Given:
The potential difference V=3000 V
The radius of curvature of the curved path of the electron, r=26.0 cm=0.26 m
The velocity of the electron, v=32.5 Mm/s=32.5×10⁶ m/s
To find:
The magnitude of the magnetic field.
Explanation:
The magnetic force acting on the electron provides it the neccessary centripetal force to trace a curved path.
Thus the centripetal force acting on the electron is equal to the magnetic force acting on it.
Therefore,
\(\frac{mv^2}{r}=\text{evB}\)Where m is the mass of the electron, e is the charge of the electron, and B is the magnitude of the magnetic field.
On rearranging the above equation,
\(B=\frac{mv}{er}\)On substituting the known values,
\(\begin{gathered} B=\frac{9.1\times10^{-31}\times32.5\times10^6}{1.6\times10^{-19}\times0.26} \\ =7.1\times10^{-4} \\ =710\text{ }\mu\text{T} \end{gathered}\)Final answer:
The magnitude of the magnetic field is 710 μT.
A car travels with speed 3 m/s for the first half distance of the journey and with speed 6 m/s for the remaining half. What is the average speed of the entire journey?
(1) 6 m/s
(2) 18 m/s
(3) 9 m/s
(4) 4 m/s
Explanation:
hope this gives u a little hint!!!!
The average speed of the entire journey is 4 m/s.
The given parameters:
Initial speed of the car, u = 3 m/sFinal speed of the car, v = 6 m/sLet the total distance of the journey = d
The time taken for the first half of the journey is calculated as follows;
\(t_1= \frac{d}{v_1} = \frac{d}{3} \)
The time taken for the second half of the journey is calculated as follows;
\(t_2 = \frac{d}{v_2} = \frac{d}{6} \)
The average speed of the entire journey is calculated as follows;
\(v = \frac{d + d}{t_1 + t_2} \\\\ v = \frac{2d}{d/3 \ + \ d/6} \\\\ v = \frac{2d}{d/2} \\\\ v = \frac{4d}{d} \\\\ v = 4 \ m/s\)
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Suppose that a series RL circuit is connected to a voltage source whose input voltage (Vin) is shown in the figure above. As shown in the figure above, the input voltage Vin = Vmax only within time interval 0 ≤ t ≤ T. The input voltage Vin = 0 outside this time interval. Assume that initially (at t = 0), no current is flowing in this circuit (I = 0)! A Determine the output voltage Vout as a function of time t! B Assume that the time interval T is very short so that T → 0, and also assume the the maximum voltage Vmax is quite high, so that VmaxT ≈ Φimp. Show that the output voltage Vout can be approximated by the following equation : Vout(t) ≈ Φimp τ e −t/τ where τ = L R
A. The output voltage, Vout, as a function of time, t, in a series RL circuit can be determined using the equation: Vout(t) = Vmax * (1 - e^(-t/τ)), where τ = L/R.
B. When the time interval T is very short (T → 0) and the maximum voltage Vmax is quite high (VmaxT ≈ Φimp), we can approximate the output voltage Vout using the equation: Vout(t) ≈ Φimp * e^(-t/τ), where τ = L/R.
A. To determine the output voltage Vout as a function of time t in a series RL circuit, we use the following equation:
Vout(t) = Vmax * (1 - e^(-t/τ))
Here, Vmax is the maximum input voltage, τ = L/R is the time constant of the circuit (where L is the inductance and R is the resistance).
B. When the time interval T is very short (T → 0) and the maximum voltage Vmax is quite high (VmaxT ≈ Φimp), we can make the following approximation:
Vout(t) ≈ Vmax * e^(-t/τ)
In this case, we substitute VmaxT with Φimp, which is the total magnetic flux in the circuit.
Rearranging the equation, we get:
Vout(t) ≈ Φimp * e^(-t/τ)
This approximation is valid when the time interval T is very small compared to the time constant τ of the circuit and when the maximum voltage is sufficiently high.
The time constant τ is determined by the values of inductance (L) and resistance (R) in the circuit. It represents the characteristic time scale over which the current and voltage in the circuit change in response to a voltage or current input.
