(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 & Chemical Reactivity
9th Edition
ISBN:9781133949640
Author:John C. Kotz, Paul M. Treichel, John Townsend, David Treichel
Publisher:John C. Kotz, Paul M. Treichel, John Townsend, David Treichel
Chapter14: Chemical Kinetics: The Rates Of Chemical Reactions
Section14.1: Rates Of Chemical Reactions
Problem 2RC: 2. Use the graph provided in Example 14.1 to estimate the average rate of disappearance of dye for...
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![One of the most important mechanisms in Jupiter's atmosphere begins with the photochemical
ionization 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 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.]](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F48e43d24-e797-4c18-89f0-87785ffa58f5%2F37958782-6f4a-4c37-be52-1635c521c147%2F8lsojhs_processed.jpeg&w=3840&q=75)
Transcribed Image Text:One of the most important mechanisms in Jupiter's atmosphere begins with the photochemical
ionization 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 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.]
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