The location of four towns P,Q,R and T are such that Q is on a bearing of 270° from P. T is 12km due north of P and on a bearing of 047° from Q. R is due north of Q and 16km from P. Calculate, correct to three significant figures a. The distance between P and Q. b. The distance between Q and R. c. The bearing of R from P.​

The correct answer is B) 6.04A. In a rectifier circuit, the current output is directly proportional to the voltage input, according to Ohm's Law (V = IR), where V is voltage, I is current, and R is resistance.

Given:

Voltage input (before doubling): 5.9V

Current output: 3.02A

If the voltage output of the rectifier doubles, the new voltage output would be 5.9V x 2 = 11.8V (assuming all else remains equal).

Using the current-voltage relationship, we can calculate the new current output:

I = V/R

Where V is the new voltage output (11.8V) and R is the resistance of the rectifier circuit (which remains constant in this case).

Plugging in the values:

I = 11.8V / R

Since we do not have information about the resistance of the rectifier circuit, we cannot determine the exact value of the new current output. Therefore, the correct answer is D) not enough information.

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The minimum gauge pressure needed is 470,880 Pa or approximately 471 kPa.

To determine the minimum gauge pressure needed in the water pipe leading into a building for water to come out of a faucet on the fifteenth floor, 48 m above the pipe, we must first calculate the pressure required to lift the water to that height.

We can use the formula P = ρgh, where P is the pressure, ρ is the density of water (1000 kg/m³), g is the acceleration due to gravity (9.81 m/s²), and h is the height (48 m).

Calculating P:
P = (1000 kg/m³)(9.81 m/s²)(48 m)
P = 470880 Pa

Therefore, the minimum gauge pressure needed is 470,880 Pa or approximately 471 kPa.

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The wavelength of light can be determined using the double-slit interference equation.The wavelength of light is Ld/a So, so the correct option is b: Ld/a.

L = (mλD)/d
Where L is the distance between adjacent bright or dark fringes, m is the order of the fringe (starting at m=1 for the first bright fringe), λ is the wavelength of the light, D is the distance from the slits to the screen, and d is the distance between the centers of the two slits.
If we rearrange this equation to solve for λ, we get:
λ = (Ld)/mD
Note that a and D do not appear in this equation, so options a, c, and e can be eliminated.
Option b, Ld/a, does not match this equation and is therefore also incorrect.
The correct answer is d, lD/a, which is equivalent to the equation we derived above, but with m=1. This gives us the wavelength of the light for the first bright fringe:
λ = (LD)/d
So, the wavelength of the light is directly proportional to the distance between the screen and the slit, and inversely proportional to the distance between the centers of the two slits.
The correct formula for the wavelength of light in a double-slit interference pattern is:
λ = (Ld) / D
where λ represents the wavelength of light, L is the adjacent dark line spacing in the interference pattern, d is the center-to-center slit spacing, and D is the screen-to-slit distance.

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Starting with the given phase expression:

wt - βz

We can take the time derivative of this expression to derive the velocity expression:

d/dt (wt - βz) = w d/dt t - β d/dt z

Since d/dt t = 1 and there is no explicit time dependence on β, this simplifies to:

d/dt (wt - βz) = w - β(dz/dt)

Recall that the wave speed is given by the ratio of the angular frequency to the wave number, i.e. v = w/β. We can use this relationship to rewrite the above expression:

d/dt (wt - βz) = vβ - v(dz/dt)

Simplifying, we get:

d/dt (wt - βz) = -v(dz/dt) + vβ

Therefore, the velocity expression is:

v = -d/dt (wt - βz) / (dz/dt) + β

which can be further simplified to:

v = -dw/dβ + β

This is the velocity expression in terms of the wave frequency and wave number.

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Micah and Lyra have different near points and are inspecting an object through the same magnifier. Micah's near point is farther away from his eye compared to Lyra's near point. Micah will experience a larger magnification for the following reasons:

1. Micah's longer near point distance allows him to see the object more clearly through the magnifier, which increases the perceived magnification.