Therefore, in the given scenario, when T is very small and Vmax is high, we can approximate the output voltage Vout(t) in the series RL circuit by the equation: Vout(t) ≈ Φimp * e^(-t/τ), where τ = L/R.
Note: The symbol Φimp in the equation represents the total magnetic flux in the circuit.
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how long does it take energy to pass through the radiative zone
8 minutes A
100,000 years B
10,000 years C
100 years D
Time it takes energy to pass through radiative zone is : A) 8 minutes
How long does it take energy to pass through radiative zone?Energy generated in the core of the Sun takes about 8 minutes to pass through radiative zone and reach the top of convective zone. The radiative zone is a layer of the Sun that lies just outside the core and it is characterized by high density and high temperature.
In this zone, energy is transported by photons that bounce around between atoms and ions that make up the plasma of the Sun. This process is known as radiative diffusion and is relatively slow compared to convective transport of energy that takes place in the outer layers of Sun.
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Hunting a black hole Observations of the light from a certain star indicate that it is part of a binary (two-star) system: This visible star has orbital speed v = 270 km/s, orbital period T = 18.1 days, and approximate mass m1 6.9Ms, where Ms is the Sun's mass, 1.99 x 1030 , kg: Assume that the visible star and its companion star; which is dark and unseen, are both in circular orbits (see the figure). Find the ratio of the approximate mass mz of the dark star to Ms: Number Units Nounits
The approximate mass of a dark star is 4.35 times the mass of the Sun.
To find the ratio of the mass of the dark star to the mass of the Sun, we can use the binary star formula, which states that the total mass of a binary star system is equal to the mass of the visible star divided by the sine of the angle between the line of sight and the line connecting the two stars:
m1 / sin i = (v² ×T) / (4 × pi² ×d)
where m1 is the mass of the visible star, v is the orbital velocity of the visible star, T is the orbital period of the visible star, i is the angle between the line of sight and the line connecting the two stars, and d is the distance between the two stars.
In this case, we are given the mass of the visible star (m1 = 6.9 Ms), the orbital velocity of the visible star (v = 270 km/s), the orbital period of the visible star (T = 18.1 days), and we can assume that the angle between the line of sight and the line connecting the two stars is 90 degrees (since we cannot see the dark star).
Substituting these values into the binary star formula, we get:
m1 / sin i = (270² × 18.1) / (4 ×pi² × d)
Since sin 90 = 1 and m1 = 6.9 Ms, we can simplify the equation to:
6.9 Ms = (270²× 18.1) / (4 × pi²× d)
Solving for d, we find that d = (270²× 18.1) / (4 × pi²× 6.9 Ms) = 2.43 x 10¹¹ meters.
Now that we know the distance between the two stars, we can use the binary star formula again to find the mass of the dark star. Substituting the values we have calculated into the binary star formula, we get:
m2 / sin i = (v²×T) / (4 × pi²× d)
where m2 is the mass of the dark star and v, T, and d are the same as before. Knowing that m1 = 6.9 Ms and sin i = 1, we can solve for m2 to find the mass of the dark star.
m2 = (v²×T × m1) / (4 × pi²× d)
Substituting the known values, we get:
m2 = (270²× 18.1 × 6.9Ms) / (4 × pi²× 2.43 x 10¹¹)
Simplifying, we find that the mass of a dark star is m2 = 8.7 Ms.
Therefore, the ratio of the mass of a dark star to the mass of the Sun is m2 / Ms = 8.7 / 1.99 = 4.35.
Therefore, the approximate mass of a dark star is 4.35 times the mass of the Sun.
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calculate the gravitational potential Energy of the ball relative to the ground before being thrown
Given,
The mass of the ball, m=0.11 kg
The height of the ball before it was thrown, h₁=0.24 m
The height of the ball after it was caught by Donald, h₂=0.82 m
The gravitational potential energy is the energy stored in an object due to its position above the ground.
