the tilt of the earth's axis relative to its plane of orbit is 23.5 degrees. which of the following events might you predict to occur if the angle of tilt increased to 33 1/2 degrees? * 5 points a) summers in the united states would likely become warmer. b) winters and summers in australia would become indiscrete. c) seasonal variation at the equator might decrease significantly. d) the north and south poles would experience massive ice melts.

Answers

Answer 1

If the Earth's axial tilt is increased from 23.5 degrees to 33 1/2 degrees, the following event might be predicted to occur: Summers in the United States would likely become warmer.

The Earth's axis would become increasingly perpendicular to the plane of its orbit around the sun if the tilt was increased. Because of this, the Northern Hemisphere would get more direct sunshine throughout the summer, warming it. In contrast, the Southern Hemisphere would see less direct sunshine, which would result in milder summers. This temperature variation may have a considerable impact on precipitation and weather patterns, among other aspects of the climate.

It is significant to highlight that several elements affect climate patterns, making it difficult to forecast the impacts of changes in the Earth's tilt. Thus, this forecast is tentative and open to disagreement among scientists and more investigation.

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Related Questions

What is the rotational inertia of the following body about the indicated rotation axis? (The masses of the connect ing rods are negligible.)

Answers

The solution would involve identifying the relevant masses and distances, squaring the distances, multiplying by the masses, and summing them up to obtain the total rotational inertia.

When solving a physics problem, the first step is to clearly identify the given information, what is being asked, and any relevant equations or principles that apply. This problem provides a diagram of a rotating body and asks for its rotational inertia about a specific axis.

The problem also specifies that the masses of the connecting rods can be ignored. Rotational inertia, also known as moment of inertia, is a property of a rotating object that depends on its mass distribution and the axis of rotation. It can be calculated using the equation I = ∑mr², where I is the rotational inertia, ∑m is the sum of the masses, and r is the distance from the axis of rotation to each mass element squared.

Given the information in the problem and applying the relevant equation, the rotational inertia of the body about the indicated rotation axis can be calculated. To find the total rotational inertia, the answer would entail determining the pertinent masses and distances, squaring the distances, multiplying by the masses, and adding the results together.

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the general momentum equation for elastic and inelastic collisions should be used to determine if the collision is elastic or inelastic. the general momentum equation for elastic and inelastic collisions should be used to determine if the collision is elastic or inelastic. true false

Answers

false. The general momentum equation may be used to evaluate both elastic and inelastic collisions, but it cannot tell whether a collision is elastic or inelastic on its own.

The quantity of kinetic energy preserved during the impact determines the definition of elastic and inelastic collisions. Kinetic energy is conserved in an elastic collision, which means that the total kinetic energy before and after the impact stays constant. Some kinetic energy is lost in an inelastic collision, and the total kinetic energy after the collision is less than the total kinetic energy before the contact. To evaluate whether a collision is elastic or inelastic, one must examine the amount of kinetic energy preserved during the collision, in addition to applying the general momentum equation.

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estimate the thickness of the earth's atmosphere. from your chemistry class, you know that the most common speed of a nitrogen molecule is 670 m/s. the molecules' velocity is pointed along random directions, but some molecules head straight up; i.e. directly away from the earth's center. consider the thickness of the atmosphere as the highest point that such a nitrogen molecule can fly to, if it goes straight up. what is the altitude?

Answers

The estimated thickness of the Earth's atmosphere, the altitude at which a nitrogen molecule would stop traveling straight up, is approximately 22.4 km.

The maximum altitude that a molecule can reach is determined by the balance between the molecule's kinetic energy, which is proportional to the square of its velocity, and the potential energy due to gravity, which is proportional to the distance from the center of the Earth.

Using the equation for potential energy :

[tex]mgh = 1/2mv^2\\h = v^2/2g\\h = (670 m/s)^2 / (2 * 9.81 m/s^2) = 22.4 km[/tex]

Therefore, the estimated thickness of the Earth's atmosphere, defined as the altitude at which a nitrogen molecule would stop traveling straight, is approximately 22.4 km.

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describe briefly what types of observations you will make in activity 1-1 and 1-2 to examine the interactions of magnetic poles with various objects and with each other

Answers

As we observe the Activity 1-1 we can make observations while interactions of magnetic poles with various objects using magnets.

If objects like aluminum foil or coins or paper clips can be test by a magnet and can see if they are attracted to or repelled by the magnet.

