The work done on the spool when it reaches an angular speed of 8.00 rad/s is 4.00 Joules.
To determine the work done on the spool when it reaches an angular speed of 8.00 rad/s, we need to consider the rotational kinetic energy of the spool.
The rotational kinetic energy of an object with a moment of inertia I and angular speed ω is given by the formula:
K_rot = (1/2)Iω²
In this case, the spool is initially at rest and is pulled by the cord with a constant acceleration. We can use the relationship between linear and angular quantities to relate the linear acceleration of the cord to the angular acceleration of the spool.
The linear acceleration of the cord is equal to the radius of the spool multiplied by the angular acceleration of the spool:
a_linear = r * a_angular
where r is the radius of the spool and a_angular is the angular acceleration.
Given that the linear acceleration of the cord is 2.50 m/s² and the radius of the spool is 0.500 m, we can find the angular acceleration:
a_angular = a_linear / r
= 2.50 m/s² / 0.500 m
= 5.00 rad/s²
Next, we need to find the moment of inertia of the spool. For a cylindrical spool, the moment of inertia can be calculated as:
I = (1/2)mr²
where m is the mass of the spool and r is its radius.
Given that the mass of the spool is 1.00 kg and the radius is 0.500 m, we can find the moment of inertia:
I = (1/2)(1.00 kg)(0.500 m)²
= 0.125 kg·m²
Now, we can calculate the final rotational kinetic energy of the spool when it reaches an angular speed of 8.00 rad/s:
K_rot = (1/2)Iω²
= (1/2)(0.125 kg·m²)(8.00 rad/s)²
= 4.00 J
Therefore, the work done on the spool when it reaches an angular speed of 8.00 rad/s is 4.00 Joules.
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Which diagram below shows the earth moon sun system arranged to cause a total solar eclipse
Answer:
its D
Explanation:
It is time when the moon completely covers the sun. So, the diagram that shows the earth moon and sun system arranged to cause a full solar eclipse is in option D.
What is a solar eclipse?A solar eclipse happens when the Moon moves in front of the Sun, blocking the Sun's light entirely or partially from a tiny portion of the Earth.
During the new moon phase of the eclipse season, when the Moon's circular plane is close to the Earth's orbital plane, such an alignment takes place around every six months.
A total eclipse occurs when the Moon completely blocks out the Sun's disk. Only a portion of the Moon is covered by annular and partial eclipses.
In contrast to a total eclipse, which can be seen from any place on Earth's night side, a partial eclipse is only viewable from a fairly tiny portion of the globe.
Therefore, it concludes that option D in the figure shows the cause of the total solar eclipse.
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Two students are studying for a Science Test. On the table, they had a glass of water and identical cell phones. Both of their phones had run out of battery, therefore they were both charging in the same wall outlet. One student’s charging cord was 3ft and the other student’s charging cord was 9ft. which of the phones charged the fastest using Ohm’s Law. Cite evidence to support your theory.
Answer:
The student with the 3ft charger
Explanation:
Because the electricity from the 3ft charger has a shorter distance to mooves than the 9ft one
A girl on a bicycle rides down a hill 500 meters long in 50 seconds. What is the girl’s speed?
Answer:
10m/s
Explanation:
500÷50 gets your answer
This equation goes with which law?
Answer:
I think that's Newton's second law of motion
Explanation:
f = m(v-u)
________
t
since a = (v-u)t
f = ma
a ball is thrown striaght up in the air and then falls back to earth. if the downward fall takes 2.2s, how fast is the ball traveling when it striker the ground
The velocity of the ball when it strikes the ground, given the data is 21.56 m/s
Data obtained from the questionFrom the question given above, the following data were obtained:
Time to reach ground from maximum height (t) = 2.2 sInitial velocity (u) = 0 m/sAcceleration due to gravity (g) = 9.8 m/s²Final velocity (v) =? How to determine the velocity when the ball strikes the groundThe velocity of the ball when it strikes the ground can be obtained as illustrated below:
v = u + gt
v = 0 + (9.8 × 2.2)
v = 0 + 21.56
v = 21.56 m/s
Thus, the velocity of the ball when it strikes the ground is 21.56 m/s
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A 51 cm diameter wheel accelerates uniformly about its center from 150 rpm to 290 rpm in 4.0 s. (A)Determine the radial component of the linear acceleration of a point on the edge of the wheel 1.1 s after it has started accelerating.
