Energy is generally used to complete tasks, such as moving an object from one location to another, heating up or cooling down a material, or lighting up a room. Work is defined as the transfer of energy to an object via a force applied to the object over a given distance, as per the statement. Work is usually identified as the displacement of an object through a force applied to it in the direction of its displacement against an opposing force.Energy and work are two distinct but interrelated concepts in physics. Energy is the capacity to perform work, and work is the transfer of energy from one object to another through a force acting over a distance. Energy and work are both expressed in joules (J), the unit of energy in the International System of Units (SI).
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trying to solve this please i need help asap
The force from student is positive, the force due to gravity is zero and the frictional force due to air is negative.
Given the distance of the bag from the room = 3m
From the diagram we can see that there are three different forces acting on the bag such as:
Fs : force from the student
FG: Force due to gravity
f: force of friction from air
Here we can say that according to the free-body diagram:
The force from from student(Fs) is acting upwards and is positive since the student is pushing the bag across the room, the force from the student (Fs) is doing positive work on the bag.
The force due to gravity(FG) is acting downwards and is zero since the bag is moving in a level room, the force of gravity (FG) is parallel to the motion of the bag and therefore isn't doing any work on the bag.
The work done by the frictional force of air (f) on the bag is negative since it is opposing the displacement of the bag.
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a 300n force is applied to a bolt by a wrench at 180 degrees. the length of the wrench is 0.2m. what is the torque? justify your answer.
Torque is the rotational force acting on an object due to a force applied at a certain distance away from its pivot point. Since the force is 300N and the wrench is 0.2m away from the pivot point, the torque is 300N * 0.2m, which equals 60Nm.
The torque is the result of the force applied by a wrench multiplied by the length of the wrench. In this case, the force applied is 300N and the length of the wrench is 0.2m, so the torque is 60Nm (300N x 0.2m = 60Nm). Justification of this answer can be seen using the definition of torque. Torque is defined as the product of the magnitude of the force applied, and the distance from the force to the axis of rotation. In this case, the force of 300N is being applied at 180 degrees, so the distance from the force to the axis of rotation is 0.2m (the length of the wrench). Therefore, the torque is equal to the force multiplied by the distance, which is 60Nm (300N x 0.2m = 60Nm).
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is it possible for an observer to travel fast enough so that in his system the earthquake happens also exactly now?
Yes, it is theoretically possible for an observer to travel fast enough so that in his system the earthquake happens also exactly now. This is due to the fact that time slows down as an object approaches the speed of light, a phenomenon known as time dilation.
The equation for time dilation states that the elapsed time T observed in the frame of reference of an observer travelling at velocity v is given by
[tex]T = T0 / \sqrt{(1 - v^2/c^2)}[/tex] ,
where ,T0 is the elapsed time as observed from the reference frame of an observer at rest relative to the travelling object, c is the speed of light, and v is the velocity of the travelling object. Therefore, the greater the velocity of the travelling object, the slower the elapsed time in its reference frame.
For an observer to travel fast enough so that in his system the earthquake happens also exactly now, he would need to travel at a velocity equal to or greater than the speed of light. This is impossible according to Einstein's theory of relativity, since nothing can travel faster than the speed of light in a vacuum.
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if it rotates through 8.00 revolutions in the first 2.50 s , how many more revolutions will it rotate through in the next 5.00 s ?
The object will rotate through 16.00 revolutions in the next 5.00s if it rotates through 8.00 revolutions in the first 2.50s.
The first step to answer this question is to determine the rotational speed (angular velocity) of the object. To do this, we use the formula:
Angular velocity = number of revolutions / time
So, the angular velocity of the object is given by:
Angular velocity = 8.00 revolutions / 2.50 s
Angular velocity = 3.20 revolutions per second
Now, we can use this angular velocity to determine the number of revolutions the object will rotate through in the next 5.00 s. To do this, we use the formula:Number of revolutions = angular velocity x time
So, the number of revolutions the object will rotate through in the next 5.00 s is given by:
Number of revolutions = 3.20 revolutions per second x 5.00 s
Number of revolutions = 16.00 revolutions
Therefore, the object will rotate through 16.00 revolutions in the next 5.00 s.
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what observation can you make that allows you to determine the relative magnitudes of the forces on the upper book?
Observing the reaction of the book when placed on the table, we can determine the relative magnitudes of the forces on the upper book. If the book stays in place, then the magnitude of the normal force is equal to the gravitational force. If the book slides down, then the gravitational force is greater than the normal force, and if the book slides up, then the normal force is greater than the gravitational force.
To determine the relative magnitudes of the forces on the upper book, we can observe the reaction of the book when placed on the table. If the book stays in place and does not move, then the forces on the upper book are in balance, meaning that the magnitude of the normal force is equal to the gravitational force.
To explain further, the normal force is the force that the table exerts on the book. It opposes the force of gravity, which is the force of attraction between the book and the Earth. When the normal force is equal to the gravitational force, the book is in equilibrium, meaning that it stays in place. When the gravitational force is greater than the normal force, the book slides down, and when the normal force is greater than the gravitational force, the book slides up.
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the acceleration of a super-vehicle is proportional to the difference between 240 km/h and the velocity of this sports car. if it can accelerate from rest to 120 km/h in one second, what speed can it reach from rest in three seconds?
The speed that the car can reach from rest in three seconds is 79.73 km/hr.
The acceleration of a super-vehicle is proportional to the difference between 240 km/h and the velocity of this sports car.
Initial speed u = 0 km/hr,
Final speed v = ? t
Time t = 3 s,
Velocity at a particular time = v,
Acceleration = proportional to the difference between 240 km/h and the velocity of this sports car Given acceleration is proportional to the difference between 240 km/h and the velocity of this sports car
So, a ∝ (240 - v)To find constant of proportionality k, Let's assume acceleration when velocity is 0 is 100m/s² when t=1sWhen v=0, a=k(240 - 0) = 240k ⇒ 100=k(240 - 0) = 240k ⇒ 100=k
Therefore acceleration is a=100(240-v)When t=3 seconds, u=0km/hr, v=? and a=100(240-v)Using the formula, v=u+atWe get, v = u + at=0+(100(240 - v)) * 3v = 24000 - 300v⇒ 301v = 24000⇒ v = 79.73 km/hr
Therefore, the speed that the car can reach from rest in three seconds is 79.73 km/hr.
Note: While solving these types of questions, we should try to find out the constant of proportionality and then substitute the values to get the result.
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The work function for barium is 2. 48ev. If light of 400nm is shined on barium cathode. What is the maximum velocity of the ejected electron?
The work function for barium is 2.48eV. If light of 400nm is shined on the barium cathode, the maximum velocity of the ejected electron is 4.54 × 105 m/s.
Energy can be transferred from electromagnetic radiation to matter in the form of photons. The energy of each photon is equal to the product of Planck's constant (h) and the frequency of radiation (ν), which is related to the wavelength (λ) by the equation c = νλ, where c is the speed of light in vacuum. Because of the photoelectric effect, which is a quantum effect in which electrons are ejected from matter when exposed to radiation with sufficiently high frequency, this energy can ionize atoms or eject electrons from metal surfaces.
The maximum kinetic energy that an electron can acquire in the photoelectric effect is equal to the energy of the incident photon minus the work function of the metal. If the metal is irradiated with monochromatic radiation, the maximum kinetic energy of the photoelectron can be calculated using the equation KEmax = hν – φ, where KEmax is the maximum kinetic energy of the ejected electron, h is Planck's constant, and φ is the work function of the metal.Barium has a work function of 2.48 eV, and radiation with a wavelength of 400 nm has a photon energy of 3.1 eV. If the photon is absorbed by a barium atom, the maximum kinetic energy of the ejected electron is:KEmax = hν – φ = hc/λ – φ = 3.1 eV – 2.48 eV = 0.62 eV.To convert this to velocity, the kinetic energy must first be converted to joules, and then to velocity using the following equation:KE = ½ mv2 ⇒ v = √(2KE/m),where m is the mass of the electron, which is 9.11 × 10–31 kg.Therefore,v = √[2(0.62 × 1.6 × 10–19)/9.11 × 10–31] = 4.54 × 105 m/s.So, the maximum velocity of the ejected electron is 4.54 × 105 m/s.
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first you walk 5.38 m in a direction 35.0 degrees north of east. then you walk 8.50 m in a direction 60.0 degrees south of east. what is your total displacement for this trip, both magnitude and direction?
The total displacement for this trip is 10.50 m in a direction 25.0 degrees south of east.
The total displacement for this trip can be calculated by first breaking the trip into its two components and then combining the two.
First, you walked 5.38 m in a direction 35.0 degrees north of east. This can be written in vector form as <5.38, 35.0>.
Second, you walked 8.50 m in a direction 60.0 degrees south of east. This can be written in vector form as <8.50, -60.0>.
To find the total displacement, we can add the two vectors together: <5.38, 35.0> + <8.50, -60.0> = <13.88, -25.0>. This means that the total displacement is 13.88 m in a direction 25.0 degrees south of east.
We can also calculate the magnitude of the displacement by using the Pythagorean theorem: d = √(5.38² + 8.50²) = 10.50 m. This means that the total magnitude of the displacement is 10.50 m.
In summary, the total displacement for this trip is 10.50 m in a direction 25.0 degrees south of east.
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a space traveler weighs 682 n on earth. what will the traveler weigh on another planet whose radius is 3 times that of earth and whose mass is 2 times that of earth?
The traveler's weight on another planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth is 21.647 N
The following is the solution to the given problem:
Mass and gravity are related to one another. Gravity is generated by the planet's mass, and the magnitude of the gravitational force is determined by the mass of the planet on which the object is situated, as well as the mass of the object.
Mass, distance, and gravity are all factors that influence the gravitational force. Mass is directly proportional to the gravitational force and inversely proportional to the square of the distance from the gravitational force's center.
Here is the formula: Force of gravity = G(M1M2)/d²where, G is the gravitational constant 6.67 x 10^{-11} N(m/kg)^2, M1 is the mass of the first body, M2 is the mass of the second body, d is the distance between the centers of two bodies.
On earth, the traveler weighs 682 N. On another planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth, we have to calculate the traveler's weight.
Mass of Earth is 5.972 × 10^24 kg2,
Radius of Earth is 6.371 x 10^63.
The mass of the planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth.
Mass of the planet = 2 x mass of Earth = 2 x 5.972 × 10^24 kg = 1.1944 × 10^25 kg4.
The radius of the planet whose radius is 3 times that of Earth,
Radius of the planet = 3 x radius of Earth = 3 x 6.371 x 10^6 m = 1.9113 × 10^7 m5.
The distance between the two planets.
Distance between two planets = radius of planet + radius of Earth
= 1.9113 × 10^7 m + 6.371 x 10^6 m
= 2.54813 x 10^7 m
= 2.54813 x 10^10 cm.
Putting all the values in the formula.
Force of gravity = G (M1 M2) / d²
Where, Mass of the traveler on the other planet is m.
Mass of the Earth is M1 = 5.972 × 10^24 kg.
Mass of the other planet is M2 = 2 x 5.972 × 10^24 kg = 1.1944 × 10^25 kg.
Radius of the Earth is r1 = 6.371 x 10^6 m.
Radius of the other planet is r2 = 3 x 6.371 x 10^6 m = 1.9113 × 10^7 m.
Distance between the two planets is d = 2.54813 x 10^10 cm.682
= G (M1 M2)/d²
G = 6.674 × 10^-11 N m² / kg²
Force of gravity on other planet = G(mM2)/r² where m is the mass of the traveler on the other planet
= 6.674 × 10^-11 × (m × 1.1944 × 10^25)/(1.9113 × 10^7)²
Weight on another planet = force of gravity on another planet × mass of the traveler on another planet
= (6.674 × 10^-11 × (m × 1.1944 × 10^25)/(1.9113 × 10^7)²) × m
= 21.647 N (approximately)
Therefore, the traveler's weight on another planet whose radius is 3 times that of Earth and whose mass is 2 times that of Earth is 21.647 N (approximately).
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T or F: Surface currents flow vertically in the uppermost 400 meters of the water column. False (horizontally).
The given statement, "surface currents flow vertically in the uppermost 400 meters of the water column," is false because surface currents flow horizontally in the uppermost 400 meters of the water column. They move water parallel to the surface, driven by factors such as wind and temperature differences.
Surface currents are driven by the wind, and they are characterized by movement across the surface of the water. The direction and intensity of surface currents are influenced by a variety of factors, including wind speed and direction, the shape of the coastline, and the rotation of the Earth. These currents are an essential component of the ocean circulation system and can have a significant impact on the climate and the distribution of marine life. They flow parallel to the water columns in the uppermost parts.
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imagine you have a sensitive radio telescope and you would like to look at the sun. is it reasonable to expect that you would see it?
Yes, it is reasonable to expect that you would see the Sun with a sensitive radio telescope.
Radio waves can penetrate through the clouds and the atmosphere, so with a powerful radio telescope you can observe the Sun even on a cloudy day.
Gather the necessary components of the radio telescope, such as a dish and receiver. Point the radio telescope towards the Sun. Tune the receiver to the proper frequency. Take a look at the results from the telescope and observe the Sun.
Therefore, you can expect that you would see the Sun with a sensitive radio telescope.
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a student exerts a horizontal force of 40.0 n with her hand and pushes a 10.0 kg box a distance of 2.0 m across a frictionless floor. calculate the magnitude of the work done by the student. group of answer choices 40.0 j 60.0 j 80.0 j 100.0 j
The magnitude of the work done by the student is 80.0 J. Option c is correct.
The work done by the student can be calculated using the formula,
W = Fd cos(theta)
where W is the work done, F is the force exerted, d is the distance moved, and theta is the angle between the force vector and the displacement vector.
In this problem, the force exerted by the student is a horizontal force of 40.0 N, and the box is moved a distance of 2.0 m across a frictionless floor. Since the force and displacement vectors are in the same direction (horizontal), the angle between them is 0 degrees, so cos(theta) = 1. Therefore, we can calculate the work done as,
W = (40.0 N)(2.0 m) cos(0) = 80.0 J
Hence, option c is correct choice.
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logs sometimes float vertically in a lake because one end has become water-logged and denser than the other. what is the average density of a uniform-diameter log that floats with 20.0% of its length above water?
Uneven-diameter logs that float with 20.0% of their length above water have an average density of 0.8g/cm3. The density is the proportion of weight to capacity.
An item it's far less compact that liquid may be supported up liquid water, and hence it floats. More dense objects can sink when submerged in water. Less dense logs float whereas more thick logs sink. A body can change its condition of rest or motion by the application of force
Instead of obliquely reading from either the side, read the scale stick straight from of the end of both the log. → The diameter of a log is only ever calculated within the bark. Employ a log measuring rod to determine the log's small end's "diameter from within bark," also known as "d.i.b."
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at what speed is a bicyclist traveling when his 27 inch diameter tires are rotating at an angular speed of 5p radians per second?
The bicyclist is travelling at 0.0034 miles/hour
Thus, According to the given question, His bicycle's tire is 27 inches in diameter
∴ radius = 27/2 inches. His angular speed is 5π rad/sec.
1 complete rotation is 2π rad
∴ 5π rad/sec = 5π/2π = 2.5 complete rotations/sec
∴ It will be 2.5 times 60 complete rotations per minute. = 150 rpm.
Circumference of a circle is 2πr
= 2π(27/2) inches
= 84.82 inches which is equivalent to 0.00135 miles per rotation. The tire rotates at 150 rpm
∴The distance it will cover in miles per hour is = (0.00135×150)/60 miles/hour = 0.0034 miles/hour.
Thus, The bicyclist is travelling at 0.0034 miles/hour.
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if the sun is located at one focus of earth's elliptical orbit, the earth is at the other focus. question 20 options: true false
A Frisbee gets stuck in a tree. You want to get it out by throwing a 1.0-kg rock straight up at the Frisbee. If the rock’s speed as it reaches the Frisbee is 4.0 m/s, what was its speed as it left your hand 2.8 m below the Frisbee? Specify the system and the initial and final states.
Answer: The rock's speed as it left your hand was 8.8 m/s.
Explanation: The system is the rock and the Earth. The initial state is the rock at rest in your hand 2.8 m below the Frisbee. The final state is the rock hitting the Frisbee at a speed of 4.0 m/s.
Using conservation of energy, we know that the initial potential energy of the rock-Earth system is transformed into both kinetic energy and potential energy at its maximum height. Therefore, we can use the conservation of energy equation:
potential energy (initial) = kinetic energy (final) + potential energy (final)
mgh = 1/2mv^2 + mgh
where m is the mass of the rock, g is the acceleration due to gravity, h is the height that the rock has been raised, and v is the velocity of the rock.
We can solve for the initial velocity by rearranging the equation:
v = sqrt(2gh + v^2)
Plugging in the values, we get:
v = sqrt(2 * 9.81 * 2.8 + 4^2)
v ≈ 8.8 m/s
Therefore, the rock's speed as it left your hand was 8.8 m/s.
what happens to the water level in the tub if i open the faucet further and water enters at a higher rate?
If you open the faucet further and water enters the tub at a higher rate, the water level in the tub will: rise
The water level will increase at a faster pace, and the tub will fill up more quickly than before. This happens because the rate of water flow into the tub is now higher than the rate at which it can drain away. Therefore, opening the faucet further increases the flow of water into the tub, which raises the water level at a higher rate.
The faucet opening determines the water flow rate, and the flow rate affects the filling rate of the tub. Thus, a higher flow rate leads to a higher filling rate of the tub. As a result, the water level in the tub increases more quickly when the faucet is opened further. The pressure of the incoming water is a critical factor in determining the rate at which the water fills up the tub.
When you turn the faucet on all the way, it releases the highest possible amount of water pressure into the tub, causing the water level to rise rapidly. In summary, opening the faucet further and letting water enter the tub at a higher rate will increase the water level in the tub, and the tub will fill up more quickly than before.
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the space station rotates in order to simulate earth's gravity - so that the normal force on an astronaut at the outer edge would be the astronaut's weight on earth. what is the period of the rotation, t (time for one complete revolution) needed to achieve this?
The space station rotates in order to simulate earth's gravity so that the normal force on an astronaut at the outer edge would be the astronaut's weight on earth. The period of rotation needed to achieve this is: 29.27 minutes
The Space Station is a microgravity environment that is constantly in freefall around the Earth, but it is not affected by gravity. As a result, the astronauts in the Space Station float and move around in the Station. However, by rotating the Space Station, a simulated gravity effect can be created that is comparable to gravity on Earth.
This is due to the centrifugal force that is generated as a result of the rotation. The period of rotation required to generate the required centrifugal force can be calculated.
The centrifugal force generated by the rotation of the Space Station is equal to the force of gravity acting on the astronauts on Earth. Therefore, the formula used to calculate the period of rotation is given:
T = 2π √(R/g)
Where T is the period of rotation, R is the radius of the Space Station, and g is the acceleration due to gravity on Earth. The value of g is 9.8m/s², and the radius of the Space Station is approximately 420 kilometers.
T = 2π √(420,000 / 9.8)
T = 1,756.22 seconds
The period of rotation of the Space Station required to generate a centrifugal force equivalent to the force of gravity on Earth is approximately 1,756.22 seconds or approximately 29.27 minutes.
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