2. Since both are using the same magnifier, the lens properties remain constant. However, Micah's farther near point effectively increases the distance between the object and his eye, resulting in a larger magnification due to the increased distance.

In summary, Micah experiences a larger magnification because his near point is farther away from his eye, allowing him to see the object more clearly and at an effectively greater distance through the magnifier.

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The Sun and Moon's gravitational pull has an effect on the tides that affect coastal areas on Earth. High tides are got on by the Moon's bulge of water on the Earth's side that faces the Moon as it circles the Earth.

On the contrary side of the Earth, there is one more lump of water brought about by the divergent power created by the Earth-Moon framework, which likewise prompts elevated tides. There are low tides in the areas in between.

The hypothetical locations of the Moon in relation to the Earth and the Sun, as well as the kind of tide that would affect Earth's coastal areas, are as follows:

Moon New: Between the Sun and Earth is the Moon. As a result, there is a spring tide with high and low tides.

Waxing Bow Moon: The Moon is to the east of the Sun and is partially illuminated. A moderate spring tide is the result of this.

Quarter Moon at First: The Moon is perpendicular to the Sun and only partially illuminated. As a result, the high tides are lower and the low tides are higher during a neap tide.

Gibbous-Waxing Moon: The Moon, which lies to the east of the Sun and receives the majority of its light, A moderate spring tide is the result of this.

New Moon: The Sun and the Moon are on opposite sides of the Earth. As a result, there is a spring tide with high and low tides.

Gibbous-waning Moon: The Moon, lies to the west of the Sun and receives the majority of its light, A moderate spring tide is the result of this.

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Comets are believed to be loosely consolidated, fluffy mixtures of ice and rock based on several lines of evidence and observations: Cometary activity: Comets exhibit activity when they approach the Sun,

such as the formation of a coma (a glowing coma or "atmosphere" surrounding the nucleus) and a tail that points away from the Sun. This activity is thought to be caused by the sublimation of ices (such as water, carbon dioxide, and other volatile compounds) from the nucleus, where they transition directly from solid to gas without passing through a liquid phase. This suggests that comets contain a significant amount of volatile ices that can readily vaporize when exposed to sunlight, indicating a relatively low density and loose composition.

Comet structure: Observations of comets that have been visited by spacecraft, such as Comet Halley (visited by the European Space Agency's Giotto spacecraft in 1986) and Comet Wild 2 (visited by NASA's Stardust spacecraft in 2004), have revealed their structure to be porous and loosely consolidated. Images and data from these missions show a rough and irregular surface with cliffs, boulders, and pits, which suggest a "fluffy" or loosely bound structure.

Comet composition: Analysis of the dust and gas particles emitted by comets during their active phases has provided insights into their composition. The presence of water ice, carbon dioxide, and other volatile compounds in cometary samples collected by spacecraft, as well as spectroscopic observations of comets from telescopes,

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The wave on the string is moving at a pace of 70.7 m/s.

A wave is an energetic disturbance in a medium that doesn't include any net particle motion. Elastic deformation, a change in pressure, an electric or magnetic intensity, an electric potential, or a change in temperature are a few examples.

The speed of a wave on a string can be calculated using the formula:

v = √(T/μ)

where v is the speed of the wave, T is the tension in the string, and μ is the linear density of the string (mass per unit length).

We are given that the string has a total length of 5 m and a total mass of 0.01 kg, so the linear density can be calculated as:

μ = m/length = 0.01 kg / 5 m = 0.002 kg/m

We are also given that the tension in the string is 10 N. Substituting these values into the formula, we get:

v = √(T/μ) = √(10 N / 0.002 kg/m) = √(5000 m^2/s^2)

Simplifying this expression, we get:

v = 70.7 m/s

Therefore, the speed of the wave on the string is 70.7 m/s.

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The grinding wheel stops turning after 6.10 seconds.

