University Physics with Modern Physics, Books a la Carte Edition; Modified MasteringPhysics with Pearson eText -- ValuePack Access Card -- for ... eText -- Valuepack Access Card (14th Edition)
14th Edition
ISBN: 9780134308142
Author: Hugh D. Young, Roger A. Freedman
Publisher: PEARSON
expand_more
expand_more
format_list_bulleted
Concept explainers
Question
Chapter 39, Problem 39.9DQ
To determine
Why elements in gaseous state emit line spectra while hot solids emit continuous spectra.
Expert Solution & Answer
Want to see the full answer?
Check out a sample textbook solution
Students have asked these similar questions
Elements in the gaseous state emit line spectra with well- defined wavelengths. But hot solid objects always emit a continuous spectrum—that is, a continuous smear of wavelengths. Can you account for this difference?
Elements in the gaseous state emit line spectra with well- defined
wavelengths. But hot solid objects always emit a continuous spectrum-
that is, a continuous smear of wavelengths. Can you account for this
difference?
A cavity radiator has its maximum spectral radiance at a wavelength of 6.8×10
-7 m. If the body is heated so that T/T 0 = 2.2, at what wavelength (in nm) will
the spectral radiance have its new maximum value? Wien's constant b = 2.897
x 10 3 m K.
Answer:
Chapter 39 Solutions
University Physics with Modern Physics, Books a la Carte Edition; Modified MasteringPhysics with Pearson eText -- ValuePack Access Card -- for ... eText -- Valuepack Access Card (14th Edition)
Ch. 39.2 - Prob. 39.2TYUCh. 39.3 - Prob. 39.3TYUCh. 39.4 - Prob. 39.4TYUCh. 39.5 - Prob. 39.5TYUCh. 39.6 - Prob. 39.6TYUCh. 39 - Prob. 39.1DQCh. 39 - Prob. 39.2DQCh. 39 - Prob. 39.3DQCh. 39 - When an electron beam goes through a very small...Ch. 39 - Prob. 39.5DQ
Ch. 39 - Prob. 39.6DQCh. 39 - Prob. 39.7DQCh. 39 - Prob. 39.8DQCh. 39 - Prob. 39.9DQCh. 39 - Prob. 39.10DQCh. 39 - Prob. 39.11DQCh. 39 - Prob. 39.12DQCh. 39 - Prob. 39.13DQCh. 39 - Prob. 39.14DQCh. 39 - Prob. 39.15DQCh. 39 - Prob. 39.16DQCh. 39 - Prob. 39.17DQCh. 39 - Prob. 39.18DQCh. 39 - Prob. 39.19DQCh. 39 - Prob. 39.20DQCh. 39 - Prob. 39.21DQCh. 39 - When you check the air pressure in a tire, a...Ch. 39 - Prob. 39.1ECh. 39 - Prob. 39.2ECh. 39 - Prob. 39.3ECh. 39 - Prob. 39.4ECh. 39 - Prob. 39.5ECh. 39 - Prob. 39.6ECh. 39 - Prob. 39.7ECh. 39 - Prob. 39.8ECh. 39 - Prob. 39.9ECh. 39 - Prob. 39.10ECh. 39 - Prob. 39.11ECh. 39 - Prob. 39.12ECh. 39 - Prob. 39.13ECh. 39 - Prob. 39.14ECh. 39 - Prob. 39.15ECh. 39 - Prob. 39.16ECh. 39 - Prob. 39.17ECh. 39 - Prob. 39.18ECh. 39 - Prob. 39.19ECh. 39 - Prob. 39.20ECh. 39 - Prob. 39.21ECh. 39 - Prob. 39.22ECh. 39 - Prob. 39.23ECh. 39 - Prob. 39.24ECh. 39 - Prob. 39.25ECh. 39 - Prob. 39.26ECh. 39 - Prob. 39.27ECh. 39 - Prob. 39.28ECh. 39 - Prob. 39.29ECh. 39 - Prob. 39.30ECh. 39 - Prob. 39.31ECh. 39 - Prob. 39.32ECh. 39 - Prob. 39.33ECh. 39 - Prob. 39.34ECh. 39 - Prob. 39.35ECh. 39 - Prob. 39.36ECh. 39 - Prob. 39.37ECh. 39 - Prob. 39.38ECh. 39 - Prob. 39.39ECh. 39 - Prob. 39.40ECh. 39 - Prob. 39.41ECh. 39 - Prob. 39.42ECh. 39 - Prob. 39.43ECh. 39 - Prob. 39.44ECh. 39 - Prob. 39.45ECh. 39 - Prob. 39.46ECh. 39 - Prob. 39.47ECh. 39 - Prob. 39.48ECh. 39 - Prob. 39.49ECh. 39 - Prob. 39.50PCh. 39 - Prob. 39.51PCh. 39 - Prob. 39.52PCh. 39 - Prob. 39.53PCh. 39 - Prob. 39.54PCh. 39 - Prob. 39.55PCh. 39 - Prob. 39.56PCh. 39 - Prob. 39.57PCh. 39 - Prob. 39.58PCh. 39 - Prob. 39.59PCh. 39 - An Ideal Blackbody. A large cavity that has a very...Ch. 39 - Prob. 39.61PCh. 39 - Prob. 39.62PCh. 39 - Prob. 39.63PCh. 39 - Prob. 39.64PCh. 39 - Prob. 39.65PCh. 39 - Prob. 39.66PCh. 39 - Prob. 39.67PCh. 39 - Prob. 39.68PCh. 39 - Prob. 39.69PCh. 39 - Prob. 39.70PCh. 39 - Prob. 39.71PCh. 39 - Prob. 39.72PCh. 39 - Prob. 39.73PCh. 39 - Prob. 39.74PCh. 39 - Prob. 39.75PCh. 39 - Prob. 39.76PCh. 39 - Prob. 39.77PCh. 39 - Prob. 39.78PCh. 39 - Prob. 39.79PCh. 39 - Prob. 39.80PCh. 39 - A particle with mass m moves in a potential U(x) =...Ch. 39 - Prob. 39.82PCh. 39 - Prob. 39.83PCh. 39 - DATA In the crystallography lab where you work,...Ch. 39 - Prob. 39.85PCh. 39 - Prob. 39.86CPCh. 39 - Prob. 39.87CPCh. 39 - Prob. 39.88PPCh. 39 - Prob. 39.89PPCh. 39 - Prob. 39.90PPCh. 39 - Prob. 39.91PP
Knowledge Booster
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Similar questions
- What can be said about the relative temperatures of whitish-yellow, reddish, and bluish stars? Explain.arrow_forwardCalculate the wavelength (in nm) for a photon with a frequency of 3.70e+15 Hz.?arrow_forwardA cavity radiator has its maximum spectral radiance at a wavelength of 6,9×10-7 m. If the body is heated so that T/T0 = 9,4, what will be the ratio of radiant powers W/W0? Wien's constant b = 2.897 ×10-3 m·K.arrow_forward
- Please don't provide handwritten solution .... An electron in the n = 6 level of the hydrogen atom emits a photon with a wavelength of 410.2 nm. To what transition does this wavelength correspond?arrow_forwardConsider the following table: Energy (J) Wavelength (nm) Frequency (s-1) region of spectrum A B 1.50 × 1014 C D 500 E F 9.94 × 10-19 G H I J 1 K L Part 1: What goes in position A? (The answer in scientific notation is of the form M × 10N. In this part you will only answer what goes in position M. In the next part you will enter what goes in position N.) Part 2: What goes in position A? (The answer in scientific notation is of the form M × 10N. In this part you will only answer what goes in position N. In the previous part you entered what goes in position M.)arrow_forwardcan u give answerarrow_forward
- That the ratio between the amount of illumination emitted by the sun at the greatest wavelength λmax = 0.5 pm and the greatest wavelength λmax = 0.8 pm is equal to ..?arrow_forwardWhat temperature, in °C, is a blackbody whose emission spectrum peaks at 320 nm ? T= Submit Request Answer Part B VE ΑΣΦ T= Submit What temperature, in °C, is a blackbody whose emission spectrum peaks at 4.60 m? VE ΑΣΦ P By Request Answer ? Stag °C ? °Carrow_forwardThe temperature of the surface of Pluto is about T(K) = 40 K (TC = -230 °C). According to Wien's law, the maximum wavelength of light emitted by Pluto in the IR or infrared region of the spectrum, is Amax = 2900 K•µm/T(K) = 72.5 um. %3D What is the frequency of this radiation? Af =c c = 3x108 m/s O 1.6 x 1019 Hz O 4.1 x 1012 Hz 3.2 x 1013 Hz 39 x 1013 Hz 99.1 MHzarrow_forward
- Photons of a certain ultraviolet light have an energy of 6.34 * 10-19 J. (1a) What is the frequency of this UV light?=______ Hz(1b) Use λ = c/f to calculate its wavelength in nanometers (nm).=_____ nm (1c) Light that has a frequency of about 5.20 * 1014 Hz (a wavelength of about 578 nm) appears yellow to our eyes. What is the energy in joules of the photons associated with this light?=______ J (1d) The human eye is sensitive to orange light having a frequency of about 5.0 * 1014 Hz (a wavelength of about 608 nm). What is the energy in joules of the photons associated with this light? =________Jarrow_forwardWhat are the two distinct components of X-ray spectrum emitted by an X-ray tube? a continuous distribution of wavelengths with a sharp cut-off at short wavelength plus a series of high-intensity spikes. a continuous distribution of wavelengths with a sharp cut-off at long wavelength plus a series of high-intensity spikes. a discontinuous distribution of wavelengths with a sharp cut-off at short wavelength plus a series of high-intensity spikes. a continuous distribution of wavelengths with a sharp cut-off at long wavelengthplus a series of low-intensity spikes.arrow_forwardBy what rate a photon emitted from a sodium vapor lamp? Assume that the lamp's light is monochromatic and of wavelength 589 nm? Answer : 1.5*10^20 s^-1arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
University Physics Volume 3PhysicsISBN:9781938168185Author:William Moebs, Jeff SannyPublisher:OpenStax
Stars and Galaxies (MindTap Course List)PhysicsISBN:9781337399944Author:Michael A. SeedsPublisher:Cengage Learning
Foundations of Astronomy (MindTap Course List)PhysicsISBN:9781337399920Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
Glencoe Physics: Principles and Problems, Student...PhysicsISBN:9780078807213Author:Paul W. ZitzewitzPublisher:Glencoe/McGraw-Hill
Modern PhysicsPhysicsISBN:9781111794378Author:Raymond A. Serway, Clement J. Moses, Curt A. MoyerPublisher:Cengage Learning
University Physics Volume 3
Physics
ISBN:9781938168185
Author:William Moebs, Jeff Sanny
Publisher:OpenStax
Stars and Galaxies (MindTap Course List)
Physics
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Cengage Learning
Foundations of Astronomy (MindTap Course List)
Physics
ISBN:9781337399920
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Glencoe Physics: Principles and Problems, Student...
Physics
ISBN:9780078807213
Author:Paul W. Zitzewitz
Publisher:Glencoe/McGraw-Hill
Modern Physics
Physics
ISBN:9781111794378
Author:Raymond A. Serway, Clement J. Moses, Curt A. Moyer
Publisher:Cengage Learning