Asterisms are smaller, recognizable shapes formed by stars within a constellation or spanning multiple constellations. They can take the form of familiar objects or geometric shapes.
All stars within well-defined regions of the sky are members of constellations. These constellations are a way to organize and divide the celestial sphere into recognizable patterns.
The star in Taurus is designated Alpha Tauri, which means it is considered the brightest star in that particular constellation. Patterns of stars in the night sky are called asterisms.
Asterisms are smaller, recognizable shapes formed by stars within a constellation or spanning multiple constellations. They can take the form of familiar objects or geometric shapes.
While there are 88 official constellations recognized by the International Astronomical Union, there are countless asterisms that astronomers and stargazers observe and appreciate within these constellations.
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All stars within well-defined regions of the sky are members of constellations. The star in Taurus is designated Alpha Tauri. Patterns of stars in the night sky are called asterisms and are part of one or more constellations.
The International Astronomical Union (IAU) recognizes 88 constellations. These constellations are well-defined areas in the sky that contain groups of stars forming recognizable patterns. Some of the most famous constellations include Orion, Ursa Major (the Big Dipper), and Cassiopeia.
Asterisms, on the other hand, are smaller, distinct patterns formed by stars within a constellation or across multiple constellations. These patterns may be easily recognizable and have cultural or historical significance. For example, the Big Dipper is an asterism within the Ursa Major constellation.
In total, there are 15 asterisms that are officially recognized by the IAU. These include the Big Dipper, the Little Dipper, the Northern Cross, and the Summer Triangle.
Constellations and asterisms help astronomers navigate the night sky and locate specific celestial objects. They provide a way to organize and identify stars and other celestial bodies.
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Consider a one directional 2 km bridge with two lanes that connects two freeways. The bridge, which never gets congested due to sufficient capacity in its downstream, pertains a saturation flow of 2500 [veh/h/In] and a jam density of 300 [veh/km]. For safety of the bridge the speed limit is designed at 70 [km/h]. What is the maximum number of vehicles that the bridge can carry at a time? (maximum number of vehicles that can be on the bridge)
The maximum number of vehicles that the bridge can carry at a time is 600 vehicles.
As per data:
Length of bridge, L = 2 kmm,
Saturation flow, S = 2500 veh/h/ln,
Jam density, J = 300 veh/km,
Speed limit, V = 70 km/h.
Here, the bridge has two lanes, and the downstream is sufficient to handle all the traffic.
Hence, we can assume that all the traffic on the bridge is moving at the same speed as the speed limit.
Therefore, the maximum number of vehicles that can be on the bridge at any instant is given by the product of the density and the length of the bridge.
N_max = J x L
If we convert the given data in the same unit, then we have:
J = 300 veh/km
= 0.3 veh/m,
V = 70 km/h
= 70,000 m/h,
Substitute values,
N_max = J x L
= 0.3 x 2000
= 600 vehicles
Hence, the maximum number of vehicles that the bridge can carry at a time is 600 vehicles.
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which is 20 light years planet from earth
A light-year is a unit of distance, specifically the distance that light travels in one year.
Light travels at a speed of approximately 299,792 kilometers per second (or about 186,282 miles per second) in a vacuum. Therefore, to determine which planet is 20 light-years away from Earth, we need to identify a planet located at a distance of approximately 20 times this speed of light.
As of my knowledge cutoff in September 2021, no known exoplanets have been directly observed and confirmed to be located exactly 20 light-years away from Earth. However, there are numerous exoplanets that have been discovered within a range of distances from Earth.
Some notable exoplanets discovered within approximately 20 light-years of Earth include:
Proxima Centauri b: This exoplanet is located in the habitable zone of the closest star system to our Solar System, Proxima Centauri. It is estimated to be around 4.24 light-years away.Ross 128 b: This exoplanet orbits a red dwarf star known as Ross 128, located approximately 11 light-years away from Earth.TRAPPIST-1 system: This system hosts seven Earth-sized planets orbiting the ultra-cool dwarf star TRAPPIST-1. The TRAPPIST-1 system is located around 39 light-years away from Earth.know more about light-year here:
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Silver (Z = 47), copper (Z = 29), and platinum (Z = 78) can be used as the target in an X-ray tube. Rank in descending order (largest first) the energies needed for impinging electrons to knock a K-shell electron completely out of an atom in each of these targets.
platinum, silver, coppersilver, copper, platinum platinum, copper, silversilver, platinum, coppercopper, silver, platinum
The correct ranking in descending order (largest first) of the energies needed for impinging electrons to knock a K-shell electron completely out of an atom in each of these targets is: Platinum, Silver, Copper
To rank the energies needed for impinging electrons to knock a K-shell electron completely out of an atom in each of the given targets, we need to consider the ionization energies of the K-shell electrons for each element. The ionization energy represents the energy required to remove an electron from its respective shell.
The ionization energy generally increases as we move across a period in the periodic table and decreases as we move down a group. Based on the given elements, we can determine their relative ionization energies:
Platinum (Z = 78): Platinum has the highest atomic number among the given elements. Generally, higher atomic number elements have higher ionization energies. Therefore, platinum would require the highest energy to knock out a K-shell electron.
Silver (Z = 47): Silver has an intermediate atomic number. It is expected to have a lower ionization energy compared to platinum but higher than copper.
Copper (Z = 29): Copper has the lowest atomic number among the given elements. It is expected to have the lowest ionization energy among the three.
Therefore, the correct ranking in descending order (largest first) of the energies needed for impinging electrons to knock a K-shell electron completely out of an atom in each of these targets is:
Platinum, Silver, Copper
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MEN A rocketmastering tight the normal force in nating on a massa, niin e auto's Darlletter that even with the your HINT Need Help
The normal force (in N) acting on an astronaut of mass 824 kg, including her space, is 3872.8 N.
The push or pull on a mass-containing item changes its velocity. An external force is an agent that has the power to alter the resting or moving condition of a body.