Angular Acceleration is defined as the time rate of change of angular velocity. It is usually expressed in radians per second per second.

To solve this problem, we can use the following kinematic equation:

ωf = ωi + αt

where:

ωi = initial angular velocity

ωf = final angular velocity (zero in this case, since the motor is switched off)

α = angular acceleration (constant negative value in this case)

t = time

We want to find the time it takes for the grinding wheel to come to a stop, so we can rearrange the equation to solve for t:

t = (ωf - ωi) / α

Since ωf = 0 and ωi = (1.20 x 10² rev/min) x (2π rad/rev) / (60 s/min) = 12.57 rad/s, we can substitute these values into the equation:

t = (0 - 12.57) / (-2.06) = 6.10 s

Therefore, it takes 6.10 seconds for the grinding wheel to come to a stop.

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The grinding wheel stops turning after 6.10 seconds.

Angular Acceleration is defined as the time rate of change of angular velocity. It is usually expressed in radians per second per second.

To solve this problem, we can use the following kinematic equation:

ωf = ωi + αt

where:

ωi = initial angular velocity

ωf = final angular velocity (zero in this case, since the motor is switched off)

α = angular acceleration (constant negative value in this case)

t = time

We want to find the time it takes for the grinding wheel to come to a stop, so we can rearrange the equation to solve for t:

t = (ωf - ωi) / α

Since ωf = 0 and ωi = (1.20 x 10² rev/min) x (2π rad/rev) / (60 s/min) = 12.57 rad/s, we can substitute these values into the equation:

t = (0 - 12.57) / (-2.06) = 6.10 s

Therefore, it takes 6.10 seconds for the grinding wheel to come to a stop.

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The speed of light in furlongs per fortnight is approximately 1.802 x 10¹² furlongs/fortnight.

We can start by converting meters to furlongs and seconds to fortnights.

1 meter = 1/201.17 furlongs (since 1 furlong = 220 yards and 1 yard = 0.9144 meters)

1 second = 1/1,209,600 fortnights (since 1 day = 24 hours, 1 hour = 60 minutes, 1 minute = 60 seconds, and 1 fortnight = 14 days)

Using these conversions, we have:

Speed of light = 2.998 x 10⁸ m/s

= (2.998 x 10^⁸ m/s) x (1/201.17 furlongs/m) x (86,400 s/day) x (1 day/14 fortnights)

= 1.802 x 10^¹² furlongs/fortnight

Therefore, the speed of light in furlongs per fortnight is approximately 1.802 x 10^¹² furlongs/fortnight.

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The theory of the Moon's origin that best fits with the current scientific understanding is c. a large object hit the Earth and the collision produced a filament of material that condensed to make the Moon. This theory is known as the Giant Impact Hypothesis and is currently the most widely accepted explanation for the formation of the Moon.

It proposes that a Mars-sized body collided with the Earth about 4.5 billion years ago, creating a massive impact that ejected a large amount of material into space. This material then formed a ring around the Earth, which eventually condensed to form the Moon.

This theory is supported by several lines of evidence, including the similar isotopic composition of the Earth and Moon, the Moon's low iron content, and the presence of water on the Moon that is thought to have originated from the Earth's mantle.

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The wavelength of the monochromatic source of light used is: 600nm.

In a Young's double slit experiment, the separation between the two slits is 0.9mm and the fringes are observed one metre away.

To find the wavelength of the monochromatic source of light used, when it produces the second dark fringe at a distance of 1mm from the central fringe, you can use the formula for dark fringes:
d*sin(θ) = (m - 1/2) * λ
where d is the slit separation,
θ is the angle between the central maximum and the dark fringe,
m is the order of the dark fringe, and
λ is the wavelength of light.

First, find the angle θ using the small angle approximation tan(θ) ≈ sin(θ):
θ ≈ y/L
where y is the distance between the central fringe and the dark fringe, and
L is the distance from the slits to the screen.

