Create an argument on how "Gradualism, Uniformism, Volcanism and
nepotism, Discovery of time timeline" disregards time in a
mythological way and introduces the idea of analyzing time in a
naturalistic

Answers

Answer 1

The concepts of gradualism, uniformism, volcanism, and nepotism, along with the discovery of the geological time timeline, are fundamental principles in understanding Earth's history and the processes that shape it. These principles promote a naturalistic approach to analyzing time, devoid of mythological interpretations.

Gradualism suggests that geological changes occur slowly and incrementally over time, rather than through sudden, catastrophic events. Uniformism emphasizes the idea that the same natural laws and processes observed today have operated throughout Earth's history, enabling scientists to study present-day phenomena to understand past events. Volcanism, as a geological process, plays a significant role in shaping the Earth's surface through volcanic eruptions and associated landforms. Nepotism, however, seems to be out of place in this context, as it refers to favoritism based on family relationships rather than a geological concept. It seems to be an incorrect inclusion in the list of concepts related to time analysis.

The discovery of the geological time timeline has allowed scientists to reconstruct the Earth's history, understanding the sequence of geological events and the vast timescales involved. By studying the layers of rock and the fossils contained within them, scientists can piece together a naturalistic understanding of the Earth's past. Overall, these principles and the study of geological time provide a scientific framework to analyze and comprehend Earth's history, allowing us to move away from mythological interpretations and instead embrace a naturalistic approach to understanding the passage of time and the processes that have shaped our planet.

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Related Questions

newton's law of universal gravitation describes the relationship between:

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Newton's law of universal gravitation describes the relationship between the gravitational forces of two objects.

The Newton's law of universal gravitation is defined as the physical law that states that every point mass in the universe attracts every other point mass with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between them. In simpler terms, this law explains the relationship between the gravitational forces of two objects. This law is usually expressed in the mathematical equation F = G(m1m2/r2). Where F is the force between the masses, m1, and m2 are the masses, r is the distance between the centers of the masses, and G is the gravitational constant

According to Newton's law of universal gravitation, every point mass in the universe attracts every other point mass with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between them. This law applies to all objects regardless of their shape, size, or position. This law is one of the foundations of classical mechanics and helped scientists to explain a wide range of physical phenomena, including the orbits of planets around the sun, the movement of the moon around the earth, and the tides. The law of universal gravitation also explains why objects fall to the ground when dropped, why the Earth is able to keep a satellite in orbit, and why the force of gravity decreases with distance

Newton's law of universal gravitation is a significant law in physics that describes the relationship between the gravitational forces of two objects. This law is essential in explaining various physical phenomena and is a foundation for classical mechanics.

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What are some myths vs facts about climate change? Will climate
change affect food and/or energy supply?

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Myth: Climate change is a natural occurrence and not influenced by human activities. Fact: Extensive scientific evidence supports the conclusion that human activities, primarily the burning of fossil fuels and deforestation, are the primary drivers of the current climate change trends.

The release of greenhouse gases into the atmosphere is leading to the warming of the planet. Climate change is just a theory, and there is no consensus among scientists. The overwhelming majority of climate scientists agree that climate change is happening and is primarily caused by human activities. This consensus is supported by various scientific organizations and institutions worldwide, such as the Intergovernmental Panel on Climate Change (IPCC).

Climate change will have minimal impact on food and energy supplies. Climate change poses significant risks to global food and energy supplies. Rising temperatures, changing rainfall patterns, and extreme weather events can negatively affect agricultural productivity, leading to food shortages and price volatility. Additionally, climate change impacts energy supply by influencing the availability and distribution of renewable and non-renewable resources, affecting energy production and infrastructure. In summary, climate change is real, primarily caused by human activities, and has the potential to significantly impact food and energy supplies. Addressing climate change is crucial to mitigate these risks and ensure a sustainable future.

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1.Discuss why the division of the sensible (Ranciere) may be taken as a central argument to understand visual culture.
2. Discuss the concept of Panopticon and its relationship with the modern visual experience. In youranswers, do not forget to mention concepts like surveillance society, docile bodies, visibility... etc. Try to support your arguments with suitable examples

Answers

1. The division of the sensible according to Ranciere. The division of the sensible is an idea introduced by Jacques Ranciere that refers to the ways that society distributes roles and identities to individuals based on their position. This division creates distinctions between those who can be seen, heard, and understood and those who cannot.

2. Panopticon and its relationship with the modern visual experience. The panopticon is a concept introduced by Jeremy Bentham that refers to a prison design where inmates are constantly monitored by a single guard. This design allows the guard to observe all prisoners without them knowing when they are being watched.

1. The division of the sensible according to Ranciere. The division of the sensible is an idea introduced by Jacques Ranciere that refers to the ways that society distributes roles and identities to individuals based on their position. This division creates distinctions between those who can be seen, heard, and understood and those who cannot.

As a result, certain groups are given more power than others because of the ability to influence the way society views them. This concept is useful in understanding visual culture because it helps us see how certain images and objects are privileged over others.

We can see this in advertising, where certain images are used to sell products based on the values that society has assigned to them. For example, a luxury car may be advertised using images of wealth and success, whereas a family car may be advertised with images of safety and reliability.

2. Panopticon and its relationship with the modern visual experience. The panopticon is a concept introduced by Jeremy Bentham that refers to a prison design where inmates are constantly monitored by a single guard. This design allows the guard to observe all prisoners without them knowing when they are being watched.

This creates a sense of constant surveillance, which Bentham believed would be enough to reform prisoners. The panopticon has been used as a metaphor for modern society, where individuals are constantly being monitored through various means. This includes CCTV cameras, social media, and online tracking.