According to question:
m = 82.4 kg
a = 37.2 m/s2
Assume the normal force acting on the astronaut is N
So,
N - mg = ma
N = m (a+g)
= 82.4 (37.2+9.8
= 3872.8 N
Therefore, the normal force (in N) acting on an astronaut of mass 824 kg, including her space, is 3872.8 N.
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A rocket takes eft from Earth's surface, accelerating straight so at 37.2 m/s Calculate the normal force (in N) acting on an astronaut of mass 824 kg, including her space utt. (Assume the rocker's Initia motion parallel to the y-direction. Indicate the direction with the sign of your answer)
A
heat engine is measured to have 30% efficiency. Is the theoretical
efficiency going to be greater or less than that? Why?
The theoretical efficiency is greater than that of the actual efficiency of the engine. This is because heat engine always produces some waste heat.
The Second Law of Thermodynamics states that a heat engine cannot be 100% efficient. In practice, a heat engine is only 100% efficient when it is operating at about 30-50% efficiency.
If we were to multiply this by 100, we would get the efficiency as a percent: 49%. This is the theoretical maximum efficiency. If we were to actually build an engine, it would be less efficient than the theoretical engine. The theoretical engine that can achieve this theoretical maximum efficiency is called the Carnot Engine.
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A concave mirror has a 42 cm radius of curvature. How far from the mirror must an object be placed to create an upright image three times the height of the object? Express your answer using two significant figures. x= _____cm
The object must be placed 14 cm away from the concave mirror in order to create an upright image three times the height of the object.
Given:
The radius of curvature (R) = 42 cm
Focal length (f) = R/2
In order to determine the distance from the mirror at which an object must be placed to create a specific image size, the mirror equation can be used: [tex]\frac{1}{f} = \frac{1}{u}+ \frac{1}{v}[/tex]
Let's assume the object height (h₀) is represented by h and the image height ([tex]h_i[/tex]) is represented by 3h.
For an upright image, the magnification is positive, so M = hi/h₀
= 3h/h
= 3.
Using the magnification formula:
M = -v/u
= 3
The object distance (u) using the mirror equation and the magnification:
[tex]\frac{1}{f} = \frac{1}{u}+ \frac{1}{v}[/tex]
[tex]\frac{1}{\frac{R}{2} } = \frac{1}{u} + \frac{1}{v}[/tex]
Substituting the values:
[tex]\frac{1}{\frac{42}{2} } = \frac{1}{u} + \frac{1}{v}[/tex]
[tex]\frac{1}{21} } = \frac{1}{u} + \frac{1}{v}[/tex]
Since M = -v/u = 3, the equation as:
[tex]\frac{1}{21} = \frac{1}{u} - \frac{1}{3u}[/tex]
Combining the terms:
[tex]\frac{1}{21} = \frac{3-1}{3u}[/tex]
[tex]\frac{1}{21} = \frac{2}{3u}[/tex]
3u = 42
u = 14 cm
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A
paddlewheel increases the thermal energy of a bucket of water by
20J. How much heat is added to the water?
20J of heat is added to the bucket of water by the paddlewheel.
Conservation of energy states that energy can neither be created nor be destroyed but can only be transformed from one form to another.
Paddlewheel is increasing the thermal energy of water. so by conservation of energy, the amount of work done by the paddlewheel is stored as the thermal energy of water which in turn increases the temperature of water.
So the amount of work done by the paddlewheel is equal to the heat added to water.
Therefore, 20J of heat is added to the bucket of water by the paddlewheel.
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The position of a block of a mass-spring system undergoing SHM is given by the following function
x(t) = −(0.067 m) cos ([2.41 rad] t) . s
a. What is the amplitude of the block’s motion.
b. What is the frequency, f of the block’s motion?
c. What is the time period, T of the block’s motion?
d. When is the first time the block is at the position x = 0?
e. Draw the position versus time graph for this motion, include time
period in the x axis with numbers (you can choose any scale, as we
did in class).
f. Express velocity of the block as a function of time.
g. What is the maximum speed of the block?
h. Draw the velocity versus time graph for this motion as in class.
i. Express acceleration of the block as a function of time.
j. Draw the acceleration versus time graph for this motion.
k. What is the maximum magnitude of acceleration of the block as in class?
The amplitude is 0.067 m. Therefore, the frequency is f = 2.41 rad / (2π) ≈ 0.384 Hz. Therefore, T = 1 / f ≈ 1 / 0.384 ≈ 2.604 s. The times when the block is at the position x = 0. The time period, T, represents one complete cycle of the motion. v(t) = dx/dt = (0.067 m) sin (2.41 rad t). In this case, the maximum speed is equal to the amplitude of the velocity function. The maximum magnitude of acceleration is equal to the amplitude of the acceleration function, which is (0.067 m) ×ω².
a. The amplitude of the block's motion is the maximum displacement from the equilibrium position. In this case, the amplitude is 0.067 m.
b. The frequency of the block's motion can be determined from the angular frequency, ω, which is the coefficient of t in the argument of the cosine function. In this case, ω = 2.41 rad. The frequency, f, is related to ω by the equation f = ω / (2π). Therefore, the frequency is f = 2.41 rad / (2π) ≈ 0.384 Hz.
c. The time period, T, is the inverse of the frequency. Therefore, T = 1 / f ≈ 1 / 0.384 ≈ 2.604 s.
d. To find when the block is at the position x = 0, we set x(t) = 0 and solve for t:
0 = −(0.067 m) cos (2.41 rad t)
cos (2.41 rad t) = 0
This occurs when 2.41 rad t = π/2 + nπ or 2.41 rad t = 3π/2 + nπ, where n is an integer. Solving for t, we have:
t = (π/2 + nπ) / (2.41 rad) or t = (3π/2 + nπ) / (2.41 rad)
This gives us the times when the block is at the position x = 0.
e. The position versus time graph can be represented as a cosine function with the given amplitude and angular frequency. The time period, T, represents one complete cycle of the motion. The graph will oscillate symmetrically around the x-axis.
f. The velocity of the block can be found by taking the derivative of the position function with respect to time:
v(t) = dx/dt = (0.067 m) sin (2.41 rad t)
g. The maximum speed of the block occurs when the magnitude of the velocity is maximum. In this case, the maximum speed is equal to the amplitude of the velocity function.
h. The velocity versus time graph can be represented as a sine function with the same angular frequency as the position function but with an amplitude of (0.067 m) × ω.
i. The acceleration of the block can be found by taking the derivative of the velocity function with respect to time:
a(t) = dv/dt = (0.067 m) ω cos (2.41 rad t)
j. The acceleration versus time graph can be represented as a cosine function with the same angular frequency as the position and velocity functions but with an amplitude of (0.067 m) ×ω².
k. The maximum magnitude of acceleration occurs when the magnitude of the acceleration function is maximum. In this case, the maximum magnitude of acceleration is equal to the amplitude of the acceleration function, which is (0.067 m) × ω².
