The marine chronometer changed the world by revolutionizing the way people navigated. It allowed ships to accurately measure their longitude, enabling them to determine their exact positions at sea.
This greatly improved the accuracy of navigation and allowed ships to travel farther and more safely. Additionally, the introduction of the marine chronometer allowed for the development of global trade and the exploration of new lands.
The Impact of the Marine Chronometer on Global Exploration and TradeThe marine chronometer was a revolutionary invention that changed the world by revolutionizing the way people navigated. Prior to its introduction, navigation was an imprecise art that relied on guesswork and educated guesses. However, with the invention of the marine chronometer, ships were now able to accurately measure their longitude and determine their exact positions at sea. This greatly improved the accuracy of navigation and allowed ships to travel farther and more safely.
The impact of the marine chronometer can be seen in the development of global trade and the exploration of new lands. By allowing ships to navigate more precisely, the marine chronometer enabled more efficient trade routes and allowed for new areas to be explored. For example, the marine chronometer played a key role in the exploration of the Pacific Ocean and the discovery of Australia and New Zealand. Additionally, the marine chronometer allowed merchants to expand the scope of their trading activities and the reach of their goods.
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a solution that is 1.10% hcl by mass (assume a density of 1.01 g/ml for the solution.)
A solution that is 1.10% hcl by mass means that 1.10 grams of HCl is present in every 100 grams of solution. Molarity of the solution is 0.003M.
A 1.10% solution of HCl by mass means that 1.10 grams of HCl is present in every 100 grams of solution.
The density of the solution is 1.01 g/ml, which means that 1 milliliter of the solution weighs 1.01 grams.
To find the molarity of the solution, you need to know the molar mass of HCl which is 36.46 g/mol.
Molarity (M) = (moles of solute) / (volume of solution in liters)
The number of moles of solute can be found by dividing the mass of the solute (1.10 g) by the molar mass of the solute (36.46 g/mol)
The volume of the solution can be found by converting the mass of the solution (100 g) to volume (100g/1.01g/ml = 99 ml)
So the molarity of the solution is: (1.10 g / 36.46 g/mol) / (99 ml / 1000 ml/L) = 3.03 x 10^-3 M or 0.003M
It is important to note that this is an approximation assuming a density of 1.01 g/ml and that the density of the solution can vary depending on the temperature and pressure. Additionally, the molarity of the solution can change if the volume is changed
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describe how a chain reaction can be set up if the neutrons produced by one fission
strike other U-235 nuclei
Neutrons produced by one fission strike other U-235 nuclei In chain reaction the three neutrons produced by the fission may hit other nuclei of uranium 235 causing the process to repeat.
What is nuclear fission?Nuclear fission can be defined as subdivision of a heavy atomic nucleus such as that of uranium or plutonium into two fragments of roughly equal mass. The process is accompanied by the release of a large amount of energy. In nuclear fission the nucleus of an atom breaks up into two lighter nuclei.
Therefore chain reaction the three neutrons produced by the fission may hit other nuclei of uranium 235 causing the process to repeat.
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What is the instantaneous angular acceleration, in radians per squared second, at time 11.5 s? What is the change in angular velocity, in radians per second, during the time interval from 1.75 s to 5.25 s?
Calculate angular velocity with this angular acceleration calculator. Angular velocity is defined as one revolution (360°) per 10 seconds, or 36° per second.
How can instantaneous velocity be used to calculate angular velocity?
The instantaneous angular velocity, de, is obtained by taking the immediate change in angle, d, and dividing it by the instantaneous change in time, dt. We may calculate the instantaneous angular acceleration d by dividing d by dt. We can state that d = if the angular acceleration is constant.
How is the instantaneous velocity formula created?
Calculus may be used to determine an object's velocity at every point in its journey. The term "instantaneous velocity" refers to the derivative of an object's speed, which is determined by the equation v = (ds)/(dt).
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An ideal gas is placed in an expandable container of volume V at pressure P. If the volume of the container is doubled to 2V at constant temperature, what is the resulting gas pressure
If the volume of the container is doubled to 2V at a constant temperature, then the resulting gas pressure will be halved.
