where is the string experiencing maximum oscillation amplitude (anti-node location) and where is the string experiencing minimum, or zero, oscillation amplitude (node location)?

The lamppost is approximately 11.69 feet high.

To find the height of the lamppost, you can use the tangent function in trigonometry. Given the angle of elevation (33°) and the shadow length (18 feet), you can set up the equation:

tan(33°) = height / 18 feet

To solve for the height, multiply both sides by 18 feet:

height = 18 feet * tan(33°)

Using a calculator to find the tangent of 33°:

height ≈ 18 feet * 0.6494

height ≈ 11.69 feet

Therefore, the lamppost is approximately 11.69 feet high.

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The decay of radium is exponential, so we can use the following equation to calculate the amount remaining after a given time.after 6480 years, you would have 4 grams of radium remaining.

Radium is a radioactive element with the symbol Ra and atomic number 88. It is an alkaline earth metal that is silvery-white in color and tarnishes rapidly in air. Radium is highly radioactive and is one of the most dangerous and toxic elements known. Its most stable isotope, radium-226, has a half-life of 1600 years and decays into radon gas, which is also radioactive and poses a significant health risk. Radium was once used in luminous paint, but due to its health hazards, its use has been discontinued. It is still used in some medical applications, such as cancer treatment, but its use is strictly controlled.

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To find the focal length of a mirror or lens, the light source should be located at a distance greater than or equal to the focal length. When light rays pass through a converging lens or reflect off a concave mirror, they converge at a point called the focal point.

The distance between the focal point and the lens or mirror is known as the focal length. To measure the focal length accurately, the light source should be placed at a distance greater than or equal to the focal length.  Placing the light source closer than the focal length would result in a diverging beam of light, making it difficult to measure the focal length accurately.

On the other hand, placing the light source further than the focal length would cause the light rays to converge at a point beyond the measuring apparatus, again making it difficult to determine the focal length. Therefore, the light source should be located at a distance equal to or greater than the focal length for accurate measurement.

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The weight of the atmosphere pressing down on the table is given by the product of the atmospheric pressure and the area of the table. Therefore, the weight of the atmosphere pressing down on the table is 4.0 x 10^5 N.

The atmospheric pressure is the force per unit area exerted by the weight of the atmosphere. In this case, the atmospheric pressure is 1.0 x 10^5 N/m^2. Multiplying this pressure by the area of the table (1.6 m x 2.5 m) gives the weight of the atmosphere pressing down on the table, which is 4.0 x 10^5 N. This weight is distributed evenly over the entire surface of the table, so each square meter of the table is subjected to a force of 1.0 x 10^5 N, which is the atmospheric pressure.

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The process of an automobile heating up while sitting in a parking lot on a sunny day can be assumed to be an isobaric process.The correct answer is: A. Isobaric


An isobaric process occurs when the pressure remains constant while other properties change. In the case of an automobile heating up in a parking lot, the pressure inside the car remains roughly constant, even as the temperature increases due to the sun's heat.

An isothermal process, on the other hand, is when the temperature remains constant while other properties change. This is not the case for the automobile scenario since the temperature inside the car increases as it absorbs the sun's heat. Therefore, the process is not isothermal.

In conclusion, the process of an automobile heating up while sitting in a parking lot on a sunny day can be assumed to be an isobaric process.

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The foreman shouts at John to hurry up and he increases his pushing force to 50N. Calculate the wheelbarrow's acceleration. When the foreman shouts at John to hurry up and John increases his pushing force to 50N, the wheelbarrow's acceleration can be calculated as follows:

F = 50N and m = 20 kg. Now, the acceleration of the wheelbarrow can be calculated using the formula below;

F = m × a, Where, F is the force applied, m is the mass of the object and, a is the acceleration of the object.

Rearranging the formula, we have; a = F/m.

Substituting the values in the formula; a = 50/20a = 2.5 m/s².

Therefore, the wheelbarrow's acceleration is 2.5 m/s².

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For an observer located on the North Pole, the altitude of the stars in the East will (c) stay the same.