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An electron enters a region of B field where B = (+41 +8j) x 10-4 Teslas. Its initial position is (4,2) meters and its velocity is v = (61 - 7j) x 104 m/s. What is the radius of the helix made by this electron?
The radius of the helix made by the electron is approximately 1.328 x 10⁻³ meters.
To determine the radius of the helix made by the electron, it is required to consider the Lorentz force acting on the electron due to the magnetic field. The Lorentz force is given by the equation:
F = q(v x B),
The cross product of the velocity and the magnetic field can be calculated as:
v x B = [tex](v_x \times B_y - v_y \times B_x)[/tex]
where [tex]v_x[/tex] and [tex]v_y[/tex] are the x and y components of the velocity, and [tex]B_x[/tex] and [tex]B_y[/tex] are the x and y components of the magnetic field.
Given,
[tex]v_x[/tex] = 61 x 10⁴ m/s,
[tex]v_y[/tex] = -7 x 10⁴ m/s,
[tex]B_x[/tex] = 41 x 10⁻⁴ T,
[tex]B_y[/tex] = 8 x 10⁻⁴ T.
Calculating cross-products:
[tex]v_x \times B_y - v_y \times B_x = (61 \timesa 10^4 \times 8 \times 10^{-4}) - (-7 \times 10^4 \times 41 \times 10^{-4}) \\= 0.488 - (-2.867) \\= 3.355 \times 10^4[/tex]
Now, by Lorentz force,
F = [tex]m \times\frac{ v^2}{r}[/tex]
where m is the mass of the electron and r is the radius of the helix.
The mass of an electron is m = 9.11 x 10⁻³¹ kg
rearrange the equation to solve for the radius:
[tex]r = m \times (\frac{v^2}{F}).[/tex]
Substituting the values, we get:
[tex]r = \frac{9.11 \times 10^{-31}) \times ((61 \times 10^4)^2}{(3.355 \times 10^4)}[/tex]
Calculating the expression,
r = 1.328 x 10⁻³ meters.
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A 2.1 ✕ 103-kg car starts from rest at the top of a 4.8-m-long driveway that is inclined at 24° with the horizontal. If an average friction force of 4.0 ✕ 103 N impedes the motion, find the speed of the car at the bottom of the driveway.
The speed of the car at the bottom of the driveway is approximately 5.85 m/s.
To find the speed of the car at the bottom of the driveway, we can use the principle of conservation of energy.
The initial potential energy of the car at the top of the driveway is converted into kinetic energy at the bottom. We'll assume there is no loss of energy due to friction along the inclined plane.
The potential energy (PE) of the car at the top of the driveway can be calculated as:
PE = m * g * h,
where m is the mass of the car (2.1 × 10² kg), g is the acceleration due to gravity (9.8 m/s²), and h is the vertical height of the driveway (h = 4.8 m * sin(24°)).
The work done by the friction force (Work_friction) can be calculated as:
Work_friction = -F_friction * d,
where F_friction is the average friction force (4.0 × 10³ N) and d is the length of the driveway (4.8 m).
The initial potential energy of the car is converted into the final kinetic energy (KE) at the bottom of the driveway:
KE = (1/2) * m * v²,
where v is the speed of the car at the bottom of the driveway.
Applying the principle of conservation of energy:
PE + Work_friction = KE
m * g * h - F_friction * d = (1/2) * m * v²
Substituting the given values and solving for v:
(2.1 × 10² kg) * (9.8 m/s²) * (4.8 m * sin(24°)) - (4.0 × 10³ N) * (4.8 m) = (1/2) * (2.1 × 10² kg) * v²
Simplifying the equation:
v² = [(2.1 × 10² kg) * (9.8 m/s²) * (4.8 m * sin(24°)) - (4.0 × 10³ N) * (4.8 m)] / (1/2) * (2.1 × 10² kg)
v² = 34.265 m²/s²
Taking the square root of both sides:
v ≈ 5.85 m/s
Therefore, the speed of the car at the bottom of the driveway is approximately 5.85 m/s.
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A pendulum is released from rest from a height of 20 cm. What is the maximum speed of the pendulum?
1. Not enough information
2. 19.8 ms/
3. 14 m/s
4. 1.98 m/s
A pendulum is released from rest from a height of 20 cm and The maximum speed of the pendulum is 1.98 m/s.
The gravitational potential energy is given by:
Potential Energy = mgh
Kinetic Energy = (1/2)mv²
Where:
m is the mass of the pendulum,
g is the acceleration due to gravity,
h is the height (20 cm or 0.2 m),
v is the velocity of the pendulum,
Since the pendulum is released from rest, the potential energy is converted entirely into kinetic energy at the lowest point of the swing.
On equating Potential Energy and Kinetic Energy,
mgh = (1/2)mv²
gh = (1/2)v²
v² = 2gh
v = √(2gh)
v = 1.98 m/s
The maximum speed of the pendulum is 1.98 m/s.