Radial component of the linear acceleration = 99.47 m/s^2
Explanations:The diameter of the wheel, d = 51 cm
The radius, r = d/2 = 51/2 = 25.5 cm
r = 25.5/100 = 0.255 m
r = 0.255 m
\(\begin{gathered} N_{i\text{ }}=\text{ 150 rpm} \\ w_i=\text{ 150}\times\frac{2\pi}{60} \\ w_i=\text{ }15.71\text{ rad/s} \end{gathered}\)\(\begin{gathered} N_f=\text{ 290 rpm} \\ w_f=\text{ 290}\times\frac{2\pi}{60} \\ w_f=\text{ }30.37\text{ rad/s} \end{gathered}\)\(\begin{gathered} w_f=w_i+\alpha t \\ 30.37=15.71+4\alpha \\ 4\alpha=30.37-15.71 \\ 4\alpha=\text{ }14.66 \\ \alpha=\frac{14.66}{4} \\ \alpha\text{ = }3.67rad/s^2 \end{gathered}\)At t = 1.1, first calculate the new angular velocity
\(\begin{gathered} w=w_1+\alpha t \\ w\text{ = 15.71+3.67(1.1)} \\ w\text{ = 15.71+}4.04 \\ w\text{ = }19.75\text{ rad/s} \end{gathered}\)The radial component of the linear acceleration is given as:
\(\begin{gathered} a_r=w^2r \\ a_r=19.75^2\times0.255 \\ a_r=\text{ }99.47\text{ m/}s^2 \end{gathered}\)which type of galaxy has a stellar disk, but without gas and dust?
The type of galaxy that has a stellar disk but without gas and dust is an **elliptical galaxy**.
Elliptical galaxies are characterized by their smooth and featureless appearance, lacking the distinct spiral arms seen in disk galaxies like the Milky Way. They are composed mostly of old stars and have little to no ongoing star formation. As a result, they have depleted their interstellar gas and dust reservoirs over time, leaving behind primarily stellar populations. Elliptical galaxies can vary in size from small to massive, and their shape ranges from nearly spherical to elongated ellipsoids. They are commonly found in dense regions of galaxy clusters, where interactions and mergers between galaxies have stripped away their gas and disrupted their original disk structures.
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3. Since Aspeon is not expected togrow, Emily believes that the following equations can be used in the valuation analysis: (1) S=[EBIT−kd(D)](1−ks)
(2) V=S+D
(3) P=(V−D0)/n0
(4) n1=n0−D/P
(5) VL=VU+TD
The equations mentioned by Emily in the valuation analysis for Aspeon are as follows:
1) Equation (1): This equation represents the value of equity (S) and calculates it based on the EBIT (earnings before interest and taxes), the tax shield provided by debt (D), and the required return on debt (kd) and equity (ks). It implies that the value of equity is equal to the adjusted EBIT after deducting the tax shield from debt.
2) Equation (2): This equation calculates the total enterprise value (V) by adding the value of equity (S) and debt (D). It represents the total worth of the company, considering both equity and debt.
3) Equation (3): This equation calculates the price per share (P) by dividing the total enterprise value (V) minus the initial debt (D0) by the number of shares (n0). It represents the price per share based on the valuation of the company.
4) Equation (4): This equation calculates the new number of shares (n1) by subtracting the dividend (D) from the initial number of shares (n0) divided by the price per share (P). It represents the adjusted number of shares after the payment of dividends.
5) Equation (5): This equation calculates the levered value (VL) by adding the unlevered value (VU) with the tax shield value (TD). It represents the value of the company after considering the tax advantages of debt.
These equations provide a framework for valuation analysis, considering factors such as earnings, taxes, debt, and equity. They help assess the value and financial implications of Aspeon's growth prospects.
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is the only planet in the solar system whose axis of rotation lies close to the plane of the solar system.
a. Uranus b, Neptunus c. Pluto
d. Yupiter
Option A i.e. Uranus is the only planet in the solar system whose axis of rotation lies close to the plane of the solar system.
The correct answer is a. Uranus. Uranus is the only planet in the solar system whose axis of rotation is tilted at an angle of almost 98 degrees relative to the plane of the solar system. This means that Uranus essentially rolls around the sun on its side, while the other planets rotate more or less upright. This is in contrast to the other planets in the solar system, whose axes of rotation are more or less perpendicular to the plane of the solar system.
Hence, the correct answer is option A i.e. Uranus.
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A man can jump 1.5 m on earth. calculate the approximate
height he might be
able to jump on
a planet whose
density is one quarter of the earth and where radius
is one third that of earth.
