One of the most important mechanisms in Jupiter's atmosphere begins with the photochemicalionization of H2e) induced by sąlar radiation with wavelength 2= c/v 80.4 nm:(9)• H2 + hv → H2* +e,H2+H2 H3 +H,H3 +e H2 +H,Ia.k2.k3.Find the rate equation for the disappearance of H2, considering that H2", H3", and e are attheir stationary states. Verify that the mechanism is consistent with the global stoichiometryH2 → 2H. [Note that H-atom is a product, and not in steady state.]

From the steady state approximation the rate of disappearance of H2 can be expressed as:

(9) One of the most important mechanisms in Jupiter's atmosphere begins with the photochemical ionization of Hze) induced by sęlar radiation with wavelength 2 = c/v = 80.4 nm: • H2 + hv → H2* +e, H2+H2 H3 +H, k2- • H3* +e → H2 +H, k3. Find the rate equation for the disappearance of H2, considering that H2", H3", and e are at their stationary states. Verify that the mechanism is consistent with the global stoichiometry H2 → 2H. [Note that H-atom is a product, and not in steady state.]

(9) One of the most important mechanisms in Jupiter's atmosphere begins with the photochemical ionization of Hze) induced by sęlar radiation with wavelength 2 = c/v = 80.4 nm: • H2 + hv → H2* +e, H2+H2 H3 +H, k2- • H3* +e → H2 +H, k3. Find the rate equation for the disappearance of H2, considering that H2", H3", and e are at their stationary states. Verify that the mechanism is consistent with the global stoichiometry H2 → 2H. [Note that H-atom is a product, and not in steady state.]

Chemistry

10th Edition

ISBN:9781305957404

Author:Steven S. Zumdahl, Susan A. Zumdahl, Donald J. DeCoste

Publisher:Steven S. Zumdahl, Susan A. Zumdahl, Donald J. DeCoste

Chapter1: Chemical Foundations

Section: Chapter Questions

Problem 1RQ: Define and explain the differences between the following terms. a. law and theory b. theory and...

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