which particles have positive charges, and which have negative charges? sort the particles into positive and negative charged.

The objective lens is a long focal length, convex lens and the eyepiece functions as a simple magnifier is the correct statement about a compound microscope. Option b is correct.

In a compound microscope, the objective lens is a long focal length, convex lens that produces an inverted, magnified real image of the specimen. The eyepiece, on the other hand, functions as a simple magnifier, which further magnifies the real image produced by the objective lens and forms a virtual image that can be viewed by the observer's eye. Therefore, option b is the correct statement.

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--The complete question is, A compound microscope is a two-lens system used to look at very small objects. Which of the following statements is correct?

a. The objective lens is a short focal length, convex lens and the eyepiece functions as a simple magnifier.

b. The objective lens is a long focal length, convex lens and the eyepiece functions as a simple magnifier.

c.  The objective lens and the eyepiece both have the same focal length and both serve as simple magnifiers.--

The reason we do not see the lines of hydrogen in the spectra of the hottest stars is due to the ionization of hydrogen atoms at high temperatures.

In these stars, the temperatures are so high that the electrons in the hydrogen atoms are stripped away, leaving behind only the protons. This ionized hydrogen does not produce the same spectral lines as neutral hydrogen, which is what we typically observe in cooler stars. Instead, the spectra of hot stars are dominated by lines from ionized metals, such as helium, carbon, and oxygen. So while hydrogen is indeed the most common element in the universe, its presence in the spectra of hot stars is not as prominent due to ionization.

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The Chen notation of entity-relationship modelling can be used for both conceptual and implementation modelling.

The Chen notation of entity-relationship modelling can be used for both conceptual and implementation modelling. Notation refers to the symbols and conventions used to represent concepts in a model. Entity-relationship modelling is a technique used in database design to represent the relationships between entities. Conceptual modelling is the process of creating a high-level representation of a system, while implementation modelling involves creating a detailed representation of the system's implementation.

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To find the focal length of a convex lens, we can use the formula:
1/f = 1/di + 1/do

Where f is the focal length, di is the distance of the image from the lens, and do is the distance of the object from the lens.

We are given that the student is 2.50m away from the lens, so do = 2.50m. We are also given that the image is 1.80m from the lens, so di = 1.80m.

Plugging these values into the formula, we get:
1/f = 1/1.80 + 1/2.50

Simplifying this equation, we get:
1/f = 0.5556

Multiplying both sides by f, we get:
f = 1.80 / 0.5556

Solving for f, we get:
f ≈ 3.24 meters

Therefore, the focal length of the convex lens is approximately 3.24 meters.

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A convex lens is 1.80 meters from a student who is 2.50 meters distant, and its focal length is 1.04 meters.

To solve this problem, we can use the lens equation:

1/f = 1/do + 1/di

where f is the focal length of the lens, do is the object distance (distance of the object from the lens), and di is the image distance (distance of the image from the lens).

In this problem, the object distance is do = 2.50 m and the image distance is di = 1.80 m. We can plug these values into the lens equation and solve for the focal length:

1/f = 1/do + 1/di

1/f = 1/2.50 + 1/1.80

1/f = 0.4 + 0.56

1/f = 0.96

f = 1/0.96

f ≈ 1.04 meters

Therefore, the focal length of the convex lens is approximately 1.04 meters.

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The instantaneous angular velocity is 20.0 s is 400 rad/s.

Since the angular acceleration is constant, we can use the formula:

[tex]θ = 1/2 * α * t^2 + ω0 * t[/tex]

where

[tex]θ = angle rotated = 50 rad[/tex]

[tex]α = angular acceleration[/tex]

[tex]t = time = 5.0 s[/tex]

[tex]ω0 = initial angular velocity = 0 (starting from rest)[/tex]

Solving for α, we get:

[tex]α = 2 * (θ - ω0 * t) / t^2 = 2 * 50 rad / 5.0 s^2 = 20 rad/s^2[/tex]

Now, using the formula:

[tex]ω = α * t + ω0[/tex]

where

ω = instantaneous angular velocity at the end of 20.0 s (what we need to find)

[tex]α = angular acceleration = 20 rad/s^2[/tex]

[tex]t = time = 20.0 s[/tex]

[tex]ω0 = initial angular velocity = 0 (starting from rest)[/tex]

we get:

[tex]ω = 20 rad/s^2 * 20.0 s + 0 = 400 rad/s[/tex]

Therefore, the instantaneous angular velocity of the disk at the end of 20.0 s is 400 rad/s.

