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Ch.6 - Electronic Structure of Atoms

Chapter 6, Problem 33b

Molybdenum metal must absorb radiation with an energy higher than 7.22 * 10-19 J ('energy threshold') before it can eject an electron from its surface via the photoelectric effect. (b) What wavelength of radiation will provide a photon of this energy?

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Hey everyone in this example, we need to calculate the wavelength of radiation that will provide a photon that would reach the energy threshold of iron at this value given. So we're going to begin by recalling our formula for the energy of a photon, which we would recall is equal to Planck's constant, multiplied by our frequency. We also want to recall our formula where wavelength is equal to our speed of light divided by frequency. So we first need to find frequency. So we're going to reinterpret our formula for energy of a photon and say that that's equal to our energy divided by plank's constant. So finding frequency according to the info and are pumped. We would say that frequency is equal to Our energy threshold given in the prompt is 6.878 times 10 to the negative 19th power jewels. And we're dividing this by plank's constant, which we recall is 6.626 times 10 to the 23rd power or sorry to the negative 34th power jules times seconds. So now we're able to cancel out jewels were left with inverse seconds for frequency which is the proper unit. And this gives us a value equal to 1.03, 8 times 10 to the positive 15th power in units of inverse seconds. So this is step one of our solution. And now we're going to move on to step two to find our wavelength. So we should recall that in our numerator, our speed of light is equal to a value of 2.998 Times 10 to the 8th power m/s. And then in our denominator we're going to recall that Our frequency, which we just calculated above is equal to 1.38 times 10 to the 15th power inverse seconds. So we're able to cancel out inverse seconds with seconds were left with meters as our unit for wavelength. And we get our final value for wavelength equal to 2.888 times 10 to the negative seventh power meters. So this was step two of our solution and this was our final answer for our wavelength of radiation. That gives our photon the energy threshold of 6.87, 8 times 10 to the negative 19th power jewels. So what's boxed in is our final answers? If you have any questions, please leave them down below and I will see everyone in the next practice video.
Related Practice
Textbook Question

A diode laser emits at a wavelength of 987 nm. (a) In what portion of the electromagnetic spectrum is this radiation found? (b) All of its output energy is absorbed in a detector that measures a total energy of 0.52 J over a period of 32 s. How many photons per second are being emitted by the laser?

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Textbook Question

A stellar object is emitting radiation at 3.0 mm. (a) What type of electromagnetic spectrum is this radiation (b) If a detector is capturing 3.0 3 108 photons per second at this wavelength, what is the total energy of the photons detected in 1 day?

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Textbook Question

Molybdenum metal must absorb radiation with an energy higher than 7.22 * 10-19 J ('energy threshold') before it can eject an electron from its surface via the photoelectric effect. (a) What is the frequency threshold for emission of electrons?

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Textbook Question

Molybdenum metal must absorb radiation with an energy higher than 7.22 * 10-19 J ('energy threshold') before it can eject an electron from its surface via the photoelectric effect. (c) If molybdenum is irradiated with light of wavelength of 240 nm, what is the maximum possible velocity of the emitted electrons?

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Textbook Question

Does the hydrogen atom 'expand' or 'contract' when an electron is excited from the n = 1 state to the n = 3 state?

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Textbook Question

Classify each of the following statements as either true or false: (a) A hydrogen atom in the n = 3 state can emit light at only two specific wavelengths (b) a hydrogen atom in the n = 2 state is at a lower energy than one in the n = 1 state (c) the energy of an emitted photon equals the energy difference of the two states involved in the emission.

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