As a result, individuals are more aware of how they are being seen and how their actions are being judged. This has led to the concept of a surveillance society, where individuals are expected to conform to certain norms in order to avoid negative consequences.

This has also led to the idea of docile bodies, where individuals are expected to be compliant and obedient to those in power. The panopticon and its associated concepts have had a profound impact on the way we experience the world around us.

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__________ is the termination of a licensee’s privilege to drive a motor vehicle.

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License revocation is the termination of a licensee's privilege to drive a motor vehicle.

When a license is revoked, it means that the licensing authority has taken away the individual's driving privileges due to certain violations or offenses. License revocation is a more severe penalty compared to license suspension, as it typically involves a longer duration and stricter requirements for reinstatement.

The reasons for license revocation can vary depending on the jurisdiction, but common causes include serious traffic offenses, repeated violations, DUI (driving under the influence) convictions, reckless driving, or being deemed medically unfit to drive.

During a license revocation period, the individual is not legally allowed to operate a motor vehicle. To regain the driving privileges, the licensee usually needs to go through a reinstatement process, which may involve fulfilling certain conditions, such as completing a driver improvement program, paying fines, and serving the revocation period.

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a) Estimate the voltage of a typical car battery (in Volt).
b) Estimate the current delivered by a typical car battery (in Amp).
c) Estimate the power delivered by a car battery (in Watt).
d) Estimate the voltage of a typical lemon battery (in Volt).
e) Estimate the current delivered by a typical lemon battery (in Amp).
f) Estimate the power delivered by a lemon battery (in Watt).
g) Estimate how many lemons batteries would it take to start a car.

Answers

a) The voltage of a typical car battery is around 12 volts.

b) The current delivered by a typical car battery can vary, but it is typically in the range of a few hundred amps (e.g., 200-800 amps).

c) The power delivered by a car battery can be calculated by multiplying the voltage and current. Using an average current of 500 amps, the power delivered would be:

Power = Voltage x Current

Power = 12 volts x 500 amps

Power = 6000 watts or 6 kilowatts.

d) The voltage of a typical lemon battery is relatively low, usually around 0.7 to 1.5 volts. The exact voltage depends on factors such as the type and size of the lemon, as well as the electrodes used.

e) The current delivered by a typical lemon battery is very low, typically in the milliamp range (e.g., 0.1-1 milliamp).

f) The power delivered by a lemon battery can be calculated by multiplying the voltage and current. Assuming a voltage of 1 volt and a current of 0.5 milliamp:

Power = Voltage x Current

Power = 1 volt x 0.5 milliamp

Power = 0.5 milliwatts or 0.0005 watts.

g) It would take a large number of lemon batteries to start a car due to their low voltage and current. The specific number would depend on the power requirements of the car's starter motor and the capacity of the lemon batteries. In practice, it would be highly impractical to use lemon batteries to start a car.

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what can be said about the sign of the work done by the force

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The sign of the work done by a force depends on the angle between the force vector and the displacement vector of the object on which the force is acting.

If the force and displacement vectors are in the same direction (angle of 0 degrees), the work done by the force is positive. This means that the force is doing positive work, adding energy to the system.

If the force and displacement vectors are in opposite directions (angle of 180 degrees), the work done by the force is negative. This means that the force is doing negative work, removing energy from the system.

If the force and displacement vectors are perpendicular (angle of 90 degrees), the work done by the force is zero. This means that the force is not contributing or removing any energy from the system.

In summary, the sign of the work done by a force can be positive, negative, or zero depending on the angle between the force and displacement vectors.

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Why is terminal voltage of the cell more than its emf?

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The terminal voltage of a cell is less than its emf because of the internal resistance of the cell.

The voltage of the cell is commonly called the emf, or electromotive force. The energy of the cell, which is supplied by the chemical reactions that take place inside it, is represented by this voltage. The terminal voltage of a cell is the voltage that is present at the ends of the cell's terminals when the cell is connected to a circuit. When a cell is connected to a circuit, the current that flows through it experiences some resistance. This resistance causes the voltage that is present at the terminals of the cell to decrease. As a result, the terminal voltage of the cell is lower than its emf. The resistance is due to the internal resistance of the cell, which is the resistance of the cell's components to the flow of current. The internal resistance of the cell is caused by the cell's components, such as the electrodes and electrolytes. This resistance is always present, regardless of whether the cell is connected to a circuit or not. When the cell is connected to a circuit, the internal resistance is in series with the external resistance of the circuit. This causes the voltage that is present at the terminals of the cell to decrease.

When a cell is connected to a circuit, it is possible for the voltage that is present at the terminals of the cell to be less than the emf of the cell. This happens because of the internal resistance of the cell, which is always present. The internal resistance is caused by the components of the cell, such as the electrodes and electrolyte. This resistance is always present, regardless of whether the cell is connected to a circuit or not.When the cell is connected to a circuit, the internal resistance is in series with the external resistance of the circuit. This causes the voltage that is present at the terminals of the cell to decrease. The voltage drop that is caused by the internal resistance is directly proportional to the current that flows through the cell. As the current that flows through the cell increases, the voltage drop that is caused by the internal resistance also increases.

In conclusion, the terminal voltage of a cell is less than its emf because of the internal resistance of the cell. This resistance is caused by the components of the cell, such as the electrodes and electrolyte. When the cell is connected to a circuit, the internal resistance is in series with the external resistance of the circuit. This causes the voltage that is present at the terminals of the cell to decrease. The voltage drop that is caused by the internal resistance is directly proportional to the current that flows through the cell.

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Ping-Pong is another name for ____ ____, which is played at the Olympic level. Players use _____ to whack the ball across the table at dizzying speeds.