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Give two reasons why skiers typically assume a crouching position when going down a slope. (Select all that apply.) In the crouching position there is less air resistance. Crouching lowers the skier's center of mass, making it easier to balance Crouching decreases the mass of the skier. The acceleration of gravity is increased by crouching. Crouching decreases the skier's inertia. PRACTICE IT Use the worked example above to help you solve this problem. A skier starts from rest at the top of a frictionless incline of height 20.0 m, as shown in the figure. At the bottom of the incline, the skier encounters a horizontal surface where the coefficient of kinetic friction between skis and snow is 0.199. Neglect air resistance. (a) Find the skier's speed at the bottom. m/s (b) How far does the skier travel on the horizontal surface before coming to rest? EXERCISE HINTS: GETTING STARTED I'M STUCK! Use the values from PRACTICE IT to help you work this exercise. Find the horizontal distance the skier travels before coming to rest of the incline also has a coefficient of kinetic friction equal to 0.199. Assume that 8 - 20.00
The amount of wind resistance is lower while crouching. Additionally, crouching reduces the skier's center of mass, which facilitates balance. The skier's speed at the bottom is 19.809 m/s, and the skier travel on the horizontal surface is 108.69 m.
Speed at bottom:
Vb = to find
Energy conservation:
Let the mass of skier is M
energy at A = energy at B
mgh = 1/2 mv²b
vb = [tex]\rm \sqrt{2gh}[/tex]
vb = 19.809 m/s
B energy
1/2 mv² = u mg d
d = 108.69 m
Thus, the skier's speed at the bottom is 19.809 m/s and the skier travel on the horizontal surface before coming to rest 108.69 m.
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One of the concrete pillars that support a house is 2.3 m tall and has a radius of 0.49 m. The density of concrete is about 2.2 103 kg/m3. Find the weight of this pillar in pounds (1 N = 0.2248)
_____lb
Weight is the force experienced by an object due to gravity. It is a measure of the gravitational force exerted on an object's mass. The weight of the concrete pillar is approximately 541.05 pounds.
To find the weight of the concrete pillar in pounds, we can calculate the volume of the pillar and then multiply it by the density to obtain the mass. Finally, we can convert the mass from newtons to pounds using the conversion factor provided.
The volume of the pillar can be calculated using the formula for the volume of a cylinder:
V = πr²h
where:
V is the volume,
r is the radius,
h is the height.
Substituting the given values:
V = π(0.49 m)² × 2.3 m
V ≈ 1.094 m³
Next, we can calculate the mass of the pillar using the formula:
mass = density × volume
mass = 2.2 × 10³ kg/m³ × 1.094 m³
mass ≈ 2406.8 kg
Finally, we convert the mass from newtons to pounds using the conversion factor:
weight = mass × 0.2248 lb/N
weight ≈ 2406.8 kg × 0.2248 lb/N
weight ≈ 541.05 lb
Therefore, the weight of the concrete pillar is approximately 541.05 pounds.
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What makes it so difficult to measure circular objects?
3. Which is harder to measure, the circumference or the diameter? Why?
Measuring circular objects is challenging due to the lack of well-defined edges, curvature, and irregularities, making precise measurements difficult.
1. Lack of well-defined edges: Unlike measuring straight-edged objects, circular objects lack clear endpoints or edges. This can make it difficult to establish precise starting and ending points when measuring.
2. Curvature and irregularities: Circular objects can have variations in their curvature or irregularities, which further complicates measurement accuracy. These variations can make it challenging to determine a consistent reference point for measurements.
3. Dimensional properties: Circles have specific dimensional properties, such as the relationship between their circumference and diameter, which affects the accuracy of measurements. This leads us to the second question:
Regarding the difficulty of measurement, the circumference and diameter of a circle are interrelated. The circumference is the distance around the outside of a circle, while the diameter is a straight line segment passing through the center, connecting two points on the circle's circumference.
Typically, the circumference is harder to measure accurately compared to the diameter. This is primarily because measuring the circumference requires measuring a curved path, while the diameter can be measured as a straight line. The curvature of the circumference introduces additional challenges in accurately determining its length, whereas measuring the diameter is comparatively more straightforward.
However, it's worth noting that the difficulty of measurement can also depend on the specific tools or techniques employed. Specialized instruments, such as digital calipers or laser measuring devices, can improve the accuracy of measuring both the circumference and diameter of circular objects.
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A ball is launched from inside a cylindrical device that has been set on a frictionless incline and turned loose
What can be determined about where the ball will land ?
The ball will land back in the cylinder.
The ball will land behind the cylinder.
It depends on the mass of the ball.
The ball will land in front of the cylinder.
It cannot be determined.
The velocity of the ball in the forward direction is the same as the initial velocity with which it was launched.
A ball is launched from inside a cylindrical device that has been set on a frictionless incline and turned loose. What can be determined about where the ball will land?It can be determined that the ball will land in front of the cylinder.
This can be explained with the help of a few concepts of Physics. When an object moves on an incline without friction, then it can be divided into two components, which are: gravity and normal force.
Here, gravity is acting towards the center of the Earth, whereas the normal force is perpendicular to the incline. Let's suppose that the ball is launched with a certain velocity, which makes it move along the incline and get projected in the forward direction.
If we think of the motion of the ball from the observer's point of view who is standing on the incline, then the motion will appear to be parabolic. This is because the observer would see that the ball is moving forward with a constant velocity, but its vertical position keeps changing due to the effect of gravity.
However, from the observer's point of view who is standing in front of the cylinder, the motion of the ball will look like it is a projectile.
The velocity of the ball in the forward direction is the same as the initial velocity with which it was launched.
But, due to the effect of gravity, the vertical component of the velocity would change, which would result in a parabolic path of the ball. Therefore, the ball will land in front of the cylinder.
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The velocity of the ball in the forward direction is the same as the initial velocity with which it was launched. It can be determined that the ball will land in front of the cylinder. The correct option is The ball will land in front of the cylinder.
A ball is launched from inside a cylindrical device that has been set on a frictionless incline and turned loose. What can be determined about where the ball will land?It can be determined that the ball will land in front of the cylinder.
This can be explained with the help of a few concepts of Physics. When an object moves on an incline without friction, then it can be divided into two components, which are: gravity and normal force.
Here, gravity is acting towards the center of the Earth, whereas the normal force is perpendicular to the incline. Let's suppose that the ball is launched with a certain velocity, which makes it move along the incline and get projected in the forward direction.
