A person is riding a skateboard on a U-shaped ramp. At which point does the person have the greatest potential energy?(1 point)

on the downswing as the person is dropping into the ramp
on the downswing as the person is dropping into the ramp

at the top of the ramp before dropping in
at the top of the ramp before dropping in

in the middle of the ramp at the lowest point
in the middle of the ramp at the lowest point

on the upswing as the person is coming up the other side of the ramp

Answer:

False

Explanation:

Meters are a unit of length and seconds are a unit of time.

Rigel, which appears blueish in color, has a higher surface temperature compared to Betelgeuse, which has a distinctly reddish appearance. This is because blue stars have higher surface temperatures, emitting shorter wavelength light, while red stars have lower surface temperatures, emitting longer wavelength light.

The image shows the constellation Orion, which is one of the most prominent winter constellations in the Northern Hemisphere. The star Betelgeuse, marking Orion's left shoulder, has a reddish appearance, while the star Rigel, marking Orion's right foot, appears bluish in color. The star with the lower surface temperature is Betelgeuse.

The reason for this is that stars with a reddish appearance have a lower surface temperature compared to stars with a bluish appearance. This is because cooler stars emit more light in the red part of the spectrum, while hotter stars emit more light in the blue part of the spectrum.

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Answer:

Density → Mass and Length.

Acceleration → Length and Time.

Force → Mass, Length and Time.

Pressure → Mass, Length and Time.

Work → Mass, Length and Time.

Answer: 45 meters

Explanation:

3 m/s ==> 3 meters/second

15 seconds * 3 meters/second=

15*3/1=

15*3=45 meters

The distance which the football which cover before landing back on the ground level will be about 56.4 meters.

The mass of football, m = 0.43 kg, Initial velocity of football (v) = 24 m/s, Angle of inclination(θ) = 53°

From the given data, we know that the vertical component of the initial velocity is given by, vsin(θ) and the horizontal component of initial velocity is given by, vcos(θ). So, the time taken by the football to reach the maximum height is given by,

t = (vsin(θ))/g

Here, g = 9.8 m/s²

Now, the maximum height attained by the football is given by,h = (vsin(θ))²/(2g).

Therefore, the time of flight or the total time which is taken by the football to land on the ground level is given by,

T = 2t

Now, the horizontal distance travelled by the ball is given by, d = (vcos(θ))T

Substituting the given values in the above formulas, we get:

t = (24sin(53°))/9.8 = 1.71 s

h = (24sin(53°))²/(2×9.8) = 23.4m

T = 2×1.71 = 3.42 s

d = (24×cos(53°))×3.42 = 56.4 m

Therefore, the football will go 56.4 m before it is landing back on the level ground.

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Freefall is the state of a body that moves freely in any direction in the presence of gravity. The window is 15.01 meters above the ground.

According to free fall,

vf = g * t

here Vf = 17.2 m/s

g = 9.8 m/s^2

then t = vf/ g = 17.2/9.8 =1.75 sec

According to free fall Equation,

Distance d = 1/2 g * t^2

d= 1/2 *9.8 * 1.75^2= 15.01 m

Window is located 15.01 m height from the Ground.

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Explanation:

The surface tension of a liquid results from an imbalance of intermolecular attractive forces, the cohesive forces between molecules: A molecule in the bulk liquid experiences cohesive forces with other molecules in all directions. A molecule at the surface of a liquid experiences only net inward cohesive forces.

A condition which would always result in a net force of zero (0) Newton is: A. Two equal but opposite forces act on an object.

Newton's Second Law of Motion states that the acceleration of an object is inversely proportional to its mass and directly proportional to the net force acting on the physical object.

Mathematically, Newton's Second Law of Motion is given by this formula;

\(Acceleration = \frac{Net \; force}{Mass}\)

According to Newton's Second Law of Motion, the acceleration of a physical object occurs when there is a net force on an object while a net force (sum of all the forces) zero (0) causes no acceleration.

In Science, an object is said to be at equilibrium when two equal but opposite forces are acting on it and this would always result in a net force of zero (0) Newton.

For example:

\(0 N = 5N + (-5N)\\\\0N = 5N - 5N\)

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Answer:

An object is at rest

Explanation:

An audience member covers her ears during a loud concert shows evidence that matter can reflect waves.

An audience member covers her ears during a loud concert is an event that provides evidence that matter can reflect waves because a sound is heard again and again due to the reflection of waves. This repetition of sound is due to the property of reflection of sound waves.

So we can conclude that an audience member covers her ears during a loud concert shows evidence that matter can reflect waves.

