
Q5. A possible ion-molecule reaction mechanism for the synthesis of ammonia in interstellar gas clouds is shown below.
N+ + H2 ® NH+ + H k1
NH+ + H2 ® NH2+ + H k2
NH2+ + H2 ® NH3+ + H k3
NH3+ + H2 ® NH4+ + H k4
NH4+ + e- ® NH3 + H k5
NH4+ + e- ® NH2 + 2H k6
- Use the steady-state approximation to derive equations for the concentrations of the intermediates NH+, NH2+, NH3+ and NH4+ in terms of the reactant concentrations [N+], [H2] and [e-]. Treat the electrons as you would any other reactant.
b) Show that the overall rate of productionmjngbh of NH3 is given by
d[NH3]/dt = (k1k5/k5+k6) [N+][H2]
c) What is the origin of the activation energy in a
d) The rates of many ion-molecule reactions show virtually no dependence on temperature.
(i) What does this imply about their activation energy?
(ii) What relevance does this have to reactions occurring in the interstellar medium

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