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Ping-Pong is another name for Table tennis, which is played at the Olympic level. Players use different types of strokes to whack the ball across the table at dizzying speeds.

Ping-Pong is another name for Table tennis, which is played at the Olympic level. Table Tennis is a sport played using a small, lightweight ball and a paddle. The players are separated by a net and they take turns hitting the ball back and forth across the table at high speeds.

The objective is to keep the ball in play and to force the other player to make a mistake.Table Tennis is played both as a singles and doubles game and is enjoyed by players of all ages and skill levels. It is played indoors on a table that is 2.74 meters long and 1.525 meters wide.

The net is 15.25 centimeters high and is placed directly in the center of the table.Each player uses a paddle, which is also called a racket or a bat, to hit the ball. The paddle is usually made of wood, rubber, or a combination of both. The rubber is used on both sides of the paddle to give it more grip and to help control the ball's spin.Players use different types of strokes to hit the ball, including forehand and backhand strokes.

There are also different types of serves, such as the topspin serve, the backspin serve, and the sidespin serve. Players can use these serves to put spin on the ball and make it more difficult for their opponent to return it.

In conclusion, Table Tennis is a fast-paced, exciting sport that requires speed, skill, and precision. It is a popular sport worldwide and is enjoyed by millions of people of all ages and skill levels.

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The weight of an object _________ as it moves away from the center of Earth.

Answers

Answer:

It Decreases

why is flood hazard mapping considered an important step in floodplain management?

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Flood hazard mapping is considered an important step in floodplain management because it provides valuable information about the areas at risk of flooding.

Detailed and accurate flood hazard maps depict the extent and magnitude of potential flooding, including flood-prone areas, flood depths, flow velocities, and flood frequencies. These maps help identify and assess the vulnerability of communities, infrastructure, and natural resources to floods.

By having access to flood hazard maps, policymakers, urban planners, and emergency management agencies can make informed decisions regarding land-use planning, zoning regulations, and development restrictions. This proactive approach helps reduce the exposure of communities to flood risks and minimizes potential damages to properties and infrastructure.

Furthermore, flood hazard maps aid in emergency preparedness and response efforts. They assist in the development of evacuation plans, the positioning of emergency resources, and the dissemination of early warning systems to alert residents in at-risk areas.

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what is the difference between a fire tube and a water tube boiler?

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The type of boiler that has the water running through the tubes is called a fire tube boiler. In a fire tube boiler, hot gases from a combustion process pass through the tubes that are submerged in water.

This heats up the water and generates steam which can be used for various industrial applications. Fire tube boilers are commonly used in small to medium-sized facilities, as they are compact and easy to install. They are also generally less expensive than water tube boilers, which have the water running through the tubes and the hot gases passing around them. Water tube boilers are typically used in larger facilities such as power plants.

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Geophysical surveys can provide information about the distribution of a physical property. What is the principle difficulty encountered when trying to use this information ?to identify a rock type There aren't any real difficulties Different rock types can have different values of a physical property A single sample of rock has multiple values of a physical property Different rock types can have the same value of a physical property O O O

Answers

The principle difficulty encountered when trying to use geophysical surveys to identify a rock type is that different rock types can have the same value of a physical property. Geophysical surveys rely on measuring specific physical properties, such as density, magnetism, electrical conductivity, or seismic wave velocity, to infer the composition or characteristics of subsurface rocks.

It is common for multiple rock types to exhibit similar values for a given physical property, making it challenging to differentiate them solely based on geophysical data. For example, two rock types may have similar densities, making it difficult to distinguish between them using density measurements alone. This can lead to ambiguities and uncertainties in interpreting the subsurface geology based solely on geophysical survey results.To overcome this difficulty, it is crucial to integrate geophysical data with other geological information, such as surface rock samples, borehole  including geophysical surveys, geological observations, and laboratory analyses, a more accurate characterization of rock types and subsurface geology can be achieved. Therefore, while geophysical surveys provide valuable insights into the distribution of physical properties, the challenge lies in the fact that different rock types can exhibit similar values for a given physical property, requiring the integration of multiple data sources for robust rock type identification.

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In order to determine the electrical resistance of the wire, the students connected it to a voltage source of 5 V and measured the current strength of 143 mA. What amount of electrical resistance did the students get if they had a wire 4 m long and 0.4 mm thick?​

Answers

The electrical resistance of the wire is 34.965 ohms.

The electrical resistance of the wire, the formula used is:

[tex]R=\frac{V}{I}[/tex]

where R is resistance, V is voltage and I is current.

To determine the electrical resistance of the wire, which is 4m long and 0.4mm thick, and connected to a voltage source of 5V with a current strength of 143 mA, the following formula can be used:

[tex]Resistance = \frac{Voltage }{Current }[/tex]

[tex]Resistance = \frac{5 V }{0.143 A}[/tex]

[tex]Resistance = 34.965 \Omega[/tex]

Where:

[tex]Resistance = 34.965 \Omega (ohms)[/tex]

[tex]Current = 143 mA = 0.143 A (amperes)[/tex]

[tex]Voltage = 5 V (volts)[/tex]

[tex]Length = 4 m (meters)[/tex]

[tex]Thickness = 0.4 mm (millimeters)[/tex]

In this case, we have all the data necessary to determine the electrical resistance of the wire.

To do this, we divide the voltage of 5 volts by the current strength of 143 milliamps, which gives us a result of 34.965 ohms.

Therefore, the students obtained 34.965 ohms as the amount of electrical resistance they measured of the wire.

Hence, the electrical resistance of the wire is 34.965 ohms.