Radius of earth = 6400km
Acc. due to gravity=9.8 m/s²
Mass of earth = 6X10^24 kg
Answer:
18 m
Explanation:
G = Gravitational constant
m = Mass of planet = \(\rho V\)
\(\rho\) = Density of planet
V = Volume of planet assuming it is a sphere = \(\dfrac{4}{3}\pi r^3\)
r = Radius of planet
Acceleration due to gravity on a planet is given by
\(g=\dfrac{Gm}{r^2}\\\Rightarrow g=\dfrac{G\rho V}{r^2}\\\Rightarrow g=\dfrac{G\rho \dfrac{4}{3}\pi r^3}{r^2}\\\Rightarrow g=\dfrac{4G\rho\pi r}{3}\)
So,
\(g\propto \rho r\)
Density of other planet = \(\rho_p=\dfrac{1}{4}\rho_e\)
Radius of other planet = \(r_p=\dfrac{1}{3}r_e\)
\(\dfrac{g_e}{g_p}=\dfrac{\rho_e r_e}{\rho_p r_p}\\\Rightarrow \dfrac{g_e}{g_p}=\dfrac{\rho_e r_e}{\dfrac{1}{4}\rho_e\times \dfrac{1}{3}r_e}\\\Rightarrow \dfrac{g_e}{g_p}=12\\\Rightarrow g_p=\dfrac{g_e}{12}\\\Rightarrow g_p=\dfrac{9.8}{12}\)
Since the person is jumping up the acceleration due to gravity will be negative.
From kinematic equations we have
\(v^2-u^2=2g_es\\\Rightarrow u^2=v^2-2g_es\\\Rightarrow u^2=0-2\times -9.8\times 1.5\\\Rightarrow u^2=2\times 9.8\times 1.5\)
On the other planet
\(v^2-u^2=2g_ps\\\Rightarrow s=\dfrac{v^2-u^2}{2g_p}\\\Rightarrow s=\dfrac{0-(2\times 9.8\times 1.5)}{2\times -\dfrac{9.8}{12}}\\\Rightarrow s=18\ \text{m}\)
The man can jump a height of 18 m on the other planet.
After stellar supernova, one of two things can occur: Neutron star formation, or Black Hole formation. Which property of stars gives a clue as to what will happen?
Answer:
sorry I needed points to ask my question
\(\boxed{\color\red\huge\tt\bold\purple{Question}}\)
Define Inertia.
Answer:
Inertia : a property of matter by which it continue in its existing state of rest or uniform motion in a straight line, unless that state is changed by external force.
HOPE ITS HELPS!!
\(\boxed{\color{red}\huge\tt\bold\purple{Answer}}\)
Inertia is the tendency of an object to continue in the state of rest or of uniform motion. The object resists any change in its state of motion or rest.
A carnot engine has a thermal energy of 0.5. It had a cold temperature reservoir temperature of Tc = 100K. if this engine is run in reverse as a heat pump used for cooling, what is its coefficient of performance, K?
A. 0.5
B. 5
C. 1
D. 2
E. 1/3
The correct answer is C. 1. The coefficient of performance for the reversed Carnot engine used as a heat pump is equal to 1.
The coefficient of performance (K) of a heat pump is defined as the ratio of the heat energy transferred from the cold reservoir to the input work energy. In the case of the reversed Carnot engine, the coefficient of performance can be calculated using the formula:
K = (Qc / W)
where Qc is the heat energy extracted from the cold reservoir and W is the work input to the system. In the reversed Carnot engine, the heat energy extracted from the cold reservoir is the same as the thermal energy of the engine (0.5), and the work input is equal to the thermal energy minus the heat energy.
W = 0.5 - 0 = 0.5
Therefore, the coefficient of performance (K) is:
K = (0.5 / 0.5) = 1
Hence, the correct answer is C. 1. The coefficient of performance for the reversed Carnot engine used as a heat pump is equal to 1.
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water is not used as thermometric liquid.why?
Answer:
Water cannot be used in thermometer because of its higher freezing point and lower boiling point than other liquids . If water is used in a thermometer , it will start phase change at 0\(degree\\\)C and 100\(degree\)C and will not measure temperature , out of this range . This range is very small as compared to other liquids as mercury , having freezing point about −39\(degree\)C and boiling point 356\(degree\)C.
Explanation:
A constellation’s changing position in the sky, at the same time of the evening, over a period of several weeks is evidence that:
a- Earth is round b- Earth’s axis is tilted. c- Earth rotates on its axis.
d- Earth revolves around the sun.