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The magnetic field on the axis of the solenoid is 5.03 × 10⁻⁴ T.

The magnetic field on the axis of a solenoid can be calculated using the formula:

B = μ₀ * n * I

Where B denotes the intensity of the magnetic field, 0 denotes the permeability of empty space, n denotes the number of turns per unit length, and I is the current flowing through the solenoid.

In this case, the solenoid is 1 meter long and has 200 turns, so n = 200 turns / 1 meter = 200 turns/meter. The solenoid is delivering 2A of current.

The value of μ₀ is a constant, equal to 4π × 10⁻⁷ T·m/A

When we enter these values into the formula, we get:

B = μ₀ * n * I

= 4π × 10⁻⁷ T·m/A * 200 turns/m * 2A

= 5.03 × 10⁻⁴ T

Therefore, the magnetic field on the axis of the solenoid is 5.03 × 10⁻⁴ T.

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magnetic field on the axis of the solenoid is approximately 0.005 T

Solution -  Hi! To calculate the magnetic field on the axis of a solenoid, you can use the formula:

Magnetic field (B) = μ₀ * n * I . (applicable for ideal long solenoid)

where μ₀ is the permeability of free space (approximately 4π x 10^-7 Tm/A), n is the number of turns per unit length, and I is the current.

In your case, the solenoid is 1 meter long with 200 turns and carries a 2 A current. To find n, divide the number of turns by the length:

n = 200 turns / 1 m = 200 turns/m

Now, plug the values into the formula:

B = (4π x 10^-7 Tm/A) * (200 turns/m) * (2 A)

B ≈ 0.005 T

The magnetic field on the axis of the solenoid is approximately 0.005 T (Tesla).

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The priority nursing action in this scenario would be to notify the provider.

An epidural anesthesia block can cause a drop in blood pressure in the mother, which can in turn affect the fetal heart rate.

A blood pressure reading of 80/40 mmHg is considered low, and can indicate hypotension.

Hypotension can lead to decreased blood flow to the placenta and fetus, which can result in fetal distress.

Therefore, it is important for the provider to be notified of the low blood pressure reading and fetal heart rate, so that appropriate interventions can be implemented to address the situation.

The provider may choose to adjust the dosage of the epidural anesthesia, administer IV fluids, or consider other measures to stabilize the mother's blood pressure and fetal well-being.

While monitoring vital signs and positioning the client can also be important interventions, they are not the priority in this scenario.

Elevating the client's legs may help to increase blood flow to the heart and improve blood pressure, and placing the client in a lateral position may also help to improve blood flow and prevent supine hypotensive syndrome.

These actions should be taken after the provider has been notified and appropriate interventions have been implemented.

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To determine the focal length of a corrective lens required to make the far point distance infinite, we need to follow these steps:

1) Measure the person's far point distance: This can be done by having the person read letters on an eye chart or by using a refractometer.

Let's assume the person's far point distance is 3 meters.

2) Determine the person's current corrective lens prescription: If the person already wears corrective lenses, their current prescription can be used to calculate the required focal length of the corrective lens.

If they do not wear corrective lenses, this step can be skipped.

3) calculate the person's current refractive error: This can be done by subtracting the measured far point distance from infinity (1/∞) and converting the result to diopters.

For example, if the person's far point distance is 3 meters, their refractive error would be -0.33 diopters (1/3m = 0.33 D).

4) Determine the focal length of the corrective lens required to make the far point distance infinite: This can be done by adding the person's refractive error to the desired focal length of infinity (1/0 = 0 D).

For example, if the person's refractive error is -0.33 diopters, the required focal length of the corrective lens would be 0.33 meters or 33 centimeters.

Therefore, the person would need a corrective lens with a focal length of 33 centimeters to make their far point distance infinite.

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To determine the ratio of turns of the transformer, we can use the principle of conservation of power, which states that power in equals power out in an ideal transformer.

The power input to the hair dryer is:

P = VI = (8 A)(114 V) = 912 W

The power output of the transformer should be the same as the input power, so we can use this equation to find the current in the secondary circuit:

P = VI = (I_s)(237 V)

where I_s is the current in the secondary circuit. Solving for I_s, we get:

I_s = P/V_s = (912 W)/(237 V) = 3.85 A

Now we can use the turns ratio equation to find the ratio of the turns in the transformer:

N_p/N_s = V_p/V_s = (114 V)/(237 V)

where N_p and N_s are the number of turns in the primary and secondary coils, respectively. Solving for N_p/N_s, we get:

N_p/N_s = 0.481

Therefore, the ratio of turns in the transformer should be approximately 0.481.

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True a significant factor in algal blooms and the excessive growth of aquatic vegetation that results in competition for sunlight and congestion.

Job competition is fierce. Computer firms compete fiercely with one another. The two businesses are in opposition to one another.It can also be described more broadly as the either direct or indirect relationship between species that affects fitness when they share a resource.When there is monopolistic competition, several vendors offer differentiated goods—goods with minor differences but similar functions.

Therefore, every animal, plant, mould, protist, organism, or archaeon found on Earth would be considered an organism. There are numerous methods to categorise these species.a single organism that uses its organs to carry out its life's functions

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The new velocity of the less massive train car has a velocity of 10 m/s after the collision.

Velocity is a measure of the rate and direction of an object's motion. It is a vector quantity, meaning it has both magnitude and direction. Velocity is typically represented by the equation v = s/t, where v is the velocity, s is the displacement (or distance travelled), and t is the time taken. Velocity is often confused with speed, which is the measure of the magnitude of an object's motion. Speed is a scalar quantity and is represented by the equation s = t/v.

The total momentum of the two train cars before the collision is calculated by multiplying the mass of each car by its velocity.

The total momentum of the system before the collision is 2000 kg x 10 m/s + 1000 kg x 3 m/s = 23000 kg m/s.

The total momentum of the system after the collision is 2000 kg x 6 m/s + 1000 kg x v, where v is the velocity of the less massive train car after the collision.

Therefore, we can set up the equation 23000 = 12000 + 1000v and solve for v.

v = 10 m/s.

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As a planet orbits a star, it makes a big ellipse, but its gravity has a similar effect on the star, causing the star to make a small star. This is called the "gravitational wobble" or "stellar wobble".

As a planet orbits a star, it follows an elliptical path due to the gravitational pull of the star. The shape of the planet's orbit is determined by the balance between the gravitational force of the star and the planet's own motion. However, the planet's gravity also affects the star, causing it to move slightly in response to the planet's pull. This motion of the star is much smaller than that of the planet, but it is still measurable and can be observed. This phenomenon is known as the planet's gravitational influence on the star, which causes the star to wobble slightly. This effect is used by astronomers to detect and study exoplanets orbiting distant stars.

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The phenomenon that occurs when a planet orbits a star, causing both the planet and the star to make elliptical motions due to their mutual gravitational effects.

This phenomenon is known as the "wobble" or "stellar wobble" and is caused by the gravitational interaction between a planet and its star. As a planet orbits a star, it exerts a gravitational force on the star, causing it to move slightly in response. This movement results in a small, periodic shift in the star's spectral lines, which can be detected by astronomers.

By analyzing this shift, astronomers can determine the presence, size, and orbital characteristics of planets around other stars. At the same time, the planet's gravity also affects the star, causing the star to make a smaller elliptical motion in response. This mutual gravitational interaction results in the observed stellar wobble.

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Answer:

1990.47 m/s

Explanation:

Answer: the answer is in the screen shots

Explanation:

Answer:

The basic concept of how a simple motor works is that you put electricity into it at one end and an axle (metal rod) rotates at the other end giving you the power to drive a machine of some kind. The simple motors you see explained in science books are based on a piece of wire bent into a rectangular loop, which is suspended between the poles of a magnet. In order for a motor to run on AC, it requires two winding magnets that don’t touch. They move the motor through a phenomenon known as induction.

I hope this helps! Let me know if I'm wrong!

Explanation:

Polaris and Kochab's apparent magnitude of 2 and their proximity to the celestial pole make them appear larger in a photo or planetarium simulation compared to other stars.

A comparatively brilliant star as compared to other stars in the night sky, Kochab and Polaris both have an apparent magnitude of 2, making them both bright stars. In addition, they are both close to the celestial pole, which gives them a motionless appearance in the sky while giving the impression that other stars are rotating around them.