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In a manufacturing facility, 5-cm-diameter brass balls (r = 8522 kg/m3 and cp = 0.385 kJ/kg • °C) initially at 120°C are quenched in a water bath at 50°C for a period of 2 min at a rate of 100 balls per minute. If the temperature of the balls after quenching is 74°C, determine the rate at which heat needs to be removed from the water in order to keep its temperature constant at 50°C.

Answers

To determine the rate at which heat needs to be removed from the water in order to keep its temperature constant at 50°C, we can use the principles of heat transfer and energy conservation.

First, let's calculate the heat transferred from each ball during the quenching process. We can use the equation:

Q = mcΔT

Where Q is the heat transferred, m is the mass of the ball, c is the specific heat capacity of brass, and ΔT is the change in temperature.

Given that the diameter of the ball is 5 cm, the radius (r) is 2.5 cm or 0.025 m. The volume of the ball is:

V = (4/3)πr^3

The mass can be calculated using the density formula:

m = ρV

Where ρ is the density of brass.

Now, we can calculate the mass of each ball and the total heat transferred from all the balls in 2 minutes.

Let's assume there are 100 balls per minute, so in 2 minutes, we have 200 balls.

Using the given values:

Density of brass (ρ) = 8522 kg/m^3

Specific heat capacity of brass (c) = 0.385 kJ/kg • °C

Initial temperature of the balls (T1) = 120°C

Final temperature of the balls (T2) = 74°C

For each ball:

V = (4/3)π(0.025)^3

m = ρV

Q = mcΔT

Calculate the total heat transferred:

Total heat transferred = Q × Number of balls

Finally, to determine the rate at which heat needs to be removed from the water, we divide the total heat transferred by the duration of quenching (2 minutes).

Rate of heat removal = Total heat transferred / Quenching time

Please note that the specific heat capacity is given in kJ/kg • °C, so we need to convert the mass of the ball from kg to grams for consistent units. Performing these calculations will provide the rate at which heat needs to be removed from the water.

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A sphere of radius r0 = 23.0 cm and mass = 1.20 kg starts from rest and rolls without slipping down a 33.0 degree incline incline that is 12.0 m long.
1.Calculate its translational speed when it reaches the bottom.
v=______________m/s
2. Calculate its rotational speed when it reaches the bottom.

Answers

1) The the translational speed of sphere when it reaches the bottom is 4.830 m/s.

v=4.830 m/s

2) The rotational speed of the sphere when it reaches the bottom is 21.0 rad/s.

Let us calculate the translational speed of the sphere when it reaches the bottom using the principle of conservation of energy.

Total energy at the top, E = Potential energy = mgh

Total energy at the bottom, E' = Kinetic energy + rotational kinetic energy + potential energy

V = Translational speed of sphere

ω = Rotational speed of sphere

Kinetic energy, K.E = 1/2 mv²

Rotational kinetic energy, K.E' = 1/2 Iω²

Where, I = Moment of inertia of the sphere

Let us calculate each term one by one

1) We know that

Moment of inertia of solid sphere, I = 2/5 mr²

Where, r is the radius of sphere, m is the mass of sphere

Substitute the given values and calculate

I = 2/5 × 1.20kg × (23.0cm)²

I = 0.686kg m²

Potential energy at the top, E = mgh

Where, g is the acceleration due to gravity

Substitute the given values and calculate

E = 1.20kg × 9.8 m/s² × 12.0mE

= 141.12 J

Kinetic energy at the bottom, K.E = E' - K.E'

Where, E' is the total energy at the bottom

Substitute the given values and calculate

K.E = (1/2) mv² + (1/2) Iω² - mgh

But, here the sphere is rolling without slipping. Therefore, v = rω

v = r0 ω

Substitute the given values and calculate

K.E = (1/2) mv² + (1/2) I (v/r0)² - mgh

141.12 = (1/2) (1.20kg) (r0ω)² + (1/2) (0.686kg m²) (ω/r0)² - (1.20kg) (9.8m/s²) (12.0m)

141.12 = 0.5 × 1.20 × (0.23ω)² + 0.5 × 0.686 × (ω/0.23)² - 137.088ω = 4.830 m/s

2) Now, let us calculate the rotational speed of the sphere when it reaches the bottom by substituting the value of v in the above equation.

ω = v/r0

ω = 4.830m/s / 0.23m

ω = 21.0 rad/s

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If a Solar Eclipse occurs when the Moon is farthest to Earth, and at some point, during the eclipse, the Moon is exactly in between the Sun and where we are standing on Earth's surface, what kind of Solar Eclipse would we observe (Total Solar Eclipse or Annular Solar Eclipse)? and Why? Note: Choose the type of eclipse and the reason [mark all correct answers]
a. Total Solar Eclipse
b. Annular Solar Eclipse
c. Reason: Because the Moon is too close to Earth and its angular size is too large, covering the whole sun as seen from earth.
d. Reason: Because the Moon is too far away from earth and its angular size is too large, covering the whole sun as seen from earth.
e. Reason: Because the Moon is not in the correct lunar phase
f. Reason: Because the angular size of the Moon is not large enough to cover the whole sun as seen from earth.
g. Reason: Because the angular size of the Moon is not small enough to cover the whole sun as seen from earth.

Answers

If a Solar Eclipse occurs when the Moon is farthest from Earth and aligns exactly between the Sun and Earth's surface, the type of Solar Eclipse observed would be an Annular Solar Eclipse. The correct reasons for this are options d and f.

During a Solar Eclipse, the Moon moves between the Sun and Earth, causing a temporary blockage of sunlight. In the given scenario where the Moon is farthest from Earth and in perfect alignment, an Annular Solar Eclipse would occur.

This means that the Moon's apparent size is not large enough to completely cover the Sun, resulting in a ring of sunlight known as an annulus being visible around the Moon. Option d is correct because when the Moon is farther away from Earth, its angular size appears larger, but it still does not cover the entire Sun. Option f is also correct because the angular size of the Moon is not large enough to fully block the Sun's disk, leading to the formation of the annulus.

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The current level of atmospheric _____ recently surpassed parts per million.
(a) chlorofluorocarbons
(b) water vapor
(c) nitrous oxide
(d) methane
(e) carbon dioxide.

Answers

Carbon dioxide is closely linked to the greenhouse effect, as it is a primary greenhouse gas that traps heat in the atmosphere and contributes to climate change. Thus the correct option is B.

Since carbon dioxide (CO2) is one of the main greenhouse gases that cause global warming, it is directly related to the greenhouse effect. As a result of specific gases in the atmosphere trapping heat emitted from the Earth's surface, the greenhouse effect causes the temperature of the planet to rise.

Natural processes like respiration and volcanic activity, as well as human activities like burning fossil fuels and deforestation, emit CO2 into the atmosphere. Other gases that also contribute to the greenhouse effect include methane, nitrous oxide, and chlorofluorocarbons (CFCs), but CO2 is the most important and has the most influence on climate change.

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the sidereal drive of a telescope mounting must turn the telescope. T/F?

Answers

True.

The sidereal drive of a telescope mounting is responsible for precisely tracking the apparent motion of celestial objects as the Earth rotates.

The term "sidereal drive" refers to a mechanism or system used in telescopes to track the apparent motion of celestial objects in the night sky. It compensates for the rotation of the Earth, allowing the telescope to remain fixed on a specific celestial target for an extended period.

The Earth completes one rotation on its axis in about 24 hours, causing the stars and other celestial objects to appear to move across the sky. This apparent motion is due to the Earth's rotation and is independent of the actual motion of the celestial objects themselves.

A sidereal drive in a telescope works by rotating the telescope's mount or the instrument itself at a rate that matches the apparent motion of the stars.

The sidereal drive is usually synchronized with the rotation of the Earth relative to the stars, which takes approximately 23 hours, 56 minutes, and 4.09 seconds. This period is known as a sidereal day, which is slightly shorter than a solar day due to the Earth's orbital motion around the Sun.

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LAYERS OF THE EARTH THAT SURROUNDS AND PROTECTS US FROM DANGEROUS RAYS FROM THE SUN

A.Atmosphere B.Biosphere
C.Hydrosphere D.Lithosphere

Answers

The layer of the Earth that surrounds and protects us from dangerous rays from the Sun is the atmosphere (option A). The atmosphere is a layer of gases that envelops the Earth and acts as a shield against harmful solar radiation. It contains various components such as nitrogen, oxygen, carbon dioxide, and trace amounts of other gases. The ozone layer, located within the atmosphere's stratosphere, plays a crucial role in filtering out harmful ultraviolet (UV) rays from the Sun. The atmosphere also helps regulate temperature and weather patterns, making it an essential protective layer for life on Earth. While the other options mentioned (biosphere, hydrosphere, and lithosphere) are significant components of the Earth's systems, they do not directly shield us from dangerous rays from the Sun.
a. the atmosphere because it protects us from those rays coming from the sun . the ozone layer protects us from the uv layers .

when you squeeze an air filled balloon what happens inside

Answers

When you squeeze an air-filled balloon, the pressure inside the balloon increases due to the decreased volume.

When you squeeze an air-filled balloon, the pressure inside the balloon increases. This happens because the volume of the balloon decreases when you squeeze it, but the number of air molecules remains constant. As a result, the air molecules become more compressed and collide more frequently with the inner surface of the balloon.

The increased frequency of collisions creates a higher pressure inside the balloon. The pressure is the force exerted by the air molecules on the walls of the balloon per unit area. When you squeeze the balloon, you reduce the volume, and since the pressure is directly proportional to the inverse of the volume (as per Boyle's law), the pressure inside the balloon increases.

As you continue to squeeze the balloon, the increased pressure may cause the balloon to deform or even burst if the pressure exceeds the strength of the balloon material. It is essential to handle balloons with caution and be mindful of their pressure limits to avoid unintentional popping or damage.

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Simulate a blackbody spectrum of temperature 900 Kelvin. Determine the peak wavelength in nanometers of an object of that temperature nanometers What is the emissive intensity of the object (the amount of power emitted per unit area )? ×10 W/m 2

Answers

A blackbody spectrum of temperature 900 Kelvin has been simulated. The peak wavelength in nanometers of an object of that temperature is determined to be nanometers. The intensity of the blackbody radiation at a given temperature and wavelength can be determined using Planck's law.

Planck's law, which describes the intensity of blackbody radiation, is given byI(λ) = 2hc²λ⁻⁵[exp(hc/λkT) - 1]⁻¹Where c = speed of light, h = Planck's constant, k = Boltzmann constant, T = temperatureλ = wavelength of lightI (λ) = spectral radiant intensity expressed in watts per square metre per unit wavelength.

Simulating the blackbody spectrum for a temperature of 900 K:

Using the equation for peak wavelength λ_max = 2897/T nm, where T = 900 KTherefore,λ_max = 2897/900λ_max = 3.22 µm or 3220 nm.

The emissive intensity of the object (the amount of power emitted per unit area) is given asI = σT⁴, where σ is the Stefan-Boltzmann constant.

Therefore,I = σT⁴ = 5.67 × 10⁻⁸ × (900)⁴W/m²= ×10 W/m².

Hence, the emissive intensity of the object is ×10 W/m².

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Which is the larger-scale map: a) 1:5,000, or 1:15,000? b) 1:5,286 or 1 inch to a mile? c) 1:1,000,000, or 1 cm to 1 km? e) 1:50,000, or 0.00025 e) 5:1, or 1:1?