We can also observe the strength of magnetic force. To do this we will make changes in distance between the magnet and the object

If we are considering Activity 1-2 there also we can make observations while interactions of magnetic poles with various objects

We can brought the two magnets together and observe if they attract or repel each other. We can make observations.

We will observe the interaction between magnets with the distance between them.

We will observe the behavior of magnetic poles also- with opposite poles and with like poles. Similarities and differences in their interactions.

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A car traveling 127 m/s is 7895 meters away from Bojangles. How long will it take the car to reach Bojangles

Answers

Answer:

10s

Explanation:

a wire is drawn through a die, stretching it to six times its original length. by what factor does its resistance increase?

Answers

When a wire is pulled through a die and stretched six times its initial length, the cross-sectional area reduces according to the length increase. According to Ohm's law,

this change in cross-sectional area influences the wire's resistance, which is directly proportional to its length and inversely proportional to its cross-sectional area. The wire's resistance grows by a factor of 36, which is equal to the square of the stretching factor (6 x 6 = 36). This is due to the wire's length increasing by a factor of six while its cross-sectional area decreasing by a factor of six times six. As a result, the resistance of the wire after stretching it to six times its original length will be  36 times its original resistance, assuming all other factors (such as the resistivity of the material) remain constant.

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if a dung beetle can roll (without slipping) a ball of dung whose radius is 2.5 cm at a linear speed if 3.5 m/s, through what angle does the ball roll as the ball moves a distance of 15 cm?

Answers

If a dung beetle can roll (without slipping) a ball of dung whose radius is 2.5 cm at a linear speed if 3.5 m/s, the angle through which the ball rolls as the ball moves a distance of 15 cm is approximately 343.8 degrees.

Assuming that the ball of dung rolls without slipping, the distance traveled by any point on the circumference of the ball is given by the circumference of the circle it traces. The circumference of the ball can be calculated as follows:

C = 2πr

C = 2π(2.5 cm)

C = 15.7 cm

The distance traveled by the ball is given as 15 cm. Therefore, the number of revolutions made by the ball can be calculated as follows:

Number of revolutions = Distance traveled by ball / Circumference of ball Number of revolutions

Number of revolutions = 15 cm / 15.7 cm

Number of revolutions = 0.955

Since the ball completes less than one full revolution, the angle through which it rolls can be calculated as follows:

Angle = Number of revolutions x 360 degrees

Angle = 0.955 x 360 degrees

Angle = 343.8 degrees (rounded to one decimal place)

Therefore, the ball of dung rolls through an angle of approximately 343.8 degrees as it moves a distance of 15 cm.

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describe photoelectric effect. group of answer choices photoelectric effect is the hypothesis that many metals emit electrons when light of high enough energy shines upon them. photoelectric effect is the observation that many metals emit electrons when light of high enough energy shines upon them. photoelectric effect is the observation that many metals absorb electrons when light of high enough energy shines upon them

Answers

The correct answer is: "Photoelectric effect is the observation that many metals emit electrons when light of high enough energy shines upon them."

The photoelectric effect is a phenomenon in which electrons are emitted from the surface of a material when it is exposed to light of a sufficiently high frequency or energy.

When light is incident on the surface of a metal, the photons of the light interact with the electrons in the metal. If the energy of the photons is greater than the work function of the metal

Which is the minimum amount of energy required to remove an electron from the metal, then electrons are emitted from the metal surface. These emitted electrons are called photoelectrons.

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The surface of a small lake froze, reaching thermal equilibrium with the air above it at -5ºC. The bottom of the lake is at 4ºC. Determine the width of the ice surface, knowing that the depth of the lake plus the ice surface equals 1.4 m.
Make all necessary assumptions for the above case. (Use thermal equilibrium and Fourier's law of conduction)

Answers

The width of the ice surface is 0.108 meters or approximately 11 centimeters of thermal equilibrium.

What, using an illustration, is thermal conductivity?

Actually, thermal conductivity is concerned with the transmission or conduction of heat. 2) Due to the heat transfer from the tea to the cup, pouring hot tea into a cup will result in the cup becoming heated as well.

