Inquiry into Physics
8th Edition
ISBN: 9781337515863
Author: Ostdiek
Publisher: Cengage
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Chapter 10, Problem 16P
To determine
Wavelength of the x-ray photon.
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A buckyball consists of 60 carbon atoms arranged in the form of a hollow ball. Say that we illuminate a free, initially non-rotating buckyball with visible light with the intensity of sunlight (1000 W / m2) whose photons all have their spins aligned with their direction of motion. About how long after the illumination begins will the buckyball (on the average) be spinning a million times per second, assuming it absorbs all the light falling on it? (Hints: look in a periodic table to see the mass of a mole of carbon atoms, and remember that Avogadro's number is 6.02 x 1023. Estimate the average wavelength of visible light. You should find that you don't need to know the buckyball's radius.)
Your answer is partially correct.
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Number
1.429048888
Units
photons/s-m^2
Question 6.
a) Photons of incoming radiation have an energy of E = 2500 kJ/mol. Calculate the wavelength (in
nm) of those photons.
b) Would photons from part (a) be able to ionize a Be3+ ion if the electron is found in n=3? Show a
calculation to support your answer.
c). Consider the following balanced combustion reaction:
C7H16(1) + 11 O2(g) → 7 CO2(e) + 8 H2O(g) AcH°= -1160 kJ/mol
If the density of C7H16(1) is 0.68 g/mL, how much heat (in J and scientific notation) is released if 125
mL of C7H16()) undergoes complete combustion?
Chapter 10 Solutions
Inquiry into Physics
Ch. 10 - Prob. 1SACh. 10 - Prob. 1OACh. 10 - Prob. 1PIPCh. 10 - Prob. 1MIOCh. 10 - Prob. 2MIOCh. 10 - Prob. 1QCh. 10 - Prob. 2QCh. 10 - Prob. 3QCh. 10 - Prob. 4QCh. 10 - Prob. 5Q
Ch. 10 - Prob. 6QCh. 10 - Prob. 7QCh. 10 - Prob. 8QCh. 10 - Prob. 9QCh. 10 - Prob. 10QCh. 10 - Prob. 11QCh. 10 - (Indicates a review question, which means it...Ch. 10 - Prob. 13QCh. 10 - Prob. 14QCh. 10 - (Indicates a review question, which means it...Ch. 10 - Prob. 16QCh. 10 - Prob. 17QCh. 10 - Prob. 18QCh. 10 - Prob. 19QCh. 10 - Prob. 20QCh. 10 - Prob. 21QCh. 10 - Prob. 22QCh. 10 - Prob. 23QCh. 10 - Prob. 24QCh. 10 - Prob. 25QCh. 10 - Prob. 26QCh. 10 - Prob. 27QCh. 10 - Prob. 28QCh. 10 - Prob. 29QCh. 10 - Prob. 30QCh. 10 - Prob. 31QCh. 10 - Prob. 32QCh. 10 - Prob. 33QCh. 10 - Prob. 34QCh. 10 - Prob. 35QCh. 10 - Prob. 36QCh. 10 - Prob. 37QCh. 10 - Prob. 38QCh. 10 - Prob. 39QCh. 10 - Prob. 40QCh. 10 - Prob. 41QCh. 10 - Prob. 42QCh. 10 - Prob. 1PCh. 10 - Prob. 2PCh. 10 - Prob. 3PCh. 10 - Prob. 4PCh. 10 - Prob. 5PCh. 10 - Prob. 6PCh. 10 - Prob. 7PCh. 10 - Prob. 8PCh. 10 - Prob. 9PCh. 10 - Prob. 10PCh. 10 - Prob. 11PCh. 10 - Prob. 12PCh. 10 - . Figure 10.47 is the energy-level diagram for a...Ch. 10 - Prob. 14PCh. 10 - Prob. 15PCh. 10 - Prob. 16PCh. 10 - Prob. 17PCh. 10 - Prob. 18PCh. 10 - Prob. 19PCh. 10 - Prob. 20PCh. 10 - Prob. 21PCh. 10 - Prob. 22PCh. 10 - Prob. 23PCh. 10 - Prob. 1CCh. 10 - Prob. 2CCh. 10 - The rate at which solar wind particles enter the...Ch. 10 - Prob. 4CCh. 10 - Prob. 5CCh. 10 - Prob. 6C
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