(334-17) Nonmetallic sheathed cables run through framing members are considered to be adequately supported.(True/False)

Galaxy evolution refers to the changes that occur in galaxies over time. These changes can include the formation of new stars, the merging of galaxies,

And the development of different structures within a galaxy Telescopic observations are crucial for studying galaxy evolution because they allow us to observe galaxies in great detail, both in visible and non-visible wavelengths.

By studying these observations, astronomers can track changes in a galaxy's structure, composition, and behavior over time. Theoretical models are also essential for studying galaxy evolution.

These models use complex mathematical equations to simulate how galaxies form and evolve over time.

These models can help astronomers understand how galaxies form, how they grow, and how they change over time. Theoretical models can also help predict future changes in galaxies, allowing astronomers to better understand the long-term evolution of the universe.

In summary, galaxy evolution refers to the changes that occur in galaxies over time. Telescopic observations are essential for studying galaxy evolution, as they allow astronomers to observe galaxies in great detail.

Theoretical models are also crucial, as they allow astronomers to simulate the formation and evolution of galaxies and make predictions about future changes.

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Jupiter is the largest. It is the largest planet in the Solar System, with a diameter of about 86,881 miles (139,822 kilometers).

The International Space Station (ISS) is a habitable artificial satellite in low Earth orbit, with a size of approximately 357 feet (109 meters) in length and 240 feet (73 meters) in width.

Venus is the second planet from the Sun and has a diameter of about 7,520 miles (12,104 kilometers), which makes it similar in size to Earth.

Mercury is the smallest planet in the Solar System, with a diameter of about 3,032 miles (4,879 kilometers).

Therefore, the correct answer is Jupiter.

The conductor allowable ampacity is a term used to refer to the maximum current that can safely flow through a conductor without causing damage or overheating. According to Section 240.4(D) of the National Electrical Code (NEC), the maximum overcurrent protection device for a No. 14 conductor is 15 amperes, for a No. 12 conductor it is 20 amperes, and for a No. 10 conductor it is 30 amperes.

However, it is important to note that this is a general rule and may not apply to all types of electrical equipment. Specifically, for motors or air-conditioners, a different set of rules apply, as stated in Section 240-3 of the NEC. It is crucial to follow these guidelines and regulations to ensure the safety and efficiency of the electrical system.

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To find the potential difference across the coil at this moment, we can use the formula:

V = L di/dt + R i

where V is the potential difference, L is the inductance, di/dt is the rate of change of current, R is the resistance, and i is the current.

Plugging in the given values, we get:

V = (440 m H)(3.60 A/s) + (3.25 ohms)(3.00 A)
V = 1.584 V + 9.75 V
V = 11.334 V

Therefore, the potential difference across the coil at this moment is 11.334 volts.
Hi! To calculate the potential difference across the coil, you need to consider both the resistive and inductive components.

For the resistive part, use Ohm's Law: V = I * R, where V is the voltage, I is the current, and R is the resistance.

V_resistive = 3.00 A * 3.25 ohms = 9.75 V

For the inductive part, use the formula: V = L * (dI/dt), where V is the voltage, L is the inductance, and (dI/dt) is the rate of change of current.

V_inductive = 440 mH * 3.60 A/s = 0.440 H * 3.60 A/s = 1.584 V

Now, sum up the resistive and inductive voltages to get the total potential difference across the coil:

V_total = V_resistive + V_inductive = 9.75 V + 1.584 V = 11.334 V

The potential difference across the coil at this moment is 11.334 V.

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The work done lifting the bucket to the top of the building is 3234 joules.

To find the work done, we need to calculate the energy required to lift the bucket to the top of the building.
First, we need to calculate the mass of the sand without the bucket. We can do this by subtracting the mass of the bucket from the total mass:
25 kg - 0.2 kg/m x 15 m = 22 kg
Now we can calculate the work done:
Work = Force x Distance
The force required to lift the bucket is equal to the weight of the sand (since the rope has negligible weight). The weight of the sand is equal to its mass multiplied by the acceleration due to gravity (9.8 m/s^2):
Weight of sand = 22 kg x 9.8 m/s^2 = 215.6 N
The distance lifted is 15 meters.
Work = 215.6 N x 15 m = 3234 J

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The work done in lifting the bucket to the top of the building is approximately 2940 joules.

To find the work done in lifting the bucket to the top of the building, we need to calculate the total amount of sand leaked and subtract that from the initial mass of the bucket.

The total amount of sand leaked can be found by multiplying the height of the building (15m) by the rate of leakage (0.2kg/m). So, the total amount of sand leaked is 15m x 0.2kg/m = 3kg.

The work done is given by the formula W = mgh, where W is the work done, m is the mass, g is the acceleration due to gravity (9.8 m/s^2), and h is the height. Plugging in the values, we get W = (25kg - 3kg) x 9.8 m/s^2 x 15m = 2940 J.

Therefore, the work done in lifting the bucket to the top of the building is approximately 2940 joules.

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The type structures are indoor levels of formaldehyde likely to be rather high in Mobile homes. Option C is the correct answer.

Indoor levels of formaldehyde are likely to be rather high in mobile homes. This is because formaldehyde is commonly used in the manufacturing of many of the building materials used in mobile homes, such as particleboard, plywood, and insulation.

These materials are known to release formaldehyde gas over time, particularly in warm and humid conditions. As a result, mobile homes, which are often constructed with these materials in enclosed spaces, can have higher levels of formaldehyde than other types of structures.

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The term is used to describe the exposure of large populations to ionizing radiation (c). radiation-rem is correct option.

Therefore the correct option is (c).

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The volume in the cylinder after the gas is compressed is 68.75 in³, which is closest to option A (23.6 in³).

To solve this problem, we can use Boyle's law, which states that the product of the pressure and volume of a gas is constant as long as the temperature remains constant. We can express this law using the following formula:

P₁V₁ = P₂V₂

Where P₁ and V₁ are the initial pressure and volume, and P₂ and V₂ are the final pressure and volume.

First, we need to convert the atmospheric pressure from psi to lb/in² by multiplying it by 144 (since there are 144 square inches in a square foot):

14.7 psi * 144 = 2116.8 lb/in²

Next, we can use the formula to solve for the final volume:

30 lb/in² * 50 in³ = 80 lb/in² * V₂

V₂ = (30 lb/in² * 50 in³) / 80 lb/in²

V₂ = 18.75 in³

Finally, we need to add the initial volume to the final volume to get the total volume after compression:

V_total = V₁ + V₂ = 50 in³ + 18.75 in³ = 68.75 in³

Closest choice is option A.

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D) the combined effect of spiral density waves can cause a galactic fountain.

Galactic fountains are a phenomenon where gas is ejected from the disk of a galaxy into the halo and then falls back onto the disk. The gas is heated and ionized by various processes, including winds and jets from newly-formed protostars and supernovae occurring in the halo. However, the primary mechanism that drives the gas out of the disk is the combined effect of spiral density waves, which can create areas of higher pressure and density that cause the gas to move outward. Once in the halo, the gas can cool and fall back onto the disk, contributing to the formation of new stars.

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a. Two conditions that can affect friction and traction are the type of surface and the presence of contaminants.

b. Loss of friction and traction can cause a car to slide, skid, or lose control.

Friction and traction are crucial for vehicle handling and control. Two conditions that can affect friction and traction are the surface condition and the tire condition.

Wet, icy, or uneven road surfaces can decrease friction and traction, while worn or improperly inflated tires can also reduce the ability to maintain traction.

Loss of friction and traction can result in a variety of handling issues, such as difficulty steering, reduced braking ability, and increased risk of skidding or sliding.

This can be particularly dangerous in adverse weather conditions or during sudden stops or turns, making it important for drivers to maintain their vehicles properly and adjust their driving habits to match the current road conditions.

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Answer:

a c

Explanation:

Crystal form, hardness, cleavage, color, and density. Option D

Crystal form is the most useful physical property for mineral identification, as it is unique for each mineral and can be easily observed with the eye. Hardness is the next most useful property, as it can be tested with common tools like fingernails. Cleavage, or the way a mineral breaks along planes of weakness, can also provide important clues to identification.

Color is generally considered a less reliable indicator of mineral identity, as many minerals can have a wide range of colors. Density can be helpful in distinguishing between similar-looking minerals, but is not always a definitive characteristic.

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a. True. The dose or energy absorbed by an irradiated object is indeed a function of both the kilovolt and the milliampere settings of the machine.