The rate of heat transfer through the ice surface is calculated using Fourier's rule of heat conduction as follows:

q1 = k1 * A * (T1 - T2) / x

Similarly, the rate of heat transfer through the lake is:

q2 = k2 * A * (T2 - T3) / d

We can set q1 = q2 and solve for x because the rates of heat transmission through each layer are equal:

k1 * A * (T1 - T2) / x = k2 * A * (T2 - T3) / d

Simplifying and rearranging, we get:

x = k1 * d * (T1 - T2) / (k2 * (T2 - T3))

Substituting the given values, we get:

x = 2.18 * 1.4 * (4 - (-5)) / (0.606 * (-5 - (-0)))

x = 0.108 m

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at what part of an elliptical orbit does an earth satellite have the greatest speed? the least speed?

Answers

An elliptical orbit is an oval-shaped path that a satellite takes around its primary body, such as the Earth. The speed of a satellite in its orbit varies depending on its distance from the primary body, which changes throughout the elliptical orbit.

According to Kepler's laws of planetary motion, a satellite moves fastest when it is closest to the primary body, and slowest when it is farthest away. Therefore, an Earth satellite has the greatest speed at the point in its orbit called perigee, which is the point where it is closest to the Earth. At perigee, the satellite experiences the strongest gravitational pull from the Earth, which accelerates it and increases its speed.

Conversely, the satellite has the least speed at the point called apogee, which is the farthest point in its orbit from the Earth. At apogee, the satellite experiences the weakest gravitational pull from the Earth, which decelerates it and decreases its speed.

It's important to note that the speed of a satellite in orbit is also affected by other factors, such as the presence of other gravitational bodies and atmospheric drag. However, the varying distance from the primary body is the primary factor affecting the speed of a satellite in an elliptical orbit around the Earth.

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the circuit in the drawing contains five identical resistors. the 45-v battery delivers 58 w of power to the circuit. what is the resistance r of each resistor?

Answers

The resistance R of each resistor is approximately 6.976 Ω.


To find the resistance R of each resistor in the circuit, first, we need to determine the total resistance in the circuit and the current flowing through it.

We can use the formula for power: P = V * I, where P is power, V is voltage, and I is current. Rearranging for I, we get:

I = P / V
I = 58 W / 45 V
I = 1.29 A

Now, we can use Ohm's Law, V = I * R, to find the total resistance in the circuit:

R_total = V / I
R_total = 45 V / 1.29 A
R_total = 34.88 Ω

Since there are five identical resistors in the circuit, we can find the resistance of each resistor by dividing the total resistance by 5:

R = R_total / 5
R = 34.88 Ω / 5
R = 6.976 Ω

Therefore, the resistance R of each resistor is approximately 6.976 Ω.

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A clown figurine is located 10.0 cm in front of a thin lens that has a focal length of 14.0 cm. Where would the image appear?

Answers

An optical system's focal length, which is the inverse of a system's optical power, indicates how strongly a system converges and diverges light. A system with a good focal length is said to converge light.

A focal length is defined.

The focal length of the a mirror (or lenses) is the separation between its pole and focal point. It can also be measured as the distance between its optical centre and pole. A point where a parallel light ray is "focused" after reflection inside the mirror is known as the central focus (F) of a mirror.

What does focal length vs. focal distance mean?

In photography, focal length—which is a completely different characteristic of a lens—is mentioned much more frequently than focal distance. While not entirely dependent on it, focal length and focal distance are connected. This is what? The focal distance measures how far the object you are focused is from the camera sensor.

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Answer: 5.25cm,virtual

Explanation:

you decide to re-orient the wire to minimize the magnetic force acting on the wire. in what direction(s) could the current flow?

Answers

You may reduce the magnetic force acting on a wire by adjusting its orientation and/or the direction of the current flowing through it. One method for reducing magnetic force is to position.

the wire perpendicular to the magnetic field's direction. The magnetic force on the wire would be decreased in this design. You might even adjust the direction of the electricity flowing through the wire. The force on the wire will be greatest if the current flows in the same direction as the magnetic field. Yet, reversing the direction of the current reduces the stress on the wire. As a result, the current might run perpendicular to the magnetic field or parallel to it. the opposite direction to the original current flow to minimize the magnetic force acting on the wire.

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the two speakers in the drawing are vibrating in phase, and a listener is standing at point p. doesconstructive or destructive interference occur at p when the speakers produce sound waves whose frequency is(a) 1466 hz and(b) 977 hz?

Answers

When the two speakers in the drawing are vibrating in phase, constructive or destructive interference occurs at point P depending on the path difference between the sound waves reaching the listener on these "frequency."  