If we think of the motion of the ball from the observer's point of view who is standing on the incline, then the motion will appear to be parabolic. This is because the observer would see that the ball is moving forward with a constant velocity, but its vertical position keeps changing due to the effect of gravity.
However, from the observer's point of view who is standing in front of the cylinder, the motion of the ball will look like it is a projectile.
The velocity of the ball in the forward direction is the same as the initial velocity with which it was launched.
But, due to the effect of gravity, the vertical component of the velocity would change, which would result in a parabolic path of the ball. Therefore, the ball will land in front of the cylinder.
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Bonus: Your company is considering submitting a bid on a major project. You determine that the expected completion time is 100 weeks and the standard deviation is 10 weeks. It is assumed that the normal distribution applies. You wish to set the due date for the project such that there is an 85 percent chance that the project will be finished by this time. What due date should be set? O 108.0 O 1104 O 89.6 O 85.0 O Not enough information
The due date that should be set is 114.4 weeks. Therefore, the correct option is option (A) 108.0.
the expected completion time = μ = 100 weeks
Standard deviation = σ
= 10 weeks
We need to find the due date such that there is an 85 percent chance that the project will be finished by this time.
Here, we need to find the z-value for which the area under the standard normal distribution curve is 0.85.
Therefore, using the z-table, the z-value comes out to be 1.44.
Now, we can use the formula for z-score for normal distribution as follows:
z = (X - μ) / σWe can rearrange the above formula as:
X = μ + z * σ
= 100 + 1.44 * 10
= 114.4
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A certain confined aquifer in the Inanda area in South Africa has a thickness of 18.5 m, a hydraulic conductivity of 12.5 m/day and a storativity of 0.0045. A pumping well drawing from this aquifer has a pumping rate of 0.035 L/s.
1.1 Calculate the transmissivity of the aquifer.
1.2 What is the drawdown at a distance of 15 m from the well after 24 hours of pumping?
1.3What will be the drawdown after 12 months of pumping?
1.4 What are the basic assumptions that govern groundwater flow? All geologic formations are horizontal and of infinite horizontal extent.
The values of all sub-parts have been obtained.
1.1) The transmissivity of the aquifer is 231.25 m²/day.
1.2) The drawdown at a distance of 15 m from the well after 24 hours of pumping is 0.1265 m.
1.3) The drawdown after 12 months of pumping is 0.00105 m.
1.4) The groundwater flow rate is proportional to the hydraulic conductivity and the hydraulic gradient.
The solutions to the problems related to hydraulic conductivity, transmissivity of the aquifer, and drawdown at a distance are as follows:
1.1) Calculation of the transmissivity of the aquifer.
Transmissivity is the term used to describe the capacity of an aquifer to transmit water. The transmissivity formula is as follows:
T = k * b
Where k represents hydraulic conductivity and b represents the aquifer thickness.
Substituting the given values in the formula,
T = 12.5 * 18.5
= 231.25 m2/day
Therefore, the transmissivity of the aquifer is 231.25 m2/day.
1.2) Calculation of drawdown at a distance of 15 m from the well after 24 hours of pumping.
The following equation will be used to calculate the drawdown at a distance from the well.
s = (Q / 4πT) ln (r / rw)
Where s represents the drawdown, Q represents the pumping rate, T represents transmissivity, r represents the distance from the well, and rw represents the well radius.
Substituting the given values in the above formula, we get
s = (0.035 / 4π * 231.25) ln (15 / 0)
= 0.1265 m
Therefore, the drawdown at a distance of 15 m from the well after 24 hours of pumping is 0.1265 m.
1.3) Calculation of drawdown after 12 months of pumping.
The following equation will be used to calculate the drawdown after 12 months of pumping:
s = 9.5 Q / πT
Where s represents the drawdown, Q represents the pumping rate, and T represents transmissivity.
Substituting the given values in the above formula, we get
s = (9.5 * 0.035) / (π * 231.25)
= 0.00105 m
Therefore, the drawdown after 12 months of pumping is 0.00105 m.
1.4) Basic assumptions that govern groundwater flow are as follows:
All geological formations are horizontal and of infinite horizontal extent.
Each formation is porous and permeable and contains groundwater.
The pressure head and the hydraulic gradient are always in the direction of the groundwater flow.
The groundwater flow rate is proportional to the hydraulic conductivity and the hydraulic gradient.
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Baelin is a man who understands when it’s a nice day to fish. Let Baelin have
just caught a fish, and noted its mass is 8.67 kg. He had put a force sensor on his fishing
rod to measure the tension of the line. When the fish was totally immersed in water, the
tension of the fishing rod line was 50 N. Baelin now fishes in a murky pond. A nearly
identically sized fish is caught from this pond water, and Baelin finds the tension of his
line to be 35 N. What is the density of the pond water? The density of water is 1000
kg/m3.
The density of the pond water is calculated to be 1429 kg/m³.
Density is the mass of the substance per unit volume. The most common symbol for density is the lowercase Greek letter Rho (Latin letter D).
Density depends on temperature and pressure. For solids and liquids, the difference in density is usually small. For gases, the difference is much larger. When pressure is applied to an object, it reduces its volume, resulting in an increase in density.
Given,
gravitational acceleration g = 9.8 m/s²
density of water ρ = 1000kg/m³
Mass of fish = 8.67 kg
The volume of the fish = V
Buoyancy force on the fish submerged in water = Fb1
[tex]\rm Mg = \rho Vg[/tex]
When the fish is immersed in water, the tension in the fishing rod line T1 = 50 N
The weight of the fish is equal to the buoyancy force acting on the fish plus the tension in the fishing rod line.
