Computer Science
Scientific paper
Jan 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999p%26ss...47..151v&link_type=abstract
Planetary and Space Science, Volume 47, Issue 1-2, p. 151-162.
Computer Science
4
Scientific paper
The thermochemistry of several ion-molecule clustering reactions of HCNH+, HCNH+(N2) and HCNH+(CH4) ions with C2H2 was determined from chemical equilibrium measurements. Inorder to better understand the chemistry of Titan, a gas mixture containing 97% N2, 3% CH4 anda small amount of 0.005% C2H2 was irradiated by α-particles in the temperature range 140-320 K and analysed by high-pressure mass spectrometry. The enthalpy and entropy changes for thereactions HCNH+(C2H2)n+C2H2+N2<---- >HCNH+(C2H2)n+1+N2 (n=0-2), HCNH+(C2H2)n+N2+N2<---- >HCNH+(C2H2)n(N2)+N2 (n=1, 2), HCNH+(C2H2)n+CH4+N2<---- >HCNH+(C2H2)n(CH4)+N2 (n=1, 2), HCNH+(C2H2)n(N2)+C2H2+N2<---- >HCNH+(C2H2)n+1(N2)+N2 (n=0, 1) have been determined. For the HCNH+(C2H2)n series,the absolute enthalpy change decreases monotonically from 12.1 to 2.8 kcal mol-1 for n=1 to 3,showing no noticeable effect concerning the filling of shells. The nature of the bonding remainsmainly electrostatic. For the HCNH+(C2H2)n(X) series with X=N2 or CH4, the free energychanges ΔG° were calculated for T=90 K and 165 K. For both temperatures, ΔG°~0 forreplacement of N2 by CH4 for n=0 to 2 wheareas ΔG° for the substitution of N2 or CH4 by C2H2are negative for n=0, 1. The ligand-exchange reaction leading to the formation of HCNH+(C2H2)and HCNH+(C2H2)2 could exist in the lower Titans atmosphere. Paths involving HCNH+(C2H2)(N2) or HCNH+(C2H2)(CH4) and yielding to HCNH+(C2H2)2 ions could also be possible and thuscould lead to heavier organic-nitrogen compounds and eventually large aerosols.
Duc E. L.
Fitaire M.
Vacher J. R.
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