Answer:
d- Earth revolves around the sun.
Explanation:
Earth rotation can be defined as the amount of time taken by planet earth to complete its spinning movement on its axis.
This ultimately implies that, the rotation of earth refers to the time taken by earth to rotate once on its axis. One spinning movement of the earth on its axis takes approximately 24 hours to complete with respect to the sun.
On the other hand, earth revolution can be defined as a complete trip along a path around the sun. This path is known as an orbit and it typically takes the Earth 365¼ days to complete it's journey around the Sun.
When a constellation (stars) changes its position in the sky, at the same time of the evening and over a period of several weeks; it ultimately implies or is an evidence that Earth revolves around the sun.
What does it mean if electric field lines are close together versus farther apart ?
Answer:
As a result, if the field lines are close together (that is, the field line density is greater), this indicates that the magnitude of the field is large at that point. If the field lines are far apart at the cross-section, this indicates the magnitude of the field is small. (Figure) shows the idea.
Explanation:
interpreting the right-hand rule for magnetic fields which is the correct representation of the right-hand rule for a current flowing to the right?
The correct representation of the right-hand rule for a current flowing to the right is as follows:
Hold your right hand out with your thumb pointing in the direction of the current flow.
Curl your fingers towards the direction of the magnetic field.
Your fingers will indicate the direction of the magnetic field lines around the current-carrying wire.
This right-hand rule is also known as the "right-hand grip rule" or the "right-hand screw rule". It is used to determine the direction of the magnetic field created by a current-carrying wire.
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driver-side and passenger-side air bags will only deploy when the collision impact is within approximately of the vehicle centerline
Driver-side and passenger-side airbags will only deploy when the collision impact is within approximately 15 degrees of the vehicle centerline.
The purpose of airbags is to provide protection to occupants during a collision by rapidly inflating and cushioning the impact. To ensure their effectiveness, airbags are designed to deploy primarily in frontal collisions, where the collision force is directed towards the front of the vehicle.
Modern vehicles are equipped with sensors and algorithms that analyze various factors, including the direction and severity of impact, to determine whether to deploy the airbags. In the case of driver-side and passenger-side airbags, they are typically programmed to deploy when the collision impact is within a certain angle of the vehicle centerline. This angle is generally around 15 degrees on either side of the centerline.
This deployment range is chosen to provide protection for occupants in scenarios where the collision is likely to affect the front of the vehicle, where the driver and front passenger are seated. By limiting the deployment to a specific angle range, the airbags are optimized to deploy when most needed while minimizing unnecessary deployments in situations where the collision impact is not directly towards the front of the vehicle.
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A molecule of oxygen (O2) has a speed of 473 m/s at a certain temperature. Determine the speed of the molecule in kilometers per hour (km/h).
Answer: 1702.8 km/h
Explanation:
The speed of the molecule in kilometers per hour (km/h) will be, {473x(3600÷1000)} km/h
= 1702.8 km/h
What is the new orbital speed after friction from the earth's upper atmosphere has done −7. 5×109J of work on the satellite?
The new orbital speed after friction from the earth's upper atmosphere is 8674.15 m/s.
When the work done by a force does not depend on the choice of path, the force is called the conservative force. Some examples are a gravitational force, elastic spring force and electric force. On the other hand, when the work done by a force relies on the choice of the path of the motion, it is called non-conservative force.
The net work done by non-conservative force is W = ΔK + ΔP ----(1)
Given that, work done W = -7.5 * 10⁹ J
Change in kinetic energy = (Kf - Ki)
Final kinetic energy Kf = 1/2* m * Vf²
Initial kinetic energy Ki = 1/2* m * Vi²
Mass of the satellite m = 848 kg
Vf = Final speed
Vi = Initial speed = 9640 m/s
Change in gravitational potential energy ΔP = 0
Substituting the values in (1),
1/2* m (Vf² - Vi²) = W
1/2 * 848( Vf² -9640²) = W
Making Vf as subject,
Vf = √( 2W/m + Vi²)
⇒ √( -2* 7.5 * 10⁹/848 + 9640²)
⇒ 8674.15 m/s
Thus, the final speed decreases due to friction.
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is heat the same as thermal energy?