This is because the North Pole is located at the Earth's axis, which is perpendicular to the plane of the Earth's orbit. As a result, the North Pole is constantly pointed towards the same region of space, and the stars in the East will always be at the same altitude.
This is different from what would be observed at other latitudes on Earth. For example, an observer at the Equator would see the stars in the East rise and set over the course of a day, as the Earth rotates on its axis. Similarly, an observer at a mid-latitude would see the stars in the East rise at an increasing altitude, reach their highest point in the sky, and then decrease in altitude as they set in the West.
However, at the North Pole, the stars in the East will appear to circle around the observer at a constant altitude, never rising or setting. This can make navigation and timekeeping more challenging, as there are no clear markers for the passage of time or changes in direction. Nevertheless, this unique perspective on the stars can also be a source of wonder and inspiration, as the observer is able to witness the timeless dance of the heavens from a truly unique vantage point.

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The differences among the terms "observable universe expanding", "universe expanding", and "universe's expansion accelerating" are as follows:

1. "Observable universe expanding" refers to the growth of the portion of the universe that we can observe and gather information from. This is due to the ongoing expansion of the universe, which causes objects within the observable universe to move away from us, increasing the size of the region we can detect.

2. "Universe expanding" describes the overall increase in size of the entire universe, including both observable and unobservable regions. This expansion occurs as a result of the Big Bang and the subsequent stretching of space, causing galaxies and other cosmic structures to move apart from one another.

3. "Universe's expansion accelerating" refers to the observation that the rate at which the universe is expanding is not constant but is instead increasing over time. This acceleration is attributed to dark energy, a mysterious form of energy that works against gravity and drives the universe to expand at a faster pace.

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At t=0, the voltage v(t) across the inductor and the current i(t) through the inductor experience an abrupt change and may become discontinuous, as the initial energy stored in the inductor is released and the current and voltage begin to change from their initial values.

More specifically, prior to t=0, the current i(t) was assumed to be zero, and the voltage v(t) across the inductor was also zero, as there was no change in current flowing through the inductor. However, at t=0, when the voltage source is connected to the circuit, the current starts to flow, and the voltage across the inductor changes abruptly, leading to a change in current.

The amount of change in current and voltage depends on the inductance of the inductor and the other circuit parameters. In general, the current and voltage may oscillate or decay towards steady-state values depending on the circuit parameters.

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The period of the pendulum is 1.59 seconds and its length is 0.623 meters.

The first step in solving this problem is to understand the terms being used. A pendulum is an object that swings back and forth on a fixed axis. The oscillations of a pendulum are repeated back-and-forth movements. The period of a pendulum is the time it takes for one complete oscillation.

Given that the pendulum makes 136 complete oscillations in 3.60 min, we can use this information to calculate the period. We know that the time it takes for 136 oscillations is 3.60 min, so we can divide 3.60 by 136 to find the time it takes for one oscillation. This gives us a period of 0.0265 min (or 1.59 seconds).

Next, we can use the period to find the length of the pendulum. The formula for the period of a simple pendulum is T = 2π√(L/g), where T is the period, L is the length of the pendulum, and g is the acceleration due to gravity. We know the period (1.59 seconds) and the value of g (9.80 m/s2), so we can rearrange the formula to solve for L.

T = 2π√(L/g)
1.59 = 2π√(L/9.80)
1.59/2π = √(L/9.80)
0.252 = √(L/9.80)
0.252^2 = L/9.80
0.0635 = L/9.80
L = 0.623 meters (or 62.3 centimeters)

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The frequency of the orange light is 4.6 x 10^14 sec^-1. To calculate the frequency, we can use the formula:  frequency = speed of light / wavelength. The speed of light is approximately 3 x 10^8 m/s. However, we need to convert the wavelength from nm to m by multiplying it by 10^-9. So,

frequency = (3 x 10^8 m/s) / (650 x 10^-9 m)
frequency = 4.6 x 10^14 sec^-1

To find the frequency of the orange light with a wavelength of 650 nm, we will use the formula:

Frequency (f) = Speed of Light (c) / Wavelength (λ)

First, we need to convert the given wavelength from nanometers (nm) to meters (m) using the conversion factor 1 nm = 10^-9 m:

650 nm * (10^-9 m/nm) = 6.50 * 10^-7 m

Now, we will use the speed of light (c), which is approximately 3.00 * 10^8 m/s:

f = (3.00 * 10^8 m/s) / (6.50 * 10^-7 m)

After dividing, we get:

f ≈ 4.62 * 10^14 sec^-1

So, the frequency of this particular color of orange light is approximately 4.62 * 10^14 sec^-1.