In this case, y = 1mm and L = 1m, so:
θ ≈ (1mm) / (1m) = 0.001

Now, plug the values into the dark fringe formula for the second dark fringe (m = 2):
(0.9mm) * 0.001 = (2 - 1/2) * λ

Solve for λ:
λ = (0.9mm * 0.001) / (3/2) = 0.0006mm

Convert the wavelength to nanometers:
λ = 0.0006mm * (1000nm/mm) = 600nm

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In this experiment to investigate the specific heat capacity of iron, it is important to identify the independent variables that were held constant throughout the trials.

The mass of water and the mass of the iron sample are examples of quantities that were held constant, as they were always 175g and 75g respectively. The initial temperature of the water was also held constant at 20°C. However, the initial temperature of the iron sample varied in each trial, with options of 30°C, 40°C, 60°C, or 80°C.

Therefore, the initial temperature of the iron sample is not an example of a quantity that was held constant.

The final temperature of the mixture of water and iron is also not a quantity that was held constant, as it was recorded as the dependent variable and varied depending on the initial temperature of the iron sample.

By holding certain variables constant, the experiment can be conducted more accurately and effectively to investigate the specific heat capacity of iron.

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(a) The kinetic energy of the carbon nucleus is equal to the absorbed photon's energy.

(b) The energy of the emitted photon is equal to the initial kinetic energy of the carbon nucleus.

(a) To calculate the kinetic energy of the carbon nucleus, we need to use the principle of conservation of momentum. Since the carbon nucleus is initially at rest, its momentum is zero.

When it absorbs the 15 MeV photon, the recoil momentum of the carbon nucleus will be 15 MeV/c. We can convert this momentum into kinetic energy using the equation:

Kinetic Energy = (recoil momentum)^2 / (2 * mass of carbon nucleus)

The mass of a carbon nucleus (approximately 12 atomic mass units) is 12 times the mass of a proton, which is approximately 1.67 × 10^-27 kg. By substituting these values into the equation, we can find the kinetic energy of the carbon nucleus.

(b) After the carbon nucleus comes to rest, it can lose its internal energy by emitting a photon. The energy of this photon will be equal to the internal energy of the nucleus.

Since the internal energy of the nucleus is equal to the kinetic energy it possessed before coming to rest, we can use the value calculated in part (a) as the energy of the emitted photon.

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Answer:

An active galaxy emits up to thousands of times more energy than a normal galaxy and long jets of gas can spew forth from the galaxy at nearly the speed of light.

Explanation:

       A normal galaxy has a dormant super massive black hole at the center, and it is at a sleeping state after being fed on gas and matter. Whereas an active galaxy also has a super massive black hole at the center and is constantly feeding on gas, matter, stars and other things.

      Active galaxies are either quasars, blazars, or radio galaxies. They are significantly more luminous than a normal galaxy because they produce more electro-magnetic radiations across the spectrum from x-rays to radio waves.

      Active galaxies have shown to have a smaller number of star forming regions than normal galaxies because of the active nature of the AGN at the center causes high amounts of electromagnetic radiation which disturbs the star forming regions and it would take so much time to form new stars.

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Answer:B

Explanation: reistance is constant so b

The planet with an axis that points roughly straight up and thus has no seasons to speak of is Uranus. This unique orientation of Uranus' axis causes its poles to receive almost the same amount of sunlight all year round, resulting in a lack of seasonal variation.

While all the giant planets experience some level of seasonal changes, Uranus stands out as having the most extreme lack of seasonal variation due to its axial tilt.

It's important to note that the other giant planets (Jupiter, Saturn, and Neptune) all have dramatically different seasons due to their axial tilts, which are not as extreme as Uranus'. Jupiter and Saturn have noticeable seasons, but they are less dramatic than those experienced on Earth. Neptune also has seasonal variations, but due to its great distance from the Sun, these changes are less pronounced than those on Uranus.

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Spheres A and B have the same mass and radius but are composed of different materials. Sphere B has a denser core and a less dense shell.