The kilovolt setting affects the energy of the radiation, while the milliampere setting influences the intensity of the radiation. Both settings play a role in determining the absorbed dose. he kilovolt (kV) setting on an X-ray machine determines the peak energy of the X-ray beam and the milliampere (mA) setting determines the amount of X-ray photons emitted. The kilovolt setting determines how efficiently the X-ray beam penetrates the object, while the milliampere setting determines the total number of X-ray photons in the beam. Therefore, the dose or energy absorbed by an irradiated object is a function of both the kilovolt and the milliampere settings of the machine.

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The average acceleration during skiing is 0.4 [tex]m/s^2.[/tex]

To calculate the average acceleration, we can use the following equation:

average acceleration = (final velocity - initial velocity) / time

We can assume that the initial velocity is 0 m/s since we start from rest. We need to find the time it takes to travel the horizontal distance of 500 m.

To do this, we can use the following equation:

distance = average velocity x time

We can calculate the average velocity as:

[tex]average velocity = (0 m/s + 20 m/s) / 2 \\= 10 m/s[/tex]

Substituting this and the distance of 500 m into the equation above, we get:

[tex]500 m = 10 m/s * time[/tex]

Solving for time, we get:

[tex]time = 500 m / 10 m/s \\= 50 s[/tex]

Now we can calculate the average acceleration as:

average acceleration = (final velocity - initial velocity) / time

[tex]= (20 m/s - 0 m/s) / 50 s \\= 0.4 m/s^2[/tex]

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--The complete Question is, If you go skiing on a 1200 m vertical mountain and reach a final velocity of 20 m/s after traveling a horizontal distance of 500 m, what is your average acceleration? --

The speed of the spaceship in terms of the speed of light is approximately 0.7807.So the speed of the spaceship is approximately 0.6 times the speed of light.

This is a question related to special relativity and time dilation. The time dilation formula is given by:

t' = t / sqrt(1 - v^2/c^2)

Where t' is the time interval measured by the astronaut, t is the time interval measured by the observer on earth, v is the velocity of the spaceship, and c is the speed of light.

We know that t = 10.0 years and t' = 6.27 years. Substituting these values into the formula, we get:

6.27 = 10.0 / sqrt(1 - v^2/c^2)

Squaring both sides and rearranging, we get:

v^2/c^2 = 1 - (6.27/10.0)^2

v^2/c^2 = 0.6084

Taking the square root of both sides, we get:

v/c = 0.7807

Therefore, the speed of the spaceship in terms of the speed of light is approximately 0.7807.

To find the speed of the spaceship in terms of the speed of light, we can use the concept of time dilation in special relativity. Time dilation occurs when an object is moving at a significant fraction of the speed of light.

The time dilation formula is:
t' = t / √(1 - v²/c²)

where t' is the time experienced by the astronaut on the spaceship (6.27 years), t is the time experienced by someone in Earth's rest frame (10.0 years), v is the spaceship's velocity, and c is the speed of light.

Rearranging the formula to solve for v, we get:
v = c * √(1 - (t'/t)²)

Substituting the given values, we find the speed of the spaceship:
v = c * √(1 - (6.27/10.0)²)

v ≈ 0.6c

So the speed of the spaceship is approximately 0.6 times the speed of light.

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A steadily rising pressure usually indicates clearing weather or fair weather.

In general, changes in barometric pressure can be used to predict changes in weather conditions. A rising barometric pressure usually indicates that the weather is clearing up or will remain fair, while a falling barometric pressure often indicates that stormy weather is on the way.

A steadily rising pressure indicates that the air pressure is increasing and the weather is likely to improve or remain stable. In contrast, a steadily falling pressure indicates that the air pressure is decreasing, which could indicate an approaching storm or other atmospheric disturbance. Fluctuating pressure and constant pressure are not necessarily indicative of any specific weather conditions.

So, the correct answer is a. steadily rising.

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A steadily rising pressure usually indicates clearing weather or fair weather.

The pressure is an important factor in predicting weather conditions.

A barometer is used to measure atmospheric pressure and it is typically reported in inches of mercury or millibars.

Changes in atmospheric pressure can provide important clues about the weather conditions that are expected to occur in the near future.

When the atmospheric pressure is steadily rising, it typically indicates that clearing weather or fair weather is on the way.

This is because high pressure systems generally bring with them clear skies and dry air, which can make for pleasant weather conditions.

In contrast, when the atmospheric pressure is steadily falling, it is typically an indication that stormy weather is on the way.

This is because low pressure systems generally bring with them cloudy skies and moist air, which can lead to precipitation and thunderstorms.

A constant pressure may indicate that the current weather conditions are likely to persist for a while.

However, it is important to note that changes in wind patterns or temperature can still affect the weather, even if the pressure remains constant.

Fluctuating pressure can be an indication that weather conditions are likely to change rapidly.

For example, if the pressure is dropping quickly, it may indicate that a storm is approaching.

In summary, understanding the relationship between atmospheric pressure and weather conditions can be helpful in predicting the weather.

A steadily rising pressure usually indicates clearing weather or fair weather, while a steadily falling pressure usually indicates stormy weather.

A constant pressure may indicate that the current weather conditions are likely to persist, while fluctuating pressure can be an indication that weather conditions are likely to change rapidly.

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The vectors graphically, you must place the tail of the second vector at the tail of the first vector. This means that the starting point of the second vector will be connected to the endpoint of the first vector. The sum of the two vectors will then be represented by a vector from the tail of the first vector to the head of the second vector.

The head of the first vector represents the starting point of the motion, and the tail of the second vector represents the final point of the motion. Remember that momentum is a vector quantity, meaning that it has both magnitude and direction, so it's important to take into account the direction of the vectors when adding them graphically.  To add two vectors graphically, follow these steps Draw the first vector on a graph, using an arrow to represent its direction and magnitude. Place the tail of the second vector at the head of the first vector, drawing an arrow to represent its direction and magnitude. Draw a new arrow the resultant vector that starts from the tail of the first vector and ends at the head of the second vector. This arrow represents the sum of the two vectors. So, to add vectors graphically, you place the tail of the second vector at the head of the first vector, and the sum is a vector from the tail of the first vector to the head of the second vector.

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The acceleration is calculated using the equation a = (2π/T)2x, where T is the period of oscillation (55 seconds), and x is the amplitude of oscillation (10 cm).

Acceleration is the rate of change of velocity. It is a vector quantity, meaning it has both magnitude and direction. Acceleration is the rate at which an object's speed or velocity changes over time. It can be described as the rate at which an object's velocity changes with respect to time. Acceleration can be positive, negative, or zero.

a) It will take approximately 27.5 seconds for the pumpkin to reach the equilibrium position for the first time.

b) The maximum speed of the pumpkin will be 0.18 m/s.

c) The maximum acceleration of the pumpkin will be 0.0032 m/s2.

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Overriding your headlights at night is dangerous because it reduces your reaction time and visibility. When you drive at a speed that doesn't allow you to stop within the distance illuminated by your headlights, you're overriding them. This can lead to accidents, as you might not see obstacles, pedestrians, or other vehicles in time to react.

Driving too fast for your headlights also affects your peripheral vision, making it more difficult to notice potential hazards on the side of the road.

Additionally, high speeds increase the likelihood of overcorrecting if you suddenly encounter a sharp curve or unexpected obstacle, potentially causing a loss of control.

To avoid these dangers, it is crucial to maintain a safe driving speed at night, ensuring you can stop within the illuminated area provided by your headlights.

This practice will help increase visibility and reaction time, reducing the risk of accidents and keeping you and others on the road safe.

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It's risky to turn off your headlights at night since it makes it harder to see and react. You are overriding your headlights when you are travelling at a speed that prevents you from stopping in the area.

That your headlights are illuminating. Because you might not see barriers, pedestrians, or other vehicles in time to react, this can result in accidents.

Peripheral vision is also impacted by driving too fast for your headlights, making it more challenging to see possible hazards on the side of the road.

High speeds also make it more likely that you may overcorrect if you suddenly come upon a sharp curve or an unexpected barrier, which could result in a loss of control.

Maintaining a safe speed while driving at night is essential to avoiding these risks and making sure you can stop inside the area your headlights have illuminated.

This routine will improve your vision and reaction time, lowering your risk of accidents and ensuring your safety and the safety of other drivers.

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The smallest number of cubes needed is 28. This forms a 3x3x3 cube with one central cube missing.

To minimize the number of protruding snaps while maximizing the number of receptacle holes, the cubes should be arranged in a 3x3x3 cube formation.

This structure would have 27 cubes, but one central cube must be removed to eliminate all protruding snaps.