The gravitational potential energy of the ball before being thrown is given by,
\(E=\text{mgh}_1\)On substituting the known values,
\(\begin{gathered} E=0.11\times9.8\times0.24 \\ =0.26\text{ J} \end{gathered}\)Thus the gravitational potential energy of the ball relative to the ground, before being thrown is 0.26 J
Help me with the following problem
The net magnetic field between the two parallel wires is determined as 1775 nT.
Magnetic field at wire 2 due to current 1
The magnetic field is calculated as follows;
\(B_z_1 = \frac{\mu _0 I_1}{2\pi r} \\\\B_z_1 = \frac{4\pi \times 10^{-7} \times 42 }{2\pi \times 7} \\\\B_z_1 = 1.2 \times 10^{-6} \ T\)
Magnetic field at wire 1 due to current 2The magnetic field is calculated as follows;
\(B_z_2= \frac{\mu _0 I_2}{2\pi r} \\\\B_z_2 = \frac{4\pi \times 10^{-7} \times 23 }{2\pi \times 8} \\\\B_z_2 = 5.75 \times 10^{-7} \ T\)
Net magnetic fieldB = BZ1 + BZ2
B = 1.2 x 10⁻⁶ + 5.75 x 10⁻⁷
B = 1.775 x 10⁻⁶ T
B = 1775 x 10⁻⁹ T
B = 1775 T nT
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During a solar eclipse, which of the following is true?
Another planet blocks the Sun's light from hitting the surface of the Earth.
The Earth blocks the sun's light from hitting the surface of the moon
The Moon blocks the Sun's light from hitting the surface of the Earth.
Another planet blocks the Sun's light from hitting the surface of the Moon.
Answer:
The Moon blocks the suns light from hitting the surface of the earth
Answer:
The Moon blocks the Sun's light from hitting the surface of the Earth.
I want for more information for these subject ,EXITONS AND BIEXITONS IN SEMICONDUCTOR QUANTUM DOLLS, I have to write a project about EXITONS AND BIEXITONS IN SEMICONDUCTOR QUANTUM DOLLS.
The study of excitons and biexcitons in semiconductor quantum dots is a fascinating and rapidly evolving field in semiconductor physics. Excitons are bound states of an electron and a hole created by the absorption of a photon in a semiconductor material. These quasi-particles exhibit unique optical and electronic properties, making them important for various applications such as optoelectronic devices and quantum information processing.
1. Introduction:
- Provide an overview of excitons and biexcitons in semiconductor quantum dots.
- Mention their significance in semiconductor physics and applications.
2. Excitons:
- Define excitons as bound electron-hole pairs.
- Explain how they form through photon absorption.
- Discuss their properties, such as energy levels, binding energies, and radiative lifetimes.
- Describe their behavior under external electric and magnetic fields.
3. Semiconductor Quantum Dots:
- Introduce semiconductor quantum dots as nanoscale structures with unique quantum confinement effects.
- Explain the synthesis methods for quantum dots, such as colloidal synthesis or epitaxial growth.
- Discuss their size-dependent electronic and optical properties.
4. Biexcitons:
- Define biexcitons as two excitons bound together.
- Explain the conditions for biexciton formation.
- Discuss their properties, including binding energies, lifetimes, and interaction with external fields.
5. Experimental Techniques:
- Describe the experimental methods used to study excitons and biexcitons in semiconductor quantum dots, such as photoluminescence spectroscopy or ultrafast spectroscopy.
- Highlight the importance of time-resolved techniques for understanding exciton dynamics.
6. Applications:
- Discuss the applications of excitons and biexcitons in semiconductor quantum dots, such as in optoelectronic devices (e.g., solar cells, light-emitting diodes) and quantum information processing (e.g., quantum dots as qubits).
7. Current Research and Future Directions:
- Provide an overview of recent advancements in the field.
- Mention ongoing research efforts and emerging areas of interest.
- Discuss potential future directions and challenges in the study of excitons and biexcitons in semiconductor quantum dots.
8. Conclusion:
- Summarize the key points discussed in the project.
- Emphasize the significance of excitons and biexcitons in semiconductor quantum dots for fundamental research and technological applications.
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Bent over row trains what specific muscle?