Comparing the moment of inertia of spheres A and B. Given that both spheres A and B have identical mass and radius, but sphere B has a more dense core and a less dense shell, we can determine the relationship between their moments of inertia about their centers of mass.

To do this, we'll use the following equation for the moment of inertia of a solid sphere: I = (2/5)MR², where M is the mass of the sphere, R is its radius, and I is its moment of inertia.

For sphere A (uniform density), its moment of inertia can be calculated as:
Ia = (2/5)MaRa²

For sphere B (non-uniform density with a denser core), its moment of inertia can also be calculated using the same equation, but since it has a more dense core and a less dense shell, its moment of inertia will be smaller than that of sphere A. This is because the mass is distributed closer to the center, which reduces the moment of inertia.

So, comparing the moments of inertia for spheres A and B:
Ia > Ib

Thus, the correct answer is (a): Ia > Ib.

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Answer: acceleration = -1.68 m/s^2

Explanation: First, you need to convert the speeds to meters per second (m/s) since acceleration is typically measured in m/s^2.

2.0 km/hr = 0.56 m/s

0.5 km/hr = 0.14 m/s

Next, you use the formula for acceleration: acceleration = (final velocity - initial velocity) / time

Plugging in the values, we get: acceleration = (0.14 m/s - 0.56 m/s) / 0.25 hr

acceleration = (-0.42 m/s) / 0.25 hr

acceleration = -1.68 m/s^2

To levitate the foil, the laser beam must exert enough radiation pressure to counteract the force of gravity on the foil. This radiation pressure is proportional to the intensity of the laser beam, which can be related to its power using the formula:

power = intensity x area

Assuming that the laser beam is circular and has a radius r, the area it covers on the foil is πr^2. Therefore, the power needed to levitate the foil can be expressed as:

p = (mg) / (πr^2)

where m is the mass of the foil, g is the acceleration due to gravity, and π is a constant.

This expression shows that the power needed to levitate the foil is directly proportional to its mass, and inversely proportional to the area covered by the laser beam. This makes intuitive sense, as a larger laser beam will spread the radiation pressure over a larger area, making it less effective at levitating the foil.

In practice, other factors such as the reflectivity of the foil and the absorption properties of the laser beam will also affect the power required to levitate it. However, the above expression provides a good starting point for understanding the basic physics of laser levitation.

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Answer:

Explanation:

kinetic energyu inmcrease

The determine the temperature increase needed for the square steel bar in fig 3.6-3 to be stress-free when attached to the rigid wall at points A and B, we need to consider the following steps Identify the dimensions and material properties of the square steel bar, such as length, cross-sectional area, coefficient of thermal expansion, and modulus of elasticity.

The Determine the initial temperature of the steel bar, usually denoted as T1. Set up an equation to describe the relationship between the change in length (ΔL) of the steel bar and the temperature change (ΔT). The equation is ΔL = α × L × ΔT where ΔL is the change in length, α is the coefficient of thermal expansion, L is the initial length of the bar, and ΔT is the temperature change. Since we want the bar to be stress-free when attached to the wall, the change in length (ΔL) should be equal to the allowable deformation or strain of the material, which can be calculated using the modulus of elasticity (E) and the applied stress (σ). Substitute the calculated strain for ΔL in the equation from step 3 and solve for ΔT ΔT = (ΔL) / (α × L) Finally, add the initial temperature (T1) to the temperature change (ΔT) to obtain the required final temperature (T2) for the bar to be stress-free T2 = T1 + ΔT Using this step-by-step method, you can determine the temperature increase needed for the square steel bar to be stress-free when attached to the rigid wall at points A and B.

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To find the moment of inertia of a 4-kg connecting rod experimentally, first, the rod is suspended from a cord at point a while held horizontally. A piezoelectric sensor located at point b records a force of 14.6 N under this situation.

This force measurement can be used to determine the location of the center of mass, g, of the connecting rod.