Each of the remaining 26 cubes will have at least one side with receptacle holes facing outward.

The missing central cube ensures no protruding snaps are exposed.

Therefore, the smallest number of snap-together cubes needed to have only receptacle holes showing is 28.

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The well needs 7.94 pounds of chlorine gas to meet the water quality objectives.

To calculate the pounds of chlorine gas required per day, we need to convert the flow rate and dosage into consistent units.

First, we convert the flow rate of 2000 gallons per minute to pounds per day.

2000 gpm x 60 minutes x 24 hours = 2,880,000 gallons per day

1 gallon of water weighs approximately 8.34 pounds, so 2,880,000 gallons weigh:

2,880,000 gallons x 8.34 pounds/gallon = 24,019,200 pounds per day

Next, we convert the chlorine dosage of 2.5 gpm to pounds per day:

2.5 grams per minute x 60 minutes x 24 hours = 3,600 grams per day

1 pound is equivalent to 453.59 grams, so we convert the dosage to pounds:

3,600 grams per day / 453.59 grams per pound = 7.94 pounds per day

Therefore, the well needs 7.94 pounds of chlorine gas to meet the water quality objectives.

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Those involved in hazardous waste operations at permitted TSD facilities must receive 40 hours of initial training. The correct answer is (c).

Hazardous waste operations involve handling and managing potentially dangerous substances, and it is essential that employees are adequately trained to ensure their safety and the safety of others. OSHA's Hazardous Waste Operations and Emergency

Response (HAZWOPER) standard requires employees involved in hazardous waste operations at permitted Treatment, Storage, and Disposal (TSD) facilities to receive a minimum of 40 hours of initial training. This training includes topics such as hazard recognition, personal protective equipment, and emergency response procedures. Additionally, employees who are expected to respond to emergency situations must receive an additional 8 hours of specialized training. The correct answer is (c).

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Since the red ball attains twice the speed of the blue ball, we know that it also travels twice the distance in the same amount of time.

Since both balls have the same mass, we can use the equation:
work = force x distance
to compare the work done on each ball.
Let's call the force applied to the red ball F1 and the force applied to the blue ball F2.
We know that the red ball attains twice the speed of the blue ball, so we can write:
v1 = 2v2
Using the equation for acceleration:
a = F/m
we can rearrange to solve for the net force on each ball:
F1 = m*a1
F2 = m*a2

We can then substitute the equation for acceleration:

F1 = m*(v1/t)

F2 = m*(v2/t)

where t is the time it takes for each ball to reach its final speed.
We can then compare the work done on each ball:
work1 = F1*d
work2 = F2*d

where d is the distance each ball travels during the time it takes to reach its final speed.

d1 = 2d2
Substituting this into the equations for work:
work1 = F1*2d2
work2 = F2*d2

Dividing these two equations:
work1/work2 = (F1*2d2)/(F2*d2)
Simplifying:
work1/work2 = F1/F2

Since we know that the red ball attains twice the speed of the blue ball, we can also conclude that the net force applied to the red ball is twice that of the blue ball:

F1 = 2F2
Substituting this into the equation for work ratio:
work1/work2 = 2F2/F2
work1/work2 = 2

Therefore, the work done on the red ball is twice that of the blue ball.
When comparing the work done on the red ball to the blue ball, the work done on the red ball is four times greater than the work done on the blue ball. Since both balls have the same mass and the red ball attains twice the speed of the blue ball, the kinetic energy (which is proportional to the work done) is greater for the red ball by a factor of 2^2, as kinetic energy is calculated as (1/2)mv^2.

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Crater density and the color of the surface can be used to estimate the age of surfaces in the outer solar system.

Crater density is the number of craters per unit area on a planetary surface, and it is a useful indicator of the age of that surface. The basic principle is that the more craters a surface has, the older it is, because it has had more time to accumulate impacts.

By counting the number of craters on a surface, and comparing it to the number of craters on other surfaces of known age, scientists can estimate the age of that surface.

Another factor that can be used to estimate the age of a surface is the color of the surface. Over time, the surfaces of planets and moons are bombarded by solar radiation and cosmic rays, which can alter the chemical composition of the surface.

This alteration can change the color of the surface, and the amount of alteration can be used to estimate the age of the surface. Generally, the darker and redder the surface, the older it is, because it has had more time to be altered by radiation.

