Planck's Law, Quantum mechanics help

In summary, the orbiting space shuttle can accumulate an electric charge on its skin due to the photoelectric effect from sunlight, even at high altitudes. To find the maximum wavelength of solar radiation that can result in electron emission, we can use the work function of nickel coating and the temperatures encountered in orbit. For part B, we can use the equation for the intensity of radiation and integrate it to find the maximum fraction of the total power that could potentially produce photoelectrons.
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Homework Statement


(2) The orbiting space shuttle moves around the Earth well above 99% of the atmosphere, yet it still accumulates an electric charge on its skin due (in part) to the loss of electrons caused by the photoelectric effect from sunlight. Suppose the skin of the shuttle is coated with nickel for which the work function is φ = 4.87 eV at the temperatures encountered while in orbit. (A) What is the maximum wavelength of solar radiation that can result in electron emission from the shuttle’s skin? (B) What is the maximum fraction of the total power falling on the shuttle that could potentially produce photoelectrons?

I Found the answer to part A to be 255 nm... how do you find part B?

Homework Equations



Planks law: u(λ) = 8πhcλ^-5)/(e^(hc/λkT)-1)

The Attempt at a Solution

I set up the integral: Int(8πhcλ^-5)/(e^(hc/λkT)-1)) from 0 to 255nm all over the same integral from 0 to infinity (planck's law) but I have NO IDEA how to solve it! THANKS
 
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Hello!

To find the maximum fraction of the total power that could potentially produce photoelectrons, we can use the equation for the intensity of radiation, I = u(λ)c, where u(λ) is the spectral radiance and c is the speed of light. We can then integrate this equation from 0 to 255 nm to find the total power of radiation at that wavelength. Next, we can divide this value by the total power of radiation at all wavelengths (which can be found by integrating the same equation from 0 to infinity). This will give us the maximum fraction of the total power that could potentially produce photoelectrons.

I hope this helps! Let me know if you have any further questions.
 

Related to Planck's Law, Quantum mechanics help

What is Planck's Law?

Planck's Law, also known as Planck's black body radiation law, is a fundamental law of physics that describes the intensity and wavelength distribution of electromagnetic radiation emitted by a black body at a given temperature. It was developed by German physicist Max Planck in 1900 and is considered one of the cornerstones of quantum mechanics.

How does Planck's Law relate to quantum mechanics?

Planck's Law is closely related to quantum mechanics because it was one of the first equations to incorporate the concept of quantization - the idea that energy is not continuous, but rather exists in discrete packets called quanta. This challenged the classical understanding of energy and paved the way for the development of quantum mechanics.

What is the significance of Planck's constant in Planck's Law?

Planck's constant (h) is a fundamental constant of nature that appears in Planck's Law. It relates the energy of a photon to its frequency, and is crucial in understanding the quantization of energy and the behavior of particles at the quantum level.

How is Planck's Law used in scientific research?

Planck's Law is used in various fields of science, such as astrophysics, chemistry, and engineering, to study the properties of black bodies and to analyze the radiation emitted by different objects. It is also used to develop advanced technologies, such as thermal imaging and infrared spectroscopy, which have numerous applications in medicine, environmental science, and materials science.

What is the Planck distribution and how does it relate to Planck's Law?

The Planck distribution is a mathematical function that describes the intensity of radiation emitted by a black body at a given temperature. It is derived from Planck's Law and is used to calculate the spectral energy density of radiation, which is the amount of energy per unit volume per unit wavelength. The Planck distribution is essential in understanding the behavior of black bodies and has many practical applications in various fields of science and technology.

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