The ideal gas law states that the product of the pressure and volume of an ideal gas is equal to the product of the number of moles of the gas and the ideal gas constant multiplied by the temperature of the gas.
PV=nRT
This means that if the volume of the container is doubled to 2V at a constant temperature, the resulting gas pressure will be halved to P/2.
This is because the number of moles of gas and the temperature remains constant, so the only variable that can change is the pressure, which is inversely proportional to the volume.
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a 3.00 x 10^2 kg piano is being lifted at a steady speed from ground level straight up to an apartment 10.0 m above the ground. the crane that is doing the lifting produces a steady power of 4.00 x 102 w. how much time does it take to lift the piano?
It takes to lift the piano is 73.5 seconds
calculationWorkdone againstgravity W = mass(m) * acceleration due to gravity (g) * height (h)
W = 3* 102 * 9.8 * 10.0
= 2.94* 104 J
Power = work done / time
=> time taken to lift the piano t = W/ P
= 2.94* 104 / 4.00 * 102
= 73.5 s
What exactly is a high-power query?Powerful inquiries are open-ended and provide the respondent the freedom to pick the course they pursue. They open up options and promote research, in-depth comprehension, and fresh perspectives. They want to advance learning and connection, therefore they are perceptive and nonjudgmental.
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What is the index if refraction of glass?
The index of refraction of glass typically ranges from 1.4 to 1.6.
Exploring the Refractive Index of GlassThe refractive index of glass is an important metric used to measure the optical properties of this versatile material. It is used to quantify how much light is bent, or refracted, when it passes through glass, and is a critical factor in determining the quality of glass lenses and other optical components. In this essay, we will explore the refractive index of glass and discuss how it is measured and applied in real-world applications.
The refractive index of glass is usually expressed as a number between 1.4 and 1.6. This number is determined by the ratio of the speed of light in a vacuum to the speed of light in the given material. In the case of glass, the refractive index is generally higher than that of air, meaning that light bends more when it passes through glass than it would if it passed through air.
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Matter from space can response area to form a nebula or matter from a star can response area to form a nebula.
Matter from space can condense to form a nebula or matter from a star can explode to form a nebula.
The nebula is made up of dust and gas, most of which are Helium and Hydrogen gases. Dust and gas in the Nebula spread easily, but due to the gravitational pull, these clumps of dust and gas slowly coalesce. The bigger the lump that is produced, the stronger the gravitational pull.
Finally, the resulting lump of dust and gas becomes very large and explodes under its gravity. The collapse of this gas column causes the substance at the center of the cloud to heat up. Later this hot nebula core will become a new star.
Complete questions:
Matter from space can ____ to form a nebula or matter from a star can____ to form a nebula.
A. warm B. condense c. explode d. coolThe correct choice is B and C
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a frog in a hemispherical pod finds that he just floats without sinking in a fluid of density 1.35 g/cm3. if the pod has a radius of 6.00 cm and negligible mass, what is the mass of the frog?
The information in the question about the frog's mass states that it weighs 354 g.
What is a mass ?The quantity of matter in an object is expressed in terms of mass. Typically, mass is expressed in kilograms (kg) or grams (g) (kg). No matter where in the universe it is or how much gravitational force is exerted on it, mass is a measure of how much matter there is.
Recall that a hemisphere's volume is determined by;
V = 2/3 πr^3
The pod's volume is equal to 2/3 x 22/7 x (5.00) 3.
The pod's volume is 262 cm3.
Remember that the mass is that of the frog because the mass of the pod is minimal.
Since;
Density= mass/volume
mass = Density × volume
Mass = 1.35 g/cm3 × 262 cm^3
Mass = 354 g
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if "fair" weather were approaching, the pressure tendency would probably be ________.
The pressure tendency would likely be growing if "good" weather was on the horizon.
What kind of general weather can be anticipated when the pressure tendency is rising?The forecast calls for fair to good weather when the pressure tendency is rising. It is common to expect stormy or inclement weather while the pressure tendency is declining. Clouds and precipitation are linked to low pressure systems because warm air (which holds a lot of water vapour) rises because it is denser than the air above.