By combining these two methods, scientists can estimate the age of surfaces in the outer solar system, where direct observations and measurements are difficult to obtain. This information can help us better understand the history of these distant worlds and how they have evolved over time.

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The correct statement is: a carnot cycle has two isentropic processes and two isobaric reversible processes.

Any process that does not affect the system's entropy is called isentropic. It is reversible because it is a reversible of the cosmos. Real processes are irreversible because trying to turn them around would result in the cosmos becoming less entropic, which is not feasible.

There are 4 stages in the Carnot cycle:

-Gas expansion that is isothermal. It uses heat from a hot source in this procedure. It is not isentropic, but it is reversible.

– Diabatic growth. This one is isentropic, meaning that the entropy of the gas doesn't change over time and that it doesn't interact with its environment. The mechanism pulls on the gas to cause it to expand rather than the gas expanding on its own. The gas becomes cooler.

compression that is isothermal. adiabatic but not reversible. The gas's volume is decreased as a result of heat exchange with the cold source.

Diabatic compression. isentropic and adiabatic. The gas heats up as a result of the machine's compression of it.

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When possible, a water main should be tapped while still pressurized to ensure minimal disruption to the water supply and maintain system integrity.

1. Pressurized water main: A pressurized water main is a pipe that carries water under pressure from a treatment facility to homes and businesses. Maintaining pressure is important for efficient and reliable water delivery.
2. Tapping: Tapping is the process of connecting a new pipe or service line to an existing pressurized water main. This is usually done to extend water services to new customers or for infrastructure upgrades.
3. Minimal disruption: By tapping a water main while it is still pressurized, service providers can minimize disruptions to the water supply. This means customers may not experience a loss of water service during the tapping process.
4. System integrity: Keeping the water main pressurized during tapping helps maintain the overall integrity of the water distribution system. This is important to prevent leaks, contamination, and other potential problems.
In summary, when possible, a water main should be tapped while still pressurized to minimize disruption to the water supply, maintain system integrity, and provide a more efficient and reliable connection to the water distribution network.

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The energy becomes four times greater than the original energy.

The energy of a wave is proportional to the square of its amplitude. In the given problem, the amplitude of the 6 PM wave increases from 0.3 m to 0.6 m.

If the amplitude of the 6 PM wave increases to 0.6 m, the ratio of the new energy to the original energy can be calculated as follows:

(new energy) / (original energy) = (new amplitude)^2 / (original amplitude)^2

(new energy) / (original energy) = (0.6)^2 / (0.3)^2

(new energy) / (original energy) = 4

Therefore, if the amplitude of the 6 PM wave increases to 0.6 m, the energy becomes four times greater than the original energy.

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The frequency of light in a vacuum that has a wavelength of 71200 m is 4.213 kHz.

The frequency of light is obtained from the ratio of the speed of light and wavelength of light. The frequency,ν = c / λ, where c is the speed of the light in vacuum and is equal to 3×10⁸ m/s and λ is the wavelength of light.

From the given,

the wavelength of light = 71200 m

speed of light = 3×10⁸ m/s

Frequency =?

ν = c / λ

=  3×10⁸ / 71200

= 4.213 kHz.

The frequency of light in a vacuum is 4.213 kHz.

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The subject that is said to be at the crossroads of biology, physics, and geology is none of the above because It is actually the field of biophysics, which applies principles of physics to study biological systems and processes. Option D.

The subject that is said to be at the crossroads of biology, physics, and geology is none other than Biophysics. Biophysics is an interdisciplinary field that combines the principles of physics, biology, and chemistry to study biological systems at different levels, from molecules to organisms.

It involves the application of physical and mathematical tools to solve biological problems, such as understanding the structure and function of biomolecules, the mechanics of cells and tissues, the dynamics of neural networks, and the interactions between organisms and their environment. Therefore, option D) "none of the above" is the correct answer.

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Answer: Sand, anthracite, and garnet are all frequently used as filter material for water treatment.

Explanation:

Filtration: It is the process by which fine floc particles, color, dissolved minerals and micro-organisms are removed. It also removes suspended solids that do not get removed in sedimentation and it is also economically effective.

The following different types of material are used for water filtration process:

Carbon or activated carbon: Carbon is also known as charcoal. Anthracite is mostly used for water filtration.

Garnet sand ( chemically inert or non metallic mineral) is an ideal water filter media.