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Answer:

A laser beam bounces off a series of mirrors

Explanation:

Answer:

Following are the answer to this question:

Explanation:

The wave is propagating at the incident wave which focuses on the stretchy and rotational inertia features of the whole medium via a material system.  For both the mechanical waves there are many two basic types of incident waves: quality management program and transverse waves.

The rumor is also known as the "Norman Rockwell", in which the environment of some of the greatest physics attempts of our time, it pays to remain suspicious when remarkable reports of historical findings are made on social media.

Answer:

soln

work done= 200J

Time taken = 5 sec

power=?

We know that,

power=w/t

= 2000/5

= 400W

Explanation:

hopw this will help you

The inductance of a coil if the coil produces an emf of 2.50 v when the current in it changes from -28.0 ma to 25.0 ma in 12.0 ms is L   = 0.566 H

An inductor is a passive electronic component that stores energy in the form of a magnetic field. In its simplest form, an inductor consists of a wire loop or coil. The inductance is directly proportional to the number of turns in the coil.

The SI unit of inductance is Henry abbreviated as 'H'. It is defined as the measure of electric current changes at one ampere per second resulting in an electromotive force of one volt across the inductor.

The expression for induced emf

E=−L (di /dt)

L= E (dt / di )

di = 25 - ( -28) = 53 mA = 53 * \(10^{-3}\)  A

dt = 12 ms = 12 *  \(10^{-3}\) sec

E = 2.5 V

L = 2.5 ( 12 *  \(10^{-3}\)  / 53 * \(10^{-3}\) )

L   = 0.566 H

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The value of resistor R that gives the circuit in the figure a time constant of 22 μs is 220 Ω.

The circuit that is in the figure is shown below:Given that time constant (RC) = 22 μs. To find the value of resistor R, we need to use the formula for the time constant:

RC = τ, where R is the resistance and C is the capacitance of the circuit.

Rearranging the above formula, we get:R = τ / C

Where τ is the time constant and C is the capacitance of the circuit.

From the figure, the capacitance is given as 0.1 μF

.Substituting the values of τ and C in the above formula, we get:

R = (22 × 10⁻⁶ s) / (0.1 × 10⁻⁶ F)

R = 220 Ω

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Answer:

its 4 right

i hope it is

Answer:

im pretty positive its 4 , if not its 1

Explanation:

Ellie, the machine that can detect depression

Technology is an important channel to treat mental illness,

Abuse. Physical or emotional abuse can make you more vulnerable to depression later in life.

Age. People who are elderly are at higher risk of depression. That can be made worse by other factors, such as living alone and having a lack of social support.

Certain medications. Some drugs, such as isotretinoin (used to treat acne), the antiviral drug interferon-alpha, and corticosteroids, can increase your risk of depression.

Conflict. Depression in someone who has the biological vulnerability to it may result from personal conflicts or disputes with family members or friends.

Death or a loss. Sadness or grief after the death or loss of a loved one, though natural, can increase the risk of depression.

Gender. Women are about twice as likely as men to become depressed. No one's sure why. The hormonal changes that women go through at different times of their lives may play a role.

Genes. A family history of depression may increase the risk. It's thought that depression is a complex trait, meaning there are probably many different genes that each exert small effects, rather than a single gene that contributes to disease risk. The genetics of depression, like most psychiatric disorders, are not as simple or straightforward as in purely genetic diseases such as Huntington's chorea or cystic fibrosis.

Major events. Even good events such as starting a new job, graduating, or getting married can lead to depression. So can moving, losing a job or income, getting divorced, or retiring. However, the syndrome of clinical depression is never just a "normal" response to stressful life events.

Other personal problems. Problems such as social isolation due to other mental illnesses or being cast out of a family or social group can contribute to the risk of developing clinical depression.

Serious illnesses. Sometimes, depression happens along with a major illness or may be triggered by another medical condition.

Substance misuse. Nearly 30% of people with substance misuse problems also have major or clinical depression. Even if drugs or alcohol temporarily make you feel better, they ultimately will aggravate depression.

The displacement is 900 meter current to the South.

We know that velocity is the ratio of the displacement of a body to time. Displacement is a vector quantity just as velocity. We know that given the fact that velocity and displacement are vectors, the direction of the movement is very important.