O A. triceps
O B. trapezius
O C. latissimus dorsi
D. pectoralis major
It is the source and summit of the whole Christian Life."
Answer:
CRISTO
Explanation:
UWU
Answer:
The Eucharist
Explanation:
In The Catechism of the Catholic Church (1324-1327), it states that The Eucharist is the source and summit of the whole Christian Life.
Pls answer when u can
Answer:
I believe the answer is C. 1 and 3
Explanation:
I'm 100% sure that 1 is correct, from what I remember learning.
As for 3, it was hard to choose between 3 and 4, but I'm pretty certain that covalent bonds shared electrons rather than transfer them.
Hope this helps you, please let me know if it was correct :DWhich one of the following variables is the best indicator of thermal equilibrium between to systems in thermal contact?a) pressureb) volumec) temperatured) masse) time
The variable that is the best indicator of thermal equilibrium between two systems in thermal contact is temperature.Thermal equilibrium occurs when two systems in thermal contact with each other are at the same temperature.
In simpler terms, the net heat flow between the systems will be zero if they are in thermal equilibrium. Furthermore, when two systems reach thermal equilibrium, there is no longer a temperature difference between them.Temperature is a measure of the amount of heat in a substance. It's measured in Celsius, Kelvin, and Fahrenheit. A substance's temperature is a reflection of how fast the molecules in it are moving. The faster the molecules move, the higher the temperature of the substance. The slower the molecules move, the lower the temperature of the substance. The Kelvin scale is used to measure temperature in scientific experiments since it begins at absolute zero, the point at which there is no thermal energy present. As a result, it is the most accurate scale for measuring temperature.for more such question on equilibrium
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Brainlist!! Help!! The nucleus contains protons and neutrons. Being positively charged, the protons repel each other. The nucleus should fly apart due to the repulsive force. Yet, the nuclei of most atoms are stable - explain.
Answer:
The reason that the nucleus of most atoms does not fall apart despite the oppositely charged protons exerting a repulsive force on each other is the strong nuclear force.
What is the strong nuclear force?The strong nuclear force is one of the fundamental forces in nature that acts between protons and neutrons in the atomic nucleus. It is a short-range force that is much stronger than the electromagnetic force (which produces the repulsion between protons).
The strong nuclear force is responsible for holding the nucleus together.
Additionally, the ratio of protons to neutrons in a nucleus also affects its stability. Therefore, if there is an imbalance in this ratio, the repulsive force between the protons can become too strong, causing the nucleus to become unstable and undergo radioactive decay.
Overall, the nucleus remains stable due to the balance between the strong nuclear force and the repulsive force between the protons.
I NEED ANSWER NOW
A variety of mature plants and trees indicates this level of ecological succession:
Responses
opportunists
pioneer species
climax community
primary succession
A hiker enters an area where there are large mature trees and a diverse population of other mature plants and shrubs.
Which statement best describes this ecosystem?
It is a climax community.
It is populated with pioneer plants.,
It features many opportunists.,
A hiker approaches a region with many enormous, mature trees and just a variety of other mature bushes and plants. The ecosystem is best describe by the "climax community."
Explain the term climax community?In ecology, the term "climax" refers to the last stage that biotic succession that a plant community can reach in a region depending on the environmental factors in place at the time.
For instance, in the eastern United States, cleared forests develop from fields to older fields with migrating trees and plants to forests among these early colonists, and finally towards climax communities comprising longer-lived tree species. The climax community's species composition doesn't change since all of the existing species are able to reproduce, whereas invasive species are unable to establish a presence. The climax stage isn't really entirely permanent since ecological processes, evolutionary processes, and climate changes all alter the environment over extremely long stretches of time.A hiker approaches a region with many enormous, mature trees and just a variety of other mature bushes and plants.
Thus, this ecosystem is best describe by the "climax community."
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The correct question is-
A hiker enters an area where there are large mature trees and a diverse population of other mature plants and shrubs.
Which statement best describes this ecosystem?
It is a climax community.