Answer:
To be 100% honest im nkt sure but I'm gonna take a gander. yes i think it is the same
Answer:
Yes heat is the same as thermal energy
Explanation:
Heat is the same thing as thermal because Thermal energy refers to the energy contained within a system that is responsible for its temperature. Heat is the flow of thermal energy. A whole branch of physics, thermodynamics, deals with how heat is transferred between different systems and how work is done in the process (see the 1ˢᵗ law of thermodynamics).
a sample of octane burns releasing 2290 j of heat to the surroundings, and the gases produced expands against a piston to do 560 joules of work. calculate the internal energy change for this reaction.
Therefore, this reaction's internal energy change is -2850 J. This indicates a loss of 2850 J in the system's internal energy.
What is a energy in science?The definition defined energy as that of the "power to accomplish work" refers to the capacity to apply a force that moves an object. Kinetic energy and potential energy are the two categories of energy. The quantitative characteristic that is transferred to the a body or into a physical process in physics is energy, which is visible in the performance of labor as well as in form of heat and light. Energy is a resource that is conserved; it can only be changed through one form to another and it cannot be produced or destroyed, according to the law of conservation of energy.
What is the formula of energy and who defined energy?According to the formula E = mc2, a body's mass (m) will vary by an amount equal to E/c2 if its energy increases by an amount E (in any form). This equation was developed by Albert Einstein.
Thomas Young coined the term "energy" for the first time in the realm of physics in 1800, but it didn't catch on. Later, Young utilized interference tests to demonstrate that light is indeed a wave.
The equation: can be used to determine the internal energy change for a reaction.
ΔU = Q - W
where U represents the change in internal energy, Q represents heat added to or released from the system, and W represents work performed by or on the system.
Since it is being released into the environment, the heat contributed to the system in this instance is -2290 J, and the work performed by the system is 560 J. Consequently, the internal energy change can be determined as follows:
ΔU = Q - W
ΔU = -2290 J - 560 J
ΔU = -2850 J
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The Moon orbits Earth at an average distance of 384,000 km and completes one sidereal orbit (with respect to the stars) in about 27.3 days. Based on these two numbers, what is its average orbital speed? Express your answer in km/s.
The given average distance of the Moon from the Earth is 384,000 km and the sidereal period of the moon is 27.3 days. We need to find the average orbital speed of the moon.So, we can use the formula to calculate the average orbital speed of the Moon as follows:
Average orbital speed (V) = distance/time.
To get the distance covered by the moon in one orbit, we will multiply the distance of the Moon from the Earth by the circumference of the orbit:
Distance = 2 × π × r = 2 × π × 384000 = 2.41 × 10^6 km.
Therefore, the average orbital speed of the Moon is given by the formula:V = Distance / Time periodV = 2.41 × 10^6 km / 27.3 days.
We need to convert the time period from days to seconds:1 day = 24 hours1 hour = 60 minutes1 minute = 60 seconds1 day = 24 × 60 × 60 seconds1 day = 86400 seconds.
Therefore, the time period is:27.3 days = 27.3 × 86400 seconds27.3 days = 2.36 × 10^6 seconds.
Substituting this value in the formula we get:V = 2.41 × 10^6 km / 2.36 × 10^6 secondsV = 1.02 km/s.
Therefore, the average orbital speed of the moon is 1.02 km/s.
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A solid 62-kg cylinder has a radius of 0.10 m. What minimum work is required to get the cylinder rolling without slipping at a rotational speed of 20 s^−1 ?
The work done on the solid cylinder is 192 J.
Work corresponds to a change in energy. So, the work required to make this cylinder roll is equal to its final kinetic energy minus its initial kinetic energy.
= W = K' - K
Here, W = work done
K' = Final Kinetic Energy
K = Initial Kinetic Energy
We can assume that this cylinder begins from rest, K = 0,
If an object is rolling, it is undergoing both rotational and translational motion. So, the cylinder's kinetic energy is equal to its translational kinetic energy plus rotational kinetic energy.
= W = (1/2)mv² - (1/2)Iω²
We have values for the cylinder's mass and its rotational speed.
Mass = 62 Kg
Radius = 0.1 m
Rotational Speed = ω = 20 /s
Velocity = v = rω
Moment of inertia = I = (1/2)mr²
Thus,
= W = (1/2)mv² - (1/2)Iω²
= W = (1/2)m(rω)² - (1/2)Iω²
= W = (1/2)m(rω)² - (1/2)X (1/2)mr²X ω²
= W = (1/2)m(rω)² - (1/4)mr²X ω²
= W = (3/4)mr²ω²
= W = (3/4) X 62 X 0.1² X 20²
= W = 192 J
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The ratio of the number of pigs to the number of horses in a farm is 2 to 2(2:3), if there are 24 horses, what is the number of pigs?