Next, the cord is cut, and the force at point b drops to 9.3 N in that instant. This measurement can be used to calculate the moment of inertia for the connecting rod. The change in force is due to the sudden drop in the rod's potential energy as it falls.

The force of gravity acting on the rod can be calculated using the mass and acceleration due to gravity. The distance between point b and the center of mass g can be calculated using the previous force measurement and the weight of the rod.

With these values, the moment of inertia is of the connecting rod can be calculated using the formula for the moment of inertia of a rigid body rotating about a fixed axis.

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The speed of the moving train is approximately 33.5 m/s.

The beat frequency is given by the difference in frequency between the two horns, which is equal to the Doppler shift in frequency due to the motion of the moving train. Using the formula for the Doppler effect, we can solve for the speed of the train:

[tex]f_b = f_s\dfrac{(v + v_o)}{(v + v_s)}[/tex]

where [tex]f_b[/tex] is the beat frequency, [tex]f_s[/tex] is the horn frequency, v is the speed of sound, [tex]v_o[/tex] is the observer's speed, and [tex]v_s[/tex] is the speed of the source.

We know that [tex]f_s[/tex] = 410 Hz and [tex]f_b[/tex] = 35 Hz. The speed of sound in air at standard temperature and pressure is approximately 343 m/s. Since the observer is stationary, [tex]v_o[/tex] = 0.

Solving for [tex]v_s[/tex], we get:

[tex]v_s = \dfrac{(f_s + f_b)}{f_s - 1} \times v[/tex]

[tex]v_s[/tex] = ((410 Hz + 35 Hz) / 410 Hz - 1) * 343 m/s

[tex]v_s[/tex] = 33.5 m/s

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Answer:

D. Jupiter

Explanation:

The largest planet in the solar system is Jupiter (by Mass)

The gas state of a substance that is normally a solid or a liquid at room temperature occurs when the substance undergoes a phase change from solid or liquid to gas.

This phase change is known as sublimation for solids and evaporation for liquids. The temperature and pressure conditions at which sublimation or evaporation occurs depend on the substance's properties, such as its intermolecular forces and molecular weight. For example, dry ice (solid carbon dioxide) sublimes at -78.5°C and atmospheric pressure, while water (a liquid at room temperature) evaporates at 100°C and atmospheric pressure. The gas state of normally solid or liquid substances has many practical applications, such as in refrigeration, gas storage, and chemical synthesis.

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The work done on the mass by the applied force f is approximately 0.052 J.

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The correct equation for this wave traveling to the right with an amplitude of 0.020 cm and D=-0.020 cm at t=0 and x=0 is option G) D(x,t) = -0.020 cos(9.69x – 3340t) cm.

To determine the correct option, we need to analyze the given parameters. The wave is traveling to the right, which means the sign of the coefficient of x in the cosine function should be negative.

Also, the amplitude is given as 0.020 cm, which eliminates options B, C, D, and F, as they have a positive amplitude. Next, D=-0.020 cm at t=0 and x=0, which means the cosine function should be evaluated at x=0 and t=0 to get the value of D.

Option G satisfies all these conditions, with a negative sign in front of the x term, a negative amplitude of 0.020 cm, and the correct value of D at t=0 and x=0.

Therefore, the correct equation for this wave is D(x,t) = -0.020 cos(9.69x – 3340t) cm.

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Answer:

Explanation:

a) Spring Constant

b) Amplitude of the oscillation

c)Frequency o the oscillation

Answer:

Most meteoroids are small fragments of rock created by asteroid collisions. Comets also create meteoroids as they orbit the sun and shed dust and debris. When a meteoroid enters Earth's upper atmosphere, it heats up due to friction from the air.

Explanation:

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Answer:

Most meteoroids are small fragments of rock created by asteroid collisions. Comets also create meteoroids as they orbit the sun and shed dust and debris. When a meteoroid enters Earth's upper atmosphere, it heats up due to friction from the air.

Explanation: