Answer:
i actually giggled at that oml.
Explanation:
that was good
A slingshot sends a stone vertically upward from a height of 20 feet above a pool of
water. The starting speed of the stone is 90 feet per second. Its distance in feet, d.
above the water is given by the equation:
d-20+90t-16t^2, where t is the time in seconds after the launch.
Drag statements to the table to show what each coordinate labeled on the graph
represents in this problem situation.
the height of the stone when it is launched
the time when the stone hits the water
the time when the stone is launched the maximum height of the stone
the time when the stone reaches its maximum height
Coordinate
A
the height of the stone when it hits the water
What the Coordinate Represents
DRAG AND DROP
AN ITEM HERE
DRAG AND DROP
AN ITEM HERE
DRAG AND DROP
DRAG AND DROP
Coordinate , A - the height of the stone when it hits the water. A slingshot sends a stone vertically upward from a height of 20 feet above a pool of water.
What the Coordinate Represents?The coordinate A represents the height of the stone when it hits the water. When the stone hits the water, its height above the water surface is zero.
So, we can set the expression for the stone's height equal to zero and solve for t to find the time when the stone hits the water. The height of the stone when it is launched is given as 20 feet, which is a fixed value in this problem.
The time when the stone is launched is also a fixed value, which is zero. The maximum height of the stone is the highest point the stone reaches above its initial height of 20 feet. The time when the stone reaches its maximum height is the time at which the vertical velocity of the stone becomes zero.
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A gas is compressed at a constant pressure from a volume of 10 m3 to a volume of 4 m3 , then work done on the system is:
a) nRT ln 1/6
b) nRT In2/5
c) nRT In 5/2
d) nRT In 6
None of the answer options provided are correct as they all involve calculations that assume certain values for the pressure, volume, and temperature of the gas.
What is Constant Pressure?
Constant pressure is a thermodynamic process in which the pressure of a system remains constant during the process. This means that any change in volume or temperature of the system must be accompanied by a corresponding change in some other property, such as the amount of heat added or removed from the system.
Since the gas is compressed at a constant pressure, the work done on the system can be calculated as:
W = -PΔV
In this case, P is constant, so we have:
W = -P(V2 - V1)
W = -P(4 m^3 - 10 m^3)
W = -P(-6 m^3)
W = 6P m^3
Since we are not given any information about the type of gas or its properties, we cannot use the ideal gas law to calculate the pressure P. Therefore, we cannot determine the exact value of the work done on the system.
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please help!!
If an object were in motion, how might you use a magnet to change the direction of its motion? Diagram the setup and explain your reasoning.
If the object in motion has some magnetic properties or contains a magnet, we can use another magnet to change its direction of motion by exerting a force on it through magnetic interaction. This principle is known as the Lorentz force.
Here's how we can set up the experiment:
Take a magnet and place it on a flat surface.
Take another magnet or the object with magnetic properties that is in motion.
Hold the magnet or the object in your hand and bring it close to the stationary magnet without touching it.
Move the magnet or the object towards the stationary magnet and observe its behavior.
If the magnet or the object has the same polarity as the stationary magnet, they will repel each other, and the motion of the object will be deflected in a direction away from the stationary magnet. If the magnet or the object has opposite polarity to the stationary magnet, they will attract each other, and the motion of the object will be deflected in a direction towards the stationary magnet.
Here's a diagram to help you visualize the setup:
N S N S
__________ __________
| | | |
| M1 | | M2 |
|__________| |__________|
( ) ( )
| |
Motion Stationary
Object Magnet
In this diagram, M1 represents the motion object or magnet, and M2 represents the stationary magnet. The N and S represent the North and South poles of the magnets. The arrows indicate the direction of motion and the direction of the magnetic field.
As we move M1 towards M2, the magnetic interaction will exert a force on M1, causing it to change its direction of motion. The direction of deflection will depend on the polarity of the magnets.
Note: It's important to keep in mind that the magnetic force is only one of the many factors that can affect the motion of an object. Other factors such as friction, air resistance, and gravitational forces can also play a significant role.
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A ball is attached to the end of a string it swung at a vertical circle of three of 0.33M what is the minimum velocity that the ball must have to make it around the circle
Answer:
To make it around the circle, the tension in the string must provide the necessary centripetal force to keep the ball moving in a circle. At the top of the circle, the tension in the string must provide all the force to keep the ball moving in a circle. At the bottom of the circle, the tension in the string must provide the centripetal force in addition to the force of gravity.
We can use the centripetal force formula to solve for the minimum velocity: F_c = m * a_c
where F_c is the centripetal force, m is the mass of the ball, and a_c is the centripetal acceleration.
At the top of the circle, the centripetal force is equal to the tension in the string: F_c = T
where T is the tension in the string.
At the bottom of the circle, the centripetal force is equal to the sum of the tension in the string and the force of gravity:
F_c = T + mg
where m is the mass of the ball, g is the acceleration due to gravity (9.8 m/s^2), and T is the tension in the string.
The centripetal acceleration is given by: a_c = v^2 / r
where v is the velocity of the ball and r is the radius of the circle.
Since the circle has a radius of 0.33 m, we can substitute this into the equation for a_c: a_c = v^2 / 0.33
Combining these equations, we get:
At the top of the circle: T = m * v^2 / 0.33
At the bottom of the circle: T + mg = m * v^2 / 0.33
We can solve for the minimum velocity by using these two equations to eliminate the tension in the string: m * v^2 / 0.33 + mg = m * v^2 / 0.33
Simplifying this equation, we get: v = sqrt(0.33 * g)
Plugging in the values, we get: v = sqrt(0.33 * 9.8) = 1.81 m/s
Therefore, the minimum velocity that the ball must have to make it around the circle is 1.81 m/s
The scale on the horizontal axis is 9 s per division and on the vertical axis 9 m per division
What is the time represented by the third tic mark on the horizontal axis
Answer in units of s
Each tic mark indicates a time period of 9 seconds if the scale on the horizontal axis has a division of 9 seconds. As a result, the third tic point on the horizontal axis would denote the following period of time:
3 x 9 s = 27 s
Hence, 27 seconds are indicated by the third tic point on the horizontal axis.
It is true! The third tic point would represent three times nine seconds, or 27 seconds, as each tic mark on the horizontal axis denotes a time interval of nine seconds.Each tic mark indicates a time period of 9 seconds if the scale on the horizontal axis has a division of 9 seconds. As a result, the third tic point on the horizontal axis would denote the following period of time:Hence, 27 seconds are indicated by the third tic point on the horizontal axis.
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Discuss three applications of the effects of surface tension.
How does a nuclear power plant produce electricity?
Responses
Quickly moving neutrons coming out of the reaction create a gas which turns a turbine that produces electricity.
Quickly moving neutrons coming out of the reaction create a gas which turns a turbine that produces electricity.
Quickly moving neutrons coming out of the reaction are slowed down by water. The water heats up and turns into steam. The steam turns the turbine and produces electricity.
Quickly moving neutrons coming out of the reaction are slowed down by water. The water heats up and turns into steam. The steam turns the turbine and produces electricity.
Quickly moving neutrons coming out of nuclear reactions are used to turn turbines that produce electricity.
Quickly moving neutrons coming out of nuclear reactions are used to turn turbines that produce electricity.
Quickly moving neutrons give their kinetic energy to the surrounding water. The water's energy is then used to turn turbines and produce electricity.
Water slows down neutrons that are leaving nuclear processes quickly. As the water warms up, steam is produced. Electricity is generated by the turbine that the steam turns.
Nuclear power plantA facility that uses nuclear reactions to produce electricity is known as a nuclear power plant. Nuclear fission—the splitting of an atom's nucleus—is used in these reactions to release a significant quantity of energy.Nuclear fission is started at a nuclear power plant's reactor core by blasting the fuel, which is typically uranium-235 or plutonium-239, with neutrons. The heat produced by the fuel's fission is utilized to boil water into steam. To generate electricity, the steam powers a turbine, which in turn powers a generator.The reactor core is encased in a substantial, protective vessel known as the reactor vessel in order to prevent the uncontrolled emission of radioactive particles.learn more about electricity here
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Consider the spectra of the two main sequence stars below (Star 1 on the left and Star 2 on the right) and sort the statements into the true or false bins. The intensity axes are not necessarily on the same scale. 350 450 550 Wavelength (nm) 350 45Q750 650 750 Wavelength (nm) true false Star 1 has a longer lifetime than Star 2 Star 2 is bluer than Star 1 Star 2 has a lower mass than Star 1 Star 1 has prominent hydrogen lines Star 2 has a higher luminosity than Star 1 Star 2 is cooler than Star 1.
. Additionally, Star 1 has prominent hydrogen lines, indicating a lower temperature than Star 2. Therefore, the statements can be sorted into the true and false bins as indicated above.
True: Star 1 has a longer lifetime than Star 2; Star 2 is bluer than Star 1; Star 2 has a lower mass than Star 1; Star 1 has prominent hydrogen lines.
False: Star 2 has a higher luminosity than Star 1; Star 2 is cooler than Star 1.
The spectra of the two main sequence stars illustrate some differences between the two stars. Star 1 is on the left and has a longer lifetime than Star 2, which is on the right. This is evident from the intensity axes that are not on the same scale. Star 2 has a lower mass than Star 1, is bluer than Star 1, and has a lower luminosity
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in the heliocentric model of the solar system, one planet passing another in its orbit gives rise to ...
In the heliocentric model of the solar system, one planet passing another in its orbit gives rise to gravitational forces.
It can also lead to an alteration in the planets' orbits. This is due to the gravitational forces produced by the interaction between the planets. A heliocentric model is a model of the solar system in which the sun is at the center and the planets orbit it. This model was first proposed by Nicolaus Copernicus, a Polish astronomer in the 16th century. He proposed this model after observing that it better explained the motions of the planets than the previous geocentric model, in which Earth was at the center and everything else revolved around it. An orbit gives rise to the gravitational force that causes a planet to continue to travel in a circle around the sun. It is also responsible for the gravitational pull between planets, which affects their orbits. A planet passing another planet in its orbit can also cause some gravitational perturbations in its orbit. This can lead to an alteration in the planets' orbits or cause their orbits to change slightly over time. The heliocentric model is currently the widely accepted theory of how our solar system is arranged. It states that the planets orbit the sun, which is a massive ball of hot gas at the center of the solar system. The sun's gravity is what keeps the planets in their orbits.
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one electron collides elastically with a second electron initially at rest. after the collision, the radii of their trajectories are 0.00 cm and 3.00 cm. the trajectories are perpendicular to a uniform magnetic field of magnitude 0.0350 t. determine the energy (in kev) of the incident electron.
The energy of the incident electron is 26.3 keV. The energy is calculated from the conservation of energy which states that the initial energy is equal to the final energy of the electrons. Total energy is sum of kinetic energy and potential energy of the electrons.
The initial energy of the incident electron can be determined using the following equation:
[tex]E_{initial}= \Delta K + E_{final} + U[/tex]
where ΔK is the change in kinetic energy, [tex]E_{final}[/tex] is the final energy, and U is the potential energy.
Here, the second electron is initially at rest, and after the collision, the trajectories of the two electrons are at 90° to a uniform magnetic field. The magnetic force is perpendicular to the direction of motion, and hence, there is no work done. The potential energy U is, therefore, zero.
Initially, only the incident electron has energy, and hence, its initial energy is equal to its kinetic energy.
[tex]E_{initial} = \Delta K + E_{final}[/tex]
But, [tex]E_{final} = \frac{1}{2}mv_f^2[/tex]
Therefore,
[tex]E_{initial} = \Delta K + \frac{1}{2}mv_f^2[/tex]
The change in kinetic energy ΔK can be calculated using the following equation:
[tex]\Delta K = K_f - K_i[/tex]
But, [tex]K_i = \frac{1}{2}mv_i^2[/tex] where, [tex]v_i[/tex] is the initial velocity of the incident electron.
Therefore,
[tex]\Delta K = K_f - K_i= \frac{1}{2}mv_f^2 - \frac{1}{2}mv_i^2[/tex]
Substituting the given values,
[tex]\Delta K = \frac{1}{2}(9.11 \times 10^{-31} kg)(4.24\times 10^5 m/s)^2 - \frac{1}{2}(9.11\times10^{-31} kg)(3\times10^8 m/s)^2\\= -4.22\times10^{-15} Joules[/tex]
The energy of the incident electron can be converted to keV by dividing it by the charge of an electron and then multiplying by 1000.eV .
Therefore,
[tex]E_{initial} = 4.22 \times 10^{-15} J / (1.602 \times 10^{-19} C/eV)\\ = 26.3 keV[/tex]
Thus, the energy of the incident electron is 26.3 keV.
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charge q1 is distance s from the negative plate of a parallel-plate capacitor. charge is distance 2s from the negative plate. what is the ratio of their potential energies?
The electric potential energy, U, of two point charges is given by the equation, U = kq1q2/r where k is Coulomb's constant, q1 and q2 are the charges and r is the distance between the two charges. Now, let's solve the question using this equation. There are two charges, q1 and q2, and a parallel plate capacitor between them. The distance of q1 from the negative plate is s, and the distance of q2 from the negative plate is 2s. The charges have the same magnitude of charge, so let's assume q1 = q2 = q. Using the formula mentioned earlier, we get U1= kq^2/sU2= kq^2/2s. Therefore, the ratio of their potential energies is U2/U1= kq^2/2s / kq^2/sU2/U1= (kq^2/2s) × (s/kq^2)U2/U1= 1/2.
Therefore, the ratio of their potential energies is 1:2.
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an incompressible substance with a density of 1000 kg/m3 is isothermally compressed from 100 to 1000 kpa. determine the change in enthalpy. multiple choice question. 0 kj/kg 0.9 kj/kg 10 kj/kg 900 kj/kg
The change in enthalpy of an incompressible substance with a density of 1000 kg/m³ that is isothermally compressed from 100 to 1000 kPa is 0 kJ/kg.
What is enthalpy?Enthalpy is a measure of the total energy of a thermodynamic system. In addition, it incorporates the energy that is supplied to the system as heat, as well as any energy that is used as work. Enthalpy is represented by the symbol H and is usually calculated in units of joules (J).
What is an incompressible substance?An incompressible substance is one that cannot be compressed or compressed to a significant degree. Liquids are examples of such materials. They are often described as having a constant density because, unlike gases, they do not easily change in volume in response to pressure or temperature changes. Therefore, the change in enthalpy is 0 kJ/kg.
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what factor does not determine how much gravitational potential energy is in an object-earth system?
The factor that does not determine how much gravitational potential energy is in an object-earth system is the object's mass.
An object-earth system is a system in which an object interacts with the earth by exerting a force of attraction. The object's energy is derived from the work done by gravitational forces when the object is moved away from the earth's surface.
An object in an object-earth system's gravitational potential energy is the work done by gravitational forces on the object when it is moved from a lower position to a higher one in the object-earth system. The factor that does not determine how much gravitational potential energy is in an object-earth system is the object's mass. The gravitational potential energy of an object in the earth-object system is determined by the distance between the object and the earth's surface. The gravitational potential energy of an object increases as the distance between it and the earth's surface increases.
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An electroscope is a device with a metal knob, a metal stem, and freely hanging metal leaves used to detect charges. The diagram below shows a positively charged leaf electroscope.
As a positively charged glass rod is brought near the knob of the electroscope, the separation of the leaves will
remain the same
increase
As a positively charged glass rod is brought near the knob of the electroscope, the separation of the leaves will increase.
What is Charge?
Charge is a fundamental property of matter that determines how objects interact with each other through the electromagnetic force. It is a physical property that can be positive or negative and can be measured in coulombs (C).
This is because the positively charged glass rod will induce a negative charge on the metal knob of the electroscope. The negative charges will repel the electrons in the metal leaves, causing them to move away from each other and increasing their separation. The greater the amount of charge on the glass rod, the greater the separation between the leaves will be.
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1 80 kg scaffold is 5.80 m long. it is hanging with two wires, one from each end. a 580 kg box sits 1 m from the left end. what is the tension in the right hand side wire?
The tension in the right-hand side wire is 6525 N.
Given:
Weight of the scaffold = 180 kgLength of the scaffold = 5.8 mWeight of the box = 580 kgDistance of the box from left end = 1 mLet the tension in the left wire = T1Let the tension in the right wire = T2To find: Tension in the right-hand side wireWe know that the sum of forces acting in a vertical direction should be equal to 0 as there is no acceleration in the vertical direction. ∑Fv = 0In the horizontal direction, there are no forces acting on the system.
∑Fh = 0Now considering forces in the vertical direction: T1 + T2 = (Weight of scaffold + Weight of the box) gT1 + T2 = (180 + 580) x 9.8T1 + T2 = 7644 N1. From the diagram, we can see that the box is nearer to the left side. Hence, the tension force in the left wire is greater than the tension force in the right wire.
T1 > T22. Let's take moments about the right end of the scaffold as shown in the figure below.
∑Mr = 0T1 × 5.8 = T2 × 1T2 = 5.8/1 × T1T2 = 5.8T1Now, we can substitute the value of T2 in equation (1):
T1 + T2 = 7644N6.8 T1 = 7644 N T1 = 1125 NTo find T2, we can substitute the value of T1 in equation (2):
T2 = 5.8 × T1T2 = 5.8 × 1125 N T2 = 6525 NTherefore, the tension in the right-hand side wire is 6525 N.
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suppose your planet at 1 meter from the basketball represents a distance of 4 x 107 km (-0.3 al) from the star. the next closest star to the sun is 4 x 1013 km away. how far away from the model star/planet would you have to be for the distances in the system to be to scale? express your answer in meters and kilometers.
Answer: The model star/planet would have to be 1,000 km away from the next closest star.
Explanation:
We need to find out the distance required for the distances in the system to be in scale.
Let's use the proportion to solve the problem:
1 m/4 × 10⁷ km = x/4 × 10¹³ km
Where x is the distance required for the distances in the system to be in scale.
Cross-multiply: 4 × 10¹³ km × 1 m = 4 × 10⁷ km × x
Simplify: 4 × 10¹³ m = 4 × 10⁷ x
Divide both sides by 4 × 10⁷ :1 × 10⁶ = x
Therefore, the distance required for the distances in the system to be in scale is 1 × 10⁶ m or 1,000 km.
So the model star/planet would have to be 1,000 km away from the next closest star.
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what state of matter is rutherfordium in while at room temperature
Rutherfordium is a synthetic element with the atomic number 104 and symbol Rf. As a synthetic element, it is not found naturally on Earth and is produced through nuclear reactions in laboratories.
Rutherfordium is a member of the transition metals group and is expected to have similar physical and chemical properties to its neighboring elements in the periodic table. However, due to its radioactive nature and short half-life, its physical properties are difficult to determine.
While there is no experimental data available on the state of matter of rutherfordium at room temperature, it is expected to be a solid metal, similar to other transition metals, such as copper or nickel.
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Why are masses listed on the periodic table not whole #'s. Ex. 15.9999 for oxygen?
The masses listed on the periodic table are not whole numbers because they represent the weighted average of all the naturally occurring isotopes of an element.
What are Isotopes ?Isotopes are atoms of the same element that have different numbers of neutrons in their nuclei, resulting in slightly different masses. Since the abundance of each isotope in nature can vary, the weighted average takes into account the abundance of each isotope and their corresponding masses, resulting in a decimal value. For example, oxygen has three naturally occurring isotopes, with mass numbers of 16, 17, and 18.
Why only O-16 isotopes ?The most abundant isotope is oxygen-16, but the other isotopes are also present in trace amounts, leading to a weighted average of 15.9994 amu (atomic mass units). This is why the mass listed on the periodic table for oxygen is 15.999, which is a rounded value of the weighted average.
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The masses listed on the periodic table are not whole numbers because they represent the average atomic mass of all the naturally occurring isotopes of an element, taking into account their relative abundances.
What are isotopes ?
Isotopes are atoms of the same element that have different numbers of neutrons in their nucleus, which affects their atomic mass. Some isotopes of an element are more abundant than others, and their relative abundances are taken into account when calculating the average atomic mass.
For example, oxygen has three naturally occurring isotopes: oxygen-16, oxygen-17, and oxygen-18. Oxygen-16 is the most abundant isotope, making up about 99% of all oxygen atoms. Oxygen-17 and oxygen-18 are much less abundant, but they still contribute to the overall atomic mass of the element.
The atomic mass listed on the periodic table for oxygen (15.9994) is the weighted average of the atomic masses of all three isotopes, taking into account their relative abundances. This average is not a whole number because the isotopes have different atomic masses and abundances, and their contributions to the overall average are weighted accordingly.
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Five docks are being tested in a laboratory. Exactly at noon, as determined by the WWV
Exactly at noon, as determined by the WWV time signal, on successive days of a week the clocks according to their relative value as good timekeepers, best to worst.
Time signals are also used in many everyday applications, such as GPS navigation, where precise timing is essential for calculating positions accurately. A time signal refers to any signal that provides information about the passage of time. Time signals are often used in experiments to measure the duration of events or to synchronize the timing of multiple processes.
One common type of time signal is a periodic signal, which repeats itself at regular intervals. This can be used to measure the period or frequency of a phenomenon, such as the oscillation of a pendulum or the vibration of a guitar string. Another type of time signal is a pulse signal, which provides a brief burst of energy at a specific time. This can be used to trigger the start or stop of a process or to measure the time delay between different events.
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a fixed amount of a molecular substance in the liquid phase is placed in a flask at constant temperature. the flask is closed and is allowed to come to equilibrium. select all the statements that correctly describe the processes occurring in the flask. multiple select question. a. the relative amounts of liquid and vapor in the flask remain constant. b. molecules are leaving and entering the liquid phase at the same rate. c. no changes are occurring because the system is at equilibrium. d. the amount of liquid remains the same because evaporation is no longer occurring.
The statements that correctly describe the processes occurring in the flask are A and B. C and D are incorrect statetment.
a) States that the relative amounts of liquid and vapor in the flask remain constant, which is true as equilibrium has been reached, meaning that the rate of evaporation equals the rate of condensation. b) states that molecules are leaving and entering the liquid phase at the same rate, which is also true as equilibrium has been reached.
c) and d) are incorrect because they do not accurately describe the processes occurring in the flask; while the system is at equilibrium, it is still in a state of change with molecules leaving and entering the liquid phase at the same rate.
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A typical neutron star has a mass of about 1.5Msun and a radius of 10 kilometers Calculate the average density of a neutron star. Express your answer in kilograms per cubic centimeter to two significant figures.
The average density of the neutron star that has a mass of about 1.5Msun and a radius of 10 kilometers rounded off to two significant figures is 5.9 × 10¹⁴ kg/cm³
The average density of a neutron star can be calculated using the following formula;`d = (3M)/(4πr³)`where `d` is the average density of the neutron star, `M` is the mass of the neutron star, and `r` is the radius of the neutron star.Using the given values in the formula, we get;`d = (3 × 1.5 × 1.989 × 10³⁰)/(4π × (10 × 10³)³)` = 5.9 × 10¹⁷ kg/m³To convert kg/m³ to kg/cm³, we can use the following conversion factor;1 m³ = 10⁶ cm³Therefore,1 kg/m³ = 10⁻³ kg/cm³So, the average density of the neutron star in kg/cm³ is;`d = (5.9 × 10¹⁷) × (10⁻³)` = 5.9 × 10¹⁴ kg/cm³Therefore, the average density of the neutron star is 5.9 × 10¹⁴ kg/cm³ (rounded to two significant figures).Answer: 5.9 × 10¹⁴ kg/cm³.
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what's the correct answer.
The coordinated functions of the Nervous, Endocrine, and Reproductive systems are:
D. CerebrumN. Wernicke's AreaF. Occipital LobeH. HypothalamusJ. ThalamusH. HypothalamusC. CerebellumL. Superior ColliculusA. AmygdalaM. Pineal GlandWhat are coordinated functions?Coordinated functions refer to the integration and communication between different organs, systems, and tissues in the body to achieve a common goal or purpose. In biological terms, coordinated functions often involve multiple physiological systems working together to maintain homeostasis, respond to stimuli, or carry out complex behaviors or processes.
Examples of coordinated functions include the regulation of blood glucose levels by the pancreas and liver, the coordination of movement by the nervous and musculoskeletal systems, and the release of hormones by the endocrine system to control various physiological processes.
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The question is:
"COORDINATED FUNCTIONS OF THE NERVOUS, ENDOCRINE, AND REPRODUCTIVE SYSTEMS"
Directions: Identify the part of the brain that is involved in each situation below. Write only the letter of your answer.
A. Amygdala
B. Brocka's Area
C. Cerebellum
D. Cerebrum
E. Hippocampus
F. Occipital Lobe
G. Hippocampus
H. Hypothalamus
I. Inferior Colliculus.
J. Thalamus
K. Pons
L Superior Colliculus
M. Pineal Gland
N. Wernicke's Area
O. Pituitary Gland
1. "My heart tells me that you are the one. I love you so much!"
2. "IAOCEVOY! I don't know what that means. It's all Greek to me!"
3. "Chartreuse, Olive,Turquoise, and Mint are all shades of green."
4. "Janna always wakes up at 4 in the morning, regardless of whether she uses an alarm clock or not."
5. "I don't remember the way going to Myla's house. Can you accompany me there?"
6. Jenny's mother is about to give birth, she complains about contraction and pain usually when the baby is kicking
7. "Anthony is a very skilled dancer. He just won the school hip hop dance competition last week."
8. "As Nica was walking on the road she readily moved to the side for she heard an incoming ambulance"
9. "Elsa loves making faces whenever she talks to her friends."
10. "Ryan usually talks about how happy his high school days were to his grandchildren."
Imagine another solar system, with a star of the same mass as the Sun. Suppose a planet with a mass twice that of Earth (2MEarth) orbits at a distance of 1 AU from the star. What is the orbital period of this planet? Hint: Think about how the mass of the Sun compares with the mass of the Earth. a. 3 months b. 6 months
c. 1 year d. 2 years
e. It would not be able to orbit at this distance.
The correct answer is option D.2 years
What is Kepler's third law of planetary motion?According to Kepler's Third Law of Planetary Motion, T² is proportional to r³, where T is the period of revolution of the planet and r is the distance between the planet and the star.
In order to solve for T,
AU = 1
Astronomical Unit = the average distance between the Earth and the Sun = 149.6 million kilometres
Therefore, the planet is orbiting at a distance of 149.6 million kilometres from the star.
Substituting the values of r and solving for
T².T² ∝ r³T² ∝ (149.6)³T²
= (149.6)³T²
= 3.522 x 10¹²T
= √3.522 x 10^¹²T
= 1.87 x 10⁶ seconds
T = 31,100 minutes
T = 518 hours
T = 21.6 days
T = 2 years
Therefore, the orbital period of the planet with twice the mass of Earth orbiting at a distance of 1 AU from a star with the same mass as the Sun is 2 years.
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when one stationary object is replaced by another stationary object, the change between the two objects maybe perceived as the movement of a single object. this creates?
When one stationary object is replaced by another stationary object, the change between the two objects maybe perceived as the movement of a single object. This creates an optical illusion.
An optical illusion is defined as a visual phenomenon in which the information gathered by the eye is processed in a way that results in a false perception of reality or the visual impression of seeing something that is not present or incorrectly perceiving it. It is a misinterpretation of a visual stimulus caused by the brain's ability to misjudge sensory information.
It can happen when visual information is processed in the brain, and it can create an impression of movement that isn't there. This phenomenon occurs when an object is moving or when the eyes are moving around, but it can also happen when the object being looked at is stationary.
When one stationary object is replaced by another stationary object, the change between the two objects maybe perceived as the movement of a single object. This creates an optical illusion because the visual system is misled into thinking that the object is moving.
The brain continues to process visual information even when the object is stationary, creating the impression that the object is moving. This is why an optical illusion can be used to make a stationary object appear to move or to make a moving object appear to be stationary.
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as noted in this chapter, plants help to reduce water runoff and soil erosion, both of which affect the health of streams and rivers by impacting water quality. soil erosion increases the silt load in water and this literally smothers living organisms, particularly plants and invertebrate species. runoff water can carry pollutants, particularly pesticides and herbicides from agricultural land. read the description of each landscape and rank them from best stream quality to worst stream quality. 1: streams cutting through small farms with several different crop types and natural vegetation buffers between the fields and the streams. 2: a large floodplain area covered with lowland forests and swamps full of emergent vegetation, with small streams cutting through the area. 3: an urban housing development where the trees growing along the streams were removed and replaced with lawns. 4: a system of large farms with no buffer vegetation between the fields and the streams that cut through the farms. question list (4 items) (drag and drop into the appropriate area) landscape 1 landscape 2 landscape 3 landscape 4 correct answer list best stream quality
Plants help to reduce water runoff and soil erosion, both of which affect the health of streams and rivers by impacting water quality.
Soil erosion increases the silt load in the water, which can smother living organisms, particularly plants and invertebrate species. Runoff water can carry pollutants, particularly pesticides, and herbicides from agricultural land.
Landscape 1 (streams cutting through small farms with a variety of crop types and natural vegetation buffers between the fields and the streams) would be the best quality, followed by Landscape 2 (a large floodplain area covered in lowland forests and swamps full of emergent vegetation, with small streams cutting through the area) and Landscape 3 (an urban housing development where the streams are surrounded by emergent vegetation).
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A car’s cooling system contains 25 kg of water. What is the increased change in temperature of the water if 872. 0 kJ of thermal energy is added?
When 872.0 kJ of thermal energy are injected, the temperature of the 25 kg of water in the car's cooling system changes by 35.0 degrees Celsius.
Water's specific heat capacity (J/(gK), or 4,180 J/ (kgK). Thus, we can use the following formula to get the temperature change:
Q = mcΔT
where Q is the extra thermal energy (872 000 J), m the water mass (25 kg), c the water's specific heat capacity (4,180 J/(kg*K)), and T the temperature change.
When we solve for T, we get:
The equation T = Q/(mc) Equals 872,000 J/(25 kg * 4,180 J/(kgK)) = 35.0 °C.
When 872.0 kJ of thermal energy are injected, the temperature of the 25 kg of water in the car's cooling system changes by 35.0 degrees Celsius.
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4. Once the child in the sample problem reaches the bottom of the hill,
she continues sliding along flat; snow-covered ground until she comes
to a stop. If her acceleration during this time is -0.392 m/s², how long
does it take her to travel from the bottom of the hill to her stopping
point?
Answer:
8.04 seconds
Explanation:
Assuming that the child starts from rest at the bottom of the hill and travels until she comes to a stop, we can use the following kinematic equation:
v_f^2 = v_i^2 + 2ad
where v_f is the final velocity (which is zero since the child comes to a stop), v_i is the initial velocity (which is the velocity at the bottom of the hill), a is the acceleration (-0.392 m/s²), and d is the distance traveled.
We can solve for d:
d = (v_f^2 - v_i^2) / (2a)
= (0 - v_i^2) / (2-0.392)
= v_i^2 / 0.784
Since the child is sliding along flat snow-covered ground, there is no change in elevation, so we can use the distance traveled from the bottom of the hill to the stopping point as the distance d.
To find the time it takes for the child to travel this distance, we can use the following kinematic equation:
d = v_it + 0.5a*t^2
where t is the time and all other variables are as previously defined.
Substituting the expression for d obtained above, we get:
v_i^2 / 0.784 = v_it + 0.5(-0.392)*t^2
Solving for t, we get:
t = (2 * v_i) / 0.392
We still need to find the value of v_i, the initial velocity of the child at the bottom of the hill. To do so, we can use conservation of energy. The child starts at rest at the top of the hill, so all the initial energy is potential energy. At the bottom of the hill, all the potential energy has been converted to kinetic energy. Assuming no energy is lost to friction, we can equate these two energies:
mgh = 0.5mv_i^2
where m is the mass of the child, g is the acceleration due to gravity (9.8 m/s²), and h is the height of the hill.
Solving for v_i, we get:
v_i = √(2gh)
Substituting this expression for v_i into the expression for t obtained earlier, we get:
t = (2 * √(2gh)) / 0.392
Plugging in the values of g, h, and a, we get:
t = (2 * √(29.820)) / 0.392 = 8.04 seconds
When Joselyn went to the store she bought 2.7kg of salt water taffy. What would Joselyn do to find out how many grams she bought?A. Divide by 1000B. Multiply by 1000C. Divide by 100D. Multiply by 100
At the shop, Joselyn purchased 2700 grammes of salt water taffy.
To convert kilograms (kg) to grams (g), Joselyn would need to multiply the weight in kilograms by 1000. This is because there are 1000 grams in 1 kilogram. Therefore, to find out how many grams of salt water taffy Joselyn bought, she would need to multiply 2.7kg by 1000.
The correct answer is (B) Multiply by 1000.
Multiplying 2.7kg by 1000 gives:
2.7kg x 1000 = 2700g
So Joselyn bought 2700 grams of salt water taffy at the store.
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Need help on my homework! Thanks.
Answer: Noble Gases (Blue)
if the average arterial pressure at your heart is a typical 100 mmhg , what is the average arterial pressure in your hands when they are held at your side? assume your hands are 60 cm below your heart.
The average arterial pressure in your hands when they are held at your side is 47.5 mmHg.
The average arterial pressure in your hands when they are held at your side can be determined using the hydrostatic pressure formula, which is a function of height, gravity, and density. When the hands are held at the side, they are 60 cm below the heart, which means they are at a distance of 0.6 m.
The hydrostatic pressure formula is given by
P = ρgh
Where,
P is the pressure, ρ is the density, g is the acceleration due to gravity, and h is the height. We can assume that the density of blood is constant, and we can take the value of g to be 9.81 m/s², the standard acceleration due to gravity.
Therefore, the pressure at the heart is 100 mmHg, or 100/760 = 0.131 atm. The pressure in the hands can be calculated as follows:
P = ρghP = (1.06 × 10³ kg/m³) × (9.81 m/s²) × (0.6 m)
P = 6.26 × 10³ N/m²
P = 6.26 × 10³ Pa
P = 47.5 mmHg
Therefore, the average arterial pressure in the hands when they are held at the side is 47.5 mmHg.
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