Step 1: Calculate the path difference between the sound waves from each speaker.
Path difference = |Distance from Speaker 1 to P - Distance from Speaker 2 to P|
Step 2: Determine the wavelength of the sound waves.
Wavelength (λ) = Speed of sound (v) / Frequency (f)
Assuming the speed of sound (v) is approximately 343 m/s,
For (a) 1466 Hz frequency:
λ1 = 343 m/s / 1466 Hz ≈ 0.234 m
For (b) 977 Hz frequency:
λ2 = 343 m/s / 977 Hz ≈ 0.351 m
Step 3: Check if the path difference corresponds to constructive or destructive interference.
Constructive interference occurs when the path difference is a multiple of the wavelength (nλ), where n is an integer.
Destructive interference occurs when the path difference is an odd multiple of half the wavelength ((2n+1)λ/2), where n is an integer.
Compare the calculated path difference with the wavelengths λ1 and λ2, and check for the conditions mentioned above.
Based on the given information, it is not possible to provide a definitive answer without knowing the distances from the speakers to point P. However, by following these steps and plugging in the necessary values, you can determine whether constructive or destructive interference occurs at point P for the given frequencies.

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at the center of the sun, the mass density is rho = 1.52 × 105 kg m−3 and the mean opacity is κ = 0.12 m2 kg−1 . what is the mean free path for a photon at the sun’s center?

Answers

The mean free path for a photon at the sun's center is $\boxed{5.92 \times 10^{-8} \text{ m}}$.

When answering questions on the platform Brainly, you should always be factually accurate, professional, and friendly, be concise and not provide extraneous amounts of detail, and use the terms provided in the student's question when appropriate.

Here is an answer to the given question:At the center of the sun, the mean free path for a photon can be determined using the following formula:$$\ell = \frac{1}{\rho \kappa}$$Where $\rho = 1.52 \times 10^5 \text{ kg m}^{-3}$ and $\kappa = 0.12 \text{ m}^2 \text{ kg}^{-1}$.

The values given are in SI units, so there is no need for conversion. Substituting these values into the formula gives:$$\ell = \frac{1}{(1.52 \times 10^5) (0.12)} = 5.92 \times 10^{-8} \text{ m}$$

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a torroidal solenoid has inner and outer radii of 6.06 cm and 16.6 cm and carries a current of 20.3 a. calculate the number of wire turns required to produce a 13.5 mt magnetic field inside the coil a distance of 10.5 cm from its center

Answers

We would need approximately 45,420 wire turns to produce a 13.5 mT magnetic field inside the toroidal solenoid at a distance of 10.5 cm from its center.

The magnetic field inside a toroidal solenoid is given by:

B = (μ0 * N * I) / (2 * π * r)

where B is the magnetic field, μ0 is the permeability of free space, N is the number of wire turns, I is the current, and r is the radial distance from the center of the toroid. In this case, we want to find N, so we can rearrange the equation to solve for it:

N = (2 * π * r * B) / (μ0 * I)

Plugging in the given values, we get:

N = (2 * π * 0.105 m * 13.5 T) / (4 * π * 10^-7 T·m/A * 20.3 A)

N ≈ 45,420 turns

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jet fighter planes are launched from aircraft carriers with the aid of their own engines and a catapult. if in the process of being launched from rest, the thrust of a jet's engines is 2.30 105 n and after moving through a distance of 90.0 m the plane lifts off with a kinetic energy of 5.40 107 j, what is the work done on the jet by the catapult?

Answers

Work done on the jet by the catapult is 5.40x10^7 J, and Force exerted by the catapult is 6.00x10^5 N.

By using the work-energy principle, we can calculate the work done on the jet and the force exerted by the catapult, given information about  initial and final kinetic energies and  distance traveled. In this case, initial kinetic energy of the jet is zero, and final kinetic energy is 5.40x10^7 J.

[tex]Work = Kinetic\ Energy\ final - Kinetic\ Energy\ initial\\Work = 5.40 * 10^7 J - 0 J\\Work = 5.40 * 10^7 J[/tex]

Since the work done on the jet is equal to the force exerted by the catapult times the distance it moves, we can find the force:

[tex]Work = Force * Distance\\5.40 * 10^7 J = Force * 90.0 m\\Force = 6.00 * 10^5 N\[/tex]

Therefore, the work done on the jet by the catapult is 5.40x10^7 J, and the force exerted by the catapult is 6.00x10^5 N.