They stand out in the night sky because of their fixed location and brightness, and because of their brightness and proximity to the celestial equator, they look bigger than other stars in pictures or planetarium simulations.

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When retrograde motion occurs and how it is related to Mars's orbit around the Sun:

Retrograde motion occurs when a planet appears to move backward in the sky from Earth's perspective. In the case of Mars, this happens when Earth overtakes Mars in their respective orbits around the Sun.

To understand when Mars will be in retrograde motion, consider these steps:

1. Picture both Mars and Earth orbiting the Sun, with Mars having a larger, slower orbit due to its greater distance from the Sun.
2. As Earth moves faster in its orbit, it eventually catches up to and passes Mars.
3. During this time, the relative positions of Earth, Mars, and the Sun create the illusion of Mars moving backward in the sky, as seen from Earth.

So, when trying to identify the spot where Mars will be in retrograde motion, look for the point in its orbit where Earth is passing Mars, creating the optical illusion of Mars moving backward in the sky.

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Voyager 1 will continue moving with the speed it will have when the fuel runs out. The probe is traveling through the vacuum of space, where there is negligible gravity and no significant air resistance to slow it down.

Without the ability to adjust its trajectory, Voyager 1 will continue on its current path indefinitely unless it encounters a gravitational field that alters its trajectory. The probe may eventually drift off course and potentially collide with other celestial objects in its path. While Voyager 1 will continue to communicate data to Earth until its systems eventually fail, it will eventually become just another piece of space debris, floating silently through the cosmos.

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Distance the masses on the right of the fulcrum need to be to balance with the two masses on the left is (3.5kgm - x kg * d m) / 1kg

In order for a lever to be balanced, the moments on either side of the fulcrum need to be equal. The moment is calculated by multiplying the distance from the fulcrum by the mass of the object. Therefore, to balance the two masses on the left of the fulcrum with the masses on the right, we need to calculate the moment on each side and make them equal.

Let's assume the masses on the left of the fulcrum are 2kg and 3kg, and the masses on the right are x kg and y kg, respectively. If the distance between the fulcrum and the 2kg mass is 1m, and the distance between the fulcrum and the 3kg mass is 0.5m.

we can calculate the moments on each side as follows:

Moment on the left side = 2kg x 1m + 3kg x 0.5m = 2kg + 1.5kg = 3.5kgm

Moment on the right side = x kg * d m + y kg * e m

where d and e are the distances between the fulcrum and the masses on the right.

To make the moments equal, we can set them equal to each other:

3.5kgm = x kg * d m + y kg * e m

If we know the mass of one of the objects on the right, we can solve for the distance needed for the other mass to balance the lever. For example, if we know the mass of the object closest to the fulcrum is 1kg.

we can rearrange the equation to solve for e:

e = (3.5kgm - x kg * d m) / 1kg

Once we know the distance needed for the other mass, we can set up the lever accordingly and it should be balanced.

The Question was Incomplete, Find the full content below :

A balanced lever has two weights on it, the masses on the left of the fulcrum are 2kg and 3kg, and the masses on the right are x kg and y kg. If the distance between the fulcrum and the 2kg mass is 1m, and the distance between the fulcrum and the 3kg mass is 0.5m.what is the distance the masses on the right of the fulcrum need to be to balance with the two masses on the left?

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the acceleration of the mass is 0.7212 m/s^2.

To find the acceleration of the mass, we need to first determine the net force acting on it. We can do this by using vector addition to add the two forces together.

Using the Pythagorean theorem, we can find the magnitude of the diagonal force:

sqrt[[tex](15N)^{2}[/tex] + [tex](10N)^{2}[/tex]] = sqrt[225 + 100] = sqrt(325) = 18.03 N

The direction of this force can be found using the inverse tangent function:

theta =[tex]tan^{-1}(10.0N/15.0N)[/tex] = 33.69 degrees north of east

We can now use vector addition to find the net force on the mass:

F_net = sqrt[[tex](15N)^{2}[/tex] + [tex](10N)^{2}[/tex]] = 18.03 N, at an angle of 33.69 degrees north of east

To find the acceleration of the mass, we can use Newton's second law, which states that the net force acting on an object is equal to its mass times its acceleration:

F_net = ma

Solving for the acceleration, we get:

a = F_net / m = 18.03 N / 25.0 kg = 0.7212 m/s^2

Therefore, the acceleration of the mass is 0.7212 m/s^2.