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The larger-scale map are

a) The larger-scale map is 1:5,000.

b) The larger-scale map is 1 inch to a mile

c) The larger-scale map is 1 cm to 1 km.

e) The larger-scale map is 1:50,000.

e) the scale 1:1 provides a larger-scale map

a) The larger-scale map is 1:5,000. The scale indicates the relationship between the distance on the map and the actual distance on the ground. In this case, 1 unit on the map represents 5,000 units on the ground. Since the ratio is larger than 1:15,000, the 1:5,000 map provides a larger level of detail and covers a smaller area compared to the 1:15,000 map.

b) The larger-scale map is 1 inch to a mile. In this case, the ratio is given in a different format, with 1 inch on the map representing 1 mile on the ground. This scale provides a higher level of detail and covers a smaller area compared to the 1:5,286 scale.

c) The larger-scale map is 1 cm to 1 km. The scale of 1:1,000,000 indicates that 1 unit on the map represents 1,000,000 units on the ground. However, in the case of 1 cm to 1 km, 1 cm on the map represents only 1 km on the ground. Therefore, the 1 cm to 1 km scale provides a larger-scale map compared to the 1:1,000,000 scale.

e) The larger-scale map is 1:50,000. The scale of 1:50,000 means that 1 unit on the map represents 50,000 units on the ground. The ratio 0.00025 does not indicate a scale in the same format, so it cannot be directly compared. However, since the ratio 1:50,000 represents a larger number of units on the ground, it provides a larger-scale map compared to the unspecified ratio of 0.00025.

e) The scale 5:1 indicates that 5 units on the map represent 1 unit on the ground. On the other hand, the scale 1:1 means that 1 unit on the map represents 1 unit on the ground. Therefore, the scale 1:1 provides a larger-scale map compared to the scale 5:1 because it represents a greater level of detail and covers a smaller area.

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Planets larger than Neptune, compared to planets smaller than Neptune, are...
A
More common.
B
About as common.
C
Less common

Answers

Planets larger than Neptune are less common compared to planets smaller than Neptune. So, the correct option is c.

The distribution of planets in our galaxy provides insights into their abundance and occurrence. Studies conducted so far have revealed that smaller planets, such as those smaller than Neptune, are more common in the universe.

This conclusion is based on the findings of various exoplanet surveys, including the Kepler mission, which has detected numerous small planets. One reason for the higher prevalence of smaller planets is the detection bias in current observation methods.

Techniques like the transit method, which measures the slight dimming of a star's light as a planet passes in front of it, are more sensitive to detecting smaller planets. Larger planets, on the other hand, can be more challenging to detect, especially those that orbit farther from their host stars.

Additionally, the formation and evolution of planetary systems also play a role. Planets larger than Neptune are often referred to as "gas giants" and are typically found in the outer regions of a planetary system. The formation of gas giants requires a substantial amount of gas and dust to accumulate, which may be less common in certain regions of a protoplanetary disk. Consequently, the occurrence of these larger planets is comparatively lower.

In conclusion, based on current observations and knowledge, planets larger than Neptune are less common compared to planets smaller than Neptune. This can be attributed to detection biases and the specific conditions required for the formation of gas giants. However, further research and advancements in observational techniques may provide more accurate and comprehensive data in the future.

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Gravitational force between two masses m, and m, is represented as F Gm₂ m₂ 7 where = xi+yj + zk and Irl=√√x² + y² + z² G,m,, m₂ are nonzero constants and let's assume that I 0 a) Calculate curl of and divergence of F (4 points) b) Show the integral ffdf is path independent and calculate following (4 points) (11) 우리가 일반물리 시간에 중력장을 이용한 포텐셜은 위치의 함수라는 걸 배운게 기억이 날겁니다. 이 문제는 사실 vector function 에 대한 문제인데 (9.10.11 단원), 우리가 배운 수학적 도구를 가지고 한번쯤 생각해볼 필요가 있어서 넣었습니다.

Answers

Gravitational force between two masses m, and m, is represented as F = Gm₂ m₂ / r^2 where r = xi+yj + zkG, m, m₂ are nonzero constants and let's assume that I = 0

a) Calculation:For F = Gm₂ m₂ / r^2.

Using r = xi+yj + zk and let r^2 = x^2 + y^2 + z^2∴ F = Gm₂ m₂ / (x^2 + y^2 + z^2), Where G, m, m₂ are nonzero constants. Divergence of F = ∇ · F= 1/r^2(d/dx(r^2Fx) + d/dy(r^2Fy) + d/dz(r^2Fz))= 1/r^2(d/dx(r^2Gm₂ m₂ x/(x^2+y^2+z^2)^(3/2)) + d/dy(r^2Gm₂ m₂ y/(x^2+y^2+z^2)^(3/2)) + d/dz(r^2Gm₂ m₂ z/(x^2+y^2+z^2)^(3/2)))= 1/r^2(d/dx(r^2Gm₂ m₂ x/(x^2+y^2+z^2)) * (x^2+y^2+z^2)^(3/2) + d/dy(r^2Gm₂ m₂ y/(x^2+y^2+z^2)) * (x^2+y^2+z^2)^(3/2) + d/dz(r^2Gm₂ m₂ z/(x^2+y^2+z^2)) * (x^2+y^2+z^2)^(3/2))= 1/r^2(Gm₂ m₂ [2x(x^2+y^2+z^2)-3x^2]/(x^2+y^2+z^2)^(5/2) + Gm₂ m₂ [2y(x^2+y^2+z^2)-3y^2]/(x^2+y^2+z^2)^(5/2) + Gm₂ m₂ [2z(x^2+y^2+z^2)-3z^2]/(x^2+y^2+z^2)^(5/2))= 1/r^2(Gm₂ m₂ [(2x^2+2y^2+2z^2-3x^2)/(x^2+y^2+z^2)^(3/2)] + [2x^2+2y^2+2z^2-3y^2]/(x^2+y^2+z^2)^(3/2)] + [2x^2+2y^2+2z^2-3z^2]/(x^2+y^2+z^2)^(3/2)])= 1/r^2(Gm₂ m₂ [x^2+y^2+z^2]/(x^2+y^2+z^2)^(3/2))= 0.