Answer:
36
Explanation:
2=24
24÷2=1
1=12
12*3=36
Ratio is from pigs to horses so:
Let no. of pigs be x
= 2:3 :: x:24
= 2/3 = x/24
= 2 × 24 = 3x
= 48/3 = x
= 16 = x
So the no. of pigs in farm - 16.
suppose we wish to represent the electric potential around q1q1 and q2q2 by drawing isolines. what is the relationship of the isolines of electric potential to the net electric field vectors in the region around q1q1 and q2q2?
The isolines are always opposite to the electric field vectors in the region around q1q1 and q2q2.
isolines - The lines known as isolines link points with equal values.
To draw Isolines of Electric Potential :
They are usually closed loops, for oneThey always make a right angle turn to cross the electric field lines.They are prohibited from crossing any other electric potential lines. Where the electric field is stronger They are closer together.They do not go via a conductor.The isolines are always opposite to the electric field vectors in the region around q1q1 and q2q2.
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A snap together cube has a protruding snap on one side and receptacle holes on the other 55 sides. What is the smallest number of these cubes that can be snapped together so that only receptacle holes are showing
The smallest number of cubes needed is 28. This forms a 3x3x3 cube with one central cube missing.
To minimize the number of protruding snaps while maximizing the number of receptacle holes, the cubes should be arranged in a 3x3x3 cube formation.
This structure would have 27 cubes, but one central cube must be removed to eliminate all protruding snaps.
Each of the remaining 26 cubes will have at least one side with receptacle holes facing outward.
The missing central cube ensures no protruding snaps are exposed.
Therefore, the smallest number of snap-together cubes needed to have only receptacle holes showing is 28.
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Do greenhouse gases impact global temperatures? Use evidence collected from your model to support your answer.
In context to the given question the answer is yes, greenhouse gases provide great impact global temperatures. Climate scientists totally appreciate and agree that increasing levels of carbon dioxide and other greenhouse gases are severely and directly linked to the increasing global temperatures.
Greenhouse gases aids to absorb heat radiating from the Earth’s surface and re-release it in all directions—involving back toward Earth’s surface. The concept of not having carbon dioxide will conclude and make the Earth’s natural greenhouse effect too weak comparatively than before to keep the average global surface temperature above freezing.
The IPCC have predicted and forecasted that greenhouse gas emissions will carry on and lead to increase over the next few decades. The result being severe, they forcasted that the average global temperature will gradually increase by about 0.2 degrees Celsius per decade.
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f the oldest rocks in the 19 km wide strip are about 750,000 years old, what has been the average speed of the sea floor expansion during this time? type your answer here
The average speed of the sea floor expansion during this time has been approximately 8.03 x \(10^{-7\) meters per second.
The sea floor expansion can be calculated using the age of the oldest rocks and the width of the strip. In this case, the oldest rocks are 750,000 years old, and the strip is 19 km wide. To find the average speed of expansion, we need to divide the width of the strip by the age of the rocks.
Average speed of sea floor expansion = (Width of the strip) / (Age of the oldest rocks)
Average speed = (19 km) / (750,000 years)
To convert years to seconds, multiply by the number of seconds in a year (365.25 days/year * 24 hours/day * 60 minutes/hour * 60 seconds/minute):
750,000 years * 365.25 * 24 * 60 * 60 = 23,652,060,000 seconds
Now, divide the width of the strip by the age of the rocks in seconds:
Average speed = (19,000 meters) / (23,652,060,000 seconds)
Average speed ≈ 8.03 x \(10^{-7\) meters/second
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A rock moving through a gravitational field is analogous to a _______________ charge moving through an electric field.
Answer:A rock moving through a gravitational field is analogous to a "massive" charge moving through an electric field.
Just as a charged particle experiences a force when moving through an electric field, a massive object experiences a force when moving through a gravitational field. The strength of the force depends on the mass of the object and the strength of the field. This is described by Newton's law of gravitation.
Explanation:
A rock moving through a gravitational field is analogous to a positive or negative charge moving through an electric field
Comparison between gravitational field and electric field:
A rock moving through a gravitational field is analogous to a positive or negative charge moving through an electric field, depending on the direction of the gravitational force and the sign of the charge.
Both the gravitational field and the electric field are conservative fields that exert a force on objects or charges within their respective fields.
However, the strength and nature of the force depend on the mass or charge of the object or particle, as well as the distance and direction from the source of the field.
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