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two long parallel wires 45.6 cm apart are carrying currents of 13.0 a and 23.0 a in the same direction. what is the magnitude of the magnetic field halfway between the wires?

Answers

The magnitude of the magnetic field halfway between the wires is 2.14×[tex]10^{-5[/tex] T.

The magnitude of the magnetic field halfway between the wires can be calculated using the formula:

B = μ0I1I2/(2πd)

where B is the magnetic field, μ0 is the permeability of free space, I1 and I2 are the currents in the two wires, and d is the distance between the wires.

Plugging in the given values, we get:

B = (4π T*m/A) * (13.0 A) * (23.0 A) / (2π * 0.456 m)

B = 2.14×[tex]10^-5[/tex] T

Therefore, the magnitude of the magnetic field halfway between the wires is 2.14×[tex]10^-5[/tex]T.

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How does a balanced chemical equation show the law of conservation
of matter?

Answers

A balanced chemical equation demonstrates the Law of Conservation of Mass because it shows that the same amount of mass is present on both sides of the equation. This means that the total mass of the reactants is equal to the total mass of the products.

a nucleus at rest spontaneously disintegrates into 3 equal masses. if one mass flies east and a second north, what is the direction of the third piece? take all the 3 masses to have equal speeds.

Answers

A nucleus at rest spontaneously disintegrates into 3 equal masses. if one mass flies east and a second north, the direction of the third piece will be in the southwest direction.

When a nucleus at rest spontaneously disintegrates into three equal masses with equal speeds, the total momentum before and after the disintegration must be conserved.

Since the initial momentum was zero, the final momentum must also be zero. If one mass flies east and another flies north, the third mass must fly in a direction that cancels out the momentum of the other two masses.

In this case, the third mass must fly in the southwest direction, forming a 45-degree angle with both the east and north directions. This will ensure that the total momentum remains conserved at zero.

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compare that speed with the sun's orbital speed around our galaxy. based on your comparison, do you think the galaxy's gravity would be strong enough to retain the supernova debris if there were no interstellar medium to slow it down? compare that speed with the sun's orbital speed around our galaxy. based on your comparison, do you think the galaxy's gravity would be strong enough to retain the supernova debris if there were no interstellar medium to slow it down? supernova debris moves about 5000 times faster than the sun. the gravity of galaxy alone would not retain the supernova debris. supernova debris moves about 100 times faster than the sun. the gravity of galaxy alone would not retain the supernova debris. supernova debris moves about 100 times faster than the sun. the gravity of galaxy would not retain the supernova debris even if debris are slowed by the interstellar medium. supernova debris moves about 5000 times faster than the sun. the gravity of galaxy would not retain the supernova debris even if debris are slowed by the interstellar medium.

Answers

Supernova debris moves about 100 times faster than the Sun's orbital speed around our galaxy. Based on this comparison, the galaxy's gravity alone would not be strong enough to retain the supernova debris, even if the interstellar medium were to slow it down.

A supernova is a powerful and luminous explosion that occurs when a star dies. It releases an enormous amount of energy into space, sending a shock wave of gas and dust out into the surrounding space. The shock wave disperses the star's elements into space, including heavier elements that were produced during the supernova, such as gold and platinum. Supernova debris moves at a speed of about 5000 times faster than the sun's orbital speed around the galaxy. Therefore, if there were no interstellar medium to slow it down, the supernova debris would continue to move at that high speed and would not be retained by the gravity of the galaxy alone. This is because the speed at which the supernova debris is moving is much greater than the escape velocity of the galaxy, which is the minimum speed required for an object to break free from the gravitational pull of the galaxy.

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5. Protons and anti-protons interact via the process:
p+p2n+2π* + n°
a) Write this interaction at the quark level and hence show that there is no change in quark flavour.
b) Show that baryon number is conserved.
c) What evidence is there that this is controlled by the strong interaction?

Answers

a) The interaction between a proton and an antiproton can be written at the quark level as:  uud + uud → udd + udd + uubar + uubar.

b) the total baryon number before and after the interaction is the same:

B_before = 1 (proton) + 1 (neutron) = 2

B_after = 1 (neutron) + 1 (neutron) + 1 (Λ0) = 3

c) This interaction is controlled by the strong interaction, which is one of the four fundamental forces of nature.

What is an interaction ?

a) The interaction between a proton and an antiproton can be written at the quark level as:

uud + uud → udd + udd + uubar + uubar.

where u, d, and ubar denote the up quark, down quark, and anti-up quark, respectively. This interaction does not involve any quark flavor change since the number of each type of quark (up, down, and anti-up) is conserved.