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Sonar can be a useful tool for monitoring the hydrosphere, which includes all of the water on and beneath the Earth's surface.

Sonar works by emitting sound waves that bounce off objects in the water, and then measuring the time it takes for the sound waves to return to the source. By analyzing the echoes, scientists can map the seafloor, measure the depth of the water, and even identify the size and location of marine organisms.

Sonar can also be used to monitor the movements of water masses, including ocean currents, tides, and storm surges. This information is important for understanding global climate patterns and predicting the effects of natural disasters

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The amplitude of the magnetic field of the electromagnetic wave is 6.53 x 10^-7 T.

To find the amplitude of the magnetic field of an electromagnetic wave, we need to use the relationship between the electric and magnetic fields in an electromagnetic wave.

According to this relationship, the amplitude of the magnetic field is equal to the amplitude of the electric field divided by the speed of light (c). Therefore, if the amplitude of the electric field of an electromagnetic wave is 196 V/m, the amplitude of the magnetic field can be calculated as follows:

Amplitude of magnetic field = Amplitude of electric field / Speed of light
Amplitude of magnetic field = 196 V/m / 3 x 10^8 m/s
Amplitude of magnetic field = 6.53 x 10^-7 T

It is important to note that the amplitude of the magnetic field and the electric field of an electromagnetic wave are perpendicular to each other and are responsible for the wave's propagation through space.

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The intensity level of the resulting sound is approximately 73 dB, the correct option is (e)

To calculate the intensity level of the resulting sound, we use the formula:

L = 10 log(I ÷ I0)

where L is the intensity level in decibels, I is the intensity of the sound wave in watts per square meter, and I0 is the reference intensity, which is equal to 1 x 10⁻¹² watts per square meter.

Since the motorcycles emit identical sound waves, the intensity of each wave is the same. We can calculate the intensity of a single motorcycle's sound wave using the formula:

I = [tex](10^{L/10} )[/tex] x I0

where L is the intensity level of the sound wave in decibels. Substituting L = 70 dB and I0 = 1 x 10⁻¹² watts per square meter, we get:

I = (10⁷) x 1 x 10⁻¹²

= 1 x 10⁻⁵ watts per square meter

To calculate the intensity level of the resulting sound, we use the formula:

L = 10 log(2I ÷ I0)

where 2I is the intensity of the sound waves produced by two identical motorcycles. Substituting I = 1 x 10⁻⁵ watts per square meter and I0 = 1 x 10⁻¹² watts per square meter, we get:

2I = 2 x 1 x 10⁻⁵

= 2 x 10⁻⁵ watts per square meter

L = 10 log(2 x 10⁻⁵ ÷ 1 x 10⁻¹²)

= 10 log(2 x 10⁷)

= 10 (7.301)

= 73.01 dB

Therefore, the correct option is (e)

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The complete question is:

A motorcycle passing by your apartment emits a sound with an intensity level of 70 dB. If two identical motorcycles passed by together, what would be the intensity level of the resulting sound?

a. 80 dB

b. 140 dB

c. 103 dB

d. 70 dB

e. 73 dB

The upper limb is the side of the chicken's body did this wing belong to.

Humerus, shoulder, and joint are related to the anatomy of the upper limb. The humerus is the long bone in the upper arm, the shoulder is the joint that connects the arm to the body, and the joint refers to the articulation between bones.

In a chicken, the shoulder joint is located at the junction of the humerus (upper arm bone) and the scapula (shoulder blade). It is a ball-and-socket joint that allows for a wide range of motion in the chicken's wing. The shoulder joint is important for a chicken's ability to fly, flap its wings, and perform other movements that require mobility and stability in the upper limb.

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The equivalent capacitance of the new circuit with an identical capacitor added in series is half of the original circuit's capacitance.

When a second capacitor, identical to the original, is added in series to the circuit, the equivalent capacitance of the new circuit is reduced. This is because the total capacitance in a series circuit is always less than the individual capacitances. The formula for calculating the equivalent capacitance of a series circuit is:

[tex]1/Ceq = 1/C1 + 1/C2 + ... + 1/Cn[/tex]

Where C1, C2, ..., Cn are the capacitances of the individual capacitors.