It is populated with pioneer plants.,
It features many opportunists.,
Answer: c
Explanation:
A dolphin has a mass of 125 kg and is moving along with 775 J of kinetic energy. How fast is it moving? (Hint: use the formula to solve for KE)
Question 43 options:
12.4 m/s
3.52 m/s
0 m/s
6.2 m/s
Answer: 3.52m/s
Explanation:
Kinetic energy is calculated as:
= 1/2mv²
where,
m = mass
v = velocity
Therefore,
775 = 1/2 × 125 × v²
775 = 62.5v²
v² = 775/62.5
v² = 12.4
v = ✓12.4
v = 3.52m/s
If two clay masses produce a gravitational force of 340N, what will be the force if the distance is divided by 3 and the mass of one is divided by 2?
75.56 N
1530 N
510 N
56.67 N
Answer:
B: 1530 N
Explanation:
We know ghat formula for force of gravity is;
F_grav = G•m1•m2/d²
We are told that two clay masses produce a gravitational force of 340N.
Thus;
G•m1•m2/d² = 340
Now, if the distance is divided by 3 and the mass of one is divided by 2, we have;
F_g = (G × m1/2 × m2)/(d/3)²
Thus gives;
F_g = ½(G•m1•m2)/((1/9)d²)
Simplifying this gives;
F_g = (9/2)G•m1•m2/d²
From earlier, we saw that;
G•m1•m2/d² = 340
Thus;
F_g = (9/2) × 340
F_g = 1530 N
Postural deviations can result in
Answer:
Postural deviations can cause poor balance, muscle pain and skeletal stress.
Explanation:
The mass percent of hydrogen in CH₄O is 12.5%.
What is the mass percent?Mass percent is the mass of the element divided by the mass of the compound or solute.
Step 1: Calculate the mass of the compound.
mCH₄O = 1 mC + 4 mH + 1 mO = 1 (12.01 amu) + 4 (1.00 amu) + 1 (16.00 amu) = 32.01 amu
Step 2: Calculate the mass of hydrogen in the compound.
mH in mCH₄O = 4 mH = 4 (1.00 amu) = 4.00 amu
Step 3: Calculate the mass percent of hydrogen in the compound.
%H = (mH in mCH₄O / mCH₄O) × 100%
%H = 4.00 amu / 32.01 amu × 100% = 12.5%
The mass percent of hydrogen in CH₄O is 12.5%.
CO2 = 1.580 grams H2O = 0.592 grams Lookup the molar mass of each element in the compound Carbon = 12.0107 Hydrogen = 1.00794 Oxygen = 15.999 Calculate the molar mass of CH4O by adding the total masses of each element used. 12.0107 + 4 * 1.00794 + 15.999 = 32.04146 Now calculate how many moles of CH4O you have by dividing by the molar mass. m = 1.15 g / 32.04146 g/mole = 0.035891 mole Now figure out how many moles of carbon and hydrogen you have. Carbon = 0.035891 moles Hydrogen = 0.035891 moles *
Therefore, The mass percent of hydrogen in CH₄O is 12.5%.
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A girl is swinging on a rope. Does the rope supporting the swing act on the girl at the very top of her swing?
A) yes
B) no
prepare a report on why a vehicle needs to be maintained/serviced after a certain period of time. How is servicing different in a petrol/diesel and electric vehicle?
Vehicles need to be serviced for several reasons such as preventing costly repairs and improving fuel economy.
Why should cars be maintained and / or serviced ?First, regular maintenance can help to prevent costly repairs down the road. Second, maintenance can help to improve fuel economy and emissions. Third, maintenance can help to keep your vehicle safe and reliable.
The servicing requirements for petrol/diesel and electric vehicles differ in a number of ways. Petrol/diesel vehicles require oil changes more frequently than electric vehicles. This is because petrol/diesel engines use oil to lubricate the moving parts, while electric motors do not. Petrol/diesel vehicles also require tune-ups more frequently than electric vehicles.
This is because petrol/diesel engines have more moving parts that need to be synchronized, while electric motors have fewer moving parts.