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The largest axial force P that can be applied without causing the W14 X 30 A992 steel column to buckle is approximately 345 kips.

To determine the largest axial force P that can be applied to the W14 X 30 A992 steel column without causing it to buckle, we need to use the Euler buckling formula. This formula takes into account the column's length, its end conditions, and its cross-sectional area. Assuming the column is pinned at both ends, its effective length will be equal to its actual length, which is 30 feet in this case. We can then calculate its critical buckling load using the formula:
Pcr = (π²EI) / (Kl)²
Where Pcr is the critical load, E is the modulus of elasticity for A992 steel, I is the moment of inertia of the W14 X 30 section, K is the effective length factor (which is equal to 1.0 for pinned-pinned columns), and l is the length of the column. Using the values for E and I for A992 steel, we can calculate the critical load to be approximately 345 kips.
To determine the largest axial force P that can be applied without causing buckling, we need to ensure that P is less than Pcr. Based on the critical load calculation, we can conclude that the largest axial force P that can be applied without causing the W14 X 30 A992 steel column to buckle is approximately 345 kips.

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A B-52 aircraft is a physical good that is used by the United States military in armed conflict. Specifically, it is a type of bomber aircraft that is designed for long-range strategic bombing missions.

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The torque exerted by the object on the wheel is equal to (ms * wo * cit) / R.

The torque exerted by the self-propelled object on the wagon wheel is dependent on several variables including the mass of the object, its distance from the axle, the initial angular velocity of the wheel, and the radius of the wheel.

To calculate the torque, we can use the equation T = I * alpha, where T is the torque, I is the moment of inertia, and alpha is the angular acceleration.

Since the object is moving along a spoke, we need to find the component of its motion that is perpendicular to the radius of the wheel.

Using trigonometry, we can determine that the distance from the axle to the object is cit * sin(theta), where theta is the angle between the spoke and the radius.

Thus, the torque is equal to (ms * wo * cit * sin(theta)) / R, where ms is the mass of the object, wo is the initial angular velocity of the wheel, and R is the radius of the wheel.

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We would need to find a concave lens with a power of -0.37 diopters and place it in front of the person's eye. This lens would diverge the incoming light rays and reduce the refractive power of the eye, allowing the light to focus correctly on the retina and correcting the person's near-sightedness.

To correct the vision of a near-sighted person with a maximum clear distance of 37 cm, we need to design a concave lens that will diverge the light rays before they enter the eye, so that they will focus correctly on the retina.

The strength of the lens required to correct the vision depends on the refractive power of the eye, which is measured in diopters. A near-sighted person has too much refractive power, which causes the light rays to focus in front of the retina, resulting in a blurry image.

To correct this, we need to add a negative lens (concave lens) in front of the eye that will reduce the total refractive power. The strength of the lens needed can be calculated using the formula:

Lens power (in diopters) = 1 / focal length (in meters)

Since the person can only see clearly up to a distance of 37 cm, the focal length of the lens needed is:

focal length = 1 / (dmax / 100) = 1 / 0.37 = 2.70 meters

Therefore, the lens power required to correct the near-sightedness is:

Lens power = 1 / focal length = 1 / 2.70 = 0.37 diopters

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To correct the vision of a near-sighted person who can only see objects clearly up to a maximum distance of d max = 37 cm, a concave lens would be required.

This type of lens diverges light rays and causes them to spread out, which corrects the near-sightedness. The strength of the lens would need to be calculated based on the distance of the object that the person wants to see clearly. For example, if the person wants to see an object at a distance of 50 cm, a lens with a strength of -2.5 diopters would be needed. It is important to note that the lens can only correct vision up to a certain point, and the person may still need to wear corrective lenses for distant vision beyond their dmax.
To design a lens to correct the vision of a near-sighted person with a maximum clear distance (dmax) of 37 cm, follow these steps:
1. Identify the person's maximum clear distance: In this case, dmax = 37 cm.
2. Determine the focal length (f) needed to correct their vision: Use the formula 1/f = 1/dmax. In this case, 1/f = 1/37 cm.
3. Calculate the focal length (f): Solve the equation from step 2 to find f. In this case, f = 37 cm.
4. Choose a lens with a negative focal length: Since the person is near-sighted, you'll need a diverging lens with a negative focal length. In this case, choose a lens with a focal length of -37 cm.
To summarize, to correct the vision of a person with a dmax of 37 cm, you would need a diverging lens with a focal length of -37 cm. This lens will help the person see objects clearly at a greater distance.