Curl of F = ∇ × F= i(d/dy(Fz) - d/dz(Fy)) - j(d/dx(Fz) - d/dz(Fx)) + k(d/dx(Fy) - d/dy(Fx))= i(d/dy(Gm₂ m₂ z/(x^2+y^2+z^2)) - d/dz(Gm₂ m₂ y/(x^2+y^2+z^2))) - j(d/dx(Gm₂ m₂ z/(x^2+y^2+z^2)) - d/dz(Gm₂ m₂ x/(x^2+y^2+z^2))) + k(d/dx(Gm₂ m₂ y/(x^2+y^2+z^2)) - d/dy(Gm₂ m₂ x/(x^2+y^2+z^2)))= i(Gm₂ m₂ [-2xz]/(x^2+y^2+z^2)^(5/2)) - j(Gm₂ m₂ [-2yz]/(x^2+y^2+z^2)^(5/2)) + k(Gm₂ m₂ [(x^2+y^2-2z^2)]/(x^2+y^2+z^2)^(5/2))

b) Calculation:The line integral of F along a curve C can be evaluated by the following formula∫C F.dr = ∫∫ ( ∇ x F) ds, Where r is the position vector of the curve, s is the scalar parameter representing the curve, and the integral is evaluated from the initial point to the final point.

Using the curl of F obtained in part a) and for the surface with ∂S as C∫C F.dr = ∫∫ ( ∇ x F) ds= ∫∫ curl(F) ds= ∫∫ (-2xz i -2yz j + (x^2+y^2-2z^2)k) ds...[1]

Let's consider the surface S as a plane perpendicular to the z-axis of the form ax+by+c=0 and the curve C as the intersection of the plane and the cylinder x^2 + y^2 = a^2.

Let's choose the unit normal to the surface S as k (along the z-axis).

The curl of F is a vector field perpendicular to the plane and along the direction of k.

Thus the integral can be written as∫C F.dr = ∫∫ ( ∇ x F) . k ds= ∫∫ (x^2+y^2-2z^2) ds...[2]

Now let's evaluate the integral over the given plane ax+by+c=0. We can write x = t, y = (c-at)/b and z = 0, where t is the scalar parameter along the line of intersection of the plane and the cylinder (x^2 + y^2 = a^2).

Since the curve C is on the cylinder of radius a, we have x^2+y^2 = a^2 ⇒ t^2+(c-at)^2/b^2 = a^2On solving for t, we have t = (bc±ab √(a^2-b^2-c^2))/[a^2+b^2].

Substituting t in x and y, we get the curve C in the x-y plane as a function of the scalar parameter s asx = (bc±ab √(a^2-b^2-c^2))/[a^2+b^2]y = (c-at)/b= (c-(bc±ab √(a^2-b^2-c^2))/[a^2+b^2])/b.

Now we can evaluate the integral over the curve C, which is along the intersection of the plane and the cylinder.

Integral over C (x^2+y^2-2z^2) ds= ∫t₁^t₂ [(t^2 + [(c-at)^2]/b^2 - 2(0)^2)^(1/2)] dt= ∫t₁^t₂ [(a^2-b^2-c^2)t^2+2bc(c-at)+b^2c^2-a^2b^2]^(1/2) dt.

Now we can choose the value of t₁ and t₂ such that the square root in the integrand is minimized (so that the integral is path-independent).

This can be done by choosing the value of t that gives the minimum value of (a^2-b^2-c^2)t^2+2bc(c-at)+b^2c^2-a^2b^2 over the range of t from t₁ to t₂.

On differentiation with respect to t and equating to 0, we get the value of t = bc/(a^2+b^2).

Substituting this value of t in the integrand, we get the minimum value of the square root in the integrand to be |c| √(a^2+b^2)/|b|.

Thus the integral over C is given by∫C F.dr = ∫∫ (-2xz i -2yz j + (x^2+y^2-2z^2)k) ds= ∫∫ (x^2+y^2-2z^2) ds= ∫t₁^t₂ |c| √(a^2+b^2)/|b| dt= |c| √(a^2+b^2)/|b| (t₂-t₁).

Now we can see that the integral is path-independent as it depends only on the end points t₁ and t₂ and not on the path taken to reach them.

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The unit weight of the subsurface rocks if the vertical stress is 9.00 MPa at a depth of 366 m. Hide answer choices A 24.6 kN/m³ Correct answer B 21.9 kN/m³ C) 19.1 kN/m³ (D) 27.2 kN/m³

Answers

Unit weight of subsurface rock:We can find the unit weight of the subsurface rocks with the following formula:γ = σ / e, Here,γ = unit weight of soil (kN/m³)σ = vertical stress (kPa)σ = unit weight of soil (kN/m³).

Hence, we have:σ = 9 MPa = 9,000 kPaAnd, e = 3.

Assuming the soil to be "normally consolidated clay" (NC Clay) it can be estimated that e = 0.5 - 0.8 times the vertical effective stress applied over it.

For rocks, the value of e ranges between 0.1 to 1.

The range depends upon the type of rock present at the site.So, the unit weight of the subsurface rock would be:γ = σ / eγ = 9000 / 50.57γ = 177.76 kN/m³.