Adding another capacitor in series to the circuit means that the equivalent capacitance will be smaller, and the total charge stored in the circuit will be less. This will affect the behavior of the circuit when connected to a voltage source, as it will take less time to charge and discharge.

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The wavelength of a radio photon from an AM radio station broadcasting at 1270 kilohertz is 236 meters.

To find the wavelength of a radio photon from an AM radio station broadcasting at 1270 kilohertz, we can use the formula:
wavelength (λ) = speed of light (c) / frequency (f)

1. First, we need to convert the frequency from kilohertz to hertz:
1270 kilohertz = 1270 * 10³ hertz = 1,270,000 hertz

2. Next, we will use the speed of light, which is approximately 3.00 * 10⁸ meters per second (m/s).

3. Now, we can plug in the values into the formula:
wavelength (λ) = (3.00 * 10⁸ m/s) / (1,270,000 Hz)

4. Calculate the wavelength:
λ ≈ 236.22 meters

5. Finally, express the answer to three significant figures and include the appropriate units:
λ ≈ 236 meters

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The hotter an object is, the brighter and redder it appears, while cooler objects appear dimmer and bluer.

The question is asking about the relationship between an object's temperature and its brightness, color, and speed. The correct answers are that the hotter an object is, the brighter it appears and the redder it appears.

This is because hot objects emit more light, including more of the red end of the spectrum. The opposite is also true, meaning that cooler objects appear dimmer and bluer.

The speed of an object is not directly related to its temperature, so that answer is incorrect. However, it is important to note that the temperature of an object can affect its movement and velocity in certain situations.

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The i component of the magnetic force on the wire is 1.06 × 10^-13 N. The k component of the magnetic force on the wire is 6.69 × 10^-14 N. The magnitude of the magnetic force on the wire is 1.26 × 10^-13 N.

To calculate the i component of the magnetic force, we use the formula:

F = I * L x B

where I is the current, L is the length of the wire, B is the magnetic field, and x represents the cross product.

The cross product of L and B gives a vector perpendicular to both L and B, which is in the i direction. So we only need to find the magnitude of the cross product and multiply it by I to get Fx.

|L x B| = |L| |B| sinθ

where θ is the angle between L and B. Since L is in the j direction and B has i and k components, we have:

|L x B| = L * Bz = (3.8 × 10^-3 m) * (1.1 × 10^-4 T) = 4.18 × 10^-8 N

Then, Fx = I * |L x B| = (2.54 × 10^-6 A) * (4.18 × 10^-8 N) = 1.06 × 10^-13 N

To calculate the k component of the magnetic force, we use the same formula and take the k component of the cross product:

|L x B|k = |L| |B| sin(π/2) = |L| |B| = (3.8 × 10^-3 m) * (6.9 × 10^-5 T) = 2.63 × 10^-7 N

Then, Fz = I * |L x B|k = (2.54 × 10^-6 A) * (2.63 × 10^-7 N) = 6.69 × 10^-14 N

The magnitude of the magnetic force is given by,

F = sqrt(Fx^2 + Fz^2) = sqrt((1.06 × 10^-13 N)^2 + (6.69 × 10^-14 N)^2) = 1.26 × 10^-13 N

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The solid forms of ice last longer because there is more weight with less surface area. This statement is false.

Factors like temperature, shape, size, humidity and impurities are some of the factor decides the time for which the ice survives. Even though larger ice particles may have more surface area than solid forms of ice, this does not always imply that they will persist longer.

In reality, due to the insulating effect of the ice itself, larger ice formations, like glaciers, can melt more quickly. In the end, a complex combination of physical, chemical, and environmental elements determines how long ice will last.

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When the distance between two charges is halved, the electrical force between the charges quadruples. This is due to the inverse square relationship between distance and electrical force, which means that when distance is halved, the force increases by a factor of 4.

The electrical force between the charges quadruples when the distance between them is halved. This is due to Coulomb's Law, which states that the electrical force (F) between two charges (q1 and q2) is directly proportional to the product of the charges and inversely proportional to the square of the distance (r) between them. Mathematically, it can be expressed as:

F = k * (q1 * q2) / r^2

When the distance (r) is halved, the denominator (r^2) becomes 1/4 of its original value, which causes the electrical force (F) to be 4 times greater, or quadruple.

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Answer:

C

Explanation:

Glass is one of the objects included in an insular so glass rod will be the final ans.