What kinds of wind patterns and climate are related to low pressure systems?High-pressure regions are linked to calmer winds and sunny sky, while low-pressure regions are frequently connected with unfavourable weather (such as gloomy, windy, with potential for rain or storms).
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A galaxy cluster contains between _____ galaxies. 5,000 to 10,000 50 to 1,000 1,000 to 5,000 5 to 50 10,000 to 50,000
A galaxy cluster contains between 50 to 1,000 galaxies.
How far apart are galaxy clusters?A supercluster's galaxy clusters are frequently millions of light years apart from one another, making it difficult to estimate their distance with accuracy. The distance between us and the galaxy clusters in the Hydra Supercluster, which is around 100 million light years long, ranges from 105 to 160 million light years.
In accordance with this theory, groupings of dozens of galaxies are gravitationally drawn together to create galaxy clusters, which then combine to form clusters of hundreds or even thousands of galaxies.
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two objects are separated by a distance of 1.2mm. the objects are initially neutral, and then each receive the same number of electrons, giving them the same charge. the force between the objects is now 24.0 pn. how many electrons did the two objects each receive?
The number of electrons is = =3.875∙〖10〗^5 ,if the objects are initially neutral, and then each receive the same number of electrons, giving them the same charge.
What is electron example?Electrons are the smallest of the particles that make up an atom, and they carry a negative charge. The number of protons and electrons is equal in a neutral atom. The hydrogen atom, for example, has just one electron and one proton.
Where are the electrons?Where Are Electrons Unlike protons and neutrons, which are located inside the nucleus at the center of the atom, electrons are found outside the nucleus. Because opposite electric charges attract each other, negative electrons are attracted to the positive nucleus.
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Visible light from a distant star can be spread into a spectrum by using a glass prism or ______.
A) a diffraction grating.
B) adaptive optics.
C) a telescope.
D) a flat glass mirror.
Option a is Correct. Using a diffraction grating or a glass prism, it is possible to disperse the visible light from a far-off star into a spectrum.
To split polychromatic light into its underlying constituent wavelengths, diffraction gratings are optical components found in equipment like spectrometers. Diffraction gratings are periodic optical components that divide light into several beams that move in diverse directions. It is a different approach to using a prism to study spectra.
Usually, when light strikes the grating, the split light will have a maxima at an angle. The idea of diffraction explains how a diffraction grating can split a beam of different wavelengths into a spectrum of related lines, with only waves of a particular wavelength conserving energy in a given direction while all other waves being destroyed by interference.
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Three boxes, A, B, and C, are placed on a frictionless surface as shown in the diagram below. If you push on box A with a force of 8.25 N, find the contact force (in N) between each pair of boxes. Here mA -5.50 kg, Mg = 4.40 kg, and mc-1.50 kg. contact force between A and B 4.26 contact force between B and C 7.45 - X How much force does box B apply to Box C? N
The contact force (in N) between each pair of boxes is mathematically:
F_{ab} = 3.56 N
F_{bc} = 1.2 N
The net force gives you the system acceleration, and then each box's acceleration gives you the pushing force.
8.25 N = (5.5 + 4.4 + 1.5)kg * a → a = 0.724 m/s²
Therefore the B&C force is
Fab = (1.5 + 4.4)kg * 0.724m/s² = 4.27 N
and
Fbc = 1.5kg * 0.724m/s² = 1.09 N
Five instances of contact force:
Contact force is a force that, when applied to an item, can initiate or modify the motion of the object. For instance, the force exerted by muscles, friction, springs, tension, air resistance, etc.
What do contact force examples mean?(a) A contact force is precisely what it sounds like: it is the force that one body exerts on another when they are in close proximity. For instance, you are exerting a contact force on a box when you pull it off the ground.
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An explanation on how to calculate this would be appreciated
Answer:The initial position of the car was x = -245 + 103 = -142 m.
Explanation:
To solve this problem, you need to reverse the displacement by adding it to the final position. The displacement of -103 m takes the car from its initial position to its final position at x = -245 m, so to find the initial position, you need to reverse this displacement by adding it to the final position. This gives you the initial position of the car, which is x = -245 + 103 = -142 m.
A spherical Christmas tree ornament is 4.00 cm in diameter. What is the magnification of an object placed 7.0 cm away from the ornament
The magnification of an object that placed 7.0 cm away from the ornament with 4.0 cm in diameter is -8.167
How to calculate the magnification?D = diameter = 4 cm
u = object distance = 7 cm
The magnification can be calculated by dividing the scale image by the actual image length. So, we must find the scale image first.
We use a convex mirror formula to determine the scale image. But before that, we change the diameter of the ornament to focal length.
f = D/4 = 1 cm
The scale image is,
1/f = 1/v + 1/u
1/v = 1/f - 1/u
1/v = 1/1 - 1/7
1/v = 7/7 - 1/7
1/v = 6/7
v = 7/6
v = 1.167
Then magnification is,
M = -v/u
= -1.167/7
= -8.167.
Thus, the magnification is -8.167.
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what signs of energy transfer do you see in the photo? how do you think geothermal energy from inside earth is being used to produce electricity?
To create steam, geothermal power plants pump liquids from subsurface reservoirs to the surface. The steam is then used to power electricity-producing turbines.
What is an easy way to define electricity?The movement of electric energy or charge is known as electricity. It's a secondary energy source, meaning that we obtain it through the conversion of main energy sources like coal, nat gas, oil, nuclear power, and other natural sources.
How exactly does electricity function?There are instances when the protons and electrons inside an atom's outer shells are not strongly attracted to one another. It is possible to force these electrons out of normal orbits. They can move through one atom to the other by exerting force. Electricity is made up of these moving electrons.
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in a hydraulic car lift, the input piston has a cross-sectional area 0.0028 square meters and the output piston has a cross-sectional area of 0.0759 square meters. what would be the output force (in newtons) if the input force on the lift is 24,824 newtons?
The cross-sectional areas of the input and output pistons in a hydraulic automobile lift are 0.0028 and 0.0759 square meters, respectively. 1250 N in weight at the output piston
What is the equivalent of a newton?A newton is equal to 100,000 dynes in the centimeter-gram-second (CGS) system or approximately 0.2248 pounds inside the foot-pound-second (English, usually customary) system.
Why are forces measured in Newtons?The letter N, which stands for "Newtons," is the unit of force measurement most frequently used. It bears Isaac Newton's name, as you probably have guessed. A force of 1 Newton is needed to accelerate a mass of 1 kilogram (kg) by 1 meter per second squared.
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An electric fan is turned off, and its angular velocity decreases uniformly from 600 rev/min to 200 rev/min in 4. 00 s. Find the angular acceleration of electric fan in 4. 00 minutes.
When an electric fan is switched off, its angular velocity uniformly drops. angular acceleration of an electric fan in 4.0 minutes is equal to -1.66 rev/s².
What does the term "angular acceleration" mean?Angular acceleration is the term used to describe the temporal pace at which rotational inertia varies. 360 ° per moment per second is the unit of measurement that is typically used. Consequently, = d d t. Angular acceleration is also known as rotating acceleration.
Is there a constant rate of angular acceleration?Researchers are aware that it's because vertical velocity increases linearly with time, it is possible that an object's acceleration is constant and separate of the time variable. The angular acceleration is shown by the degree of the centripetal velocity vs. time graph.
ω1 = 600rev/min
= 600×(2π/60) rad/s
= 62.8rad/s
ω2 = 200rev/min
=200×(2π/60) rad/s
= 20.9rad
t=4 s
angular acceleration α = ?rev/s²
ω2 = ω1+αt
= (ω_2-ω_1)/t
ω_1 = 600rev/min
=(600/60) rev/s
=10rev/s
ω_2 = 200rev/min
=(200/60) rev/s
=3.33rev/s
α = (3.33-10)/4
α = -1.66rev/s²
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The angular acceleration of the electric fan is
−125/2 π rad/min ^2 in 4.00 minutes.
Angular acceleration(α)=Δω/ Δt
Δω is the change in angular velocity, and
Δt is the change in time.
ωi =600rev/min×2π rad/1 rev × 1 min/60s = 20π rad/s
ωf =200rev/min×2π rad/1 rev × 1 min/60s = 10/3π rad/s
Δω=ωf−ωi = 10/3π rad/s −20πrad/s = −50/3π rad/s
Δt=4.00s × 1 min/60s = 2/15 min
α = Δω/Δt = − 50/3π rad/s / 2/15 min = − 125/2π rad/min^2
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You (weighing 871 N) run up the stairs to class. If your power output was 3,087 watts, what was your velocity?
The force acting here is 871 N. And the time take for displacement is 3.54 seconds. The Then the velocity is 34 m/s against the acceleration due to gravity.
What is velocity?Velocity is the measure of distance covered within the unit time. The force according to second law of motion is the product of mass and acceleration. Where acceleration is the rate of change in velocity.
Power = force × time
thus, time of run = power/ force
= 3087 / 871 N = 3.4 s
The force acting here is the normal force by its own weight , so that the acceleration is 9.8 m/s².
Then velocity = 9.8 m/s² × 3.4 s = 34 m/s.
Therefore, the velocity of the running person is 34 m/s.
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A 2,400-kilogram car is traveling at a speed of 20. meters per second. compared to the magnitude of the force required to stop the car in 12 seconds, the magnitude of the force required to stop the car in 6.0 seconds is
In order to bring down that car in 6.0 seconds, twice as much force is needed.
What in science is a force?The definition of the word "force" is obvious. It is quite acceptable to refer to a force of this level as a push or a pull. Strength is not something that something "is in there" or that something "contains." A force is applied to one thing by another. The idea of a force encompasses both living & non-living things.
Does power involve use of force?Energy is an operation on something other than a body, whereas power is the interaction of two bodies. The main difference between the two ideas is this. Power, on the other hand, is the amount of energy needed when an activity is carried out over the body.
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How do scientists know how old the solar system is ?
Scientists have established that the Solar System is 4.6 billion years old by examining a variety of items, primarily meteorites, and using radioactive dating methods, particularly by examining daughter isotopes.
How did the scientist establish the solar system's age?Plate tectonics has destroyed the oldest rocks on Earth, thus we must rely on meteorites to determine the age of the solar system. The oldest of these meteorites that we have discovered point to a solar system that is 4.568 billion years old, which is also the age of their origin.
The universe is 13.8 billion years old, but how can we know this?Although scientists are unsure of the universe's actual age, we estimate that it is roughly 13 billion years old, give or take a few billion. Two methods are used by astronomers to determine the age of the universe: (a) searching for the oldest stars, and (b) measuring the rate of expansion.
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By investigating a number of objects, principally meteorites, and using radioactive dating techniques, by looking at daughter isotopes, scientists have determined that the Solar System is 4.6 billion years old.
Because the oldest rocks on Earth have been destroyed by plate tectonics, scientists must rely on meteorites to estimate the age of the solar system. The oldest of these meteorites that we have found indicate a solar system that is 4.568 billion years old, which is also the age of their genesis. Although scientists are unaware of the universe's exact age, we calculate mass of that it is around 13 billion years old, give or take a few billion. Astronomers employ two techniques to establish the age of the cosmos.
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For each of the distances marked on the ruler below give the measurement in centimeters and millimeters
One centimeter is divided into 10 equally spaced portions that are designated by tiny lines on the ruler, which you can see if you look at it. A millimeter is represented by each line.
What is distance ?Distance is a measurement of how far apart two things or points are, either numerically or occasionally qualitatively. Distance can refer to a physical length in physics or to an estimate based on other factors in common usage.
Distance is the length of an object's real route in its entirety. The displacement of an object between two points is defined as the straight line (shortest) distance between those two points when directed from one position to another. The metre is the SI unit for measuring distance and displacement (m).
Thus, One centimeter is divided into 10 equally spaced portions that are designated by tiny lines on the ruler, which you can see if you look at it. A millimeter is represented by each line.