[tex]\rm Mg = Fb1 + T1[/tex]
[tex]\rm Mg = \rho Vg + T1[/tex]
[tex](8.67)(9.8) = (1000)V(9.8) + 50[/tex]
[tex]84.966 = 9800V + 50[/tex]
[tex]34.966 = 9800V[/tex]
[tex]\rm V = 3.568 \times 10^{-3} kg/m^{3}[/tex]
The density of the pond water = [tex]\rm \rho[/tex]
Buoyancy force on the fish when it is in the pond water = Fb2
[tex]\rm Fb2 = \rho Vg[/tex]
Tension in the fishing rod line when the fish in the pond water = T2 = 35 N
[tex]\rm Mg = Fb2 + T2[/tex]
[tex]\rm Mg = \rho Vg + T2[/tex]
[tex]\rm (8.67)(9.8) = \rho(3.568x10-3)(9.8) + 35[/tex]
[tex]\rm 84.966 = 0.0349664\rho + 35[/tex]
[tex]\rm 49.966 = 0.0349664\rho[/tex]
[tex]\rm \rho = 1429 kg/m^{3}[/tex]
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Copepods are tiry crastacears that aro an estontal link in the estuarine food web, Morine scientiets designed an experiment to determine whether dietary lipid (tat) centent is important in the poputation growth of a copepod. Independent randem samples of copepods were placed in containers containing lpidierich diasons. bacteria, or leaty macroalgan. There were 12 containers total with four feplicates per det. Five gravid (egg-bearing) femaies were placed in each container. Afer 14 days, the number of copepods in each container were as given to the right. At the 5%. significance level, do the data provide sufficient ovidence to conclude that a dillerence exists in mesn number of copepods among the three different diets?
We have sufficient evidence to conclude that a difference exists in the mean number of copepods among the three different diets.
At the 5% significance level, we need to test if the data provide sufficient evidence to conclude that a difference exists in the mean number of copepods among the three different diets.
Null hypothesis: H0: μ1 = μ2 = μ3
Alternative hypothesis: Ha: At least one mean is different from the other.
Using ANOVA, the test statistic F is calculated as follows:
F = MST/MSE where MST is the mean square treatment
MSE is the mean square error
Based on the results given to the right, we have the following information:
Total Sum of Squares (SST) = 126.09Sum of Squares Treatment (SSTR) = 87.50
Sum of Squares Error (SSE) = 38.59
Degrees of Freedom (DF) Total = n - 1 = 11
Degrees of Freedom (DF) Treatment = k - 1 = 2
Degrees of Freedom (DF) Error = (n - 1) - (k - 1) = 8
Mean Square Treatment (MST) = SSTR/DF Treatment = 87.50/2 = 43.75
Mean Square Error (MSE) = SSE/DF Error = 38.59/8 = 4.82The value of F is calculated as follows:
F = MST/MSE = 43.75/4.82 = 9.07
Using an F-table with DF treatment = 2 and DF error = 8, the critical value of F Is 4.46.
Since 9.07 > 4.46, the calculated F value is greater than the critical F value.4
Hence, we reject the null hypothesis.
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A current of 3.70 A is carried by a 250 m long copper wire of radius 1.25 mm. Assume an electronic density of 8.47 × 1028m−3 , resistivity rho = 1.67 × 10−8Ω · m, and resistivity temperature coefficient of α = 4.05 × 10−3 0C −1 at 20 0C.
(a) Calculate the drift speed of the electrons in the copper wire. (2)
(b) Calculate the resistance of the at 35 (4) 0C.
(c) Calculate the difference of potential between the two ends of the copper wire.
(a) The drift speed of electrons in the copper wire is approximately 0.0026 m/s.
(b) The resistance of the copper wire at 35°C is approximately 5.88 Ω.
(c) The potential difference between the two ends of the copper wire is approximately 21.7 V.
a) To calculate the drift speed, we use the formula:
drift speed = current / (electronic charge * electronic density * cross-sectional area)
Given:
current (I) = 3.70 A
electronic charge (e) = 1.6 × 10¹⁹ C
electronic density (n) = 8.47 × 10²⁸ m⁻³
radius (r) = 1.25 mm = 1.25 × 10⁻³ m
The cross-sectional area (A) of the wire can be calculated using the formula for the area of a circle:
A = π * r²
Plugging in the values, we have:
A = π * (1.25 × 10⁻³ m)²
Now we can calculate the drift speed:
drift speed = 3.70 A / (1.6 × 10⁻¹⁹ C * 8.47 × 10²⁸ m⁻³ * π * (1.25 × 10⁻³ m)²)
≈ 0.0026 m/s
Therefore, the drift speed of electrons in the copper wire is approximately 0.0026 m/s.
b) To calculate the resistance, we use the formula:
resistance = resistivity * (length / cross-sectional area)
Given:
resistivity (ρ) = 1.67 × 10⁻⁸ Ω·m
length (L) = 250 m
cross-sectional area (A) calculated using the radius (r) from the previous part
Now we can calculate the resistance:
resistance = (1.67 × 10⁻⁸ Ω·m) * (250 m / (π * (1.25 × 10⁻³ m)²))
≈ 5.88 Ω
Therefore, the resistance of the copper wire at 35°C is approximately 5.88 Ω.
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The index of refraction for violet light in most materials is higher than for red light. Rays of violet and red light come from air and are incident on a glass surface at an angle of 50°. Circle an answer for each statement. a. True/False Violet light moves slower in the glass than red light. b. True/False Violet light refracts at a smaller angle than the red light. c. True/False Violet light completely reflects, while red light goes into the glass. d. True/False Violet light has a smaller frequency in the glass than red light.
Violet light moves slower in the glass than red light is true, Violet light refracts at a smaller angle than the red light is false, hence correct answers are true, false, false, and false.
Red light penetrates the glass more quickly than violet light. This is due to the fact that most materials have a violet light index of refraction that is greater than their red light index. Light slows down as it enters a material with a higher refractive index.
Compared to red light, violet light refracts at a narrower angle. This is because of Snell's law, which stipulates that the relationship between the index of refraction and the angle of refraction is inverse.
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The stopping potential for electrons emitted from a surface illuminated by light of wavelength 525 nm is 0.800 V. When the incident wavelength is changed to a new value, the stopping potential is 1.30 V. (a) What is this new wavelength in meters? (b) What is the work function for the surface in Joules?
The stopping potential for electrons emitted from a surface illuminated by light of wavelength 525 nm is 0.800 V. When the incident wavelength is changed to a new value, the stopping potential is 1.30 V.