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Our Sun has a radius of about 695,800 km and a mass of about 2.0 × 1030 kg, and rotates around its axis about once every 29 days.
Calculate the rotational velocity of the Sun.
Calculate the linear speed of particles on the outermost portion of the Sun.
Calculate the angular acceleration, tangential acceleration, and radial acceleration of the Sun.
Calculate the rotational (angular) momentum of the Sun, modeled as a uniform solid sphere. The rotational inertia of a solid sphere is (2/5)MR2.
Imagine that without any external objects interacting with it, the Sun were to collapse to the size of a neutron star, with a radius of about 15 km–about the size of Manhattan Island.
What would be its rotational inertia when it was finished collapsing?
What would be its rotational momentum when it was finished collapsing?
In what time interval would the Sun complete one rotation around its axis after it was finished collapsing
When a skater pulls in her arms, a kid starts up a merry-go-round from a stop, or a computer's hard disk slows to a stop when it is turned off, angular velocity is not constant.
Thus, There is an angular acceleration in each of these situations, in which changes. The angular acceleration increases with the rate of change. The rate at which angular velocity changes is referred to as angular acceleration.
The answer is that the air masses that generate tornadoes rotate, and their rate of rotation rises as their radii get smaller and angular velocity.
The skater begins her rotation by extending her limbs, then she pulls them in closer to her torso to increase the spin.
Thus, When a skater pulls in her arms, a kid starts up a merry-go-round from a stop, or a computer's hard disk slows to a stop when it is turned off, angular velocity is not constant.
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The rotational velocity or angular velocity of the sun is 2.5 x 10⁻⁶ rad/s.
The angular acceleration of the sun is 43.5 x 10⁻⁴ rad/s².
The angular momentum is 96.8 x 10⁴⁰kgm²/s.
Radius of the sun, R = 6.96 x 10⁸m
Mass of the sun, m = 2 x 10³⁰kg
Time period of the sun, T = 29 days = 2.51 x 10⁶s
Angular velocity is the rate of change in the angular displacement between two bodies or the pace at which an object revolves or rotates around an axis.
The rotational velocity or angular velocity of the sun is,
ω = 2π/T
ω = 2 x 3.14/2.51 x 10⁶
ω = 2.5 x 10⁻⁶ rad/s
The linear speed of particles on the outermost portion of the sun is,
v = Rω
v = 6.96 x 10⁸x 2.5 x 10⁻⁶
v = 1.74 x 10³m/s
The angular acceleration of the sun,
α = Rω²
α = 6.96 x 10⁸x (2.5 x 10⁻⁶)²
α = 43.5 x 10⁻⁴ rad/s²
The moment of inertia of the solid sphere, I = 2/5MR²
The expression for the angular momentum is given by,
L = Iω
L = 2/5 x 2 x 10³⁰ x (6.96 x 10⁸)² x 2.5 x 10⁻⁶
L = 96.8 x 10⁴⁰kgm²/s
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A 8.5 kg brick is dropped onto a 6.5 kg toy truck, which is moving across a level floor at 0.50 m/s. With what velocity do the truck and brick continue to move, after the brick has landed on the truck?
Answer:0.2167 m/s
Explanation:
Given
mass of brick M=8.5 kg
mass of toy truck m=6.5 kg
the velocity of truck u=0.5 m/s
Suppose v is the velocity after brick is landed on the truck
There is no external force acting so momentum is conserved
mu=(M+m)v
\(v=\dfrac{6.5}{15}\times 0.5\\v=0.2167\ m/s\)
Question 21 of 25
Which is the smallest frequency?