What is baryon?

b) Baryon number (B) is defined as the total number of baryons minus the total number of antibaryons. In this interaction, we start with two baryons (a proton and a neutron) and end with three baryons (two neutrons and a Λ0 particle) and no antibaryons. Therefore, the change in baryon number is:

ΔB = (number of baryons) - (number of antibaryons) = 2 - 0 = 2

Since ΔB is non-zero, we might think that baryon number is not conserved. However, it is important to note that the Λ0 particle is a baryon with a baryon number of +1, which cancels out the baryon number of the two neutrons (-1 each). Therefore, the total baryon number before and after the interaction is the same:

B_before = 1 (proton) + 1 (neutron) = 2

B_after = 1 (neutron) + 1 (neutron) + 1 (Λ0) = 3

Therefore, baryon number is conserved in this interaction.

c) This interaction is controlled by the strong interaction, which is one of the four fundamental forces of nature. The strong interaction is responsible for binding quarks together to form hadrons, such as protons, neutrons, and Λ0 particles. The exchange of gluons, which are the carrier particles of the strong force, between quarks is what allows them to interact and bind together. The fact that this interaction involves the production of multiple hadrons and conservation of baryon number is consistent with it being a strong interaction. Additionally, experiments have shown that the strong force is responsible for binding protons and neutrons together in the nucleus of an atom.

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11. What kind of force did the levitating rings display? What does this say
about the magnetic domains of these objects? Record your evidence.

Answers

answer :

force is called the magnetic force of repulsion, and it happens when two magnets have the same poles (either both north or both south) and they push away from each other.

When all the domains in a material are aligned in the same direction, the material becomes strongly magnetized.

explanation :

magnetic domains in the rings were stable and strong enough to resist the force of gravity.

In the case of the levitating rings, the magnetic domains were aligned in such a way that they created a strong magnetic field, which allowed the rings to levitate in mid-air.

tiny regions within ferro magnetic  material that have their own magnetic fields are called magnetic domains.

Magnetic domains in the rings refer to the tiny regions within the ring's ferro magnetic material that have their own magnetic fields.

the light spots that form a circle around the outside of the fountain below come from a light source in the center of the fountain. explain how the light makes it from the center of the fountain to the circles of light on the ground where the water hits.

Answers

When a light source is present in the center of the fountain, light spots that form a circle around the outside of the fountain are observed.

In order to explain how the light makes it from the center of the fountain to the circles of light on the ground where the water hits, the following points should be considered: The water in the fountain's center captures the light's brightness and refracts it into the water droplets. This makes the water droplets illuminate in all directions. The refracted light is scattered throughout the water droplets, generating a brilliant glow that illuminates the droplets.

The illuminated droplets are then sprayed out of the fountain and into the air, where they meet the ground at a distance, creating light circles or patterns. The angle at which the water droplets meet the ground and the intensity of the light hitting them influence the size and clarity of the circles, which can be visible even when there is ambient light present. The light source in the center of the fountain provides the essential component for the creation of the light circles.

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URGENT!!!
A small glass ball is rubbed with a piece of silk, giving the ball a charge of 1.0 x 10^-8 C. determine the magnitude of the force due to the Earth's magnetic field if the ball is thrown to the west with a velocity 8.0 m/s .
The earth's magnetic field is 5.0 x 10^-5 T

Answers

Answer:

[tex]F = 3\times 10^{-12} \ N [/tex]

Explanation:

To find:-

The magnitude of force due to Earth's magnetic field.

Answer:-

We are here given that, a ball having a charge of 1*10-C is thrown with a velocity of 8m/s towards west . We are interested in finding out the magnetic force due to the earth .

As we know that, the magnetic force is given by,

[tex]\longrightarrow\boxed{ F = q[\vec{v} \times \vec{B} ]} \\[/tex]

So here we have,

q = 1 * 10-⁸ C v = 6m/s WestB = 5*10-⁵ T

So on substituting the respective values, we have;

[tex]\longrightarrow F = 10^{-8} C [ v B \sin\theta ] \\[/tex]

Here [tex]\theta[/tex] is the angle between velocity and the magnetic field, which is here 90° . So that, we have;

[tex]\longrightarrow F = 10^{-8} C [ 6 \ m/s \times (5\times 10^{-5} \ T) \times \sin90^o \\[/tex]

The value of sin90° is " 1 " . So we have;

[tex]\longrightarrow F = 10^{-8} \times 30 \times 10^{-5} \times 1 \ N \\[/tex]

[tex]\longrightarrow F = 30 \times 10^{-13} \ N \\[/tex]

[tex]\longrightarrow \boxed{\boldsymbol{ F = 3 \times 10^{-12} N }}\\[/tex]

This is the required magnetic force by the earth's magnetic field.

how much work is done when John did when lifting a 20kg mass to a height of 2m?

Answers

Answer:

To calculate the work done by John when lifting a 20kg mass to a height of 2m, we can use the formula: work = force x distance x cos(theta) where force is the weight of the mass (20kg x 9.81 m/s^2 = 196.2 N), distance is the height the mass is lifted (2m), and cos(theta) is the angle between the force and the displacement (cos(0) = 1, since the force and displacement are in the same direction). Substituting these values into the formula, we get: work = 196.2 N x 2m x 1 work = 392.4 J Therefore, John did 392.4 joules of work when lifting the 20kg mass to a height of 2m.

Help asap 50 points!! What form of energy is stored in a battery?
O chemical
O sound
O light
O heat​

Answers

Answer:

The answer to your question is O chemical

Explanation:

Chemical potential energy

Batteries store energy in the form of chemical potential energy. This energy is converted into electrical energy when the battery is connected to an electrical circuit.

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a rock of mass m is thrown horizontally off a building from a height h, as shown above. the speed of the rock as it leaves the thrower's hand at the edge of the building is vo question what is the kinetic energy of the rock just before it hits the ground?

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The kinetic energy of the rock simply earlier than it hits the ground is [tex]\frac{1}{2}mv^2[/tex]

Kinetic energy is a fundamental concept that describes the strength possessed by an object due to its movement. Its miles are defined because the energy that a body possesses as a result of its motion, which relies upon its mass and velocity. The method for kinetic energy is KE = 1/2mv², in which m is the mass of the object and v is its speed.

Kinetic energy is a scalar quantity and is measured in joules (J) in the SI system. Kinetic energy plays an essential role in many areas of physics, such as mechanics, thermodynamics, and relativity. It is an important concept in understanding the behavior of moving objects and how they interact with their environment. In summary, kinetic energy is the energy possessed by a moving object and is dependent on its mass and velocity.

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two objects are initially the same height above the ground. simultaneously, one is released from rest and the other is shot fof horizontally with a n initial speed of 2.5 m/s. the two objects collide after falling 20m. how far apart were the object initially?

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We may use the equations of motion to calculate the initial distance between the two objects in this issue. Let's call the starting height of the objects "h." Because the first item is at rest, its initial vertical velocity is 0.

When the second item is launched horizontally at a speed of 2.5 m/s, its initial vertical velocity is also 0. When the items crash after falling 20 meters, we may apply the following equation of motion: h = 1/2gt^2 where g denotes gravity's acceleration and t the time it takes for the objects to collide. The horizontal velocity of the second item may be used to calculate the time t: distance = time x speed 20m = 2.5m/s x t t = 8 seconds Now we can use the equation of motion again to find h: h = 1/2gt^2 = 1/2 x 9.81 m/s^2 x (8 s)^2 = 313.92 m Therefore, the initial distance between the objects was 313.92 meters.

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compared to terrestrial planets, jovian planets are group of answer choices larger and denser smaller and denser larger and less dense smaller and less dense

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Jovian planets are a group of answer choices that are larger and less dense compared to Terrestrial planets. The term "jovian" was coined after the planet Jupiter, which is the largest planet in the Solar System.

These planets are made up mostly of hydrogen, helium, and other gases, and have a gaseous, liquid, or icy outer layer that surrounds a dense, rocky core.The four jovian planets in the Solar System are Jupiter, Saturn, Uranus, and Neptune.

They are also known as gas giants or outer planets. Compared to terrestrial planets, they are larger and have a lower density due to their composition of gases and lack of a solid surface.

They also have a greater mass and gravity, which allows them to retain large atmospheres and maintain many moons and rings.Jovian planets are also characterized by their longer orbital periods, slower rotations, and lower temperatures.

They are located farther from the Sun than terrestrial planets and have a lower surface temperature due to their distance from the Sun and their composition. They are important to study because they can provide insights into the formation and evolution of our Solar System and other planetary systems.

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