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If x=15cm, the laser beam will refract back into the air through side b.

Refraction occurs when a light beam passes through a boundary between two different mediums at an angle. In this case, the laser beam is traveling from water (with a refractive index of 1.33) to air (with a refractive index of 1.00) through the glass block. The angle of incidence at side a will be greater than the critical angle (approximately 48.75 degrees), causing the beam to refract back into the air through side b. Reflection would occur if the angle of incidence was less than the critical angle, but in this scenario, the angle is greater.

The laser beam will refract back into the air through side b. When a laser beam travels from one medium to another with different refractive indices, such as from water to air, it will experience refraction. In this case, as the laser beam moves from the denser medium (water) to the less dense medium (air) through side b, the beam will refract away from the normal, allowing it to pass back into the air.

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It's worth noting that the mean time between collisions is just an average value, and individual electrons may go longer or shorter periods of time without colliding.

The mean time between collisions for electrons in a gold wire is 25 femtoseconds (fs), which is a very short amount of time. To give some perspective, 1 fs is one quadrillionth (or one millionth of one billionth) of a second. This means that, on average, an electron in a gold wire collides with another particle every 25 fs.

This short time period is due to the fact that electrons in a wire are constantly colliding with atoms and other particles in their surroundings. These collisions can result in energy transfer, resistance, and other effects that can impact the behavior of the wire.

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The sample is approximately 1785 years old.

Carbon dating is a technique used to determine the age of organic materials. Carbon-14 is a radioactive isotope of carbon that decays at a known rate over time, and by measuring the amount of carbon-14 in a sample, scientists can determine its age.

In this case, the sample of charcoal contains 65.0% of carbon, and we know that carbon-14 decays at a rate of 0.897 per 5,700 years. Using the formula for exponential decay, we can calculate the age of the sample:

Solving for t, we get:

Therefore, the sample is approximately 1785 years old.

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To find the binding energy of the nucleus 30ne, we need to use the formula:

Binding energy = (mass of neutral atom - mass of nucleus) x [tex]c^{2}[/tex]

where c is the speed of light.

The mass of the neutral atom can be calculated by adding the atomic mass (which includes the electrons) and the atomic number (which is the number of protons) of neon, which is 20.

So, the mass of the neutral atom is:

20 + 20.1797 = 40.1797 u

Now we can calculate the binding energy:

Binding energy =[tex](40.1797 - 30.0192) × (3.00 × 10^{8} )^2[/tex]

Binding energy =[tex]1.08 × 10^{-10} J[/tex]

Therefore, the binding energy of the nucleus 30ne is [tex]1.08 × 10^{-10} J[/tex]

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The current in the microwave is 10 amps.

To calculate the current in the microwave, we need to use Ohm's law, which states that current (I) is equal to voltage (V) divided by resistance (R). In this case, the resistance is the impedance of the microwave, which we can calculate using the formula: impedance (Z) = voltage (V) / current (I).

First, we need to convert the wattage rating of the microwave to its apparent power, which is given by the formula: apparent power (S) = voltage (V) x current (I).

So, for a microwave rated at 1,200 watts and receiving 120 volts of potential difference, the apparent power is:

S = V x I
1,200 = 120 x I
I = 1,200 / 120
I = 10 amps

Therefore, the current in the microwave is 10 amps.

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When a straightened wire coat hanger is spun in the Earth's magnetic field, an electromotive force (EMF) can be generated. This answer provides an estimation of the EMF that can be produced.

When the wire coat hanger is spun in the Earth's magnetic field, it creates a changing magnetic flux through the triangular loop formed by the wire. According to Faraday's law of electromagnetic induction, this changing magnetic flux induces an electromotive force (EMF) in the loop. The EMF can be estimated using the equation EMF = -N(dΦ/dt), where N is the number of turns in the loop and dΦ/dt is the rate of change of magnetic flux.

In this case, the wire coat hanger forms a single-turn loop, and the magnetic field strength of the Earth is approximately [tex]5 * 10^-^5[/tex] T. Assuming a reasonable spinning speed, we can estimate a rate of change of magnetic flux. Plugging in these values into the equation, we can calculate an approximate value for the EMF generated by the spinning hanger.

It's important to note that this is a simplified estimation and various factors such as the exact shape of the hanger, its orientation, and the speed of spinning can affect the actual EMF generated. For a more precise calculation, one would need to consider these factors and apply more complex mathematical models.

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The provided equation represents the transition rate for an electric dipole transition of an atom between an initial state, i, and a final state, f, through the absorption of electromagnetic radiation.

The transition rate, Wf, is given by the product of the electric dipole transition moment, dij, and the spectral density of the electromagnetic radiation, plw).

The spectral density, plw), is multiplied by the polarization vector of the electromagnetic radiation, e, and is integrated over all wavelengths, w. The difference in energy between the final state, EF, and the initial state, Ei, is divided by Planck's constant, ħ, and is denoted by wfi.

The electric dipole transition moment, dij, is given by the dot product of the electric field vector of the electromagnetic radiation, E, and the position vector of the electron, r, associated with the electric dipole transition.

The transition rate, Wf, represents the probability per unit time of the atom making the transition from the initial state to the final state.

This equation is important in describing various physical phenomena, such as absorption spectra in atomic and molecular physics, and is useful in the development of technologies such as lasers and spectroscopy.

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The waves with the longest wavelengths in the electromagnetic spectrum are radio waves.

Radio waves have wavelengths ranging from about 1 millimeter to over 100 kilometers. These waves are used for various forms of communication, such as broadcasting radio and television signals. Due to their long wavelengths, radio waves have low frequencies and carry less energy compared to other waves in the spectrum, like visible light or X-rays. Their long wavelengths allow them to propagate over long distances and penetrate obstacles like buildings, making them suitable for long-range communication. Additionally, radio waves are used in radar systems, satellite communication, and wireless networking.

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The 83.0 kg person absorbed approximately 2.2×10⁻⁵ γ rays with an energy of 3.30×10⁻¹⁴ J and an RBE of 1.

The calculation to determine the number of γ rays absorbed by an 83.0 kg person with an exposure primarily in the form of γ rays with an energy of 3.30×10⁻¹⁴ J and an rbe of 1 requires a few steps. First, we need to convert the energy of the γ ray to joules per kilogram (J/kg) using the conversion factor of 1 Gy = 1 J/kg. This gives us an absorbed dose of 3.30×10⁻¹⁴ Gy.

Next, we need to determine the number of γ rays absorbed by the person by using the equation:

Number of γ rays absorbed = Absorbed dose (Gy) / Absorbed dose per γ ray (Gy/γ)

The absorbed dose per γ ray is the energy deposited by one γ ray in a specific material and can be found in tables. For example, for water, the absorbed dose per γ ray with an energy of 3.30×10⁻¹⁴ J is approximately 1.5×10–9 Gy/γ.

Using this information, we can calculate the number of γ rays absorbed by the person:

Number of γ rays absorbed = 3.30×10⁻¹⁴ Gy / (1.5×10⁻⁹ Gy/γ) = 2.2×10⁻⁵ γ rays

Therefore, the 83.0 kg person absorbed approximately 2.2×10⁻⁵ γ rays with an energy of 3.30×10⁻¹⁴ J and an RBE of 1. This is a very small number, highlighting the fact that the effects of ionizing radiation are typically measured in terms of absorbed dose rather than the number of particles or photons absorbed.

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True. Experiments can measure not only whether a compound is paramagnetic, but also the number of unpaired electrons.

Paramagnetic substances are those that contain unpaired electrons, leading to an attraction to an external magnetic field. To determine if a compound is paramagnetic and to measure the number of unpaired electrons, various experimental techniques can be employed. One common method is Electron Paramagnetic Resonance (EPR) spectroscopy, also known as Electron Spin Resonance (ESR) spectroscopy.

EPR spectroscopy is a powerful tool for detecting and characterizing species with unpaired electrons, such as free radicals, transition metal ions, and some rare earth ions. This technique works by applying a magnetic field to the sample and then measuring the absorption of microwave radiation by the unpaired electrons as they undergo transitions between different energy levels.

The resulting EPR spectrum provides information about the electronic structure of the paramagnetic species, allowing researchers to determine the number of unpaired electrons present and other characteristics, such as their spin state and the local environment surrounding the unpaired electrons. In this way, EPR spectroscopy can provide valuable insights into the nature of paramagnetic compounds and their role in various chemical and biological processes.