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An electron moves along the trajectory from i to f as shown.
a) is the electron's speed at f greater than, less than, or equal to its speed at i? Explain
a)U=kq1q2/r^2
As the potential energy is inversely proportional to r, since both the charges have different polarity so the potential energy will increase as the distance between the charges increases.
b)Electron speed will be less than since the charges will slow down as they move apart because of their different polarity.
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Differentiating between Serpentinite and Chlorite Schist The difference between serpentinite and chlorite schist is that View Available Hints) chlorite schist effervesces with application of dilute HCl, whereas serpentinite does not chlorite schist can be scratched by a fingernail, but serpentinite cannot chlorite schistis foliated, whereas serpentinite is unfoliated serpentinite effervesces with application of dilute HCI, whereas chlorite schist does not the layers of serpentinite are more flat than the layers of chlorite schist, which are noticeably wavy the layers of chlorite schist are more flat than the layers of serpentinite, which are noticeably wavy serpentinite is foliated, whereas chlorite schist is unfoliated. serpentinite can be scratched by a fingernail, but chlorite schist cannot
Foliated HCI, chlorine schost. Schist formed of serpentinite is not foliated. Chlorine schist developed from the foliation of pellitic rocks that underwent greenschist metamorphic rocks.
Where in the body can you find HCl?Mammals create hydrochloric acid (HCl), a naturally occurring acid, in their stomachs to help in digestion. It is present in human gastric juice, often known as gastric acid, where it aids in the digestion of food. However, industrial production of HCl also involves combining water with gaseous hydrogen chlorine.
How does one get HCl into their system?The parietal cells of the stomach create HCl. In the beginning, carbonic anhydrase catalyzes the reaction of oxygen (H2O) and carbon dioxide (CO2) within the cytoplasm of the parietal cell to form carbonic acid (H2CO3).
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at the university of florida, we can remember the spectral type of the sun by thinking the sun is
The surface temperature of our Sun, a class G star, is 5800 K. Since it is hotter than a type M star, we can infer that it is cooler than a type O star. Williamina Fleming developed a system to categorize stars in the 1880s based on the potency of hydrogen absorption lines.
The stars with the strongest hydrogen lines were designated as "A" stars, followed by "B" stars with the second-strongest hydrogen lines, and so on until "O" stars with the weakest hydrogen lines.
However, as we saw above, hydrogen lines by themselves are not a very reliable indicator for classifying stars since they vanish from the visible light spectrum when stars get too hot or too cool.
A, B, F, G, K, M, and O were the only letters from the old system that Annie Jump Cannon focused on when she redesigned this classification system in the 1890s.
Instead of beginning over, Cannon also rearranged the existing classes into the order we are familiar with: O, B, A, F, G, K, M, in decreasing order of temperature.
In her lifetime, she classified over 500,000 stars, classifying up to three stars each minute by examining the stellar spectra, as you can read in the piece on Annie Cannon: Classifier of the Stars later in this section.
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Our Sun is a class G star with a surface temperature of 5800 K. We may conclude that it is colder than a type O star since it is hotter than a type M star.
In the 1880s, Williamina Fleming created a classification system for stars based on the strength of hydrogen absorption lines.
The stars were categorized as "A" stars, "B" stars with the second-strongest hydrogen lines, "C" stars with the strongest hydrogen lines, and so on until "O" stars with the weakest hydrogen lines.
Since they disappear from the visible light spectrum when stars get too hot or too cold, hydrogen lines by themselves are not a particularly accurate signal for categorizing stars, as we have shown above.
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How many light years in diameter have scientists estimated that our milky way galaxy is?
Milky way galaxy is about 100,000 light-years in diameter.
Milky way galaxy is the galaxy where our solar system is included is formed approximately 14 billion years ago. It got the name because of its appearance while viewed from Earth.
Ancient astronomers believed that all stars and planets of the universe is in milky way galaxy.
The number of stars in milky way galaxy is estimated at around 100-400 billion in number.
Sagittarius A is the blackhole that situated in the centre of Milky way galaxy.
It is approximated that Milky way galaxy moves at a velocity of 600 km/s and it is expanding at a rate of 500 m/s.