Thus, we can see that;

Velocity =  3 meter/sec  current to the South

Time = 5 minutes or 300 sec

Velocity = displacement/ time

displacement = velocity * time

displacement = 3 meter/sec  current to the South *  300 sec

= 900 meter current to the South

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The radioactive decay equation is \(Th^{232} - > Ra^{228} + He^{4}\). The activity of 10 g of thorium, calculate the initial activity using the decay constant and the number of nuclei.  the activity after 10 years, use the radioactive decay law with the appropriate values.

a) The radioactive decay equation for thorium-232 (\(Th^{232}\)) can be represented as follows:

\(Th^{232} - > Ra^{228} + He^{4}\)

In this equation, thorium-232 decays into radium-228 and emits an alpha particle (helium-4 nucleus). This decay process occurs spontaneously over time.

b) To find the radioactive radiation activity of 10 g of thorium, we need to use the concept of activity, which represents the rate of decay of radioactive material. The activity (A) is given by the equation:

A = λ * N

Where λ is the decay constant and N is the number of radioactive nuclei present. The decay constant is related to the half-life (T1/2) of the isotope by the equation:

λ = ln(2) / T1/2

For thorium-232, with a half-life of 1.4 * \(10^{10}\) years, the decay constant is approximately λ = ln(2) / (1.4 * \(10^{10}\) years).

To find the number of radioactive nuclei (N) in 10 g of thorium, we can use Avogadro's number and the molar mass of thorium-232. The molar mass of thorium-232 is 232 g/mol, so we have:

N = (10 g) / (232 g/mol) * (6.022 * \(10^{23}\)nuclei/mol)

Now, we can calculate the activity (A) by substituting the values into the equation A = λ * N.

c) To find the activity after 10 years, we need to consider the radioactive decay law, which states that the activity of a radioactive substance decreases exponentially over time. The equation for the remaining activity (A_t) after time t is given by:

A_t = A_0 * e^(-λ * t)

Where A_0 is the initial activity at t = 0.

By substituting the appropriate values into the equation, including the initial activity calculated in part b, we can determine the activity after 10 years.

In summary, to find the radioactive radiation activity of thorium-232, we use the decay equation, the concept of activity, and the radioactive decay law. By applying these principles, we can calculate the initial activity of 10 g of thorium and determine the activity after a specified time, such as 10 years.

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Explanation:

Hope this helps,

Juno entered a polar orbit of Jupiter on July 5th 2016 UTC, to begin a scientific investigation of the planet. After completing its mission, Juno will be intentionally deorbited into Jupiters atmosphere. Junos mission is to measure Jupiters composition, gravitational field, magnetic field, and polar magnetosphere.

Answer:

1

3

4

5

or

a

c

d

e

Explanation:

We've got m/s, which is value of distance ÷ time

(distance/time)

3 x 10^8 is:

300,000,000m/s

1km = 1000m

1hr = 3600secs

So, divide 300,000,000m by 1000 to get in km & you get:

300,000km

Now divide this value by 3600 seconds to get it in km/hr

300,000km/3600 = 83.33333333

Thus, answer is 83.3km/h

Or

8.33 x 10^1 km/h (in standard form)

(doing 83.3 recurring multipled by 1000 & 3600 gets you back to original answer. So, 83.33333...x1000x3600= 300,000,000)

Hope this helps!

Use the formula for distance dropped from rest:

D = 1/2 a t^2 .

With no air resistance, you get about 8.8 sec.

I'm pretty sure you can fill in the missing work.

The value of the current flowing through the shunt is 0.08 A.

The value of the current flowing through the shunt is calculated by applying the following formula.

I = V/R

where;

The voltage flowing through the shunt is calculated as;

V/V'  = L/L'

where;

V/3 = 80/100

V = (3 x 80 ) / 100

V = 2.4 V

The current flowing through the shunt is calculated as;

I = 2.4 / 30

I = 0.08 A

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Answer: The spring constant of a given spring is \(40 N/m\).

Explanation:

Given,

Force (F) = 20N

The displacement of the spring\(= x = 0.5 m\)

To find: Spring constant (k) = ?

As we know that,

Hook's law states that,

\(F = k\) · \(x\)

Therefore, \(k = \frac{F}{x}\)

\(k = \frac{20}{0.5}\)

\(k = \frac{(20)(10)}{5}\)

\(k = 40 N/m\)

Hence, The spring constant of a given spring is \(40 N/m\).

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Answer:

In the NBA that's true

The maximum kinetic energy of an electron ejected by a photon with energy 3.31 eV from a metal with a work function of 1.56 eV is 2.8 × 10⁻¹⁹ Joule.

Given data:

Work Function of metal (Φ) = 1.56 eV = 1.56 × 1.6 × 10⁻¹⁹ Joule

Energy of the photon (E) = 3.31 eV = 3.31 × 1.6 × 10⁻¹⁹ Joule

We can calculate the maximum kinetic energy (K.E.) of the ejected electron using the equation:

K.E. = E - Φ

Substituting the values into the equation:

K.E. = 3.31 × 1.6 × 10⁻¹⁹ - 1.56 × 1.6 × 10⁻¹⁹

Simplifying the equation:

K.E. = (3.31 - 1.56) × 1.6 × 10⁻¹⁹

K.E. = 1.75 × 1.6 × 10⁻¹⁹ Joule

K.E. = 2.8 × 10⁻¹⁹ Joule

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Answer:

1.03 * 10^-5

Explanation:

The magnetic flux through the loop is approximately 1.317 × \(10^{(-5)\)T·m².

To calculate the magnetic flux through a loop, we use the formula:

Φ = B × A × cos(θ)

Where:

Φ is the magnetic flux

B is the magnetic field strength

A is the area of the loop

θ is the angle between the magnetic field and the normal to the loop

Given:

Magnetic field strength (B) = 3.09 × \(10^{(-4)\) T (east direction)

Area of the loop (A) = 0.0471 m²

The loop faces directly northeast

To find the angle θ,  determine the angle between the magnetic field direction (east) and the normal to the loop (northeast).

Since the loop faces northeast, the angle between the normal to the loop and the east direction is 45 degrees (90 degrees divided by 2).

Now calculate the magnetic flux:

Φ = B  × A  × cos(θ)

Φ = (3.09 × \(10^{(-4)\) T) × (0.0471 m²) × cos(45°)

Using the value of cos(45°) as 0.7071:

Φ = (3.09 × \(10^{(-4)\) T) × (0.0471 m²) ×0.7071

Φ = 1.317 × \(10^{(-5)\) T·m²

Therefore, the magnetic flux through the loop is approximately 1.317 × \(10^{(-5)\) T·m².

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Answer: The rocket spent 4 seconds accelerating is the answer to this question

Explanation:

Answer:

the answer is B. the rocket spent 4 seconds accelerating

Explanation:

I just took the test

hope this helps :)

To show that matrix A is diagonalizable, we need to demonstrate that there exists an invertible matrix P such that the diagonal matrix D is given by D = P^(-1)AP, where D represents the eigenvalues of A along its diagonal.

Given the matrix D =

```

1  6

0 -9

```

We can see that the eigenvalues of A are λ₁ = 1 and λ₂ = -9.

To find matrix P, we need to find the corresponding eigenvectors for each eigenvalue. Let's denote the eigenvector for λ₁ as v₁ and the eigenvector for λ₂ as v₂.

For λ₁ = 1, we solve the equation (A - λ₁I)v₁ = 0, where I is the identity matrix:

```

A - λ₁I =

1 -1  2

3 -5  0

(A - λ₁I)v₁ =

1 -1  2

3 -5  0  * v₁ = 0

This system of equations can be solved to find v₁ = [2, 1]ᵀ.

```

For λ₂ = -9, we solve the equation (A - λ₂I)v₂ = 0:

``

A - λ₂I =

1 -1  2

3 -5  0

(A - λ₂I)v₂ =

1 -1  2

3 -5  0  * v₂ = 0

This system of equations can be solved to find v₂ = [-1, 3]ᵀ.

``

Now that we have the eigenvectors v₁ and v₂, we can form matrix P using these vectors as columns:

```

P = [v₁, v₂] =

2 -1

1  3

```

Finally, we can calculate A^4 using the diagonalization method:

```

A^4 = (PDP^(-1))^4 = P D^4 P^(-1)

Since D is a diagonal matrix, we can simply raise each diagonal entry to the fourth power:

D^4 =

1^4  0

 0   (-9)^4

    =

1  0

0  6561

Therefore,

A^4 = P D^4 P^(-1) =

2 -1   *   1  0   *   2 -1

1  3       0  6561       1  3

       =

2 -1   *   2 -1   =   4 -2

1  3       1  3         5  7

```

Thus, A^4 is equal to the matrix

```

4 -2

5  7

```

This is the result obtained using the diagonalization method.

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Radiative energy is the energy carried by light.

What is radiative energy?

Radiative energy is the energy carried by light. It is a form of energy that can be transmitted through space without requiring a medium for it to move through. Radiative energy can come from natural sources like the sun or artificial sources like light bulbs.

Radiative energy is important for a variety of reasons. For one thing, it is the primary source of energy for many living organisms on Earth, particularly plants. Energy from the sun helps plants photosynthesize and produce food that they can use to grow and reproduce.

Radiative energy is also important for human life. It is used in a variety of ways, including in the form of light for illuminating spaces and in the form of heat for cooking and keeping warm. Understanding the nature and properties of radiative energy is important for a wide range of scientific and technological fields.

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