/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 62 An owl has good night vision bec... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

An owl has good night vision because its eyes can detect a light intensity as faint as \(5.0 \times 10^{-13} \mathrm{W} / \mathrm{m}^{2} .\) What is the minimum number of photons per second that an owl eye can detect if its pupil has a diameter of \(8.5 \mathrm{mm}\) and the light has a wavelength of $510 \mathrm{nm} ?$

Short Answer

Expert verified
Answer: _________________

Step by step solution

01

Calculate the area of the owl's pupil

First, let's find the area of the owl's pupil using the given diameter. The formula for the area of a circle is: \(A = \pi r^{2}\), where A is the area and r is the radius. We need to convert the diameter to radius by dividing by 2. So, \(r = \frac{8.5 \mathrm{mm}}{2} = 4.25 \mathrm{mm}\). Now we need to convert the radius to meters: \(r = 4.25 \times 10^{-3} \mathrm{m}\). Now, we can calculate the area: \(A = \pi (4.25 \times 10^{-3})^{2} \mathrm{m^2}\).
02

Find the energy of each photon

To find the energy of each photon, we can use the formula: \(E = \frac{hc}{\lambda}\), where E is the energy, h is the Planck's constant (\(6.63 \times 10^{-34} \mathrm{Js}\)), c is the speed of light (\(3 \times 10^8 \mathrm{m/s}\)), and λ is the wavelength. We are given λ = \(510 \mathrm{nm}\). First, we need to convert it to meters: \(\lambda = 510 \times 10^{-9} \mathrm{m}\). Now, we can calculate the energy of each photon: \(E = \frac{6.63 \times 10^{-34} \mathrm{Js} \times 3 \times 10^8 \mathrm{m/s}}{510 \times 10^{-9} \mathrm{m}}\).
03

Calculate the number of photons detected per second

Now, we need to calculate the number of photons detected per second. We can do this by dividing the light intensity by the energy per photon and then multiplying by the area of the pupil. The formula is: \(N = \frac{I \times A}{E}\), where N is the number of photons per second, I is the light intensity, A is the area of the pupil, and E is the energy per photon. We have \(I = 5.0 \times 10^{-13} \mathrm{W/m^2}\), A from Step 1 and E from Step 2. Now, we can calculate the number of photons detected per second: \(N = \frac{5.0 \times 10^{-13} \mathrm{W/m^2} \times \pi (4.25 \times 10^{-3})^{2} \mathrm{m^2}}{E}\). To find the minimum number of photons, round up the result to the nearest whole number.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Two different monochromatic light sources, one yellow \((580 \mathrm{nm})\) and one violet \((425 \mathrm{nm}),\) are used in a photoelectric effect experiment. The metal surface has a photoelectric threshold frequency of $6.20 \times 10^{14} \mathrm{Hz}$. (a) Are both sources able to eject photoelectrons from the metal? Explain. (b) How much energy is required to eject an electron from the metal? (Use \(h=4.136 \times\) \(10^{-15} \mathrm{eV} \cdot \mathrm{s} .\)
A \(100-\) W lightbulb radiates visible light at a rate of about $10 \mathrm{W} ;$ the rest of the EM radiation is mostly infrared. Assume that the lightbulb radiates uniformly in all directions. Under ideal conditions, the eye can see the lightbulb if at least 20 visible photons per second enter a dark-adapted eye with a pupil diameter of \(7 \mathrm{mm}.\) (a) Estimate how far from the source the lightbulb can be seen under these rather extreme conditions. Assume an average wavelength of 600 nm. (b) Why do we not normally see lightbulbs at anywhere near this distance?
Find the wavelength of the radiation emitted when a hydrogen atom makes a transition from the \(n=6\) to the \(n=3\) state. $(\text {tutorial: hydrogen atom })$
What is the energy of a photon of light of wavelength \(0.70 \mu \mathrm{m} ?\)
Follow the steps outlined in this problem to estimate the time lag (predicted classically but not observed experimentally) in the photoelectric effect. Let the intensity of the incident radiation be $0.01 \mathrm{W} / \mathrm{m}^{2} .\( (a) If the area of the atom is \)(0.1 \mathrm{nm})^{2},$ find the energy per second falling on the atom. (b) If the work function is 2.0 eV, how long would it take (classically) for enough energy to fall on this area to liberate one photoelectron? (c) Explain briefly, using the photon model, why this time lag is not observed.
See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.