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The angle is measured relative to the original direction of the beam.

The total number of bright fringes can be determined using the formula:

N = (d sin θ)/λ

where d is the distance between the slits, λ is the wavelength of the light, and θ is the angle between the central bright fringe and the nth bright fringe.

The maximum value of sin θ is 1, which occurs when θ = 90 degrees. Thus, the maximum value of m (the number of bright fringes on one side of the central fringe) is given by:

m_max = (d/λ)sin θ_max = (0.010 mm/633 nm)(1) = 15.8

Therefore, the total number of bright fringes on both sides of the central fringe, including the central fringe itself, is:

N = 2m_max + 1 = 2(15.8) + 1 = 31.6 + 1 = 32.6

So there are a total of 32.6 bright fringes.

(b) The angle of the nth bright fringe is given by:

θ = sin^-1(nλ/d)

The fringe that is most distant from the central bright fringe corresponds to the largest value of n. We can find this value using the fact that sin θ cannot be greater than 1, so we have:

nλ/d ≤ 1

n ≤ d/λ

n_max = int(d/λ) = int(0.010 mm/633 nm) = int(15.8) = 15

Therefore, the fringe that is most distant from the central bright fringe occurs at an angle:

θ_max = sin^-1(n_maxλ/d) = sin^-1(15(633 nm)/0.010 mm) = 54.4 degrees

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The gradient at B is zero because the rocket's velocity changes from positive to zero, and the shaded areas above and below the time axis are equal. If the rocket opens a parachute at B, its speed decreases gradually until it reaches the ground.

(a) (i) The gradient of the graph at B is zero.

(ii) The gradient has this value at B because the velocity of the rocket is changing from positive (upward) to zero at its maximum height.

The shaded areas above and below the time axis are equal. The area above the time axis represents the increase in the rocket's potential energy as it gains height, while the area below the time axis represents the decrease in its kinetic energy due to air resistance.

If the rocket opens a parachute at point B, its speed will decrease gradually until it reaches the ground.

The speed-time graph of the rocket with the parachute will show a shallow slope, indicating a gradual decrease in speed over time. This slope will become steeper as the rocket approaches the ground, until it reaches a speed of zero at E.

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The average power delivered by the ideal current source is zero.

Since the circuit contains only passive elements (resistors and capacitors), the average power delivered by the ideal current source must be zero, as passive elements only consume power and do not generate it. The average power delivered by the current source can be calculated using the formula:

where T is the period of the waveform, and p(t) is the instantaneous power delivered by the source. For a sinusoidal current waveform, the instantaneous power is given by:

where R is the resistance in the circuit.

Substituting the given current waveform, we get:

Integrating this over one period, we get:

Hence, the average power delivered by the ideal current source is zero.

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As no specific power series is given, it is impossible to determine the convergence set. The convergence set of a power series depends on its coefficients and the variable it is being evaluated at. The convergence set can be determined using various tests such as the ratio test, root test, or comparison test. The radius of convergence can also be found using the ratio or root test. If the convergence set is the entire real line, the power series is said to converge everywhere, while if it is empty, the power series does not converge anywhere.

In summary, the convergence set of a power series depends on its coefficients and variable. Various tests can be used to determine the convergence set, and if the set is the entire real line, the power series converges everywhere, while if it is empty, the power series does not converge anywhere.

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The correct option is a. The work done by the gas is 1.2 x 10^{4} J.

To calculate the work done by an ideal gas during a constant pressure expansion, we use the formula W = P * ΔV, where W represents work, P is the constant pressure, and ΔV is the change in volume. In this case, P = 4 x 10^{5} Pa, and ΔV = 0.050 m^{3} - 0.020 m^{3} = 0.030 m^{3}. Plugging these values into the formula, we get W = (4 x 10^{5} Pa) * (0.030 m^{3}), which results in W = 1.2 x 10^{4} J. Therefore, the work done by the gas is 1.2 x 10^{4} J, and the correct option is a.

Calculation steps:
1. Determine ΔV: ΔV = 0.050 m^{3} - 0.020 m^{3} = 0.030 m^{3}
2. Apply the formula W = P * ΔV: W = (4 x 10^{5} Pa) * (0.030 m^{3})
3. Calculate W: W = 1.2 x 10^{4} J

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