(a) The new wavelength is 3.78 × 10⁻⁷ m.
(b) The work function for the surface is 3.78 × 10⁻¹⁹ Joules.
(a) To find the new wavelength in meters, we can use the equation for the photoelectric effect:
ΔV = (hc / λ) - (hc / λ₀)
where ΔV is the change in stopping potential, h is the Planck's constant, c is the speed of light, λ is the new wavelength, and λ₀ is the initial wavelength.
Given:
ΔV = 1.30 V - 0.800 V = 0.5 V
λ₀ = 525 nm = 525 × 10⁻⁹ m
h = 6.626 × 10⁻³⁴ J·s
c = 3.00 × 10⁸ m/s
Rearranging the equation, we can solve for λ:
λ = (hc / ΔV) - (hc / λ₀)
λ = (6.626 × 10⁻³⁴ J·s * 3.00 × 10⁸ m/s / (0.5 V)) - (6.626 × 10⁻³⁴ J·s * 3.00 × 10⁸ m/s / (525 × 10⁻⁹ m))
λ ≈ 3.78 × 10⁻⁷ m
Therefore, the new wavelength is approximately 3.78 × 10⁻⁷ m.
(b) The work function (φ) of the surface can be determined using the equation:
φ = (hc / λ₀) - eV₀
where e is the elementary charge and V₀ is the initial stopping potential.
Given:
λ₀ = 525 nm = 525 × 10⁻⁹ m
V₀ = 0.800 V
e = 1.602 × 10⁻¹⁹ C
Substituting the values, we can calculate the work function:
φ = (6.626 × 10⁻³⁴ J·s * 3.00 × 10⁸ m/s / (525 × 10⁻⁹ m)) - (1.602 × 10⁻¹⁹ C * 0.800 V)
φ ≈ 3.78 × 10⁻¹⁹ J
Therefore, the work function for the surface is approximately 3.78 × 10⁻¹⁹ Joules.
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A satellite has a mass of 5540 kg and is in a circular orbit 1.09 x 105 m above the surface of a planet. The period of the orbit is 1.74hours. The radius of the planet is 9.42 x 106 m. What is the true weight of the satellite when it is at rest on the planet's surface?
The true weight of the satellite when it is at rest on the planet's surface is approximately 5.42 x 10⁴ Newtons.
To calculate the true weight of the satellite when it is at rest on the planet's surface, we need to consider the gravitational force between the satellite and the planet.
The gravitational force between two objects can be calculated using Newton's law of universal gravitation:
F = (G * m₁ * m₂) / r²
Where:
F is the gravitational force,
G is the gravitational constant (approximately 6.67430 x 10⁻¹¹ N·m²/kg²),
m1 and m2 are the masses of the two objects, and
r is the distance between the centers of the two objects.
In this case, we are interested in finding the weight of the satellite when it is at rest on the planet's surface, so we need to calculate the gravitational force between the satellite and the planet.
Given:
Mass of the satellite (m₁) = 5540 kg
Radius of the planet (r) = 9.42 x 10⁶ m
To calculate the weight of the satellite on the planet's surface, we can equate the gravitational force between the satellite and the planet to the weight of the satellite:
Weight = F = (G * m1 * m2) / r²
Since the satellite is at rest on the planet's surface, the weight is equal to the gravitational force between the satellite and the planet.
Substituting the values into the equation, we have:
Weight = (6.67430 x 10⁻¹¹ N·m²/kg² * 5540 kg * m₂) / (9.42 x 10⁶ m)²
To find the value of m2 (mass of the planet), we can use the fact that the period of the satellite's orbit is related to the radius of the orbit and the mass of the planet:
T = 2π * √(r³ / (G * m₁))
Given:
Period of the orbit (T) = 1.74 hours = 1.74 * 60 * 60 seconds
Radius of the orbit (r) = 1.09 x 10⁵ m
Gravitational constant (G) = 6.67430 x 10⁻¹¹ N·m²/kg²
Solving the equation for m₁:
m2 = (r³ * (2π / T)²) / G
Substituting the values, we can calculate m₁:
m₂ = (1.09 x 10⁵ m)³ * (2π / (1.74 * 60 * 60 seconds))² / (6.67430 x 10⁻¹¹ N·m²/kg²)
Now, we can substitute the calculated value of m2 into the equation for weight:
Weight = (6.67430 x 10⁻¹¹ N·m²/kg² * 5540 kg * m₁) / (9.42 x 10⁶ m)²
Evaluating the expression, we find that the true weight of the satellite when it is at rest on the planet's surface is approximately 5.42 x 10⁴Newtons.
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A wire carries a current. If both the wire diameter and the electron drift speed are doubled, the electron current increases by a factor of A. 2 B. 4 C. 6 D. 8 E. Some other value.
A wire carries a current. If both the wire diameter and the electron drift speed are doubled, the electron current increases by a factor of A. 2 B. 4 C. 6 D. 8 E. Some other value.
A wire carries a current. If both the wire diameter and the electron drift speed are doubled, the electron current increases by a factor of 8, hence option D is correct.
When an electric field is produced, it exerts a force on the moving electrons, which causes their random motion to become a tiny flow in one direction. This flow's velocity is known as the drift velocity.
The current through the wire is,
I = neAvd
= ne([tex]\rm\pi \frac{d^2}{4} v_d[/tex])
= [tex]\frac{\rm \pi ned^2v_d}{4}[/tex]
The current through the wire when the wire diameter and electron drift speed are doubled.
I' = [tex]\frac{\pi ne(2d)^2(2v_d) }{4}[/tex]
= 8 [tex]\frac{\pi ne(2d)^2(2v_d) }{4}[/tex]
= 8 I
Thus, the current increased by the factor of 8.
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A 12-meter-long rope is pulled tight with a tension of 92 N as shown below. When one end of the rope is given a "thunk" (disturbance), it takes 1.0 s for the disturbance to propagate to
the other end.
F= 29 N -12m
(a) Is this wave on the rope transverse or longitudinal? Explain why.
(b) What is the speed of the wave v?
(c) What is the linear density (mass per length, μ) of the string?
(d) What is the total mass of the rope?
The wave on the rope is transverse. The speed of the wave on the rope is 24 m/s.The linear density is 2kg/m. The total mass of the rope is 24kg.
a) The wave on the rope is transverse.
When one end of the rope is given a "thunk," the disturbance travels along the rope in a direction perpendicular to the length of the rope. This is the reason the wave on the rope is transverse.
b) The speed of the wave (v),
v = λ / T
Where λ is the wavelength and T is the period.
The period (T) is equal to 1.0 s.
The wavelength (λ) can be calculated
λ = 2L
λ = 2 × 12
λ = 24 m
v = λ / T
v = 24 m/s
Therefore, the speed of the wave on the rope is 24 m/s.
(c) The Velocity of the wave in string v = μT
24 = μ × 12
μ = 2kg/m
The linear density is μ = 2kg/m.
(d) The linear density of the string,
μ = m / L
where m is the mass of the rope and L is the length of the rope.
m =2 * 12
m = 24 kg
The total mass of the rope is 24kg.
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What is a starburst galaxy and what main features might we look
for in detecting a starburst galaxy?
A starburst galaxy is a type of galaxy that experiences an exceptionally high rate of star formation. It is characterized by intense bursts of star formation activity, hence the name "starburst."
These bursts result in the rapid formation of new stars within a relatively short period compared to the average star formation rate in other galaxies.
Starburst galaxies are typically identified by specific features and observations, including high infrared emission, strong emission lines, compact and concentrated regions, blue colors, luminosity and star formation rate, galactic winds, and super winds.
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Three current carrying wires are arranged as shown below. The top wire is infinitely long, situated 0.040 m from the near edge of the rectangle and carries a current of 5.00 A to the left. The rectangular loop has a length of 0.150 m and a height of 0.080 m and carries a clockwise current of 2.00 A. The circular loop has radius of 0.040 m situated directly in the center of the rectangle and carries a counterclockwise current of 3.00 A
What is the magnetic field vector at the center of the circle due to only the rectangular loop?
The magnetic field vector at the center of the circle due to only the rectangular loop is zero.
The magnetic field due to a wire is given by
B = (μ₀/ 4π) × (I/ a) × (sin α - sin β)
where:
B = magnetic field
μ₀ is permeability in free space
I is the current in the wire
a is the distance between the wire and the point of observation
α and β are angles made by endpoints of wire at the point of observation
the direction of the magnetic field is given by the right-hand screw rule with the thumb pointing in the direction of current
For the given case, the direction of the magnetic field due to the opposite parts of the rectangular loop being in opposite directions hence they cancel out each other.
Therefore, the magnetic field vector at the center of the circle due to only the rectangular loop is zero.
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With all of the electric wires and current running through your house, what direction would a compass point if you were standing in the middle of your room? Why is this? What property of magnetic fields does this demonstrate, and how would the magnetic field lines look in this region?
1) The direction it points depends on the direction of the electric current in the wires.
2) The magnetic field lines in the region would form circles around each individual wire carrying current.
3) This is because of the right-hand rule
Where does the current point?The magnetic field produced by the electric current forms a circular magnetic field around the wire in accordance with the right-hand rule, which is applicable to conventional current flow.
The current's flow direction determines the direction of the magnetic field lines. The curled fingers of your right hand, which is holding the wire with your thumb pointing in the direction of the current flow, would point in the direction of the magnetic field.
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A uniform thin rod of length 0.813 m is hung from a horizontal nail passing through a small hole in the rod located 0.033 m from the rod's end. When the rod is set swinging about the nail at small amplitude, what is the period of oscillation?
The time period of the rod of length 0.813 m hung from a horizontal nail passing through a small hole in the rod located 0.033 m from the rod's end is 1.772 s.
The time period for a simple pendulum performing simple harmonic motion is given by
T = 2π√(l/g)
where T = time period in s,
l = length of a simple pendulum, and
g = acceleration due to gravity at the place of the simple pendulum
Given: length of rod = 0.813 m
position of nail = 0.033 m
so the effective length will be = 0.813 - 0.033
l = 0.78
amplitude is small so we can use the above formula,
so the time period of the rod will be
T = 2π√(l/g)
T = 2π√(0.78/9.8)
T = 1.772 s
Therefore, the time period of the rod is 1.772 s.
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In a Photoelectric experiment the work function for Lead is 4.5eV. If light of wavelength 250nm is incident on the surface, find (a) KE (b) the minimum wavelength in order to get photo electrons: ac a. .23eV, 340nm b. .23eV, 275.6nm c. .46eV, 340nm d. .46eV, 275.6nm
(a) The kinetic energy (KE) of the photoelectron is approximately 7.69 x 10⁻²¹ J.
(b) The minimum wavelength required to eject photoelectrons is approximately 920 nm.
Given:
Work function (ϕ) for Lead = 4.5 eV
Wavelength of incident light (λ) = 250 nm
Let's calculate the values:
(a) KE:
First, we need to convert the work function from electron volts (eV) to joules (J) using the conversion factor: 1 eV = 1.6 x 10⁻¹⁹ J.
Work function (ϕ) = 4.5 eV × 1.6 x 10⁻¹⁹ J/eV = 7.2 x 10⁻¹⁹ J
Now, we can calculate the energy of the incident photon:
Energy = (6.626 x 10⁻³⁴ J·s × 3 x 10⁸ m/s) / (250 nm × 10⁻⁹ m/nm)
Energy ≈ 7.969 x 10⁻¹⁹ J
Finally, we can find the kinetic energy of the photoelectron:
KE = 7.969 x 10⁻¹⁹ J - 7.2 x 10⁻¹⁹ J
KE ≈ 7.69 x 10⁻²¹ J
(b) Minimum Wavelength:
To find the minimum wavelength, we use the threshold energy equal to the work function:
Threshold wavelength = (6.626 x 10⁻³⁴ J·s × 3 x 10^8 m/s) / (7.2 x 10 J)⁻¹⁹
Threshold wavelength ≈ 9.2 x 10⁻⁷ m or 920 nm
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