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The pressure of a gas is reduced from 1200. 0 mmhg to 850. 0 mmhg as the volume of its container is increased by moving a piston from 85. 0 ml to 350. 0 ml. What would the final temperature be if the original temperature was 90 deg celcius?.
The final temperature would be 46.9 deg Celsius
To determine the final temperature of the gas after the pressure has been reduced, we can use the ideal gas law:
PV = nRT
Where P is the pressure, V is the volume, n is the number of moles of gas, R is the universal gas constant, and T is the temperature.
Since the number of moles of gas and the universal gas constant are constants, we can rearrange the equation to solve for temperature:
T = (PV)/(nR)
We know the initial pressure, volume, and temperature of the gas, so we can plug in these values to solve for the final temperature:
Tfinal = (850.0 mmhg * 350.0 ml)/(nR)
To solve for the final temperature, we need to know the value of nR. We can use the initial pressure, volume, and temperature to calculate this value:
nR = (1200.0 mmhg * 85.0 ml)/(90 deg C)
Plugging this value into the equation for Tfinal, we get:
Tfinal = (850.0 mmhg * 350.0 ml)/((1200.0 mmhg * 85.0 ml)/(90 deg C))
Solving this equation, we find that the final temperature of the gas is approximately 46.9 degrees Celsius.
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what is the displacement of the elevator between 8-20 seconds
This is an application of Newton's second law to the forces felt in an elevator.
What law of motion is an elevator?
The use of elevators in public places is a sample of rectilinear motion. If you are accelerating uphill you feel heavier, and if you are accelerating downward you feel lighter. In free fall mode, the elevator's acceleration is the same as the acceleration due to gravity. The enormity of the acceleration due to gravity is 9,8 m/s2,
Since your true weight remains the same, the net force appears because the elevator exerts a smaller normal force on you which is complemented by Newton's Third Law by an equal force downwards on the elevator
So we can conclude that an elevator going up shows constant linear motion, as the elevator will move in a linear line with a constant speed.
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What do I have to answer guys? I really didn’t get this theme so I would be grateful for explanation or answer
The complete equations are:
Charge flows Q = electric current (I) x (t) time.The potential difference V = I current x R resistance.Resistance R = V potential difference / I current.What is the potential difference?The difference that might exist between any two points. The amount of work required to move a unit positive charge along any path from one point to another without accelerating is referred to as the electric field.
The external effort required to move a charge in an electric field from one position to another is known as an electric potential difference or voltage.
Therefore, the formula are:
Charge flows Q = electric current (I) x (t) time.The potential difference V = I current x R resistance.Resistance R = V potential difference / I current.To learn more about potential differences, refer to the link:
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Combustion reactions take place between a fuel and oxygen and produce carbon dioxide and water. Balance the following combustion reaction.
The balanced reaction of combustion of a fuel is 6H2O + 4CO2 = 2C2H6 + 7O2 which produces oxygen.
Combustion is a chemical reaction during which a fuel is oxidized and a large quantity of energy is released. The oxidizer is often air. Fuel: any material that can be burned to release thermal energy. Most familiar fuels are hydrocarbons and are denoted by the general formula of CnHm. For example octane is C8H18.
A combustion process is complete if all the carbon in the fuel burns to CO2, all the hydrogen burns to H2O, and all the sulfur (if any) burns to SO2. That is, all the combustible components of a fuel are burned to completion during a complete combustion process.
In actual combustion processes, it is common practice to use more air than the stoichiometric amount to increase the chances of complete combustion or to control the temperature of the combustion chamber. The amount of air in excess of the stoichiometric amount is called excess air.
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Balanced reaction of combustion of a energy is 6H2O 4CO2 = 2C2H6 7O2 which produces oxygen.
Combustion can be defined as a chemical response in which which a energy is oxidized and a large volume of energy is released. The oxidizer is frequently air. Energy any material that can be burned to release thermal energy. utmost familiar energies are hydrocarbons and are denoted by the general formula of CnHm. For illustration octane is C8H18.
A combustion process is complete if all the carbon in the energy burns to CO2, all the hydrogen burns to H2O, and all the sulfur( if any) burns to SO2. That is, all the combustive factors of a energy are burned to completion during a complete combustion process.
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