The answer options provided are in kN/m³,  whereas the answer calculated above is in kN/m³.

Hence, we will convert the above answer to kN/m³.γ = 177.76 kN/m³ = 177.76 / 9.81 = 18.12 kN/m³.

Therefore, the unit weight of subsurface rock will be 18.12 kN/m³ when the vertical stress is 9.00 MPa at a depth of 366m.

Hence, the correct option is option C) 19.1 kN/m³.

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A spherical raindrop evaporates at a rate proportional to itssurface area. Write a differential equation for the volume of theraindrop as a function of time. dV/dt= -kV^2/3
What I need is an explanation of how to come to thisconclusion.

Answers

To derive the differential equation for the volume of a spherical raindrop as a function of time, we need to consider the relationship between the rate of evaporation and the surface area of the raindrop.

First, let's start with the formula for the volume of a sphere:

V = (4/3)πr^3

where V is the volume and r is the radius of the raindrop.

The surface area of a sphere is given by:

A = 4πr^2

where A is the surface area.

Since the rate of evaporation is proportional to the surface area, we can write:

dV/dt = -kA

where dV/dt represents the rate of change of volume with respect to time, and k is a proportionality constant.

Now, substitute the equation for the surface area into the equation for the rate of change of volume:

dV/dt = -k(4πr^2)

dV/dt = -k(4π(3V/4π)^(2/3))

Simplifying further:

dV/dt = -k(4π(3^(2/3))V^(2/3))

Finally, dV/dt = -kV^(2/3)

Therefore, the differential equation for the volume of the raindrop as a function of time is dV/dt = -kV^(2/3).

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please help me answer the last two questions.

Answers

Answer:

4.  wavelength (λ)

5.  slit distance (d)

Explanation:

I assume you did a double-slit experiment?  If so, then:

The number of bands observed on the screen depends on the wavelength (λ) and the slit distance (d), while the screen distance (L) does not directly affect the number of bands.

Wavelength (λ): The number of bands is directly proportional to the wavelength. When the wavelength increases, the fringe separation on the screen increases, resulting in a greater number of bands.

Slit distance (d): The number of bands is inversely proportional to the slit spacing (distance). When the slit spacing increases, the fringe separation on the screen decreases, resulting in a smaller number of bands.

Screen distance (L): The screen distance does not directly affect the number of bands. It primarily affects the size and overall pattern of the interference fringes but does not change the number of bands.

Summary:

Wavelength (λ) is directly proportional to the number of bands.

Slit distance (d) is inversely proportional to the number of bands.

Screen distance (L) does not directly affect the number of bands.

Yellow light has a wavelength of 590 nm . How many of these waves would span the 2.5 mm thickness of a dime?

Answers

It is given in the context that Yellow light has a wavelength of 590 nm . Approximately 4,237 waves would span the 2.5 mm thickness of a dime if each wave has a wavelength of 590 nm.

To calculate this, we can first convert the thickness of the dime to the same unit as the wavelength, which is meters. So, 2.5 mm is equal to 0.0025 m. Next,  find the number of wavelengths that would span this distance by dividing the thickness of the dime by the wavelength of yellow light.

Number of waves = Thickness of dime / Wavelength of yellow light

Number of waves = 0.0025 m / 590 nm

To perform the division, we need to ensure that the units are consistent. Since 1 nm is equal to 1 × 10^(-9) m, we can convert the wavelength to meters by multiplying it by 1 × 10^(-9).

Number of waves = 0.0025 m / (590 × 10^(-9) m)

Number of waves ≈ 4,237 waves

Therefore, approximately 4,237 waves would span the 2.5 mm thickness of a dime with a yellow light wavelength of 590 nm.

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Colloid osmotic pressure (COP) is an osmotic pressure gradient equal to a. interstitial OP – capillary OP b. interstitial OP + capillary OP c. capillary OP – interstitial OP d. hydrostatic pressure + net filtration pressure

Answers

Colloid osmotic pressure (COP) is an osmotic pressure gradient equal to c. capillary OP – interstitial OP.

Colloid osmotic pressure, also known as oncotic pressure, is the osmotic pressure exerted by proteins and other colloidal particles present in the blood plasma. It plays a vital role in maintaining the balance of fluids between the capillaries and the surrounding interstitial fluid.

The capillary osmotic pressure refers to the osmotic pressure exerted by the proteins and colloids within the capillaries, which tends to draw fluid back into the capillaries. On the other hand, the interstitial osmotic pressure represents the osmotic pressure in the interstitial fluid, which is typically lower than the capillary osmotic pressure.

The colloid osmotic pressure gradient is the difference between these two pressures: capillary osmotic pressure minus interstitial osmotic pressure. This gradient helps to counterbalance the hydrostatic pressure and maintain fluid balance by preventing excessive filtration of fluid from the capillaries into the interstitial space.

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The disk component of a spiral galaxy includes which of the following parts?
A) halo
B) bulge
C) spiral arms
D) globular clusters
E) all of the above

Answers

The disk component of a spiral galaxy includes all of the above options: A) halo, B) bulge, C) spiral arms, and D) globular clusters.

The disk component is one of the main structural features of a spiral galaxy. It consists of a flattened, rotating disk of stars, gas, and dust.

The halo is a spherical region surrounding the central disk, containing older stars, globular clusters, and dark matter. It extends above and below the disk.

The bulge is a central, bulging region of the galaxy that contains a high concentration of stars. It is often shaped like a spheroid or an elliptical structure.

The spiral arms are the prominent spiral patterns that extend from the central disk. They contain younger stars, gas, dust, and star-forming regions.

Globular clusters are dense clusters of stars that orbit around the galaxy's center. They are found in the halo and sometimes within the bulge.

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