O A. 8.1 x 1012 Hz
O B. 6.2 x 1016 Hz
C. 5.7 x 1018 Hz
O D. 3.4 x 1014 Hz
a driver travels 4.25 km in two minutes. if the driver's initial velocity is 20m/s, what is the acceleration
Recall the definition of average velocity:
average v = ∆x / ∆t
The driver moves a distance of ∆x = 4.25 km = 4250 m in 2 min = 120 s, so the average velocity is
average v = (4250 m) / (120 s) ≈ 35.4 m/s
Under constant acceleration, the average velocity can also be computed by taking the average of the initial and final velocities:
average v = (initial v + final v) / 2
Solve for (final v) :
35.4 m/s = (20 m/s + final v)/2
final v ≈ 50.83 m/s
Recall the definition of average acceleration:
average a = ∆v / ∆t
Solve for a :
a = (50.83 m/s - 20 m/s) / (120 s)
a ≈ 0.257 m/s²
A body is projected horizontally downward from a rock 80m high with a velocity of 20m/s ! calculate (1) the time taken for the body to fall to ground. (2)the vertical component of the velocity when the body falls to the ground (3) the distance from the rock when it strick the ground 10m/s
1. The time taken for the body to fall to ground is 4 s
2. The vertical component of the velocity when the body falls to the ground is 39.2 m/s
3. The distance from the rock when it strick the ground 10m/s is 40 m
1. How to determine the time Height (h) = 80 mHorizontal velocity = 20 m/sTime (t) =?h = ut
80 = 20 × t
Divide both sides by 20
t = 80 / 20
t = 4 s
Thus, it will take the body 4 s to land on the ground.
2. How to determine the vertical component of the velocityTime (t) = 4 sAcceleration due to gravity (g) = 9.8 m/s²Velocity (v) =?v = gt
v = 9.8 × 4
v = 39.2 m/s
3. How to deteremine the distanceHorizontal velocity = 10 m/sTime (t) = 4 sHorizontal distance (s) =?s = ut
s = 10 × 4
s = 40 m
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Despite their name, standing waves actually do cause the medium to move.
True or False
Answer:
TRUEE
Explanation:
Julie blows a bubble. At first, the pressure of the gas in the bubble is 4kPa. The bubble floats into the air and expands. When it gets to the top of a tree the bubble has a pressure of 2kPa and a volume of 3.5m³. Assuming a constant temperature, what was the volume in m³ of the bubble when it was first blown?
Answer:
V₁ = 1.75 m³
Explanation:
Assuming the gas to be an ideal gas. At constant temperature, the relationship between the volume and temperature of an ideal gas is given by Boyle's Law as follows:
\(P_{1}V_{1} = P_{2}V_{2}\)
where,
P₁ = Initial Pressure of the Gas = 4 KPa
V₁ = Initial Volume of the Gas = ?
P₂ = Final Pressure of the Gas = 2 KPa
V₂ = Final Volume of the Gas = 3.5 m³
Therefore,
\((4\ KPa)V_{1} = (2\ KPa)(3.5\ m^{3})\\\\V_{1}=\frac{2\ KPa}{4\ KPa}(3.5\ m^{3})\\\\\)
V₁ = 1.75 m³
If the velocity of a car is 45 kilometers per hour west.How far can it travel in 0.5 hours?
Answer:
144 kilometers
Explanation:
\(\frac{45}{0.5} = 90 miles\\ convert\\ kilometers\\ 144\)
Final Answer:144
To accelerate, an object must
Answer:
be acted upon an object or person
Explanation:
The energy diagram shows the changes in energy during a chemical reaction.
Which statement best describes the total energy change of the system?
Potential energy
Reaction progress
• A. The reactants have higher potential energy, and energy is released.
absorbed.
• B. The reactants have higher potential energy, and energy is
absorbed.
C. The products have higher potential energy, and energy is
D. The products have higher potential energy, and energy 1S released.
B. The reactants have higher potential energy, and energy is absorbed is the statement that best describes the total energy change of the system.
What term best explains the energy shifts that occur during chemical reactions?The difference in the amounts of chemical energy that are stored in the products and reactants accounts for the energy change in a chemical reaction. Enthalpy refers to the system’s heat content or stored chemical energy.
What is potential energy?Potential energy can be described as the energy which a body possess because of its position. The potential energy can also be said as stored energy. The energy diagram that shows the changes in energy is called as a chemical reaction.
Potential energy and the Reaction progress are shown in the problem and from this the reactants are seen as the substance which reacts and form one or more than one product.
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Is lightning ac or dc?
Answer:
ac
Explanation: